tag:blogger.com,1999:blog-83315119205863239892024-03-04T20:47:14.832-08:00Visitando os Objetos MessierJanine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comBlogger36125tag:blogger.com,1999:blog-8331511920586323989.post-18153594890067553002014-09-12T12:09:00.003-07:002015-06-14T11:22:36.891-07:00Sobre o Catálogo Messier e sobre Charles Messier e Pierre Méchain<div style="text-align: center;">
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><span style="line-height: 18px;"><br /></span></span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">Olá!</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">Inicialmente, Caro Leitor,</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">nossa Visita aos Objetos Messier</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">nos trará, </span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">nesta Postagem de Apresentação,</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;"> alguma informação sobre este valioso Trabalho</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">realizado por Charles Messier e Pierre Méchain, originalmente.</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">Mais abaixo, </span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">encontre o Índice das Constelações que acolhem os famosos Objetos Messier.</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">Boa Leitura, Bons Estudos e Boa Observação!</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">Com um abraço estrelado,</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.6000003814697px;"><span style="line-height: 18px;">Janine Milward</span></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><span style="line-height: 18px;"><br /></span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria"><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">História</span></span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<b>Charles Joseph Messier</b> (<a href="http://pt.wikipedia.org/wiki/Badonviller" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Badonviller">Badonviller</a>, <a href="http://pt.wikipedia.org/wiki/26_de_junho" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="26 de junho">26 de junho</a> de <a href="http://pt.wikipedia.org/wiki/1730" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1730">1730</a> – <a href="http://pt.wikipedia.org/wiki/Paris" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Paris">Paris</a>, <a href="http://pt.wikipedia.org/wiki/12_de_abril" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="12 de abril">12 de abril</a> de <a href="http://pt.wikipedia.org/wiki/1817" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1817">1817</a>) foi um <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="França">francês</a>, conhecido pela compilação e publicação, com a coautoria de <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, de seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo</a> de <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos de céu profundo</a>, uma lista de 110 objetos astronômicos como <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que vieram a ser conhecidos como os "objetos Messier".<span class="reference" id="cite_ref-Brittanica_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier#cite_note-Brittanica-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Pretendia, com a publicação do catálogo, auxiliar a si mesmo e outros astrônomos e observadores em sua atividade astronômica principal durante sua carreira, a investigação de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Cometas" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Cometas">cometas</a>, listando todos objetos que pôde identificar e que poderiam ser facilmente confundidos com cometas transientes, mas que, na realidade, tinham naturezas completamente diferentes e eram fixos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>. Contudo, Messier, sem intenção, catalogou alguns dos astros mais interessantes para a atual <a href="http://pt.wikipedia.org/wiki/Astronomia_amadora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia amadora">astronomia amadora</a>.<span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier#cite_note-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Tornou-se um observador do céu ao trabalhar para <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background: none; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a> em seu observatório em Paris, aos 21 anos. Foi o primeiro astrônomo a dedicar-se quase exclusivamente à procura de cometas e, enquanto aguardava o retorno do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a>, deparou-se com um falso positivo ao confundir uma nebulosa com o cometa. Para evitar novos enganos, começou a compilar os objetos fixos no céu profundo que poderiam ser facilmente confundidos com um cometa, objeto difuso e de fraco brilho. De 1758 a 1782, com a ajuda de <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> após 1774, compilou 107 objetos entre nebulosas, aglomerados estelares e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xias" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxias">galáxias</a>.<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">nota 1</a></span>Três objetos adicionais foram mais tarde adicionados ao catálogo, após a morte de Messier, completando 110 objetos ao todo.</div>
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Leia muito mais sobre Charles Messier</div>
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<span style="background-color: white; font-family: sans-serif; line-height: 17.3185615539551px; text-align: left;"><span style="color: #073763;">Desenho da "nebulosa" de Andrômeda, por Messier</span></span></div>
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<b>Pierre François André Méchain</b> (<a href="http://pt.wikipedia.org/wiki/Laon" style="background: none; color: #0b0080; text-decoration: none;" title="Laon">Laon</a>, <a href="http://pt.wikipedia.org/wiki/16_de_agosto" style="background: none; color: #0b0080; text-decoration: none;" title="16 de agosto">16 de agosto</a> <a href="http://pt.wikipedia.org/wiki/1744" style="background: none; color: #0b0080; text-decoration: none;" title="1744">1744</a> — <a href="http://pt.wikipedia.org/wiki/Castell%C3%B3_de_la_Plana" style="background: none; color: #0b0080; text-decoration: none;" title="Castelló de la Plana">Castelló de la Plana</a>, <a href="http://pt.wikipedia.org/wiki/20_de_setembro" style="background: none; color: #0b0080; text-decoration: none;" title="20 de setembro">20 de setembro</a> de <a href="http://pt.wikipedia.org/wiki/1804" style="background: none; color: #0b0080; text-decoration: none;" title="1804">1804</a>) foi um <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> e <a href="http://pt.wikipedia.org/wiki/Ge%C3%B3grafo" style="background: none; color: #0b0080; text-decoration: none;" title="Geógrafo">geógrafo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a>.</div>
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Famoso por ter descobertos 8 <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a> e 26 objetos celestes, assim como por ter feito parte em numerosas expedições. Sua maior contribuição foi a medida do<a href="http://pt.wikipedia.org/wiki/Metro" style="background: none; color: #0b0080; text-decoration: none;" title="Metro">metro</a>, junto com <a href="http://pt.wikipedia.org/wiki/Jean_Baptiste_Joseph_Delambre" style="background: none; color: #0b0080; text-decoration: none;" title="Jean Baptiste Joseph Delambre">Delambre</a>.</div>
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Em 1774 estava com <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> e ambos trabalharam no Hotel de Cluny catalogando estrelas. Neste período de colaboração descobriram muitos objetos que Messier comprovou posteriormente sua posição. Alguns dos objetos catalogados por Messier foram descobertos por Méchain, tais como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M104" style="background: none; color: #0b0080; text-decoration: none;" title="M104">M104</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M105" style="background: none; color: #0b0080; text-decoration: none;" title="M105">M105</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M106" style="background: none; color: #0b0080; text-decoration: none;" title="M106">M106</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M107" style="background: none; color: #0b0080; text-decoration: none;" title="M107">M107</a>.</div>
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Participou de inúmeras expedições pela costa francesa e em 1774 observou a ocultação de <a href="http://pt.wikipedia.org/wiki/Aldebar%C3%A3" style="background: none; color: #0b0080; text-decoration: none;" title="Aldebarã">Aldebarã</a> pela <a href="http://pt.wikipedia.org/wiki/Lua" style="background: none; color: #0b0080; text-decoration: none;" title="Lua">lua</a>; após isto apresentou uma memória a <a href="http://pt.wikipedia.org/wiki/Acad%C3%A9mie_des_Sciences" style="background: none; color: #0b0080; text-decoration: none;" title="Académie des Sciences">Academia de Ciências de Paris</a>.</div>
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Méchain descobriu cometas, seus primeiros foram em 1781 e por meio de seu conhecimento matemático trabalhou em calcular suas <a href="http://pt.wikipedia.org/wiki/%C3%93rbita" style="background: none; color: #0b0080; text-decoration: none;" title="Órbita">órbitas</a>. Algumas de suas descobertas foram atribuídas a outros astrônomos, assim como o descobrimento de <a href="http://pt.wikipedia.org/wiki/Cometa_Encke" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa Encke">2P/Encke</a> (redescoberto anos mais tarde por <a href="http://pt.wikipedia.org/wiki/Johann_Franz_Encke" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Franz Encke">Johann Franz Encke</a>).</div>
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<b>Leia muito mais sobre Charles Messier e Pierre Méchain</b></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif; font-size: large;">VISITANDO OS OBJETOS MESSIER</span><br />
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Constelações acolhendo os Objetos Messier</h2>
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<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/hercules_6.html" style="color: #274e13; text-decoration: none;"><b>Hercules</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/hydra_6.html" style="color: #274e13; text-decoration: none;"><b>Hydra</b></a></li>
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<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/lepus.html" style="color: #274e13; text-decoration: none;"><b>Lepus</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/lyra.html" style="color: #274e13; text-decoration: none;"><b>Lyra</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/monoceros_6.html" style="color: #274e13; text-decoration: none;"><b>Monoceros</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/ophiucus.html" style="color: #274e13; text-decoration: none;"><b>Ophiucus</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/orion.html" style="color: #274e13; text-decoration: none;"><b>Orion</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/pegasus.html" style="color: #274e13; text-decoration: none;"><b>Pegasus</b></a></li>
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<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/sagittarius.html" style="color: #274e13; text-decoration: none;"><b>Sagittarius</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/scorpius.html" style="color: #274e13; text-decoration: none;"><b>Scorpius</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/scutum.html" style="color: #274e13; text-decoration: none;"><b>Scutum</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/serpens-caput-e-serpens-cauda.html" style="color: #274e13; text-decoration: none;"><b>Serpens Caput e Serpens Cauda</b></a></li>
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<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/triangulum.html" style="color: #274e13; text-decoration: none;"><b>Triangulum</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/ursa-major.html" style="color: #274e13; text-decoration: none;"><b>Ursa Major</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/virgo.html" style="color: #274e13; text-decoration: none;"><b>Virgo</b></a></li>
<li style="background: none; border-bottom-color: rgb(148, 74, 10); border-bottom-style: solid; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/vulpecula_6.html" style="color: #274e13; text-decoration: none;"><b>Vulpecula</b></a></li>
<li style="background: none; border-bottom-style: none; border-top-color: rgb(102, 0, 0); border-top-style: solid; border-width: 0px; list-style: none outside none; margin: 0.25em 0px; padding: 0.25em 15px 0.25em 1.3em;"><a href="http://visitandoosobjetosmessier.blogspot.com.br/2014/09/comentario_12.html" style="color: #274e13; text-decoration: none;"><b>Sobre o Catálogo Messier e sobre Charles Messier e...</b></a></li>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-51108385409275550542014-09-06T10:29:00.005-07:002015-04-02T09:14:58.968-07:00Vulpecula<div class="MsoNormal" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: -webkit-center;">
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">Olá!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sempre fico feliz ao admirar e comentar</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> sobre o quão rica em vizinhança estrelada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e de constelações pequenas porém encantadoras</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é a maravilhosa constelação Aquila, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">a Águia em seu voo balizado por suas três estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- Alshain, Terazed e Altair, estrela-alpha Aquilae!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Na descrição sobre esta vizinhança estrelada </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que visualmente apreciamos </span><span style="font-family: Arial, Helvetica, sans-serif;">ao redor da belíssima Águia,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">podemos notar a delicadeza de figura de um diamante polido</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que </span><span style="font-family: Arial, Helvetica, sans-serif;"> Delphinus, o Delfim, nos revela!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(veja em h<a href="ttp://oceudomes.blogspot.com.br/2014/08/a-delicada-constelacao-delphinuso-delfim.html" style="color: #274e13;">ttp://oceudomes.blogspot.com.br/2014/08/a-delicada-constelacao-delphinuso-delfim.html</a>)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">E também é sempre um imenso prazer</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">delinearmos as estrelas e comentarmos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"> sobre a pequena porém encantadora</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Flecha dos céus estrelados, Sagitta!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(veja em http://oceudomes.blogspot.com.br/2014/08/sagitta-estrelada-flecha-certeira.html)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Bem grudada à Flecha, a Seta, Sagitta,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">encontra-se uma constelação criada por Hevelius, em 1690,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">na intenção de ocupar um espaço no céu</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">com um animal (a Raposa caçando o Ganso)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tão astuto e voraz e corajoso quanto a Águia, Aquila, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e como o Corvo Caído, Vultur Cadens (outra denominação para a Lyra!):</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">entrou em cena, então, a constelação Vulpecula et Anser, a Raposa e o Ganso.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A bem da verdade </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(e como nos diz Ronaldo Rogério de Freitas Mourão),</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;"><i>a Via Láctea passa por Vulpécula,</i></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;"><i> o que faz com que suas estrelas não apareçam de maneira proeminente.</i></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i>Esta constelação pode ser encontrada ao longo de Sagitta </i></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i>ou a partir da estrela Beta Cygni, Albireo</i></span><span style="font-family: Arial, Helvetica, sans-serif;">. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">De qualquer forma, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">mesmo não sendo uma constelação de estrelas expressivas a olho nu, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">bem ao contrário... porém nos trazendo Exoplanetas e</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nos brindando com <b>a belíssima M27, Dumbbell Nebula </b></span><b><br /></b><span style="font-family: Arial, Helvetica, sans-serif;"><b>(a Nebulosa da Bolha do Sabão ou do Halteres)..</b>..,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e mesmo que ocupe uma área extensa nos céus estrelados do norte,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Vulpecula et Anser ajudam a enriquecer</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">a vizinhança estelar em torno à Águia</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e estas constelações vicinais nos trazem muito prazer</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">em buscar visualizá-las e divisá-las</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">- sempre em noites sem-Lua e em lugares de céus escuros e transparentes.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Assim como as cartas celestes nos mostram, Vulpecula encontra-se</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">praticamente grudada à Sagitta </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e ambas constelações situando-se na Grande Fenda, The Great Rift, o Rio do Vazio,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">a bifurcação que acontece naquele ponto da Via Lactea</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> entre as estrelas Altair e Deneb, estrelas-alpha Aquilae e Cygni, respectivamente.... </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">- porém é preciso que estejamos em lugar realmente de céus transparentes</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para bem visualizarmos esses pormenores na Via Lactea...</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Realmente, não é nada fácil divisar e visualizar Vulpecula em bons termos</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">- porém eu penso que existe a boa ajuda </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">da imensa e belíssima constelação do Cisne, Cygnus,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> que se espraia em seu voo </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">como se estivesse recém sendo alçado </span><span style="font-family: Arial, Helvetica, sans-serif;">através os céus mais ao norte! </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">A estrela-beta Cygni, Albireo</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">- que é sugerida ora como o Olho do Cisne e ora como o Bico do Cisne -,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">aponta para a vicinitude da Raposa com o Ganso.</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">É bem interessante também percebermos</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">que as constelações Sagitta, a Flecha, e Vulpecula, a Raposa,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">encontram-se bem no caminho do meio</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">da deslumbrante imagem que nomeamos de Grande Triângulo do Norte</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">(do Verão, no hemisfério norte, e do Inverno, no hemisfério sul)</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">realizado a partir das estrelas Alpha das constelações Aquila, Lyra e Cygnus,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">quer dizer, das belíssimas estrelas Altair, Vega e Deneb!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em outros Trabalhos, viemos comentando sobre</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">os Objetos Messier acolhidos pela constelação Cygnus</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- veja em</span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m29-e-m39-os-objetos-messier-em-cygnus.html -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e pela constelação Lyra...</span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">- veja em </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m56-e-m57-os-objetos-messier-em-lyra.html</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"> -,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém não encontramos nenhum desses Objetos em Aquila</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- mas, ao invés da Águia, estaremos comentando neste Trabalho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>sobre o Objeto Messier encontrado em Vulpecula, a Raposa</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>(constelação que se encontra entre Cygnus e Aquila!),</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e esse Objeto é a famosa Dumbbell Nebula, M27</b>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">VULPECULA ET ANSER, </span></b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">A RAPOSA E O GANSO</span></b><o:p></o:p></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><br /></span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 18h56m / 21h28m Declinação +19<sup>o</sup>.5 / +29<sup>o</sup>.4<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Constelação formada por Hevelius em 1690 </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">porém hoje em dia abreviada para Vulpecula.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Algumas Informações Interessantes acerca esta Constelação:</span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esta constelação pode ser encontrada ao longo de Sagitta </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">ou a partir da estrela Beta Cygni, Albireo. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">A Via Láctea passa por Vulpécula,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> o que faz com que suas estrelas não apareçam de maneira proeminente.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp?rightAscension=20.3&declination=23.6" style="color: #274e13; text-decoration: none;">http://www.nightskyatlas.com/index.jsp?rightAscension=20.3&declination=23.6</a></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">Fronteiras:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Vulpecula situa-se entre as constelações </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Sagitta, Delphinus, Pegasus Cignus Lyra, Hercules</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://www.iau.org/static/public/constellations/gif/VUL.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; padding: 8px; text-align: -webkit-center;" /></div>
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<b style="background-color: white; line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">M27,</span></b></div>
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<b style="background-color: white; line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">O ÚNICO OBJETO MESSIER</span></b></div>
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<b style="background-color: white; line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">NA CONSTELAÇÃO DA RAPOSA:</span></b></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.3999996185303px;"><br /></b><b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.3999996185303px;"><br /></b><b style="background-color: white; color: #252525; font-family: sans-serif; font-size: 14px; line-height: 22.3999996185303px;"><br /></b></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/dumbbellatlas.jpg" /></div>
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http://www.ipac.caltech.edu/2mass/gallery/dumbbellatlas.jpg</div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 27</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Planetary Nebula</a> M27 (NGC 6853)</i>, type 3a+2, in <a href="http://messier.obspm.fr/map/Vul.html">Vulpecula</a></center>
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<br /><b><span style="font-size: large;">Dumbbell Nebula</span></b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m27.jpg"><img align="right" alt="[m27.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m27.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0" style="font-family: 'Times New Roman';"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">19 : 59.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+22 : 43 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.25 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">8.0x5.7 (arc min)</td></tr>
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Discovered by Charles Messier in 1764.</div>
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The Dumbbell Nebula Messier 27 (M27, NGC 6853) is perhaps the finest planetary nebula in the sky, and was the first planetary nebula ever discovered.</div>
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On July 12, 1764, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> discovered this new and fascinating class of objects, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M27">describes this one</a> as an oval nebula without stars. The name "Dumb-bell" goes back to the <a href="http://messier.obspm.fr/Mdes/dm027.html#JH">description</a> by <a href="http://messier.obspm.fr/xtra/Bios/jherschel.html">John Herschel</a>, who also compared it to a "double-headed shot."</div>
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We happen to see this one approximately from its equatorial plane (approx. left-to-right in our image); this is similar to our view of another, fainter Messier planetary nebula, <a href="http://messier.obspm.fr/m/m076.html">M76</a>, which is called the Little Dumbbell. From near one pole, it would probably have the shape of a ring, and perhaps look like we view the Ring Nebula <a href="http://messier.obspm.fr/m/m057.html">M57</a>.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m027.html</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e8/M27_-_Dumbbell_Nebula.jpg/800px-M27_-_Dumbbell_Nebula.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br />
<span style="font-family: Arial, Helvetica, sans-serif;">http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:M27_-_Dumbbell_Nebula.jpg</span><br />
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">M27 - Dumbbell Nebula</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">ESO</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/eso9846a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.eso.org/public/images/eso9846a/</a></span></span></div>
<span style="color: #555555; font-family: sans-serif; line-height: 24px; text-align: start;">The </span><a class="extiw" href="http://en.wikipedia.org/wiki/Dumbbell_Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 24px; text-align: start; text-decoration: none;" title="en:Dumbbell Nebula">Dumbbell Nebula</a><span style="color: #555555; font-family: sans-serif; line-height: 24px; text-align: start;"> — also known as Messier 27 or NGC 6853 — is a typical planetary nebula and is located in the constellation </span><a class="extiw" href="http://en.wikipedia.org/wiki/Vulpecula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 24px; text-align: start; text-decoration: none;" title="en:Vulpecula">Vulpecula</a><span style="color: #555555; font-family: sans-serif; line-height: 24px; text-align: start;"> (The Fox). The distance is rather uncertain, but is believed to be around 1200 light-years. It was first described by the French astronomer and comet hunter </span><a class="extiw" href="http://en.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 24px; text-align: start; text-decoration: none;" title="en:Charles Messier">Charles Messier</a><span style="color: #555555; font-family: sans-serif; line-height: 24px; text-align: start;"> who found it in 1764 and included it as no. 27 in his famous list of extended sky objects. Despite its class, the Dumbbell Nebula has nothing to do with planets. It consists of very rarified gas that has been ejected from the hot central star now in one of its last evolutionary stages. Colours & filters Band Wavelength Telescope Optical B 429 nm Very Large Telescope FORS1 Optical Oiii 501 nm Very Large Telescope FORS1 Optical H-alpha 656 nm Very Large Telescope FORS1 .</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 6853 - M 27 - Vulpecula - Nebulosa Planetária - Bolha de Sabão</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 19h58m Declinação +22<sup>o</sup>.40<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP Dimensão 7,0 Magnitude 20<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 13 Distância em anos-luz 3,5<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Encontrada mais ao sul e na fronteira com Sagitta.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px;"> É uma nebulosa planetária e conhecida como Dumbbell.<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<tr><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1112/m27_snyder_900.jpg" height="477" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" width="640" /></span></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="font-size: small;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/ap111227.html" style="color: #274e13; text-decoration: none;">http://apod.nasa.gov/apod/ap111227.html</a></span><br /><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M27: The Dumbbell Nebula<br />Image Credit & Copyright: <a href="http://billsnyderastrophotography.com/?page_id=2" style="color: #274e13; text-decoration: none;">Bill Snyder</a> (<a href="http://billsnyderastrophotography.com/" style="color: #274e13; text-decoration: none;">Bill Snyder Photography</a>) </span></span></td></tr>
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<b style="color: #073763;"> Explanation: </b><span style="color: #073763;">The first hint of what will become of our </span><a href="http://www.nineplanets.org/sol.html" style="color: #274e13; text-decoration: none;">Sun</a><span style="color: #073763;"> was discovered inadvertently in </span><a href="http://en.wikipedia.org/wiki/1764" style="color: #274e13; text-decoration: none;">1764</a><span style="color: #073763;">. At that time, </span><a href="http://www.seds.org/messier/xtra/history/biograph.html" style="color: #274e13; text-decoration: none;">Charles Messier</a><span style="color: #073763;"> was compiling a list of diffuse objects not to be confused with comets. The 27th object on </span><a href="http://apod.nasa.gov/apod/ap960626.html" style="color: #274e13; text-decoration: none;">Messier's list</a><span style="color: #073763;">, now known as </span><a href="http://www.seds.org/messier/m/m027.html" style="color: #274e13; text-decoration: none;">M27</a><span style="color: #073763;"> or the Dumbbell Nebula, is a </span><a href="http://apod.nasa.gov/apod/planetary_nebulae.html" style="color: #274e13; text-decoration: none;">planetary nebula</a><span style="color: #073763;">, the type of nebula our </span><a href="http://asterisk.apod.com/viewtopic.php?f=24&t=18012" style="color: #274e13; text-decoration: none;">Sun</a><span style="color: #073763;"> will produce when </span><a href="http://fusedweb.pppl.gov/" style="color: #274e13; text-decoration: none;">nuclear fusion</a><span style="color: #073763;"> stops in its core. </span><a href="http://apod.nasa.gov/apod/ap020302.html" style="color: #274e13; text-decoration: none;">M27</a><span style="color: #073763;"> is one of the brightest </span><a href="http://www.seds.org/messier/planetar.html" style="color: #274e13; text-decoration: none;">planetary nebulae</a><span style="color: #073763;"> on the sky, and can be seen toward the </span><a href="http://www.astro.wisc.edu/~dolan/constellations/extra/constellations.html" style="color: #274e13; text-decoration: none;">constellation</a><span style="color: #073763;"> of the Fox (</span><a href="http://en.wikipedia.org/wiki/Vulpecula" style="color: #274e13; text-decoration: none;">Vulpecula</a><span style="color: #073763;">) with binoculars. It takes light about 1000 years to reach us from M27, </span><a href="http://billsnyderastrophotography.com/?page_id=1767" style="color: #274e13; text-decoration: none;">shown above</a><span style="color: #073763;"> in colors emitted by </span><a href="http://en.wikipedia.org/wiki/H-alpha" style="color: #274e13; text-decoration: none;">hydrogen</a><span style="color: #073763;"> and </span><a href="http://periodic.lanl.gov/8.shtml" style="color: #274e13; text-decoration: none;">oxygen</a><span style="color: #073763;">. Understanding the physics and significance of </span><a href="http://apod.nasa.gov/apod/ap100826.html" style="color: #274e13; text-decoration: none;">M27</a><span style="color: #073763;"> was well beyond 18th century science. Even today, many things remain mysterious about </span><a href="http://apod.nasa.gov/apod/ap040201.html" style="color: #274e13; text-decoration: none;">bipolar planetary nebula</a><span style="color: #073763;"> like M27, including the physical mechanism that expels a low-mass star's gaseous outer-envelope, leaving an </span><a href="http://science.hq.nasa.gov/kids/imagers/ems/xrays.html" style="color: #274e13; text-decoration: none;">X-ray</a><span style="color: #073763;"> hot </span><a href="http://imagine.gsfc.nasa.gov/docs/science/know_l2/dwarfs.html" style="color: #274e13; text-decoration: none;">white dwarf</a><span style="color: #073763;">.</span><br />
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<span style="color: #660000;">A <b>Nebulosa do Haltere</b> (Messier 27, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC 6853</a>)</span><span style="color: #252525;">, foi a primeira <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> descoberta. Está localizada a cerca de mil e duzentos <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> de distância da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, na direção da <a href="http://pt.wikipedia.org/wiki/Vulpecula" style="background: none; color: #0b0080; text-decoration: none;" title="Vulpecula">Constelação da Raposa</a>.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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Foi descoberta em <a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a>, por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>. Com seu brilho de magnitude aparente 7,5 e com <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background: none; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a> aparente de cerca de 8 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>, é facilmente visível com<a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> e bastante observada por <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomos</a> amadores. Situa-se aproximadamente a 1000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e sua idade, cerca de 10 000 anos, é extremamente pequena em termos astrônomicos, embora comum para nebulosas planetárias.</div>
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<span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d7/Weighing_in_on_the_Dumbbell_Nebula.jpg/1920px-Weighing_in_on_the_Dumbbell_Nebula.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:Weighing_in_on_the_Dumbbell_Nebula.jpg" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:Weighing_in_on_the_Dumbbell_Nebula.jpg</a></span><br />
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Weighing in on the Dumbbell Nebula</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">NASA/JPL-Caltech/J. Hora (Harvard-Smithsonian CfA)</span> - <span class="mw-mmv-source"><a class="external text" href="http://www.spitzer.caltech.edu/images/4409-sig11-011-Weighing-in-on-the-Dumbbell-Nebula" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">JPL</a></span></span></div>
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Image from the <a href="http://en.wikipedia.org/wiki/Spitzer_Space_Telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Spitzer Space Telescope">Spitzer Space Telescope</a>.</div>
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The Dumbbell nebula, also known as Messier 27, pumps out <a href="http://commons.wikimedia.org/wiki/Category:Infrared" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Infrared">infrared</a> light in this image from NASAs <a href="http://commons.wikimedia.org/wiki/Category:Spitzer_space_telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Spitzer space telescope">Spitzer Space Telescope</a>. Spitzers infrared view shows a different side of this recycled stellar material. It is interesting how different Spitzers view of the Dumbbell looks compared to optical images, comments Dr. Joseph Hora of the <a href="http://commons.wikimedia.org/wiki/Category:Harvard-Smithsonian_Center_for_Astrophysics" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Harvard-Smithsonian Center for Astrophysics">Harvard Smithsonian Center for Astrophysics</a>. The diffuse <a href="http://commons.wikimedia.org/wiki/Green" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Green">green</a> glow, which is brightest near the center, is probably showing us hot gas atoms being heated by the ultraviolet <a href="http://commons.wikimedia.org/wiki/Light" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light">light</a> from the central white dwarf. A collection of clumps fill the central part of the nebula, and <a class="mw-redirect" href="http://commons.wikimedia.org/wiki/Red" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Red">red</a>-coloured radial spokes extend well beyond. Astronomers think these features represent molecules of <a href="http://commons.wikimedia.org/wiki/Hydrogen" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hydrogen">hydrogen</a> gas, mixed with traces of heavier elements</div>
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<span style="color: #073763;"><span style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px;"><img src="http://upload.wikimedia.org/wikipedia/commons/e/e3/TwoDumbbells.JPG" height="400" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="335" /></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell#mediaviewer/File:TwoDumbbells.JPG" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Dumbbell#mediaviewer/File:TwoDumbbells.JPG</a></span><br />
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<span style="color: #073763;"><span style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px;"><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/db/Halteres_from_ancient_Greece.JPG/1024px-Halteres_from_ancient_Greece.JPG" height="425" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></span><br />
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Halteres from ancient Greece</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Author and source information" style="font-size: 0.8em;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/User:Portum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="en:User:Portum">Portum</a> (<a class="extiw" href="http://en.wikipedia.org/wiki/User_talk:Portum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="en:User talk:Portum">talk</a>). Original uploader was <a class="extiw" href="http://en.wikipedia.org/wiki/User:Portum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="en:User:Portum">Portum</a> at <a class="external text" href="http://en.wikipedia.org/" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;">en.wikipedia</a></span></span></div>
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Foi a primeira <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> a ser descoberta e o primeiro a visualizá-la foi o astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, em 12 de julho de 1764. Ele descreveu o objeto como uma nebulosa oval sem estrelas. O nome "haltere" foi dado por <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>, que o comparou-o a uma "marca de dois tiros próximos".<span class="reference" id="cite_ref-seds_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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A partir da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, tem-se a vista equatorial da nebulosa planetária, de forma semelhante à vista de outra nebulosa planetária, a<a href="http://pt.wikipedia.org/wiki/Pequena_Nebulosa_do_Haltere" style="background: none; color: #0b0080; text-decoration: none;" title="Pequena Nebulosa do Haltere">Pequena Nebulosa do Haltere</a> (Messier 76). Posicionando-se em um dos polos da nebulosa, seria possível visualizar sua forma de um anel, forma semelhante a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Anel">nebulosa do Anel</a> (Messier 57).<span class="reference" id="cite_ref-seds_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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<span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjfcRxKyCgBdax-0nTVoegtlLAQISveGhWST9L8Z3kRsHncWF7a5vUMwsfx0dtu9GLUJLn8XJY0Tears3B7MFy9vE8a-Dz19zM9Pa6rW3Lly_Oi_21ly72uz9a7fQKYuky9HUa1V8_0oTM/s1600/Messier27.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjfcRxKyCgBdax-0nTVoegtlLAQISveGhWST9L8Z3kRsHncWF7a5vUMwsfx0dtu9GLUJLn8XJY0Tears3B7MFy9vE8a-Dz19zM9Pa6rW3Lly_Oi_21ly72uz9a7fQKYuky9HUa1V8_0oTM/s1600/Messier27.jpg" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#mediaviewer/Ficheiro:Messier27.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#mediaviewer/Ficheiro:Messier27.jpg</a></span></span></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Like many nearby planetary nebulae, <b>the Dumbbell contains knots</b>. Its central region is marked by a pattern of dark and bright cusped knots and their associated dark tails (see picture). The knots vary in appearance from symmetric objects with tails to rather irregular tail-less objects. Similarly to the </span><a href="http://en.wikipedia.org/wiki/Helix_Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Helix Nebula">Helix Nebula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> and the </span><a href="http://en.wikipedia.org/wiki/Eskimo_Nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Eskimo Nebula">Eskimo Nebula</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, the heads of the knots have bright cusps which are local </span><a href="http://en.wikipedia.org/wiki/Photoionization" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Photoionization">photoionization</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> fronts.</span><sup class="reference" id="cite_ref-ODelletal2003_5-1" style="color: #252525; font-family: sans-serif; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula#cite_note-ODelletal2003-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Dumbbell_Nebula</a></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgiGSWBBYcXPYDyzt-MAjvgqW64dPxkGYLCO7kP5qVeil46tHWvu6G1QK8LkxVyeXdOMTGZ-GUd8n0ijUs7UYnPFuYEO53SrlFPruCwgeYB5viD6DyssJegbaNhX2Dxe-kGqKw1vZOO124/s1600/M27_Knots.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgiGSWBBYcXPYDyzt-MAjvgqW64dPxkGYLCO7kP5qVeil46tHWvu6G1QK8LkxVyeXdOMTGZ-GUd8n0ijUs7UYnPFuYEO53SrlFPruCwgeYB5viD6DyssJegbaNhX2Dxe-kGqKw1vZOO124/s1600/M27_Knots.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:M27_Knots.jpg" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Dumbbell_Nebula#mediaviewer/File:M27_Knots.jpg</a></span><br />
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">M27 Knots</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">C.R. O'Dell (Vanderbilt University)</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2003/06/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/2003/06/image/a</a> (<a class="external text" href="http://imgsrc.hubblesite.org/hu/db/2003/06/images/a/formats/full_jpg.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)</span></span></div>
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A estrela central de M27 é uma <a href="http://pt.wikipedia.org/wiki/Estrela_an%C3%A3" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela anã">estrela anã</a> brilhante, de magnitude aparente 13,5, e é extremamente quente, azul, com <a href="http://pt.wikipedia.org/wiki/Temperatura" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Temperatura">temperatura</a>superficial de 85 000 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>, pertencente à <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe espectral</a> O7, com uma provável companheira de magnitude aparente 17.<span class="reference" id="cite_ref-seds_5-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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Adotando-se um valor médio para sua distância em 1 200 anos-luz, a luminosidade intrínseca da nebulosa é cerca de 100 vezes mais do que a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luminosidade_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade solar">luminosidade solar</a> (-0,5 de<a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a>), embora a estrela geradora da nebulosa tenha apenas um terço da luminosidade solar e sua companheira apenas um centésimo, considerando-se o<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Espectro_visual" style="background: none; color: #0b0080; text-decoration: none;" title="Espectro visual">espectro visual</a>. A grande luminosidade da nebulosa deve-se a absorção radiação de alta energia da estrela central e na sua reemissão no espectro visível, sendo a maior parte emitida em apenas uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Linha_espectral" style="background: none; color: #0b0080; text-decoration: none;" title="Linha espectral">linha espectral</a> centrada no verde, conhecida como a linha 5007 Ångström, gerada pela dupla ionização do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background: none; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a>.<span class="reference" id="cite_ref-seds_5-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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Praticamente nos limites da nebulosa, existe uma <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela variável">estrela variável</a>, em correlações com a nebulosa, chamada variável de Goldilocks. Esta nebulosa planetária apresenta uma aparência de <a href="http://pt.wikipedia.org/wiki/Esferoide" style="background: none; color: #0b0080; text-decoration: none;" title="Esferoide">esferoide</a> dilatada e é visível da perspetiva terrestre ao longo do plano de seu <a href="http://pt.wikipedia.org/wiki/Linha_do_equador" style="background: none; color: #0b0080; text-decoration: none;" title="Linha do equador">equador</a>.<span class="reference" id="cite_ref-seds_5-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere</a></span><br />
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<b>Com um abraço estrelado,</b><br />
<b>Janine Milward</b><br />
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background: none; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background: none; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background: none; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>CARO LEITOR,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">devem requerer do Caro Leitor</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Visitando os Sites abaixo,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<b><o:p></o:p></b></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> - AS CONSTELAÇÕES - </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> entre o céu e a terra..., </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vagarosamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> e este por nossa mente sendo conscientizado.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-42699906405769874442014-09-06T10:28:00.003-07:002015-04-02T09:18:21.084-07:00Virgo<div class="MsoNormal" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: -webkit-center;">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ao mergulharmos em <b>nossa visita</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>aos Objetos Messier constantes da constelação Virgo</b>,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">certamente estaremos também mergulhando</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em grande parte do Aglomerado de Galáxias Virgo!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Aglomerado Virgo</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Este é o mais famoso aglomerado de galáxias. É bem maior do que qualquer outro grupo dentre 100 milhões de anos-luz. Existem cerca de 150 grandes galáxias nesse aglomerado e, pelo menos, mil conhecidas galáxias anãs. Este aglomerado domina completamente nosso pequeno pedaço do Universo e até nosso Grupo Local de galáxias vem sendo gravitacionalmente atraído por este aglomerado. No centro do aglomerado Virgo, encontram-se três grandes galáxias elípticas: M84, M86 e M87. Estas galáxias provavelmente formaram a partir da fusão de muitas galáxias menores e são bem mais massivas do que nossa própria galáxia.</i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(minha simples e direta tradução para o texto abaixo)</span><br />
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<tr><th colspan="2" style="vertical-align: middle;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html" style="background-color: white;"><span style="color: #073763;">Virgo Cluster</span></a></th></tr>
<tr><td style="vertical-align: middle;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html" style="background-color: white;"><span style="color: #073763;"></span></a></td><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">This is the most famous cluster of galaxies. It is much larger than any other group within 100 million light years. There are about 150 large galaxies in this cluster and at least a thousand known dwarf galaxies. This cluster completely dominates our tiny corner of the Universe, and even our Local Group of galaxies is being gravitationally pulled by this cluster. At the core of the Virgo cluster lie the three large elliptical galaxies M84, M86 and M87. These galaxies probably formed from the merger of many smaller galaxies and are much more massive than our own galaxy.<br /><br /><a href="http://www.atlasoftheuniverse.com/virgo.html">http://www.atlasoftheuniverse.com/virgo.html</a> - </span></span><span style="color: #073763;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="text-decoration: none;">Richard Powell</a><span style="color: #073763;">.</span><span style="background-color: white;"><span style="color: #073763;"><br /></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>O Aglomerado Virgem é um aglomerado massivo de galáxias que dominam o superaglomerado Virgo. Existem cerca de 2.000 galáxias nesse aglomerado (embora noventa por cento das mesmas sejam galáxias anãs). Este algomerado possui um diâmetro de aproximadamente 15 milhões de anos-luz - e o que não é tão maior do que nosso Grupo Local, porém contém cinquenta vezes mais galáxias. Este mapa mostra 600 das mais brilhantes galáxias dentro de 7.5 graus a partir do centro do aglomerado - essa é uma divisa arbitrária, existem muitas outras galáxias para além desse limite, especialmente em direção ao sul do aglomerado, onde existem vários outros grupos de galáxias adcionais. As 160 maiores galáxias são apresentadas neste mapa.</i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(tradução simples e literal de Janine para o texto abaixo)</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">The Virgo cluster is a massive cluster of galaxies which dominates the Virgo supercluster. There are roughly 2000 galaxies in this cluster (although ninety percent of them are dwarf galaxies). This cluster has a diameter of approximately 15 million light years which is not much larger than our Local Group but it contains fifty times the number of galaxies. This map shows 600 of the brightest galaxies within 7.5 degrees of the centre of the cluster - this is an arbitary border, there are many other galaxies beyond this limit especially to the south of the cluster where there are several additional galaxy groups. The 160 largest galaxies are labelled on this map. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763;">LEIA MAIS EM</span></span></div>
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<span lang="PT" style="line-height: 22px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html">http://www.atlasoftheuniverse.com/galgrps/vir.html</a></span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: normal; text-align: start;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="line-height: normal; text-align: start; text-decoration: none;">Richard Powell</a><span style="line-height: normal; text-align: start;">.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start; text-decoration: none;">Richard Powell</a><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">.</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><b style="color: black; font-family: 'Times New Roman';">Virgo Cluster Galaxies</b></span></span></div>
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http://apod.nasa.gov/apod/image/1104/201103_VirgoGCM_andreo.jpg</div>
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<b>Virgo Cluster Galaxies </b><br /><b>Image Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Copyright</a>: </b><a href="http://blog.deepskycolors.com/about.html">Rogelio Bernal Andreo</a></center>
<b>Explanation: </b>Well over a thousand galaxies are known members of <a href="http://www.seds.org/messier/more/virgo.html">the Virgo Cluster</a>, the closest large cluster of galaxies to our own <a href="http://www.atlasoftheuniverse.com/localgr.html">local group</a>. In fact, the galaxy cluster is difficult <a href="http://www.atlasoftheuniverse.com/galgrps/vir.html">to appreciate</a> all at once because it covers such a large area on the sky. Spanning about 5x3 degrees, this careful <a href="http://blog.deepskycolors.com/archive/2011/03/18/virgo-Cluster-Deep-Widefield.html">mosaic of telescopic images</a> clearly records the central region of the Virgo Cluster through faint <a href="http://www.galaxyimages.com/UNP1.html">foreground dust</a> clouds lingering above the plane of our own Milky Way galaxy. The cluster's dominant giant elliptical <a href="http://apod.nasa.gov/apod/ap100520.html">galaxy M87</a>, is just below center in the frame. Above M87 is the famous interacting galaxy pair NGC 4438, also known <a href="http://apod.nasa.gov/apod/ap070608.html">as The Eyes</a>. A closer examination of the image will reveal many Virgo cluster member galaxies as small fuzzy patches. Sliding your cursor over the image will label the larger galaxies using <a href="http://apod.nasa.gov/apod/ap990429.html">NGC catalog</a> designations. Galaxies are also shown with <a href="http://www.seds.org/messier/xtra/history/m-cat-i.html">Messier catalog</a> numbers, including <a href="http://apod.nasa.gov/apod/ap080425.html">M84, M86</a>, and prominent colorful spirals <a href="http://apod.nasa.gov/apod/ap100130.html">M88</a>, <a href="http://apod.nasa.gov/apod/ap960316.html">M90</a>, and M91. On average, Virgo Cluster galaxies are measured to be about 48 million light-years away. <a href="http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1996PASP%2E%2E108%2E1091V">The Virgo Cluster distance</a> has been used to give an important determination of the Hubble Constant and <a href="http://antwrp.gsfc.nasa.gov/diamond_jubilee/debate96.html">the scale of the Universe</a>. (<i>Editor's Note:</i> Labels courtesy of <a href="http://astrometry.net/">Astrometry.net</a>.)<br />
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<b>Virgo Cluster Galaxies </b><br />Image Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Copyright</a>:<b> </b><a href="http://blog.deepskycolors.com/about.html">Rogelio Bernal Andreo</a></center>
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(<i>Editor's Note:</i> Labels courtesy of <a href="http://astrometry.net/">Astrometry.net</a>.)</center>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">OS OBJETOS MESSIER</span></b></center>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">ACOLHIDOS PELA CONSTELAÇÃO VIRGO:</span></b></center>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Virgo é o mais próximo dos grandes Aglomerados de Galáxias</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> de forma que muitas de suas brilhantes galáxias </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>podem ser observadas por telescópios amadores</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>(como por exemplo M84 e M86).</b></span></div>
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"></span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Caro Leitor,</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>veja que um dos mais conhecidos Objetos Messier</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> (ou o mais conhecido!) </b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>acolhidos pela constelação da Virgem</b></span></div>
<div style="line-height: 18.2000007629395px;">
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>encontra-se mais ao sul da Linha da Eclíptica</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e bem extremamente próximo à divisa entre Virgo e Corvus:</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>é o Objeto Messier 104</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>mais conhecido como o Sombreiro ou Sombrero!</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Todos os demais Objetos Messier</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>acolhidos pela constelação da Virgem</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>podem ser encontrados praticamente em linha reta a partir do Sombreiro,</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>porém em direção ao norte da Linha da Eclíptica</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e em direção da constelação Coma Berenices:</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M49, M58, M59, M60, M61, M84, M86, M87, M89 e M90</b></span></div>
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Carta Celeste realizada por Mario Jaci Monteiro - CARJ<br />(a imagem ao inverso foi realizada por Janine)</span></td></tr>
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<span style="color: #783f04; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
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<span style="color: #783f04; font-family: Arial, Helvetica, sans-serif;"><b>NA CONSTELAÇÃO VIRGO</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Primeiramente, Caro Leitor,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">estaremos comentando um tantinho</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Messier</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">acolhidos pela constelação da Virgem</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">e</span></b></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">encontrados mais ao norte da Linha da Eclíptica:</span></b></div>
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<a href="http://messier.obspm.fr/m/m049.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M49</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> elliptical galaxy (type E1 or S0_1(1))</span><br />
<a href="http://messier.obspm.fr/m/m058.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M58</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> spiral galaxy (type Sab(s)II)</span><br />
<a href="http://messier.obspm.fr/m/m059.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M59</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> elliptical galaxy (type E5)</span><br />
<a href="http://messier.obspm.fr/m/m060.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M60</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> elliptical galaxy (type E2 or S0_1(2))</span><br />
<a href="http://messier.obspm.fr/m/m061.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M61</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> spiral galaxy (type Sc(s)I.2)</span><br />
<a href="http://messier.obspm.fr/m/m084.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M84</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> elliptical or lenticular galaxy (type SB0_2/3(r)(3))</span><br />
<a href="http://messier.obspm.fr/m/m086.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">M86</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;"> elliptical galaxy (type E3 or S0_1(3))</span><br />
<a href="http://messier.obspm.fr/m/m087.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">M87</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;"> </span><b style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">Virgo A </b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">elliptical galaxy (type E0), with Smoking Gun</span><br />
<a href="http://messier.obspm.fr/m/m089.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;">M89</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: start;"> elliptical galaxy (type E0)</span><br />
<a href="http://messier.obspm.fr/m/m090.html" style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: normal;">M90</a><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal;"> spiral galaxy (type Sab(s)I-II)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste - constelação Virgo</span><br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m49atlas.jpg" /></div>
<span style="line-height: 18.2000007629395px;"><a href="http://www.ipac.caltech.edu/2mass/gallery/m49atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m49atlas.jpg</a></span><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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Messier 49</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Elliptical Galaxy</a> M49 (NGC 4472)</i>, type E4, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m49.jpg"><img align="right" alt="[m49.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m49.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 29.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+08 : 00 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">9x7.5 (arc min)</td></tr>
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Discovered 1771 by Charles Messier.</div>
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Elliptical galaxy Messier 49 (M49, NGC 4472) is one of the brightest member galaxies of the <a href="http://messier.obspm.fr/more/virgo.html">Virgo cluster</a>.</div>
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M49 was the first member of the Virgo cluster of galaxies to be discovered, by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M49">cataloged it</a> on February 19, 1771. It is also the second galaxy discovered beyond the Local Group after Lacaille's discovery of <a href="http://messier.obspm.fr/m/m083.html">M83</a>.<br />
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LEIA MAIS<br />
em</div>
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<a href="http://messier.obspm.fr/m/m049.html">http://messier.obspm.fr/m/m049.html</a></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/29/Messier_49_Hubble_WikiSky.jpg/800px-Messier_49_Hubble_WikiSky.jpg" /></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_49#mediaviewer/File:Messier_49_Hubble_WikiSky.jpg">http://pt.wikipedia.org/wiki/Messier_49#mediaviewer/File:Messier_49_Hubble_WikiSky.jpg</a></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Messier 49 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://wikisky.org/snapshot?img_size=&img_res=&ra=12.495925240874536&de=8.003754796726883&angle=0.05587008343265793&projection=tan&rotation=24.593242760491712&survey=astrophoto&img_id=905786&width=4000&height=4000&img_borders=0&interpolation=bicubic2&jpeg_quality=0.8" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<b style="line-height: 18.2000007629395px;"><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">NGC 4472 - M49 - Galáxia</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h28m Declinação +08<sup>o</sup>.08</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo (Classificação Hubble) E - Galáxia Elíptica Magnitude fotográfica aparente 9,33</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões Angulares 9,8 X 6,6 Distância (milhões de anos-luz) 37,0</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M 49 - NGC 4472 - </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma galáxia elíptica, com magnitude 9.1 e tamanho de 8’x7’,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> localizada a 5<sup>o</sup>. ao sul de M87. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma das galáxias mais brilhantes do grupo de Virgo, situada a 4/7 da reta imaginária que vai de Denebola a Delta da Virgem, a cerca de 4<sup>o</sup>. a oeste de 32 Virginis e próxima a uma estrela de quinta magnitude.</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Em sua vizinhança encontramos</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> <b>NGC 4535 e NGC 4526 e NGC 4365.</b> </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda outras tantas galáxias rodeiam M 49.</span><br />
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></b><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></b><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">.........................</span></b></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">É uma das </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia">galáxias</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> mais brilhantes pertencentes ao </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de Virgem</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, com uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> 8,5, correspondente a uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> -22,8, consdierando sua distância de 60 milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. É uma das </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia elíptica">galáxias elípticas</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> gigantes desse aglomerado (juntamente com </span><a href="http://pt.wikipedia.org/wiki/Messier_60" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 60">Messier 60</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e </span><a href="http://pt.wikipedia.org/wiki/Messier_87" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 87">Messier 87</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">), e pertence à classe E4 segundo a classificação de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Têm um diâmetro aparente de 9 x 7,5 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de grau</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, correspondendo a um </span><a href="http://pt.wikipedia.org/wiki/Elipsoide" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Elipsoide">elipsoide</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> com </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Semi-eixo_maior" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Semi-eixo maior">semi-eixo maior</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">de 160 000 anos-luz. É menos maciça que sua companheira, </span><a href="http://pt.wikipedia.org/wiki/Messier_87" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 87">Messier 87</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, embora seja maior em extensão. Pertencente à </span><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Classificação estelar">classe espectral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> integrada G7 e </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/%C3%8Dndice_de_cor" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Índice de cor">índice de cor</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> +0,76, é mais amarelada do que a maioria das galáxias do aglomerado de Virgem.</span><span class="reference" id="cite_ref-seds_2-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 49</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_49_Hubble_WikiSky.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="4000" data-file-width="4000" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/29/Messier_49_Hubble_WikiSky.jpg/280px-Messier_49_Hubble_WikiSky.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/29/Messier_49_Hubble_WikiSky.jpg/420px-Messier_49_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/29/Messier_49_Hubble_WikiSky.jpg/560px-Messier_49_Hubble_WikiSky.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 49, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1771" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1771">1771</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">E4, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=LINER&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="LINER (página não existe)">LINER</a><span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 29<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 46,7<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+08° 00′ 02″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">60 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (18,4<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">mpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">0,003326 ± 0,000022<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">9,4<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">10,2 × 8,3 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4472, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7629, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 41220, <a href="http://pt.wikipedia.org/wiki/Atlas_of_Peculiar_Galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atlas of Peculiar Galaxies">Arp</a> 134.<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_49#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 49"><img alt="Messier 49" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m58atlas.jpg" /></div>
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<span style="line-height: 18.2000007629395px;"><a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span> <span style="line-height: 18.2000007629395px;"><br /></span><br />
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Messier 58</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M58 (NGC 4579)</i>, type SBc, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m58.jpg"><img align="right" alt="[m58.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m58.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 37.7 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+11 : 49 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">5.5x4.5 (arc min)</td></tr>
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Discovered 1779 by Charles Messier.<br />
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Messier 58 (M58, NGC 4579) is one of the four barred spiral galaxies in Messier's catalog (the others are <a href="http://messier.obspm.fr/m/m091.html">M91</a>, <a href="http://messier.obspm.fr/m/m095.html">M95</a>,and <a href="http://messier.obspm.fr/m/m109.html">M109</a>), although it is sometimes classified as intermediate between normal and barred spirals (e.g., in R. Brent Tully's<i>Nearby Galaxies Catalog</i>). It is one of the brightest galaxies in the <a href="http://messier.obspm.fr/more/virgo.html">Virgo cluster</a>.<br />
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<a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> discovered M58, together with the apparently nearby elliptical galaxies <a href="http://messier.obspm.fr/m/m059.html">M59</a> and <a href="http://messier.obspm.fr/m/m060.html">M60</a>, on the occasion of following the comet of 1779, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M58">cataloged it</a> on April 15, 1779.<br />
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LEIA MAIS<br />
em</div>
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<a href="http://messier.obspm.fr/m/m058.html">http://messier.obspm.fr/m/m058.html</a><br />
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<img src="http://upload.wikimedia.org/wikipedia/commons/e/ea/M58s.jpg" height="522" width="640" /></div>
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http://pt.wikipedia.org/wiki/Messier_58#mediaviewer/File:M58s.jpg</div>
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Messier 58, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a></div>
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An <a class="extiw" href="http://en.wikipedia.org/wiki/infrared" style="background: none; color: #0b0080; text-decoration: none;" title="en:infrared">en:infrared</a> image of M 58 by the <a class="extiw" href="http://en.wikipedia.org/wiki/Spitzer_Space_Telescope" style="background: none; color: #0b0080; text-decoration: none;" title="en:Spitzer Space Telescope">en:Spitzer Space Telescope</a> Credit: SIRTF/<a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>/<a class="extiw" href="http://en.wikipedia.org/wiki/JPL" style="background: none; color: #0b0080; text-decoration: none;" title="en:JPL">en:JPL</a>. <a class="external free" href="http://www.spitzer.caltech.edu/images/2265-sig06-003-NGC-4579" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.spitzer.caltech.edu/images/2265-sig06-003-NGC-4579</a></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M58 - NGC 4579</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12H37M44 Declinação +11<sup>O</sup>.49 11</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 9.66:1.48 dimensões 5.89x4.68</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M 58 é uma galáxia espiral com aquilo que podemos denominar de barra central. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com magnitude de 11, é uma galáxia irregular</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e bem condensada </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de maneira que pode ser observada </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">mais facilmente do que sua magnitude poderia indicar.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white;"><img src="http://upload.wikimedia.org/wikipedia/commons/f/f7/M58_3.6_5.8_8.0_microns_spitzer.png" height="640" width="566" /></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Messier_58#mediaviewer/File:M58_3.6_5.8_8.0_microns_spitzer.png">http://pt.wikipedia.org/wiki/Messier_58#mediaviewer/File:M58_3.6_5.8_8.0_microns_spitzer.png</a></span></span></div>
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<span style="background-color: white;"><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; line-height: 24px; text-align: start;">M58 3.6 5.8 8.0 microns spitzer</span></span></div>
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O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> descobriu a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">galáxia espiral barrada</a> juntamente com duas outras galáxias companheiras aparentes, <a href="http://pt.wikipedia.org/wiki/Messier_59" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 59">Messier 59</a> e <a href="http://pt.wikipedia.org/wiki/Messier_60" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 60">Messier 60</a>, enquanto acomapanhava o progresso de um <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometa</a> em 1779. Adicionou-a em seu<a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> em 15 de abril daquele ano, e a galáxia é uma das primeiras a ser reconhecida como tal, listada por <a href="http://pt.wikipedia.org/wiki/William_Parsons" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Parsons">William Parsons</a>como uma de suas 14 galáxias espirais por ele listadas em 1850.<span class="reference" id="cite_ref-seds_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_58#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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Em pequenos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pios" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópios">telescópios</a>, a galáxia parece-se com muitas das <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxias elítpticas</a> do <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de Virgem</a>, exibindo seu núcleo brilhante. Em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> sob boas condições, um telescópio de 4 polegadas de abrtura pode distinguir um <a href="http://pt.wikipedia.org/wiki/Halo_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Halo galáctico">halo</a> em torno do núcleo, com pequenas condensações que parecem coincidir com os braços da galáxias. Com telescópios de 8 polegadas de abertura pode-se notar as primeiras pistas da <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">barra</a> associada ao núcleo.<span class="reference" id="cite_ref-seds_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_58#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">M58</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M58_3.6_5.8_8.0_microns_spitzer.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="200" data-file-width="177" src="http://upload.wikimedia.org/wikipedia/commons/f/f7/M58_3.6_5.8_8.0_microns_spitzer.png" height="316" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 58, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1779" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1779">1779</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">SAB(rs)b</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 37<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 43.5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+11° 49′ 05″</td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">68 M <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">1519 ± 6 km/s</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">+10.5</td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">5′.9 × 4′.7</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top">NGC 4579, UGC 7796, PGC 42168, VCC 1727</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_58">http://pt.wikipedia.org/wiki/Messier_58</a></span></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m59atlas.jpg" /></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.ipac.caltech.edu/2mass/gallery/m59atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m59atlas.jpg</a></span></span><br />
<span style="background-color: white;"><a href="https://www.blogger.com/null" name="m81">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span></div>
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<h1>
Messier 59</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Elliptical Galaxy</a> M59 (NGC 4621)</i>, type E5, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m59.jpg"><img align="right" alt="[m59.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m59.jpg" /></a><br />
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<tr><th align="left">Right Ascension</th><td align="center">12 : 42.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+11 : 39 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">5x3.5 (arc min)</td></tr>
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Discovered 1779 by Johann Gottfried Koehler.<br />
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Messier 59 (M59, NGC 4621) is a member of the <a href="http://messier.obspm.fr/more/virgo.html">Virgo cluster</a> of galaxies, and one of the larger elliptical galaxies there, although it is considerably less luminous and massive than the greatest ellipticals in this cluster, <a href="http://messier.obspm.fr/m/m049.html">M49</a>, <a href="http://messier.obspm.fr/m/m060.html">M60</a> and, above all,<a href="http://messier.obspm.fr/m/m087.html">M87</a>. ..............................<br />
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In our image, M59 is the elongated elliptical in the lower left, while in the right are <a href="http://messier.obspm.fr/m/m060.html">M60</a> and its companion NGC 4647, and at the top is faint NGC 4638, an elliptical with photographic mag 12.2.<br />
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LEIA MAIS<br />
em<br />
<a href="http://messier.obspm.fr/m/m059.html">http://messier.obspm.fr/m/m059.html</a><br />
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 59</span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier59.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="300" data-file-width="300" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/04/Messier59.jpg/280px-Messier59.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/0/04/Messier59.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/0/04/Messier59.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 5p, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Johann_Gottfried_Koehler" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann Gottfried Koehler">Johann Gottfried Koehler</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1779" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1779">1779</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a><span class="reference" id="cite_ref-sinnott1988_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-sinnott1988-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">E5<span class="reference" id="cite_ref-ned_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 02.3<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+11° 38′ 49″<span class="reference" id="cite_ref-ned_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">60 ± 5 M<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">al</a><span class="reference" id="cite_ref-tonryetal2001_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-tonryetal2001-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> (18,3 ± 1,7 M<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">410 ± 6 km/s<span class="reference" id="cite_ref-ned_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">+10,6<span class="reference" id="cite_ref-ned_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">5′.4 × 3′.7<span class="reference" id="cite_ref-ned_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4621, UGC 7858, PGC 42628<span class="reference" id="cite_ref-ned_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 59"><img alt="Messier 59" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> foi descoberta pelo alemão <a href="http://pt.wikipedia.org/wiki/Johann_Gottfried_K%C3%B6hler" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann Gottfried Köhler">Johann Gottfried Köhler</a> em 11 de abril de 1779, juntamente com <a href="http://pt.wikipedia.org/wiki/Messier_60" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 60">Messier 60</a> enquanto observava um <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Cometa">cometa</a> naquele ano, também observado por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que também redescobriu independentemente a galáxia e Messier 60 quatro dias depois e descobriu <a href="http://pt.wikipedia.org/wiki/Messier_58" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 58">Messier 58</a>, que Köhler não observou apesar da proximadade dessa galáxia às outras duas. Segundo Messier, é uma galáxia tão tênue quanto M58 e mais fraca do que M60.<span class="reference" id="cite_ref-seds_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-seds-4" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<span class="mw-headline" id="Caracter.C3.ADsticas">Características</span></h2>
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É uma das maiores <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxias elípticas</a> pertencentes a <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado de Virgem">galomerado de galáxias de Virgem</a>, apenas menor que <a href="http://pt.wikipedia.org/wiki/Messier_60" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 60">Messier 60</a> e<a href="http://pt.wikipedia.org/wiki/Messier_87" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 87">Messier 87</a>. Está situado a uma distância de 60 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e seu diâmetro aparente de 5 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de grau</a> ao longo de seu <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Semi-eixo_maior" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Semi-eixo maior">semi-eixo maior</a> corresponde a um diâmetro real de 87 000 anos-luz.<span class="reference" id="cite_ref-seds_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_59#cite_note-seds-4" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_59">http://pt.wikipedia.org/wiki/Messier_59</a></span></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m60atlas.jpg" /></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a><a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a><br />
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Messier 60</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Elliptical Galaxy</a> M60 (NGC 4649)</i>, type E2, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m60.jpg"><img align="right" alt="[m60.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m60.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 43.7 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+11 : 33 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">7x6 (arc min)</td></tr>
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Discovered 1779 by Johann Gottfried Koehler.<br />
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Messier 60 (M60, NGC 4649) is one of the giant elliptical galaxies in the <a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster of galaxies</a>. As the most following (eastern) Messier galaxy in this cluster, it is the last in a row of three (<a href="http://messier.obspm.fr/m/m058.html">M58</a>, <a href="http://messier.obspm.fr/m/m059.html">M59</a>, and M60), which comes into the field of view of a telescope pointed to this region of the sky. At lower magnifications, it lies in the same field of view as M59 (25 arc minutes away).<br />
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M60 was discovered by <a href="http://messier.obspm.fr/xtra/Bios/koehler.html">Johann Gottfried Koehler</a> on April 11, 1779, when he was following the comet of that year, together with neighboring M59. It was independently found one day later by <a href="http://messier.obspm.fr/xtra/Bios/oriani.html">Barnabus Oriani</a>, who missed M59, and four days later, on April 15, 1779, by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who also found nearby M58. Messier <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M60">describes M60</a> as "a little more distinct" than M58 and M59.</div>
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The Hubble Space telescope has <a href="http://messier.obspm.fr/more/m060_hst.html">investigated M60's core</a> and found evidence that it contans a <a href="http://messier.obspm.fr/xtra/supp/mdo.html">massive central object</a> of about 2 billion solar masses.<br />
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LEIA MAIS<br />
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<a href="http://messier.obspm.fr/m/m060.html">http://messier.obspm.fr/m/m060.html</a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;">http://pt.wikipedia.org/wiki/Messier_60#mediaviewer/File:Messier_60_Hubble_WikiSky.jpg</span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 60 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool</span></span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia">galáxia</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> foi descoberta pelo alemão </span><a href="http://pt.wikipedia.org/wiki/Johann_Gottfried_K%C3%B6hler" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Johann Gottfried Köhler">Johann Gottfried Köhler</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 11 de abril de 1779, juntamente com </span><a href="http://pt.wikipedia.org/wiki/Messier_59" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 59">Messier 59</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> enquanto observava um </span><a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Cometa">cometa</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> naquele ano, também observado por </span><a href="http://pt.wikipedia.org/wiki/Barnaba_Oriani" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Barnaba Oriani">Barnaba Oriani</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que não observou </span><a href="http://pt.wikipedia.org/wiki/Messier_59" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 59">Messier 59</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, e </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que também redescobriu independentemente a galáxia e Messier 60 quatro dias depois e descobriu </span><a href="http://pt.wikipedia.org/wiki/Messier_58" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 58">Messier 58</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que Köhler não observou apesar da proximadade dessa galáxia às outras duas. Segundo Messier, é uma galáxia mais brilhante do que M58 e M59.</span><span class="reference" id="cite_ref-seds_5-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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É uma das maiores <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxias elípticas</a> pertencentes a <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de galáxias de Virgem</a>. Situado a uma distância de 60 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, o diâmetro aparente de seu <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Semi-eixo_maior" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Semi-eixo maior">semi-eixo maior</a> de 7 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de grau</a> corresponde a um diâmetro real de 122 000 anos-luz. Entretanto, com pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores é possível visualizar apenas seu <a href="http://pt.wikipedia.org/wiki/N%C3%BAcleo_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Núcleo galáctico">núcleo</a> galáctico de diâmetro aparente de 4 x 3 minutos.<span class="reference" id="cite_ref-seds_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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Sua <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 9 corresponde a uma galáxia brilhante, de <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> -22,3, correspondendo a uma luminosidade 60 bilhões de vezes maior do que a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luminosidade_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Luminosidade solar">luminosidade solar</a>. De acordo com William E. Harris, M60 contém 5 100<a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a> em seu <a href="http://pt.wikipedia.org/wiki/Halo_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Halo galáctico">halo</a>. Segundo pesquisas realizadas com o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a>, há evidências sobre a existência de um <a href="http://pt.wikipedia.org/wiki/Buraco_negro_supermaci%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Buraco negro supermaciço">buraco negro supermaciço</a> seu seu núcleo, com massa equivalente a 2 bilhões de vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massa solar</a>.<span class="reference" id="cite_ref-seds_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 60</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_60_Hubble_WikiSky.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="4000" data-file-width="4000" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a4/Messier_60_Hubble_WikiSky.jpg/280px-Messier_60_Hubble_WikiSky.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a4/Messier_60_Hubble_WikiSky.jpg/420px-Messier_60_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a4/Messier_60_Hubble_WikiSky.jpg/560px-Messier_60_Hubble_WikiSky.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 60, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Johann_Gottfried_Koehler" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann Gottfried Koehler">Johann Gottfried Koehler</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1779" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1779">1779</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a><span class="reference" id="cite_ref-sinnott1988_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-sinnott1988-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">E2<span class="reference" id="cite_ref-ned_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 43<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 39.6<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+11° 33′ 09″<span class="reference" id="cite_ref-ned_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">55 ± 4 M<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">al</a><span class="reference" id="cite_ref-tonryetal2001_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-tonryetal2001-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> (16,8 ± 1,2 M<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">1117 ± 6 km/s<span class="reference" id="cite_ref-ned_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">+9,8<span class="reference" id="cite_ref-ned_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">7′.4 × 6′.0<span class="reference" id="cite_ref-ned_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top">M60, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4649,<span class="reference" id="cite_ref-ned_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7898,<span class="reference" id="cite_ref-ned_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 42831<span class="reference" id="cite_ref-ned_2-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> <a href="http://pt.wikipedia.org/wiki/Atlas_of_Peculiar_Galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atlas of Peculiar Galaxies">Arp</a>116<span class="reference" id="cite_ref-ned_2-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_60#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 60"><img alt="Messier 60" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_60">http://pt.wikipedia.org/wiki/Messier_60</a></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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Messier 61</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M61 (NGC 4303)</i>, type SABbc, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 21.9 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+04 : 28 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">6x5.5 (arc min)</td></tr>
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Discovered 1779 by Barnabus Oriani.<br />
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Messier 61 (M61, NGC 4303) is a considerable spiral galaxy in the southernmost part of the <a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster of Galaxies</a>.<br />
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M61 was discovered by <a href="http://messier.obspm.fr/xtra/Bios/oriani.html">Barnabus Oriani</a> on May 5, 1779 when following the comet of that year, 6 days before <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>'s <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M61">discovery</a>, who had seen it on the same day as Oriani but mistaken it for the comet. Messier mistook it for two nights more, until he realized that it did not move.<br />
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LEIA MAIS<br />
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<a href="http://messier.obspm.fr/m/m061.html">http://messier.obspm.fr/m/m061.html</a></div>
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<span style="background-color: white; font-family: Georgia, serif; line-height: 19.5px; text-align: start;">The galaxy known as M61 as seen by Hubble. Credit: ESA/Hubble & NAS, Acknowledgement: Det58</span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> foi descoberta por </span><a href="http://pt.wikipedia.org/wiki/Barnaba_Oriani" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Barnaba Oriani">Barnaba Oriani</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 5 de maio de 1771 enquanto seguia o </span><a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Cometa">cometa</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> daquele ano, seis dias antes de o astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> redescobriu independente o objeto enquanto também observava o cometa. Messier visualizou a galáxia no mesmo dia que Oriani, mas confundiu-a com o próprio cometa, cometendo o mesmo erro nos dias seguintes, chegando à conclusão de que o objeto não movia em 11 de maio. Foi catalogado por </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="William Herschel">William Herschel</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, descobridor de </span><a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Urano (planeta)">Urano</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, como o objeto H I.139 embora Herschel não costumasse catalogar objetos já catalogados por Messier.</span><span class="reference" id="cite_ref-seds_1-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_61#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">É uma das maiores </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xias" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxias">galáxias</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> do </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de Virgem</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">; seu diâmetro aparente de 6 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de grau</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> corresponde a um diâmetro real de 105 000 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, considerando sua distância em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de 60 milhões de anos-luz. Sua </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">10 equivale a uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> -21,2.</span><span class="reference" id="cite_ref-seds_1-1" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_61#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 61</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
<div class="floatnone" style="margin-left: auto; margin-right: auto;">
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ngc4303-hst-R814GB450.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="2050" data-file-width="2050" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/73/Ngc4303-hst-R814GB450.jpg/280px-Ngc4303-hst-R814GB450.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/73/Ngc4303-hst-R814GB450.jpg/420px-Ngc4303-hst-R814GB450.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/73/Ngc4303-hst-R814GB450.jpg/560px-Ngc4303-hst-R814GB450.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 61, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Barnabus_Oriani" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Barnabus Oriani">Barnabus Oriani</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/5_de_Maio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="5 de Maio">5 de Maiode</a> <a href="http://pt.wikipedia.org/wiki/1779" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1779">1779</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> SABbc</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 21<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 54,895<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+04° 28' 25,13"</td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">~60 <a href="http://pt.wikipedia.org/wiki/Milh%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Milhão">milhão</a> <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (~18,4 milhão <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">9,7</td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">6' x 5,5’</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Características físicas</b></th></tr>
<tr><td scope="row" valign="top">Raio</td><td valign="top">100 mil <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">Magnit. abs.</a></td><td valign="top">-21,2</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><center>
M61, NGC 4303</center>
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<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><div style="position: relative;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 61"><img alt="Messier 61" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_61">http://pt.wikipedia.org/wiki/Messier_61</a></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEguhn66q5Q8U008xlWte37RJD9BgJET30SF2LjhLVBYWJnsRMnDjJLkARBDm0At59buFfLaAtMrsatJW4fbw-fq1ngSOZVudXTGaX3F17nltrh9b-JKOc-CVVCkZcEiVJNDI31XNUWdioE/s1600/MakariansChain+(1).jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEguhn66q5Q8U008xlWte37RJD9BgJET30SF2LjhLVBYWJnsRMnDjJLkARBDm0At59buFfLaAtMrsatJW4fbw-fq1ngSOZVudXTGaX3F17nltrh9b-JKOc-CVVCkZcEiVJNDI31XNUWdioE/s1600/MakariansChain+(1).jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="line-height: 18px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The Virgo Cluster</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">[JLC] </span><a href="http://asterisk.apod.com/viewtopic.php?f=29&t=31295&start=125#p199678" rel="nofollow nofollow" style="cursor: pointer; line-height: 18px; text-decoration: none;" target="_blank">http://asterisk.apod.com/<wbr></wbr><span class="word_break" style="display: inline-block;"></span>viewtopic.php?f=29&t=31295&<wbr></wbr><span class="word_break" style="display: inline-block;"></span>start=125#p199678</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; line-height: 18px;">Copyright: Stephen Mounioloux</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhy-8A1Ug-E2awxzf57A1MAdOQuksxaOwZVgLc-lpbhWXJB29rVZhj4iPzaP3gv-qydWyJn1VoGwgZWlfVRyNICb8ZRbCF25SWbu_fPk5oVrczWanVKjD0ESnEmVX_OSNxwJSu79Cvy6P4/s1600/NGC4438_NGC4435_crawford_rc720.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhy-8A1Ug-E2awxzf57A1MAdOQuksxaOwZVgLc-lpbhWXJB29rVZhj4iPzaP3gv-qydWyJn1VoGwgZWlfVRyNICb8ZRbCF25SWbu_fPk5oVrczWanVKjD0ESnEmVX_OSNxwJSu79Cvy6P4/s1600/NGC4438_NGC4435_crawford_rc720.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></span></a></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://apod.nasa.gov/apod/ap070608.html">http://apod.nasa.gov/apod/ap070608.html</a></span></span></span><br />
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><b>Markarian's Eyes </b><br /><b>Credit & Copyright: </b><a href="http://rdelsol.com/mailme.htm" style="text-decoration: none;">Ken Crawford</a> (<a href="http://rdelsol.com/" style="text-decoration: none;">Rancho Del Sol Observatory</a>)</span></span></center>
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Explanation: <b>Across the heart of the Virgo Galaxy Cluster lies a string of galaxies known as <a href="http://apod.nasa.gov/apod/ap061011.html" style="text-decoration: none;">Markarian's Chain</a></b>. Prominent in Markarian's Chain are these <b>two interacting galaxies</b>, <b>NGC 4438 (left) and NGC 4435 - also known as The Eyes</b>. About 50 million light-years away, the two <a href="http://www.messier45.com/cgi-bin/dsdb/dsb.pl?str=NGC+4438" style="text-decoration: none;">galaxies appear</a> to be about 100,000 light-years apart in <a href="http://www.rdelsol.com/Galaxy/NGC4435_NGC4438.html" style="text-decoration: none;">this sharp close-up</a>, but have likely approached to within an estimated 16,000 light-years of each other in their <a href="http://chandra.harvard.edu/photo/cosmic_lookback.html" style="text-decoration: none;">cosmic past</a>. Gravitational tides from <a href="http://chandra.harvard.edu/photo/2003/ngc4438/" style="text-decoration: none;">the close encounter</a> have ripped away at their stars, gas, and dust. The more massive NGC 4438 managed to hold on to much of the material torn out in the<a href="http://burro.cwru.edu/JavaLab/GalCrashWeb/main.html" style="text-decoration: none;">collision</a>, while material from the smaller NGC 4435 was more <a href="http://www.astropix.com/wp/2007/05/13/ngc-4438-and-ngc-4435/" style="text-decoration: none;">easily lost</a>. The remarkably deep image of this crowded region <a href="http://bigpicture.caltech.edu/" style="text-decoration: none;">of the universe</a> also includes many more distant background galaxies.</span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Os Olhos</span></b><span style="color: #073763;"> são um par de galáxias </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">situadas bem neste ponto central:</span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><b>NGC4438</b>, um dos dois Olhos, </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">é uma galáxia brilhante e razoavelmente grande,</span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> enquanto <b>NGC 4435</b>, </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">um tantinho ao norte, </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">é bem brilhante (magnitude 11.7) </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">e bem grande e arredondada (2.8’x2’).</span></span></div>
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2009 June 9<br /><a href="http://apod.nasa.gov/apod/image/0906/markarian_sadowski_big.jpg"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/0906/markarian_sadowski.jpg" /></a></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/ap090609.html">http://apod.nasa.gov/apod/ap090609.html</a></span></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Markarian's Chain of Galaxies </b><br /><b>Credit & Copyright: </b><a href="mailto: piotr_sadowski at wr.home.pl">Piotrek Sadowski</a></span></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>Across the heart of the <a href="http://en.wikipedia.org/wiki/Virgo_Cluster">Virgo Cluster of Galaxies</a> lies a striking string of galaxies known as Markarian's Chain. The chain, <a href="http://www.astrofotografia.com.pl/photogallery/Markarians_Chain/markarian_full.jpg">pictured above</a>, is highlighted on the upper right with two large but featureless <a href="http://www.seds.org/messier/lenticul.html">lenticular</a> galaxies, <a href="http://www.seds.org/messier/m/m084.html">M84</a> and<a href="http://www.seds.org/messier/m/m086.html">M86</a>. Prominent to their lower left is a pair of interacting galaxies known as <a href="http://apod.nasa.gov/apod/ap070608.html">The Eyes</a>. The home <a href="http://www.seds.org/messier/more/virgo.html">Virgo Cluster</a> is the nearest <a href="http://www.astr.ua.edu/white/mug/cluster/clusters.html">cluster of galaxies</a>, contains over 2000 galaxies, and has a noticeable gravitational pull on the galaxies of the <a href="http://www.seds.org/messier/more/local.html">Local Group of Galaxies</a> surrounding our <a href="http://apod.nasa.gov/apod/ap070930.html">Milky Way Galaxy</a>. The <a href="http://apod.nasa.gov/apod/ap050213.html">center</a> of the <a href="http://www.seds.org/messier/more/virgo.html">Virgo Cluster</a> is located about 70 million <a href="http://chandra.harvard.edu/photo/cosmic_distance.html">light years</a> away toward the <a href="http://www.astro.wisc.edu/~dolan/constellations/extra/constellations.html">constellation</a> of <a href="http://en.wikipedia.org/wiki/Virgo_(constellation)">Virgo</a>. At least seven galaxies in <a href="http://www.astropix.com/HTML/C_SPRING/MARKS.HTM">the chain</a> <a href="http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1983AN....304...69L">appear to move coherently</a>, although others appear to be superposed by chance.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>A <metricconverter productid="23’" w:st="on">23’</metricconverter> oeste dos Olhos,</b> </span><br />
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;">situam-se a galáxia elíptica <b><span style="color: #660000;">M86 - NGC 4406</span></b> -, com magnitude 9.8 e tamanho de 9’x6’ </span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;">e a galáxia <b><span style="color: #660000;">M84 - NGC 4374</span></b> -,</span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"> com magnitude 10, tamanho 6.4’x5.6’.</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M84 - NGC 4374</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h25m03 declinação +12<sup>o</sup>.53 15</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.11:10.09 dimensões 6.46x5.62</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M86 - NGC 4406</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h26m11 declinação +12<sup>o</sup>.56 49</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 8.90:9.83 dimensões 8.91x5.75</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M86 apresenta um anel de galáxias formando um colar </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e estes objetos podem ser vistos em telescópios de abertura <metricconverter productid="8”" w:st="on">8”</metricconverter> ou 10”:</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> NGC 4402, NGC 4387, NGC 4388, NGC 4413, NGC 4425.</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M87 - NGC 4486 - Galáxia</span></b><br />
<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">Virgo A</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h30m49 declinação +12<sup>o</sup>.23 24</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 8.63:9.59 dimensões 8.32x6.61</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um dos maiores membros do Aglomerado de Galáxias em Virgem, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma galáxia brilhante e eliptical</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e uma das mais massivas e luminosas galáxias conhecidas. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao mesmo tempo, é uma das mais vigorosas fontes de radiação de radio, </span></div>
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;">designada como <b><span style="color: #660000;">Virgo A</span></b> ou pelo número <metricconverter productid="3C" style="color: black;" w:st="on">3C</metricconverter> 274 (Catálogo de Fontes de Radio). </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Sua poderosa radiação de rádio e também a poderosa emissão de raio-x </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acontecem como um jato luminoso que se extende para mais de 4 mil anos-luz</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> para fóra do núcleo da galáxia. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dentro do núcleo podemos encontrar um jato de elétrons, acelerado por um campo magnético bem forte e para velocidade imensa:</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> isso faz acontecer uma radiação extremamente enérgica </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e estes processos podem ter sido causados,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> por exemplo, por um supermassivo buraco negro no núcleo da galáxia.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Aglomerado Virgo</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Este é o mais famoso aglomerado de galáxias. É bem maior do que qualquer outro grupo dentre 100 milhões de anos-luz. Existem cerca de 150 grandes galáxias nesse aglomerado e, pelo menos, mil conhecidas galáxias anãs. Este aglomerado domina completamente nosso pequeno pedaço do Universo e até nosso Grupo Local de galáxias vem sendo gravitacionalmente atraído por este aglomerado. <b>No centro do aglomerado Virgo, encontram-se três grandes galáxias elípticas: M84, M86 e M87</b>. Estas galáxias provavelmente formaram a partir da fusão de muitas galáxias menores e são bem mais massivas do que nossa própria galáxia.</i></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(minha simples e direta tradução para o texto abaixo</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- negrito Janine)</span></div>
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<tr><th colspan="2" style="vertical-align: middle;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html" style="background-color: white;"><span style="color: #073763;">Virgo Cluster</span></a></th></tr>
<tr><td style="vertical-align: middle;"><a href="http://www.atlasoftheuniverse.com/galgrps/vir.html" style="background-color: white;"><span style="color: #073763;"></span></a></td><td style="vertical-align: middle;"><span style="background-color: white;"><span style="color: #073763;">This is the most famous cluster of galaxies. It is much larger than any other group within 100 million light years. There are about 150 large galaxies in this cluster and at least a thousand known dwarf galaxies. This cluster completely dominates our tiny corner of the Universe, and even our Local Group of galaxies is being gravitationally pulled by this cluster. At the core of the Virgo cluster lie the three large elliptical galaxies M84, M86 and M87. These galaxies probably formed from the merger of many smaller galaxies and are much more massive than our own galaxy.<br /><br /><br /><a href="http://www.atlasoftheuniverse.com/virgo.html">http://www.atlasoftheuniverse.com/virgo.html</a> - </span></span><span style="color: #073763;">This website belongs to </span><a href="http://www.atlasoftheuniverse.com/me.html" style="text-decoration: none;">Richard Powell</a><span style="color: #073763;">.</span><span style="background-color: white;"><span style="color: #073763;"><br /></span></span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"><a href="http://apod.nasa.gov/apod/image/0906/markarian_sadowski_big.jpg">http://apod.nasa.gov/apod/image/0906/markarian_sadowski_big.jpg</a></span><br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m84atlas.jpg" /></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;">http://www.ipac.caltech.edu/2mass/gallery/m84atlas.jpg</span><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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<h1>
Messier 84</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Lenticular (S0) Galaxy</a> M84 (NGC 4374)</i>, type S0, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m84.jpg"><img align="right" alt="[m84.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m84.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 25.1 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 53 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.1 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">5.0 (arc min)</td></tr>
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Discovered 1781 by Charles Messier.<br />
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Messier 84 (M84, NGC 4374) is one of the brighter member galaxies of the <a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster of Galaxies</a>. It is a giant lenticular or elliptical galaxy: Either a lenticular of type S0 seen face-on, or an elliptical galaxy of type E1.<br />
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M84 has been discovered and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M84">cataloged</a> by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> on March 18, 1781 when he also cataloged 7 more nebulous objects in the same celestial region, all of them member galaxies of the Virgo Cluster, as well as <a href="http://messier.obspm.fr/m/m092.html">globular cluster M92</a>.<br />
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LEIA MAIS<br />
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<a href="http://messier.obspm.fr/m/m084.html">http://messier.obspm.fr/m/m084.html</a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://upload.wikimedia.org/wikipedia/commons/7/7a/Messier_84_nucleus_Hubble.jpg" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;">http://pt.wikipedia.org/wiki/Messier_84#mediaviewer/File:Messier_84_nucleus_Hubble.jpg</span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 84 nucleus Hubble</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source">Hubble source data: <a class="external autonumber" href="http://archive.stsci.edu/cgi-bin/mastpreview?mission=hst&dataid=J8FS06011" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">[1]</a>, <a class="external autonumber" href="http://archive.stsci.edu/cgi-bin/mastpreview?mission=hst&dataid=J8FS06021" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">[2]</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> foi originalmente descoberta pelo astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;" title="Charles Messier">Charles Messier</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que descobriu e </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Catálogo Messier">catalogou</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> 7 outros objetos na mesma noite, seis galáxias pertencentes ao </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de Virgem</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, </span><a href="http://pt.wikipedia.org/wiki/Messier_92" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 92">Messier 92</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><span class="reference" id="cite_ref-seds_5-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">É uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> ou </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia elíptica">elíptica</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> gigante e é um dos membros mais brilhantes do aglomerado de Virgem. Está situada na região central, super povoada por galáxias, do aglomerado. Historicamente, foi classificada como uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, mas há evidências que se trate de uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, contituída principalmente de estrelas amarelas velhas. Contém mais de 1000</span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, entretanto esse número é muito menor do que o encontrado em </span><a href="http://pt.wikipedia.org/wiki/Messier_87" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 87">Messier 87</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que marca o centro do aglomerado de Virgem.</span><span class="reference" id="cite_ref-seds_5-1" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 84</span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_84_nucleus_Hubble.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="656" data-file-width="633" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/7a/Messier_84_nucleus_Hubble.jpg/280px-Messier_84_nucleus_Hubble.jpg" height="290" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/7a/Messier_84_nucleus_Hubble.jpg/420px-Messier_84_nucleus_Hubble.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/7a/Messier_84_nucleus_Hubble.jpg/560px-Messier_84_nucleus_Hubble.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>M84<br />Crédito: <a class="new" href="http://pt.wikipedia.org/w/index.php?title=NOAO&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="NOAO (página não existe)">NOAO</a>.</small></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">E1<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 25<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 03,7<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+12° 53′ 13″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">60 ± 3 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (18,4 ± 0,9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)<span class="reference" id="cite_ref-tonryetal2001_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-tonryetal2001-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">1060 ± 6 km/s<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">10,1<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">6′.5 × 5′.6<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4374, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7494, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 40455, VCC 763.<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_84#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 84"><img alt="Messier 84" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_84">http://pt.wikipedia.org/wiki/Messier_84</a></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m86atlas.jpg" /></div>
<span style="line-height: 18.2000007629395px;">http://www.ipac.caltech.edu/2mass/gallery/m86atlas.jpg</span><br />
<span style="line-height: 18.2000007629395px;"><a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
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<h1>
Messier 86</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Lenticular (S0) Galaxy</a> M86 (NGC 4406)</i>, type S0, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m86.jpg"><img align="right" alt="[m86.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m86.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">12 : 26.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 57 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">7.5x5.5 (arc min)</td></tr>
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Discovered 1781 by Charles Messier.<br />
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Messier 86 (M86, NGC 4406) is one ogf the brightest member galaxies of the <a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster og Galaxies</a>, and situated close to that cluster's apparent center.<br />
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M86 has been discovered and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M86">cataloged</a> by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> on March 18, 1781 when he also cataloged 7 more nebulous objects in the same region of the sky, all member galaxies of the Virgo Cluster, and in addition, globular cluster <a href="http://messier.obspm.fr/m/m092.html">M92</a>.<br />
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LEIA MAIS<br />
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<a href="http://messier.obspm.fr/m/m086.html">http://messier.obspm.fr/m/m086.html</a><br />
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e5/Messier_86_Hubble_WikiSky.jpg/280px-Messier_86_Hubble_WikiSky.jpg" height="640" width="640" /></div>
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http://pt.wikipedia.org/wiki/Messier_86#mediaviewer/File:Messier_86_Hubble_WikiSky.jpg</div>
<div class="mw-mmv-title-para" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; line-height: 1.5em; overflow: visible; padding: 10px 20px 0px; text-overflow: ellipsis;">
<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 86 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Autor e informação sobre a fonte" style="cursor: pointer; font-size: 0.8em;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> </span></div>
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<b>Messier 86</b> (também conhecido como <b>M86</b> ou <b>NGC 4406</b>) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a>. Foi descoberta por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1781. Se situa no centro do <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado de Virgem">Aglomerado de Virgem</a> e forma um agrupamento com outra galáxia lenticular, <a href="http://pt.wikipedia.org/wiki/Messier_84" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 84">Messier 84</a>. Apresenta o maior <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Desvio_para_o_azul&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Desvio para o azul (página não existe)">desvio para o azul</a> de todos os objetos Messier, e está se aproximando da <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a> a uma velocidade de 244 km/s. Acredita-se que essa aproximação se deve ao fato de estar caindo em direção ao centro do Aglomerado de Virgem, o que deixa ela mais próxima da Via Láctea.<span class="reference" id="cite_ref-Jacobyetal2005_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-Jacobyetal2005-3" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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<span class="mw-headline" id="Descoberta_e_visualiza.C3.A7.C3.A3o">Descoberta e visualização</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a> foi descoberta pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 18 de março de 1981, quando decidiu realizar um empreendimento de observações de nebulosas que estavam naquela região da <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esfera celeste">esfera celeste</a>, na constelação de <a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgem</a>. Em apenas uma única noite, catalogou 8 <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a>, incluindo M86, além de um<a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a>, <a href="http://pt.wikipedia.org/wiki/Messier_92" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 92">Messier 92</a>.<span class="reference" id="cite_ref-seds_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-seds-4" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 86</span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_86_Hubble_WikiSky.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="3280" data-file-width="3280" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e5/Messier_86_Hubble_WikiSky.jpg/280px-Messier_86_Hubble_WikiSky.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/e5/Messier_86_Hubble_WikiSky.jpg/420px-Messier_86_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/e5/Messier_86_Hubble_WikiSky.jpg/560px-Messier_86_Hubble_WikiSky.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 86 pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">S0(3)/E3<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 26<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 11,7<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+12° 56′ 46″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">52 ± 3 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><br />
(15,9 ± 1,0 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)<span class="reference" id="cite_ref-jensenetal2003_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-jensenetal2003-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">-0,000814 +/- 0,000017<br />
(-244 ± 5 km/s)<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">9,8<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">8′,9 × 5′,8<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4406, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7532, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 40653, VCC 0881.<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_86#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 86"><img alt="Messier 86" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_86">http://pt.wikipedia.org/wiki/Messier_86</a><br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m87atlas.jpg" /></div>
<span style="line-height: 18.2000007629395px;">http://www.ipac.caltech.edu/2mass/gallery/m87atlas.jpg</span><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 87</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Elliptical Galaxy</a> M87 (NGC 4486)</i>, type E1, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a><b>Virgo A</b></center>
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<a href="http://messier.obspm.fr/Jpg/m87.jpg"><img align="right" alt="[m87.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m87.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 30.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 24 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">7.0 (arc min)</td></tr>
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Discovered 1781 by Charles Messier.<br />
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The giant elliptical galaxy Messier 87 (M87, NGC 4486), also called Virgo A, is one of the most remarkable objects in the sky. It is perhaps the dominant galaxy in the closest big cluster to us, the famous<a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster</a> of galaxies (sometimes also called "Coma-Virgo cluster" which is more acurate, as it extends into constellation Coma), and lies at the distance of this cluster (about 60 million light-years). M87 lies well in the <a href="http://messier.obspm.fr/more/m087_etc.html">heart of the Virgo cluster</a> (together with a lot of galaxies including <a href="http://messier.obspm.fr/m/m084.html">M84</a> and <a href="http://messier.obspm.fr/m/m086.html">M86</a>).<br />
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M87 has been discovered and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M87">cataloged</a> by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> on March 18, 1781 when he also cataloged 7 more nebulous objects in the same region, and actually are all member galaxies of the Virgo Cluster, as well as globular cluster <a href="http://messier.obspm.fr/m/m092.html">M92</a>.</div>
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LEIA MAIS<br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"><a href="http://messier.obspm.fr/m/m087.html">http://messier.obspm.fr/m/m087.html</a></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/8/83/M87_Super-Volcano.jpg/800px-M87_Super-Volcano.jpg" /><br />
<span style="background-color: white;">http://pt.wikipedia.org/wiki/Messier_87#mediaviewer/File:M87_Super-Volcano.jpg</span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">M87 Super-Volcano</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author">X-ray: NASA/CXC/KIPAC/N. Werner et al Radio: NSF/NRAO/AUI/W. Cotton</span> - <span class="mw-mmv-source"><a class="external text" href="http://www.nasa.gov/multimedia/imagegallery/image_feature_1743.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">NASA Image of the Day</a></span></span></div>
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Messier 87, <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">Observatório de raios-X Chandra</a></div>
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This image shows the eruption of a galactic “super-<a href="http://commons.wikimedia.org/wiki/Volcano" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Volcano">volcano</a>” in the massive galaxy M87, as witnessed by <a href="http://commons.wikimedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NASA">NASA's</a> <a href="http://commons.wikimedia.org/wiki/Category:Chandra_X-ray_Observatory" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Chandra X-ray Observatory">Chandra X-ray Observatory</a>and NSF's <a href="http://commons.wikimedia.org/wiki/Category:Very_Large_Array" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Category:Very Large Array">Very Large Array</a> (VLA). The cluster surrounding M87 is filled with hot gas glowing in <a href="http://commons.wikimedia.org/wiki/X-ray" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="X-ray">X-ray</a> <a href="http://commons.wikimedia.org/wiki/Light" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light">light</a> (and shown in <a href="http://commons.wikimedia.org/wiki/Blue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Blue">blue</a>) that is detected by Chandra. As this gas cools, it can fall toward the galaxy's centre where it should continue to cool even faster and form new stars. However, radio observations with the VLA (<a class="mw-redirect" href="http://commons.wikimedia.org/wiki/Red" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Red">red</a>) suggest that in M87 jets of very energetic particles produced by the <a href="http://commons.wikimedia.org/wiki/Black_hole" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Black hole">black hole</a> interrupt this process. These jets lift up the relatively cool gas near the centre of the galaxy and produce shock waves in the galaxy's atmosphere because of their supersonic speed.</div>
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<img alt="Skyatlas PNG Image" src="http://www.nightskyatlas.com/skyatlas.jsp?rightAscension=12.5137222222&declination=12.3905555556&viewAngle=20.0&viewRotation=0.0&width=700&height=500" /><br />
<a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=12.5137222222&declination=12.3905555556&viewAngle=20">http://www.nightskyatlas.com/viewer.jsp?rightAscension=12.5137222222&declination=12.3905555556&viewAngle=20</a><br />
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M87 - NGC 4486 - Galáxia</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h30m49 declinação +12<sup>o</sup>.23 24</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 8.63:9.59 dimensões 8.32x6.61</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Um dos maiores membros do Aglomerado de Galáxias em Virgem</b>, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma galáxia brilhante e eliptical</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e uma das mais massivas e luminosas galáxias conhecidas. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Ao mesmo tempo, é uma das mais vigorosas fontes de radiação de radio,</span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> designada como </span><b><span style="color: #660000;">Virgo A</span></b><span style="color: #073763;"> ou pelo número </span><metricconverter productid="3C" w:st="on">3C</metricconverter><span style="color: #073763;"> 274 (Catálogo de Fontes de Radio). </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Sua poderosa radiação de rádio e também a poderosa emissão de raio-x </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> acontecem como <b>um jato luminoso</b> que se extende para mais de 4 mil anos-luz </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">para fóra do núcleo da galáxia. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dentro do núcleo podemos encontrar um jato de elétrons, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acelerado por um campo magnético bem forte </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e para velocidade imensa: </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">isso faz acontecer uma radiação extremamente enérgica </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e estes processos podem ter sido causados, por exemplo, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">por um supermassivo buraco negro no núcleo da galáxia.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/39/M87_jet.jpg/800px-M87_jet.jpg" /><br />
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<a href="http://pt.wikipedia.org/wiki/Messier_87#mediaviewer/File:M87_jet.jpg">http://pt.wikipedia.org/wiki/Messier_87#mediaviewer/File:M87_jet.jpg</a><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">M87 jet</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">NASA and The Hubble Heritage Team (STScI/AURA)</span> - <span class="mw-mmv-source">HubbleSite: <a class="external text" href="http://hubblesite.org/gallery/album/exotic/pr2000020a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">gallery</a>, <a class="external text" href="http://hubblesite.org/newscenter/archive/releases/2000/20/image/a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">release</a>.</span></span></div>
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<span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">Black Hole-Powered Jet of Electrons and Sub-Atomic Particles Streams From Center of Galaxy M87</span></div>
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<b>Messier 87</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 4486</a>) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a> localizada a aproximadamente sessenta milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> (cerca de 18,4 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da<a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">constelação de Virgem</a> localizada no centro do massivo Grupo Galáctico Virgo. Possui pouco mais de cento e vinte cinco mil anos-luz de <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a>, sendo assim uma das maiores galáxias elípticas conhecidas, uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de +8,6, uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> de -22, uma declinação de +12° 23' 26" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 12 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 30 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 49,3 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia NGC 4486 foi descoberta e catalogada em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/18_de_Mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="18 de Março">18 de Março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a> por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>. No centro desta galáxia encontra-se um dos maiores <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Buraco_negro_supermassivo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Buraco negro supermassivo">buracos negros supermassivos</a> de que se tem conhecimento, com 6,4 bilhões de massas solares. Essa galáxia emite grande quantidade de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ondas_de_r%C3%A1dio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ondas de rádio">ondas de rádio</a>, possui mais de um trilhão de estrelas e é a mais brilhante galáxia do aglomerado a que pertence, o <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado de Virgem">Aglomerado de Virgem</a>.</div>
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<span style="line-height: 22.3999996185303px;">Também chamada de "Virgo A", é um dos objetos mais notáveis do céu. É a galáxia dominante do </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de Virgem</a><span style="line-height: 22.3999996185303px;">, o maior grande grupo galáctico próximo da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Terra">Terra</a><span style="line-height: 22.3999996185303px;">, situado a uma distância de cerca de 60 milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 22.3999996185303px;">. M87 representa o centro do aglomerado, próximo das galáxias </span><a href="http://pt.wikipedia.org/wiki/Messier_84" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 84">Messier 84</a><span style="line-height: 22.3999996185303px;"> e </span><a href="http://pt.wikipedia.org/wiki/Messier_86" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 86">Messier 86</a><span style="line-height: 22.3999996185303px;">.</span><span class="reference" id="cite_ref-seds_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-seds-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 87</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M87_jet.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="1276" data-file-width="1222" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/39/M87_jet.jpg/280px-M87_jet.jpg" height="292" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/39/M87_jet.jpg/420px-M87_jet.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/39/M87_jet.jpg/560px-M87_jet.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 87, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/18_de_mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="18 de março">18 de marçode</a> <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">E+0-1 pec, NLRG Sy<br />
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<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 30<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 49.42338<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-aaa493_1_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-aaa493_1-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+12° 23′ 28.0439″<span class="reference" id="cite_ref-aaa493_1_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-aaa493_1-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">53,5 ± 1,63 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><br />
(15,9 ± 1,0 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)<span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> (16,4 ± 0,50 milhões de <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">0,004360 ± 0,000022<br />
(1254 ± 7 km/s)<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">9,59<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">8.3 × 6.6 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top">Virgo A, Virgo X-1, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4486, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7654, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a>41316, VCC 1316, <a href="http://pt.wikipedia.org/wiki/Atlas_of_Peculiar_Galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atlas of Peculiar Galaxies">Arp</a> 152, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Third_Cambridge_Catalogue_of_Radio_Sources&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Third Cambridge Catalogue of Radio Sources (página não existe)">3C</a> 274,<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> 3U 1228+12.<span class="reference" id="cite_ref-mnras170_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_87#cite_note-mnras170-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><div style="position: relative;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 87"><img alt="Messier 87" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_87">http://pt.wikipedia.org/wiki/Messier_87</a></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M 89 - NGC 4552 - e M90 - NGC 4569</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - são duas galáxias brilhantes, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sendo que<b> M90 </b>possui uma magnitude de 11</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e é bem grande (11’x5’)</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e apresentando-se como uma galáxia espiral com uma barra difusa. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Situa-se a 2.2<sup>o</sup>. a leste dos Olhos.</b> </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um tantinho ao norte de M90, situa-se IC 3583 (magnitude 13.8)</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M89</b> é uma galáxia elíptica brilhante (magnitude 10.5), </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">pequena (5’x5’) e e situada a <metricconverter productid="40’" w:st="on">40’</metricconverter> sudoeste de M90. </span><br />
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M 89 - NGC 4552</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h53m39 declinação +12<sup>o</sup>.33 25</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.75:10.73 dimensões 5.13x4.68</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M 90 - NGC 4569</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão reta 12h36m50 declinação +13<sup>o</sup>.09 48</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo eg magnitude 9.54:10.26 dimensões 9.55x4.37</span><br />
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m89atlas.jpg" /><br />
http://www.ipac.caltech.edu/2mass/gallery/m89atlas.jpg<br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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<h1>
Messier 89</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Elliptical Galaxy</a> M89 (NGC 4552)</i>, type E0, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m89.jpg"><img align="right" alt="[m89.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m89.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">12 : 35.7 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 33 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">4.0 (arc min)</td></tr>
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Discovered 1781 by Charles Messier.<br />
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Messier 89 (M89, NGC 4552) is another member of the <a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster of Galaxies</a>. It is a beautiful example of an elliptical galaxy of type E0.<br />
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M89 is one of <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>'s own discoveries. He <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M89">cataloged it</a> on March 18, 1781, together with seven other newly discovered galaxies in the Coma-Virgo region (i.e., Virgo Cluster members), and <a href="http://messier.obspm.fr/m/m092.html">globular cluster M92</a>, to make this his most successful discovery day.<br />
<br />
LEIA MAIS<br />
em</div>
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<a href="http://messier.obspm.fr/m/m089.html">http://messier.obspm.fr/m/m089.html</a></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/ad/Messier_089_Hubble_WikiSky.jpg/800px-Messier_089_Hubble_WikiSky.jpg" /></div>
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<span style="line-height: 18.2000007629395px;">http://pt.wikipedia.org/wiki/Messier_89#mediaviewer/File:Messier_089_Hubble_WikiSky.jpg</span><br />
<div class="mw-mmv-title-para" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 1.5em; overflow: visible; padding: 10px 20px 0px; text-overflow: ellipsis;">
<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 089 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool </span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> foi descoberta pelo astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 18 de março de 1981, quando decidiu realizar um empreendimento de observações de nebulosas que estavam naquela região da </span><a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Esfera celeste">esfera celeste</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, na constelação de </span><a href="http://pt.wikipedia.org/wiki/Virgo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Virgo">Virgem</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Em apenas uma única noite, catalogou 8 </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia">galáxias</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, incluindo M89, além de um</span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, </span><a href="http://pt.wikipedia.org/wiki/Messier_92" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 92">Messier 92</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><span class="reference" id="cite_ref-seds_3-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">É uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a>, praticamente <a href="http://pt.wikipedia.org/wiki/Esfera" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esfera">esférica</a>. É uma fraca fonte de <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_eletromagn%C3%A9tica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Radiação eletromagnética">rádio</a> e <a href="http://pt.wikipedia.org/wiki/Astrofotografia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astrofotografia">astrofotografias</a> de alta sensitividade indicaram a presença de um envelope envolvendo a galáxia, a primeira estrutura dessa natureza descoberta em uma galáxia. Seu envelope se estende para mais de 150 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. Destaca-se uma estrutura em forma de jato em torno da galáxia, mas diferentemente de <a href="http://pt.wikipedia.org/wiki/Messier_87" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 87">Messier 87</a>, que possui um jato de matéria que sai diretamente de seu núcleo a altíssima velocidade, o jato de M89 na verdade é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a> que está sendo deformada pela ação <a href="http://pt.wikipedia.org/wiki/Gravidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Gravidade">gravitacional</a> da galáxia. Essa característica pode indicar que M89 pode ter sido um <a href="http://pt.wikipedia.org/wiki/Quasar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Quasar">quasar</a> ativo ou uma <a href="http://pt.wikipedia.org/wiki/Radiogal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Radiogaláxia">radiogaláxia</a> bilhões de anos antes.<span class="reference" id="cite_ref-seds_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> <span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Como membro do <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Virgem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado de Virgem">aglomerado de Virgem</a>, situa-se a cerca de 60 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Seu diâmetro aparente de 4 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a> corresponde a um diâmetro real de 70 000 anos-luz.<span class="reference" id="cite_ref-seds_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Possui uma grande população de<a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a> em comparação com a <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a>, que tem 150-200. Uma pesquisa de <a href="http://pt.wikipedia.org/wiki/2006" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="2006">2006</a> mostrou que há 2 000 ± 700 aglomerados globulares em um raio de 10 minutos de arco do núcleo.<span class="reference" id="cite_ref-Tamuraetal2006_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-Tamuraetal2006-5" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 89</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_089_Hubble_WikiSky.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="3200" data-file-width="3200" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/ad/Messier_089_Hubble_WikiSky.jpg/280px-Messier_089_Hubble_WikiSky.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/ad/Messier_089_Hubble_WikiSky.jpg/420px-Messier_089_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/ad/Messier_089_Hubble_WikiSky.jpg/560px-Messier_089_Hubble_WikiSky.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 89, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/18_de_mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="18 de março">18 de marçode</a> <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">E, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=LINER&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="LINER (página não existe)">LINER</a>, <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_Seyfert" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia Seyfert">H<span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">II</span>Sy2</a><span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 35<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 39,8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+12° 33′ 23″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">50 ± 3 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><br />
(15 ± 0,92 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">0,001134 ± 0,000014<br />
(290 ± 5 km/s)<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">10,73<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">5,1 × 4,7 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4552, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7760, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 41968.<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_89#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 89"><img alt="Messier 89" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="line-height: 18.2000007629395px;">http://www.ipac.caltech.edu/2mass/gallery/m90atlas.jpg</span><br />
<span style="line-height: 18.2000007629395px;"><a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
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Messier 90</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M90 (NGC 4569)</i>, type Sb, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m90.jpg"><img align="right" alt="[m90.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m90.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">12 : 36.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+13 : 10 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">60000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">9.5x4.5 (arc min)</td></tr>
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Discovered 1781 by Charles Messier.<br />
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Messier 90 (M90, NGC 4569) is one of the brighter spiral galaxies situated in the <a href="http://messier.obspm.fr/more/virgo.html">Virgo Cluster of Galaxies</a>.<br />
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Spiral galaxy M90 is one of the eight galaxies found and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M90">cataloged</a> on March 18, 1781 by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> in the Coma-Virgo region, in addition to <a href="http://messier.obspm.fr/m/m092.html">M92</a>, the Hercules globular, to round up score to nine newly cataloged objects on that day.<br />
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LEIA MAIS<br />
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<a href="http://messier.obspm.fr/m/m090.html">http://messier.obspm.fr/m/m090.html</a></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e8/NGC_4569_in_UV_and_Visible.jpg/220px-NGC_4569_in_UV_and_Visible.jpg" height="640" width="640" /></div>
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<span style="line-height: 18.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_90#mediaviewer/File:NGC_4569_in_UV_and_Visible.jpg">http://pt.wikipedia.org/wiki/Messier_90#mediaviewer/File:NGC_4569_in_UV_and_Visible.jpg</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Messier 90</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4569) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> localizada a cerca de sessenta milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> (aproximadamente 18,39 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da<a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">constelação de Virgem</a>. Possui aproximadamente anos-luz de <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a>, uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de +9,5, uma declinação de +13º 09' 45" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 12<a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a> 36 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> 49,9 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A galáxia NGC 4569 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/18_de_Mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="18 de Março">18 de Março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a> por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> e pertence ao aglomerado de galáxias de Virgem.</span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Messier 90</span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ngc4569-hst-R814GB555.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="1743" data-file-width="1425" src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/68/Ngc4569-hst-R814GB555.jpg/280px-Ngc4569-hst-R814GB555.jpg" height="342" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/68/Ngc4569-hst-R814GB555.jpg/420px-Ngc4569-hst-R814GB555.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/68/Ngc4569-hst-R814GB555.jpg/560px-Ngc4569-hst-R814GB555.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Messier 90, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/18_de_mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="18 de março">18 de marçode</a> <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">SAB(rs)ab,<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=LINER&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="LINER (página não existe)">LINER</a>,<span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Sy<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 36<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 49.8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+13° 09′ 46″<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">58,7 ± 2,8 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">Mal</a> (18,0 ± 0,86<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">-0,000784 ± 0,000013<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><br />
(−282 ± 4 <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Metro por segundo">km/s</a>)<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">10,26<span class="reference" id="cite_ref-ned_1-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">9,5 × 4,4 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-ned_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4569,<span class="reference" id="cite_ref-ned_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 7786,<span class="reference" id="cite_ref-ned_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 42089,<span class="reference" id="cite_ref-ned_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a href="http://pt.wikipedia.org/wiki/Atlas_of_Peculiar_Galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atlas of Peculiar Galaxies">Arp</a> 76<span class="reference" id="cite_ref-ned_1-12" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_90#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_90">http://pt.wikipedia.org/wiki/Messier_90</a></span></div>
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<span style="margin: 0px; padding: 0px;">Credit: </span><strong style="margin: 0px; padding: 0px;"> </strong><span style="color: #888888; line-height: 1.4em;">ESO/P. Barthel</span></div>
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<span style="line-height: 1.4em;">Acknowledgments: Mark Neeser (Kapteyn Institute, Groningen) and Richard Hook (ST/ECF, Garching, Germany).</span></div>
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<span style="color: #888888; font-family: Arial, sans-serif, Helvetica Neue, Verdana;"><span style="line-height: 16.7999992370605px;"><a href="http://www.eso.org/public/images/eso0007a/">http://www.eso.org/public/images/eso0007a/</a></span></span></div>
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<span style="background-color: white; color: #073763; font-family: sans-serif; font-size: 1.2em; line-height: 1.5em; white-space: nowrap;">M104 - Sombrero</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">veja que um dos mais conhecidos Objetos Messier</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(ou o mais conhecido!) </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acolhidos pela constelação da Virgem</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">encontra-se mais </span><b><span style="color: #660000;">ao sul da Linha da Eclíptica</span></b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>e bem próximo à divisa entre Virgo e Corvus:</b></span></div>
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<b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">é </span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">o Objeto Messier 104</span></b></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>mais conhecido como o Sombreiro!</b></span></div>
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<li style="text-align: center;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://messier.obspm.fr/m/m104.html">M104</a> <b>The Sombrero Galaxy </b>spiral galaxy (type Sa+/Sb-)</span></span></li>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><br /><b><span style="color: #660000;">Messier 104 - O Sombreiro -</span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Messier 104 (M104, NGC 4594) é numericamente o primeiro objeto</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i> que não foi incluído no Catálogo Messier originalmente publicado.</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Entretanto, Charles Messier o adicionou manualmente em sua cópia pessoal, em 11 de maio de 1781, descrevendo este objeto como uma 'nebulosa muito pálida'.</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Foi Camille Falmmarion que descobriu que a posição mencionada por Messier coincindia com a de Herschel (em H I,43) - a Galáxia Sombrero (NGC 4594), e adicionou este objeto à Lista oficial Messier, em 1921</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(tradução simples e direta de Janine para o texto abaixo)</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="line-height: normal; text-align: start;">Messier 104 (M104, NGC 4594) is numerically the first object of the catalog which was not included in Messier's originally published catalog. However, </span><a href="http://messier.obspm.fr/xtra/history/biograph.html" style="line-height: normal; text-align: start;">Charles Messier</a><span style="line-height: normal; text-align: start;"> added it by hand to his personal copy on May 11, 1781, and </span><a href="http://messier.obspm.fr/xtra/history/m-cat.html#M104" style="line-height: normal; text-align: start;">described it</a><span style="line-height: normal; text-align: start;">as a "very faint nebula." It was </span><a href="http://messier.obspm.fr/xtra/Bios/flammarion.html" style="line-height: normal; text-align: start;">Camille Flammarion</a><span style="line-height: normal; text-align: start;"> who found that its position coincided with Herschel's H I.43, which is the Sombrero Galaxy (NGC 4594), and </span><a href="http://messier.obspm.fr/addition.html" style="line-height: normal; text-align: start;">added it</a><span style="line-height: normal; text-align: start;"> to the official Messier list in 1921.</span></div>
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<a href="http://messier.obspm.fr/m/m104.html" style="line-height: normal; text-align: start;">http://messier.obspm.fr/m/m104.html</a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEizC3h-OW3XTYa_inlgLkfVH9Dqxi_MwEVQVBx8sjYHaWwepsmUc8IxjsHZYbRWmwMcFA7lWpostOcaw8KW5XVik2lJ8nioAva6B0HL2K8crDBiXc3Pt0U9EF6tX17l-92cmoEG2nQNbKs/s1600/VIRGEM++-+104+-+ao+sul.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEizC3h-OW3XTYa_inlgLkfVH9Dqxi_MwEVQVBx8sjYHaWwepsmUc8IxjsHZYbRWmwMcFA7lWpostOcaw8KW5XVik2lJ8nioAva6B0HL2K8crDBiXc3Pt0U9EF6tX17l-92cmoEG2nQNbKs/s1600/VIRGEM++-+104+-+ao+sul.png" /></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Excerto da constelação Virgo - Mario Jaci Monteiro - As Constelações, Cartas Celestes - CARJ</span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m104atlas.jpg" /></div>
<span style="line-height: 18.2000007629395px;">http://www.ipac.caltech.edu/2mass/gallery/m104atlas.jpg</span><br />
<span style="line-height: 18.2000007629395px;"><a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
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Messier 104</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M104 (NGC 4594)</i>, type Sa, in <a href="http://messier.obspm.fr/map/Vir.html">Virgo</a><b>Sombrero Galaxy</b></center>
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<table border="2" cellpadding="5" cellspacing="0" style="line-height: 18.2000007629395px;"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">12 : 40.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-11 : 37 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">50000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">9x4 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.<br />
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Messier 104 (M104, NGC 4594) is numerically the first object of the catalog which was not included in Messier's originally published catalog. However, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> added it by hand to his personal copy on May 11, 1781, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M104">described it</a>as a "very faint nebula." It was <a href="http://messier.obspm.fr/xtra/Bios/flammarion.html">Camille Flammarion</a> who found that its position coincided with Herschel's H I.43, which is the Sombrero Galaxy (NGC 4594), and <a href="http://messier.obspm.fr/addition.html">added it</a> to the official Messier list in 1921. This object is also mentioned by<a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> as his discovery in his <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m104">letter of May 6, 1783</a>. <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> found this object independently on May 9, 1784.<br />
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LEIA MAIS<br />
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<a href="http://messier.obspm.fr/m/m104.html">http://messier.obspm.fr/m/m104.html</a></div>
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<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#mediaviewer/File:Sombrero_Galaxy_in_infrared_light_(Hubble_Space_Telescope_and_Spitzer_Space_Telescope).jpg">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#mediaviewer/File:Sombrero_Galaxy_in_infrared_light_(Hubble_Space_Telescope_and_Spitzer_Space_Telescope).jpg</a></div>
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<span style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-title mw-mmv-reduce-toolong" original-title="Nome do ficheiro" style="font-size: 1em; max-width: 60%;">Sombrero Galaxy in infrared light (Hubble Space Telescope and Spitzer Space Telescope)</span></span></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Autor e informação sobre a fonte" style="background-color: white; font-size: 0.8em;"><span style="color: #073763;"><span class="mw-mmv-author">NASA/JPL-Caltech and The Hubble Heritage Team (STScI/AURA)</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/html/opo0328b.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://www.spacetelescope.org/images/html/</a></span></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span lang="ES-TRAD">NGC 4594 - </span><span lang="ES-TRAD">M 104 - </span><span lang="ES-TRAD"> Galáxia Sombrero:</span></span></b><span lang="ES-TRAD" style="color: #073763;"></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 12h40m00 Declinação - 11<sup>o</sup>.37</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 104</b>: é uma galáxia com magnitude 8.6 e tamanho de 9’x4’. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Vista de lado, com um simples telescópio de abertura <metricconverter productid="4”" w:st="on">4”</metricconverter>, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">poderá apresentar um plano de poeira correndo em direção ao seu centro. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta galáxia situa-se na fronteira com o Corvo.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh1QhWcLGBfbdMJCFBX4I2wv_Dgg3Zi0ifF0uDSRiPySm4AwMY2TKVKG1dIG4BkBca8G-kODdQE1JRs765D5kSAQxnVp2rwoiP8rN73qG3h4y04l0BEaE7hqUz68GbgRNMZ_uDgnHM15pI/s1600/M104_ngc4594_sombrero_galaxy_hi-res.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh1QhWcLGBfbdMJCFBX4I2wv_Dgg3Zi0ifF0uDSRiPySm4AwMY2TKVKG1dIG4BkBca8G-kODdQE1JRs765D5kSAQxnVp2rwoiP8rN73qG3h4y04l0BEaE7hqUz68GbgRNMZ_uDgnHM15pI/s1600/M104_ngc4594_sombrero_galaxy_hi-res.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="line-height: 18.2000007629395px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/thumb/5/5e/M104_ngc4594_sombrero_galaxy_hi-res.jpg/1280px-M104_ngc4594_sombrero_galaxy_hi-res.jpg</span></span></div>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.2000007629395px; padding: 5px; text-align: center; width: 1348px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/ESA and The Hubble Heritage Team (STScI/AURA)</span></td></tr>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> foi a primeira entrada constada apenas nas versões modernas do <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo de objetos do céu profundo</a> do astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>: sua última edição, publicada no anuário astronômico francês <i><a href="http://pt.wikipedia.org/wiki/Connaissance_des_temps" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Connaissance des temps">Connaissance des temps</a></i>, contém apenas 103 entradas. Messier 104 foi adicionado ao catálogo em meados do século XX por <a href="http://pt.wikipedia.org/wiki/Helen_Sawyer_Hogg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Helen Sawyer Hogg">Helen Sawyer Hogg</a> e <a href="http://pt.wikipedia.org/wiki/Owen_Gingerich" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Owen Gingerich">Owen Gingerich</a> baseado em cartas enviadas pelo assistente de Messier, <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Jacob_Bernoulli" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jacob Bernoulli">Jacob Bernoulli</a> alguns anos após a publicação da última edição do catálogo.<span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Em 1921, <a href="http://pt.wikipedia.org/wiki/Camille_Flammarion" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Camille Flammarion">Camille Flammarion</a>, de posse da cópia pessoal de Messier de seu próprio catálogo, também notou que o objeto havia sido acrescentado pelo astrônomo francês em suas anotações em 11 de maio de 1781, logo após a publicação da última edição de seu catalogo. <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, descobriu independentemente o objeto em 9 de maio de 1784.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Galáxia do Sombreiro</span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M104_ngc4594_sombrero_galaxy_hi-res.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="6429" data-file-width="11472" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5e/M104_ngc4594_sombrero_galaxy_hi-res.jpg/280px-M104_ngc4594_sombrero_galaxy_hi-res.jpg" height="157" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5e/M104_ngc4594_sombrero_galaxy_hi-res.jpg/420px-M104_ngc4594_sombrero_galaxy_hi-res.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5e/M104_ngc4594_sombrero_galaxy_hi-res.jpg/560px-M104_ngc4594_sombrero_galaxy_hi-res.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Galáxia do Sombreiro, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1767" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1767">1767</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Virgo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Virgo">Virgo</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">SA(s)a;<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=LINER&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="LINER (página não existe)">LINER</a><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 39<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 59.4<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">-11° 37′ 23″<span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">29,3 ± 1,6 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">Mal</a> (9,0 ± 0,49<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">0,003416 ± 0,000017<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><br />
(904 ± 7 <a href="http://pt.wikipedia.org/wiki/Metro_por_segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Metro por segundo">km/s</a>)<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">8,98<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">8′,7 × 3′,5<span class="reference" id="cite_ref-ned_1-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objeto Messier">Messier</a> 104,<span class="reference" id="cite_ref-ned_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4594,<span class="reference" id="cite_ref-ned_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 42407,<span class="reference" id="cite_ref-ned_1-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> UGCA 293<span class="reference" id="cite_ref-ned_1-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Sombreiro#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><div style="position: relative;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Sombreiro"><img alt="Galáxia do Sombreiro" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Virgo_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Virgo constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/240px-Virgo_constellation_map.png" height="187" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/360px-Virgo_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Virgo_constellation_map.png/480px-Virgo_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18.2000007629395px;">http://imgsrc.hubblesite.org/hu/db/images/hs-2003-28-b-full_jpg.jpg</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-title mw-mmv-reduce-toolong" original-title="Nome do ficheiro" style="font-size: 1em; max-width: 60%;">Sombrero Galaxy in infrared light (Hubble Space Telescope and Spitzer Space Telescope)</span></span></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Autor e informação sobre a fonte" style="background-color: white; font-size: 0.8em;"><span style="color: #073763;"><span class="mw-mmv-author">NASA/JPL-Caltech and The Hubble Heritage Team (STScI/AURA)</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/html/opo0328b.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://www.spacetelescope.org/images/html/opo0328b.html</a> <a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2003/28/image/b/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/2003/28/image/b/</a> (<a class="external text" href="http://imgsrc.hubblesite.org/hu/db/images/hs-2003-28-b-full_jpg.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">direct link</a>)</span></span></span></div>
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Galáxia do Sombreiro, imagem conjunta dos telescópios espaciais <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Hubble</a> e Spitzer</div>
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NASA/ESA <a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Hubble Space Telescope">Hubble Space Telescope</a> and NASA's <a class="extiw" href="http://en.wikipedia.org/wiki/Spitzer_Space_Telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Spitzer Space Telescope">Spitzer Space Telescope</a> joined forces to create this striking composite image of one of the most popular sights in the universe. <a class="extiw" href="http://en.wikipedia.org/wiki/Messier_104" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Messier 104">Messier 104</a> is commonly known as the Sombrero galaxy because in <a class="extiw" href="http://en.wikipedia.org/wiki/visible_light" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:visible light">visible light</a>, it resembles the broad-brimmed Mexican hat. However, in Spitzer's striking <a class="extiw" href="http://en.wikipedia.org/wiki/infrared" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:infrared">infrared</a> view, the galaxy looks more like a "bull's eye." Spitzer's full view shows the disk is warped, which is often the result of a gravitational encounter with another galaxy, and clumpy areas spotted in the far edges of the ring indicate young star-forming regions. The Sombrero galaxy is located some 28 million light-years away. Viewed from Earth, it is just six degrees south of its <a class="extiw" href="http://en.wikipedia.org/wiki/equatorial_plane" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:equatorial plane">equatorial plane</a>. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge <a class="extiw" href="http://en.wikipedia.org/wiki/black_hole" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:black hole">black hole</a>, believed to be a billion times more massive than our <a class="extiw" href="http://en.wikipedia.org/wiki/Sun" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Sun">Sun</a>. The Spitzer picture is composed of four images taken at 3.6 (blue), 4.5 (green), 5.8 (orange), and 8.0 (red) microns. The contribution from starlight (measured at 3.6 microns) has been subtracted from the 5.8 and 8-micron images to enhance the visibility of the dust features.</div>
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<span style="color: #274e13;"><strong>Title: </strong>La Vierge (Virgo) <strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">MJ Fortin</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">maiores informações sobre</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>as Galáxias que fazem parte do Aglomerado Virgo</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>na constelação da Virgem,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acesse meu Trabalho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span></div>
<span style="line-height: 18.2000007629395px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><a href="http://sobrevirgo.blogspot.com.br/2011/09/galaxias-e-aglomerado-de-galaxias-em.html">http://sobrevirgo.blogspot.com.br/2011/09/galaxias-e-aglomerado-de-galaxias-em.html</a></b></span></span><br />
<span style="line-height: 18.2000007629395px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="line-height: 18.2000007629395px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="line-height: 18.2000007629395px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></span><br />
<span style="line-height: 18.2000007629395px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></span><br />
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
<dl style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;">"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></dd><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;"><br /></dd></dl>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>CARO LEITOR,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">devem requerer do Caro Leitor</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Visitando os Sites abaixo,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<b><o:p></o:p></b></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> - AS CONSTELAÇÕES - </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> entre o céu e a terra..., </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vagarosamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> e este por nossa mente sendo conscientizado.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-24980232195635748142014-09-06T10:27:00.005-07:002015-04-02T09:21:55.655-07:00Ursa Major<div class="MsoNormal" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: -webkit-center;">
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nas madrugada sonolentas,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nós, moradores da região sudeste do Brasil,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">já podemos bem reconhecer um bom pedaço </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">composto por estrelas formando as patas</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e um pedaço do corpo (a parte inferior) e a cabeça (quase) inteira</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">da constelação Ursa Major</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- no entanto, infelizmente, não podemos</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">observar as estrelas formadoras do Grande Carro</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(parte superior do corpo e cauda da Ursa),</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">esse asterismo tão interessante</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que torna felizes os moradores bem mais ao norte,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem mais ao norte.</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiNsSdJ5Al3-F7RJfG819JKaKYH6NmpxdV-3jNtqg1xY_w8r5mkFcopsG8er8NlO3ewK9bJFen6xspBEQAJSMnTOUwI1ps9oTt5YDkT3A8yUmqLzBLfjyVeFSmqvEUnFulnuN3UHZGbZJE/s1600/Ursa+na+madrugada.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiNsSdJ5Al3-F7RJfG819JKaKYH6NmpxdV-3jNtqg1xY_w8r5mkFcopsG8er8NlO3ewK9bJFen6xspBEQAJSMnTOUwI1ps9oTt5YDkT3A8yUmqLzBLfjyVeFSmqvEUnFulnuN3UHZGbZJE/s1600/Ursa+na+madrugada.png" /></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Caro Leitor,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sabemos que o Brasil é um país de dimensões continentais</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, sendo assim,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">existem cidades bem ao norte que podem, com toda a certeza,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">observar a Ursa Major em sua inteireza!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesse sentido, as Ilustrações Stellarium apresentadas nesta Postagem</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">foram realizadas para a maravilhosa cidade de Manaus</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- denominada de A Paris dos Trópicos -,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">sendo acolhida pela imensa Floresta Amazônica.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Vincent Van Gogh pintou o Grande Carro</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de maneira inteiramente magistral!</span></span></div>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" dir="ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; font-family: 'Helvetica Neue', Helvetica, Arial, sans-serif; font-size: 13px; line-height: 21px; padding: 5px; text-align: center; width: 1346px;"><tbody>
<tr valign="top"><td><div class="vcard">
<table cellpadding="2" cellspacing="0" class="toccolours collapsible collapsed" id="collapsibleTable0" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); direction: ltr; font-size: 13px; padding: 5px;"><tbody>
<tr valign="top"><th colspan="4" style="border: 1px solid rgb(170, 170, 170);"><span style="color: #073763; font-size: x-small;"><span class="fn" id="creator"><bdi><a class="extiw" href="http://en.wikipedia.org/wiki/Vincent_van_Gogh" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Vincent van Gogh">Vincent van Gogh</a></bdi></span> (1853–1890) </span></th></tr>
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<tr valign="top"><td class="fileinfo-paramfield" id="fileinfotpl_art_title" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="color: #073763; font-size: x-small;">Title</span></td><td><span class="fn"><i><a class="extiw" href="http://tr.wikipedia.org/wiki/Rhone_fazla_Starry_Night" style="background-image: none; color: #274e13; text-decoration: none;" title="tr:Rhone fazla Starry Night"><span style="color: #073763; font-size: x-small;">Starry night over the Rhône</span></a></i></span></td></tr>
<tr valign="top"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="color: #073763; font-size: x-small;">Description</span></td><td><div class="description">
<span style="color: #073763; font-size: x-small;">depicts the <a href="http://commons.wikimedia.org/wiki/Rh%C3%B4ne_River" style="background-image: none; color: #274e13; text-decoration: none;" title="Rhône River">Rhône River</a> at night</span></div>
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<tr valign="top"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="color: #073763; font-size: x-small;">Date</span></td><td><span style="color: #073763; font-size: x-small;"><time class="dtstart" datetime="1888-09" style="display: inline;">September 1888</time> (<a class="extiw" href="http://en.wikipedia.org/wiki/Arles" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Arles">Arles</a>)</span></td></tr>
<tr valign="top"><td class="fileinfo-paramfield" id="fileinfotpl_art_medium" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="color: #073763; font-size: x-small;">Medium</span></td><td><a class="extiw" href="http://en.wikipedia.org/wiki/oil_on_canvas" style="background-image: none; color: #274e13; text-decoration: none;" title="en:oil on canvas"><span style="color: #073763; font-size: x-small;">oil on canvas</span></a></td></tr>
<tr valign="top"><td class="fileinfo-paramfield" id="fileinfotpl_art_dimensions" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="color: #073763; font-size: x-small;">Dimensions</span></td><td><span style="color: #073763; font-size: x-small;">72.5 × 92 cm (28.5 × 36.2 in)</span></td></tr>
<tr valign="top"><td class="fileinfo-paramfield" id="fileinfotpl_art_gallery" rowspan="2" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;"><span style="color: #073763; font-size: x-small;">Current location</span></td><td><div class="vcard">
<table cellpadding="2" cellspacing="0" class="toccolours collapsible collapsed" id="collapsibleTable1" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); direction: ltr; font-size: 13px; padding: 5px;"><tbody>
<tr valign="top"><th colspan="3" style="border: 1px solid rgb(170, 170, 170);"><span class="collapseButton" style="float: right; font-weight: normal; margin-left: 0.5em; text-align: right; width: auto;"><span style="font-size: x-small;"><span class="fn" style="color: #073763; line-height: 21px; text-align: center;"><a class="extiw" href="http://en.wikipedia.org/wiki/Mus%C3%A9e_d%27Orsay" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Musée d'Orsay">Musée d'Orsay</a></span><span style="color: #073763; line-height: 21px; text-align: center;"> </span><span class="wpImageAnnotatorControl wpImageAnnotatorOff" style="color: #073763; line-height: 21px; text-align: center;"></span><span style="color: #073763; line-height: 21px; text-align: center;"> </span><span class="wpImageAnnotatorControl wpImageAnnotatorOff" style="color: #073763; line-height: 21px; text-align: center;"></span></span></span></th></tr>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem, Caro Leitor,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nosso Trabalho nesta Postagem</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não é voltado para as estrelas formando o Asterismo do Grande Carro</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em Ursa Major</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que você poderá conferir em</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com.br/2014/06/ursa-maior-e-cruzeiro-do-sul-nos.html">http://oceudomes.blogspot.com.br/2014/06/ursa-maior-e-cruzeiro-do-sul-nos.html</a>)</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e sim </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sobre os Objetos Messier</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>nesta imensa constelação dos céus bem ao norte:</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M40, M81, M82, M97, M101, M102(?), M108 e M109.</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Será bem interessante observamos algumas questões</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acerca alguns desses Objetos, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como por exemplo:</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- <b>M40 é uma estrela dupla e não uma nebulosa</b> </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- assim como havia sido reportado</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> por Hevelius. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mesmo não encontrando qualquer nebulosidade, </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier catalogou</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">este objeto em sua Lista.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Segundo Ronaldo Rogério de Freitas Mourão,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em sua 6a. Edição de seu Atlas Celeste,</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><b>M81 e M82 </b></i></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><i>- um par de galáxias ao centro do grupo de galáxias na Ursa Maior - </i></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><i>provavelmente o grupo externo mais próximo ao nosso próprio Grupo Local.</i></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><b>Estas duas galáxias - M81 e M82 - </b></i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><b>são interligadas por uma imensa nuvem de gás intergaláctico</b>. </i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i> É possível que, no passado distante, </i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>M82 tenha passado próxima à M81,</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i> que é mais massiva,</i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i> e que o efeito gravitacional da última </i></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>tenha sido a causa do fenômeno extraordinário </i></span></div>
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<i><span style="background-color: white;"></span></i></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>que pode ser observado em M82.</i></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- Sobre <b>M102</b>:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Objeto Messier localizado na constelação Draco</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ou </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">na constelação Ursa Major?</span></span></div>
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<span style="background-color: white;"></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M102, Objeto Messier em Draco (?) </span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">ou</span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;">NGC 5866, Galáxia do Fuso/do Eixo?</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">ou ainda</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> ..... </span><span style="color: #660000;">uma duplicata</span><span style="color: #073763;"> de M101, em Ursa Major?</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta dicotomia</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">pode nos trazer, em um primeiro momento,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma surpresa e uma indagação de seu porquê !?!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div align="center" class="MsoNormal">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">Situações não muito bem explicadas, dúvidas, duplo êrro, não-verificação,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e até situações bem controversas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> acerca trabalhos realizados por Messier e Mechain,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> sugerem que o objeto observado e catalogado foi, na verdade,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> a galáxia lenticular NCG 5866, denominada Galáxia do Fuso/do Eixo... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e ainda incluindo a possibilidade de engano,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> ou seja,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> de que o objeto que teria sido nomeado enquanto M102 </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">seria uma possível duplicata do Objeto Messier 101, em Ursa Maior... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">Ao final, </span></div>
<div align="center" class="MsoNormal">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">parece que tanto Messier quanto Mechain </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">observaram NGC 5866 no passado </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e, portanto, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">este objeto acabou sendo listado </span></div>
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<span style="background-color: white;"></span></div>
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<div align="center" class="MsoNormal" style="-webkit-text-stroke-width: 0px; color: black; font-family: 'Times New Roman'; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: auto; text-align: -webkit-center; text-indent: 0px; text-transform: none; white-space: normal; widows: auto; word-spacing: 0px;">
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como o item perdido (no Catálogo Messier).</span><span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Boa Observação e Bons Estudos!</span></span></div>
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></span></div>
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjfq4MYNmsK2uHaTdrBBRezaOFrJo6YSn10S2VW7IwUyUWhpGg5lL2suEVn7r8LVuenwDZyFaTANiNYvmfnvYrdNa4vVJAzxROhiLZXLKGIntoWbr_oNoJ-fI54zVqgRfzrAiMTKnVx9vs/s1600/ursa+maior.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjfq4MYNmsK2uHaTdrBBRezaOFrJo6YSn10S2VW7IwUyUWhpGg5lL2suEVn7r8LVuenwDZyFaTANiNYvmfnvYrdNa4vVJAzxROhiLZXLKGIntoWbr_oNoJ-fI54zVqgRfzrAiMTKnVx9vs/s1600/ursa+maior.png" /></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - CARJ</span><br />
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US" style="mso-ansi-language: EN-US; mso-themecolor: text2; mso-themeshade: 128;"> </span>URSA MAJOR, </b></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>A URSA MAIOR</b></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 8h5m / 14h27m Declinação +28<sup>o</sup>.8 / +73<sup>o</sup>.3<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Calisto, filha de Lion, rei da Arcádia, teve Júpiter como um dos seus enamorados </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e tornou-se uma seguida de Diana, Pallas, em função de seu amor pela caçada. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Júpiter quis namorar Calisto e para tanto, tomou a forma de Diana. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Juno, a esposa de júpiter, ao descobrir essa verdade, transformou Calisto em um urso.</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Porém, ao saber que seu marido tinha colocado o urso no céu, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Juno pediu ao seu irmão Câncer </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">para providenciar que nunca as estrelas daquela constelação </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">desaparecessem em seu reino</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - e por essa mesma razão, esta constelação pode sempre ser vista por inteiro</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> acima do horizonte, na Europa. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Para dar conta do imenso tamanho da cauda da Ursa, diz-se que júpiter, com medo de seus dentes, levantou-a pela cauda ... </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que por isso, tornou-se alongada ao longo do caminho entre a terra e o céu.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao longo dos milênios, a Ursa Maior teve várias denominações. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Para os árabes, era uma caravana no horizonte;</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> para os romanos, bois de atrelagem;</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> para os índios da América do Norte, uma concha; </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e para os povos da América Central, uma pessoa de uma perna só.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação de Ursa Major faz fronteiras com Camelopardalis, Draco, Bootes, Canes Venatici, Coma Berenices, Leo, Leo Minor e Lyince.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Não existe dúvida que, em meio a todas as constelações, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a mais conhecida é a Grande Ursa, cujas estrelas são confiáveis </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em nos ajudar a localizar Polaris, estrela Alfa da Ursa Menor, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e a direção para o Polo norte celestial.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As sete estrelas formando O Carro são uma rara exceção </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em não serem um grupo de estrelas puramente acidental. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com a exceção da estrela Dubhe, a estrela Alpha da Grande Ursa, e de Benetnash (a estrela Eta da Ursa Maior), as demais cinco estrelas brilhantes viajam juntas</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> através o espaço e formam </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- juntamente com 12 outras estrelas em vários pontos do céu -</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> um aglomerado de estrelas que se movimenta </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e que está mais próximo de nós do que todos os demais aglomerados estelares. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sua movimentação se faz em direção ao Sagitário em cerca de 14 km por segundo. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> A conexão física das estrelas do aglomerado</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> são testemunhas de suas origens em comum</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - assim como acontece no aglomerado das Hyades, em Taurus, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">com uma formação similar.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6a. Edição do Atlas Celeste</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 40</h1>
<i><b><a href="http://messier.obspm.fr/cluster.html">Double Star</a> </b>M40 (WNC 4)</i> in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a><b>Winnecke 4</b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m40.jpg"><img alt="[m40.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m40.jpg" style="text-align: right;" /></a></div>
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<tr><th align="left">Right Ascension</th><td>12 : 22.4 (h:m)</td></tr>
<tr><th align="left">Declination</th><td>+58 : 05 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td>0.51 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td>8.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td>0.8 (arc min)</td></tr>
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Discovered by Charles Messier 1764.</div>
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Messier 40 (M40) is one of the three "curiosities," or unusual objects, in Messier's catalog. It is a double star, which was also cataloged later as Winnecke 4 (WNC 4). Most probably, it is an optical double star, i.e. a chance alignment of two independent stars at different distances.</div>
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This faint double star was found by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> when he was searching for a nebula which was - erroneously - reported by the 17th-century observer <a href="http://messier.obspm.fr/xtra/Bios/hevelius.html">Johann Hevelius</a> in this vicinity. According to <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M40">his catalog description</a>, Messier did not see any nebulosity associated with them. As Messier had measured the position of these stars, he gave them a number in his catalog.</div>
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This fact gives some suggestion on how this catalog was compiled: Messier collected positions while he was cataloging the star clusters and nebula which could be taken for comets. M40 was apparently the last one he recorded when he was busy in checking the reports available to him in 1764, of previously recorded "nebulae."</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m040.html</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Veja o Vídeo</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.deepskyvideos.com/videos/messier/M40_optical_double_star.html">http://www.deepskyvideos.com/videos/messier/M40_optical_double_star.html</a></span><br />
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<span style="background-color: white; color: #333333; font-family: arial, sans-serif; line-height: 17px; text-align: start;"><b>The optical double star M40 is perhaps the biggest disappointment in Messier's Catalogue</b> - so we've used our own star to liven up the video with a cameo from Sir Patrick Moore.</span></div>
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<span style="background-color: white; color: #333333; font-family: arial, sans-serif; line-height: 17px; text-align: start;">Also featuring Mike Merrifield and Pete Lawrence. Details on our speakers at </span><a class="yt-uix-redirect-link" dir="ltr" href="http://www.deepskyvideos.com/pages/contributors.html" rel="nofollow" style="background: rgb(255, 255, 255); border: 0px; color: #167ac6; cursor: pointer; font-family: arial, sans-serif; line-height: 17px; margin: 0px; padding: 0px; text-align: start; text-decoration: none;" target="_blank" title="http://www.deepskyvideos.com/pages/contributors.html">http://www.deepskyvideos.com/pages/co...</a></div>
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<span style="background-color: white; color: #333333; font-family: arial, sans-serif; line-height: 17px; text-align: start;">Also thanks to Fred Espenak: <a class="yt-uix-redirect-link" dir="ltr" href="http://astropixels.com/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border: 0px; color: #167ac6; cursor: pointer; margin: 0px; padding: 0px; text-decoration: none;" target="_blank" title="http://astropixels.com">http://astropixels.com</a></span></div>
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<span style="background-color: white; line-height: 17px; text-align: start;"><span style="color: #333333; font-family: arial, sans-serif;"><a href="https://www.youtube.com/watch?v=JGlhgXvn7Xk">https://www.youtube.com/watch?v=JGlhgXvn7Xk</a></span></span></div>
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<b>Messier 40</b>, (Winnecke 4) é uma <a href="http://pt.wikipedia.org/wiki/Estrela_dupla" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela dupla">estrela dupla</a> na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ursa_Major" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ursa Major">Ursa Major</a>. Ela foi descoberta por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em <a href="http://pt.wikipedia.org/wiki/1764" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1764">1764</a> à procura de uma nebulosa nesta área, como foi relatado por <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Johann_Hevelius&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Johann Hevelius (página não existe)">Johann Hevelius</a>. Não confirmado a existência da nebulosa, em vez disso, Messier catalogou esta como uma estrela dupla. Ela foi subseqüntemente redescoberta por <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Friedrich_August_Theodor_Winnecke&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Friedrich August Theodor Winnecke (página não existe)">Friedrich August Theodor Winnecke</a>, em 1863.</div>
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Em 1991 a separação entre os componentes foi mensurado em 51″.7, aumentando desde o tempo de Messier. O consenso geral está se levantando dúvidas se são mesmo estrelas muito próximas ou se são estrelas em uma mesma linha de visão mas à distâncias diferentes.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #99c9e6; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ursa_Major" style="background: none; color: #0b0080; text-decoration: none;" title="Ursa Major">Ursa Major</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 22<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 12,5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">58° 04' 59"</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">9,65 + 10,10</td></tr>
<tr style="vertical-align: top;"><td>Tipo espectral</td><td style="background-color: #f8f8f8;">G0+F8</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">510 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><br />
156 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #99c9e6; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">M</a>40, BD+56 1372, <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Henry_Draper" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Henry Draper">HD</a> 238107 + HD 238108, SAO 28353 + SAO 28355, CCDM 12223+5805.</td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Winnecke_4</span><br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m97atlas.jpg" /><br />
http://www.ipac.caltech.edu/2mass/gallery/m97atlas.jpg<br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 97</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Planetary Nebula</a> M97 (NGC 3587)</i>, type 3a, in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a></center>
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<br /><b><span style="font-size: large;">Owl Nebula</span></b><br /><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m97.jpg"><img align="right" alt="[m97.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m97.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">11 : 14.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+55 : 01 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">2.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">3.4x3.3 (arc min)</td></tr>
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Dicovered by Pierre Méchain in 1781.<br />
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The Owl Nebula Messier 97 (M97, NGC 3587) is one of the fainter objects in Messier's catalog. It is one of the four planetary nebulae in that catalog, and situated in constellation Ursa Major.<br />
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M97 was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on February 16, 1781. In <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M97">his description</a> of this object, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> also mentions two other nebulous objects that he (and Méchain) have seen at about the same time, but which he had not added in his printed catalog version of 1781 (in the <i>Connoissance des Temps</i> for 1784). As the description is obvious and he added positions by hand in his personal copy, as well as descriptions in his manuscript personal pre-print version, we now know that he had observed the objects <a href="http://messier.obspm.fr/m/m108.html">M108</a> and <a href="http://messier.obspm.fr/m/m109.html">M109</a>. <a href="http://messier.obspm.fr/xtra/Bios/smyth.html">Admiral William H. Smyth</a> first classified it as planetary nebulae in 1844. The name "Owl Nebula" goes back to <a href="http://messier.obspm.fr/xtra/Bios/rosse.html">Lord Rosse</a>, who first used it in 1848; <a href="http://messier.obspm.fr/more/m097_rosse.html">see his drawing</a>. In 1866, <a href="http://messier.obspm.fr/xtra/Bios/huggins.html">William Huggins</a>recognized its nature as a gaseous nebula from the observation of its spectrum, where he discovered two spectral lines.<br />
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LEIA MAIS<br />
em<br />
http://messier.obspm.fr/m/m097.html<br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjfENWAsF6r7ypz2VfanOPz_vBZnw9W-zmE2WHlV82H3H9MTRZH2Rrnr91SILl5jAN1NVWLiUIKlqFVM3ATRguFn1pwAYMHdrs-8y97RXLvJeK95IpBs2tdVjVo3vkaqshMZ4XjOoCLEDY/s1600/M97.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjfENWAsF6r7ypz2VfanOPz_vBZnw9W-zmE2WHlV82H3H9MTRZH2Rrnr91SILl5jAN1NVWLiUIKlqFVM3ATRguFn1pwAYMHdrs-8y97RXLvJeK95IpBs2tdVjVo3vkaqshMZ4XjOoCLEDY/s1600/M97.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M97 - NGC 3587 - A Nebulosa Coruja</b></span></div>
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A <b>Nebulosa da Coruja</b> (também conhecida como <b>Messier 97</b> ou <b><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 3587</b>) é uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> localizada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ursa_Major" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ursa Major">Ursa Major</a>. Foi descoberta por<a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> em <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a>.</div>
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É considerada uma das mais complexas nebulosas planetárias. A estrela central de <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude</a> 16 tem cerca de 0,7 <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a> e a nebulosa em si cerca de 0,15 massas solares. A nebulosa foi formada cerca de 6 000 anos atrás.</div>
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A Nebulosa da Coruja recebeu o seu nome devido aos seus "olhos" parecidos com o de uma coruja quando vista através de um <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópio</a> (> 200 mm) grande sob um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu">céu</a>escuro com o auxílio de um "filtro de nebulosa". Os "olhos" são também facilmente visíveis através de <a href="http://pt.wikipedia.org/wiki/Fotografia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Fotografia">fotografias</a> tiradas da nebulosa.</div>
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<a href="http://pt.wikipedia.org/wiki/Nebulosa_da_Coruja">http://pt.wikipedia.org/wiki/Nebulosa_da_Coruja</a></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/6/64/M97.jpg" /><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">http://pt.wikipedia.org/wiki/Nebulosa_da_Coruja#mediaviewer/File:M97.jpg</span></span><br />
<span style="background-color: white; font-family: sans-serif; font-size: 15px; line-height: 22.7999992370605px; text-align: start;">M97(NGC 3587) Planetary nebula in Ursa Major 11H49',+55°1') The planetary nebula Owl Nebula in Ursa Major is regarded as a very nice object. The 16th magnitude central star illuminate the clouds and carve two holes like eyes. 60'Luminance - 30'RGB - Bin2X2 - STL11K - C14</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a7/AnttlersM81M82.jpg/1024px-AnttlersM81M82.jpg" /><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Messier_82#mediaviewer/File:AnttlersM81M82.jpg">http://pt.wikipedia.org/wiki/Messier_82#mediaviewer/File:AnttlersM81M82.jpg</a></span><br />
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<div class="mw-mmv-title-para mw-mmv-ttf-container mw-mmv-ttf-normal" style="font-size: 20px; height: 36px; line-height: 36px; margin-bottom: 20px; overflow: hidden; padding: 10px 20px 0px; position: relative;">
<span class="mw-mmv-title" original-title="" style="max-width: 60%;">Messier 82 (à direita) e a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Bode" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia de Bode">Galáxia de Bode</a> (à esquerda)</span></div>
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<span style="font-size: 0.95em; line-height: 1.5em;">This is a visible light image of Messier 81 (left) and Messier 82 (right) taken with my backyard telescope in Kalkaska, MI in April of 2007.</span><a class="extiw" href="http://en.wikipedia.org/wiki/en:Category:Galaxy_images" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.95em; line-height: 1.5em; text-decoration: none;" title="w:en:Category:Galaxy images">w:en:Category:Galaxy images</a></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M81 e M82</span></b><span style="color: #073763;"> </span></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">- um par de galáxias ao centro do grupo de galáxias na Ursa Maior - </span></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">provavelmente o grupo externo mais próximo ao nosso próprio Grupo Local.<o:p></o:p></span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Estas duas galáxias - M81 e M82 - </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>são interligadas por uma imensa nuvem de gás intergaláctico. </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> É possível que, no passado distante, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M82 tenha passado próxima à M81,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> que é mais massiva,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e que o efeito gravitacional da última </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">tenha sido a causa do fenômeno extraordinário </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que pode ser observado em M82.<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6a. Edição do Atlas Celeste</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://www.ipac.caltech.edu/2mass/gallery/m81atlas.jpg" /><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m81atlas.jpg</span><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 81</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M81 (NGC 3031)</i>, type Sb, in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a></center>
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<br /><b><span style="font-size: large;">Bode's Galaxy</span></b><br /><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m81.jpg"><img align="right" alt="[m81.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m81.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">09 : 55.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+69 : 04 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">12000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">21x10 (arc min)</td></tr>
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Discovered by Johann Elert Bode in 1774.</div>
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Messier 81 (M81, NGC 3031) in Ursa Major is one of the most conspicuous galaxies in the sky, and one of the nearest beyond the Local Group. It is a conspicuous spiral galaxy.</div>
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M81 is one of the easiest and most rewarding galaxies to observe for the amateur astronomer on the northern hemisphere, because with its total visual brightness of about 6.8 magnitudes it can be found with small instruments.</div>
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M81 is the first of the four objects originally discovered by <a href="http://messier.obspm.fr/xtra/Bios/bode.html">Johann Elert Bode</a>, who found it, together with its neighbor <a href="http://messier.obspm.fr/m/m082.html">M82</a>, on December 31, 1774. Bode described it as a "nebulous patch", about 0.75 deg away from M82, which "appears mostly round and has a dense nucleus in the middle," and included it as No. 17 in his list. <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> independently rediscovered both galaxies as nebulous patches in August 1779 and reported them to <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who added them to<a href="http://messier.obspm.fr/xtra/history/m-cat.html#M81">his catalog</a> after his position measurement on February 9, 1781.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m081.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgowiQV8eetdOB34K9WjBMnC6wc2iDXfWkAMnwWK-0enl2o80Hph2QERcJRqNwQoJgJZsuLdG0oaBqaQS_9SyheiOPR5KPiSdBBeFczsBDHNk2zk2n7_TXcVyOGfCjI8LiOfI0R9Ozc_bk/s1600/M81.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgowiQV8eetdOB34K9WjBMnC6wc2iDXfWkAMnwWK-0enl2o80Hph2QERcJRqNwQoJgJZsuLdG0oaBqaQS_9SyheiOPR5KPiSdBBeFczsBDHNk2zk2n7_TXcVyOGfCjI8LiOfI0R9Ozc_bk/s1600/M81.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/static/archives/images/wallpaper2/heic0710a.jpg</span><br />
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The sharpest image ever taken of the large "grand design" spiral galaxy M81 is being released today at the American Astronomical Society Meeting in Honolulu, Hawaii.</div>
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A spiral-shaped system of stars, dust, and gas clouds, the galaxy's arms wind all the way down into the nucleus. Though the galaxy is located 11.6 million light-years away, the Hubble Space Telescope's view is so sharp that it can resolve individual stars, along with open star clusters, globular star clusters, and even glowing regions of fluorescent gas. The Hubble data was taken with the Advanced Camera for Surveys in 2004 through 2006. This colour composite was assembled from images taken in blue, visible, and infrared light.</div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit:</strong></div>
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<a href="http://www.nasa.gov/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>, <a href="http://www.esa.int/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a> and the Hubble Heritage Team <a href="http://www.stsci.edu/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="border: 0px; color: #1596c1; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">AURA</a>). Acknowledgment: A. Zezas and J. Huchra (Harvard-Smithsonian Center for Astrophysics)</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/heic0710a/</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Veja o vídeo: </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/videos/heic0710b/</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 3031 - M 81 - Galáxia Ursa Maior</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 09h53m Declinação +69<sup>o</sup>.09<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo SB - Galáxia Barrada Magnitude fotográfica aparente 7,85<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões Angulares 25 X 12 Distância (milhões de anos-luz) 6,5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando observada através um telescópio pequeno, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">o grande núcleo central parece-se com uma nuvem esfumaçada, pequena e oval. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Claramente visível em fotografias</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> encontram-se os extraordinariamente simétricos braços espiralados</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - que provam consistirem de nuvens de estrelas. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Os planos do material escuro interestelar enfatizam a estrutura interior espiralada </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">da parte central da galáxia.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Alguns objetos (galáxias) encontrados em M81 são </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 2976, NGC 3077 E I 2574<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6a. Edição do Atlas Celeste</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://www.astropt.org/blog/wp-content/uploads/2014/11/m81_colombari_1080c.jpg?261f6d" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.astropt.org/blog/wp-content/uploads/2014/11/m81_colombari_1080c.jpg?261f6d</span><br />
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<span style="background-color: white;">Crédito: <a href="http://www.naoj.org/Introduction/index.html" style="color: #1772af; text-decoration: none;">Subaru Telescope</a> (<a href="http://www.naoj.org/" style="color: #1772af; text-decoration: none;">NAOJ</a>), <a href="http://hla.stsci.edu/hla_welcome.html" style="color: #1772af; text-decoration: none;">Hubble Space Telescope</a>; <a href="http://www.astrobin.com/users/rob77/" style="color: #1772af; text-decoration: none;">Roberto Colombari</a> & <a href="http://www.robgendlerastropics.com/" style="color: #1772af; text-decoration: none;">Robert Gendler</a></span></div>
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<a href="http://apod.nasa.gov/apod/ap141119.html" style="color: #1772af; text-decoration: none;">A imagem</a><span style="background-color: white;"> </span><span style="background-color: white;">mostra a M81, uma bela galáxia semelhante à nossa Via Láctea.</span></div>
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<span style="background-color: white;">O centro da M81 contém idosas estrelas amarelas, enquanto nos seus braços são visíveis jovens estrelas azuis.</span></div>
<span style="background-color: white;">M81 tem uma faixa bem evidente de poeira, que será provavelmente resultado de um encontro próximo entre M81 e a sua pequena companheira M82.</span><br />
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<span style="color: #2c2b2b; font-family: arial;"><span style="background-color: white; line-height: 18px;"><a href="http://www.astropt.org/2014/11/25/a-brilhante-galaxia-m81/">http://www.astropt.org/2014/11/25/a-brilhante-galaxia-m81/</a></span></span></div>
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<b>Galáxia de Bode</b> (também conhecida como <b>NGC 3031</b>, <b>M81</b> ou <b>Messier 81</b>) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> localizada a cerca de doze milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>(aproximadamente 3,679 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Ursa_Maior" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação de Ursa Maior">constelação de Ursa Maior</a>. Possui aproximadamente trinta e seis mil anos-luz de <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a>, uma<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 6,93, uma declinação de +69º 03' 55" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 09 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 55 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Minuto">minutos</a> e 32,9 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia NGC 3031 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/31_de_Dezembro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="31 de Dezembro">31 de Dezembro</a> de <a href="http://pt.wikipedia.org/wiki/1774" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1774">1774</a> pelo astrônomo alemão <a href="http://pt.wikipedia.org/wiki/Johann_Elert_Bode" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann Elert Bode">Johann Elert Bode</a>.</div>
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<span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Bode</span></div>
<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/4d/Messier81_highres.jpg/640px-Messier81_highres.jpg" /><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Bode#mediaviewer/File:Messier81_highres.jpg</span><br />
<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 21px;">Galáxia de Bode, Telescópio Espacial Hubble</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m82atlas.jpg</span><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 82</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Irregular Galaxy</a> M82 (NGC 3034)</i>, type Ir-II, in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a></center>
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<br /><b><span style="font-size: large;">Cigar Galaxy</span></b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m82.jpg"><img align="right" alt="[m82.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m82.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">09 : 55.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+69 : 41 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">12000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">9x4 (arc min)</td></tr>
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Discovered by Johann Elert Bode in 1774.</div>
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Messier 82 (M82, NGC 3034) is a remarkable galaxy of peculiar type in constellation Ursa Major. It is usually classified as irregular, though probably a distorted disk galaxy, and famous for its heavy star-forming activity, thus a prototype member of the class of starbursting galaxies.</div>
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Forming <a href="http://messier.obspm.fr/more/m081-082_more.html">a most conspicuous physical pair</a> with its neighbor, <a href="http://messier.obspm.fr/m/m081.html">M81</a> (THE showpiece galaxies for many Northern hemispherers), this galaxy is the prototype of an irregular of the second type, i.e. a "disk" irregular. Its core seems to have suffered dramatically from a semi-recent close encounter with M81, being in a heavy starburst and displaying conspicuous dark lanes. This turbulent explosive gas flow is also a strong source of radio noise, discovered by Henbury Brown in 1953. The radio source was first called Ursa Major A (strongest radio source in UMa) and cataloged as 3C 231 in the Third Cambridge Catalogue of Radio Sources.</div>
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As a member of the <a href="http://messier.obspm.fr/more/m081gr.html">M81 group</a>, M82 is 12 million light years distant.</div>
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M82 was discovered on December 31, 1774 by <a href="http://messier.obspm.fr/xtra/similar/bode.html">Johann Elert Bode</a> together with M81; he described it as a "nebulous patch", about 0.75 deg away from M81, which "is very pale and of elongated shape," and cataloged it as No. 18 in his catalog.<a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> independently rediscovered both galaxies as nebulous patches in August 1779 and reported them to <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who added them to <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M82">his catalog</a> after his position measurement on February 9, 1781.</div>
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LEIA MAIS</div>
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http://messier.obspm.fr/m/m082.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgnD54jivm29qSAAPmHvWrFFydAhalCmtHOyVwHVyJOwRQg5whyYGHD7ewFW_wp8NxzAoVUD7u3gnj7grcx2lAAgzN_Gu5623pLqe3QYJhyQ5Om1jqom5sRlmnaex0x4Gh4V8rQCSn9X5s/s1600/M.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgnD54jivm29qSAAPmHvWrFFydAhalCmtHOyVwHVyJOwRQg5whyYGHD7ewFW_wp8NxzAoVUD7u3gnj7grcx2lAAgzN_Gu5623pLqe3QYJhyQ5Om1jqom5sRlmnaex0x4Gh4V8rQCSn9X5s/s1600/M.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 3034 - M 82 - Galáxia</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 09h54m Declinação +69<sup>o</sup>.47<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo I - Galáxia Irregular Magnitude fotográfica aparente 9,20<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões Angulares 10 X 1,5 Distância (milhões de anos-luz) 6,5<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma galáxia luminosa, irregular e em formato de rotação e com uma estrutura extremamente incomum. É divida em planos de material interestelar escuro e em muitos laces esfumaçados. É uma intensa fonte de emissão de radio e possui um campo magnético bem forte. Existe um sistema de filamentos originados no centro da galáxia e este material está em expansão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6a. Edição do Atlas Celeste</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiu5_d5_WBBa68BBoEELVTggSxgN7-Yq2yFhmFXoQzz3KSdBK6tkL1M25P8os_VB1PgucCTXFqdtLbf45tL4AXzpuc4_5H8SQEW0cnt4gz7Z70G98iY4tWn81yxRC8Q5vXH2thJxc2q9YI/s1600/1024px-M82_HST_ACS_2006-14-a-large_web.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiu5_d5_WBBa68BBoEELVTggSxgN7-Yq2yFhmFXoQzz3KSdBK6tkL1M25P8os_VB1PgucCTXFqdtLbf45tL4AXzpuc4_5H8SQEW0cnt4gz7Z70G98iY4tWn81yxRC8Q5vXH2thJxc2q9YI/s1600/1024px-M82_HST_ACS_2006-14-a-large_web.jpg" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_82#mediaviewer/File:M82_HST_ACS_2006-14-a-large_web.jpg">http://pt.wikipedia.org/wiki/Messier_82#mediaviewer/File:M82_HST_ACS_2006-14-a-large_web.jpg</a><br />
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<span class="mw-mmv-title" original-title="" style="max-width: 60%;">To celebrate the Hubble Space Telescope's 16 years of success, the two space agencies involved in the project, NASA and the European Space Agency (ESA), are releasing this image of the magnificent starburst galaxy, Messier 82 (M82). This mosaic image is the sharpest wide-angle view ever obtained of M82. The galaxy is remarkable for its bright blue disk, webs of shredded clouds, and fiery-looking plumes of glowing hydrogen blasting out of its central regions. Throughout the galaxy's center, young stars are being born 10 times faster than they are inside our entire Milky Way Galaxy. The resulting huge concentration of young stars carved into the gas and dust at the galaxy's center. The fierce galactic superwind generated from these stars compresses enough gas to make millions of more stars. In M82, young stars are crammed into tiny but massive star clusters. These, in turn, congregate by the dozens to make the bright patches, or "starburst clumps," in the central parts of M82. The clusters in the clumps can only be distinguished in the sharp Hubble images. Most of the pale, white objects sprinkled around the body of M82 that look like fuzzy stars are actually individual star clusters about 20 light-years across and contain up to a million stars. The rapid rate of star formation in this galaxy eventually will be self-limiting. When star formation becomes too vigorous, it will consume or destroy the material needed to make more stars. The starburst then will subside, probably in a few tens of millions of years. Located 12 million light-years away, M82 appears high in the northern spring sky in the direction of the constellation Ursa Major, the Great Bear. It is also called the "Cigar Galaxy" because of the elliptical shape produced by the oblique tilt of its starry disk relative to our line of sight. The observation was made in March 2006, with the Advanced Camera for Surveys' Wide Field Channel. Astronomers assembled this six-image composite mosaic by combining exposures taken with four colored filters that capture starlight from visible and infrared wavelengths as well as the light from the glowing hydrogen filaments.</span></div>
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<span class="mw-mmv-source-author" original-title="" style="line-height: 1.8em;"><span class="mw-mmv-author">NASA, ESA, and The Hubble Heritage Team (STScI/AURA)</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/html/heic0604a.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/html/heic0604a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/large/heic0604a.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)<a class="external free" href="http://hubblesite.org/gallery/album/entire_collection/pr2006014a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/gallery/album/entire_collection/pr2006014a/</a></span></span></div>
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<span style="color: #555555; font-family: sans-serif;"><span style="font-size: 14px; line-height: 20.4000015258789px;">http://pt.wikipedia.org/wiki/Messier_82#mediaviewer/File:Hs-2006-14-h-full_jpg.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="" style="max-width: 60%;">Messier 82, <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">Observatório de raios-X Chandra</a></span></div>
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<span class="mw-mmv-source-author" original-title="" style="line-height: 1.8em;"><span class="mw-mmv-author">NASA/CXC/JHU/D.Strickland</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2006/14/image/h/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/2006/14/image/h/</a></span></span></div>
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ABOUT THIS IMAGE: Composite image of the active galaxy M82 from x-ray observations by Chandra X-Ray Observatory in three energy bands coded in red (lowest energy x-ray photons), green, and blue (highest energy). Object Names: M82, NGC 3034 Image Type: Astronomical Credit: NASA/CXC/JHU/D.Strickland</div>
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<b>Messier 82</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 3034) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia irregular">galáxia irregular</a> localizada a cerca de doze milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> (aproximadamente 3,679 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Ursa_Maior" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação de Ursa Maior">constelação de Ursa Maior</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 8,6, uma declinação de +69º 40' 43" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 09 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 55 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 50,7 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia NGC 3034 foi descoberta em <a href="http://pt.wikipedia.org/wiki/1774" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1774">1774</a> pelo astrônomo alemão <a href="http://pt.wikipedia.org/wiki/Johann_Elert_Bode" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Johann Elert Bode">Johann Elert Bode</a>.</div>
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<span style="line-height: 22.3999996185303px;">Forma um par fisicamente ligado com a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Bode" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia de Bode">galáxia de Bode</a><span style="line-height: 22.3999996185303px;"> (M81), fazendo parte de </span><a href="http://pt.wikipedia.org/wiki/Grupo_M81" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo M81">seu grupo de galáxias</a><span style="line-height: 22.3999996185303px;">. Seu </span><a href="http://pt.wikipedia.org/wiki/Plano_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Plano galáctico">plano galáctico</a><span style="line-height: 22.3999996185303px;">foi profundamente alterado devido a um choque recente (em termos astronômicos) com a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Bode" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia de Bode">galáxia de Bode</a><span style="line-height: 22.3999996185303px;">, que está apenas 150 000 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 22.3999996185303px;"> da galáxia. Seu núcleo galáctico também sofreu profundas alterações com o encontro, que é agora local de intensa </span><a href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Formação estelar">formação estelar</a><span style="line-height: 22.3999996185303px;">, mostrando também linhas escuras de </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Mat%C3%A9ria_interestelar&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; line-height: 22.3999996185303px; text-decoration: none;" title="Matéria interestelar (página não existe)">matéria interestelar</a><span style="line-height: 22.3999996185303px;">. Também é uma grande fonte de </span><a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_eletromagn%C3%A9tica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Radiação eletromagnética">rádio</a><span style="line-height: 22.3999996185303px;">, descoberta por Henbury Brown em 1953, chamada de Ursa Major A e listada como a entrada 3C 231 no </span><i style="line-height: 22.3999996185303px;">Terceiro Catálogo de Cambridge de Fontes de Rádio</i><span style="line-height: 22.3999996185303px;">.</span><span class="reference" id="cite_ref-seds_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_82#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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LEIA MAIS</div>
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<span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Messier_82</span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 101</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M101 (NGC 5457)</i>, type Sc, in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a></center>
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<br /><b><span style="font-size: large;">Pinwheel Galaxy</span></b><br /><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m101.jpg"><img align="right" alt="[m101.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m101.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">14 : 03.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+54 : 21 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">27000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">22.0 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.</div>
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Messier 101 (M101, NGC 5457) was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on March 27, 1781, and added as <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M101">one of the last entries</a> in <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>'s <a href="http://messier.obspm.fr/xtra/history/m-cat.html">catalog</a>. It was one of the <a href="http://messier.obspm.fr/more/m101_rosse.html">first "spiral nebula"</a>identified as such, in 1851 by <a href="http://messier.obspm.fr/xtra/Bios/rosse.html">William Parsons, the third Earl of Rosse</a>.</div>
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Although extended 22 arc minutes on photos and quite bright, only the central region of this galaxy is visible in smaller telescopes, best at low powers. Suggestions of the spiral arms can be glimpsed in telescopes starting from 4 inch as nebulous patches. Several of these patches (i.e., spiral arm fragments) were assigned their own catalog numbers by William Herschel and later observers; according to the NGC and Burnham, there are 9 such numbers, 3 of which go back to Herschel who has found them on April 14, 1789, while the RNGC states that five of the others don't exist (ne); it mentions however that deVaucouleurs has them as knots: NGC 5447 (H III.787), 5449 (ne), 5450 (ne), 5451 (ne), 5453 (ne), 5455, 5458 (ne), 5461 (H III.788), 5462 (H III.789), and 5471.</div>
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On photographs, however, the Pinwheel Galaxy M101 is revealed as one of the most prominent Grand Design spirals in the sky. While quite symmetric visually and in very short exposures which show only the central region, it is of remarkable unsymmetry, its core being considerably displaced from the center of the disk. Halton Arp has included M101 as No. 26 in his <a href="http://messier.obspm.fr/xtra/supp/m-arp.html">Catalogue of Peculiar Galaxies</a> as a "Spiral with One Heavy Arm".</div>
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LEIA MAIS</div>
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http://messier.obspm.fr/m/m101.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhYe73wt9RIJ06lSE7DnH1QjuUuSpNv5R08xijWTg1BphhIPTrFafETCU48WXxh0kxl2FpTp3Z1Qtq_EybbI5eOXb82b_LGnnTm4zllay1bcq7RPrzkp9yNy_9-6LBOayJgGFX7GcuKP58/s1600/M101.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhYe73wt9RIJ06lSE7DnH1QjuUuSpNv5R08xijWTg1BphhIPTrFafETCU48WXxh0kxl2FpTp3Z1Qtq_EybbI5eOXb82b_LGnnTm4zllay1bcq7RPrzkp9yNy_9-6LBOayJgGFX7GcuKP58/s1600/M101.png" /></a></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 5457 - M 101 - Galáxia Ursa Maior</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 14h01m Declinação +54<sup>o</sup>.26<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo S - Galáxia Espiral Magnitude fotográfica aparente 8,20<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões Angulares 23 X 21 Distância (milhões de anos-luz) 14,0</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M101 - NGC 5457 - Galáxia<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um dos mais belos exemplos de galáxia Sc </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">com braços espiralados pronunciados.<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6a. Edição do Atlas Celeste</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Cata-Vento#mediaviewer/File:Hs-2009-07-b-full_jpg.jpg<br />
<span style="background-color: #f9f9f9; color: #252525; font-family: sans-serif; line-height: 17.3185615539551px; text-align: left;">Galáxia do Cata-Vento, </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background: none rgb(249, 249, 249); color: #0b0080; font-family: sans-serif; line-height: 17.3185615539551px; text-align: left;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a><br />
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A <b>Galáxia do Cata-Vento</b> (catalogada também como <b>NGC 5457</b> ou <b>M101</b>), é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> localizada a cerca de vinte e sete milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>(aproximadamente 8,278 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Ursa_Maior" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação de Ursa Maior">constelação de Ursa Maior</a>. Possui entre cento e setenta e duzentos mil anos-luz de <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a>, uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 7,5, uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> de -21,6, uma declinação de +54º 20' 55" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 14 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a> 03 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> 12,4 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</div>
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A galáxia NGC 5457 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/27_de_Mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="27 de Março">27 de Março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>.</div>
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LEIA MAIS</div>
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em</div>
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<span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Cata-Vento#mediaviewer/File:M101_hires_STScI-PRC2006-10a.jpg</span></div>
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<span class="mw-mmv-title" original-title="" style="max-width: 60%;">the galaxy Messier 101 (M101, also known as NGC 5457 and also nicknamed the Pinwheel Galaxy) lies in the northern circumpolar constellation, Ursa Major (The Great Bear), at a distance of about 21 million light-years from Earth. This is one of the largest and most detailed photo of a spiral galaxy that has been released from Hubble. The galaxy's portrait is actually composed of 51 individual Hubble exposures, in addition to elements from images from ground-based photos. A high-res version with 15852 x 12392 pixels in jpg and tiff format is also available, see below for url</span></div>
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<span class="mw-mmv-source-author" original-title="" style="line-height: 1.8em;"><span class="mw-mmv-author"> Credit: Image: European Space Agency & NASA Acknowledgements: Project Investigators for the original Hubble data: K.D. Kuntz (GSFC), F. Bresolin (University of Hawaii), J. Trauger (JPL), J. Mould (NOAO), and Y.-H. Chu (University of Illinois, Urbana) Image processing: Davide De Martin (ESA/Hubble) CFHT image: Canada-France-Hawaii Telescope/J.-C. Cuillandre/Coelum NOAO image: George Jacoby, Bruce Bohannan, Mark Hanna/NOAO/AURA/NSF</span> -<span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/news/html/heic0602.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/news/html/heic0602.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/large/heic0602a.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>) See also: <a class="external free" href="http://hubblesite.org/newscenter/newsdesk/archive/releases/2006/10/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/newsdesk/archive/releases/2006/10/image/a</a></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando alcançamos o Objeto Messier 102,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">nos encontramos diante de situações bem polêmicas</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e que já foram comentadas anteriormente</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em nosso Trabalho</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sobre o Objeto Messierr 102 (?) em Draco</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com.br/2014/10/m102-objeto-messier-em-draco-ou-ngc.html">http://oceudomes.blogspot.com.br/2014/10/m102-objeto-messier-em-draco-ou-ngc.html</a></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e que acabo transcrevendo mais abaixo:</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>SOBRE M102:</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><b>Objeto Messier localizado na constelação Draco</b></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><b>ou </b></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><b>na constelação Ursa Major?</b></span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M102, Objeto Messier em Draco (?) </b></span><br />
<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">ou</span></b></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 5866, Galáxia do Fuso/do Eixo?</span></b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ou ainda</b></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;"> ..... </span><span style="color: #660000;">uma duplicata</span><span style="color: #073763;"> de M101, em Ursa Major?</span></b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta dicotomia</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">pode nos trazer, em um primeiro momento,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma surpresa e uma indagação de seu porquê !?!</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O Caro Leitor</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">haverá de encontrar situações informativas:</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- comentário </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">citando apenas NGC 5866, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sem mencionar M102), </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em pequeno trecho mais abaixo compilado</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">do astrônomo Ronaldo Rogério de Freitas Mourão:</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 5866 - Galáxia</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma galáxia observada de lado </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e mostrando uma banda estreita e escura ao longo de seu equador.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- cartas celestes não mencionando nem NGC 5866 e nem M102</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(Ilustrações em cartas celestes realizadas por</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Mario Jaci Monteiro e por IAU)</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- Imagens realizadas por Nasa/Esa</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">apresentando a Galáxia Lenticular como NGC 5866</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e não mencionando M102</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(e ainda Imagem apresentada por Apod)</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- ilustrações advindas do Programa Stellarium</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">apresentando M102 - NGC 5866 como um mesmo objeto celeste</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- a imagem realizada por Two Micron All Sky Survey</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">nos apresenta o Objeto Messier 102</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> seguido de um ponto de interrogação entre-parênteses</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> (denotando a dúvida/controvérsia acerca este objeto celeste).</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m102atlas.jpg</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"><br />- Situações não muito bem explicadas, dúvidas, duplo êrro, não-verificação,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e até situações bem controversas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> acerca trabalhos realizados por Messier e Mechain,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> sugerem que o objeto observado e catalogado foi, na verdade,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> a galáxia lenticular NCG 5866, denominada Galáxia do Fuso/do Eixo... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e ainda incluindo a possibilidade de engano,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> ou seja,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> de que o objeto que teria sido nomeado enquanto M102 </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">seria uma possível duplicata do Objeto Messier 101, em Ursa Maior... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">Ao final, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">parece que tanto Messier quanto Mechain observaram NGC 5866 no passado </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e, portanto, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">este objeto acabou sendo listado </span></div>
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<span style="font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como o item perdido (no Catálogo Messier).</span><span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><br /></span></div>
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<span style="color: #073763; font-family: "Arial","sans-serif"; mso-themecolor: text2; mso-themeshade: 128;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">Leia mais abaixo, Caro Leitor,<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">trechos de comentários e explicações<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">sobre estas situações tão controversas<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">extraídos dos Sites:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">http://messier.obspm.fr/m/m102.html</span><br />
<span style="text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">http://messier.obspm.fr/m/ngc5866.html</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">http://pt.wikipedia.org/wiki/Messier_102</span><br />
<span style="text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Grupo_NGC_5866</span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m102atlas.jpg" /></div>
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http://www.ipac.caltech.edu/2mass/gallery/m102atlas.jpg</div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a></div>
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<h1>
Messier 102</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Galaxy</a> M102</i>(<a href="http://messier.obspm.fr/m/m101.html">M101</a> or <a href="http://messier.obspm.fr/m/ngc5866.html">NGC 5866</a>)</center>
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<a href="http://messier.obspm.fr/Jpg/m102.jpg"><img alt="[m102.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m102.jpg" /></a></center>
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Evidently, Messier 102 (M102) is the last possibly "<a href="http://messier.obspm.fr/missing.html">missing</a>", or doubty, Messier object. This means that, based on the observation record of his friend, <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a>, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included this object <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M102">in his catalog</a> without verifying before publication, and it happens that Méchain's published position is erroneous. Two opinions on the identity of this object are common:<br />
<ol>
<li>M102 might be a duplication of the <i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> <a href="http://messier.obspm.fr/m/m101.html">M101 (NGC 5457)</a></i> in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a>, due to a possible error of either the catalog author Messier, or its `discoverer' Méchain, a view brought up by Méchain in a <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m102">letter of May 1783</a>.</li>
<li>Perhaps more probably (<a href="http://messier.obspm.fr/m/m102d.html">due to historical evidence</a>), M102 may be the <i><a href="http://messier.obspm.fr/galaxy.html">Lenticular Galaxy</a> <a href="http://messier.obspm.fr/m/ngc5866.html">NGC 5866</a></i> in <a href="http://messier.obspm.fr/map/Dra.html">Draco</a>, also sometimes called the <i>Spindle Galaxy</i>, as Messier's catalog description indicates, together with the position he added later by hand in his personal copy.</li>
</ol>
The authors of this page think that there is sufficient evidence that both Méchain and Messier have probably observed NGC 5866 in context of this catalog entry. Therefore, it should be considered to take this last missing object back into the catalog.<br />
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Please note our discussion of <a href="http://messier.obspm.fr/m/m102d.html">more details on this topic</a>.<br />
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<br />
LEIA MAIS<br />
em<br />
http://messier.obspm.fr/m/m102.html<br />
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<span style="color: #38761d;"><br /></span><span style="color: #38761d;"><br /></span><br />
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<h1>
<span style="color: #38761d;">NGC 5866 / Messier 102 ?</span></h1>
<span style="color: #38761d;"><i><a href="http://messier.obspm.fr/galaxy.html">Lenticular (S0) Galaxy</a> NGC 5866 (M102 ?)</i>, type S0_3, in <a href="http://messier.obspm.fr/map/Dra.html">Draco</a></span></center>
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<span style="color: #38761d;"><br /><b><span style="font-size: large;">Spindle Galaxy</span></b><br /><b><br /></b><b><br /></b></span></center>
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<tr><th align="left"><span style="color: #38761d;">Right Ascension</span></th><td align="center"><span style="color: #38761d;">15 : 06.5 (h:m)</span></td></tr>
<tr><th align="left"><span style="color: #38761d;">Declination</span></th><td align="center"><span style="color: #38761d;">+55 : 46 (deg:m)</span></td></tr>
<tr><th align="left"><span style="color: #38761d;">Distance</span></th><td align="center"><span style="color: #38761d;">45000 (kly)</span></td></tr>
<tr><th align="left"><span style="color: #38761d;">Visual Brightness</span></th><td align="center"><span style="color: #38761d;">9.9 (mag) </span></td></tr>
<tr><th align="left"><span style="color: #38761d;">Apparent Dimension</span></th><td align="center"><span style="color: #38761d;">5.2x2.3 (arc min)</span></td></tr>
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<span style="color: #38761d;"><br /></span><span style="color: #38761d;"><br /></span><span style="color: #38761d;">Discovered probably either by Pierre Méchain or by Charles Messier in 1781.</span><br />
<span style="color: #38761d;"><br /></span><span style="color: #38761d;">Independently discovered by William Herschel in 1788.</span><br />
<span style="color: #38761d;"><br /></span><span style="color: #38761d;">NGC 5866 is a beautiful lenticular galaxy in Northern constellation Draco, which is seen almost exactly edge-on, showing a prominent dust lane along its equatorial plane. It is prominent for being a good candidate for <a href="http://messier.obspm.fr/m/m102.html">Messier Object 102</a>, i.e., Messier 102 (M102).</span><br />
<span style="color: #38761d;"><br /></span><span style="color: #38761d;">NGC 5866 was probably first seen by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> in March 1781, or by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> shortly after that time. Therefore, NGC 5866 is possibly <a href="http://messier.obspm.fr/m/m102.html">M102</a>, although Pierre Méchain <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m102">disclaimed the discovery</a> two years later. Pierre Méchain's first observing report caused Messier to include it as <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M102">entry No. 102</a> in his catalog, without giving a position or further verification. Soon after, Messier added a position measurement for this object (or entry) to his personal copy of the catalog, probably shortly after publication, and still in 1781. There is evidence that Charles Messier has probably observed NGC 5866 when measuring this position, as this is almost exactly 5 degrees preceding (west) of the actual position of the object: Very probably a data reduction error of some kind. Nevertheless, this subject is still somewhat dubious and therefore <a href="http://messier.obspm.fr/m/m102d.html">controversial</a>. If, despite this evidence, it should be true that neither Méchain nor Messier have observed NGC 5866, it was probably first seen by <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> when independently discovering it in 1788; William Herschel determined its position on May 5, 1788. As the possible earlier sightings by Méchain and Messier did not result in a published position for this object, this galaxy bears <a href="http://messier.obspm.fr/xtra/similar/herschel.html">Herschel's number H I.215</a>.</span><br />
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<span style="color: #38761d;"><br /></span><span style="color: #38761d;">LEIA MAIS</span><br />
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<span style="color: #38761d;">http://messier.obspm.fr/m/ngc5866.html</span><br />
<span style="color: #38761d;"><br /></span><span style="color: #38761d;"><br /></span><span style="color: #38761d;"><br /></span><span style="color: #38761d;"><br /></span><span style="color: #38761d;"><img alt="Finder Chart for M102 (also shown M51 and M101)" src="https://blogger.googleusercontent.com/img/proxy/AVvXsEi0cR_WPjkM_5bFNDEQAUD37gUUT_rgmPFO3zVRX3P-Z4eCoqYgEhdiwqONW1IT3O4NsJAwhVRT9xp8XWEN-oyeui8KCyATcrMPDSQTCPdivNnCEidxF8h09kkej-aZpQygKPgEqwJjxcqvLexiZT3Mz_zKHSmns7e_BLuK_FkcoSdJoRd5i58=" /></span><br />
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<span style="color: #38761d;"><b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><a href="http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy"><span lang="EN-US" style="color: blue; mso-ansi-language: EN-US; mso-bidi-font-size: 11.0pt;">Messier 102 - M102 - NGC 5866 - Spindle Galaxy (Lenticular Galaxy)</span></a></span></b><b><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></b></span></div>
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<span style="color: #38761d;"><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">M102 is a galaxy catalogued by Charles Messier that hasn't been explicitly identified. It was Pierre Mechain who made the original observation in March 1781 before passing the information onto Messier, who catalogued it without verification. However, Mechain himself believed M102 was an error and wrote a letter on the May 6, 1783 expressing his view that the object was in fact a duplicate entry of</span><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;"> </span><span style="font-family: Arial, sans-serif; font-size: 9.5pt;"><a href="http://freestarcharts.com/index.php/20-guides/messier/251-messier-101-m101-the-pinwheel-galaxy-spiral-galaxy"><span lang="EN-US" style="color: blue; mso-ansi-language: EN-US; mso-bidi-font-size: 11.0pt;">M101</span></a></span><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">. The story does not end there, historical evidence based on Messier description of the galaxy combined with its co-ordinates suggest that M102 could well be lenticular galaxy NGC 5866, also known as the Spindle galaxy. A number of other possible candidates have been suggested but it seems both Messier and Mechain have observed NGC 5866 in the past and therefore we list it as the missing item.<o:p></o:p></span></span></div>
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<span style="color: #38761d;"><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">The Spindle galaxy (mag. +9.9) is located at the southern edge of the far northern constellation of Draco. It's positioned four degrees southwest of star Iota Draconis (</span><span style="font-family: Arial, sans-serif; font-size: 9.5pt;">ι</span><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;"> Dra - mag. +3.3). Directly west of NGC 5866 are the seven stars that form the famous "Plough" or "Big Dipper" asterism of Ursa Major.<o:p></o:p></span></span></div>
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<span lang="EN-US" style="color: #38761d; font-family: Arial, sans-serif; font-size: 9.5pt;">NGC 5866 is a challenging binocular object but easier to spot with small scopes. It's best seen from the Northern Hemisphere during the months of April, May and June. From latitudes of 35N or greater, the galaxy is circumpolar and therefore never sets.<o:p></o:p></span></div>
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<span lang="EN-US" style="color: #38761d; font-family: Arial, sans-serif; font-size: 9.5pt;"><a href="http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal;">http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy</a></span></div>
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<span lang="EN-US" style="color: #38761d; font-family: Arial, sans-serif; font-size: 9.5pt;"><i>(Minha, Janine, tradução simples e direta da primeira parte do texto acima)</i></span></div>
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<span style="color: #38761d; font-family: Arial, sans-serif;"><i>M102 é uma galáxia catalogada por Charles Messier mas que não foi explicitamente identificada. Pierre Mechain foi quem originalmente observou-a em março de 1781 e ainda antes de passar esta informação para Messier – que catalogou a galáxia sem verificação. No entanto, Mechain acreditou que M102 foi um erro e escreveu uma carta datada de 6 de maio de 1783, expressando sua visão de que o objeto era, de fato, uma duplicata catalogada de M101. A história não termina aí, pois que evidências históricas baseadas na descrição de Messier sobre a galáxia combinaram com as coordenadas sugeridas que M102 poderia bem ser a galáxia lenticular NCG 5866, também conhecida como galáxia do Fuso ou do Eixo. Um número de outros possíveis candidatos foi sugerido porém parece que tanto Messier quanto Mechain observaram NGC 5866 no passado e, portanto, este objeto acabou sendo listado como o item perdido (no Catálogo Messier).</i><o:p></o:p></span></div>
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<b><span style="color: #38761d; font-family: Arial, Helvetica, sans-serif;">LEIA MAIS SOBRE M102 - NGC 5866</span></b></div>
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<a href="http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy"><span style="color: #38761d;">http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy</span></a></div>
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<span style="background-color: white; color: #38761d; font-family: Arial, Helvetica, sans-serif;"><b>NGC 5866 - Galáxia</b></span></div>
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<span style="background-color: white; color: #38761d; font-family: Arial, Helvetica, sans-serif;">Uma galáxia observada de lado </span></div>
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<span style="background-color: white; color: #38761d; font-family: Arial, Helvetica, sans-serif;">e mostrando uma banda estreita e escura ao longo de seu equador.<o:p></o:p></span></div>
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<span style="color: #38761d; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #38761d; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="color: #38761d; font-family: Arial, sans-serif; font-size: 11pt; line-height: 22.3999996185303px;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #38761d;">http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/format/web_print/</span></div>
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<span style="color: #38761d;"><strong>Object Name:</strong> NGC 5866</span></div>
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<span style="color: #38761d;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="color: #38761d;"><span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)</span></div>
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<span style="color: #38761d;"><span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Acknowledgment:</span> W. Keel (University of Alabama, Tuscaloosa)</span></div>
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<span style="font-family: arial, sans-serif; font-size: x-small;"><span style="color: #38761d; line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/</span></span></div>
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<span style="color: #38761d;"><br /><br /><br /><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">NGC 5866</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> ou </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">Galáxia do Fuso</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> (e possivelmente </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">Messier 102</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">)</span><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> localizada a cerca de quarenta milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> (aproximadamente 12,26</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">) de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Drag%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px;" title="Constelação do Dragão">constelação do Dragão</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> de 9,9, uma declinação de +55º 45' 47" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> de 15</span><a href="http://pt.wikipedia.org/wiki/Hora" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Hora">horas</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">, 06 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Minuto">minutos</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> e 29,3 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Segundo">segundos</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">. Contudo, devido à razões históricas, existe a possibilidade de Messier 102 ser uma duplicata de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_101" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 101">Messier 101</a><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">.</span></span><br />
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<span style="color: #38761d;">Messier 102 tem sido considerado um objeto perdido por muito tempo e frequentemente tem sido tomado como uma duplicação de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_101" style="background: none; text-decoration: none;" title="Messier 101">Messier 101</a> no <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; text-decoration: none;" title="Catálogo Messier">catálogo de objetos do céu profundo</a> do astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; text-decoration: none;" title="Charles Messier">Charles Messier</a>. Por outro lado, evidências históricas dão conta que M102 poderia ser a galáxia <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5866" style="background: none; text-decoration: none;" title="NGC 5866">NGC 5866</a>.<span class="reference" id="cite_ref-seds_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">Em meados de 1781, Messier e seu assitente, <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, empreenderam um grande projeto com o intuito de descobrir e catalogar novos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background: none; text-decoration: none;" title="Objetos do céu profundo">objetos do céu profundo</a>: em abril daquele ano, ambos já tinham verificado as posições de 100 objetos. A data limite para novas adições ao anuário astronômico francês <i><a href="http://pt.wikipedia.org/wiki/Connaissance_des_temps" style="background: none; text-decoration: none;" title="Connaissance des temps">Connaissance des temps</a></i> estava se aproximando e Messier adicionou outros três objetos descobertos por Méchain, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_101" style="background: none; text-decoration: none;" title="Messier 101">Messier 101</a>, 102 e <a href="http://pt.wikipedia.org/wiki/Messier_103" style="background: none; text-decoration: none;" title="Messier 103">103</a>, sem a devida verificação de suas posições. A versão impressa do catálogo contém uma única posição para M101 e M102 e apenas as descrições para M103 são fornecidas. Contudo, Messier adicionou as posições de ambos os objetos em sua cópia pessoal e sempre houve consenso sobre a identidade de M101 e M103.<span class="reference" id="cite_ref-seds_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">Cerca de dois anos depois, Méchain retratou sua descoberta e afirmou que sua observação tinha sido um erro, uma observação duplicada de M101. Em 6 de maio de 1783, escreveu uma carta a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Jacob_Bernoulli" style="background: none; text-decoration: none;" title="Jacob Bernoulli">Jacob Bernoulli</a> onde descreve suas observações de "nebulosas" que não estavam na edição do catálogo de 1781. Com base nessa carta,<a href="http://pt.wikipedia.org/wiki/Helen_Sawyer_Hogg" style="background: none; text-decoration: none;" title="Helen Sawyer Hogg">Helen Sawyer Hogg</a> em 1947 e <a href="http://pt.wikipedia.org/wiki/Owen_Gingerich" style="background: none; text-decoration: none;" title="Owen Gingerich">Owen Gingerich</a> em 1953 adicionaram os objetos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_104" style="background: none; text-decoration: none;" title="Messier 104">M104</a> a <a href="http://pt.wikipedia.org/wiki/Messier_109" style="background: none; text-decoration: none;" title="Messier 109">M109</a> na versão moderna do catálogo.<span class="reference" id="cite_ref-seds_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">GC 5866 foi sugerido pela primeira vez como candidato ao objeto perdido em 1917 por <a href="http://pt.wikipedia.org/wiki/Camille_Flammarion" style="background: none; text-decoration: none;" title="Camille Flammarion">Camille Flammarion</a>, que havia adquirido as cópias pessoais de Messier. Além disso, outro fato torna NGC 5866 bom candidato para M102: situado próximo a ele, cerca de 1 grau ao sul, situa-se a estrela de magnitude aparente 5,25 HR 5635, adequada para ajudar a encontrar o objeto. Portanto, é uma boa candidata para ser a "estrela de magnitude 6" mencionada na descrição de Méchain e Messier: não há nenhuma estrela útil nas vizinhanças de M101 no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-seds_4-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">Ainda mais importante para a identificação de M102 é a evidência histórica que Charles Messier provavelmente tenha observado NGC 5866 na tentativa de verificar o objeto M102. Em sua cópia pessoal do catálogo, o astrônomo francês acrescentou posições aproximadas para ambos os objetos M102 e M103, provavelmente logo após a sua publicação em 1781. Estas posições só foram publicadas novamente por Flammarion em 1921.<span class="reference" id="cite_ref-seds_4-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">Porém, novamente há erros na descrição do astrônomo francês: não há nenhum objeto óbvio perto da posição descrita por Messier. Mas considerando válido que a referência a "Omicron" seria um erro de impressão e que na verdade seria "Theta", existe de fato um objeto que está situado quase exatamente 5 graus da descrição dada inicialmente por Messier: NGC 5866.<span class="reference" id="cite_ref-seds_4-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">Messier usava cotidianamente <a href="http://pt.wikipedia.org/wiki/Carta_celeste" style="background: none; text-decoration: none;" title="Carta celeste">cartas celestes</a> com grades de linhas com divisões a cada 5 graus e pode ter ocorrido um erro na rotulação do objeto. O astrônomo francês tinha cometido um erro semelhante na redução de dados para o cálculo da posição de um outro objeto ausente, <a href="http://pt.wikipedia.org/wiki/Messier_48" style="background: none; text-decoration: none;" title="Messier 48">M48</a>, que também tinha um desvio de 5 graus.<span class="reference" id="cite_ref-seds_4-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<span style="color: #38761d;">Portanto, parece provável que Charles Messier tenha observado NGC 5866 quando media a posição de M102, objeto que ele provavelmente poderia localizar sem muita dificuldade por causa da descrição acurada de Méchain, mas devido a algum erro reducional, foi plotado exatamente 5 graus a oeste de sua posição correta.<span class="reference" id="cite_ref-seds_4-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; text-decoration: none; white-space: nowrap;">4</a></span></span></div>
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<table border="0" cellpadding="3" class="infobox_v2" style="background: rgb(249, 249, 249); border: 1px solid rgb(170, 170, 170); clear: right; color: black; font-family: sans-serif; font-size: 12px; line-height: 1.1em; margin: 0px 0px 0.5em 1em; padding: 2px; width: 20em;"><tbody>
<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="" style="font-weight: normal;"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">NGC 5866 (possivelmente Messier 102)</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:File-Ngc5866_hst_big.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; margin-left: auto; margin-right: auto;"><span style="color: #38761d; font-family: Times New Roman; font-size: small;"><img alt="" data-file-height="3756" data-file-width="3190" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5c/File-Ngc5866_hst_big.png/280px-File-Ngc5866_hst_big.png" height="330" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5c/File-Ngc5866_hst_big.png/420px-File-Ngc5866_hst_big.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5c/File-Ngc5866_hst_big.png/560px-File-Ngc5866_hst_big.png 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></span></a></div>
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<small><span style="color: #38761d; font-family: Times New Roman; font-size: small;">NGC 5866, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></small></td></tr>
<tr><td scope="row" valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Descoberto por</span></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Pierre Méchain"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Pierre Méchain</span></a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="color: #38761d; font-weight: normal;">Dados observacionais (J2000)</span></span></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Constelação"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Constelação</span></a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Draco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Draco"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Draco</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Tipo</span></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">S0<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ascensão reta"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Asc. reta</span></a></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">15<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 06<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 29.5<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Declinação"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Declinação</span></a></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">+55° 45′ 48″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Distância</span></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">50 ± 3 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ano-luz">Mal</a> (15,3 ± 0,7 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Parsec">Mpc</a><span class="reference" id="cite_ref-tonryetal2001_2-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-tonryetal2001-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span> )</span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Desvio para o vermelho"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Redshift</span></a></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">672 ± 9 km/<a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Segundo">s</a><span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Magnitude aparente"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Magnit. apar.</span></a></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">10,7<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Dimensões</span></td><td valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">4′,7 x 1′,9<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="color: #38761d; font-weight: normal;">Outras denominações</span></span></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><span style="color: #38761d; font-family: Times New Roman; font-size: small;">Galáxia do Fuso,<span class="reference" id="cite_ref-simbad_3-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-simbad-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">3</a></span> <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Uppsala General Catalogue">UGC</a> 9723,<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 53933<span class="reference" id="cite_ref-ned_1-7" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="color: #38761d; font-weight: normal;">Mapa</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Messier 102"><span style="color: #38761d; font-family: Times New Roman; font-size: small;"><img alt="Messier 102" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Draco_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;"><span style="color: #38761d; font-family: Times New Roman; font-size: small;"><img alt="Draco constellation map.png" data-file-height="2839" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Draco_constellation_map.png/240px-Draco_constellation_map.png" height="266" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Draco_constellation_map.png/360px-Draco_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Draco_constellation_map.png/480px-Draco_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></span></a></div>
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<span style="color: #38761d;">http://pt.wikipedia.org/wiki/Messier_102</span><br />
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<span style="background-color: white; color: #38761d;">Hubble Sees Galaxy on Edge</span></h1>
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<span style="color: #38761d;">http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/format/xlarge_web/</span></div>
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<span style="color: #38761d;"><strong>Object Name:</strong> NGC 5866</span></div>
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<span style="color: #38761d;"><strong>Image Type:</strong> Astronomical</span></div>
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<span style="color: #38761d;"><span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)</span></div>
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<span style="color: #38761d;"><span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Acknowledgment:</span> W. Keel (University of Alabama, Tuscaloosa)</span></div>
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<span style="font-family: arial, sans-serif; font-size: x-small;"><span style="color: #38761d; line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/</span></span></div>
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<span style="color: #38761d;"><b>O Grupo NGC 5866 é um pequeno <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Grupo_de_gal%C3%A1xias&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Grupo de galáxias (página não existe)">grupo de galáxias</a> na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Draco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Draco">Draco</a>. O grupo está nomeado como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5866" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="NGC 5866">NGC 5866</a></b>, pois ela é galáxia com maior <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> no grupo, embora alguns catálogos de grupos de galáxias listam <a href="http://pt.wikipedia.org/wiki/NGC_5907" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5907">NGC 5907</a> como o membro mais brilhante.<span class="reference" id="cite_ref-garcia1993_1-5" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-garcia1993-1" style="background: none; text-decoration: none; white-space: nowrap;">1</a></span> <span class="reference" id="cite_ref-giuricinetal2002_2-7" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-giuricinetal2002-2" style="background: none; text-decoration: none; white-space: nowrap;">2</a></span></span></div>
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<span class="mw-headline" id="Membros" style="color: #38761d; font-family: 'Linux Libertine', Georgia, Times, serif; font-size: large; line-height: 1.3;">Membros</span></div>
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<span style="color: #38761d;">A tabela abaixo lista todas as <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xias" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxias">galáxias</a> identificadas e confirmadas como membros do grupo pelo Nearby Galaxies Catalog,<span class="reference" id="cite_ref-nbg_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-nbg-3" style="background: none; text-decoration: none; white-space: nowrap;">3</a></span> o Lyons Groups of Galaxies (LGG) Catalog,<span class="reference" id="cite_ref-garcia1993_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-garcia1993-1" style="background: none; text-decoration: none; white-space: nowrap;">1</a></span> e três listas de grupos criados pelo Nearby Optical Galaxy sample of Giuricin et al.<span class="reference" id="cite_ref-giuricinetal2002_2-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></span></div>
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<table cellpadding="2" class="wikitable" style="background-color: #f9f9f9; border-collapse: collapse; border: 1px solid rgb(170, 170, 170); color: black; font-family: sans-serif; font-size: 14px; line-height: 22.3999996185303px; margin: 1em 0px; text-align: center;"><caption style="font-weight: bold;"><b><span style="color: #38761d;">Membros do Grupo NGC 5866</span></b></caption><tbody>
<tr><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">Nome</span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;"><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_de_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Classificação de Hubble">Tipo</a><span class="reference" id="cite_ref-ned_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">4</a></span></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Ascensão reta">R.A.</a> (J2000)<span class="reference" id="cite_ref-ned_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">4</a></span></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Declinação">Dec.</a> (J2000)<span class="reference" id="cite_ref-ned_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">4</a></span></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Redshift" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Redshift">Redshift</a> (<a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Quilômetro">km</a>/<a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Segundo">s</a>)<span class="reference" id="cite_ref-ned_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">4</a></span></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Magnitude aparente">Magnitude</a><span class="reference" id="cite_ref-ned_4-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">4</a></span></span></th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5866" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="NGC 5866"><span style="color: #38761d;">NGC 5866</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">S0</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 06<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 29.5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">+55° 45′ 48″</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">672 ± 9</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">10.7</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/NGC_5879" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="NGC 5879"><span style="color: #38761d;">NGC 5879</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">SA(rs)bc</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 09<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 46.8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">+57° 00′ 01″</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">772 ± 5</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">12.4</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/NGC_5907" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="NGC 5907"><span style="color: #38761d;">NGC 5907</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">SA(s)c</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 53.8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">+56° 19′ 44″</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">667 ± 3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #38761d;">11.1</span></td></tr>
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<span style="color: #38761d;">Outros possíveis membros (galáxias listadas com uma ou duas de algumas referências acima) incluem <a class="new" href="http://pt.wikipedia.org/w/index.php?title=NGC_5866B&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="NGC 5866B (página não existe)">NGC 5866B</a>, <a href="http://pt.wikipedia.org/wiki/NGC_5963" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5963">NGC 5963</a>, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_9776&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="UGC 9776 (página não existe)">UGC 9776</a> e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_9816&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="UGC 9816 (página não existe)">UGC 9816</a>.</span></div>
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<span class="mw-headline" id="Grupos_pr.C3.B3ximos" style="color: #38761d;">Grupos próximos</span></h2>
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<span style="color: #38761d;">O Grupo NGC 5866 está localizado ao noroeste do <a href="http://pt.wikipedia.org/wiki/Grupo_M101" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grupo M101">Grupo M101</a> (que contém a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Catavento" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Catavento">Galáxia do Catavento (M101)</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia satélite">galáxias satélites</a> e companheiras) e o <a href="http://pt.wikipedia.org/wiki/Grupo_M51" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grupo M51">Grupo M51</a> (que contém a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Rodamoinho" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Rodamoinho">Galáxia do Rodamoinho (M51)</a>, a<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Girassol" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Girassol">Galáxia do Girassol (M63)</a> e algumas outras galáxias)<span class="reference" id="cite_ref-ferrareseetal00_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ferrareseetal00-5" style="background: none; text-decoration: none; white-space: nowrap;">5</a></span> . As distâncias para estes três grupos (como determinadas pelas distâncias para os membros individuais) são similares, com sugestões de que o Grupo M51, o Grupo M101 e o Grupo NGC 5866 são atualmente parte de um grande, e solta, larga estrutura.<span class="reference" id="cite_ref-ferrareseetal00_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ferrareseetal00-5" style="background: none; text-decoration: none; white-space: nowrap;">5</a></span> Contudo, a maior parte de métodos para identificação (incluindo por referências citadas acima) têm estes três grupos como grupos separados.</span></div>
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<span style="color: #38761d;">http://pt.wikipedia.org/wiki/Grupo_NGC_5866</span></div>
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<span style="color: #38761d;"><br /><a href="http://apod.nasa.gov/apod/image/0606/ngc5866_hst_big.jpg"><img alt="See Explanation. Clicking on the picture will download
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<b><span style="color: #38761d;">http://apod.nasa.gov/apod/ap060612.html</span></b></center>
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<span style="color: #38761d;"><b>Edge-On Galaxy NGC 5866 </b><br /><b>Credit: </b><a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> <a href="http://heritage.stsci.edu/commonpages/infoindex/ourproject/moreproject.html">Team</a> (<a href="http://www.stsci.edu/resources/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>); <b>Acknowledgment: </b><a href="http://www.astr.ua.edu/keel/billkeel.html">W. Keel</a> (<a href="http://www.astr.ua.edu/">U. Alabama</a>)</span></center>
<span style="color: #38761d;"><b>Explanation: </b>Why is this galaxy so thin? Many disk galaxies are actually just as thin as NGC 5866, <a href="http://hubblesite.org/newscenter/newsdesk/archive/releases/2006/24/">pictured above</a>, but are not <a href="http://apod.nasa.gov/apod/ap010510.html">seen edge-on</a> from our vantage point. One galaxy that is situated edge-on is our own <a href="http://apod.nasa.gov/apod/ap050605.html">Milky Way Galaxy</a>. Classified as a <a href="http://apod.nasa.gov/apod/ap020408.html">lenticular galaxy</a>, NGC 5866 has numerous and complex dust lanes appearing dark and red, while many of the bright stars in the disk give it a more blue underlying hue. The blue disk of young stars can be seen extending past the <a href="http://apod.nasa.gov/apod/ap990919.html">dust</a> in the extremely thin galactic plane, while the bulge in the disk center appears tinged more orange from the older and redder stars that likely exist there. Although similar in mass to our Milky Way Galaxy, light takes about 60,000 <a href="http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html">years</a> to cross <a href="http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...20311002K">NGC 5866</a>, about 30 percent less than light takes to cross our own Galaxy. In general, many disk galaxies are very thin because the gas that <a href="http://en.wikipedia.org/wiki/Galaxy_formation_and_evolution">formed them</a> collided with itself as it rotated about the gravitational center. Galaxy <a href="http://en.wikipedia.org/wiki/NGC_5866">NGC 5866</a> lies about 44 million light years distant toward the constellation of the Dragon (<a href="http://www.astronomical.org/portal/modules/wfsection/article.php?articleid=34">Draco</a>).</span></div>
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<span style="background-color: white; color: #0000ee; text-decoration: underline;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></div>
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Messier 108</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M108 (NGC 3556)</i>, type Sc, in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">11 : 11.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+55 : 40 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">45000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">10.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">8x1 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.</div>
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Messier 108 (M108, NGC 3556) is a nice edge-on spiral galaxy situated near the conspicuous star Beta Ursa Majoris, and in one field of view with the <a href="http://messier.obspm.fr/m/m097.html">Owl Nebula, M97</a>.</div>
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According to <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>'s hand-written preliminary and unpublished version of <a href="http://messier.obspm.fr/xtra/history/m-cat.html">his catalog</a>, M108, similar to <a href="http://messier.obspm.fr/m/m109.html">M109</a>, was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> shortly after <a href="http://messier.obspm.fr/m/m097.html">M97</a> (which he had found February 16, 1781): Méchain discovered M108 3 days after M97 on February 19, 1781, and M109 on March 12, 1781. Both objects were apparently also observed by Charles Messier when he measured the position of M97 (March 24, 1781), but apparently he didn't find occasion to obtain positions for these objects at that time. Messier <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M108">listed this object</a>, M108, under number "98" in his preliminary manuscript version of his catalog, without giving a position. According to <a href="http://messier.obspm.fr/xtra/Bios/gingerich.html">Owen Gingerich</a>, he measured an acurate position at a later time which he added by hand in his personal copy of the catalog. Both objects M108 and M109 are also mentioned in <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m108">Pierre Méchain's letter</a> of May 6, 1783, which supports the suspicion that he probably wanted to add them to a later edition of Messier's catalog. The object M108 was finally <a href="http://messier.obspm.fr/addition.html">added</a> to Messier's catalog by Owen Gingerich in 1953.</div>
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As the discovery of M108 had not been published, <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> independently rediscovered this object on April 17, 1789, and <a href="http://messier.obspm.fr/xtra/similar/herschel.html">cataloged it</a> as H V.46.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m108.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh-x_y_H2TiUz_ElY3K5o0UCi6jq30WevGEJqNDRBnXs-jwZ9E9yHLhhynAZ4j_q4w4Nej-W0idtDQtvZZ8oQJzBbYQ17a1QU2bnQIksrY4W8aOkr1mDxY_IDQJylCqlNW9wqHavAzRuYg/s1600/M108.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh-x_y_H2TiUz_ElY3K5o0UCi6jq30WevGEJqNDRBnXs-jwZ9E9yHLhhynAZ4j_q4w4Nej-W0idtDQtvZZ8oQJzBbYQ17a1QU2bnQIksrY4W8aOkr1mDxY_IDQJylCqlNW9wqHavAzRuYg/s1600/M108.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 108</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, também conhecida como </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 3556</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> situada perto da estrela </span><a href="http://pt.wikipedia.org/wiki/Beta_Ursae_Majoris" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Beta Ursae Majoris">Beta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ursa_Maior" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Ursa Maior">Ursa Maior</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, foi descoberta por </span><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 1781.</span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> foi descoberta por </span><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em 19 de fevereiro de 1781, três dias após a descoberta de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_97" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 97">Messier 97</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. O objeto chegou a ser considerado pelo astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> como a entrada "98" de seu </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Catálogo Messier">catálogo de objetos do céu profundo</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, mas não encontrou oportunidades de medir com precisão sua posição. Como a data limite de submissão de trabalhos no anuário astronômico francês </span><i style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Connaissance_des_temps" style="background: none; color: #0b0080; text-decoration: none;" title="Connaissance des temps">Connaissance des temps</a></i><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> estava chegando, não houve tempo hábil para incluí-lo na edição final de seu catálogo. </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="William Herschel">William Herschel</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, descobridor de </span><a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Urano (planeta)">Urano</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, redescobriu independentemente o objeto em 17 de abril de 1789.</span><span class="reference" id="cite_ref-seds_4-0" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_108#cite_note-seds-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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http://pt.wikipedia.org/wiki/Messier_108#mediaviewer/File:Messier_108_Hubble_WikiSky.jpg</div>
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<span class="mw-mmv-title" original-title="" style="max-width: 60%;">Messier 108 by Hubble Space Telescope</span></div>
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<span class="mw-mmv-source-author" original-title="" style="line-height: 1.8em;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://wikisky.org/snapshot?img_size=&img_res=&ra=11.191551317188468&de=55.67473365419516&angle=0.03708079237203604&projection=tan&rotation=-52.947086173101255&survey=astrophoto&img_id=905787&width=1340&height=1340&img_borders=0&interpolation=bicubic&jpeg_quality=0.8" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<span style="background-color: white; color: #0000ee; text-decoration: underline;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></div>
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<h1>
Messier 109</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M109 (NGC 3992)</i>, type SBc, in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a></center>
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<a href="http://messier.obspm.fr/Jpg/m109.jpg"><img align="right" alt="[m109.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m109.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">11 : 57.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+53 : 23 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">55000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">7x4 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.</div>
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NGC 3992 (Messier 109, M109) is one of the "Theta"-like barred spirals, which appears as a "hazy spot" situated just 40' SE of the mag 2.44 star Gamma Ursae Majoris (Phad, or Phecda).</div>
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This object was observed by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on March 12, 1781, and by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> on March 24, 1781, together with <a href="http://messier.obspm.fr/m/m108.html">M108</a> when he measured <a href="http://messier.obspm.fr/m/m097.html">M97</a>. Messier <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M109">listed the object</a> now called "M109" under number "99" in a preliminary manuscript version of his catalog without a position, and Méchain <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m109">mentioned it</a> in his letter to Bernoulli of May 6, 1783. But together with M108, it was not <a href="http://messier.obspm.fr/addition.html">added</a> to the "official" Messier catalog until 1953, by <a href="http://messier.obspm.fr/xtra/Bios/gingerich.html">Owen Gingerich</a>. <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> has found this galaxy independently on April 12, 1789, and <a href="http://messier.obspm.fr/xtra/similar/herschel.html">cataloged it</a> as H IV.61 (incorrectly misclassifying it as a planetary nebula).</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m109.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhWWX97Emsbb9Ai_3WM48rWSeGwBWf4z4OsojuWM5mDXFuB6JbM66vP1wg5ksRz8_vMBiZdWUdrIdFAUggffFVCVkUs4yEVKFYXDw2yKbHwRubZCKU3ZF_f7SYYIzMD1h4U1mI2lwl7rg0/s1600/M109.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhWWX97Emsbb9Ai_3WM48rWSeGwBWf4z4OsojuWM5mDXFuB6JbM66vP1wg5ksRz8_vMBiZdWUdrIdFAUggffFVCVkUs4yEVKFYXDw2yKbHwRubZCKU3ZF_f7SYYIzMD1h4U1mI2lwl7rg0/s1600/M109.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<b>Messier 109</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a>] 3992) é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral barrada">galáxia espiral barrada</a> localizada a cerca de cinquenta e cinco milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> (aproximadamente 16,86 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a>) de distância na direção da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Ursa_Maior" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação de Ursa Maior">constelação de Ursa Maior</a>. Possui aproximadamente cento e trinta mil anos-luz de <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a>, uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 9,8, uma declinação de +53º 23' 28" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 11 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 57 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 36,0s.</div>
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A galáxia NGC 3992 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/12_de_Mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="12 de Março">12 de Março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>.</div>
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<span style="line-height: 22.3999996185303px;">A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral_barrada" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia espiral barrada">galáxia espiral barrada</a><span style="line-height: 22.3999996185303px;"> foi descoberta por </span><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span style="line-height: 22.3999996185303px;"> em 19 de fevereiro de 1781, três semanas após a descoberta de</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_97" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 97">Messier 97</a><span style="line-height: 22.3999996185303px;">. O objeto chegou a ser considerado pelo astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="line-height: 22.3999996185303px;"> como a entrada "99" de seu</span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Catálogo Messier">catálogo de objetos do céu profundo</a><span style="line-height: 22.3999996185303px;">, mas não encontrou oportunidades de medir com precisão sua posição. Como a data limite de submissão de trabalhos no anuário astronômico francês </span><i style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Connaissance_des_temps" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Connaissance des temps">Connaissance des temps</a></i><span style="line-height: 22.3999996185303px;"> estava chegando, não houve tempo hábil para incluí-lo na edição final de seu catálogo.</span><span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_109#cite_note-seds-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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<span style="background-color: #f9f9f9; font-family: sans-serif; line-height: 13.5520000457764px;">Messier 109, projeto </span><a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none rgb(249, 249, 249); color: #0b0080; font-family: sans-serif; line-height: 13.5520000457764px; text-decoration: none;" title="2MASS">2MASS</a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background: none; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background: none; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background: none; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background: none; color: #0b0080; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" height="220" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br />
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>CARO LEITOR,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">devem requerer do Caro Leitor</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Visitando os Sites abaixo,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<b><o:p></o:p></b></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> - AS CONSTELAÇÕES - </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> entre o céu e a terra..., </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vagarosamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> e este por nossa mente sendo conscientizado.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<!-- Blogger automated replacement: "https://images-blogger-opensocial.googleusercontent.com/gadgets/proxy?url=http%3A%2F%2Ffreestarcharts.com%2Fimages%2FArticles%2FMessier%2FM102_Finder_Chart.jpg&container=blogger&gadget=a&rewriteMime=image%2F*" with "https://blogger.googleusercontent.com/img/proxy/AVvXsEi0cR_WPjkM_5bFNDEQAUD37gUUT_rgmPFO3zVRX3P-Z4eCoqYgEhdiwqONW1IT3O4NsJAwhVRT9xp8XWEN-oyeui8KCyATcrMPDSQTCPdivNnCEidxF8h09kkej-aZpQygKPgEqwJjxcqvLexiZT3Mz_zKHSmns7e_BLuK_FkcoSdJoRd5i58=" -->Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-56177898470785809502014-09-06T10:27:00.001-07:002015-04-05T09:26:37.144-07:00Triangulum<div class="MsoNormal" style="text-align: -webkit-center;">
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor, ao comentarmos um tantinho</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre o Objeto Messier 33, em Triangulum,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">estaremos também trazendo algumas palavras</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre o fato de que M33, a Galáxia Triangulum,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é nossa galáxia-irmã, quer dizer, pertencente ao chamado Grupo Local...</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe o chamado Grupo Local</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">formado por mais de 54 galáxias (incluindo as galáxias anãs)</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e onde reinam a Via Lactea e Andromeda, M31, e ainda a Galáxia Triangulum, M33.</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Neste nosso Grupo, </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">o centro gravitacional repousa em algum lugar entre Via Lactea e Andromeda</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(e, em algum dia do futuro bem distante, estaremos nos abraçando).</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">No entanto, vamos encontrar alguns alfarrábios</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">comentando sobre o fato da possibilidade</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">da Galáxia Triangulum ser (ou não ser)</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">uma galáxia satélite de Andromeda.</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(A galáxia-anã Pisces, satélite de Triangulum,</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">posiciona-se em equidistância entre Triangulum e Andromeda</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e, portanto, podendo ser considerada como pertencente a ambas</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> e atuando enquanto laço de união entre ambas).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Afirmam os alfarrábios,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">que a magnitude visual de Andromeda, M31, é 3.4</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(quer dizer, pode ser observada a olho nu</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">em céus escuros e transparentes e em noites de ausência de Lua</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- eu mesma já morei num Sítio de onde podia</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">observar Andromeda em visão enviesada, ou seja,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">através o rápido rasgo de visão).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Afirmam os alfarrábios,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">que a magnitude visual de Triangulum, M33, é 5.7</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(quer dizer, dificilmente pode ser observada a olho nu...</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">porém é sempre aconselhável poder se tentar - por que não? -</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e também recorrer a um bom par de binóculos</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ou mesmo a um simpático telescópio).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">De quaquer forma,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">é bom que saibamos que,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ao visualizarmos </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(seja a olho nu ou seja através alguma lente óptica)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">a Galáxia Andromeda, M31,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">estaremos também muito próximos </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">da boa visualização da Galáxia Triangulum, M33!</span></span></div>
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<span style="background-color: white; line-height: 18px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">E, após visualizarmos ou bem nos apercebermos</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">dos posicionamentos dessas nossas Galáxias-Irmãs,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ao norte - Andromeda e Triangulum -,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">sempre poderemos girar nossa cabeça</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e voltarmos nosso corpo para o sul, bem ao sul,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e observarmos, felizes e contentes e a olho nu</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(em lugares de céus escuros e transparentes e em noites sem Lua)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">as Galáxias também nossas Irmãs,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">as Nuvens Pequena e Grande de Magalhães</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- as constelações Hydrus e Tucana acolhendo a Pequena Nuvem</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e as constelações Dorado e Mons Mensa acolhendo a Grande Nuvem!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Sem dúvida alguma,</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">estaremos diante de</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">uma longa jornada</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> da Terra ao Céu e ao Infinito!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Com um abraço estrelado,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Janine Milward</span></span></div>
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<span style="color: #073763;"><span style="font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://www.hvezdnouoblohou.wz.cz/trojuhelnik.php">http://www.hvezdnouoblohou.wz.cz/trojuhelnik.php</a></span></span></span><br />
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The <b>Local Group</b> is the <a href="http://en.wikipedia.org/wiki/Galaxy_group" style="background-image: none; text-decoration: none;" title="Galaxy group">group</a> of <a href="http://en.wikipedia.org/wiki/Galaxy" style="background-image: none; text-decoration: none;" title="Galaxy">galaxies</a> that includes the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background-image: none; text-decoration: none;" title="Milky Way">Milky Way</a> among others. It comprises more than 54 galaxies, counting <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Dwarf_galaxies" style="background-image: none; text-decoration: none;" title="Dwarf galaxies">dwarf galaxies</a>. Its gravitational center is located somewhere between Milky Way and <a href="http://en.wikipedia.org/wiki/Andromeda_Galaxy" style="background-image: none; text-decoration: none;" title="Andromeda Galaxy">Andromeda Galaxy</a>. The Local Group covers a diameter of 10 <a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-image: none; text-decoration: none;" title="Light-year">megalight-years</a>(3.1 <a href="http://en.wikipedia.org/wiki/Parsec#Megaparsecs_and_gigaparsecs" style="background-image: none; text-decoration: none;" title="Parsec">megaparsecs</a>) (see <a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E%2B23_m" style="background-image: none; text-decoration: none;" title="1 E+23 m">1 E+23 m</a> for distance comparisons) and has a binary (dumbbell)<sup class="reference" id="cite_ref-Karachentsevetal2006_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-Karachentsevetal2006-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup> distribution. The group is estimated to have a total mass of 1.29±0.14 <span style="margin: 0px 0.15em 0px 0.25em;">×</span>10<sup style="line-height: 1em;">12</sup> <a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-image: none; text-decoration: none;" title="Solar mass">M<sub style="line-height: 1em;">☉</sub></a><sup class="reference" id="cite_ref-Karachentsevetal2006_1-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-Karachentsevetal2006-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup> and has a <a href="http://en.wikipedia.org/wiki/Velocity_dispersion" style="background-image: none; text-decoration: none;" title="Velocity dispersion">velocity dispersion</a> of 61±8 km/s.<sup class="reference" id="cite_ref-van_den_Bergh_1999_2-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-van_den_Bergh_1999-2" style="background-image: none; text-decoration: none; white-space: nowrap;">[2]</a></sup> The group itself is part of the <a href="http://en.wikipedia.org/wiki/Virgo_Supercluster" style="background-image: none; text-decoration: none;" title="Virgo Supercluster">Virgo Supercluster</a> (i.e. the Local Supercluster).<sup class="reference" id="cite_ref-tully1982_3-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-tully1982-3" style="background-image: none; text-decoration: none; white-space: nowrap;">[3]</a></sup></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The two most massive members of the group are Milky Way and Andromeda Galaxy. These two <a href="http://en.wikipedia.org/wiki/Spiral_galaxy" style="background-image: none; text-decoration: none;" title="Spiral galaxy">spiral galaxies</a> each have a system of satellite galaxies.</span></span></div>
<ul style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; line-height: 1.5em; list-style-image: initial; list-style-position: initial; margin: 0.5em 0px; padding: 0px 2.5em;">
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Milky Way's <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Milky_Way%27s_satellite_galaxies" style="background-image: none; text-decoration: none;" title="Milky Way's satellite galaxies">satellite system</a> consists of <a href="http://en.wikipedia.org/wiki/Sagittarius_Dwarf_Elliptical_Galaxy" style="background-image: none; text-decoration: none;" title="Sagittarius Dwarf Elliptical Galaxy">Sagittarius Dwarf Galaxy</a>, <a href="http://en.wikipedia.org/wiki/Large_Magellanic_Cloud" style="background-image: none; text-decoration: none;" title="Large Magellanic Cloud">Large Magellanic Cloud</a>, <a href="http://en.wikipedia.org/wiki/Small_Magellanic_Cloud" style="background-image: none; text-decoration: none;" title="Small Magellanic Cloud">Small Magellanic Cloud</a>, <a href="http://en.wikipedia.org/wiki/Canis_Major_Dwarf_Galaxy" style="background-image: none; text-decoration: none;" title="Canis Major Dwarf Galaxy">Canis Major Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Ursa_Minor_Dwarf" style="background-image: none; text-decoration: none;" title="Ursa Minor Dwarf">Ursa Minor Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Draco_Dwarf" style="background-image: none; text-decoration: none;" title="Draco Dwarf">Draco Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Carina_Dwarf" style="background-image: none; text-decoration: none;" title="Carina Dwarf">Carina Dwarf</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Sextans_Dwarf" style="background-image: none; text-decoration: none;" title="Sextans Dwarf">Sextans Dwarf</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Sculptor_Dwarf" style="background-image: none; text-decoration: none;" title="Sculptor Dwarf">Sculptor Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Fornax_Dwarf" style="background-image: none; text-decoration: none;" title="Fornax Dwarf">Fornax Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)" style="background-image: none; text-decoration: none;" title="Leo I (dwarf galaxy)">Leo I</a>, <a href="http://en.wikipedia.org/wiki/Leo_II_(dwarf_galaxy)" style="background-image: none; text-decoration: none;" title="Leo II (dwarf galaxy)">Leo II</a>, and <a href="http://en.wikipedia.org/wiki/Ursa_Major_I_Dwarf" style="background-image: none; text-decoration: none;" title="Ursa Major I Dwarf">Ursa Major I Dwarf</a> and <a href="http://en.wikipedia.org/wiki/Ursa_Major_II_Dwarf" style="background-image: none; text-decoration: none;" title="Ursa Major II Dwarf">Ursa Major II Dwarf</a>.</span></span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Andromeda's <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Andromeda%27s_satellite_galaxies" style="background-image: none; text-decoration: none;" title="Andromeda's satellite galaxies">satellite system</a> consists of <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Elliptical_Galaxy_M32" style="background-image: none; text-decoration: none;" title="Elliptical Galaxy M32">M32</a>, <a href="http://en.wikipedia.org/wiki/Messier_110" style="background-image: none; text-decoration: none;" title="Messier 110">M110</a>, <a href="http://en.wikipedia.org/wiki/NGC_147" style="background-image: none; text-decoration: none;" title="NGC 147">NGC 147</a>, <a href="http://en.wikipedia.org/wiki/NGC_185" style="background-image: none; text-decoration: none;" title="NGC 185">NGC 185</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_I" style="background-image: none; text-decoration: none;" title="Andromeda I">And I</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_II" style="background-image: none; text-decoration: none;" title="Andromeda II">And II</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_III" style="background-image: none; text-decoration: none;" title="Andromeda III">And III</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_IV" style="background-image: none; text-decoration: none;" title="Andromeda IV">And IV</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_V" style="background-image: none; text-decoration: none;" title="Andromeda V">And V</a>, <a href="http://en.wikipedia.org/wiki/Pegasus_Dwarf_Spheroidal_Galaxy" style="background-image: none; text-decoration: none;" title="Pegasus Dwarf Spheroidal Galaxy">Pegasus dSph (aka And VI)</a>,<a href="http://en.wikipedia.org/wiki/Cassiopeia_Dwarf" style="background-image: none; text-decoration: none;" title="Cassiopeia Dwarf">Cassiopeia Dwarf (aka And VII)</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_VIII" style="background-image: none; text-decoration: none;" title="Andromeda VIII">And VIII</a>, <a href="http://en.wikipedia.org/wiki/Andromeda_IX" style="background-image: none; text-decoration: none;" title="Andromeda IX">And IX</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Dwarf_Spheroidal_Galaxy_Andromeda_X" style="background-image: none; text-decoration: none;" title="Dwarf Spheroidal Galaxy Andromeda X">And X</a>, And XI, And XII, And XIII, And XIV, And XV, And XVI, And XVII, And XVIII, And XIX, and And XX.</span></span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The <a href="http://en.wikipedia.org/wiki/Triangulum_Galaxy" style="background-image: none; text-decoration: none;" title="Triangulum Galaxy">Triangulum Galaxy</a>, the third largest and only unbarred <a href="http://en.wikipedia.org/wiki/Spiral_galaxy" style="background-image: none; text-decoration: none;" title="Spiral galaxy">spiral galaxy</a> in the Local Group, may or may not be a companion to the Andromeda Galaxy. <a href="http://en.wikipedia.org/wiki/Pisces_Dwarf" style="background-image: none; text-decoration: none;" title="Pisces Dwarf">Pisces Dwarf</a> is equidistant from the Andromeda Galaxy and the Triangulum Galaxy, so it may be a satellite of either.<sup class="reference" id="cite_ref-apj562_2_4-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Local_Group#cite_note-apj562_2-4" style="background-image: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The membership of <a href="http://en.wikipedia.org/wiki/NGC_3109" style="background-image: none; text-decoration: none;" title="NGC 3109">NGC 3109</a>, with its companions <a href="http://en.wikipedia.org/wiki/Sextans_A" style="background-image: none; text-decoration: none;" title="Sextans A">Sextans A</a> and the <a href="http://en.wikipedia.org/wiki/Antlia_Dwarf" style="background-image: none; text-decoration: none;" title="Antlia Dwarf">Antlia Dwarf</a>, is uncertain due to extreme distances from the center of the Local Group.</span></span></li>
<li style="border: none; margin: 0px 0px 0.1em; padding: 0.25em 0px; text-align: center;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The other members of the group are gravitationally secluded from these large subgroups: <a href="http://en.wikipedia.org/wiki/IC_10" style="background-image: none; text-decoration: none;" title="IC 10">IC 10</a>, <a href="http://en.wikipedia.org/wiki/IC_1613" style="background-image: none; text-decoration: none;" title="IC 1613">IC 1613</a>, <a href="http://en.wikipedia.org/wiki/Phoenix_Dwarf" style="background-image: none; text-decoration: none;" title="Phoenix Dwarf">Phoenix Dwarf</a>, <a href="http://en.wikipedia.org/wiki/Leo_A" style="background-image: none; text-decoration: none;" title="Leo A">Leo A</a>, <a href="http://en.wikipedia.org/wiki/Tucana_Dwarf" style="background-image: none; text-decoration: none;" title="Tucana Dwarf">Tucana Dwarf</a>,<a href="http://en.wikipedia.org/wiki/Cetus_Dwarf" style="background-image: none; text-decoration: none;" title="Cetus Dwarf">Cetus Dwarf</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/PegDIG" style="background-image: none; text-decoration: none;" title="PegDIG">Pegasus Dwarf Irregular</a>, <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Wolf-Lundmark-Melotte" style="background-image: none; text-decoration: none;" title="Wolf-Lundmark-Melotte">Wolf-Lundmark-Melotte</a>, <a href="http://en.wikipedia.org/wiki/Aquarius_Dwarf" style="background-image: none; text-decoration: none;" title="Aquarius Dwarf">Aquarius Dwarf</a>, and <a class="mw-redirect" href="http://en.wikipedia.org/wiki/SagDIG" style="background-image: none; text-decoration: none;" title="SagDIG">Sagittarius Dwarf Irregular</a>.</span></span></li>
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<a href="http://en.wikipedia.org/wiki/Local_Group" style="background-color: white; font-family: Arial, Helvetica, sans-serif; text-align: center; text-decoration: none;">http://en.wikipedia.org/wiki/Local_Group</a></div>
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<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a> foi o primeiro a identificar o Grupo Local, no capítulo VI do seu livro <i>The Realm of Nebulae</i> (Hubble 1936, págs. 124-151). Ele descreve "<i>um típico e pequeno grupo de nebulosas o qual está isolado no campo geral</i>". No livro, ele descreve <b>por luminosidade decrescente, e os membros são <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M31" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M31">M31</a>, a <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M33" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M33">M33</a>, a <a href="http://pt.wikipedia.org/wiki/Grande_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grande Nuvem de Magalhães">Grande Nuvem de Magalhães</a>, a<a href="http://pt.wikipedia.org/wiki/Pequena_Nuvem_de_Magalh%C3%A3es" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pequena Nuvem de Magalhães">Pequena Nuvem de Magalhães</a></b>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M32" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M32">M32</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_205" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 205">NGC 205</a>, <a href="http://pt.wikipedia.org/wiki/NGC_6822" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6822">NGC 6822</a>, <a href="http://pt.wikipedia.org/wiki/NGC_185" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 185">NGC 185</a>, <a href="http://pt.wikipedia.org/wiki/IC_1613" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="IC 1613">IC 1613</a> e <a href="http://pt.wikipedia.org/wiki/NGC_147" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 147">NGC 147</a>. Ele também identifica <a href="http://pt.wikipedia.org/wiki/IC_10" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="IC 10">IC 10</a> como um possível membro do Grupo Local. No anos 70, desde o trabalho dele, o número de membros conhecidos no Grupo Local tem aumentado de 12 para 36, em 2003. Este foi de modo, quase duas dúzias de galáxias de baixa luminosidade.<span class="reference" id="cite_ref-Bergh2003_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_Local#cite_note-Bergh2003-3" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
<h2 style="background: none rgb(255, 255, 255); border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-bottom-width: 1px; font-family: 'Linux Libertine', Georgia, Times, serif; font-weight: normal; line-height: 1.3; margin: 1em 0px 0.25em; overflow: hidden; padding: 0px;">
<span class="mw-headline" id="Gal.C3.A1xias_componentes">Galáxias componentes</span></h2>
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<span class="mw-headline" id="Mapa">Mapa</span></h4>
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<map id="ImageMap_1_848498325" name="ImageMap_1_848498325" style="margin-left: auto; margin-right: auto;"></map><img alt="" class="thumbimage" data-file-height="480" data-file-width="640" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/fe/Local_Group.svg/640px-Local_Group.svg.png" height="480" style="border: 1px solid rgb(204, 204, 204); margin-left: auto; margin-right: auto; vertical-align: middle;" usemap="#ImageMap_1_848498325" width="640" /><br />
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<a href="http://pt.wikipedia.org/wiki/Ficheiro:Local_Group.svg" style="background: none; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;" title="Sobre esta imagem"><img alt="Sobre esta imagem" src="http://bits.wikimedia.org/static-1.25wmf2/extensions/ImageMap/desc-20.png" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" /></a></div>
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Grupo Local (mapa clicável)</div>
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<span class="mw-headline" id="Gal.C3.A1xias_membros">Galáxias membros</span></h4>
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<tr><th colspan="4" style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">Galáxias Espirais</a></th></tr>
<tr><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">nome</th><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">tipo</th><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">constelação</th><th style="background-color: #f2f2f2; border: 1px solid rgb(170, 170, 170); padding: 0.2em; text-align: center;">notas</th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">Galáxia de Andrômeda</a> (M31, NGC 224)</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SA(s)b</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Andrômeda">Andrômeda</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Maior membro do grupo, recentemente (2006) descobriu-se que também é uma espiral barrada. Pode ser menos massiva que a Via Láctea.</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SBbc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">nenhuma</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Segunda maior, contudo, a possível galáxia mais massiva do Grupo Local.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_Local#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_598" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 598">Galáxia do Triângulo</a> (M33, NGC 598)</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SAc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Triangulum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Triangulum">Triangulum</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">a única galáxia espiral não barrada e possível satélite da galáxia de Andrômeda.</td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;">A listagem continua</span></div>
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LEIA MAIS</div>
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em</div>
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http://pt.wikipedia.org/wiki/Grupo_Local</div>
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............................................<span style="font-family: Arial, Helvetica, sans-serif;"> M33, A Galáxia Triangulum</span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">É uma das únicas três </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de galáxias, as outras sendo </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Contudo, é significativamente menor comparada as suas companheiras espirais, embora seja maior do que a média das galáxias espirais do </span><a href="http://pt.wikipedia.org/wiki/Universo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Universo">Universo</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. É provável que tenha uma</span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_Pisces" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia anã Pisces">galáxia anã Pisces</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, embora também seja provável que a própria galáxia de Triângulo esteja ligada </span><a href="http://pt.wikipedia.org/wiki/Gravidade" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Gravidade">gravitacionalmente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a Andrômeda.</span><span class="reference" id="cite_ref-seds_6-2" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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<img src="http://www.galex.caltech.edu/media/images/glx2009-01f_img02.jpg" height="640" width="640" /></div>
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http://www.galex.caltech.edu/media/images/glx2009-01f_img02.jpg</div>
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<div style="background-color: white; font-family: Arial, Helvetica, Verdana, sans-serif; text-align: start;">
NASA's Galaxy Evolution Explorer Mission celebrates its sixth anniversary studying galaxies beyond our Milky Way through its sensitive ultraviolet telescope, the only such far-ultraviolet detector in space.</div>
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The mission studies the shape, brightness, size and distance of distant galaxies across 10 billion years of cosmic history, giving scientists a wealth of data to help us better understand the origins of the universe. One such object is pictured here, the galaxy NGC598, more commonly known as M33.</div>
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The image shows a map of the recent star formation history of M33. The bright blue and white areas are where star formation has been extremely active over the past few million years. The patches of yellow and gold are regions where star formation was more active 100 million years ago.</div>
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In addition, the ultraviolet image shows the most massive young stars in M33. These stars burn their large supply of hydrogen fuel quickly, burning hot and bright while emitting most of their energy at ultraviolet wavelengths. Compared with low-mass stars like our sun, which live for billions of years, these massive stars never reach old age, having a lifespan as short as a few million years.</div>
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Credit: NASA/JPL-Caltech</div>
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<span style="font-family: Arial, Helvetica, Verdana, sans-serif;"><i>http://www.galex.caltech.edu/media/glx2009-01f_img02.html</i></span></div>
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<span style="background-color: white;"><span style="color: #073763;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></div>
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<span style="background-color: white; color: #660000;"><b><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span><span style="font-family: Arial, sans-serif;">TRIANGULUM, O TRIÂNGULO</span></b></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; line-height: 22px;"><span style="background-color: white; color: #073763;">Ascensão Reta 1h29m / 2h48m Declinação +25<sup>o</sup>.4 / +37<sup>o</sup>.0<o:p></o:p></span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Mito:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">O Triângulo foi colocado no céu por Júpiter, a pedido de Ceres que gostaria de ver o formato da Ilha da Sicília representado entre as estrelas.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Esta constelação pode ser bem identificada situando-se entre as estrelas Gamma Andromedae, Alamak, e Alpha Arietis, Hamal.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Fronteiras:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">A constelação do Triangulum faz fronteira com Andrômeda, Pisces, Áries e Perseus.<o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-size: small;">http://www.ipac.caltech.edu/2mass/gallery/m33atlas.jpg</span></h1>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a></div>
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Messier 33</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M33 (NGC 598)</i>, type Sc, in <a href="http://messier.obspm.fr/map/Tri.html">Triangulum</a><b><span style="font-size: large;">Triangulum Galaxy</span></b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m33.jpg"><img align="right" alt="[m33.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m33.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">01 : 33.9 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+30 : 39 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">3000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">73x45 (arc min)</td></tr>
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Probably discovered by Hodierna before 1654.</div>
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Independently discovered by Charles Messier 1764.</div>
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The Triangulum Galaxy Messier 33 (M33, NGC 598) is another prominent member of the <a href="http://messier.obspm.fr/more/local.html">Local Group</a> of galaxies. This galaxy is small compared to its big apparent neighbor, the <a href="http://messier.obspm.fr/m/m031.html">Andromeda galaxy M31</a>, and to our <a href="http://messier.obspm.fr/more/mw.html">Milky Way galaxy</a>, but by this more of average size for spiral galaxies in the universe. One of the small Local Group member galaxies, LGS 3, is possibly a satellite of M33, which itself may be a remote but gravitationally bound companion of the <a href="http://messier.obspm.fr/m/m031.html">Andromeda galaxy M31</a>.</div>
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M33 is approaching us (our Solar System) at 182 km/s according to R. Brent Tully, or at 179 +/-3 km/s according to <a href="http://messier.obspm.fr/xtra/supp/m_NED.html#m33">NED</a>. Corrected for our motion around the Milky Way's Galactic Center, it is approaching our Galaxy at 24 km/sec.</div>
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M33 was probably first found by <a href="http://messier.obspm.fr/xtra/similar/hodierna.html">Hodierna</a> before 1654 (perhaps together with open cluster <a href="http://messier.obspm.fr/xtra/ngc/n0752.html">NGC 752</a>). It was independently rediscovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M33">cataloged by him</a> on August 25, 1764. Nevertheless, <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a>, who otherwise carefully avoided to number Messier's objects in his survey, <a href="http://messier.obspm.fr/xtra/similar/herschel.html">assigned it</a> the number H V.17, on the ground of an observation dated September 11, 1784. Also because of the cataloging of Herschel, the brightest and largest HII region (diffuse emission nebula containing ionized hydrogen) has obtained a NGC number of its own: <a href="http://messier.obspm.fr/more/m033_n604.html">NGC 604</a> (William Herschel's H III.150); it is situated in the northeastern part of the galaxy; apparently the bright knot near the top of our image. This is one of the largest H II regions known at all: it has a diameter of nearly 1500 light-years, and a spectrum similar to the Orion nebula <a href="http://messier.obspm.fr/m/m042.html">M42</a>. Hui Yang (University of Illinois) and Jeff J. Hester (Arizona State University) have taken a <a href="http://messier.obspm.fr/more/m033_n604.html">photograph of NGC 604 with the Hubble Space Tepescope</a>, resolving over 200 young hot massive stars (of 15 to 60 solar masses) which have recently formed here.</div>
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LEIA MAIS</div>
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http://messier.obspm.fr/m/m033.html</div>
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http://www.nasa.gov/mission_pages/galex/galexC-20090428.html</div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;">In these side-by-side images of M33, the ultraviolet image on the left was taken by the Galaxy Evolution Explorer, while the ultraviolet and infrared image on the right is a blend of the mission's M33 image and another taken by NASA's Spitzer Space Telescope. M33, one of our closest galactic neighbors, is about 2.9 million light-years away in the constellation Triangulum, part of what's known as our Local Group of galaxies. </span><br style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;" /><br style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 18px; text-align: left;">Image credit: NASA/JPL-Caltech </span></span></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 598 = M33 Galáxia Pinwheel</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 01h32m Declinação +30<sup>o</sup>.33<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Tipo S - Galáxia Espiral Magnitude fotográfica aparente 6,19 <o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Dimensões Angulares 61 X 42 Distância (milhões de anos-luz) 2,4<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">Pinwheel Galaxy, com um diâmetro igual ao da Lua. </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;"> Não é fácil de ser observada devido ao seu brilho pouco intenso. </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">A partir do núcleo brilhante e pequeno, </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">dois grandes e principais braços espiralados </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">e alguns outros braços auxiliares são observados. </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">Através grandes telescópios, podemos observar </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">que os braços consistem de nuvens de estrelas</span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">e outros objetos como estrelas variáveis, aglomerados abertos e globulares, </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">nebulosas, etc. </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">A distância é de 2.4 milhões de anos-luz </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">e o diâmetro é de cerca de 60 mil anos-luz </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">e sua luminosidade total é igual a 300 milhões de nosso Sol. </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;"> Como o Triângulo é vizinho à Andrômeda, </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">M33 situa-se próximo às estrelas Alpha do Triangulo e Beta de Andrômeda </span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #073763;">e esta Galáxia distancia-se da Galáxia de Andrômeda cerca de 570 mil anos-luz.</span></span><span style="background-color: #073763; color: black; font-size: 11pt;"><o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;">PIA11970: M33: A Close Neighbor Reveals its True Size and Splendor</b><span style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"> </span></div>
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One of our closest galactic neighbors shows its awesome beauty in this new image from NASA's Spitzer Space Telescope. M33, also known as the Triangulum Galaxy, is a member of what's known as our Local Group of galaxies. Along with our own Milky Way, this group travels together in the universe, as they are gravitationally bound. In fact, M33 is one of the few galaxies that is moving toward the Milky Way despite the fact that space itself is expanding, causing most galaxies in the universe to grow farther and farther apart.</div>
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M33 is located about 2.9 million light-years away in the constellation Triangulum. This composite image was taken by Spitzer's infrared array camera. The color blue indicates infrared light of 3.6 microns, green shows 4.5-micron light, and red 8.0 microns.</div>
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<dt style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; text-align: start;"><b>Image Credit:</b></dt>
<dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; text-align: start;">NASA/JPL-Caltech</dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; text-align: start;"><br /></dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; text-align: start;">LEIA MAIS</dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; text-align: start;">em</dd><dd style="background-color: white; text-align: start;"><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;">http://photojournal.jpl.nasa.gov/catalog/PIA11970</span></dd><dd style="background-color: white; text-align: start;"><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><br /></span></dd><dd style="background-color: white; text-align: start;"><span style="color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif;"><br /></span></dd><dd style="background-color: white; color: #4b5c68; font-family: Helvetica, Arial, Verdana, sans-serif; text-align: start;"><div style="text-align: center;">
<img src="http://photojournal.jpl.nasa.gov/jpeg/PIA11969.jpg" height="416" width="640" /></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">galáxia do Triângulo</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (Messier 33, </span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="New General Catalogue">NGC 598</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> localizada a cerca de três milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Tri%C3%A2ngulo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação do Triângulo">constelação do Triângulo</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Possui entre 40 a 60 mil anos-luz de </span><a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Diâmetro">diâmetro</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de 5,5. Foi descoberta antes de 1654 por </span><a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span></div>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> foi descoberta por <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de 1654, juntamente com o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> <a href="http://pt.wikipedia.org/wiki/NGC_752" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 752">NGC 752</a>. Foi redescoberta independentemente pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que o <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogou</a> em 25 de agosto de 1764.<a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, que usualmente não catalogava objetos já catalogados por Messier, catalogou a galáxia como a entrada H V.17 de seu catálogo durante uma observação em 11 de setembro de 1784. <span class="reference" id="cite_ref-seds_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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Pode ser vista a <a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> sob excelentes condições: é o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_do_c%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Objeto do céu profundo">objeto do céu profundo</a> mais distante a ser visto sem o auxílio de instrumentos ópticos. É razoavelmente observado em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>, embora todo o seu brilho esteja distribuído em uma área quatro vezes maior do que a <a href="http://pt.wikipedia.org/wiki/Lua_cheia" style="background: none; color: #0b0080; text-decoration: none;" title="Lua cheia">lua cheia</a>, deixando sua superfície extremamente pouco brilhante. Portanto, é praticamente impossível visualizar a galáxia em <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> que não permitam baixa magnificação. É um dos alvos preferidos para a<a href="http://pt.wikipedia.org/wiki/Astronomia_amadora" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia amadora">astronomia amadora</a> e para os <a href="http://pt.wikipedia.org/wiki/Astrofotografia" style="background: none; color: #0b0080; text-decoration: none;" title="Astrofotografia">astrofotógrafos</a> amadores, pois é possível visualizar seus braços espirais e nebulosas brilhantes sem a utilização de equipamentos caros.<span class="reference" id="cite_ref-seds_6-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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É uma das únicas três <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a> do <a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background: none; color: #0b0080; text-decoration: none;" title="Grupo Local">Grupo Local</a> de galáxias, as outras sendo <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a> e a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>. Contudo, é significativamente menor comparada as suas companheiras espirais, embora seja maior do que a média das galáxias espirais do <a href="http://pt.wikipedia.org/wiki/Universo" style="background: none; color: #0b0080; text-decoration: none;" title="Universo">Universo</a>. É provável que tenha uma<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a>, a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_Pisces" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia anã Pisces">galáxia anã Pisces</a>, embora também seja provável que a própria galáxia de Triângulo esteja ligada <a href="http://pt.wikipedia.org/wiki/Gravidade" style="background: none; color: #0b0080; text-decoration: none;" title="Gravidade">gravitacionalmente</a> a Andrômeda.<span class="reference" id="cite_ref-seds_6-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
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Está se aproximando radialmente do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> a uma velocidade de 182 km/s. Descontando a velocidade orbital do <a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a> em torno da Via-Láctea, Triângulo está se aproximando de nossa galáxia a 24 km/s.<br />
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<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="" style="font-weight: normal;"><span style="font-family: Times New Roman; font-size: small;">Galáxia do Triângulo</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M33HunterWilson09.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; margin-left: auto; margin-right: auto;"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="" data-file-height="850" data-file-width="850" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/2f/M33HunterWilson09.jpg/280px-M33HunterWilson09.jpg" height="280" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2f/M33HunterWilson09.jpg/420px-M33HunterWilson09.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2f/M33HunterWilson09.jpg/560px-M33HunterWilson09.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></span></a></div>
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<small><span style="font-family: Times New Roman; font-size: small;">Galáxia do Triângulo</span></small></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Dados observacionais (J2000)</span></span></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Constelação"><span style="color: black; font-family: Times New Roman; font-size: small;">Constelação</span></a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Triangulum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Triangulum"><span style="color: black; font-family: Times New Roman; font-size: small;">Triangulum</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Tipo</span></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">SA(s)cd<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ascensão reta"><span style="color: black; font-family: Times New Roman; font-size: small;">Asc. reta</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">01<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 33<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 50,02<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-SIMBAD-M33_2-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Declinação"><span style="color: black; font-family: Times New Roman; font-size: small;">Declinação</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">+30° 39′ 36,7″<span class="reference" id="cite_ref-SIMBAD-M33_2-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Distância</span></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">2,38-3,07 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ano-luz">anos-luz</a><br />(730-940 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Parsec">kpc</a>)<span class="reference" id="cite_ref-aass06_3-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-aass06-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">3</a></span> <span class="reference" id="cite_ref-apj696_4-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-apj696-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">4</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Desvio para o vermelho"><span style="color: black; font-family: Times New Roman; font-size: small;">Redshift</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">-0,000607 ± 0,000010<span class="reference" id="cite_ref-SIMBAD-M33_2-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Magnitude aparente"><span style="color: black; font-family: Times New Roman; font-size: small;">Magnit. apar.</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">5,72<span class="reference" id="cite_ref-SIMBAD-M33_2-3" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Dimensões</span></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">70,8 × 41,7 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-SIMBAD-M33_2-4" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-SIMBAD-M33-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Características físicas</span></span></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Massa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Massa"><span style="color: black; font-family: Times New Roman; font-size: small;">Massa</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">5 × 10<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">10</span><span class="reference" id="cite_ref-mnras342_1_5-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-mnras342_1-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">5</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Outras denominações</span></span></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><span style="font-family: Times New Roman; font-size: small;">Messier 33, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="New General Catalogue">NGC</a> 0598, MCG +05-04-069, 1ES 0131+303, RX J0133.8+3039, PGC 005818.<span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Mapa</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Galáxia do Triângulo"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Galáxia do Triângulo" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Triangulum_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Triangulum constellation map.png" data-file-height="1419" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/ae/Triangulum_constellation_map.png/240px-Triangulum_constellation_map.png" height="190" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/ae/Triangulum_constellation_map.png/360px-Triangulum_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/ae/Triangulum_constellation_map.png/480px-Triangulum_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></span></a></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Foi umas das primeiras galáxias espirais a ser identificada como tal, segundo </span><a href="http://pt.wikipedia.org/wiki/William_Parsons" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="William Parsons">William Parsons</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Também foi umas das primeiras galáxias, por definição, reconhecidas; </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, com base na distância estimada com o auxílio de variáveis </span><a href="http://pt.wikipedia.org/wiki/Cefeida" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Cefeida">cefeidas</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, concluiu que Triângulo era um sistema estelar extragaláctico, publicando seus resultados em 1926. <b>Vários outros objetos brilhantes da galáxia ganharam suas próprias entradas no catálogo NGC: NGC 588, 592, 595 e 603, bem como no </b></span><i style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Index_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="Index Catalogue"><b>Index Catalogue</b></a></i><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><b>, IC 131, 132, 133, 134, 135, 136, 137, 139, 140, 142 e 143</b>, todas visíveis em </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> amadores com aberturas de 12,5 polegadas ou mais.</span><span class="reference" id="cite_ref-seds_6-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">................................. M33, A Galáxia Triangulum</span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Está se aproximando radialmente do </span><a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Sistema Solar">Sistema Solar</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a uma velocidade de 182 km/s. Descontando a velocidade orbital do </span><a href="http://pt.wikipedia.org/wiki/Sol" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Sol">Sol</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em torno da Via-Láctea, Triângulo está se aproximando de nossa galáxia a 24 km/s.<b> Sua maior e mais brilhante </b></span><b><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Região HII">região HII</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (uma </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nebulosa_difusa" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Nebulosa difusa">nebulosa difusa</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> contendo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Hidrogênio">hidrogênio</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> ionizado) obteve seu próprio número </span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="New General Catalogue">NGC</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">,</span><a href="http://pt.wikipedia.org/wiki/NGC_604" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="NGC 604">NGC 604</a></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. É uma das maiores regiões HII conhecidas, tendo um diâmetro de 1 500 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e apresenta </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Linha_espectral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Linha espectral">linhas espectrais</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> semelhantes às encontradas na </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Nebulosa de Órion">nebulosa de Órion</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (M42).</span><span class="reference" id="cite_ref-seds_6-3" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Nursery of New Stars - GPN-2000-000972</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">NASA, Hui Yang University of Illinois ODNursery of New Stars</span> - <span class="mw-mmv-source"><a class="external text" href="http://dayton.hq.nasa.gov/IMAGES/LARGE/GPN-2000-000972.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Great Images in NASA</a> <a class="external text" href="http://grin.hq.nasa.gov/ABSTRACTS/GPN-2000-000972.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Description</a></span></span></div>
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<span style="background-color: #fbfbfb; color: #555555; font-size: 16px; line-height: 24px;">This is a Hubble Space Telescope image (right) of a vast nebula called NGC 604, which lies in the neighboring spiral galaxy M33, located 2.7 million light-years away in the constellation Triangulum. This is a site where new stars are being born in a spiral arm of the galaxy. Though such nebulae are common in galaxies, this one is particularly large, nearly 1,500 light-years across. The nebula is so vast it is easily seen in ground-based telescopic images (left). At the heart of NGC 604 are over 200 hot stars, much more massive than our Sun (15 to 60 solar masses). They heat the gaseous walls of the nebula making the gas fluoresce. Their light also highlights the nebula's three-dimensional shape, like a lantern in a cavern. By studying the physical structure of a giant nebula, astronomers may determine how clusters of massive stars affect the evolution of the interstellar medium of the galaxy. The nebula also yields clues to its star formation history and will improve understanding of the starburst process when a galaxy undergoes a "firestorm" of star formation. The image was taken on January 17, 1995 with Hubble's Wide Field and Planetary Camera 2. Separate exposures were taken in different colors of light to study the physical properties of the hot gas (17,000 degrees Fahrenheit, 10,000 degrees Kelvin</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 19px; line-height: 24px; max-width: 60%;"><span style="color: #333333; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#mediaviewer/File:Interstellar.cloud.arp.750pix.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Interstellar.cloud.arp.750pix</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Autor e informação sobre a fonte" style="font-size: 0.8em;"><span class="mw-mmv-author">Hui Yang (University of Illinois) and NASA/ESA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/html/opo9627a.html" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/html/opo9627a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/original/opo9627a.jpg" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">direct link</a>) <a class="external free" href="http://hubblesite.org/newscenter/archive/releases/1996/27/image/a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/1996/27/image/a/</a></span></span></div>
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Uma das maiores <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background: none; color: #0b0080; text-decoration: none;" title="Região HII">regiões HII</a> (imagem obtida do <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_Palomar" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório Palomar">Observatório Palomar</a>) encontra-se em Triângulo</div>
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The nebula cataloged as <a class="extiw" href="http://en.wikipedia.org/wiki/NGC_604" style="background: none; color: #0b0080; text-decoration: none;" title="en:NGC 604">NGC 604</a> is a giant star forming region, 1500 light years across, in the nearby spiral galaxy, <a class="extiw" href="http://en.wikipedia.org/wiki/Triangulum_Galaxy" style="background: none; color: #0b0080; text-decoration: none;" title="en:Triangulum Galaxy">M33</a>. Over 200 newly formed, hot, massive, stars are scattered within a cavern-like, gaseous, interstellar cloud. The stars irradiate the gas with energetic ultraviolet light stripping electrons from atoms and exciting them — producing a characteristic nebular glow.</div>
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<b>NGC 604</b> é uma <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> de grandes dimensões, com uma extensão de aproximadamente 1500 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. Essa nebulosa se encontra a cerca de 3 milhões de anos-luz da<a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> na direção da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Tri%C3%A2ngulo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação do Triângulo">constelação do Triângulo</a>, próxima à borda da <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M33" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M33">M33</a>.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/NGC_604#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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A nebulosa NGC 604 apresenta belas cores e intensa atividade de <a href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Formação estelar">formação estelar</a>, sendo que muitos detalhes importantes da estrutura da nebulosa foram obtidos pelo<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a> em Agosto de <a href="http://pt.wikipedia.org/wiki/1996" style="background: none; color: #0b0080; text-decoration: none;" title="1996">1996</a> e ajudaram a esclarecer muitos pontos referentes à formação de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> e à evolução do <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background: none; color: #0b0080; text-decoration: none;" title="Meio interestelar">meio interestelar</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/NGC_604</span></span></div>
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...................................... <b><span style="font-family: Arial, Helvetica, sans-serif;">M33, A Galáxia Triangulum</span></b></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">É uma das únicas três </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia espiral">galáxias espirais</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de galáxias, as outras sendo </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia de Andrômeda">Andrômeda</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Contudo, é significativamente menor comparada as suas companheiras espirais, embora seja maior do que a média das galáxias espirais do </span><a href="http://pt.wikipedia.org/wiki/Universo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Universo">Universo</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. <b>É provável que tenha uma</b></span><b><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_Pisces" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia anã Pisces">galáxia anã Pisces</a></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, embora também seja provável que a própria galáxia de Triângulo esteja ligada </span><a href="http://pt.wikipedia.org/wiki/Gravidade" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Gravidade">gravitacionalmente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a Andrômeda.</span><span class="reference" id="cite_ref-seds_6-2" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo#cite_note-seds-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a>................................</span></div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">A galáxia anã </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Pisces</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é um pequena </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia irregular">galáxia irregular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e parte do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. <b>É a possível </b></span><b><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia satélite">galáxia satélite</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> da </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Tri%C3%A2ngulo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia do Triângulo">Galáxia do Triângulo</a></b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><b> (M33)</b>. Na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de</span><a href="http://pt.wikipedia.org/wiki/Pisces" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Pisces">Pisces</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, a </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia">galáxia</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é chamada de </span><i style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Pisces</i><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> ou, para diferenciá-la de outros objetos astronômicos de nome similar, </span><i style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Pisces anã</i><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. De acordo com os o deslocamento de suas linhas espectrais, calcula-se que esta galáxia esteja se aproximando da </span><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Via Láctea">Via Láctea</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> com uma velocidade de 287 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Km/s" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Km/s">km/s</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Seu tipo morfológico está classificado alternativamente entre </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_esferoidal" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia anã esferoidal">esferoidal anã</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular_an%C3%A3" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia irregular anã">irregular anã</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, e isto é muito raro, só há duas galáxias conhecidas desse tipo.</span></div>
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<table border="0" cellpadding="3" class="infobox_v2" style="background: rgb(249, 249, 249); border: 1px solid rgb(170, 170, 170); clear: right; color: black; font-family: sans-serif; font-size: 12px; line-height: 1.1em; margin: 0px 0px 0.5em 1em; padding: 2px; width: 20em;"><tbody>
<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="">Pisces</span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:LGS_3_ubv.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; margin-left: auto; margin-right: auto; text-decoration: none;"><img alt="" data-file-height="651" data-file-width="601" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/02/LGS_3_ubv.jpg/280px-LGS_3_ubv.jpg" height="303" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/02/LGS_3_ubv.jpg/420px-LGS_3_ubv.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/02/LGS_3_ubv.jpg/560px-LGS_3_ubv.jpg 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></a></div>
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<small>Uma imagem da galáxia anã Pisces.</small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top">Karachentseva</td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1976" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1976">1976</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pisces" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pisces">Pisces</a></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">dIrr/dSph</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 03<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 55.0<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">+21° 53′ 06″</td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">2.51 ± 0.08 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>(769 ± 25 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">-287 ± 0 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Km/s" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Km/s">km/s</a></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">14.2</td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">2' × 2'</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top">LGS 3, PGC 3792.</td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Pisces_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Pisces constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Pisces_constellation_map.png/240px-Pisces_constellation_map.png" height="240" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Pisces_constellation_map.png/360px-Pisces_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Pisces_constellation_map.png/480px-Pisces_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></b><br />
<b><span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">a ir percebendo que existe mais, bem mais, </span></b><br />
<b><span style="font-family: Arial, Helvetica, sans-serif;">entre o céu e a terra...; </span></b><br />
<b><span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, vagarosamente, </span></b><br />
<b><span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">e sendo por nossa mente conscientizado. </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-32855546567218913932014-09-06T10:26:00.001-07:002015-06-14T11:14:35.101-07:00Taurus<div class="MsoNormal" style="text-align: -webkit-center;">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando a Lua visita a constelação do Touro,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">primeiramente cumprimenta M45, as Pleiades</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que se situam no ombro taurino),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, no dia seguinte, cumprimenta as Hyades</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> e Aldebaran, estrela-alpha Tauri,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Olho Iluminado;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">finalmente, já no terceiro dia, </span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">conclui sua passagem nesta constelação</span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ao cumprimentar M1, a Nebulosa do Caranguejo,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem próxima ao Chifre voltado para o sul!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Hoje a madrugada estará nos apresentando </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a Lua tornando-se Minguante</span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e visitando ....</span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(ao terceiro dia de passagem pela constelação do Touro)</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">...................</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Uma estrela que certa dia explodiu, </span></span></div>
<div style="color: black; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: medium; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">tornando-se uma chamada supernova,</span></span></div>
<div style="color: black; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: medium; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">e que, com o passar do tempo, tornou-se uma nuvem...;</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"><span style="color: #073763;">nuvem penetrada por lentes ópticas </span></span></div>
<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span><br />
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">comandadas por olhares penetrantes e estudiosos...; </span></span></div>
<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span><span style="font-family: Arial, Helvetica, sans-serif;"></span></span><br />
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">nuvem que foi revelando, descobrindo, não mais cobrindo,</span></span></div>
<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">seus segredos de vida (quase) infinita, </span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">vida que sempre encontra </span><span style="font-family: Arial, Helvetica, sans-serif;">uma nova maneira de ser, </span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">vida que se transforma em nova vida,</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">através um novo coração, um pulsar, uma estrela de nêutrons, uma nova estrela<b>!</b></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Tempo e Espaço atuando através a eterna continuidade da Vida.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Nesta Postagem, Caro Leitor,</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">encontre alguma informação</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">sobre nossa visita</span></span></div>
<div style="color: black; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: medium; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">a M1 e M45,</span></span></div>
<div style="color: black; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: medium; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">os famosos Objetos Messier na constelação do Touro.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><br /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Com um abraço estrelado,</span></span></div>
<div style="color: black; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: medium; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Janine Milward</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - Cartas Celestes, As Constelações - CARJ</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">TAURUS, O TOURO</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 3h20m / 5h58m Declinação +0<sup>o</sup>.1 / +30<sup>o</sup>.9<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Mito:</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Júpiter ansiava por encontrar-se com Europa. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Certa vez, disfarçou-se em touro e fez parte de uma manada </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">até encontrar-se com a moça, numa praia. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Europa sentiu-se encorajada com a placidez do touro</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> e montou-o </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e foi quando Júpiter correu para o mar </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e levou a moça até a ilha de Creta. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">De acordo com outro mito, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">o touro representa Io </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">a quem Júpiter transformou em vaca, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para despistar o ciúme e a vigilância de Juno, sua mulher.<o:p></o:p></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh272MEMVAAo9uKUeMdqZkWnqKvHASI8BWpvWwMQ_1CbzjEfHgFnbne9UsqjievMXCI-WNgZnD5XjpNM2mIIqplwS_Gm6y1ZRI7MFZk2n96WyhwsyIBBjcboEy6cO37OSdvOSKin4vwXf8/s1600/K1.8Zeus.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh272MEMVAAo9uKUeMdqZkWnqKvHASI8BWpvWwMQ_1CbzjEfHgFnbne9UsqjievMXCI-WNgZnD5XjpNM2mIIqplwS_Gm6y1ZRI7MFZk2n96WyhwsyIBBjcboEy6cO37OSdvOSKin4vwXf8/s1600/K1.8Zeus.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.theoi.com/Gallery/K1.8.html</span></div>
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<span style="color: #274e13;">K1.8 EUROPA & THE BULL</span></div>
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<span style="color: #274e13;"><span class="details">Museum Collection:</span> Kunst-historiches Museum, Vienna, Austria </span></div>
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<span style="color: #274e13;"><span class="details">Museum Catalogue No.:</span> TBA </span><span class="details" style="color: #274e13;">Beazley Archive No.:</span><span style="color: #274e13;"> N/A </span></div>
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<span style="color: #274e13;"><span class="details">Ware:</span> Apulian Red Figure </span><span class="details" style="color: #274e13;">Shape:</span><span style="color: #274e13;"> Kylix </span></div>
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<span style="color: #274e13;"><span class="details">Painter:</span> -- </span><span class="details" style="color: #274e13;">Date:</span><span style="color: #274e13;"> ca 330 - 320 BC </span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span class="details">Period:</span> Late Classical</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Algumas Informações Interessantes acerca esta Constelação:</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A mais antiga de todas as constelações e talvez a primeira a ser delimitada pelos babilônios, que a utilizaram para marcar o início do ano, pois o equinócio da primavera, há 4000 AC, localizava-se neste asterismo. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> Aliás, o estudo de todos os antigos zodíacos mostram o seu início no Touro: o ano começava com o aparecer matinal das Pleiades na primavera, e o inverno, com o seu aparecimento vespertino no outono. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O aparecimento das Pleiades em novembro era saudado como a festa dos mortos, que comemoramos até hoje. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Povos da antiguidade, como os caldeus e hebreus, davam ao mês de novembro o nome de Pleiades.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No mais antigo de todos os zodíacos egípcios - o de Denderah -, a constelação do Touro está associada a Osíris, que era o deus especial do Nilo.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O nascer helíaco das Hyades, principal aglomerado do Touro, era associado à estação da chuva - donde a origem do seu nome, que significava ‘chover’.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Taurus situa-se entre as constelações de Gemini, Auriga, Perseus, Áries, Cetus, Eridanus e Orion<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M1 E M45,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO TAURUS:</b></span></div>
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Messier 45</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M45 </i>, type 'c', in <a href="http://messier.obspm.fr/map/Tau.html">Taurus</a></center>
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<br /><b><span style="font-size: large;">Pleiades</span></b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m45.jpg"><img align="right" alt="[m45.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m45.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">03 : 47.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+24 : 07 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">0.44 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">1.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">110.0 (arc min)</td></tr>
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Known pre-historically. Mentioned by Homer about 750 B.C., by biblical Amos about 750 B.C., and by Hesiod about 700 B.C.</div>
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The Pleiades, also known as Messier 45 (M45), are among those objects which are known since the earliest times. At least 6 member stars are visible to the naked eye, while under moderate conditions this number increases to 9, and under clear dark skies jumps up to more than a dozen (Vehrenberg, in his <i>Atlas of Deep Sky Splendors</i>, mentions that in 1579, well before the invention of the telescope, astronomer Moestlin has correctly drawn 11 Pleiades stars, while Kepler quotes observations of up to 14).</div>
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According to Kenneth Glyn Jones, the earliest known references to this cluster are mentionings by <a href="http://messier.obspm.fr/xtra/Bios/homer.html">Homer</a> in his <i>Ilias</i> (about 750 B.C.) and his <i>Odyssey</i> (about 720 B.C.), and by <a href="http://messier.obspm.fr/xtra/Bios/hesiod.html">Hesiod</a>, about 700 B.C.. According to Burnham, they were seen in connection to the agricultural seasons of that time. Also, and the Bible has three references to the Pleiades (the Hebrew "Kiymah"): Job 9:7-9, Job 38:31-33, and Amos 5:8; the prophet Amos is believed to have given his message in 750 B.C. or 749 B.C., while there is no consent on the dating of the book of Job: Some believe it was written about 1,000 B.C. (the regency of Kings David and Solomon in old Israel) or earlier (Moses, about 13th to 16th century B.C.), others give reasons that it may have been created as late as the 3rd to 5th century B.C.. The present author [hf] does not know if the cluster is mentioned in one of the earlier Assyrian or Sumerian sources.</div>
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The Pleiades also carry the name "Seven Sisters"; according to Greek mythology, seven daughters and their parents. Their Japanese name is "Subaru", which was taken to christen the car of same name. The Persian name is "Soraya", after which the former Iranian empress was named. Old European (e.g., English and German) names indicate they were once compared to a "Hen with Chicks". Other cultures tell <a href="http://messier.obspm.fr/more/m045_lore.html">more and other lore</a> of this naked-eye star cluster. Ancient Greek astronomers Eudoxus of Knidos (c. 403-350 BC) and Aratos of Phainomena (c. 270 BC) listed them as an own constellation: <i>The Clusterers</i>. This is also referred to by <a href="http://messier.obspm.fr/xtra/Bios/smyth.html">Admiral Smyth</a> in his <a href="http://messier.obspm.fr/m-ref.html#smyth"><i>Bedford Catalog</i></a>.</div>
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Burnham points out that the name "Pleiades" may be derived from either the Greek word for "to sail", or the word "pleios" meaning "full" or "many". The present author prefers the view that the name may be derived from the mythological mother, Pleione, which is also the name of one of the brighter stars.</div>
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On March 4, 1769, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included the Pleiades as <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M45">No. 45</a> in his first list of nebulae and star clusters, published 1771</div>
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The Pleiades nebulae are blue-colored, which indicates that they are <i>reflection nebulae</i>, reflecting the light of the bright stars situated near (or within) them.</div>
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The cluster is a great object in binoculars and rich-field telescopes, showing more than 100 stars in a field about 1 1/5 degrees in diameter. In telescopes, it is frequently even too large to be seen in one lowest magnification field of view.</div>
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As the Pleiades are situated close to the ecliptic (4 degrees off), occultations of the cluster by the Moon occur quite frequently: .........................Also, planets come close to the Pleiades cluster (Venus, Mars, and Mercury even occasionally pass through) to give a conspicuous spectacle.</div>
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As mentioned in the description for the <a href="http://messier.obspm.fr/m/m042.html">Orion Nebula M42</a>, it is a bit unusual that Messier added the Pleiades (together with the Orion Nebula M42/<a href="http://messier.obspm.fr/m/m043.html">M43</a> and the <a href="http://messier.obspm.fr/m/m044.html">Praesepe cluster M44</a>) to his catalog, and will perhaps <a href="http://messier.obspm.fr/m-q&a.html#why_M42-45">stay subject to speculation</a>.</div>
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LEIA MAIS, MUITO MAIS</div>
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em</div>
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<a href="http://messier.obspm.fr/m/m045.html">http://messier.obspm.fr/m/m045.html</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> Mario Jaci Monteiro - Cartas Celestes, As Constelações (excerto) - CARJ</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Pleiades - M45</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância: cerca de 350 anos-luz.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aglomerado de mais de 400 estrelas</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> em uma área de um grau de diâmetro</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> e facilmente visível a olho nu.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As Pleiades ou Atlântidas eram as sete filhas de Atlas e Pleione, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">seis das quais podem ser vistas a olho nu e uma invisível ou “perdida”. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Elas eram as companheiras virgens de Diana </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e foram levadas para o céu </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para escaparem do Gigante Orion que as importunava. </span></div>
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<span style="font-size: 12px; line-height: 16.7999992370605px; margin: 0px; padding: 0px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/potw1347a/</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><strong style="margin: 0px; padding: 0px;">Credit: </strong><span style="line-height: 1.4em;">ESO/B. Tafreshi (</span><a href="http://www.twanight.org/tafreshi" style="background-image: url(http://www.eso.org/public/archives/app/i/ext_link2.e3e6349c34f8.gif); background-position: 0% 50%; background-repeat: no-repeat; color: #274e13; line-height: 1.4em; margin: 0px; padding-bottom: 0px; padding-left: 12px !important; padding-right: 0px; padding-top: 0px; text-decoration: none;">twanight.org</a><span style="line-height: 1.4em;">)</span></span></div>
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<span style="line-height: 19.2000007629395px; text-align: start;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Babak Tafreshi, one of the ESO Photo Ambassadors, has captured the antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) in an enthralling image combining the beauty of the southern sky with the amazing dimensions of the biggest astronomical project in the world.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Thousands of stars are revealed to the naked eye in the clear skies over the Chajnantor Plateau. Its dry and transparent night sky is one of the reasons ALMA has been built here. Surprisingly bright in the upper left corner of the picture, there is a tightly packed bunch of young stars, the Pleiades Cluster, which was already known to most ancient civilisations. The constellation of Orion (The Hunter) is clearly visible over the closest of the antennas — the hunter’s belt is formed by the three blue stars just to the left of the red light. According to classic mythology, Orion was a hunter who chased the Pleiades, the beautiful daughters of Atlas. When seen through the thin atmosphere over the Atacama, it almost seems that this epic hunt is really happening.</span></div>
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<b style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 16.7999992370605px;">http://www.eso.org/public/images/potw1347a/</b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Minha humilde tradução literal </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para o texto explicativo acima acerca esta belíssima imagem</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> realizada por Babak Tafreshi)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Milhares de estrelas nos são apresentadas a olho nu nos céus límpidos do Plateau Chajnantor. O céu noturno seco e transparente é uma das razões pelas quais ALMA foi ali construído. Surpreendentemente iluminado no canto esquerdo ao alto da foto encontra-se um aglomerado de estrelas jovens bem compactadas, o Aglomerado das Pleiades (que também era conhecido nas antigas civilizações). A constelação de Orion (O Caçador) é claramente visível e bem próximo às antenas - o Cinturão do Caçador sendo formado peles três estrelas azuladas bem à esquerda da luz vermelha. De acordo com a mitologia clássica, Orion era um caçador que buscava alcançar as Pleiades, as belas filhas de Atlas. Quando visto através a atmosfera delicada do Atacama, nos parece que esse épico de caçada está realmente acontecendo.</span><br />
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; text-align: -webkit-left;">Atlas holding the sky. 7201: Atlante sostiene la volta celeste 2C AD. Collezione Farnese. National Archaeological Museum, Naples. </span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.maicar.com/GML/Atlas.html" style="color: #274e13; text-decoration: none;">http://www.maicar.com/GML/Atlas.html</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">De acordo com outro mito, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">as Pleiades foram para o céu por causa de suas tristezas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> com o destino de seu pai, Atlas, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que carregava o mundo nas costas.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><img src="http://www.observatorio.ufmg.br/pleiades.JPG" height="528" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">http://www.observatorio.ufmg.br/dicas10.htm</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os nomes das Irmãs que Choram e de seus pais são:<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Alcyone, Maia, Electra, Merope, Taygette, Celaeno e Sterope,<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>com a adição dos pais, Atlas e Pleione.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Plêiade que se perdeu parece ser Merope, que casou-se com um mortal, Sisyplus, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e por isso escondeu-se</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> por ser a única filha que não foi casada com um deus. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Outro mito diz que foi Electra quem desapareceu</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> em função de sua dor pela destruição de Ilium, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">que foi fundada por seu filho Dardanos.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>As Pleiades formam um aglomerado, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>com Alcyone como estrela principal, situado no ombro do Touro.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj9TT2-UmAWX7jLh4jc5_I7REIPcqjvcBj2HaJBDEiPTF3BvQPnOtF-njYNpVxlQ9iYlDEXRLv_7geSilKS_rg4CtKmC_opS7NP6OIEMJVlYY5lZNPc1V16m2xSBPaXyZj4sAXoMIZvenQ/s1600/m45_colombari_960.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEj9TT2-UmAWX7jLh4jc5_I7REIPcqjvcBj2HaJBDEiPTF3BvQPnOtF-njYNpVxlQ9iYlDEXRLv_7geSilKS_rg4CtKmC_opS7NP6OIEMJVlYY5lZNPc1V16m2xSBPaXyZj4sAXoMIZvenQ/s1600/m45_colombari_960.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<cite style="font-style: normal; line-height: 17px; text-align: start;" title="apod.nasa.gov"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/ap130918.html">http://apod.nasa.gov/apod/ap130918.html</a></span></cite></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><cite style="font-style: normal; line-height: 17px; text-align: start;" title="apod.nasa.gov">apod.nasa.gov</cite><br style="line-height: 17px; text-align: start;" /><span style="line-height: 17px; text-align: start;">Astronomy</span><span style="line-height: 17px; text-align: start;"> Picture of the </span><span style="line-height: 17px; text-align: start;">Day</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">M45: The Pleiades Star Cluster </span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Credit & Copyright: <a href="mailto:%20roberto.colombari%20at%20techedgegroup%20dot%20com">Roberto Colombari</a></span></div>
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<span style="line-height: 17px; text-align: start;"><span style="background-color: white; color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap130918.html</span></span></div>
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<span style="background-color: white;"><b style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">Explanation: </b><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;">Have you ever seen the Pleiades star cluster? Even if you have, you probably have never seen it as dusty as this. Perhaps the most famous star cluster on the sky, the bright stars of the </span><a href="http://www.seds.org/messier/m/m045.html" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">Pleiades</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> can be seen without binoculars from even the depths of a </span><a href="http://antwrp.gsfc.nasa.gov/apod/image/0208/earthlights02_dmsp_big.jpg" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">light-polluted city</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;">. With a long exposure from a dark location, though, the dust cloud surrounding the </span><a href="http://apod.nasa.gov/apod/ap091205.html" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">Pleiades</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> star </span><a href="http://asterisk.apod.com/viewtopic.php?f=24&t=18009" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">cluster</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> becomes very evident. The </span><a href="http://www.astrobin.com/55798/" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">above exposure</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> took about 20 minutes and covers a sky area several times the size of the full moon. Also known as the </span><a href="http://www.ras.ucalgary.ca/~gibson/pleiades/pleiades_myth.html" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">Seven Sisters</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> and </span><a href="http://apod.nasa.gov/apod/ap960423.html" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">M45</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;">, </span><a href="http://en.wikipedia.org/wiki/Pleiades_%28star_cluster%29" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">the Pleiades</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> lies about 400 light years away toward the constellation of the Bull (</span><a href="http://en.wikipedia.org/wiki/Taurus_%28constellation%29" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">Taurus</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;">). A </span><a href="http://arxiv.org/ftp/arxiv/papers/0810/0810.1592.pdf" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">common legend</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> with a </span><a href="http://kencroswell.com/GD50.html" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">modern twist</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> is that one of the brighter stars faded since the cluster was named, leaving only six stars visible to the unaided eye. The actual number of </span><a href="http://www.youtube.com/watch?v=p6prI0Zfw80" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">Pleiades</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> stars visible, however, may be more or less than seven, depending on the </span><a href="http://apod.nasa.gov/apod/ap010827.html" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">darkness</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> of the surrounding sky and the </span><a href="http://en.wikipedia.org/wiki/File:Snellen_chart.svg" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">clarity</a><span style="color: black; font-family: 'Times New Roman'; font-size: xx-small; line-height: normal; text-align: start;"> of the observer's eyesight.</span></span></div>
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IMPERDÍVEL! Belíssimas imagens!</div>
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acesse</div>
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<span style="background-color: white;"><b style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">APOD Retrospective: </b><span style="color: black; font-family: 'Times New Roman'; font-size: small; line-height: normal;"></span><a href="http://asterisk.apod.com/viewtopic.php?&t=25327" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal;">The Pleiades Star Cluster</a><span style="color: black; font-family: 'Times New Roman'; font-size: small; line-height: normal;"> </span></span></div>
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<b><span style="color: #660000;">As Plêiades (<a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Catálogo Messier">Messier 45</a>)</span></b><span style="color: #252525;"> são um grupo de estrelas na constelação do </span><a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">Touro</a><span style="color: #252525;">. As Plêiades, também chamadas de </span><i style="color: #252525;">aglomerado estelar</i><span style="color: #252525;"> (ou </span><i style="color: #252525;">aglomerado aberto</i><span style="color: #252525;">) </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">M45</a><span style="color: #252525;"> são facilmente visíveis a olho nu nos dois hemisférios e consistem de várias </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a><span style="color: #252525;"> brilhantes e quentes, de </span><a href="http://pt.wikipedia.org/wiki/Espectro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Espectro">espectro</a><span style="color: #252525;"> predominantemente azul. As Plêiades tem vários</span><a href="http://pt.wikipedia.org/wiki/Pl%C3%AAiades_no_folclore_e_literatura" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Plêiades no folclore e literatura">significados em diferentes culturas e tradições</a><span style="color: #252525;">.</span></div>
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O cluster é dominado por <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação estelar">estrelas azuis</a> quentes, que se formaram nos últimos 100 milhões de anos. Há uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_reflex%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de reflexão">nebulosa de reflexão</a> formada por poeira em torno das estrelas mais brilhantes que acreditava-se a princípio ter sido formado pelos restos da formação do cluster (por isto receberam o nome alternativo de <b>Nebulosa Maia</b>, da estrela<a href="http://pt.wikipedia.org/wiki/Maia_(estrela)" style="background: none; color: #0b0080; text-decoration: none;" title="Maia (estrela)">Maia</a>), mas hoje sabe-se que se trata de uma nuvem de poeira não relacionada ao aglomerado, no <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background: none; color: #0b0080; text-decoration: none;" title="Meio interestelar">meio interestelar</a> que as estrelas estão atravessando atualmente. Os astrônomos estimam que o cluster irá sobreviver por mais 250 milhões de anos, depois dos quais será dispersado devido a interações gravitacionais com a vizinhança galática.</div>
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<span class="mw-headline" id="Visualiza.C3.A7.C3.A3o"><span style="font-size: small;">Visualização</span></span></h2>
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É um excelente objeto para a visualização, desde os mais simples <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> até os maiores <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>, mostrando mais de 100 estrelas em um diâmetro aparente de cerca de 72 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minuto de arco</a>. Contém inúmeras estrelas duplas ou múltiplas. A <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nebulosa_de_M%C3%A9rope" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de Mérope">nebulosa de Mérope</a>, em torno da estrela <a class="new" href="http://pt.wikipedia.org/w/index.php?title=M%C3%A9rope_(estrela)&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Mérope (estrela) (página não existe)">Mérope</a>, pode ser vista com <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores de 4 polegadas de abertura em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> de excelente qualidade.</div>
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<span style="color: #073763;">LEIA MAIS</span><br />
<span style="color: #073763;">em</span><br />
<a href="http://pt.wikipedia.org/wiki/Pl%C3%AAiades" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Pl%C3%AAiades</a><br />
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/4/4e/Pleiades_large.jpg</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2004/20/image/a/" rel="nofollow" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2004/20/image/a/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">NASA, ESA, AURA/Caltech, Palomar Observatory<br /><span style="height: 0px; line-height: 1; position: relative; top: 0.5ex; vertical-align: baseline;">The science team consists of: D. Soderblom and E. Nelan (STScI), F. Benedict and B. Arthur (U. Texas), and B. Jones (Lick Obs.)</span></span></td></tr>
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http://www.ipac.caltech.edu/2mass/gallery/crabatlas.jpg</div>
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http://www.ipac.caltech.edu/2mass/gallery/messiercat.html</div>
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<a href="https://www.blogger.com/null" name="m81" style="text-align: -webkit-center;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 1</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Supernova Remnant</a> M1 (NGC 1952)</i> in <a href="http://messier.obspm.fr/map/Tau.html">Taurus</a></center>
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<br /><b><span style="font-size: large;">Crab Nebula</span></b><br /><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m1.jpg"><img align="right" alt="[m1.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m1.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">05 : 34.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+22 : 01 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">6.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">6x4 (arc min)</td></tr>
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Discovered 1731 by British amateur astronomer John Bevis.</div>
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The Crab Nebula, Messier 1 (M1, NGC 1952), is the most famous and conspicuous known supernova remnant, the expanding cloud of gas created in the explosion of a star as supernova which was observed in the year 1054 AD. It shines as a nebula of magnitude 8.4 near the southern "horn" of Taurus, the Bull.</div>
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<a href="http://messier.obspm.fr/more/m001_sn.html">The supernova</a> was noted on July 4, 1054 A.D. by Chinese astronomers as a new or "guest star," and was about four times brighter than Venus, or about mag -6. According to the records, it was visible in daylight for 23 days, and 653 days to the naked eye in the night sky. It was probably also recorded by Anasazi Indian artists (in present-day Arizona and New Mexico), as findings in Navaho Canyon and White Mesa (both Arizona) as well as in the Chaco Canyon National Park (New Mexico) indicate; there's a review of the research on the <a href="http://www.astronomy.pomona.edu/archeo/outside/chaco/nebula.html">Chaco Canyon Anasazi art online</a>. In addition, Ralph R. Robbins of the University of Texas has found Mimbres Indian art from New Mexico, possibly depicting the supernova.</div>
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The Supernova 1054 was also assigned the variable star designation CM Tauri. It is one of few <a href="http://messier.obspm.fr/more/mw_sn.html">historically observed supernovae</a> in our <a href="http://messier.obspm.fr/more/mw.html">Milky Way Galaxy</a>.</div>
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The nebulous remnant was discovered by <a href="http://messier.obspm.fr/xtra/Bios/bevis.html">John Bevis</a> in 1731, who <a href="http://messier.obspm.fr/more/m001_bevis.html">added it</a> to his sky atlas, <i>Uranographia Britannica</i>. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> independently <a href="http://messier.obspm.fr/xtra/history/m-m001.html">found it</a> on August 28, 1758, when he was looking for comet Halley on its first predicted return, and first thought it was a comet. Of course, he soon recognized that it had no apparent proper motion, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M1">cataloged it</a> on September 12, 1758. It was the discovery of this object which caused Charles Messier to begin with the compilation of <a href="http://messier.obspm.fr/xtra/history/m-cat.html">his catalog</a>. It was also the discovery of this object, which closely resembled a comet (1758 De la Nux, C/1758 K1) in his small refracting telescope, which brought him to the idea to search for comets with telescopes (see his<a href="http://messier.obspm.fr/xtra/history/notes-c.html#1801note">note</a>). Messier acknowledged the prior, original discovery by Bevis when he learned of it in a letter of June 10, 1771.</div>
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Although Messier's catalog was primarily compiled for preventing confusion of these objects with comets, M1 was again confused with comet Halley on the occasion of that comet's second predicted return in 1835.</div>
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This nebula was christened the "Crab Nebula" on the ground of a <a href="http://messier.obspm.fr/more/m001_rosse.html">drawing made by Lord Rosse</a> about 1844. Of the early observers, Messier, Bode and William Herschel correctly remarked that this nebula is not resolvable into stars, but William Herschel thought that it was a stellar system which should be resolvable by larger telescopes. John Herschel and Lord Rosse erroneously thought it is "barely resolvable" into stars. </div>
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LEIA MAIS</div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NEBULOSA DO CARANGUEJO, M1, NGC 1952!</b></span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">NGC 1952 - M 1 - Taurus - Nebulosa Resto de Supernova - Caranguejo<o:p></o:p></span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h33m Declinação +22<sup>o</sup>.05<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária SN Dimensão 5,0 Magnitude 19<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 16V Distância em anos-luz 4,0<o:p></o:p></span></div>
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<span style="color: #274e13;"><span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Por volta do ano 5500 antes de cristo, uma imensa estrela explodiu como Supernova... seis mil e quinhentos anos mais tarde, em 4 de julho de 1054, astrônomos japoneses e chineses puderam observar a aparição de uma 'estrela convidada" no céu na constelação que hoje denominamos de Touro. Essa nova estrela, tão brilhante quanto Vênus, pôde ser vista durante o dia por cerca de 23 dias e durante dois anos pôde ser observada e estudada no céu noturno.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando a supernova esmaeceu, passaram-se mais 700 anos até que uma pequena nuvem de gás verde luminoso surgiu no lugar onde ela aparecera anteriormente, um grau ao norte e oeste de Zeta Tauri, já em um dos chifres do Touro quase aos pés dos Gêmeos.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Por volta do ano 5500 antes de cristo, uma imensa estrela explodiu como Supernova... seis mil e quinhentos anos mais tarde, em 4 de julho de 1054, astrônomos japoneses e chineses puderam observar a aparição de uma 'estrela convidada" no céu na constelação que hoje denominamos de Touro. Essa nova estrela, tão brilhante quanto Vênus, pôde ser vista durante o dia por cerca de 23 dias e durante dois anos pôde ser observada e estudada no céu noturno.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando a supernova esmaeceu, passaram-se mais 700 anos até que uma pequena nuvem de gás verde luminoso surgiu no lugar aonde ela aparecera anteriormente, um grau ao norte e oeste de Zeta Tauri, já em um dos chifres do Touro quase aos pés dos Gêmeos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Charles Messier (1730-1817) era um caçador de cometas e sempre vasculhava o céu em busca dos mesmos. Em 12 de setembro de 1758 (ou em 28 de Agosto, segundo outro documento - Nota da Tradutora), Messier apontou para esse ponto de luz difusa no céu e o descreveu a nebulosa como contendo nenhuma estrela, esbranquiçada em sua cor e alongada como a chama de uma vela. Mais tarde, Messier veio a saber que tal nebulosa já havia sido avistada por um astrônomo inglês, John Bevis, em 1731.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Messier continuou sua busca por cometas (naquele mesmo houve o retorno, já previsto, do Cometa Halley durante o mês de dezembro) - e passou então, a elaborar uma lista de objetos no céu que não eram cometas. Finalmente, uma versão final dessa lista foi publicada em 1784 contendo 109 ou 110 objetos, sendo que o primeiro objeto mencionado foi a Nebulosa que ora é visitada por Saturno. Essa lista é hoje conhecida como A Lista de Messier e seus objetos são denominados M1, M2, M3.... A Nebulosa do Caranguejo é M1.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, esse nome, Nebulosa do Caranguejo foi dado por Earl of Rosse, em 1840 que publicou um desenho da mesma com filamentos que sugeriam o formato de um caranguejo. Mais tarde, ele observou a nebulosa já com outra aparelhagem mais potente e rejeitou sua descrição anterior da mesma.... tarde demais: a Nebulosa do Caranguejo já era assim conhecida!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Nebulosa do Caranguejo não é difícil de ser localizada com um telescópio mais simples e do quintal de sua casa - afinal foi assim que Messier a encontrou! Porém, em céus mais transparentes, longe das luzes da cidade, sua visão se torna bem mais enriquecida e se você tiver um telescópio possante, será fantástico poder observar um estrela que ainda permanece em seu centro, um pulsar que gira cerca de 30 vezes por segundo!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">"<b>A Nebulosa do Caranguejo</b>" é uma re-leitura, síntese e tradução de Janine Milward de artigo extraído da Revista Astronomy em sua edição de novembro na seção "Southern Sky Show" - "The Starry Sky".</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhaeIkWiYP4O0wJVkcgjnNj0vL_szdT48B3q9i6d5oIe6DcxwylxobImTBgZAq8M99Rv71F_Mjn9sv6opBWbmzd-CM2pJ9Bbj3q2OabepB-PerZ8MDwRQJpJofuYiB_sKZxvE4dJAqnYyE/s1600/m1_hst_900.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhaeIkWiYP4O0wJVkcgjnNj0vL_szdT48B3q9i6d5oIe6DcxwylxobImTBgZAq8M99Rv71F_Mjn9sv6opBWbmzd-CM2pJ9Bbj3q2OabepB-PerZ8MDwRQJpJofuYiB_sKZxvE4dJAqnYyE/s1600/m1_hst_900.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap111225.html</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>M1: The Crab Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a>, <a href="http://hubble.esa.int/" style="color: #274e13; text-decoration: none;">ESA</a>, J. Hester, A. Loll (<a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;">ASU</a>); Acknowledgement: Davide De Martin (<a href="http://www.skyfactory.org/" style="color: #274e13; text-decoration: none;">Skyfactory</a>)</span></div>
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<b><span style="color: #660000; font-size: small;">A Nebulosa do Caranguejo (também catalogado como <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo Messier">Messier</a> 1, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC</a> 1952, Taurus A)</span></b><span style="color: #252525;"> é um <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente de supernova</a> e uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_vento_de_pulsar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de vento de pulsar">nebulosa de vento de pulsar</a> na<a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> do <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">Touro</a>. A nebulosa foi primeiramente observada por <a href="http://pt.wikipedia.org/wiki/John_Bevis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Bevis">John Bevis</a> em 1731 e corresponde a uma brilhante <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Supernova">supernova</a> (<a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">SN 1054</a>) registrada por astrônomos chineses e árabes em 1054. A nebulosa é a mais intensa fonte de <a href="http://pt.wikipedia.org/wiki/Raios_X" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raios X">raios X</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raios_gama" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raios gama">gama</a> para energias acima de 30 <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron-volt" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elétron-volt">KeV</a>, com fluxo de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Energia_luminosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Energia luminosa">energia luminosa</a> acima de 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">12</span> eV. Dista a cerca de 6 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (2 quilo<a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da Terra e tem um diâmetro de 11 anos-luz (3,4 parsecs), expandindo-se a uma taxa de aproximadamente 1 500 quilômetros por segundo.</span></div>
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No centro da nebulosa há o <a href="http://pt.wikipedia.org/wiki/Pulsar_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pulsar do Caranguejo">Pulsar do Caranguejo</a>, uma <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> com 28 a 30 quilômetros de diâmetro,<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> que emite pulsos periódicos de radiação que abrange quase todo o <a href="http://pt.wikipedia.org/wiki/Espectro_eletromagn%C3%A9tico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Espectro eletromagnético">espectro eletromagnético</a>, com uma <a href="http://pt.wikipedia.org/wiki/Frequ%C3%AAncia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Frequência">frequência</a> de 30,2 vezes por segundo, evidenciando uma rotação com período de apenas 33 milissegundos. Foi o primeiro objeto astronômico associado a uma explosão de supernova.</div>
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Age como uma fonte de radiação para o estudo de <a href="http://pt.wikipedia.org/wiki/Corpo_celeste" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Corpo celeste">corpos celestes</a> que por vezes a <a href="http://pt.wikipedia.org/wiki/Oculta%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ocultação">ocultam</a>. Na década de 1950 e 1960, a <a href="http://pt.wikipedia.org/wiki/Coroa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Coroa solar">coroa solar</a> foi mapeada a partir de observações das ondas de rádio da nebulosa que passaram através dela. Em 2003, a espessura da atmosfera de <a href="http://pt.wikipedia.org/wiki/Tit%C3%A3_(sat%C3%A9lite)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Titã (satélite)">Titã</a>, satélite de <a href="http://pt.wikipedia.org/wiki/Saturno_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Saturno (planeta)">Saturno</a>, foi medida através do bloqueio de raios-X provenientes da nebulosa pela atmosfera do satélite.</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo</a></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/c9/Chandra-crab.jpg/800px-Chandra-crab.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><span style="font-family: Arial, Helvetica, sans-serif;"><br />http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#mediaviewer/Ficheiro:Chandra-crab.jpg</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Chandra-crab</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Chandra-crab.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">Optical: NASA/HST/ASU/J. Hester et al. X-Ray: NASA/CXC/ASU/J. Hester et al.</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/newsdesk/archive/releases/2002/24/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/newsdesk/archive/releases/2002/24/image/a</a></span></span></div>
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O Pulsar do Caranguejo. Esta imagem combina informações ópticas do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Hubble</a> (em vermelho) e imagens de <a href="http://pt.wikipedia.org/wiki/Astronomia_de_raios-X" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia de raios-X">raios-X</a> do <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">Observatório de raios-X Chandra</a> (em azul).</div>
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A composite image of the Crab Nebula showing the X-ray (blue), and optical (red) images superimposed. The size of the X-ray image is smaller because the higher energy X-ray emitting electrons radiate away their energy more quickly than the lower energy optically emitting electrons as they move</div>
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<span class="mw-headline" id="Condi.C3.A7.C3.B5es_f.C3.ADsicas" style="font-weight: normal;"><span style="font-size: large;">Condições físicas</span></span></h2>
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Os filamentos observados são restos da <a href="http://pt.wikipedia.org/wiki/Atmosfera" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Atmosfera">atmosfera</a> da estrela progenitora e consistem basicamente de <a href="http://pt.wikipedia.org/wiki/H%C3%A9lio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hélio">hélio</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a> <a href="http://pt.wikipedia.org/wiki/Ioniza%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ionização">ionizado</a>, juntamente com <a href="http://pt.wikipedia.org/wiki/Carbono" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Carbono">carbono</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a>,<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nitrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nitrogênio">nitrogênio</a>, <a href="http://pt.wikipedia.org/wiki/Ferro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ferro">ferro</a>, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ne%C3%B4nio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Neônio">neônio</a> e <a href="http://pt.wikipedia.org/wiki/Enxofre" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Enxofre">enxofre</a>. A temperatura dos gases nesses filamentos é de 11 000 a 18 000 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kelvin">kelvin</a> e sua <a href="http://pt.wikipedia.org/wiki/Densidade" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Densidade">densidade</a> é de 1 300 partículas por <a href="http://pt.wikipedia.org/wiki/Cent%C3%ADmetro_c%C3%BAbico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Centímetro cúbico">centímetro cúbico</a>.<span class="reference" id="cite_ref-Fesenetal1982_17-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Fesenetal1982-17" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">17</a></span>Considerando-se a <a href="http://pt.wikipedia.org/wiki/Luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Luz">luz visível</a>, a Nebulosa do Caranguejo é composta de uma massa <a href="http://pt.wikipedia.org/wiki/Oval" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Oval">oval</a> de filamentos, com diâmetro angular de aproximadamente 6x4 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a> em torno de uma região central azul difusa. Como comparação, a <a href="http://pt.wikipedia.org/wiki/Lua_cheia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lua cheia">lua cheia</a> tem 30 minutos de arco de diâmetro. Em três dimensões, especula-se que a nebulosa tenha a forma de um <a href="http://pt.wikipedia.org/wiki/Esferoide_prolato" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esferoide prolato">esferoide prolato</a>.<span class="reference" id="cite_ref-Trimble1973_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Trimble1973-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Ao longo de sua maior dimensão visível, a nebulosa mede cerca de (13 ± 3) anos-luz.</div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/59/Filaments_in_the_Crab_Nebula.jpg/640px-Filaments_in_the_Crab_Nebula.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#mediaviewer/Ficheiro:Filaments_in_the_Crab_Nebula.jpg</span></div>
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Imagem do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a> de uma pequena região da Nebulosa do Caranguejo, mostrando sua intricada estrutura filamentar. Crédito:<a href="http://pt.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/ESA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="ESA">ESA</a>.</div>
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Hubble Space Telescope image of filaments in the Crab Nebula (M1, NGC 1952).</div>
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Em 1953, o russo <a href="http://pt.wikipedia.org/wiki/Iosif_Shklovsky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Iosif Shklovsky">Iosif Shklovsky</a> propôs que a região azul difusa fosse produzida por <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_s%C3%ADncrotron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Radiação síncrotron">radiação síncrotron</a>, que é a radiação emitida pelo movimento curvilíneo de <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elétron">elétrons</a> em velocidades próximas à <a href="http://pt.wikipedia.org/wiki/Velocidade_da_luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Velocidade da luz">velocidade da luz</a>.<span class="reference" id="cite_ref-18" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-18" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">18</a></span> Três anos depois, a hipótese foi confirmada a partir das observações. Na década de 1960, verificou-se que a origem das trajetórias curvas dos elétrons era devida ao forte <a href="http://pt.wikipedia.org/wiki/Campo_magn%C3%A9tico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Campo magnético">campo magnético</a> produzido por uma <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> no centro da nebulosa.</div>
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A Nebulosa do Caranguejo é foco de muita atenção dos astrônomos, mas a sua distância à Terra permanece uma questão em aberto devido às grandes incertezas em cada método utilizado para calcular sua distância. Fotografias tomadas ao longo de vários anos revelam a lenta expansão da nebulosa,<span class="reference" id="cite_ref-19" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-19" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">19</a></span> e comparando esta expansão angular observada no céu com a sua velocidade de expansão determinada através da <a href="http://pt.wikipedia.org/wiki/Espectroscopia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Espectroscopia">análise espectroscópica</a>, a distância da nebulosa em relação à Terra pode ser estimada com mais precisão. Em 1973, uma análise a partir dos diversos métodos utilizados para calcular a distância à nebulosa alcançou a conclusão de 6 300 anos-luz.<span class="reference" id="cite_ref-Trimble1973_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Trimble1973-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> As estimativas mais recentes dão conta que sua distância em relação à Terra é de (6,5 ± 1,8) x 10³ anos-luz, o que equivale a (2,0 ± 0,5) <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>, e que está se expandindo a uma taxa de aproximadamente 1 500 quilômetros por segundo.<span class="reference" id="cite_ref-Bietneholz_20-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Bietneholz-20" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">20</a></span></div>
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Seguindo cronologicamente de forma retrógrada e uniforme sua expansão, alcança-se uma data várias décadas após 1054, o que implica que a sua velocidade de expansão tem acelerado desde a explosão da supernova.<span class="reference" id="cite_ref-Trimble1968_21-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Trimble1968-21" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">21</a></span> Acredita-se que esta aceleração seja causada pela energia do <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pulsar">pulsar</a>, que de alguma forma interfere com o <a href="http://pt.wikipedia.org/wiki/Campo_magn%C3%A9tico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Campo magnético">campo magnético</a> da nebulosa, que se expande e força seus filamentos em direção ao espaço vazio.<span class="reference" id="cite_ref-Bejgeretal2003_22-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo#cite_note-Bejgeretal2003-22" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">22</a></span></div>
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<span style="color: #252525; font-family: sans-serif;">Acredita-se que o pulsar do Caranguejo tenha cerca de 28 a 30 km de diâmetro.30 Emite pulsos de radiação a cada 33 milissegundos,31 e são emitidos em comprimentos de onda que abrangem praticamente todo o espectro eletromagnético, desde as ondas de rádio aos raios gama. Como todos os pulsares, o seu período de rotação está diminuindo gradualmente. Ocasionalmente, o seu período de rotação passa mudanças bruscas, conhecidas como "falhas", que se acredita serem causadas por um realinhamento repentino da massa da estrela de nêutrons, mudando seu momento de inércia e sua velocidade angular para que seu momento angular seja conservado. A energia liberada quando o pulsar desacelera é enorme e causa uma maior emissão da radiação síncrotron, que tem uma luminosidade total aproximadamente 75 000 vezes maior que a do Sol.32</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">LEIA MAIS</span></div>
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<a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>SAIBA MUITO, MUITO MAIS</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>SOBRE A NEBULOSA DO CARANGUEJO</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acessando</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://chandra.harvard.edu/xray_sources/crab/crab.htm" style="color: #274e13; text-decoration: none;">http://chandra.harvard.edu/xray_sources/crab/crab.htm</a></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">PÁGINA DA CHANDRA SOBRE A NEBULOSA</span></div>
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<span style="font-size: small;">Hubble Astronomers Unveil "Crab Nebula - The Movie"</span></h1>
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<a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/" style="color: #274e13; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/1996/22/video/</a></div>
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<span class="text-holder" style="float: right; width: 248px;"><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/a/" style="color: #993333; text-decoration: none;">Crab Nebula -- The Movie</a><span class="running-time" style="color: #666666; display: block; font-style: oblique;"><strong>Running Time: </strong>10 seconds</span></span><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/a/" style="color: #993333; text-decoration: none;"><img alt="Crab Nebula -- The Movie" class="icon" src="http://imgsrc.hubblesite.org/hu/db/1996/22/videos/a/thumb.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(103, 32, 29); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span class="text-holder" style="float: right; width: 248px;"><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/b/" style="color: #993333; text-decoration: none;">Animation Depicting the Environment Around the Pulsar</a><span class="running-time" style="color: #666666; display: block; font-style: oblique;"><strong>Running Time: </strong>18 seconds</span></span><a href="http://hubblesite.org/newscenter/archive/releases/1996/22/video/b/" style="color: #993333; text-decoration: none;"><img alt="Animation Depicting the Environment Around the Pulsar" class="icon" src="http://imgsrc.hubblesite.org/hu/db/1996/22/videos/b/thumb.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(103, 32, 29); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgCZimP79jvym1X88EWowguOLgJy719JU-F3xX5iZ97gL3PcURO7Fpf_08AvGJ_eWqk0y0OJHibiEdUAPTv6O1RLbnXPgO5iWiByGqNdezr8f469X8mJsuNl0aBg-L0npG4FamS4u25a80/s1600/m1animation_block_bw.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" height="522" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgCZimP79jvym1X88EWowguOLgJy719JU-F3xX5iZ97gL3PcURO7Fpf_08AvGJ_eWqk0y0OJHibiEdUAPTv6O1RLbnXPgO5iWiByGqNdezr8f469X8mJsuNl0aBg-L0npG4FamS4u25a80/s1600/m1animation_block_bw.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/image/0112/m1animation_block_bw.gif</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/ap011227.html" style="color: #274e13; text-decoration: none;">http://apod.nasa.gov/apod/ap011227.html</a></span></div>
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<b>The Incredible Expanding Crab </b><br /><b>Credit: </b>Courtesy <a href="mailto:ablock@noao.edu" style="color: #274e13;">Adam Block</a> (<a href="http://www.noao.edu/outreach/nop/pop.html" style="color: #274e13; text-decoration: none;">KPNO Visitor Program</a>), <a href="http://www.noao.edu/" style="color: #274e13; text-decoration: none;">NOAO</a>, <a href="http://www.nsf.gov/" style="color: #274e13; text-decoration: none;">NSF</a></center>
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<b>Explanation: </b>The Crab Nebula is cataloged as M1, the first on <a href="http://apod.nasa.gov/apod/ap960626.html" style="color: #274e13; text-decoration: none;">Charles Messier's</a> famous list of things which are not comets. In fact, <a href="http://apod.nasa.gov/apod/ap010602.html" style="color: #274e13; text-decoration: none;">the Crab is</a> now known to be a supernova remnant, an expanding cloud of debris from the explosion of a massive star. The violent birth of the Crab was <a href="http://www.seds.org/messier/more/m001_sn.html" style="color: #274e13; text-decoration: none;">witnessed by astronomers</a> in the year 1054. Roughly 10 light-years across today, the nebula is still expanding at a rate of over 1,000 kilometers per second. Flipping between two images made nearly 30 years apart, this animation clearly demonstrates the expansion. The smaller Crab was recorded as a <a href="http://www.noao.edu/image_gallery/html/im0345.html" style="color: #274e13; text-decoration: none;">photographic image</a> made in 1973 using the <a href="http://www.noao.edu/kpno/" style="color: #274e13; text-decoration: none;">Kitt Peak</a> National Observatory 4-meter telescope in 1973. <a href="http://www.noao.edu/outreach/aop/observers/m1.html" style="color: #274e13; text-decoration: none;">The expanded Crab</a> was made this year with the Kitt Peak <a href="http://www.noao.edu/outreach/nop/pop.html" style="color: #274e13; text-decoration: none;">Visitor Center's</a> 0.4-meter telescope and digital camera. Background stars were used to register the two images.</div>
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<b><span style="color: #660000; font-size: small;">Supernova</span></b><span style="color: #252525;"><span style="font-size: 14px;"> </span>é o nome dado aos corpos celestes surgidos após as explosões de </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a><span style="color: #252525;"> (estimativa) com mais de 10 </span><a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a><span style="color: #252525;">, que produzem objetos extremamente brilhantes, os quais declinam até se tornarem invisíveis, passadas algumas semanas ou meses. Em apenas alguns dias o seu brilho pode intensificar-se em 1 bilhão de vezes a partir de seu estado original, tornando a estrela tão brilhante quanto uma galáxia, mas, com o passar do tempo, sua temperatura e brilho diminuem até chegarem a um grau inferior aos primeiros.</span></div>
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A explosão de uma supernova pode expulsar para o espaço até 90% da <a href="http://pt.wikipedia.org/wiki/Mat%C3%A9ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Matéria">matéria</a> de uma <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a>. O núcleo remanescente tem massa superior a 1,5 massas solares, a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Press%C3%A3o_de_Degeneresc%C3%AAncia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pressão de Degenerescência">Pressão de Degenerescência</a> dos <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elétron">elétrons</a> não é mais suficiente para manter o núcleo estável; então os <a href="http://pt.wikipedia.org/wiki/El%C3%A9tron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elétron">elétrons</a> colapsam com o núcleo, chocando-se com os <a href="http://pt.wikipedia.org/wiki/Pr%C3%B3ton" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Próton">prótons</a>, originando<a href="http://pt.wikipedia.org/wiki/N%C3%AAutron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nêutron">nêutrons</a>: o resultado é uma estrela composta de <a href="http://pt.wikipedia.org/wiki/N%C3%AAutron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nêutron">nêutrons</a>, com aproximadamente 15 km de diametro e extremamente densa, conhecida como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela de nêutron">estrela de nêutrons</a> ou <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pulsar">pulsar</a>. Mas, quando a massa desse núcleo ultrapassa 3 massas solares, nem mesmo a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Press%C3%A3o_de_Degeneresc%C3%AAncia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pressão de Degenerescência">Pressão de Degenerescência</a> dos <a href="http://pt.wikipedia.org/wiki/N%C3%AAutron" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nêutron">nêutrons</a> consegue manter o núcleo; então a estrela continua a se colapsar, dando origem a uma <a href="http://pt.wikipedia.org/wiki/Singularidade_gravitacional" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Singularidade gravitacional">singularidade</a> no espaço-tempo, conhecida como <a href="http://pt.wikipedia.org/wiki/Buraco_negro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Buraco negro">buraco negro</a>, cuja <a href="http://pt.wikipedia.org/wiki/Velocidade_de_escape" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Velocidade de escape">velocidade de escape</a> é maior do que a velocidade da luz.</div>
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Atualmente, são utilizadas como velas-padrão para estudos da expansão do universo, técnica similar à utilizada por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Edwin_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Edwin Hubble">Edwin Hubble</a> com <a href="http://pt.wikipedia.org/wiki/Cefeida" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cefeida">cefeidas</a>, mas, com eficiência muito maior, pois o brilho das Supernovas é bem maior.</div>
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LEIA MAIS em</div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/40/Crab_Nebula_NGC_1952_%28composite_from_Chandra%2C_Hubble_and_Spitzer%29.jpg/800px-Crab_Nebula_NGC_1952_%28composite_from_Chandra%2C_Hubble_and_Spitzer%29.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; text-align: -webkit-center;" /></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://en.wikipedia.org/wiki/Crab_Nebula#mediaviewer/File:Crab_Nebula_NGC_1952_(composite_from_Chandra,_Hubble_and_Spitzer).jpg</span></span></div>
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Crab Nebula NGC 1952 (composite from Chandra, Hubble and Spitzer)</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Author and source information" style="cursor: pointer; font-size: 0.8em;"><span class="mw-mmv-author">X-Ray: NASA/CXC/J.Hester (ASU); Optical: NASA/ESA/J.Hester & A.Loll (ASU); Infrared: NASA/JPL-Caltech/R.Gehrz (Univ. Minn.)</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spitzer.caltech.edu/images/2857-sig09-009-NASA-s-Great-Observatories-View-of-the-Crab-Nebula" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spitzer.caltech.edu/images/2857-sig09-009-NASA-s-Great-Observatories-View-of-the-Crab-Nebula</a> (<a class="external text" href="http://www.spitzer.caltech.edu/uploaded_files/images/0005/7591/sig09-009.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">direct link</a>)</span></span><br />
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<b><span style="font-family: Arial, Helvetica, sans-serif;">EM 04 de janeiro de 2003, SATURNO VISITOU </span></b></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">M1, A NEBULOSA DO CARANGUEJO!</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Eu me senti tão emocionada com aquele encontro que escrevi um conto surreal .</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">O Tempo e o Sonho da Luz do Passado</span></h3>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">(Uma conversa entre Saturno e a Nebulosa do Caranguejo, </span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">ouvida da Terra</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> - um conto surreal...)</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgyBWXSd0oxwNhdPghUTfzj0goKMPshOiyLHmnqqgiyUSVzmzravE_9vRJpPJTcSgPOJmXxVGJo3tQhc_SvSEvD-BNo34iWvQW0YIKZeE387jMdaBmRqanmjBH90pXhdvDdBeB2lJ72jfU/s1600/SATURNO.JPG" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" height="300" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgyBWXSd0oxwNhdPghUTfzj0goKMPshOiyLHmnqqgiyUSVzmzravE_9vRJpPJTcSgPOJmXxVGJo3tQhc_SvSEvD-BNo34iWvQW0YIKZeE387jMdaBmRqanmjBH90pXhdvDdBeB2lJ72jfU/s1600/SATURNO.JPG" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: white; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="400" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saturno - Nasa</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEia1y4KTqikT6AzU0dRW7m3-5iMveXxQcGxUsQZiHGqxSywrW42rE8X45YApbwk6o9eOjsxoQilHfQjXdSdWeULbARXIY1_fxDpTi2g6srzZzJbLKVKDsEbTd3joy4Eq2Sy1aiZgCWM4ro/s1600/m1_hst_900.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" height="347" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEia1y4KTqikT6AzU0dRW7m3-5iMveXxQcGxUsQZiHGqxSywrW42rE8X45YApbwk6o9eOjsxoQilHfQjXdSdWeULbARXIY1_fxDpTi2g6srzZzJbLKVKDsEbTd3joy4Eq2Sy1aiZgCWM4ro/s1600/m1_hst_900.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: white; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="400" /></a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap111225.html</span></div>
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<a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.3999996185303px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><a href="https://www.blogger.com/blogger.g?blogID=2442159895732486967" imageanchor="1" style="clear: right; color: #274e13; float: right; line-height: 22.3999996185303px; margin-bottom: 1em; margin-left: 1em; text-decoration: none;"></a><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>M1: The Crab Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a>, <a href="http://hubble.esa.int/" style="color: #274e13; text-decoration: none;">ESA</a>, J. Hester, A. Loll (<a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;">ASU</a>); Acknowledgement: Davide De Martin (<a href="http://www.skyfactory.org/" style="color: #274e13; text-decoration: none;">Skyfactory</a>)</span></div>
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<span style="color: #274e13;">2003 January 10 </span></div>
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<span style="color: #073763;"><b>The Crab that Played with the Planet </b><br /><b>Credit & Copyright: </b><a href="http://www.newastro.com/newastro/default.asp" style="text-decoration: none;">Ron Wodaski</a>, <a href="http://www.newastro.com/remote/" style="text-decoration: none;">Newastro Remote Telescope</a> at <a href="http://www.nmskies.com/" style="text-decoration: none;">New Mexico Skies</a></span></center>
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<span style="color: #073763;"><b>Explanation: </b><a href="http://es.rice.edu/ES/humsoc/Galileo/Things/saturn.html" style="text-decoration: none;">Wandering</a> through the constellation Taurus, <a href="http://science.nasa.gov/headlines/y2002/13dec_saturn.htm" style="text-decoration: none;">Saturn made</a> its closest approach to planet Earth last month, tilting its lovely rings toward appreciative skygazers while rising high in midnight skies. On January 4th and 5th, Saturn also crossed in front of the <a href="http://www.boop.org/jan/justso/crab.htm" style="text-decoration: none;">high and far-off</a> Crab Nebula (M1), a cosmic cloud of debris from a stellar explosion and first on the list of astronomer <a href="http://apod.nasa.gov/apod/ap960626.html" style="text-decoration: none;">Charles Messier's</a> celestial sights. But <a href="http://www.marcush.net/astronomy/m1.html" style="text-decoration: none;">Saturn and the Crab</a> made poor playmates, as light from the bright planet overwhelmed the the diffuse nebula, all but hiding the Crab <a href="http://www.surveyor.in-berlin.de/himmel/indexe.html#saturn" style="text-decoration: none;">during the transit</a>. Taken on January 2nd, a few days before their closest encounter, this composite digital image illustrates the problem. The <a href="http://www.seds.org/messier/m/m001.html" style="text-decoration: none;">subtle nebula</a> is just visible at the right, while on the left, light from a drastically over-exposed Saturn overflows its pixels. Composited into the image is a correctly exposed picture of <a href="http://apod.nasa.gov/apod/ap021104.html" style="text-decoration: none;">ringed Saturn</a> with the Saturnian moons labeled. The well-exposed Saturn image was also taken on January 2nd, but captured with an exposure lasting only a fraction of a second, in contrast with the tens of seconds of exposure time required to reveal the Crab.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium trabalhado no Programa Corel - para a data de 04 de janeiro de 2003</span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong mw-mmv-truncate-toolong" original-title="Author and source information" style="cursor: pointer;"><span class="mw-mmv-source" style="color: #660000;"><b style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">NEBULOSA DO CARANGUEJO, M1, NGC 1952!</b></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">........................... Uma estrela que certa dia explodiu, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tornando-se uma chamada supernova,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que, com o passar do tempo, tornou-se uma nuvem...;</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nuvem penetrada por lentes ópticas </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">comandadas por olhares penetrantes e estudiosos...; </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">nuvem que foi revelando, descobrindo, não mais cobrindo,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">seus segredos de vida (quase) infinita, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vida que sempre encontra </span><span style="font-family: Arial, Helvetica, sans-serif;">uma nova maneira de ser, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vida que se transforma em nova vida,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">através um novo coração, um pulsar, uma estrela de nêutrons, uma nova estrela<b>!</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tempo e Espaço atuando através a eterna continuidade da Vida.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: large;">O Tempo e o Sonho da Luz do Passado</span></h3>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">(Uma conversa entre Saturno e a Nebulosa do Caranguejo,</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> ouvida da Terra</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"> - um conto surreal...)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i>Janine Milward</i></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saturno andava pelos lados do Touro, cumprindo sua jornada em torno de sua estrela, nosso Sol. Do ponto de vista da Terra, Saturno se encontrava em movimento retrógrado, ainda cumprimentando uma vez mais e se despedindo das estrelas que compõem os chifres daquela constelação pertencente ao Zodíaco, a Roda dos Animais.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Certa noite, de 4 para 5 de janeiro de 2003, Saturno ia passando através da Nebulosa do Caranguejo (do ponto de vista da Terra) e pôde-se escutar essa conversa:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Tempo! Ó Tempo! Ó Ceifador de vidas!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saturno olhou de um lado para o outro e apenas podia ver uma nuvem difusa, com o centro azul esmeralda e as bordas amareladas, alaranjadas e avermelhadas ainda com riscos desencontrados e firulados esbranquiçados, desenhando sua visão... que bela visão!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Sim, quem me chama?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Sou eu, M1, a Nebulosa do Caranguejo como sou conhecida na Terra, sua irmã de seu sistema solar.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Olá, Nebulosa, eu já havia passado bem perto de você quando estava em meu movimento direto, já ansioso para deixar o Touro e me deixar enroscar pelos pés dos Gêmeos... mas a Terra me deu mais um movimento retrógrado... e eis-me aqui, voltando uns poucos graus Touro adentro até retomar meu movimento direto no final do mês de fevereiro... Mas, que bom revê-la, Nebulosa, assim tão difusa e maravilhante como um sonho de uma noite de verão... ou de inverno.... pois que não é verdade que você se situa bem próximo do ponto do Solstício de Junho, que traz o verão para o hemisfério norte e o inverno para o hemisfério sul?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - É bem verdade. Obviamente, esse será sempre seu ponto de vista de acordo com o lugar do espaço que você e seu sistema solar ocupam, meu caro Khronos. Nada no universo possui um lugar próprio, você bem sabe disso. Esse lugar aparentemente próprio será sempre designado por aquele que o observa e do ponto de vista de quem observa, naturalmente! Assim, para os Terrestres meu posicionamento é Ascensão Reta 05h 34m 30s e Declinação. +21 graus e 01 min.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - O Tempo contado a partir do ponto de vista da Terra é apenas uma objetividade dentro da total subjetividade do espaço e do tempo do universo - nisso você tem razão. Assim, para nós nesse sistema solar, o resto do universo parece quase não se mover.... por isso os antigos denominavam que tudo aquilo no universo para além de mim, Saturno, O Deus do Tempo, eram "estrelas fixas". Hoje, sabemos que não apenas nada é fixo no universo, como tudo se movimenta sempre, além da infinita expansão a qual, aparentemente, estamos destinados, nos separando cada vez mais uns dos outros, cada vez mais.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Diga-me, Deus do Tempo, por que seu também sou chamada de M1?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Charles Messier foi um caçador de cometas e de tal maneira estava interessado em descobrir novos cometas nos céus que fez uma lista dos objetos celestes que não eram cometas - assim ele poderia continuar em suas buscas já deixando de lado aqueles objetos eliminados! Então, ironicamente, foi exatamente esta lista que o colocou na história da astronomia - apesar de ele ter sido o descobridor ou co-descobridor de cerca de 13 cometas ao longo de sua vida.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O ano de 1758 foi um ano de expectativa de retorno do Cometa Halley, que na verdade, foi primeiramente encontrado por Palitzsch em 25 de dezembro e mais tarde, no ano seguinte, visto novamente por Messier em 21 de janeiro. Porém, ainda em 28 de Agosto de 1758, enquanto esquadrinhava os céus procurando pelo cometa, Messier encontrou uma nebulosa que acabou imortalizando seu nome e assim ele a descreveu em seus alfarrábios: ".... 28 de Agosto... ela se encontra acima do chifre mais ao sul do Taurus, sem conter qualquer estrela, tendo um névoa esbranquiçada, alongada e contornada como a luz de uma vela...." Era M1, a Nebulosa do Caranguejo, você!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Houve um tempo num passado não muito distante em que aquele pedaço do céu deu lugar a uma "estrela visitante" que surgiu com sua imensa luz mesmo durante o tempo da luz do Sol ao longo de 23 dias, maravilhando os povos que a observaram atentamente. Isso aconteceu em 04 de julho de 1054.... e por ainda mais dois anos, puderam os maravilhados Terrestres ainda observarem sua luz inebriante no céu noturno.... até que finalmente, seu brilho foi esmaecendo, esmaecendo, esmaecendo, até que desapareceu por completo, tão subitamente assim como havia chegado! E foi somente recentemente (com a ajuda de bons telescópios) que os Terrestres puderam voltar a ver aquela estrela - ou a memória do que ela havia sido no passado - através da nuvem de gases firulantes e coloridos que foram soprados, largados para trás, como um lenço de seda solto ao vento da escuridão da noite do universo sem fim....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">............... A verdade é que a explosão dessa estrela aconteceu cerca de 5500 anos antes de cristo...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Os Terrestres amantes do céu estão com seus telescópios voltados para nós, não é mesmo? Todos querem se deliciar com a bela visão que formamos num mesmo enquadramento de imagem mostrando você, Tempo, passeando contra o pano de fundo de meus restos de Luz do passado, de meu tapête bordado de sonho e de lembranças da bela e imensa estrela que já fui...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Não chore, meu sonho, minha ilusão, restos da estrela do passado, luz que se extinguiu mas que aqueceu o espaço em torno e seus planetas e sua vida durante tanto, tanto tempo! Não chore, não chore, você ainda é tão bela, tão cantada, tão encantada, tão sublime! Não é sublime morrer e ainda se deixar viver como um lenço de seda solto ao vento na noite escura, buscada por telescópios que escondem olhares ansiosos e perscrutadores...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Mas... eu já fui um sol, um imenso sol, bem maior do que o seu Sol, Tempo.... e no entanto, um dia, comecei a inchar, inchar, inchar, até que finalmente Buummm! explodi! E quando explodi pude ser vista e admirada por tantos outros sóis que de mim compadeceram e por tantos outros planetas e seres que por mim se encantaram! Mas a verdade é que eu deixei de ser um sol para me tornar apenas poeira de estrela e uma nuvem difusa e silenciosa, esvoaçante e inefável como um sonho quase intraduzível....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Mas você, meu sonho, você não morreu! Você não morreu! Você apenas se transmutou, você viveu a vida que a natureza lhe deu e viveu essa vida desde o seu princípio até o seu final.... e seu final foi apenas um "turning point" ou ponto de mutação, um ponto de transição.... porque nada no universo ou pluriverso realmente morre, apenas transmuta, muda, transforma, re-inicia sua vida através de uma outra forma, outra qualidade, outro modo de ser.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Mas eu era um sol! Eu aquecia planetas e seres, eu doava vida, eu era a vida.... e hoje, o que sou eu? Sou apenas sonho ou lembrança etérea do meu passado de glória!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Hoje você é uma Nebulosa em uma das suas formas... mas pense bem, o que terá acontecido com todo aquele material e gases ejetados no espaço intergalático depois de sua estonteante explosão?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nebulosa: - Bem, eu penso que tudo se dispersou céu a fóra, noite adentro ou a fóra.... tudo o que era vida em mim apenas se tornou lixo, solto, vagando por aí....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Quando você explodiu, numa galáxia muito distante aonde você morava, minha galáxia, meu país, a Via Láctea, já estava bem formada bem como minha casa, minha família, meu sistema solar. Eu mesmo pude observar você em sua explosão, em seu esmaecimento e quando você deixou sua casca de halo de sonhos sair de seu sol anterior e tornar-se uma nuvem vagante noite escura adentro... Mas também posso saber que seus outros restos têm formado, ao longo do Tempo - eu, Saturno, sendo o Tempo, bem sei disso - outros sóis, outros planetas, outros seres.... Você não pensa nisso? Você percebe que já hoje e certamente no futuro você estará vivendo, partes de você estarão vivendo em outras estrelas, outros planetas, outros seres, outras vidas?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - É verdade! O Tempo existe não apenas para mim hoje, que sou uma Nebulosa dos sonhos da Luz de outrora, mas também existe para todos os outros restos de mim mesma que vêm vagando universo adentro e afóra, agregando-se e fusionando-se também a outros restos de outras estrelas de outrora que também explodiram!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Assim, você, Nebulosa dos meus sonhos, você é passado, presente e futuro!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Passado porque ainda outras estrelas, planetas e seres do universo mais jovens e distantes que nós ainda não conheceram a luz advinda de sua explosão.... portanto, para eles, você ainda é uma estrela! Você ainda existe enquanto estrela!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Presente, porque para algumas estrelas, planetas e seres você está explodindo nesse exato momento: Buum! - assim, você nesse momento não é apenas uma estrela como também é uma estupenda e estonteante e maravilhante Supernova!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Futuro, porque ainda outras estrelas, planetas e seres em outros cantos ainda mais longínquos e jovens do universo não apenas sequer sonham ou têm a expectativa de ver sua luz nem como estrela nem como supernova e talvez nem como nebulosa mas que certamente serão confeccionados a partir de seus restos deixados vagando pelo universo.... Dessa forma, cara Nebulosa, você nunca deixará de ser uma estrela! Sua Luz será sempre Luz, não importa o tempo - mesmo porque o tempo é eterno e essa eternidade dará sempre berço à sua possibilidade de Luz acontecer!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Um dia também você não mais me verá, Tempo, nem mesmo como Nebulosa dos seus sonhos... Chegará um dia em que eu desvanecei por completo e em meu lugar apenas restará a escuridão dos céus.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Minha doce Nebulosa, mesmo que você hoje já seja um tanto apagada a olho nú, brilhando numa magnitude de oitava classe, quero revelar a você um segredo... você sabia que em seu centro, lá no lugar do seu coração, existe uma pulsar que gira 30 vezes por segundo, brilhando numa magnitude de décima sexta classe? Você tem coração! Seu coração bate aceleradamente e pode ser admirado somente por Terrestres munidos por telescópios poderosos!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Verdade? Sim, eu tenho um coração, assim como tudo no universo possui um coração, objetivo ou subjetivo.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Sim. E seu coração, seu pulsar, é uma estrela de nêutrons, portanto, você ainda é uma estrela!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - O que é uma estrela de nêutrons?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Bem, quando ultrapassada a fase de gigante vermelha de sua estrela enorme e maciça original, a camada externa foi perdida, dando origem a você, cara Nebulosa do Caranguejo. No entanto, as porções internas dessa estrela em sua explosão, sofreu um colapso tão violento, com sua massa atraída para o interior com tal força, que a massa da porção aniquilada, se compactou ainda para além do estágio de anã branca.... Assim, os elétrons foram forçados a se combinar com os prótons nos núcleos livres, formando nêutrons. Criou-se , então, uma estrela totalmente de nêutrons, sem carga elétrica, os quais se aproximam até se tocar.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Mas por que então as estrelas de nêutrons também são chamadas de pulsares?</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - As estrelas de nêutrons são pequenas o suficiente para dar um giro numa fração de segundo, sem se desintegrar no processo, graças à intensa gravidade em sua superfície. Elas apresentam um campo magnético fortíssimo, cujos pólos magnéticos não se localizam necessariamente nos pólos de rotação. Os elétrons, extremamente aglutinados pela atração gravitacional, conseguem escapar apenas junto aos pólos magnéticos e ao serem expulsos, perdem energia na forma de micro ondas. Quando a estrela de nêutrons lança as microondas em nossa direção, captamos uma ou duas explosões a cada rotação!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - Então... você quer dizer que meu coração é como um Farol no mar escuro dos céu profundo!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - E você mesma, Nebulosa, é como a chama de uma vela.... assim como Charles Messier bem descreveu você...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NEBULOSA: - No entanto, também meu coração vai parando, parando, vagarosamente, e desaparecendo por completo....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">SATURNO: - Isso também é uma verdade.... seu coração, seu pulsar, sua estrela de nêutrons, cara Nebulosa, vai perdendo sua energia rotatória à medida que emite microondas, aumentando o período de rotação bem vagarosamente, Na verdade, seu período fica 36,48 bilionésimos de segundo mais longo a cada dia...... Mas, veja por outro lado, é bem possível que este processo ainda dure por bilhões de anos a frente.... tempo suficiente para que você mesma, Nebulosa dos Sonhos, vá se dissipando, apagando - por não possuir mais tanta luz irradiada por sua estrela coronária - anuviando, esfumaçando, desaparecendo.... assim como a imagem do sonho que sai do consciente e retorna ao inconsciente, deixando apenas uma vaga lembrança, doce lembrança.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">.............. Nebulosa e Saturno, o Sonho de hoje e a Luz do Passado juntamente com O Tempo, explodiram em um radioso sorriso de alegria! O Tempo em sua viagem através do Sonho Desmanchado mal havia percebido que o tempo havia passado e os telescópios Terrestres já não mais apontavam para ambos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Tudo não passou de um evento astronômico que ficou no passado.....</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Bibliografia:</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">111 questões sobre a Terra e o Espaço - Isaac Asimov - Editora Best Seller</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Revista Astronomy Now, edição de Março de 1998 - seção Focus - Tema do mês: The Messier Objects: The Messier Marathon por Owen Brazell e The Messier Catalogue - páginas 41 a 52 - Tonbridge, Kent, England</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">"A Nebulosa do Caranguejo" é uma re-leitura, síntese e tradução de Janine de artigo extraído da Revista Astronomy em sua edição de novembro na seção "Southern Sky Show" - "The Starry Sky".</span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">Sobre A Nebulosa do Caranguejo</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nos dias 4 e 5 de janeiro de 2003, vimos Saturno, o Deus do Tempo, passeando através de M1,a Nebulosa do Caranguejo.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Por volta do ano 5500 antes de cristo, uma imensa estrela explodiu como Supernova... seis mil e quinhentos anos mais tarde, em 4 de julho de 1054, astrônomos japoneses e chineses puderam observar a aparição de uma 'estrela convidada" no céu na constelação que hoje denominamos de Touro. Essa nova estrela, tão brilhante quanto Vênus, pôde ser vista durante o dia por cerca de 23 dias e durante dois anos pôde ser observada e estudada no céu noturno.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando a supernova esmaeceu, passaram-se mais 700 anos até que uma pequena nuvem de gás verde luminoso surgiu no lugar aonde ela aparecera anteriormente, um grau ao norte e oeste de Zeta Tauri, já em um dos chifres do Touro quase aos pés dos Gêmeos.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Charles Messier (1730-1817) era um caçador de cometas e sempre vasculhava o céu em busca dos mesmos. Em 12 de setembro de 1758 (ou em 28 de Agosto, segundo outro documento - Nota da Tradutora), Messier apontou para esse ponto de luz difusa no céu e o descreveu a nebulosa como contendo nenhuma estrela, esbranquiçada em sua cor e alongada como a chama de uma vela. Mais tarde, Messier veio a saber que tal nebulosa já havia sido avistada por um astrônomo inglês, John Bevis, em 1731.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Messier continuou sua busca por cometas (naquele mesmo houve o retorno, já previsto, do Cometa Halley durante o mês de dezembro) - e passou então, a elaborar uma lista de objetos no céu que não eram cometas. Finalmente, uma versão final dessa lista foi publicada em 1784 contendo 109 ou 110 objetos, sendo que o primeiro objeto mencionado foi a Nebulosa que ora é visitada por Saturno. Essa lista é hoje conhecida como A Lista de Messier e seus objetos são denominados M1, M2, M3.... A Nebulosa do Caranguejo é M1.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, esse nome, Nebulosa do Caranguejo foi dado por Earl of Rosse, em 1840 que publicou um desenho da mesma com filamentos que sugeriam o formato de um caranguejo. Mais tarde, ele observou a nebulosa já com outra aparelhagem mais potente e rejeitou sua descrição anterior da mesma.... tarde demais: a Nebulosa do Caranguejo já era assim conhecida!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Nebulosa do Caranguejo não é difícil de ser localizada com um telescópio mais simples e do quintal de sua casa - afinal foi assim que Messier a encontrou! Porém, em céus mais transparentes, longe das luzes da cidade, sua visão se torna bem mais enriquecida e se você tiver um telescópio possante, será fantástico poder observar um estrela que ainda permanece em seu centro, um pulsar que gira cerca de 30 vezes por segundo!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Sítio das Estrelas - parada de um caminho a Caminho do Céu</span></div>
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<span style="color: #274e13;">http://apod.nasa.gov/apod/ap020920.html<span style="margin-left: 1em; margin-right: 1em;"></span></span></div>
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<span style="color: #274e13;"><b style="line-height: normal; text-align: -webkit-center;">The Crab Nebula Pulsar Shrugs </b></span></div>
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<span style="color: #274e13;"><span style="line-height: normal; text-align: -webkit-center;"></span><b><br style="line-height: normal; text-align: -webkit-center;" /></b><span style="line-height: normal; text-align: -webkit-center;">Credit: </span><span style="line-height: normal; text-align: -webkit-center;"></span><a href="http://eagle.la.asu.edu/hester/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">J. Hester</a><span style="line-height: normal; text-align: -webkit-center;"> (</span><a href="http://phyastweb.la.asu.edu/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">ASU</a><span style="line-height: normal; text-align: -webkit-center;">), </span><a href="http://chandra.harvard.edu/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">CXC</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.stsci.edu/hst/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">HST</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.nrao.edu/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">NRAO</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.nsf.gov/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">NSF</a><span style="line-height: normal; text-align: -webkit-center;">, </span><a href="http://www.nasa.gov/" style="color: #274e13; line-height: normal; text-align: -webkit-center; text-decoration: none;">NASA</a></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" height="220" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a></div>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a4/Charles_Messier.jpg/220px-Charles_Messier.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nossa visita</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> através a constelação da Serpente</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- Serpens Cauda e Serpens Caput -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acontecerá em</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M5 e M16, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">os Objetos Messier em Serpens.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ophiucus, o Serpentário, Aquele que Segura a Serpente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é uma constelação bem interessante</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">porém composta de estrelas não muito proeminentes</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- e, da mesma forma, assim acontece </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">com a constelação da Serpente, ou seja, Serpens Cauda e Serpens Caput.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="background-color: white; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, em lugares de céus escuros e transparentes</span></div>
<div style="background-color: white; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;">e, de preferência, em noites de ausência de iluminação da Lua,</span></div>
<div style="background-color: white; line-height: 22.3999996185303px;">
<span style="font-family: Arial, Helvetica, sans-serif;">podemos observar algumas estrelas pertencentes </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">aos desenhos estelares de Ophiucus e de Serpens!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Pessoalmente, sou muitíssimo fascinada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">pelo asterismo formado pela Cabeça propriamente dita</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de Serpens Caput:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Cabeça propriamente dita da Serpente é de uma beleza extremamente rara,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> com suas cinco estrelas (pelo menos, é bem assim que as vejo e conto)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> fazendo acontecer um Asterismo quase realizando uma imagem de um papagaio, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">uma pandorga, um <i>kite</i>, uma pipa...</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;">É uma visão magnífica e ao mesmo tempo, aterrorizante! </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> Quer dizer, a Coroa Boreal é uma constelação de delicadeza ímpar em suas estrelinhas tímidas... </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;">Mais tímidas ainda são as estrelinhas que compõem a Cabeça propriamente dita da Serpente... </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;">e é exatamente este fato que torna este conjunto de situações</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> - Coroa Boreal e Cabeça da Serpente -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> como algo que realmente vale a pena ser observado...., </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;">sempre em lugares de céus escuros e transparentes e em noites sem Lua, de preferência.</span></div>
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(Leia mais sobre Serpens,</div>
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acessando meu Trabalho em</div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/serpens-serpente.html)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Bem, o texto imediatamente acima, sobre a Cabeça da Serpente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">refere-se à nossa visão dos céus estrelados sendo exercida a olho nú.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">No entanto, é na Cauda da Serpente</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e auxiliados por lentes extremamente potentes,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é que vamos encontrar um objeto extremamente interessante</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e maravilhoso, que vem encantando a nós todos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- principalmente através a visão exuberante</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">dos chamados "Pilares da Criação",</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">inseridos na Nebulosa da Águia, M16, descrita neste Trabalho.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">É bem interessante percebermos o fato de que</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">a imensa figura estelar do Serpentário segurando a Serpente</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- é uma constelação tripla, digamos assim! -,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">se posiciona bem próxima, porém mais ao norte,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">das constelações do Escorpião e do Sagitário</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e, portanto, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem próxima do ponto que nos leva ao centro da Galáxia!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saiba sobre os Objetos Messier encontrados em Ophiucus,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">o Serpentário,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acessando nosso Trabalho em</span></div>
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<span style="font-size: small; line-height: normal;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m9-m10-m12-m14-m19-m62-e-m107-os.html</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_-AP46BdF8Q2j2-XkKAQ7DUYsmIZiar0nQlKWP0d-MhYZHacuSojSTyMNfWl1rXQzvG9owkkq_RhgGfF93tqDBXDKnlF6dGQjew3l515z334FJecL9JnijKC5UQ3g0uLS_ybctdw3IPR8/s1600/Eagle_nebula_pillars.jpg" imageanchor="1" style="color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEh_-AP46BdF8Q2j2-XkKAQ7DUYsmIZiar0nQlKWP0d-MhYZHacuSojSTyMNfWl1rXQzvG9owkkq_RhgGfF93tqDBXDKnlF6dGQjew3l515z334FJecL9JnijKC5UQ3g0uLS_ybctdw3IPR8/s640/Eagle_nebula_pillars.jpg" height="631" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 15.828125px;"><span style="color: #073763; font-size: x-small;"><b style="background-color: white;">Os "Pilares da Criação" </b></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #073763; font-size: x-small; line-height: 15.828125px;"><b>no interior da Nebulosa da Águia</b>.</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><span style="line-height: 15.828125px;"> </span><small style="line-height: 15.828125px;">Cortesia <a href="http://pt.wikipedia.org/wiki/NASA" style="background-image: none; color: #274e13; text-decoration: none;" title="NASA">NASA</a>/<a href="http://pt.wikipedia.org/wiki/ESA" style="background-image: none; color: #274e13; text-decoration: none;" title="ESA">ESA</a><br /><a href="http://pt.wikipedia.org/wiki/Ficheiro:Eagle_nebula_pillars.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Ficheiro:Eagle_nebula_pillars.jpg</a><br /><span style="line-height: 19.1875px;">Credit: NASA, Jeff Hester, and Paul Scowen (Arizona State University)</span></small></span></div>
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<span style="background-color: white; line-height: 18px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"><img src="http://www.raremaps.com/maps/medium/33412op.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://www.raremaps.com/gallery/detail/33412op/_Serpens/Bayer.html" style="color: #274e13; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/33412op/_Serpens/Bayer.html</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Johann Bayer</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;"><span style="color: #660000;">Serpens Cauda et Serpens Caput </span></b></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"> a Cauda e a Cabeça da Serpente</span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Posicionamento:</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 15h8m / 18h56m Declinação +25<sup>o</sup>.7 / -16<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando Glaucus, filho de Minos, Rei de Creta, foi afogado em uma colméia, Esculapius foi trazido para restaurar a vida ao menino. Enquanto Esculapius pensava o que iria fazer, uma serpente entrou no quarto e ele matou-a. Então, entrou outra serpente trazendo uma erva que foi colocada na cabeça da serpente morta, trazendo-a à vida. Usando a mesma erva, Esculapius trouxe a vida de volta ao menino. A serpente foi colocada nos céus e é por esta razão que muitos escritores confundem Ophiucus com Esculapius. De acordo com outro mito, a serpente seria uma das que deveriam matar Hercules em seu berço, quando ainda era uma criança.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Serpens (Cauda e Caput) acabam fazendo parte da constelação Ophiucus</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - porque este é Aquele que Segura a Serpente -</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> e todas três constelações acabam formando um conjunto imenso </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de situações entrelaçadas. </span><br />
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; margin-left: 1em; margin-right: 1em;"><br /><br /><img src="http://www.raremaps.com/maps/medium/34480.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">E também estaremos encontrando as constelações Scorpius, Sagittarius, Scutum, Aquila, Hercules Corona Borealis, Libra<o:p></o:p></span><br />
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<a href="http://www.raremaps.com/gallery/detail/34480/Ophiuchus_and_Serpent/Jamieson.html" style="background-color: white; color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/34480/Ophiuchus_and_Serpent/Jamieson.html</span></a><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1372" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Alexander Jamieson</a></span></div>
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Messier 5</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M5 (NGC 5904)</i>, class V, in <a href="http://messier.obspm.fr/map/SerCap.html">Serpens</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">15 : 18.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+02 : 05 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">24.5 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">23.0 (arc min)</td></tr>
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Discovered 1702 by Gottfried Kirch.</div>
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Globular cluster Messier 5 (M5, NGC 5904) was first seen by <a href="http://messier.obspm.fr/xtra/Bios/kirch.html">Gottfried Kirch</a> and his wife Maria Margarethe on May 5, 1702, when they observed a comet, and described as a "nebulous star". <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> found it independently on May 23, 1764, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M5">described it</a> as a round nebula which "doesn't contain any stars". <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> was the first to resolve this cluster into stars; he counted 200 of them with his 40-foot [FL] reflector in 1791, "although the middle is so compressed that it is impossible to distinguish the components."</div>
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LEIA MAIS</div>
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em</div>
http://messier.obspm.fr/m/m005.html<br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjYeYvNNTR9rVIce4Pzr9_LtFOVlxKKYLyzWD_Q5ogXcEl6dP5NMVTNfjs1-XugLainMuvV0kyLIFadfzV3jxSvK3WZ2-2v15C6xJmiRytGUxin9KEGzhLezoBJ-UrpIGIpIEPuh7cM9H8/s1600/m5.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjYeYvNNTR9rVIce4Pzr9_LtFOVlxKKYLyzWD_Q5ogXcEl6dP5NMVTNfjs1-XugLainMuvV0kyLIFadfzV3jxSvK3WZ2-2v15C6xJmiRytGUxin9KEGzhLezoBJ-UrpIGIpIEPuh7cM9H8/s1600/m5.png" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">http://www.stellarium.org/pt/</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M5 - NGC 5904 - Aglomerado Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na parte da Cabeça da Serpente, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um brilhante aglomerado globular distante cerca de 27 mil anos-luz </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e contendo cerca de meio milhão de estrelas.<o:p></o:p></span><br />
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span><br />
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjI-w8fJE0M35z3crK-AwvlfgeDMsgZ6XQ9XLW6-5Qqo1VwtycmaKHXb1VqxH3QazBXHjdUtj8-bh-GNTtu373yFL5TyOXZmLlJYYUGEXNN5PpkGr3PX8LdHXPDQBiOnxolQ7vlwxw7vp2G/s1600/Messier5_Hubble_WikiSky.jpg" imageanchor="1" style="color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjI-w8fJE0M35z3crK-AwvlfgeDMsgZ6XQ9XLW6-5Qqo1VwtycmaKHXb1VqxH3QazBXHjdUtj8-bh-GNTtu373yFL5TyOXZmLlJYYUGEXNN5PpkGr3PX8LdHXPDQBiOnxolQ7vlwxw7vp2G/s640/Messier5_Hubble_WikiSky.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><a class="extiw" href="http://en.wikipedia.org/wiki/Messier_5" style="background-image: none; color: #274e13; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Messier 5">en:Messier 5</a><span style="line-height: 18.234375px; text-align: start;"> - </span><a class="extiw" href="http://en.wikipedia.org/wiki/globular_cluster" style="background-image: none; color: #274e13; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:globular cluster">en:globular cluster</a><span style="line-height: 18.234375px; text-align: start;"> by </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; color: #274e13; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a><span style="line-height: 18.234375px; text-align: start;">. </span><i style="line-height: 18.234375px; text-align: start;">2.4′ view</i><span style="line-height: 18.234375px; text-align: start;">. The image created using </span><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; color: #274e13; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:WikiSky">en:WikiSky</a><span style="line-height: 18.234375px; text-align: start;">'s image cutout tool out of </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; color: #274e13; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a><span style="line-height: 18.234375px; text-align: start;">data. Source url: </span><a class="external autonumber" href="http://server1.wikisky.org/snapshot?survey=ASTROPHOTO&img_id=60142&angle=0.040&ra=15.3093&de=2.084&x_shift=0&y_shift=0&width=2800&height=2800&projection=tan&rotation=0&reverse=0&interpolation=bicubic&jpeg_quality=.95" rel="nofollow" style="color: #274e13; text-decoration: none;">[1]</a><span style="line-height: 18.234375px; text-align: start;"> Hubble source data: </span><a class="external autonumber" href="http://archive.stsci.edu/cgi-bin/mastpreview?mission=hst&dataid=J9DX02080" rel="nofollow" style="color: #274e13; text-decoration: none;">[2]</a><span style="line-height: 18.234375px; text-align: start;">. Related images: </span><a class="extiw" href="http://en.wikipedia.org/wiki/Image:m5--LRGB2_898x688.jpg" style="background-image: none; color: #274e13; line-height: 18.234375px; text-align: start; text-decoration: none;" title="en:Image:m5--LRGB2 898x688.jpg">en::Image:m5--LRGB2 898x688.jpg</a><span style="line-height: 18.234375px; text-align: start;">.</span><a href="http://pt.wikipedia.org/wiki/Messier_5" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_5</a></span></td></tr>
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<b>Messier 5</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 5904</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Serpens" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Serpens">Serpente</a>. Foi descoberto em 1702 pelo astrônomo alemão <a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a> e catalogado por<a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764. Sua natureza como aglomerado globular foi evidenciada pela descoberta de suas estrelas mais brilhantes, <a href="http://pt.wikipedia.org/wiki/Resolu%C3%A7%C3%A3o_de_imagem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Resolução de imagem">resolvidas</a> por <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a> da década de 1780.</div>
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Com <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,5, pode ser observado a <a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> apenas sob condições excelentes de visualização. Contudo, pode ser visto como uma mancha nebulosa e difusa com <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> e pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>. Suas estrelas mais brilhantes são resolvidas apenas com telescópios maiores. Situa-se a cerca de 14 500 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>e sua idade foi estimada em 13 bilhões de anos.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Messier 5</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_5_Hubble_WikiSky.jpg" style="background: none;" title="Messier 5 visto pelo Telescópio Espacial Hubble."><img alt="Messier 5 visto pelo Telescópio Espacial Hubble." data-file-height="3152" data-file-width="3152" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/92/Messier_5_Hubble_WikiSky.jpg/250px-Messier_5_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/92/Messier_5_Hubble_WikiSky.jpg/375px-Messier_5_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/92/Messier_5_Hubble_WikiSky.jpg/500px-Messier_5_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />Messier 5 visto pelo Telescópio Espacial Hubble.</span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Descoberto por</span></span></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background: none; line-height: 22.3999996185303px;" title="Gottfried Kirch"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Gottfried Kirch</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Data</span></span></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1702" style="background: none; line-height: 22.3999996185303px;" title="1702"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">1702</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Dados observacionais (J2000)</span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; line-height: 22.3999996185303px;" title="Constelação"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Constelação</span></a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; line-height: 22.3999996185303px;" title="Scorpius"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Scorpius</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Tipo</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">V</span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; line-height: 22.3999996185303px;" title="Ascensão reta"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Asc. reta</span></a></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">15<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 18<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 33,75<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_5#cite_note-simbad-1" style="background: none;">1</a></span></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; line-height: 22.3999996185303px;" title="Declinação"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Declinação</span></a></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">+02° 04′ 57,7″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_5#cite_note-simbad-1" style="background: none;">1</a></span></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Distância</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">14 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none;" title="Ano-luz">anos-luz</a> (7,5 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none;" title="Parsec">kpc</a>)</span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; line-height: 22.3999996185303px;" title="Magnitude aparente"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Magnit. apar.</span></a></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">6,65<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_5#cite_note-simbad-1" style="background: none;">1</a></span></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Dimensões</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">23',0</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Características físicas</span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Raio</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">80 anos-luz</span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Idade estimada</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">~13 bilhões de anos</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Outras denominações</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none;" title="New General Catalogue">NGC</a> 5904</span></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; line-height: 22.3999996185303px;" title="Messier 5"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><img alt="Messier 5" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Serpens_constellation_map.png" style="background: none; line-height: 22.3999996185303px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><img alt="Serpens constellation map.png" data-file-height="2269" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/250px-Serpens_constellation_map.png" height="222" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/375px-Serpens_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/500px-Serpens_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_5</span><br />
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<br />
<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/92/Messier_5_Hubble_WikiSky.jpg/800px-Messier_5_Hubble_WikiSky.jpg" /><br />
http://pt.wikipedia.org/wiki/Messier_5#mediaviewer/File:Messier_5_Hubble_WikiSky.jpg<br />
<div class="mw-mmv-title-para" style="color: #333333; font-family: sans-serif; line-height: 1.5em; overflow: hidden; padding: 10px 20px 0px; text-overflow: ellipsis; white-space: nowrap;">
<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 5 Hubble WikiSky</span></div>
<div class="mw-mmv-credit" style="color: #333333; font-family: sans-serif; line-height: 1.5em; overflow: hidden; padding: 5px 20px; text-overflow: ellipsis; white-space: nowrap;">
<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">ESA/Hubble & NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/potw1118a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/potw1118a/</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; margin-left: auto; margin-right: auto;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgxPHFf0IxUDPy3ls9sx8C-JvDnzfOmyMJTM8YrbRj0xEFKM-y1JPTu9-ECaRhU-_cIrn58lIXwigQpmLWZcvMs7dF4_o4mBxpqy_jz_bH5zvxD_iivisMPrpUPgQWkiklsD5jnzpvRqaqn/s1600/SERPENSA+CAUDA.jpg" imageanchor="1" style="color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgxPHFf0IxUDPy3ls9sx8C-JvDnzfOmyMJTM8YrbRj0xEFKM-y1JPTu9-ECaRhU-_cIrn58lIXwigQpmLWZcvMs7dF4_o4mBxpqy_jz_bH5zvxD_iivisMPrpUPgQWkiklsD5jnzpvRqaqn/s1600/SERPENSA+CAUDA.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></span></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></td></tr>
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<span style="background-color: white; line-height: 22.3999996185303px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m16atlas.jpg</span></span></div>
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<h1>
Messier 16</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Starforming Nebula</a> M16 (IC 4703, NGC 6611)</i>, an emission nebula, with <a href="http://messier.obspm.fr/cluster.html">Open Star Cluster</a>, type 'e', in <a href="http://messier.obspm.fr/map/SerCau.html">Serpens (Cauda)</a></center>
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<br /><b><span style="font-size: large;">Eagle Nebula</span></b><br /><b><br /></b></center>
<a href="http://messier.obspm.fr/Jpg/m16.jpg"><img align="right" alt="[m16.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m16.jpg" /></a><br />
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">18 : 18.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-13 : 47 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">7.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">7.0 (arc min)</td></tr>
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Cluster M16 (NGC 6611) discovered by Philippe Loys de Chéseaux in 1745-6.<br />
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Nebula M16 (IC 4703) discovered by Charles Messier in 1764.<br />
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The Eagle Nebula Messier 16 (M16) is a conspicuous region of active star formation, situated in Serpens Cauda. The starforming nebula, a giant cloud of interstellar gas and dust, has already created a considerable cluster of young stars. The cluster is also referred to as NGC 6611, the nebula as IC 4703.<br />
The discoverer, <a href="http://messier.obspm.fr/xtra/similar/deches.html">Philippe Loys de Chéseaux</a>, describes only the cluster when recording his 1745-1746 discovery. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, on his independent <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M16">rediscovery of June 3, 1764</a>, mentions that these stars appeared "enmeshed in a faint glow", probably suggestions of the nebula. The Herschels apparently didn't perceive the nebula, so that their catalogs and consequently, the NGC, only describe the cluster. The nebula was added in the IC II of 1908 as <a href="http://messier.obspm.fr/Mdes/dm016.html#IC">IC 4703</a>, with "cluster M16 involved", but the NGC 2000.0 erroneously classifies this object as an open cluster.<br />
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LEIA MAIS<br />
em<br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M16 - NGC 6611 - Aglomerado Aberto</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fazendo parte da Cauda da Serpente, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">encontramos um grande aglomerado aberto </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">rodeado por uma nebulosa difusa, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um dos mais interessantes objetos de sua espécie, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">denominado de <b>A Nebulosa da Águia ou a Nebulosa da Estrela da Rainha</b> </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(em função da silhueta escura no meio da nebulosa, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">parecendo uma rainha sentada no trono). </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A nebulosa luminosa encontra-se numa região de hidrogênio ionizado </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e ao fundo existem regiões de material interestelar frios e escuros</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> - tudo isso formando um modelo bizarro. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> M16 cobre uma área igual à de uma Lua cheia, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">no entanto sua luminosidade é pálida </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e difícil de ser observada mesmo em grandes telescópios.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span><br />
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<tr><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:Eagle Nebula from ESO.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/2b/Eagle_Nebula_from_ESO.jpg/600px-Eagle_Nebula_from_ESO.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; margin-left: auto; margin-right: auto; padding: 8px;" width="640" /></span></td></tr>
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<a class="external free" href="http://www.eso.org/public/images/eso0926a/" rel="nofollow" style="color: #274e13; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://www.eso.org/public/images/eso0926a/</span></a></div>
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<span style="font-size: small;">A <b>Nebulosa da Águia</b> (Messier 16, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6611</a>) é um jovem <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Serpens" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Serpens">Serpente</a>. O objeto foi descoberto pelo astrônomo francês<a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1745-46 e seu nome deriva da forma que sua <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nuvem interestelar</a> protoestelar em torno do aglomerado, que lembra uma <a href="http://pt.wikipedia.org/wiki/%C3%81guia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Águia">águia</a>. A fotografia tomada da nebulosa pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a> tomada no início de abril de 1995 ficou conhecida como os "<a href="http://pt.wikipedia.org/wiki/Pilares_da_Cria%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pilares da Criação">Pilares da Criação</a>", e mostra pilares de <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Meio interestelar">gás estelar e poeira</a>contida na nebulosa.</span></div>
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<span style="font-size: small;">Situa-se aproximadamente 7 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e sua <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> é igual a 6,4, sendo fracamente visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, mesmo em excelentes condições de observação. É um sistema relativamente jovem, em termos astronômicos, com apenas 5,5 milhões de anos.</span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; font-size: 15px; text-align: center;"><b>Nebulosa da Águia</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Stellar_spire_eagle_nebula.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="{{{legenda}}}"><img alt="{{{legenda}}}" data-file-height="7804" data-file-width="3857" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/97/Stellar_spire_eagle_nebula.jpg/250px-Stellar_spire_eagle_nebula.jpg" height="506" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/97/Stellar_spire_eagle_nebula.jpg/375px-Stellar_spire_eagle_nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/97/Stellar_spire_eagle_nebula.jpg/500px-Stellar_spire_eagle_nebula.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Nebulosa da Águia</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;">1746</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado aberto</a> (<b>II,3,m,n</b>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Serpens" style="background: none; color: #0b0080; text-decoration: none;" title="Serpens">Serpens</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">18h 18,8m}<span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_da_%C3%81guia#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">−13° 47′<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_da_%C3%81guia#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,4<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_da_%C3%81guia#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">Magnit. absol.</a></td><td style="background-color: #f8f8f8;">−8,21</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">7.000 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">7,0 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">Messier 16, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6611, IC 4703</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa da Águia"><img alt="Nebulosa da Águia" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Serpens_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Serpens constellation map.png" data-file-height="2269" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/250px-Serpens_constellation_map.png" height="222" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/375px-Serpens_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/91/Serpens_constellation_map.png/500px-Serpens_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="font-size: small;"><span style="color: #252525;">As imagens obtidas pelo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a><span style="color: #252525;">, em 1995, com a colaboração de Jeff Hestre e Paul Scowen, melhoraram significativamente o entendimento científico dos processos que ocorrem no interior da nebulosa. Uma dessas fotografias, que ficou conhecida como os </span><b><span style="color: #660000;">"<a href="http://pt.wikipedia.org/wiki/Pilares_da_Cria%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Pilares da Criação">Pilares da Criação</a>"</span></b><span style="color: #252525;">, mostra uma grande região de formação de estrelas. Acredita-se que as áreas pequenas e negras são </span><a href="http://pt.wikipedia.org/wiki/Protoestrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Protoestrela">protoestrelas</a><span style="color: #252525;">. A estrutura da região em pilares lembra uma outra região de formação de estrelas, muito maior, registrada pelo </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a><span style="color: #252525;"> em 2005, na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> da </span><a href="http://pt.wikipedia.org/wiki/Cassiopeia_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cassiopeia (constelação)">Cassiopeia</a><span style="color: #252525;">, conhecida como a </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_da_Alma" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa da Alma">Nebulosa da Alma</a><span style="color: #252525;"> (W5).</span><span class="reference" id="cite_ref-3" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_da_%C3%81guia#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><span style="color: #252525;"> Esta nebulosa também recebeu a designação "Pilares da Criação" por ter estruturas semelhantes a da Nebulosa da Águia. Estas colunas, que lembram a </span><a href="http://pt.wikipedia.org/wiki/Estalagmite" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estalagmite">estalagmites</a><span style="color: #252525;"> que bortam do chão de uma caverna, são compostas de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a><span style="color: #252525;"> e poeira, que agem como incubadores de novas estrelas. Dentro das colunas e nas suas superfícies, os astrônomos encontraram nós, ou glóbulos, de gás mais denso, chamados EGG (</span><i style="color: #252525;">Evaporating Gaseous Globules</i><span style="color: #252525;"> - Glóbulos Gasosos em Evaporação). Várias estrelas estão sendo formadas no interior destes glóbulos.</span></span></div>
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<span style="font-size: small;">Combinação de imagens de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raios-x" style="background: none; color: #0b0080; text-decoration: none;" title="Raios-x">raios-x</a> obtidas pelo <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">observatório de raios-X Chandra</a> com as imagens do Telescópio Espacial Hubble dos "Pilares da Criação" mostraram que as fontes de raios-X de estrelas jovens não coincidem com os pilares, mas em um ponto aleatório qualquer. Isto sugere que a formação de estrelas alcançou seu máximo a cerca de um milhão de anos atrás e que qualquer protoestrela contida em glóbulo gasoso em evaporação são suficientemente quentes para produzir raios-X.</span></div>
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<span style="font-size: small;">O maior de tais "pilares" tem 7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> de comprimento. Devido à sua grande densidade, os gases contidos nos pilares se aglutinam gravitacionalmente para formar estrelas. Em cada ponta do pilar, a intensa radiação emitida pelas estrelas jovens causam a dispersão de elementos menos densos, deixando exposto alguns glóbulos gasosos em evaporação, berçário de novas estrelas.</span></div>
<span style="font-size: small;">http://pt.wikipedia.org/wiki/Nebulosa_da_%C3%81guia</span><br />
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">http://apod.nasa.gov/apod/ap120722.html<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">M16: Pillars of Creation </span></b><span lang="EN-US"><br /><b>Image Credit: </b>J. Hester, P. Scowen (</span><a href="http://sese.asu.edu/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">ASU</span></a><span lang="EN-US">), </span><a href="http://www.stsci.edu/hst/HST_overview/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">HST</span></a><span lang="EN-US">, </span><span lang="EN-US" style="color: #274e13;"><a href="http://www.nasa.gov/" style="color: #274e13; text-decoration: none;">NASA</a></span></span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.1875px;">"</span><b style="font-family: Arial, Helvetica, sans-serif; line-height: 19.1875px;">Os pilares da criação</b><span style="font-family: Arial, Helvetica, sans-serif; line-height: 19.1875px;">" é um aglomerado de poeira e gás com tamanho interestelar na nebulosa de Aguia situado à aproximadamente 7,000 anos luz da terra, No nome, "Pilares" é sugestivo ao formato do lugar, e a parte "Criação" originou-se devido o local ser um enorme berço de estrelas. Sua primeira imagem datada em 1/04/1995, foi tirada pelo telescópio espacial Hubble.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Pilares_da_Cria%C3%A7%C3%A3o" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Pilares_da_Cria%C3%A7%C3%A3o</a></span></div>
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<a href="http://www.spacetelescope.org/images/heic0506b/" style="background-color: white; color: #274e13; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; text-align: center; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/heic0506b/</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">The Eagle has risen: Stellar spire in the Eagle Nebula</span></h1>
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<a href="http://www.spacetelescope.org/images/heic0506b/" style="background-color: white; color: #274e13; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; text-align: center; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.spacetelescope.org/images/heic0506b/</span></a></div>
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<strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;"><span style="font-family: Arial, Helvetica, sans-serif;">Credit:</span></strong></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nasa.gov/" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a>, <a href="http://www.esa.int/" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA</a>, and The Hubble Heritage Team <a href="http://www.stsci.edu/" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">AURA</a>)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Appearing like a winged fairy-tale creature poised on a pedestal, this object is actually a billowing tower of cold gas and dust rising from a stellar nursery called the Eagle Nebula. The soaring tower is 9.5 light-years or about 90 trillion kilometres high, about twice the distance from our Sun to the next nearest star.</span></div>
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<span style="line-height: 16px; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>Hubble peers deeply into the Eagle Nebula</b></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><img src="http://www.spacetelescope.org/static/archives/images/screen/potw1033a.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><strong style="border: 0px; margin: 0px 0px 15px; outline: 0px; padding: 0px; vertical-align: baseline;">Credit: </strong>ESA/Hubble & NASA</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The NASA/ESA Hubble Space Telescope has once more turned its attention towards the magnificent Eagle Nebula (Messier 16). This picture shows the northwestern part of the region, well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">The star cluster is very bright and was discovered in the mid-eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed “The Pillars of Creation” ever since the Hubble Space Telescope captured an iconic image of dramatic pillars of star-forming gas and dust.</span></div>
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<span class="watch-title yt-uix-expander-head" dir="ltr" id="eow-title" style="-webkit-user-select: auto; border: 0px; cursor: auto; margin: 0px; padding: 0px;" title="Pillars Of Creation"><span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Pillars Of Creation - VÍDEO</span></span></h1>
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<a href="https://www.youtube.com/watch?v=9D9q-7lqZdc" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">https://www.youtube.com/watch?v=9D9q-7lqZdc</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Saiba mais sobre</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>As Constelações Serpens Cauda e Serpens Caput</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">acessando meu Trabalho em</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/serpens-serpente.html</span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background: none; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background: none; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background: none; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
<dl style="color: #252525; font-family: sans-serif; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;">"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></dd><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;"><br /></dd></dl>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> - AS CONSTELAÇÕES - </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> entre o céu e a terra..., </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vagarosamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> e este por nossa mente sendo conscientizado.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-8168818285841492452014-09-06T10:22:00.003-07:002015-04-05T09:22:48.043-07:00Scutum<div class="MsoNormal" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: -webkit-center;">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Escudo, Scutum, é uma constelação interessante</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pois que não exatamente faz parte do Zodíaco</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mas está sempre acolhendo a Lua e Planetas e Planetóides</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(neste momento - e já por algum bom tempo -, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Scutum vem <i>praticamente</i> </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(em sua fronteira com o Sagitário)</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> abrigando </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Plutão, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">aquele que já foi rei (Planeta) e que jamais perde sua majestade.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Leia mais em</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> http://oceudomes.blogspot.com.br/2014/07/lua-plutao-e-new-horizons.html).</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Scutum, o Escudo, é abrigado, digamos assim, por apenas três constelações,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quer dizer, de um lado existe o imenso Serpentário, Ophiucus, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e a parte da Cauda da Serpente;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ao norte, encontramos a belíssima Águia, Aquila;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, finalmente, ao sul o Escudo pode sempre tomar seu chá das cinco</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">junto ao Bule de Chá que o Sagitário, o Arqueiro, apresenta.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Veja os Objetos Messier</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em Sagitário: </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/objetos-messier-em-sagitario.html</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em Ophiucus, o Serpentário:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m9-m10-m12-m14-m19-m62-e-m107-os.html</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em Serpens, a Serpente:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m5-e-m16-os-objetos-messier-em-serpens.html</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(em Águia não existem objetos messier).</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Scutum, o Escudo, é uma constelação que homenageia um rei,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma herança a todos nós legada até os dias de hoje.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em Scutum, o Escudo, vamos encontrar</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o famoso Aglomerado do Pato Selvagem, M11,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem como o Objeto Messier 26.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><br />
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http://www.stellarium.org/pt/</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Pata selvagem/domesticada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas - </span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">photo by Janine</span></div>
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<span style="line-height: 22.3999996185303px;"> http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><b><span style="color: #660000;">SCUTUM, O ESCUDO</span></b><span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Ascensão Reta 18h18m / 18h56m Declinação -4<sup>o</sup>.0 / -16<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">História:<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Constelação formada por Hevelius em 1690 em honra ao rei da Polônia.<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Fronteiras:<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;">Scutum situa-se entre as constelações Sagittarius, Aquila, Serpens</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">http://en.wikipedia.org/wiki/John_III_Sobieski#mediaviewer/File:Scutum_Sobiescianum.PNG</span></span></div>
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Scutum Sobiescianum</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">Johannes Hevelius</span> - <span class="mw-mmv-source"><a class="external text" href="http://contentdm.lindahall.org/cdm4/document.php?CISOROOT=/star_atlas&CISOPTR=479" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Atlas Coelestis</a>. Johannes Hevelius drew the constellation in Uranographia, his celestial catalogue in 1690.</span></span></div>
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<a href="https://www.blogger.com/null" name="m81">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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Messier 11</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M11 (NGC 6705)</i>, type 'g', in <a href="http://messier.obspm.fr/map/Sct.html">Scutum</a></center>
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<br /><b><span style="font-size: large;">Wild Duck Cluster</span></b><br /><b><span style="font-size: large;"><br /></span></b><div style="font-size: medium;">
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<a href="http://messier.obspm.fr/Jpg/m11.jpg"><img align="right" alt="[m11.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m11.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">18 : 51.1 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-06 : 16 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">6.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">14.0 (arc min)</td></tr>
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Discovered 1681 by Gottfried Kirch.</div>
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Messier 11 (M11, NGC 6705) is "One of the richest and most compact of the galactic (open) clusters," to say it with Robert Burnham, Jr. ..............................</div>
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M11 was discovered by the German astronomer <a href="http://messier.obspm.fr/xtra/Bios/kirch.html">Gottfried Kirch</a> of the Berlin observatory in 1681. It was apparently first resolved into stars by <a href="http://messier.obspm.fr/xtra/similar/derham.html">William Derham</a> about 1733. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included it in <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M11">his catalog</a> on May 30, 1764.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m011.html</div>
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http://www.stellarium.org/pt/</div>
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<span style="color: #252525; font-family: sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;">M11 - NGC 6705 - Aglomerado Aberto, o Pato Selvagem</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Um dos aglomerados mais interessantes e ricos. </span><br />
<span style="font-family: Arial, sans-serif;">É visível na extremidade norte da Nuvem de Estrelas em Scutum, </span><br />
<span style="font-family: Arial, sans-serif;">que é parte da Via Láctea e muito mais distante do que M11.</span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 18h50 Declinação -06<sup>o</sup>.08<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude fotográfica global 6,8 Magnitude fotográfica da mais brilhante estrela 12,0<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;"> Distância kpc 1,70 Diâmetro 13’ Tipo Espectral B8<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjxAPYgVgmteHvTxp3j9d0-Sy8KWCPnEkAfFInuNZzsn0HG455TdiBs0b_jYiO-duBpEEyBYUTU8ggmAM7ENakBMlElHu0TWijXiM4a28eWzaRQXlgd2MVy7QzHrC4cqq30DFGIZFhqTNk/s1600/Messier11.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjxAPYgVgmteHvTxp3j9d0-Sy8KWCPnEkAfFInuNZzsn0HG455TdiBs0b_jYiO-duBpEEyBYUTU8ggmAM7ENakBMlElHu0TWijXiM4a28eWzaRQXlgd2MVy7QzHrC4cqq30DFGIZFhqTNk/s1600/Messier11.jpg" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem#mediaviewer/Ficheiro:Messier11.jpg</div>
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<span style="color: #660000;">O <b>Aglomerado do Pato Selvagem</b> (Messier 11, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 6705</a>)</span><span style="color: #252525;"> é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Scutum">Escudo</a>. Foi descoberto pelo astrônomo alemão<a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a> em 1681, e o francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> incluiu o objeto em seu catálogo em 1764.</span></div>
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É um dos mais ricos e compactos aglomerados abertos conhecidos, contendo cerca de 2 900 estrelas. Sua idade é estimada em cerca de 220 milhões de anos e seu nome deriva-se de suas estrelas mais brilhantes, que formam um triângulo que podem representar um bando de <a href="http://pt.wikipedia.org/wiki/Pato" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pato">patos</a> em formação de voo. Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,3, sendo visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> apenas sob excelentes condições de observação. Suas estrelas mais brilhantes podem ser observadas em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>. Situa-se a 6 200 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</div>
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O <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> foi descoberto pelo astrônomo alemão <a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a>, no <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Observat%C3%B3rio_de_Berlim&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Observatório de Berlim (página não existe)">observatório de Berlim</a> em 1681. Suas estrelas mais brilhantes foram <a href="http://pt.wikipedia.org/wiki/Resolu%C3%A7%C3%A3o_de_imagem" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Resolução de imagem">resolvidas</a> por <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a> em 1733. Foi listado por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> como a décima primeira entrada de seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> em 30 de maio de 1764.<span class="reference" id="cite_ref-seds_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<table cellpadding="0" cellspacing="2" class="infobox" style="background: rgb(242, 242, 242); border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-size: 11px; margin: 0px 0px 1em 1em; padding: 0.2em; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Aglomerado do Pato Selvagem</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier11.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 11"><img alt="Messier 11" data-file-height="387" data-file-width="516" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/da/Messier11.jpg/250px-Messier11.jpg" height="188" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/da/Messier11.jpg/375px-Messier11.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/da/Messier11.jpg/500px-Messier11.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 11</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Gottfried_Kirch" style="background: none; color: #0b0080; text-decoration: none;" title="Gottfried Kirch">Gottfried Kirch</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1681" style="background: none; color: #0b0080; text-decoration: none;" title="1681">1681</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scutum" style="background: none; color: #0b0080; text-decoration: none;" title="Scutum">Scutum</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">18<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 51<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 06,00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-06° 16′ 00,0″</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">6 200 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (1.9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,3</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">14',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">220 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6705</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado do Pato Selvagem"><img alt="Aglomerado do Pato Selvagem" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scutum_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Scutum constellation map.png" data-file-height="1709" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/250px-Scutum_constellation_map.png" height="239" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/375px-Scutum_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/500px-Scutum_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem">http://pt.wikipedia.org/wiki/Aglomerado_do_Pato_Selvagem</a></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px; line-height: 22.3999996185303px;">http://www.ipac.caltech.edu/2mass/gallery/m26atlas.jpg</span></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 26</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M26 (NGC 6694)</i>, type 'f', in <a href="http://messier.obspm.fr/map/Sct.html">Scutum</a></center>
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<a href="http://messier.obspm.fr/Jpg/m26.jpg"><img align="right" alt="[m26.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m26.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">18 : 45.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-09 : 24 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">5.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.0 (mag)</td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">15.0 (arc min)</td></tr>
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Discovered by Charles Messier in 1764.</div>
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Open cluster Messier 26 (M26, NGC 6694) is not so impressive as its apparent neighbor, <a href="http://messier.obspm.fr/m/m011.html">M11</a>. Its discoverer <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M26">cataloged it</a> on June 20, 1764, even noted that it was "not distinguished in a 3.5 foot (FL) telescope and needed a better instrument."</div>
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LEIA MAIS</div>
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em</div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px; line-height: 22.3999996185303px;">http://messier.obspm.fr/m/m026.html</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhE0dd2TuPmYB1k0jeYOXR72FEbpc4Z8D5CF2t59WdUAli32zK6f9Xtz4wTN8Qk1wJnKUJDTeVwoKuIlv7M65n3d9vikP-WGk-76wsn91BbFqO7N4R7cOsZsVtIGfH1e-7UjNXqSQ5Wb-Q/s1600/m26.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhE0dd2TuPmYB1k0jeYOXR72FEbpc4Z8D5CF2t59WdUAli32zK6f9Xtz4wTN8Qk1wJnKUJDTeVwoKuIlv7M65n3d9vikP-WGk-76wsn91BbFqO7N4R7cOsZsVtIGfH1e-7UjNXqSQ5Wb-Q/s1600/m26.png" /></a></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></span><br />
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<span style="color: #660000;"><b>Messier 26</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 6694</a>)</span><span style="color: #252525;"> é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a>, integrante do <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">Catálogo Messier</a>. Ésta localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scutum" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Scutum">Escudo</a> e foi descoberto por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>em <a href="http://pt.wikipedia.org/wiki/1764" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1764">1764</a>.</span></div>
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O aglomerado estende-se por 22 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> e está a uma distância de 5 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Sua estrela mais brilhante tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 11,9 e tem aproximadamente 89 milhões de anos..</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 26</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_026_2MASS.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 26, projeto 2MASS"><img alt="Messier 26, projeto 2MASS" data-file-height="1204" data-file-width="842" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Messier_026_2MASS.jpg/250px-Messier_026_2MASS.jpg" height="357" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Messier_026_2MASS.jpg/375px-Messier_026_2MASS.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Messier_026_2MASS.jpg/500px-Messier_026_2MASS.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 26, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scutum" style="background: none; color: #0b0080; text-decoration: none;" title="Scutum">Scutum</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">Aglomerado estelar aberto</a> (II,2,r)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">18<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 45<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 12,00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-9° 24′ 00,0″</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">5 000 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (1 533 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">8,0</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">15',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">22 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">89 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6694</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scutum_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Scutum constellation map.png" data-file-height="1709" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/250px-Scutum_constellation_map.png" height="239" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/375px-Scutum_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/22/Scutum_constellation_map.png/500px-Scutum_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<b>Com um abraço estrelado,</b><br /><b>Janine Milward</b><br /><br /><br /><br /><div style="line-height: 1.4;">
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background: none; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background: none; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background: none; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background: none; color: #0b0080; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="background-color: white; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></span></div>
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<br /><span style="font-family: Arial, Helvetica, sans-serif;"><b>CARO LEITOR,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">devem requerer do Caro Leitor</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Visitando os Sites abaixo,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<b><o:p></o:p></b></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"><b>Janine Milward</b></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>VISITE MINHA PÁGINA</b><o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #274e13;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></b><o:p></o:p></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEivDYxknWerbIYDnEbmKvxZbzpB2Ebsv97uMUIt4tAyAvDfVwmYx5ZQsbr_DtJgrlIGvkv-g6P54r1v4J-zZxOKvO2u63g2ar3r45vJxncw0Riu7usLLxjfkoCaFoqMi6iYtI75BWo0k1g/s1600/P23-07-14_14.55.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEivDYxknWerbIYDnEbmKvxZbzpB2Ebsv97uMUIt4tAyAvDfVwmYx5ZQsbr_DtJgrlIGvkv-g6P54r1v4J-zZxOKvO2u63g2ar3r45vJxncw0Riu7usLLxjfkoCaFoqMi6iYtI75BWo0k1g/s1600/P23-07-14_14.55.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Pata selvagem/domesticada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">no Sítio das Estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">photo by Janine</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><b>http://www.eso.org/public/archives/images/screen/eso1430a.jpg</b></span></span></div>
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The Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile has taken this beautiful image of the open Wild Duck Cluster, Messier 11, or NGC 6705. The blue stars in the centre of the image are the young, hot stars of the cluster. The surrounding redder stars are older, cooler background stars.</div>
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ESO</div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-19025328344182710822014-09-06T10:21:00.001-07:002015-04-05T09:21:21.773-07:00Scorpius<div class="MsoNormal" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: -webkit-center;">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação do Escorpião</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sempre atrai a atenção</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de nossos olhos, de nossa mente e de nosso coração,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não é verdade?</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma constelação, um figuração de estrelas agrupadas, um asterismo</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">desenhando um animal rastejante</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, sem dúvida alguma, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não existe quem ali não veja um Escorpião desenhado por estrelas!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Estaremos visitando</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M80, Objeto Messier próximo às Garras (ou Cabeça) da</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">constelação do Escorpião;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M4, Objeto Messier próximo ao Coração;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M6 e M7, Objetos Messier próximos à Cauda.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em lugares de céus escuros e transparentes</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e em noites de ausência de Lua,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">certamente podemos observar os Objetos Messier M6 e M7</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a olho nu </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- às vezes, precisamos do auxílio da visão enviesada.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aliás, para testar a boa visão dos Caminhantes,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">lhes digo que muito antigamente, muito antigamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">serviam os dois objetos maravilhosos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que se apresentam quase na fronteira entre o Escorpião e o Sagitário</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e bem direcionados para a região que nos leva ao centro da Galáxia:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Messier 6 e Messier 7,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aglomerados Abertos Borboleta e Ptolomeu, respectivamente.</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">Com um abraço estrelado,</span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif;"><span style="font-size: 15px;">Janine Milward</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi6nPK_0Hlh7q5FAE2NACaE3jA1hL1aFA3nU3CvisGa_7Pv2vdTY1YSL7gYh2RJcmUMkjRbhPHwRkPepPnklTpNdNeX__LTmA8JnozScRm6USRuwbZI5A9dzaV54MpwKWid92j8yGeQyYY/s1600/scorpio_guisard_1328.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi6nPK_0Hlh7q5FAE2NACaE3jA1hL1aFA3nU3CvisGa_7Pv2vdTY1YSL7gYh2RJcmUMkjRbhPHwRkPepPnklTpNdNeX__LTmA8JnozScRm6USRuwbZI5A9dzaV54MpwKWid92j8yGeQyYY/s1600/scorpio_guisard_1328.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><b>http://apod.nasa.gov/apod/ap140504.html</b></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgvWUvQMq7vhWhqAmDGwIRJAL4CKXB1-o2vf8Fds0mPHI_wsDbX6MCcy9Ud6DyX9jOXaDEb7jh9pLmieoXJ-Vf5eiaTgNxjFPYMURBHuM8emofPbRWLaq9DjDJql_N_wRZWKvpGAGVAQ8w/s1600/scorpio_guisard_constellation_960.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgvWUvQMq7vhWhqAmDGwIRJAL4CKXB1-o2vf8Fds0mPHI_wsDbX6MCcy9Ud6DyX9jOXaDEb7jh9pLmieoXJ-Vf5eiaTgNxjFPYMURBHuM8emofPbRWLaq9DjDJql_N_wRZWKvpGAGVAQ8w/s1600/scorpio_guisard_constellation_960.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #274e13;"><b><span style="font-family: Arial, Helvetica, sans-serif;">A Scorpius Sky Spectacular </span></b><br /><span style="font-size: small;"><b>Image Credit & Copyright: </b><a href="http://sguisard.astrosurf.com/" style="color: #274e13; text-decoration: none;">Stéphane Guisard</a>, <a href="http://www.twanight.org/newTWAN/index.asp" style="color: #274e13; text-decoration: none;">TWAN</a></span></span></center>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>If Scorpius looked this good to the unaided eye, humans might remember it better. <a href="http://www.allthesky.com/constellations/scorpius/" style="color: #274e13; text-decoration: none;">Scorpius</a> more typically appears as a few bright stars in a well-known but rarely pointed out <a href="http://en.wikipedia.org/wiki/Zodiac" style="color: #274e13; text-decoration: none;">zodiacal</a> <a href="http://modernconstellations.com/constellationhistory.html" style="color: #274e13; text-decoration: none;">constellation</a>. To get a spectacular image like <a href="http://astrosurf.com/sguisard/Pagim/Scorpius_constellation-LHRVB-50mm.html" style="color: #274e13; text-decoration: none;">this</a>, though, one needs a good <a href="http://electronics.howstuffworks.com/digital-camera.htm" style="color: #274e13; text-decoration: none;">camera</a>, color <a href="http://en.wikipedia.org/wiki/Filter_%28optics%29" style="color: #274e13; text-decoration: none;">filters</a>, and a digital image processor. To bring out detail, the <a href="http://astrosurf.com/sguisard/Pagim/Scorpius_constellation-LHRVB-50mm.html" style="color: #274e13; text-decoration: none;">above image</a> not only involved long duration exposures taken in several colors, but one exposure in a <a href="http://apod.nasa.gov/apod/ap050930.html" style="color: #274e13; text-decoration: none;">very specific red color</a> emitted by <a href="http://periodic.lanl.gov/1.shtml" style="color: #274e13; text-decoration: none;">hydrogen</a>. The <a href="http://astrosurf.com/sguisard/Pagim/Scorpius_constellation-LHRVB-50mm.html" style="color: #274e13; text-decoration: none;">resulting image</a> shows many breathtaking features. Vertically across the image left is part of the <a href="http://apod.nasa.gov/apod/ap050605.html" style="color: #274e13; text-decoration: none;">plane</a> of our <a href="http://en.wikipedia.org/wiki/Milky_Way" style="color: #274e13; text-decoration: none;">Milky Way Galaxy</a>. Visible there are vast clouds of bright stars and long filaments of dark <a href="http://apod.nasa.gov/apod/ap030706.html" style="color: #274e13; text-decoration: none;">dust</a>. Jutting out diagonally from the <a href="http://apod.nasa.gov/apod/ap070123.html" style="color: #274e13; text-decoration: none;">Milky Way</a> in the image center are dark dust bands known as the <a href="http://apod.nasa.gov/apod/ap090708.html" style="color: #274e13; text-decoration: none;">Dark River</a>. This river connects to several bright stars on the right that are part of <a href="http://www.ianridpath.com/startales/scorpius.htm" style="color: #274e13; text-decoration: none;">Scorpius' head and claws</a>, and include the bright star <a href="http://stars.astro.illinois.edu/sow/antares.html" style="color: #274e13; text-decoration: none;">Antares</a>. Above and right of Antares is an even brighter planet Jupiter. Numerous red <a href="http://apod.nasa.gov/apod/emission_nebulae.html" style="color: #274e13; text-decoration: none;">emission nebulas</a> and blue <a href="http://en.wikipedia.org/wiki/Reflection_nebula" style="color: #274e13; text-decoration: none;">reflection nebulas</a> are visible throughout the image.<a href="http://en.wikipedia.org/wiki/Scorpion" style="color: #274e13; text-decoration: none;">Scorpius</a> appears prominently in southern skies after sunset during the middle of the year.</span></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><b>Mario Jaci Monteiro - As Constelações, Cartas Celestes</b></span></span><br />
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;"><span style="font-size: medium;">SCORPIUS, O ESCORPIÃO</span></span><span style="color: #0f243e; font-size: 11pt;"><o:p></o:p></span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o escorpião morto por Orion.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os poetas gregos nos ensinavam que Scorpius foi o animal enviado por Diana para matar Orion, que intervinha nas atividades da caçadora, mas ele nunca conseguia atingir a sua meta: realmente, as estrelas de Orion desaparecem no ocidente justamente quando o Escorpião nasce no oriente.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Segundo alguns autores, sua origem deve associar-se às secas e às pragas que assolavam o Egito quando o Sol se encontrava naquela região do céu.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Desde a mais remota antiguidade, esta constelação foi representada pelos gregos, latinos, árabes e persas pela figura de um escorpião.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O equinócio de outono, há 3000 aC, localizava-se aí, quando este asterismo foi instituído. Na Pérsia, Antares, a estrela mais brilhante do Escorpião, era uma das quatro “Estrelas Reais”, uma das guardiãs do céu e, naquela época, indicava o outono.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Scorpius situa-se entre Libra, Lupus, Norma, Ara, Corona Australis, Sagittarius, Ophiucus, Serpens<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M80, Objeto Messier próximo às Garras (ou Cabeça) da</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">constelação do Escorpião;</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M4, Objeto Messier próximo ao Coração;</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M6 e M7, Objetos Messier próximos à Cauda.</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://media.skysurvey.org/interactive360/index.html" style="color: #274e13; text-decoration: none;">http://media.skysurvey.org/interactive360/index.html</a></span></div>
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<b><span style="color: #660000;">Caro Leitor,</span></b></div>
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<b><span style="color: #660000;">inicialmente, estaremos visitando</span></b></div>
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<b><span style="color: #660000;">os Objetos Messier</span></b></div>
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<b><span style="color: #660000;">próximos às Garras (ou à Cabeça)</span></b></div>
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<b><span style="color: #660000;">- M80 -</span></b></div>
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<b><span style="color: #660000;">e ao Coração</span></b></div>
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<b><span style="color: #660000;">- M4 -</span></b></div>
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<b><span style="color: #660000;">do Escorpião:</span></b></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgdsxa6Ml8LXeGz9k7NglFE8tjaJrGUCLL6sCHhlsiiKy2I-tXIlTsm206EeGM8biyFrVVEx9U4m9OOVBhz2jjw6t5Kwl-Fy5GOjETW7Ai7mjvdE_KKjRJRrcbKVi6ri5zktEPA0ZFUcfI/s1600/M4+e+M80.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgdsxa6Ml8LXeGz9k7NglFE8tjaJrGUCLL6sCHhlsiiKy2I-tXIlTsm206EeGM8biyFrVVEx9U4m9OOVBhz2jjw6t5Kwl-Fy5GOjETW7Ai7mjvdE_KKjRJRrcbKVi6ri5zktEPA0ZFUcfI/s1600/M4+e+M80.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Excerto da Carta Celeste Escorpião - Mario Jaci Monteiro</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As Garras ou a Cabeça</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são as estrelas que delineiam o começo da constelação do Escorpião</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e por onde a Linha da Eclíptica passa.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjS_20C5opTznnNwTZeriJy2sheNiOkN7lKGW6VU5koCysIP2N1Q76d5sszUbDzdLmr2jf1oyHDHUNa2adAE1CNEaAAmSrxKFLqbE95qhBreAve6vy4KGqr7-oJxsWXy7p8ZEjJ7PDATcw/s1600/a+cabe%C3%A7a.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjS_20C5opTznnNwTZeriJy2sheNiOkN7lKGW6VU5koCysIP2N1Q76d5sszUbDzdLmr2jf1oyHDHUNa2adAE1CNEaAAmSrxKFLqbE95qhBreAve6vy4KGqr7-oJxsWXy7p8ZEjJ7PDATcw/s1600/a+cabe%C3%A7a.jpg" height="370" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Antigamente, muito antigamente, as duas estrelas ponteadoras da Balança</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">era consideradas como As Garras do Escorpião - e isso faz sentido,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">quando as vemos no céu estrelado!).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">AS GARRAS</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">E/OU</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">A CABEÇA DO ESCORPIÃO</span></b></div>
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<b><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">acolhendo o Objeto Messier 80</span></b></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;">http://www.ipac.caltech.edu/2mass/gallery/m80atlas.jpg</span></span></div>
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<h1>
Messier 80</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M80 (NGC 6093)</i>, class II, in <a href="http://messier.obspm.fr/map/Sco.html">Scorpius</a></center>
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<a href="http://messier.obspm.fr/Jpg/m80.jpg"><img align="right" alt="[m80.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m80.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0" style="color: #073763; font-family: 'Times New Roman';"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">16 : 17.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-22 : 59 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">32.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">10.0 (arc min)</td></tr>
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Discovered 1781 by Charles Messier.</div>
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Messier 80 (M80, NGC 6093) is a fine 8th mag globular. Its 10' angular diameter corresponds to roughly 95 light years linear dimension at its distance of 32,600 light years. Its appearance resembles very much that of a faint comet without tail.</div>
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This dense stellar swarm contains several 100,000s of stars, held together by their mutual gravitational attraction. It is one of the densest globulars in our <a href="http://messier.obspm.fr/more/mw.html">Milky Way Galaxy</a>. As was found by astronomers from <a href="http://messier.obspm.fr/more/m080_hst.html">observations with the Hubble Space Telescope</a> in 1999 in the visible and UV part of the electromagnetic spectrum, M80 contains a large number of so-called "Blue Stragglers" in its core, about twice as much as any other globular investigated with the HST. These stars are blue and bright stars which appear near the main-sequence of the Hertzsprung-Russell diagramm, and thus appear more massive and younger than the globular clusters age. The reason is very probably that these stars lost their cooler envelopes in close encounters with other stars. Their large number in M80 indicates an exceptionally high stellar collision rate in the core of this globular cluster.</div>
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Globular cluster M80 was one of the original discoveries of <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who found it on January 4, 1781, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M80">cataloged it</a> as a "Nebula without a star, .. resembling the nucleus of a comet." <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> was the first to resolve it (before 1785), and found it was "one of the richest and most compressed clusters of small stars I remember to have seen."</div>
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LEIA MAIS</div>
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<a href="http://messier.obspm.fr/m/m080.html">http://messier.obspm.fr/m/m080.html</a></div>
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Stellarium</div>
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;">NGC 6093 - M 80 - Aglomerado Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;">Ascensão Reta 16h15 Declinação -22<sup>o</sup>.56<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Magnitude fotográfica global 8,4 Diâmetro aparente 5’,1 Tipo Espectral F4<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif;">Distância kpc 11,0 Velocidade Radial (km/s) + 18</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #073763;"><b style="font-family: sans-serif; text-align: start;">Messier 80</b><span style="font-family: sans-serif; text-align: start;"> (também conhecido como </span><b style="font-family: sans-serif; text-align: start;">M80</b><span style="font-family: sans-serif; text-align: start;"> ou </span><b style="font-family: sans-serif; text-align: start;">NGC 6093</b><span style="font-family: sans-serif; text-align: start;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="font-family: sans-serif; text-align: start;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="font-family: sans-serif; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Scorpius">Scorpius</a><span style="font-family: sans-serif; text-align: start;"> a 32 600 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="font-family: sans-serif; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="font-family: sans-serif; text-align: start;">. Foi descoberto por</span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="font-family: sans-serif; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="1781">1781</a><span style="font-family: sans-serif; text-align: start;">. Possui um raio de 47,5 anos-luz e uma dimensão aparente de 10,0 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="font-family: sans-serif; text-align: start;">.</span><span class="reference" id="cite_ref-seds_2-4" style="bottom: 1ex; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none; white-space: nowrap;">2</a></span></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 80</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Imagem de Messier 80 tirada pelo Telescópio Espacial Hubble. Crédito: HST/NASA/ESA"><img alt="Imagem de Messier 80 tirada pelo Telescópio Espacial Hubble. Crédito: HST/NASA/ESA" data-file-height="1864" data-file-width="1777" src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/6a/A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg/250px-A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg" height="262" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/6a/A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg/375px-A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/6a/A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg/500px-A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Imagem de Messier 80 tirada pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a>.<br />
Crédito: HST/<a href="http://pt.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/ESA" style="background: none; color: #0b0080; text-decoration: none;" title="ESA">ESA</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1781" style="background: none; color: #0b0080; text-decoration: none;" title="1781">1781</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; color: #0b0080; text-decoration: none;" title="Scorpius">Scorpius</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">16<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 02,4<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-22° 58′ 33,9″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">32 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (10 000 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">7,87<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">10,0 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background: none; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">Classe</a></td><td style="background-color: #f8f8f8;">II<span class="reference" id="cite_ref-seds_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">47,5<span class="reference" id="cite_ref-seds_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M80, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6093, GC1 39.<span class="reference" id="cite_ref-simbad_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_80#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 80"><img alt="Messier 80" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scorpius_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Scorpius constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/250px-Scorpius_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/375px-Scorpius_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/500px-Scorpius_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="color: #274e13;"><a href="http://pt.wikipedia.org/wiki/Messier_80#mediaviewer/Ficheiro:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_80#mediaviewer/Ficheiro:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O Coração, como todos sabemos,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é a estrela-alpha Scorpii, Antares,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">maravilhosamente avermelhada/alaranjada</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e sempre rivalizando com Marte, o Planeta Vermelho -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">daí ser chamada de Anti-Ars, ou Antares </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Ares ou Ars é o nome grego para Marte).</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<b style="line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">O CORAÇÃO DO ESCORPIÃO</span></b></div>
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<b style="line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">acolhendo o Objeto Messier 4</span></b></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://nexusnow.info/forum/showthread.php?13982-Star-of-the-week-Antares-is-Heart-of-the-Scorpion" style="color: #274e13; text-decoration: none;">http://nexusnow.info/forum/showthread.php?13982-Star-of-the-week-Antares-is-Heart-of-the-Scorpion</a></span></div>
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<a href="mailto:stargazerbob@aol.com" style="color: #274e13; text-align: left;"><span style="font-family: Arial, Helvetica, sans-serif;">stargazerbob@aol.com</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Antares.</b><b> Alpha Scorpii. Estrela Dupla e Variável</b></span><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h28,2m - Declinação -26<sup>o</sup> 23’<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,22 - Distância 520 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,1 e 6,5 Distância entre estrelas 2”,90<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Uma estrela binária, intensamente avermelhada e verde-esmeralda, situada no corpo do Escorpião. De Anti-Ares, similar ou Rival de Ares, Marte. Foi uma das quatro estrelas reais da Pérsia, cerca de 3.000 anos a.c., e atuava como a Guardiã do Oeste pois marcava o Equinócio de Outono. Muitas vezes chamada de Coração do Escorpião, Cor Scorpio.<span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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Messier 4</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M4 (NGC 6121)</i>, class IX, in <a href="http://messier.obspm.fr/map/Sco.html">Scorpius</a></center>
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<a href="http://messier.obspm.fr/Jpg/m4.jpg"><img align="right" alt="[m4.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m4.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">16 : 23.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-26 : 32 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">7.2 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">36.0 (arc min)</td></tr>
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Discovered by Philippe Loys de Chéseaux in 1746.</div>
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Messier 4 (M4, NGC 6121) is one of the nearest globular clusters in the sky at an estimated distance of about 7,200 light years. Situated prominently about 1.3 degrees west of Antares, in constellation <a href="http://messier.obspm.fr/map/Sco.html">Scorpius</a>, and being as bright as mag 5.6 visually, it can be detected by the naked eye under very dark skies, and is prominent with the slightest optical aid.</div>
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Globular cluster M4 was discovered by <a href="http://messier.obspm.fr/xtra/Bios/decheseaux.html">De Chéseaux</a> in 1745-46 and <a href="http://messier.obspm.fr/xtra/similar/deches.html">listed by him</a> as No. 19, and included in <a href="http://messier.obspm.fr/xtra/Bios/lacaille.html">Lacaille</a>'s <a href="http://messier.obspm.fr/xtra/history/lacaille.html">catalog</a> as Lacaille I.9. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M4">cataloged it</a> on May 8, 1764 and was the first to resolve it into a "cluster of very small [faint] stars;" this is the only globular cluster he could resolve with his moderate instruments, and thus the first globular cluster ever to be resolved. Only about 20 years later, William Herschel was able to resolve all Messier globulars with his large telescopes.</div>
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LEIA MAIS</div>
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em</div>
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<a href="http://messier.obspm.fr/m/m004.html">http://messier.obspm.fr/m/m004.html</a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhqb6pQrtAmCDkCBYpgweodQcT4fS8SMttLp3_x3tIHK7n1v_b8VqRKFcgzhFr0gTex9IIgUVN0viTHaor5Lm3rHy18mh1bVP1DowNQ-_1687vdygi4d8aPHFcof6zhwBkJ42jvBwZ9Hvk/s1600/M4.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhqb6pQrtAmCDkCBYpgweodQcT4fS8SMttLp3_x3tIHK7n1v_b8VqRKFcgzhFr0gTex9IIgUVN0viTHaor5Lm3rHy18mh1bVP1DowNQ-_1687vdygi4d8aPHFcof6zhwBkJ42jvBwZ9Hvk/s1600/M4.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M 4 - NGC 6121 - Scorpius - Aglomerado Estelar Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h22m Declinação -26<sup>o</sup>.27<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,1 Tipo AG</span><span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px;"><a href="http://pt.wikipedia.org/wiki/Messier_4#mediaviewer/Ficheiro:Messier_4_Hubble_WikiSky.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_4#mediaviewer/Ficheiro:Messier_4_Hubble_WikiSky.jpg</a></span></span></div>
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<span class="mw-mmv-title" style="font-size: 1.2em; max-width: 60%; overflow: hidden; text-overflow: ellipsis;"><span style="color: #274e13;">Messier 4 Hubble WikiSky</span></span></div>
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<b style="color: #660000;">Messier 4</b><span style="color: #660000;"> (</span><span style="color: #073763;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC 6121</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">constela</a><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">ção</a> de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>, descoberto pelo astrônomo suíço <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Foi catalogado pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764, que foi o primeiro a reconhecer o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Objeto astronômico">objeto astronômico</a> como um aglomerado globular, o primeiro descoberto da história.</span></div>
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<span style="color: #073763;">Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 7,1, não sendo possível observá-lo a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; text-decoration: none;" title="Olho nu">olho nu</a>, mas com o uso de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; text-decoration: none;" title="Binóculo">binóculos</a> e pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; text-decoration: none;" title="Telescópio">telescópios</a> é possível identificá-lo como uma pequena mancha nebulosa e difusa. Suas estrelas mais brilhantes são vistas apenas com o uso de telescópios maiores. Está a uma distância de cerca de 33 900 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; text-decoration: none;" title="Terra">Terra</a> e sua idade foi estimada em 12,2 bilhões de anos. Localiza-se a apenas 1,3° a leste de <a href="http://pt.wikipedia.org/wiki/Antares" style="background: none; text-decoration: none;" title="Antares">Antares</a>, a estrela amarelada e a mais brilhante da constelação de<a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; text-decoration: none;" title="Scorpius">Escorpião</a>.</span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 4</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_4_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 4 visto pelo Telescópio Espacial Hubble."><img alt="Messier 4 visto pelo Telescópio Espacial Hubble." data-file-height="4200" data-file-width="4200" src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/cf/Messier_4_Hubble_WikiSky.jpg/250px-Messier_4_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/cf/Messier_4_Hubble_WikiSky.jpg/375px-Messier_4_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/cf/Messier_4_Hubble_WikiSky.jpg/500px-Messier_4_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 4 visto pelo Telescópio Espacial Hubble.</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1746" style="background: none; color: #0b0080; text-decoration: none;" title="1746">1746</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; color: #0b0080; text-decoration: none;" title="Scorpius">Scorpius</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;">IX</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">16<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 23<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 35,41<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-26° 31′ 31,9″</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">7 200 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (2,2 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">7,12</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">36',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">35 anos-luz</td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">12,2 ± 0,2 bilhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6121</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 4"><img alt="Messier 4" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scorpius_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Scorpius constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/250px-Scorpius_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/375px-Scorpius_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/500px-Scorpius_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_4" style="font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_4</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A longa Cauda, sinuosa e insinuante,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">é uma visão quase fantástica, aterradora, aterrorizante!</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi7TjydFxeP-C91-axdjXt-7Jnw1JeVJPkNDCCwM_yTvNn8NNdxOxXHRqAqs17P2qcqHbNKn7qC4wqZUhRgPBUrO-FM9bZtHMHRSTQFHZ_XE9h4KMETMrU1gEOf7zMefr7UvF3egBh5QTM/s1600/a+cauda.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi7TjydFxeP-C91-axdjXt-7Jnw1JeVJPkNDCCwM_yTvNn8NNdxOxXHRqAqs17P2qcqHbNKn7qC4wqZUhRgPBUrO-FM9bZtHMHRSTQFHZ_XE9h4KMETMrU1gEOf7zMefr7UvF3egBh5QTM/s1600/a+cauda.jpg" height="390" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiDNh78oxAd7GMOWmjF2HzRT4VZr79mFoA2FuPP7_he6t3ABkwiR9Apqgv4c4hUanxLd69PssvxziAXvhAUqJi9pz8fx40ayQpQy_gVAT66VBZRecteacvmjYuCx2q71pbXdlBSHDRBcv8/s1600/M6+e+M7.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiDNh78oxAd7GMOWmjF2HzRT4VZr79mFoA2FuPP7_he6t3ABkwiR9Apqgv4c4hUanxLd69PssvxziAXvhAUqJi9pz8fx40ayQpQy_gVAT66VBZRecteacvmjYuCx2q71pbXdlBSHDRBcv8/s1600/M6+e+M7.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">Excerto da Carta Celeste Escorpião - Mario Jaci Monteiro</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">As duas estrelas que finalizam a Cauda e escondem o veneno do animal rastejante</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- Schaula e Lesath - </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são duas joias, dois tesouros, duas ameaças!</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">Finalmente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">para testar a boa visão dos Caminhantes,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">lhes digo que muito antigamente, muito antigamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">serviam os dois objetos maravilhosos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que se apresentam quase na fronteira entre o Escorpião e o Sagitário</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e bem direcionados para a região que nos leva ao centro da Galáxia:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Messier 6 e Messier 7</b>,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Aglomerados Abertos Borboleta e Ptolomeu, respectivamente.</span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Dois Aglomerados Abertos bem próximos um ao outro<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">e facilmente encontrados ao final da cauda do Escorpião:</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><br /></span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M6 - NGC 6405 - Aglomerado Aberto - Aculeus</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Um belo aglomerado aberto bem visível a olho nú ou através pequenos telescópios.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M7 - NGC 6475 - Aglomerado Aberto - Acumen</b><o:p></o:p></span></div>
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<div style="margin: 0px;">
<span style="font-family: Arial, Helvetica, sans-serif;">Um belo aglomerado aberto bem visível a olho nú ou através pequenos telescópios.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 6405 - M 6 - Aglomerado Aberto Scorpius</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h38m Declinação -32<sup>o</sup>.12<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 4,6 Magnitude fotográfica da mais brilhante estrela 8,3<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,45 Diâmetro 26’ Tipo Espectral B4<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>NGC 6475 - M 7 - Aglomerado Aberto Scorpius</b><o:p></o:p></span></div>
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<div style="margin: 0px;">
<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h52m Declinação -34<sup>o</sup>.48<o:p></o:p></span></div>
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<div style="margin: 0px;">
<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 3,3 Magnitude fotográfica da mais brilhante estrela 7,4<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> Distância kpc 0,23 Diâmetro 50’ Tipo Espectral B5</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://www.ipac.caltech.edu/2mass/gallery/m6atlas.jpg" style="cursor: move;" /></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://www.ipac.caltech.edu/2mass/gallery/m6atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m6atlas.jpg</a></span></span></div>
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<h1 style="font-size: medium;">
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<h1>
<span style="font-size: large;">Messier 6</span></h1>
<i style="font-size: medium;"><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M6 (NGC 6405)</i>, type 'e', in <a href="http://messier.obspm.fr/map/Sco.html" style="font-size: medium;">Scorpius</a></center>
<center style="color: black; font-family: 'Times New Roman'; line-height: normal;">
<b><span style="font-size: large;">Butterfly Cluster</span></b><br /><div style="font-size: medium;">
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<b><br /></b></div>
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</center>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">
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<a href="http://messier.obspm.fr/Jpg/m6.jpg"><img align="right" alt="[m6.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m6.jpg" style="cursor: move;" /></a></div>
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<table border="2" cellpadding="5" cellspacing="0" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><tbody>
<tr><th align="left"><div style="margin: 0px;">
Right Ascension</div>
</th><td align="center"><div style="margin: 0px;">
17 : 40.1 (h:m)</div>
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Declination</div>
</th><td align="center"><div style="margin: 0px;">
-32 : 13 (deg:m)</div>
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Distance</div>
</th><td align="center"><div style="margin: 0px;">
1.6 (kly)</div>
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Visual Brightness</div>
</th><td align="center"><div style="margin: 0px;">
4.2 (mag) </div>
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Apparent Dimension</div>
</th><td align="center"><div style="margin: 0px;">
25.0 (arc min)</div>
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Discovered by Hodierna before 1654.</div>
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Open cluster Messier 6 (M6, NGC 6405) is described by Burnham as a "charming group whose arrangement suggests the outline of a butterfly with open wings."</div>
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Burnham proposes that <a href="http://messier.obspm.fr/xtra/Bios/ptolemy.html">Ptolemy</a>'s mentioning of its apparent neighbor, <a href="http://messier.obspm.fr/m/m007.html">M7</a>, may include M6; however, this proposition is speculative and improbable. The next, and first certain reported observer was <a href="http://messier.obspm.fr/xtra/Bios/hodierna.html">Giovanni Batista Hodierna</a> who <a href="http://messier.obspm.fr/xtra/similar/hodierna.html">has seen it</a>before 1654; but Hodierna's records did not become generally known before the 1980s. Thus, <a href="http://messier.obspm.fr/xtra/Bios/decheseaux.html">Philippe Loys de Chéseaux</a> independently <a href="http://messier.obspm.fr/xtra/similar/deches.html">rediscovered it</a> in 1745-46, and was the first to recognize it as "a very fine star cluster." <a href="http://messier.obspm.fr/xtra/Bios/lacaille.html">Abbe Lacaille</a>included it <a href="http://messier.obspm.fr/xtra/history/lacaille.html">in his catalog</a> of 1751-52 as Lac III.12, and <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> eventually <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M6">cataloged it</a> on May 23, 1764.</div>
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LEIA MAIS</div>
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em</div>
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<br /><a href="http://apod.nasa.gov/apod/image/1410/butterflyblue_hst_3919.jpg"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1410/butterflyblue_hst_960.jpg" style="cursor: move;" /></a></center>
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<b>http://apod.nasa.gov/apod/ap141001.html</b></center>
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<b>The Butterfly Nebula from Hubble </b><br /><b>Image Credit: </b><a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and the <a href="http://hubblesite.org/servicing_mission_4/">Hubble SM4 ERO Team</a>; <b>Reprocessing & Copyright: </b><a href="mailto: Francesco dot antonucci at fastwebnet dot it">Francesco Antonucci</a></center>
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<b>Explanation: </b>The bright clusters and nebulae of planet Earth's night sky are often named for <a href="http://apod.nasa.gov/apod/ap120929.html">flowers</a> or <a href="http://apod.nasa.gov/apod/ap100425.html">insects</a>. Though its wingspan covers over 3 light-years, <a href="http://en.wikipedia.org/wiki/NGC_6302">NGC 6302</a> is no exception. With an estimated surface temperature of about 250,000 degrees C, the dying central star of this particular <a href="http://apod.nasa.gov/apod/ap040207.html">planetary nebula</a> has become exceptionally hot, shining brightly in ultraviolet light but hidden from direct view by a dense torus of dust. This <a href="http://internal.hubblesite.org/newscenter/archive/releases/2009/25/image/f/">sharp close-up</a> of the dying star's nebula was recorded in 2009 by the Hubble Space Telescope's Wide Field Camera 3, and is presented here in reprocessed colors. Cutting across a bright cavity of ionized gas, the dust <a href="http://www.math.tamu.edu/~tkiffe/calc3/revolution3/revolution3.html">torus</a> surrounding the central star is near the center of this view, almost edge-on to the line-of-sight. Molecular hydrogen <a href="http://adsabs.harvard.edu/abs/2005hris.conf..423M">has been detected</a> in the hot star's dusty cosmic shroud. <a href="http://adsabs.harvard.edu/abs/2008MNRAS.385..269M">NGC 6302</a> lies about 4,000 light-years away in the <a href="http://www.arachnology.be/Arachnology.html">arachnologically</a> correct constellation of the Scorpion (<a href="http://hawastsoc.org/deepsky/sco/index.html">Scorpius</a>).</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhzjfRfWlXzq2Bc7RxQhMM8h3xNFbltgiDfQaYDjgqE9kmvm9GK3vQ_-TCyMp1pWAS1rAuPHbOfNjSrAPvWYICNAaqC3D3oLZfmHcaINcDvObb85ywtXgc9DyeMWHGzVN8OGgh_E26D0Ig/s1600/borboleta+-+m+6.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhzjfRfWlXzq2Bc7RxQhMM8h3xNFbltgiDfQaYDjgqE9kmvm9GK3vQ_-TCyMp1pWAS1rAuPHbOfNjSrAPvWYICNAaqC3D3oLZfmHcaINcDvObb85ywtXgc9DyeMWHGzVN8OGgh_E26D0Ig/s1600/borboleta+-+m+6.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Stellarium</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M 6 - NGC 6405 - Scorpius - Aglomerado Estelar Aberto - A Borboleta</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h38m Declinação -32<sup>o</sup>.11<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Para alguns, o desenho do aglomerado aberto M6, também conhecido como NGc 5405, se parece com uma borboleta. M5 espalha-se ao longo de cerca de 20 anos-luz e dista cerca de 2 mil anos-luz de nós. M6 pode bem ser visualizado a olho nú, sempre em lugares de céus escuros e transparentes, porém também um par de binóculos nos apresenta uma bela visão, como se fosse uma lua cheia de estrelas. Como acontece em outros aglomerados abertos, M6 é composto predominantemente de estrelas jovens e azuis, apesar de que a estrela mais brilhante é quase alaranjada. M6 é estimado em ter cerca de 100 milhões de idade. A determinação de aglomerados tais como M6 ajuda os astronomos a calibrarem a escala de distâncias do universo.<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="color: #073763;">O <b>Aglomerado da Borboleta</b> (Messier 6, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC 6405</a>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>. O primeiro astrônomo a registrar a existência do aglomerado foi o italiano <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> em 1654. Entretanto, o astronômo americano <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Robert_Burnham,_Jr.&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Robert Burnham, Jr. (página não existe)">Robert Burnham, Jr.</a> argumenta que o astrônomo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ptolomeu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Ptolomeu">Ptolomeu</a>, no <a href="http://pt.wikipedia.org/wiki/S%C3%A9culo_I" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Século I">século I</a>, observou o aglomerado enquanto observava outro objeto vizinho, o <a href="http://pt.wikipedia.org/wiki/Aglomerado_de_Ptolomeu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Aglomerado de Ptolomeu">Aglomerado de Ptolomeu</a>. O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Charles Messier">Charles Messier</a> catalogou o aglomerado como Messier 6 em 1764.</span></div>
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<span style="color: #073763;">Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 4,2, sendo possível observá-lo a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Olho nu">olho nu</a> sob boas condições de visualização. Suas estrelas mais brilhantes podem ser visualizadas com o auxílio de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Telescópio">telescópios</a>. Situa-se a apenas 6 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Terra">Terra</a> e sua idade foi estimada em 100 milhões de anos. Na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Esfera celeste">esfera celeste</a>, situa-se logo a norte da ponta da "cauda" da constelação de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>.</span></div>
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<b>Aglomerado da Borboleta (M6)</b></div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M6a.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 6"><img alt="Messier 6" data-file-height="675" data-file-width="900" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/7f/M6a.jpg/250px-M6a.jpg" height="188" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/7f/M6a.jpg/375px-M6a.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/7f/M6a.jpg/500px-M6a.jpg 2x" style="border: none; cursor: move; vertical-align: middle;" width="250" /></a></div>
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Messier 6</div>
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Descoberto por</div>
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<a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a></div>
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Data</div>
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<a href="http://pt.wikipedia.org/wiki/1654" style="background: none; color: #0b0080; text-decoration: none;" title="1654">1654</a></div>
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<b>Dados observacionais (J2000)</b></div>
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<a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></div>
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<a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; color: #0b0080; text-decoration: none;" title="Scorpius">Scorpius</a></div>
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Tipo</div>
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<a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">Aglomerado estelar aberto</a></div>
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<a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></div>
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17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 40,1<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span></div>
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<a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></div>
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-32° 13′</div>
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Distância</div>
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1 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (491 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</div>
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<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></div>
</td><td style="background-color: #f8f8f8;"><div style="margin: 0px;">
4,2</div>
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Dimensões</div>
</td><td style="background-color: #f8f8f8;"><div style="margin: 0px;">
25'</div>
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<b>Características físicas</b></div>
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Raio</div>
</td><td style="background-color: #f8f8f8;"><div style="margin: 0px;">
6 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></div>
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Idade estimada</div>
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100 milhões de anos</div>
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<b>Outras denominações</b></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><div style="margin: 0px;">
Messier 6, NGC 6405, Collinder 341, Melotte 178, Lund 769, OCL 1030, ESO 455-SC030</div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado da Borboleta"><img alt="Aglomerado da Borboleta" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; cursor: move; vertical-align: middle;" width="12" /></a></div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scorpius_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Scorpius constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/250px-Scorpius_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/375px-Scorpius_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/500px-Scorpius_constellation_map.png 2x" style="border: none; cursor: move; vertical-align: middle;" width="250" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Aglomerado_da_Borboleta</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Aglomerado_da_Borboleta#mediaviewer/File:M6a.jpg</span></span></div>
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<span class="mw-mmv-author" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; line-height: 24px; text-align: start; white-space: nowrap;"><a class="external text" href="http://www.ngc7000.org/" rel="nofollow" style="background: none; color: #0b0080;">Ole Nielsen</a></span><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; line-height: 24px; text-align: start; white-space: nowrap;"> - </span><span class="mw-mmv-source" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; line-height: 24px; text-align: start; white-space: nowrap;"><a class="external free" href="http://www.ngc7000.org/ccd/m6-20050902-900.jpg" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.ngc7000.org/ccd/m6-20050902-900.jpg</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://www.ipac.caltech.edu/2mass/gallery/m7atlas.jpg</span></span></div>
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<h1>
Messier 7</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M7 (NGC 6475)</i>, type 'e', in <a href="http://messier.obspm.fr/map/Sco.html">Scorpius</a></center>
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<br /><b><span style="font-size: large;">The Scorpion's Tail, Ptolemy's Cluster</span></b><br /><div style="font-size: medium;">
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<b><br /></b></div>
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<a href="http://messier.obspm.fr/Jpg/m7.jpg"><img align="right" alt="[m7.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m7.jpg" style="cursor: move;" /></a></div>
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Right Ascension</div>
</th><td align="center"><div style="margin: 0px;">
17 : 53.9 (h:m)</div>
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Declination</div>
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-34 : 49 (deg:m)</div>
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Distance</div>
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0.8 (kly)</div>
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Visual Brightness</div>
</th><td align="center"><div style="margin: 0px;">
3.3 (mag) </div>
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Apparent Dimension</div>
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80.0 (arc min)</div>
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Known to Ptolemy 130 AD.</div>
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Messier 7 (M7, NGC 6475) is a large and brilliant group, easily detected with the naked eye. As Burnham describes it, "the cluster is seen projected on a background of numerous faint and distant Milky Way stars."</div>
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This splendid cluster was known to <a href="http://messier.obspm.fr/xtra/Bios/ptolemy.html">Ptolemy</a>, who mentioned it about 130 AD and described it as the "nebula following the sting of Scorpius." The description may also include <a href="http://messier.obspm.fr/m/m006.html">M6</a>, but this is uncertain. Because of this presumable discovery, the present author [hf] has proposed the name "Ptolemy's Cluster" for M7 some years ago, a proposition which has found some acceptance meanwhile.</div>
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M7 was <a href="http://messier.obspm.fr/xtra/similar/hodierna.html">observed</a> by <a href="http://messier.obspm.fr/xtra/Bios/hodierna.html">Hodierna</a> before 1654, who counted 30 stars. <a href="http://messier.obspm.fr/xtra/Bios/halley.html">Edmond Halley</a> listed it as No. 29 in his <a href="http://messier.obspm.fr/xtra/similar/halley.html">catalog of southern stars</a> of 1678, and <a href="http://messier.obspm.fr/xtra/Bios/lacaille.html">Abbe Lacaille</a> added it to his <a href="http://messier.obspm.fr/xtra/history/lacaille.html">catalog of southern objects</a> as Lac II.14. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included it as <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M7">No. 7 in his catalog</a> on May 23, 1764.</div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">LEIA MAIS</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">em</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://messier.obspm.fr/m/m007.html">http://messier.obspm.fr/m/m007.html</a></span></span></div>
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<div class="separator" style="clear: both; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; margin: 0px;">
<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhBRzZrls0dqO-ZA6vWou-iNHML7t7icOZbKhmmFAMv0OgsxZ7UFtNrPxtw7jK-3Wgg9AkZqVY1xFNDeeT_MaVTydxaTH4wFGz8L2CytwfrBhYdz17s_ocR1BRXnr_hcqV2jr97meV-OPQ/s1600/m+7.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhBRzZrls0dqO-ZA6vWou-iNHML7t7icOZbKhmmFAMv0OgsxZ7UFtNrPxtw7jK-3Wgg9AkZqVY1xFNDeeT_MaVTydxaTH4wFGz8L2CytwfrBhYdz17s_ocR1BRXnr_hcqV2jr97meV-OPQ/s1600/m+7.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px;">Stellarium</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M 7 - NGC 6475 - Scorpius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<div style="margin: 0px;">
<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h52m Declinação -34<sup>o</sup>.48<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 5,0 Tipo AA<o:p></o:p></span></div>
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<span style="color: #073763;">O <b>Aglomerado de Ptolomeu</b> (Messier 7, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; text-decoration: none;" title="New General Catalogue">NGC 6475</a>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; text-decoration: none;" title="Scorpius">Escorpião</a>. O primeiro observador a registrar a existência do aglomerado foi <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ptolomeu" style="background: none; text-decoration: none;" title="Ptolomeu">Ptolomeu</a> ainda no <a href="http://pt.wikipedia.org/wiki/S%C3%A9culo_II" style="background: none; text-decoration: none;" title="Século II">século II</a>. O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> catalogou o aglomerado como Messier 7 em 1764.</span></div>
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<span style="color: #073763;">Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 3,3, sendo possível observá-lo a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Olho nu">olho nu</a> sob boas condições de visualização. Suas estrelas mais brilhantes podem ser visualizadas com o auxílio de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Telescópio">telescópios</a>. Situa-se 800 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Terra">Terra</a> e sua idade foi estimada em 220 milhões de anos. Na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Esfera celeste">esfera celeste</a>, situa-se logo a norte da ponta da "cauda" da constelação de <a href="http://pt.wikipedia.org/wiki/Scorpius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Scorpius">Escorpião</a>.</span></div>
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<b>Aglomerado de Ptolomeu</b></div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Open-cluster-Messier-7.jpeg" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado de Ptolomeu"><img alt="Aglomerado de Ptolomeu" data-file-height="604" data-file-width="900" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/eb/Open-cluster-Messier-7.jpeg/250px-Open-cluster-Messier-7.jpeg" height="168" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/eb/Open-cluster-Messier-7.jpeg/375px-Open-cluster-Messier-7.jpeg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/eb/Open-cluster-Messier-7.jpeg/500px-Open-cluster-Messier-7.jpeg 2x" style="border: none; cursor: move; vertical-align: middle;" width="250" /></a></div>
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Aglomerado de Ptolomeu</div>
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Descoberto por</div>
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<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ptolomeu" style="background: none; color: #0b0080; text-decoration: none;" title="Ptolomeu">Ptolomeu</a></div>
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Data</div>
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<a href="http://pt.wikipedia.org/wiki/130" style="background: none; color: #0b0080; text-decoration: none;" title="130">130</a></div>
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<b>Dados observacionais (J2000)</b></div>
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<a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></div>
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<a href="http://pt.wikipedia.org/wiki/Scorpius" style="background: none; color: #0b0080; text-decoration: none;" title="Scorpius">Scorpius</a></div>
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<a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></div>
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17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 53<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 54<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></div>
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<a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></div>
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-34° 49′ 00″</div>
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Distância</div>
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800 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (245 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</div>
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<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></div>
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3,3</div>
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Dimensões</div>
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80',0</div>
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<b>Características físicas</b></div>
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Raio</div>
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20 anos-luz</div>
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Idade estimada</div>
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220 milhões de anos</div>
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<b>Outras denominações</b></div>
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Messier 7, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6475</div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado de Ptolomeu"><img alt="Aglomerado de Ptolomeu" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; cursor: move; vertical-align: middle;" width="15" /></a></div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Scorpius_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Scorpius constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/250px-Scorpius_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/375px-Scorpius_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/Scorpius_constellation_map.png/500px-Scorpius_constellation_map.png 2x" style="border: none; cursor: move; vertical-align: middle;" width="250" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Aglomerado_de_Ptolomeu </span></div>
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<span style="color: #274e13; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Aglomerado_de_Ptolomeu#mediaviewer/File:Open-cluster-Messier-7.jpeg</span></span></div>
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<span class="mw-mmv-author" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">Oliver Stein</span><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"> - </span><span class="mw-mmv-source" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"><a class="external text" href="http://www.estelar.de/" rel="nofollow" style="background: none; color: #0b0080;">Homepage of Oliver Stein</a> <a class="external free" href="http://www.estelar.de/deepsky/kb_300_800mm/m7.htm" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.estelar.de/deepsky/kb_300_800mm/m7.htm</a></span></div>
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<b>Com um abraço estrelado,</b><br /><b>Janine Milward</b><br /><br /><br /><br /><div style="line-height: 1.4;">
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background: none; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background: none; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background: none; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background: none; color: #0b0080; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="background-color: white; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></span></div>
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<br /><span style="font-family: Arial, Helvetica, sans-serif;"><b>CARO LEITOR,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">devem requerer do Caro Leitor</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Visitando os Sites abaixo,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<b><o:p></o:p></b></span></span></span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;">......................................</span></span><br /><span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<b><br /></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></b></span></div>
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<b><br /></b></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"><b>Janine Milward</b></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #274e13;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></b><o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-14155644905396718062014-09-06T09:53:00.001-07:002016-09-20T11:26:37.894-07:00Sagittarius<div class="MsoNormal">
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><span style="background-color: white;">Olá!</span></span></div>
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<span style="color: #0c343d; font-family: "arial" , "helvetica" , sans-serif;">Nesta Postagem</span><br />
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<span style="color: #0c343d; font-family: "arial" , "helvetica" , sans-serif;">em continuidade aos nossos estudos sobre Objetos Messier,</span></div>
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<span style="color: #0c343d; font-family: "arial" , "helvetica" , sans-serif;">estaremos apresentando</span></div>
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<span style="color: #0c343d; font-family: "arial" , "helvetica" , sans-serif;">alguma informação sobre os Objetos Messier</span></div>
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<span style="color: #0c343d; font-family: "arial" , "helvetica" , sans-serif;">na constelação do Sagitário.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Eu penso ser sempre interessante podermos estudar</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"> e tentar observar</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">alguns de seus chamados Objetos Messier</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">- mesmo porque</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A constelação do Sagitário </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">contém muitos aglomerados estelares e nebulosas </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">que estão entre os objetos mais adoráveis em seus tipos.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Nesta Postagem, Caro Leitor,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontre alguma informação</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">sobre os Objetos Messier</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">encontrados no Arqueiro Centauro.</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Janine Milward</span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">http://www.stellarium.org/pt/</span><br />
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b><span style="color: #660000;">SAGITTARIUS, O ARQUEIRO</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Ascensão Reta 17h41m / 20h15m Declinação -11<sup>o</sup>.8 / -45<sup>o</sup>.4<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Mito:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Esta constelação representa o sábio e justo Centauro Quíron, que se distinguia dos seus semelhantes, que eram incultos e brutais, pela sua sabedoria.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Tendo aprendido dos seus preceptores a arte divina da medicina e da caça, teve como discípulos os Argonautas. Imortal, num combate de Centauros e Paites, acidentalmente foi ferido no tornozelo por uma flecha envenenada atirada por Hercules quando da luta de ambos contra os demais centauros. Como Quíron era um semideus, teria que viver eternamente com aquela ferida que nunca era curada. Sofrendo de dores atrozes, ofereceu Quíron sua imortalidade a Prometeu. Morto, foi colocado por Júpiter entre as estrelas.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Inscrições encontradas na Babilônia e nos monumentos persas mostram esse asterismo personificado como o deus arqueiro da guerra de Nergal.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">No Egito, era representado como um Centauro alado, galopando para o ocidente e trazendo um longo chapéu, com um arco esticado, a fim de arremessar uma flecha no corpo do escorpião.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">No tumulo de Ramsés VI é representado, unicamente, como um flecha.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Sagittarius situa-se entre as constelações Corona Australis, Telescopium, Microscopium, Capricornius, Aquila, Scutum, Serpens, Ophiucus, Scorpius<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Observação a olho nu ou através binóculos e/ou telescópios:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Quando olhamos para a constelação do Sagitário, </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">estamos olhando diretamente em direção ao centro de nossa Galáxia, </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">obscurecida por nuvens de estrelas e de material interestelar. </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">É possível observar o núcleo da Galáxia, entretanto, </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">O núcleo da Galáxia contém uma forte fonte de emissão de radio </span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">designada como Sagitário A. <o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">A<b> constelação do Sagitário</b></span><br />
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;"><b>que estão entre os objetos mais adoráveis em seus tipos.</b></span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #073763; font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO SAGITTARIUS:</b></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: "arial" , sans-serif;"><b>Spiculum.</b></span><span style="font-family: "arial" , sans-serif;"><b><span style="color: #660000;"> M8 e M20 e M21, Sagittarii. </span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;">Dois aglomerados (M8 e M21) e uma nebulosa</span><span style="font-family: "arial" , sans-serif;"> (M20),<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">situados na cabeça da flecha do Arqueiro. </span></span><br />
<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;"> Por se situarem bem próximas à linha da Eclíptica, </span></span><br />
<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">sempre podemos observar os Planetas e a Lua passando por suas vizinhanças.<o:p></o:p></span></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="color: black; font-family: "Times New Roman"; font-size: medium;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6523 - M8 - Sagittarius - Nebulosa de Emissão HII - Lagoa</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h02m Declinação -24<sup>o</sup>.23<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Tipo Nebulosa Planetária HII Dimensão 40,0 Magnitude 18<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">NGC 6523 - M 8 - Aglomerado Aberto Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h01 Declinação - 24<sup>o</sup>.23<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 5,2 Magnitude fotográfica da mais brilhante estrela 7,0<o:p></o:p></span></span></div>
<span style="background-color: white; font-family: "arial" , sans-serif;"><span style="color: #073763;"> Distância kpc 1,56 Diâmetro 45’ Tipo Espectral O5</span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">NGC 6523 = M8 - Nebulosa da Lagoa. <o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: "arial" , sans-serif;"><span style="color: #073763;">A oeste de Gama Sagittarii, Al Nash, encontraremos a Nebulosa da Lagoa e o Aglomerado aberto (M8) que podem ser vistos com visão enviesada ou através um bom par de binóculos e, melhor ainda, através telescópio.</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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A <b>Nebulosa Laguna</b> (Messier 8, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6523</a>) é uma gigantesca <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080;" title="Nebulosa">nuvem interestelar</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. É classificada como uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a>, cujos gases<a href="http://pt.wikipedia.org/wiki/%C3%8Don" style="background: none; color: #0b0080; text-decoration: none;" title="Íon">ionizados</a>, principalmente <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background: none; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a>, emitem radiação principalmente no <a href="http://pt.wikipedia.org/wiki/Comprimento_de_onda" style="background: none; color: #0b0080; text-decoration: none;" title="Comprimento de onda">comprimento de onda</a> na faixa da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luz_vis%C3%ADvel" style="background: none; color: #0b0080; text-decoration: none;" title="Luz visível">luz visível</a> vermelha.</div>
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Vista de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>, a nebulosa parece-se como uma mancha oval distinta com um núcleo definido. Sobreposta à nebulosa existe um pequeno <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto de estrelas</a>. Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,0 e situa-se a 4 850 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</div>
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A nebulosa foi descoberta pelo astrônomo italiano <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de 1654. Foi classificada por ele como uma<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> de brilho intermediário e listada como a entrada II.6 de seu catálogo. Foi redescoberta independemente por <a href="http://pt.wikipedia.org/wiki/John_Flamsteed" style="background: none; color: #0b0080; text-decoration: none;" title="John Flamsteed">John Flamsteed</a> por volta de 1680, catalogado por ele como a entrada 2446 de seu catálogo. Flamsteed o classificou como um<a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerado estelar</a>, segundo Kenneth Glyn Jones, mas as coordenadas dadas por Flamsteed correpondem às dadas por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> referentes à própria nebulosa. De fato há um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> pouco a oeste da nebulosa, conhecida como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6530" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6530">NGC 6530</a>.<span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Como uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a>, Laguna apresenta uma cor rosácea em fotografias de longa exposição, embora pareça cinza ao<a href="http://pt.wikipedia.org/wiki/Olho_humano" style="background: none; color: #0b0080; text-decoration: none;" title="Olho humano">olho humano</a> em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> ou pequenos <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>, já que a distinção de cores não ocorre quando a luminosidade é escassa.<span class="reference" id="cite_ref-seds_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Foi vista novamente por <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1746, classificando-a como um aglomerado aberto. Anos mais tarde, foi observada por <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a>, que percebeu a nebulosa associada ao aglomerado. <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a> listou o <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Objeto astronômico">objeto astronômico</a> em 1751 ou 1752 como a entrada Lac III.14 de seu catálogo. Em 23 de maio de 1764, Messier incluiu-o como a oitava entrada de seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a>, descrevendo primeiramente o aglomerado e afirmando que a nebulosa estava em torno da estrela 9 Sagitarii.<span class="reference" id="cite_ref-seds_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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<a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, catalogou separadamente as duas partes da nebulosa Laguna (H V.9, GC 4363, <a href="http://pt.wikipedia.org/wiki/NGC_6526" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6526">NGC 6526</a>; e H V.13, GC 4328, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6533" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6533">NGC 6533</a>), descrevendo que eram nebulosas grandes, mas fracas. Seu filho, <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a>, catalogou o aglomerado aberto associado à nebulosa como a entrada h 3725 (GC 4366, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6530" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6530">NGC 6530</a>), e a própria nebulosa como a entrada h 3723 (GC 4361, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_6523" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 6523">NGC 6523</a>). Outra região nebulosa a leste do núcleo, ainda pertecente a nebulosa, tem a designação própria IC 4678.<span class="reference" id="cite_ref-seds_3-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Laguna#cite_note-seds-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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LEIA MAIS</div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;"><span style="color: #073763;"></span></span></div>
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<b>VEJA O VÍDEO</b></div>
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<b>DIVING INTO THE LAGOON NEBULA</b></div>
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<b>Mergulhando na Nebulosa Laguna</b></div>
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<span style="font-family: sans-serif;"><span style="line-height: 24px; white-space: nowrap;">http://pt.wikipedia.org/wiki/Nebulosa_Laguna<span style="background-color: white;"><span style="color: #073763;">#mediaviewer/Ficheiro:VISTA%27s_infrared_view_of_the_Lagoon_Nebula_(Messier_8).jpg</span></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">VISTA's infrared view of the Lagoon Nebula (Messier 8)</span><a class="mw-mmv-license cc-license" href="http://creativecommons.org/licenses/by/3.0" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="_blank">CC BY 3.0</a></span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span style="color: #073763;"><span class="mw-mmv-author">ESO/VVV</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/eso1101a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://www.eso.org/public/images/eso1101a/</a></span></span></span></div>
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<span style="background-color: white;">Messier 8 em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Infravermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Infravermelho">infravermelho</a> (cores falsas), <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Observat%C3%B3rio_do_Paranal&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Observatório do Paranal (página não existe)">Observatório do Paranal</a></span></div>
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<span style="background-color: white;">This new infrared view of the star formation region Messier 8, often called the Lagoon Nebula, was captured by the VISTA telescope at ESO’s Paranal Observatory in Chile. This colour picture was created from images taken through J, H and Ks near-infrared filters, and which were acquired as part of a huge survey of the central parts of the Milky Way. The field of view is about 34 by 15 arcminutes.</span></div>
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<span style="background-color: white; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6618 - M 17 - Sagittarius - Nebulosa de Emissão HII</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h19m Declinação -16<sup>o</sup>.12<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Tipo Nebulosa Planetária HII Dimensão 20,0 Magnitude 19<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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A <b>Nebulosa Ômega</b>, também conhecida como a <b>Nebulosa do Cisne</b> ou <b>Nebulosa da Ferradura</b> (Messier 17, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6618</a>) é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background: none; color: #0b0080; text-decoration: none;" title="Região HII">região HII</a>, ou seja, uma região composta de gás estelar e poeira que recentemente começou a formar novas <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a>. A nebulosa está localizada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a> e foi descoberta pelo astrônomo francês <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a> em 1745, e catalogada pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764 em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> de objetos de aparência semelhante a<a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>. A nebulosa está localizada em uma região rica em estrelas, na região sagitariana da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>.</div>
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A Nebulosa Ômega está entre 5 000 a 6 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e mede cerca de 15 anos-luz de diâmetro. A nuvem de <a href="http://pt.wikipedia.org/wiki/Meio_interestelar" style="background: none; color: #0b0080; text-decoration: none;" title="Meio interestelar">matéria interestelar</a> onde a Nebulosa Ômega está contida tem cerca de 40 anos-luz de diâmetro. A <a href="http://pt.wikipedia.org/wiki/Massa" style="background: none; color: #0b0080; text-decoration: none;" title="Massa">massa</a> total da nebulosa está estimada em 800 <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a>. Um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a>, composto de 35 estrelas, está contida na nebulosa. Sua intensa radiação causa a diminuição do gás estelar em suas vizinhanças.</div>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> foi descoberta por <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1745 ou 1746. O astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> redescobriu-a independentemente em 3 de junho de 1764, listando-a em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> como sua décima sétima entrada. É uma de apenas seis nebulosas verdadeiras pertencentes ao catálogo de Messier.<span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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É visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> sob excelentes condições.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> A primeira tentativa de desenhar de modo apurado a nebulosa (como parte de uma série de esboços de nebulosas) foi feito pelo inglês <a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="John Herschel">John Herschel</a> em 1833, e publicada em 1836. Ele descreveu a nebulosa como:</div>
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"A figura desta nebulosa é quase aquela da letra maiúscula grega Omega (Ω), mas um pouco distorcida, embora a distribuição de brilho seja desigual. (...) [Charles] Messier percebeu apenas o brilhante braço leste da nebulosa, sem nenhuma das circunvoluções associadas, que foram notadas por meu pai. As peculariedades principais que eu tenho observado no sistema são: Um glóbulo visível na parte leste do braço brilhante da nebulosa, consideravelmente isolada da nebulosa circundante, sugerindo fortemente a ideia de uma absorção de matéria nebulosa, e outro glóbulo, mais pálido e menor do que o primeiro, na ponta noroeste do mesmo braço, onde a nebulosa faz uma súbita curva em um ângulo agudo."<span class="reference" id="cite_ref-psm1876_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega#cite_note-psm1876-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Um segundo e mais detalhado esboço foi feito por Herschel durante a sua visita à <a href="http://pt.wikipedia.org/wiki/%C3%81frica_do_Sul" style="background: none; color: #0b0080; text-decoration: none;" title="África do Sul">África do Sul</a> em 1837. A nebulosa também foi estudada pelo alemão <a href="http://pt.wikipedia.org/wiki/Johann_von_Lamont" style="background: none; color: #0b0080; text-decoration: none;" title="Johann von Lamont">Johann von Lamont</a>, e separadamente por Sr. Mason, ainda em graduação no <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Yale_University" style="background: none; color: #0b0080; text-decoration: none;" title="Yale University">Yale College</a>. Quando Herschel publicou seu esboço de 1837 em 1847, escreveu:</div>
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"Em particular, sobre o arco em forma de ferradura (...) foi representada como muito algongada em seu eixo vertical e com uma proporção muito maior do que o real tamanho do braço leste e do brilho da nebulosa. A difusão nebulosa na ponta [ocidental] daquele arco, formando o ângulo [ocidental] com a linha-base da letra maiúscula grega Ômega (Ω).......................................................................................</div>
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LEIA MAIS</div>
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EM</div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">ESO- Stellar Nursery-M 17-Phot-24a-00-normal</span></div>
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Messier 17</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Starforming Nebula</a> M17 (NGC 6618)</i>, an emission nebula, with <a href="http://messier.obspm.fr/cluster.html">Open Star Cluster</a>, in <a href="http://messier.obspm.fr/map/Sgr.html">Sagittarius</a><b>Omega, Swan, Horseshoe, or Lobster Nebula</b><br />
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<a href="http://messier.obspm.fr/Jpg/m17.jpg"><img align="right" alt="[m17.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m17.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">18 : 20.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-16 : 11 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">5.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">11.0 (arc min)</td></tr>
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Discovered by Philippe Loys de Chéseaux in 1745-46.</div>
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The Omega Nebula Messier 17 (M17, NGC 6618), also called the Swan Nebula, the Horseshoe Nebula, or (especially on the southern hemisphere) the Lobster Nebula, is a region of star formation and shines by excited emission, caused by the higher energy radiation of young stars. Unlike in many other emission nebulae, however, these stars are not obvious in optical images, but hidden in the nebula. Star formation is either still active in this nebula, or ceased very recently. A small cluster of about 35 bright but obscurred stars seems to be imbedded in the nebulosity.</div>
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This object was discovered by <a href="http://messier.obspm.fr/xtra/Bios/decheseaux.html">Philippe Loys de Chéseaux</a> and is one of only six "nebulae properly so called" in <a href="http://messier.obspm.fr/xtra/similar/deches.html">his catalog</a>. De Chéseaux's discovery didn't get widely known, thus <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> independently rediscovered it and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M17">cataloged it</a>on June 3, 1764.</div>
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The color of the Omega Nebula is reddish, with some graduation to pink. This color comes from the hot hydrogen gas which is excited to shine by the hottest stars which have just formed within the nebula. However, the brightest region is actually of white color, not overexposed as one might think. This phenomenon is apparently a result of a mixture of emission light from the hottest gas, together with reflections of the bright star light from the dust in this region. The nebula contains a large amount of dark obscuring material, which is obvious in its remarkable features. This matter has been heated by the hidden young stars, and shines brightly in infrared light.</div>
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The mass of the gas has been estimated to amount about 800 times that of the Sun, enough for forming a conspicuous cluster, and a good deal more than that of the <a href="http://messier.obspm.fr/m/m042.html">Orion nebula M42</a>. While the bright nebula seems to be roughly 15 light years in extension, the total gaseous cloud, including low-luminosity material, seems to extend to at least 40 light years. Distance estimates are spread over a wide range, but modern values are between 5,000 and 6,000 light years, thus little less than that of its apparent neighbor, <a href="http://messier.obspm.fr/m/m016.html">M16</a> with the Eagle nebula - apparently, these two star forming regions are indeed close together, in the same <a href="http://messier.obspm.fr/more/mw_arms.html">spiral arm</a> (the Sagittarius or Sagittarius-Carina arm) of the <a href="http://messier.obspm.fr/more/mw.html">Milky Way galaxy</a>, and perhaps part of the same giant complex of cosmic clouds of interstellar matter.</div>
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As for many diffuse nebulae, the overall brightness of this object is difficult to estimate, and is given discordantly in the sources. While older sources give estimates around 7.0 magnitudes, probably because these were performed at northern observatories, modern compilations list its visual magnitude brighter: Don Machholz lists it at 6.6 mag, the Sky Catalogue 2000.0 at 5.0 mag, and the Deep Sky Field Guide to Uranometria 2000.0 gives a value of 6.0 mag (which we adopt here); anyway, it is visible to the naked eye under good observing conditions from not too northern geographic latitudes!</div>
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The Omega or Swan Nebula M17 can be found quite easily, and similar and simultaneously to its apparent neighbor, <a href="http://messier.obspm.fr/m/m016.html">M16</a>. The first way to find it is locating the white giant star Gamma Scuti, of magnitude 4.70 and spectral type A2 III, e.g. from Altair (Alpha Aquilae) via Delta and Lambda Aql; M16 is slightly more than 2 degrees to the southwest of this star. Alternatively, in particular with a pair of binoculars, locate star cloud <a href="http://messier.obspm.fr/m/m024.html">M24</a> and move northward via a pair of stars of 6th and 7th mag in the north-eastern edge of M24, followed by small open cluster <a href="http://messier.obspm.fr/m/m018.html">M18</a> 1deg north, and M17 another 1deg to the north.</div>
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Under very favorable conditions, M17 is just visible to the naked eye at its apparent visual brightness of 6.0 magnitudes.</div>
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<span style="background-color: white;"><span style="color: #073763;"></span></span><span style="background-color: white;"><span style="color: #073763;"><a href="http://messier.obspm.fr/m/m017.html">http://messier.obspm.fr/m/m017.html</a></span></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><a href="http://www.ipac.caltech.edu/2mass/gallery/m18atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m18atlas.jpg</a></span></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="background-color: white; color: #660000; font-family: "arial" , sans-serif;"><b>M 18 - NGC 6613 - Sagittarius - Aglomerado Estelar Aberto</b></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h18m Declinação -17<sup>o</sup>.09<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 7,0 Tipo AA<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 18</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6613</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado aberto de estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764, que incluiu em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> de objetos com aparência semelhante a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>.</div>
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Do ponto de vista da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, Messier 18 está situado entre a <a href="http://pt.wikipedia.org/wiki/Nebulosa_%C3%94mega" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa Ômega">Nebulosa Ômega</a> (Messier 17) e da <a href="http://pt.wikipedia.org/wiki/Nuvem_Estelar_de_Sagit%C3%A1rio" style="background: none; color: #0b0080; text-decoration: none;" title="Nuvem Estelar de Sagitário">Nuvem Estelar de Sagitário</a> (Messier 24). Sua idade é estimada em 32 milhões de anos e está situada a cerca de 4 900 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> de distância.</div>
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LEIA MAIS </div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_18</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_18#mediaviewer/Ficheiro:Messier18.jpg</span></span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 1.2em; line-height: 24px; max-width: 60%; white-space: nowrap;">Messier18</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Messier18.jpg" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 0.9em; line-height: 24px; padding: 0px 10px; text-align: right; text-decoration: none; white-space: nowrap;" target="">Domínio público</a></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6514 - M 20 - Sagittarius - Nebulosa de Emissão HII - Trífida</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h01m Declinação -23<sup>o</sup>.02<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Tipo Nebulosa Planetária HII Dimensão 15,0 Magnitude 19<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Distância em anos-luz 3,5</span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">M 20 - NGC 6514 - Sagittarius - Nebulosa Difusa<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h01m Declinação -23<sup>o</sup>.02<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Tipo ND<o:p></o:p></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">M20 - NGC 6514 - A nebulosa Trifid<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">É uma nebulosa difusa e denominada de Trifid em função de sua divisão característica de partes brilhantes acentuadas por três bandas escuras. M20 é bem mais pálida e difícil de ser observada visualmente do que sua vizinha M8. No centro da nebulosa, o lugar onde as três bandas escuras se encontram, existe uma estrela sextupla. A coloração avermelhada é característica de nuvens de hidrogênio. As regiões azuis são preenchidas com partículas de poeria, as quais esfumaçam a luz das estrelas mais jovens e muito quentes.</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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A <b>Nebulosa Trífida</b> (Messier 20, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6514</a>) é uma <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background: none; color: #0b0080; text-decoration: none;" title="Região HII">região HII</a>, ou seja uma região composta de gás estelar e poeira onde recentemente, em termos astronômicos, começou formar novas estrelas. Está localizada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a> e seu nome significa "dividido em três lóbulos". O objeto é uma combinação incomum de um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado aberto de estrelas</a>, uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a> (a parte inferior, vermelho, em imagens de telescópios amadores), uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_reflex%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de reflexão">nebulosa de reflexão</a> (a parte superior, azul, em telescópios amadores) e uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_escura" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa escura">nebulosa escura</a> (aparentes "lacunas" na nebulosa de emissão, que causam a aparência trifurcarda, estes são também designados como Barnard 85).</div>
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Vista por um pequeno <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópio</a>, a nebulosa Trífida é um objeto brilhante e colorido, preferido pelos astrônomos amadores. Situa-se aproximadamente 5 200 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,3, sendo fracamente visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, mesmo sob excelentes condições de observação.</div>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> foi descoberta pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 5 de junho de 1764, listando-o em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> como sua vigésima entrada. Messier descreveu-o como um aglomerado contendo <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> de <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 9 a 8, embebidas em uma aparente nebulosidade.<span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Tr%C3%ADfida#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Famosa por exibir três ou quatro lóbulos aparentes, a nebulosa confundiu <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, que a catalogou como quatro nebulosas separadas; Herschel, em respeito ao trabalho de Messier, usualmente não atribuía sua própria nomenclatura aos objetos já nomeados por Messier.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_Tr%C3%ADfida#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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LEIA MAIS</div>
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EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Nebulosa_Tr%C3%ADfida</span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Hs-1999-42-a-full jpg</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Hs-1999-42-a-full_jpg.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></span></div>
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<span class="mw-mmv-source-author mw-mmv-reduce-toolong" original-title="Autor e informação sobre a fonte" style="background-color: white; font-size: 0.8em;"><span class="mw-mmv-author">NASA and Jeff Hester (Arizona State University)</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/1999/42/image/a" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/1999/42/image/a</a> <a class="external free" href="http://mix.msfc.nasa.gov/abstracts.php?p=2761" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://mix.msfc.nasa.gov/abstracts.php?p=2761</a></span></span></div>
<span style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /><br /><br /><br /><br /></span></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"><br /></span></span><span style="font-family: "arial" , sans-serif; font-size: 11pt;"><span style="background-color: white; color: #073763;"><img height="640" src="http://www.ipac.caltech.edu/2mass/gallery/m21atlas.jpg" width="519" /><br /><br /><br /><span style="font-size: 14.6667px;"><a href="http://www.ipac.caltech.edu/2mass/gallery/m21atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m21atlas.jpg</a></span><br /><br /><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 21 - NGC 6531 - Sagittarius - Aglomerado Estelar Aberto </span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 7,0 Tipo AA<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 21</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6531</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 5 de junho de 1764.</div>
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Messier 21 é um aglomerado relativamente jovem de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a>, com meros 4,6 milhões de anos, e situa-se aproximadamente 4 250 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. É altamente denso mas contém apenas 57 estrelas Algumas estrelas gigantes azuis foram identificadas no aglomerado, mas a maior parte de suas estrelas são pequenas. Com uma<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 6,5, Messier 21 não é visível a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, embora seja facilmente visível com bons <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> em noite com boas condições de visibilidade.</div>
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LEIA MAIS</div>
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EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_21</span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">M21</span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;">Original uploader was <a class="extiw" href="http://fr.wikipedia.org/wiki/User:Edmond_Wells" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="fr:User:Edmond Wells">Edmond Wells</a> </span></div>
<span style="background-color: white;"><span style="color: #073763;"><br /></span></span><span style="background-color: white;"><span style="color: #073763;"><br /></span></span><span style="background-color: white;"><span style="color: #073763;"><br /><br /><br /><br /><br /><br /><br /><img src="http://www.ipac.caltech.edu/2mass/gallery/m22atlas.jpg" /></span></span><span style="background-color: white;"><span style="color: #073763;">http://www.ipac.caltech.edu/2mass/gallery/m22atlas.jpg<br /><br /><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 22 - NGC 6656 - Sagittarius - Aglomerado Estelar Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h35m Declinação -23<sup>o</sup>.55<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 5,2 Tipo AG<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">NGC 6656 - M 22 - Aglomerado Globular Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h35m Declinação -23<sup>o</sup>.56<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,2 Diâmetro aparente 26’,2 Tipo Espectral F7<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 13,73<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 24 Distância kpc 3,0<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) - 144<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-family: "arial" , sans-serif;">Facies</span><span style="font-family: "arial" , sans-serif;">. A Nebulosa na Face do Arqueiro. Aglomerado globular visível a olho nu, a meio caminho entre as estrelas Mu e Sigma Sagitarii. Situado a 27.000 anos-luz, constitui o mais extenso objeto deste tipo. Formado de mais de 50.000 estrelas de décima Magnitude visual, é um notável objeto quando observado ou através bons binóculos ou bons telescópios.</span></span><br />
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<span lang="PT" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">M22 - NGC 6656 - Aglomerado Globular<o:p></o:p></span></span></div>
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<span lang="PT" style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Este é um dos mais brilhantes (e também um dos mais próximos) aglomerados globulares no céu, mais brilhante ainda do que M13, em Hercules.</span></span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 22</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6656</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> <a href="http://pt.wikipedia.org/wiki/Elipsoide" style="background: none; color: #0b0080; text-decoration: none;" title="Elipsoide">elipsoidal</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>, próximo à <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bulbo_gal%C3%A1ctico" style="background: none; color: #0b0080; text-decoration: none;" title="Bulbo galáctico">região central</a> da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a> observado na abóbada celeste. Foi decoberto pelo astrônomo <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Johann_Abrahan_Ihle&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Johann Abrahan Ihle (página não existe)">Johann Abrahan Ihle</a> em 1665 enquanto observava a passagem de <a href="http://pt.wikipedia.org/wiki/Saturno_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Saturno (planeta)">Saturno</a> pela constelação de Sagitário.</div>
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É um dos mais brilhantes aglomerados globulares visto no céu, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> igual a 5,1. Situa-se aproximadamente a 10 400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e contém mais de 70 000 estrelas.</div>
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<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">Situa-se apenas a 10 400 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, um dos </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerados_globulares" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerados globulares">aglomerados globulares</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> mais próximos de nosso planeta. Seu diâmetro aparente, cerca de 32 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de grau</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, ligeiramente maior do que o diâmetro aparente da </span><a href="http://pt.wikipedia.org/wiki/Fases_da_Lua" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Fases da Lua">Lua Cheia</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, corresponde a um diâmetro real de 97 anos-luz. A </span><a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Olho nu">olho nu</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, seu diâmetro aparente é de apenas 17 minutos e é o terceiro aglomerado globular mais brilhante do céu noturno, perdendo apenas para </span><a href="http://pt.wikipedia.org/wiki/Omega_Centauri" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;" title="Omega Centauri">Omega Centauri</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (NGC 5139) e </span><a href="http://pt.wikipedia.org/wiki/47_Tucanae" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="47 Tucanae">47 Tucanae</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (NGC 104). Está situada em frente ao</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bulbo_gal%C3%A1ctico" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Bulbo galáctico">bulbo galáctico</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, tornando-o útl como uma </span><a href="http://pt.wikipedia.org/wiki/Lente_gravitacional" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Lente gravitacional">microlente gravitacional</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> nas estrelas localizadas no bulbo galáctico.</span><span class="reference" id="cite_ref-seds_5-2" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_22#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> </span><span class="reference" id="cite_ref-Gaudi2002_4-1" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_22#cite_note-Gaudi2002-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_22</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_22#mediaviewer/Ficheiro:Messier22.jpg</span></span><br />
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<span style="background-color: white;"><span style="color: #073763;">Núcleo de Messier 22, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 23 - NGC 6494 - Sagittarius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h55 Declinação -19<sup>o</sup>.00<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 6,0 Tipo AA<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">NGC 6494 - M 23 - Aglomerado Aberto Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h55m Declinação - 19<sup>o</sup>.01<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 5,9 Magnitude fotográfica da mais brilhante estrela 10,2</span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;"> Distância kpc 0,44 Diâmetro 27’ Tipo Espectral B8<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 23</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6494</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 20 de junho de 1764.</div>
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Messier 23 está localizado a cerca de 2 150 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, e mede entre 15 a 20 anos-luz de diâmetro. Foi identificado 150 estrelas pertencentes ao aglomerado, sendo que a estrela mais brilhante tem uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 9,2. Messier 23 pode ser encontrado com o uso de <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> razoáveis entre as númerosas estrelas situadas no <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bulbo_gal%C3%A1ctico" style="background: none; color: #0b0080; text-decoration: none;" title="Bulbo galáctico">bulbo galáctico</a> da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>.</div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_23</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://www.ipac.caltech.edu/2mass/gallery/m24atlas.jpg</span></span><br />
<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 24 - NGC 6603 - Sagittarius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h17m Declinação -18<sup>o</sup>.27<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude visual integral 6,0 Tipo AA<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">M24 - uma nuvem de estrelas na Via Láctea<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Esta nuvem pode ser observada a olho nú, localizada a cerca de 3 graus a leste do brilhante Aglomerado aberto M25 (IC 4725). Outro Aglomerado aberto muito belo é M23 (NGC 6494) localizado cerca de 5.5 graus a oeste de M24.</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6603</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sagittarius">constelação de Sagittarius</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Foi descoberto pelo astrônomo inglês </span><a href="http://pt.wikipedia.org/wiki/John_Herschel" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="John Herschel">John Herschel</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em 1830. Devido a sua moderada</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (+11,1), pode ser visto mesmo com pequenos </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> amadores ou equipamentos maiores. Está na mesma região da </span><a href="http://pt.wikipedia.org/wiki/Ab%C3%B3bada_celeste" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Abóbada celeste">abóbada celeste</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> que a </span><a href="http://pt.wikipedia.org/wiki/Nuvem_Estelar_de_Sagit%C3%A1rio" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nuvem Estelar de Sagitário">Nuvem Estelar de Sagitário</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (Messier 24) e historicamente é frequentemente confundido com a própria nuvem estelar.</span></div>
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<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: sans-serif;">http://pt.wikipedia.org/wiki/NGC_6603</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://www.ipac.caltech.edu/2mass/gallery/m25atlas.jpg</span></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">M 25 - IC 4725 - Sagittarius - Aglomerado Estelar Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h30m Declinação - 19<sup>o</sup>.16<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">NGC I4725 - M 25 - Aglomerado Aberto Sagitário<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 18h30m Declinação - 19<sup>o</sup>.16<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,2 Magnitude fotográfica da mais brilhante estrela 9,3</span></span></div>
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<span style="background-color: white; color: #073763; font-family: "arial" , sans-serif;"> Distância kpc 0,60 Diâmetro 35’ Tipo Espectral B3</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 25</b> (<a href="http://pt.wikipedia.org/wiki/Index_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="Index Catalogue">IC 4725</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a>. Foi descoberto pelo suíço <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1745, e foi incluído por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> de aparência semelhante a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a> em 1764.</div>
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Messier 25 está a uma distância de cerca de 2 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Tem cerca de 19 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> de diâmetro. Uma <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela variável">estrela variável</a> em brlho, tipo <a href="http://pt.wikipedia.org/wiki/Cefeida" style="background: none; color: #0b0080; text-decoration: none;" title="Cefeida">Delta Cephei</a>, designada como <i>U Sagittari</i>, é membro do aglomerado.</div>
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LEIA MAIS EM</div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Messier_25</span></span></div>
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<span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">Messier 25, </span><a href="http://pt.wikipedia.org/wiki/NASA" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="NASA">NASA</a></div>
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<span style="background-color: white; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span><br />
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<b><span style="color: #660000;">Messier 28</span></b><span style="color: #252525;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6626</a><span style="color: #252525;">), é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagitário</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em </span><a href="http://pt.wikipedia.org/wiki/1764" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1764">1764</a><span style="color: #252525;">.</span></div>
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Situa-se a uma distância de aproximadamente 18 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.</div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_28</span></span></div>
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<span style="background-color: white; color: #073763;"><br /></span><span style="background-color: white; color: #073763;">http://pt.wikipedia.org/wiki/Messier_28#mediaviewer/Ficheiro:Messier_28_Hubble_WikiSky.jpg</span><br />
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 28 Hubble WikiSky</span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=18.408648220844615&de=-24.870597658403195&angle=0.04141311201217398&projection=tan&rotation=42.09164940087089&survey=astrophoto&img_id=60565&width=1480&height=1480&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=move" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="color: #660000;"><b>Messier 54</b> </span><span style="color: #252525;">(também conhecido como </span><b style="color: #252525;">M54</b><span style="color: #252525;"> ou </span><b style="color: #252525;">NGC 6715</b><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em 1778 e subsequentemente incluído no seu catálogo de </span><a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a><span style="color: #252525;">.</span></div>
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Modernas estimativas colocam M54 a uma distância de cerca de 87.000 anos-luz, traduzindo-se em um verdadeiro raio de 150 anos-luz de diâmetro. É um dos mais densos globulares, sendo de classe III (I sendo a mais densa e XII a menos densa). Ele brilha com <a href="http://pt.wikipedia.org/wiki/Luminosidade" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade">luminosidade</a> de cerca de 850.000 vezes a do <a href="http://pt.wikipedia.org/wiki/Sol" style="background: none; color: #0b0080; text-decoration: none;" title="Sol">Sol</a> e tem uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a>de -10,0.</div>
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M54 é facilmente encontrado no céu, estando perto da <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> <a href="http://pt.wikipedia.org/wiki/Zeta_Sagittarii" style="background: none; color: #0b0080; text-decoration: none;" title="Zeta Sagittarii">ζ Sagittarii</a>. Porém, não resolúvel em estrelas individuais, mesmo com grandes <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores.</div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_54</span></span></div>
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<span style="background-color: white; color: #073763;">http://pt.wikipedia.org/wiki/Messier_54#mediaviewer/Ficheiro:Messier_54_Hubble_WikiSky.jpg</span><br />
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Messier 54 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=18.917612480529517&de=-30.47898345725825&angle=0.05961446135552157&projection=tan&rotation=3.5940140919059433&survey=astrophoto&img_id=60489&width=4280&height=4280&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=move" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6809 - M 55 - Aglomerado Globular Sagitário</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 19h38m Declinação -30<sup>o</sup>.59<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,7 Diâmetro aparente 21’,1 Tipo Espectral F5<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 13,68<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 6 Distância kpc 6,0<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) + 170<span style="font-size: 11pt;"><o:p></o:p></span></span></span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 55</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (também conhecido como </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6809</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> ou </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">M55</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a 17 300 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em </span><a href="http://pt.wikipedia.org/wiki/1752" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1752">1752</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Possui um raio de 50 anos-luz e uma dimensão aparente de 19 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">.</span><span class="reference" id="cite_ref-seds_2-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_55#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span style="color: #073763;"><span style="background-color: white;">LEIA MAIS EM</span></span></div>
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<span style="color: #073763;"><span style="background-color: white;">http://pt.wikipedia.org/wiki/Messier_55</span></span></div>
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<span style="color: #073763;"><span style="background-color: white;"><br /></span></span><span style="color: #073763;"><span style="background-color: white;">http://pt.wikipedia.org/wiki/Messier_55#mediaviewer/Ficheiro:M55.jpg</span></span><br />
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<span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">Messier 55, </span><a href="http://pt.wikipedia.org/wiki/NASA" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="NASA">NASA</a></div>
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<span style="background-color: white; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span><br />
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<b><span style="color: #660000;">Messier 69</span></b><span style="color: #252525;"> (também conhecida como </span><b style="color: #252525;">M69</b><span style="color: #252525;"> ou </span><b style="color: #252525;">NGC 6637</b><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> localizado na constelação de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em </span><a href="http://pt.wikipedia.org/wiki/31_de_agosto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="31 de agosto">31 de agosto</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/1780" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1780">1780</a><span style="color: #252525;">, na mesma noite em que ele descobriu a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M70" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M70">M70</a><span style="color: #252525;">.</span></div>
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M69 está a uma distância de cerca de 29,700 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e tem um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raio" style="background: none; color: #0b0080; text-decoration: none;" title="Raio">raio</a> espacial de 42 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. Trata-se de um vizinho próximo do aglomerado globular <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M70" style="background: none; color: #0b0080; text-decoration: none;" title="M70">M70</a>, 1.800 anos-luz separam os dois objetos, e ambos os pólos estão localizados perto do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Centro_gal%C3%A1ctico" style="background: none; color: #0b0080; text-decoration: none;" title="Centro galáctico">centro galáctico</a>. É um dos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerados_globulares" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerados globulares">aglomerados globulares</a> com miores índices de <a href="http://pt.wikipedia.org/wiki/Metalicidade" style="background: none; color: #0b0080; text-decoration: none;" title="Metalicidade">metalicidade</a>.<span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_69#cite_note-seds-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><span style="color: #073763;"><br /></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_69</span></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_69#mediaviewer/Ficheiro:Messier_69_Hubble_WikiSky.jpg</span></span></div>
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<a class="extiw" href="http://en.wikipedia.org/wiki/Messier_69" style="background: none rgb(251, 251, 251); color: #0b0080; font-size: 16px; line-height: 24px; text-decoration: none;" title="en:Messier 69">en:Messier 69</a><span style="background-color: #fbfbfb; color: #555555; font-size: 16px; line-height: 24px;"> globular cluster by </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none rgb(251, 251, 251); color: #0b0080; font-size: 16px; line-height: 24px; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a></div>
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<span style="font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span><br />
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<b><span style="color: #660000;">Messier 70</span></b><span style="color: #252525;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6681</a><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> localizado na constelação de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> em </span><a href="http://pt.wikipedia.org/wiki/31_de_agosto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="31 de agosto">31 de agosto</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/1780" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1780">1780</a><span style="color: #252525;">, na mesma noite em que ele descobriu a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M69" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M69">M69</a><span style="color: #252525;">.</span></div>
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M70 está a uma distância de cerca de 29,300 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Trata-se de um vizinho próximo (~2 graus) do aglomerado globular <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M69" style="background: none; color: #0b0080; text-decoration: none;" title="M69">M69</a>, 1.800 anos-luz separam os dois objetos, e ambos os pólos estão localizados perto do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Centro_gal%C3%A1ctico" style="background: none; color: #0b0080; text-decoration: none;" title="Centro galáctico">centro galáctico</a>. Esta a meio caminho entre Épsilon e Zeta Sagittarius. São conhecidas apenas duas estrelas variavéis neste aglomerado.<span class="reference" id="cite_ref-seds_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_70#cite_note-seds-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_70#mediaviewer/Ficheiro:Messier70-HST-Potw1215a.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Messier70-HST-Potw1215a</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author">ESA/Hubble & NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/potw1215a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/potw1215a/</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="color: black; font-family: "times new roman"; text-decoration: underline;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</span></span></span><br />
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<span style="color: #660000;"><b>Messier 75</b> </span><span style="color: #252525;">(também conhecido como </span><b style="color: #252525;">M72</b><span style="color: #252525;"> ou </span><b style="color: #252525;">NGC 6864</b><span style="color: #252525;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="color: #252525;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagittarius" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sagittarius">Sagittarius</a><span style="color: #252525;"> a 67 500 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="color: #252525;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525;">. Foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span style="color: #252525;"> em 1780.</span><span class="reference" id="cite_ref-seds_2-4" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Possui um raio de 53 anos-luz e uma <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro_angular" style="background: none; color: #0b0080; text-decoration: none;" title="Diâmetro angular">dimensão aparente</a> de 6,6 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>. É <a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background: none; color: #0b0080;" title="Classe de Concentração de Shapley–Sawyer">classificado</a> como classe I, o que significa que é um dos aglomerados mais densos conhecidos. Sua <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> é -8,5, e é 180 000 vezes mais luminoso que o Sol.<span class="reference" id="cite_ref-seds_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi descoberto pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> em 27 de agosto de 1780, sendo <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogado</a> pelo seu colega de observatório, <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, em 18 de outubro daquele ano. <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background: none; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background: none; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, foi o primeiro a resolver suas estrelas mais brilhantes.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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É um dos <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a> mais tênues do catálogo Messier, situando-se a uma distância de 67 500 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à<a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, muito além do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea#N.C3.BAcleo" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">núcleo da Via-Láctea</a>, que está a uma distância de 47 600 anos-luz em relação ao aglomerado.<span class="reference" id="cite_ref-seds_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_75#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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LEIA MAIS EM</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_75</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">Messier 75 - Globular Cluster The image was produced by </span><a class="external text" href="http://wikisky.org/" rel="nofollow" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;">WikiSky's</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;"> image cut out tool out of DSS2 data. See </span><a class="external text" href="http://wikisky.org/wiki/Copyright_-_DSS2_images" rel="nofollow" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">Copyright notice</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px;">. Source url:</span><a class="external free" href="http://server1.wikisky.org/imgcut.jsp?survey=DSS2&img_id=all&angle=0.2&ra=20.101667&de=-21.91667&width=2000&height=2000" rel="nofollow" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;">http://server1.wikisky.org/imgcut.jsp?survey=DSS2&img_id=all&angle=0.2&ra=20.101667&de=-21.91667&width=2000&height=2000</a></span></span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>O CATÁLOGO MESSIER</b></span></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background: none; color: #0b0080; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background: none; color: #0b0080; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background: none; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background: none; color: #0b0080; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background: none; color: #0b0080; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background: none; color: #0b0080; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background: none; color: #0b0080; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background: none; color: #0b0080; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background: none; color: #0b0080; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" height="220" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br />
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>Janine Milward</b></span><br />
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://media.skysurvey.org/interactive360/index.html" style="color: #274e13; text-decoration: none;">http://media.skysurvey.org/interactive360/index.html</a></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">devem requerer do Caro Leitor</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">alguma pequena retificação.<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">Obrigada por sua compreensão.<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">Visitando os Sites abaixo,<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/" style="text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><a href="http://www.nightskyatlas.com/index.jsp" style="text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;"><a href="http://www.stellar-database.com/" style="text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="font-family: "arial" , "helvetica" , sans-serif;"><span style="color: #073763;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)<b><o:p></o:p></b></span></span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-61352158676826454922014-09-06T08:38:00.003-07:002015-01-04T10:12:47.602-08:00Sagitta<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sagitta, a Flecha certeira, é uma pequena constelação, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem pequena mesmo, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém indubitavelmente bem nomeada enquanto <i>Flecha</i> -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pois é bem assim que a visualizamos nos céus estrelados mais ao norte</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e bem ao lado da belíssima Aquila, a Águia que voa trazendo suas três estrelinhas</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que podemos nomear enquanto as<i> Três Marias do Norte</i>), </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Alshain e Tarazed</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> deixando o centro iluminado</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> para ser ocupado pela maravilhosa Altair, estrela-alpha Aquilae!</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Aliás, a Águia é uma constelação bem rica, digamos assim,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porque traz consigo e já amealhada para si,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> incorporada em seu desenho estelar,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a antiga constelação de Antinous...</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>(<span style="background-color: white; line-height: 19.0499992370605px;">A parte sul de Aquila foi subdividida por Ptolomeu</span></i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span style="background-color: white; line-height: 19.0499992370605px;"> em uma constelação agora obsoleta, chamada Antinous,</span></i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span style="background-color: white; line-height: 19.0499992370605px;"> visualizada em alguns mapas </span></i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><span style="background-color: white; line-height: 19.0499992370605px;">como sendo mantida nas garras da águia)</span></i>,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e em seu voo, a Águia vem sempre acompanhada de Delphinus e Sagitta,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Delfim e a Flecha,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Delfim nadando através as estrelas </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e a Flecha certeira buscando seu alvo através as estrelas!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E não podemos deixar de mencionar</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a constelação Vulpecula -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">adicionado por Hevelius, em 1690,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">na intenção de ocupar um espaço no céu</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">com um animal (a Raposa caçando o Ganso)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tão astuto e voraz e corajoso quanto a Águia, Aquila, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e como o Corvo Caído, Vultur Cadens (outra denominação para a Lyra!):</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">entrou em cena, então, a constelação Vulpecula et Anser, a Raposa e o Ganso.</span></div>
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<img src="http://www.raremaps.com/maps/medium/30252.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; line-height: 22.3999996185303px; padding: 8px;" /></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.raremaps.com/gallery/detail/30252/Aquila_and_Antinous_Stars_heightened_in_gold/Hevelius.html</span></div>
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<strong>Title: </strong>Aquila and Antinous (Stars heightened in gold)</div>
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<strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/2813" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Johannes Hevelius</a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Assim como as cartas celestes nos mostram, Vulpecula encontra-se</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">praticamente grudada à Sagitta </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ambas constelações situando-se na Grande Fenda, The Great Rift, o Rio do Vazio,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a bifurcação que acontece naquele ponto da Via Lactea</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> entre as estrelas Altair e Deneb, estrelas-alpha Aquilae e Cygni, respectivamente.... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- porém é preciso que estejamos em lugar realmente de céus transparentes</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para bem visualizarmos esses pormenores na Via Lactea...</span></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"></span><span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp?rightAscension=20.3&declination=23.6" style="color: #274e13; text-decoration: none;">http://www.nightskyatlas.com/index.jsp?rightAscension=20.3&declination=23.6</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">É bem interessante também percebermos</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que as constelações Sagitta, a Flecha, e Vulpecula, a Raposa,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontram-se bem no caminho do meio</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">da deslumbrante imagem que nomeamos de Grande Triângulo do Norte</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(do Verão, no hemisfério norte, e do Inverno, no hemisfério sul)</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">realizado a partir das estrelas Alpha das constelações Aquila, Lyra e Cygnus,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quer dizer, das belíssimas estrelas Altair, Vega e Deneb!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em outros Trabalhos,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> viemos comentando sobre</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>os Objetos Messier acolhidos pela constelação Cygnus</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- veja em</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m29-e-m39-os-objetos-messier-em-cygnus.html -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e os Objetos messier acolhidos pela constelação Lyra</b>...</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- veja em </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m56-e-m57-os-objetos-messier-em-lyra.html</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"> -,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém não encontramos nenhum desses Objetos em Aquila</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- mas, ao invés da Águia, estivemos comentando</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre <b>o Objeto Messier que se encontra em Vulpecula</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(veja em</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m27-o-unico-objeto-messier-em-vulpecula.html),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e<b> </b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>estaremos comentando neste Trabalho</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>sobre o Objeto Messier encontrado em Sagitta,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 71!</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">SAGITTA, A FLECHA</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 18h56m / 20h18m Declinação +16<sup>o</sup>.0 / +21<sup>o</sup>.4<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mito:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa a flecha com a qual Hercules matou a águia </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que se nutria do fígado de Prometeus. <o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">História:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É uma constelação de pequeno tamanho </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém já fazia parte do grupo de 48 constelações relacionadas por Ptolomeu. <o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span></div>
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<a href="http://www.raremaps.com/gallery/detail/33034op/_Sagitta_Stars_Heightened_in_Gold/Bayer.html">http://www.raremaps.com/gallery/detail/33034op/_Sagitta_Stars_Heightened_in_Gold/Bayer.html</a></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Title: </strong>[ Sagitta ] (Stars Heightened in Gold) </span></span><strong style="background-color: white; color: #073763;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="background-color: white; border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sagitta encontra-se bem acolhida pela Via Láctea, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">podendo ser bem visualizada em pelo menos quatro de suas estrelas, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em lugares de céus escuros e límpidos,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> ao norte de Altair, a estrela Alpha Aquilae.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A estrela Gamma parece atuar como a ponta afiada da Flecha</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> enquanto as estrelas Alpha e Beta, como a pena que enfeita a Flecha </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e que se encontram sustentadas e amarradas à Flecha através a estrela Delta.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Fronteiras:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sagitta situa-se entre as constelações Vulpecula, Hercules, Aquila, Delphinus<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a></center>
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Messier 71</h1>
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<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M71 (NGC 6838)</i>, class X-XI, in <a href="http://messier.obspm.fr/map/Sge.html">Sagitta</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">19 : 53.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+18 : 47 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">13.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.2 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">7.2 (arc min)</td></tr>
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Discovered 1745-46 by Philippe Loys de Chéseaux.<br />
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Messier 71 (M71, NGC 6838) is a loose but beautiful globular cluster in the small but nice constellation Sagitta.<br />
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M71 was first seen by <a href="http://messier.obspm.fr/xtra/Bios/decheseaux.html">De Chéseaux</a>, who <a href="http://messier.obspm.fr/xtra/similar/deches.html">cataloged it as his No. 13</a>. It was later rediscovered by <a href="http://messier.obspm.fr/xtra/Bios/koehler.html">Johann Gottfried Koehler</a>, between 1772 and 1779, and by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on June 28, 1780. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> cataloged it <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M71">as his object No. 71</a>, based on his observations of October 4, 1780, as a nebula without stars. It was first resolved into stars by <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> in 1783.<br />
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This globular cluster is easy to find and nicely observable even in good binoculars, by locating the 6th-mag star 9 Sagittae half-way between Gamma and Delta of that constellation. Medium-sized amateur telescopes are required to resolve this compressed mass of stars, but then even the center is resolved. The cluster is brighter and sharply terminated on the western side, forming a "curving V", as John Mallas describes it.<br />
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http://messier.obspm.fr/m/m071.html<br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M71 - NGC 6839 - Aglomerado de estrelas</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado bem pouco comum na constelação de Sagitta,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> possuindo características tanto de ser um aglomerado aberto </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quanto de ser um aglomerado globular.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_71#mediaviewer/Ficheiro:M71.jpg</span></div>
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<span class="mw-mmv-author" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; white-space: nowrap;">Till Credner und Sven Kohle, Calar Alto Observatory</span><span style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; white-space: nowrap;"> - </span><span class="mw-mmv-source" style="background-color: #fbfbfb; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; white-space: nowrap;"><a class="external free" href="http://www.allthesky.com/clusters/preview/m71-p.jpg" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.allthesky.com/clusters/preview/m71-p.jpg</a> (<a class="external free" href="http://www.allthesky.com/clusters/m71-d.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.allthesky.com/clusters/m71-d.html</a>)</span></div>
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<span style="color: #660000;"><span style="font-family: Arial, Helvetica, sans-serif;"> </span><span style="font-family: Arial, sans-serif;"> </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">Messier 71</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> (também conhecido como </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">NGC 6838</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> ou </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">M71</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">)</span></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de </span><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Sagitta">Sagitta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> a 13 000 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Foi descoberto por</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> em </span><a href="http://pt.wikipedia.org/wiki/1746" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="1746">1746</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Possui um raio de 13,5 anos-luz e uma dimensão aparente de 7,2 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">.</span><span class="reference" id="cite_ref-seds_2-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi primeiramente visto por <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>, que o catalogou como o décimo terceiro objeto de sua lista. Foi mais tarde redescoberto por <a href="http://pt.wikipedia.org/wiki/Johann_Gottfried_K%C3%B6hler" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Gottfried Köhler">Johann Gottfried Köhler</a> entre 1772 e 1779 e por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> em 28 de junho de 1780.<a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogou</a> o objeto em 4 de outubro daquele ano com base na descrição de Méchain, e o próprio Messier descreveu-o como "uma nebulosa sem estrelas".<span class="reference" id="cite_ref-seds_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Pode ser visto mesmo em bons <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>, embora suas estrelas mais brilhantes possam ser resolvidas a partir de <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a>amadores médios ou mais potentes.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Por um bom tempo, a classificação de M71 como um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> denso, como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_11" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 11">Messier 11</a>, ou um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> pouco denso era indefinida. <a href="http://pt.wikipedia.org/wiki/Harlow_Shapley" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Harlow Shapley">Harlow Shapley</a> e <a href="http://pt.wikipedia.org/wiki/Robert_Julius_Trumpler" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Robert Julius Trumpler">Robert Julius Trumpler</a>, alguns dos primeiros a investigar as propriedades físicas do aglomerado, classificaram-no como aberto. <a class="new" href="http://pt.wikipedia.org/w/index.php?title=James_Cuffey&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="James Cuffey (página não existe)">James Cuffey</a> investigou o <a href="http://pt.wikipedia.org/wiki/Diagrama_de_Hertzsprung-Russell" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diagrama de Hertzsprung-Russell">diagrama de magnitude de cor</a> do objeto, concluindo que o diagrama era mais semelhante a de um aglomerado aberto. Outro critério de classificação, a velocidade do radial do sistema, também não estava definido: seus valores da taxa de afastamento em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> variavam entre -80 a +80 km/s (atualmente aceita-se que M71 está se aproximando radialmente da Terra a uma velocidade de 23 km/s).<span class="reference" id="cite_ref-seds_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Atualmente, há um consenso em torno de sua classificação como aglomerado globular. Situa-se a uma distância de 13 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> e possui um núcleo mais denso, facilmente visível em <a href="http://pt.wikipedia.org/wiki/Astrofotografia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astrofotografia">astrofotografias</a> ou em telescópios amadores, com diâmetro aparente na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Esfera celeste">esfera celeste</a> de 5 a 6 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de grau</a>. Seu diâmetro aparente total é pouco maior, com 7 minutois de grau, correspondendo a um diâmetro real de apenas 27 anos-luz, muio menor comparado a outros aglomerados globulares.<span class="reference" id="cite_ref-seds_2-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span><br />
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 71</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_71_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Imagem de Messier 71 tirada pelo Telescópio Espacial Hubble. Crédito: NASA/STScI/WikiSky"><img alt="Imagem de Messier 71 tirada pelo Telescópio Espacial Hubble. Crédito: NASA/STScI/WikiSky" data-file-height="4000" data-file-width="4000" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Messier_71_Hubble_WikiSky.jpg/250px-Messier_71_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Messier_71_Hubble_WikiSky.jpg/375px-Messier_71_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Messier_71_Hubble_WikiSky.jpg/500px-Messier_71_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Imagem de Messier 71 tirada pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a>.<br />
Crédito: <a href="http://pt.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=STScI&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="STScI (página não existe)">STScI</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=WikiSky&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="WikiSky (página não existe)">WikiSky</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background: none; color: #0b0080; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1746" style="background: none; color: #0b0080; text-decoration: none;" title="1746">1746</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Sagitta" style="background: none; color: #0b0080; text-decoration: none;" title="Sagitta">Sagitta</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">19<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 53<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 46,5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">18° 46′ 45,1″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">13 000 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (4 000 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,1<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">7,2 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">Classe</a></td><td style="background-color: #f8f8f8;">X-XI<span class="reference" id="cite_ref-seds_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">13,5<span class="reference" id="cite_ref-seds_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M71, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6838, GC1 115.<span class="reference" id="cite_ref-simbad_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_71#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 71"><img alt="Messier 71" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/14px-Locator_Dot2.gif" height="14" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="14" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Sagitta_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Sagitta constellation map.png" data-file-height="1419" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/2c/Sagitta_constellation_map.png/250px-Sagitta_constellation_map.png" height="198" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2c/Sagitta_constellation_map.png/375px-Sagitta_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2c/Sagitta_constellation_map.png/500px-Sagitta_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_71">http://pt.wikipedia.org/wiki/Messier_71</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>conheça mais sobre</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>a Constelação Sagitta</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acessando meu Trabalho</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"> http://oceudomes.blogspot.com.br/2014/08/sagitta-estrelada-flecha-certeira.html</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br /><div style="font-family: 'Times New Roman'; font-size: medium; line-height: 18px;">
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<img alt="Sagitta" height="463" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_sagitta.jpg" width="640" /></div>
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http://www.aradergalleries.com/detail.php?id=3659</div>
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<span style="font-family: Georgia, 'Times New Roman', Times, serif; font-size: 14px;"><span style="color: #073763;">Johann Bayer — Sagitta</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward<b><o:p></o:p></b></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">VISITE MINHA PÁGINA<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">DA TERRA AO CÉU E AO INFINITO<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/">http://daterraaoceueaoinfinito.blogspot.com.br/</a></span></span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-5124328638676843742014-09-06T08:37:00.007-07:002015-01-04T10:07:32.760-08:00Puppis<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É sempre muito fácil nos sentirmos atraídos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pelo chamado do brilho intenso e do piscar</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">da estrela-alpha Canis Majoris, Sirius, a bela.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olhando um tantinho ao sul,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Canopus, estrela-alpha Carinae, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o comandante de Argo Navis, o Navio,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">também nos atrai a atenção!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Se bem observarmos</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- e sempre em lugares de céus escuros e transparentes</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e em noites de ausência de Lua -,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontraremos entre essas duas maravilhosas estrelas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">uma espécie de paredão, uma muralha de estrelinhas tímidas...:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é a Pôpa do Navio, Puppis!</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgqefwtWtWks1AM0ztcWFWPXH_gStDX6xOR77l1DTDfvnacewV9q39ElryCTCOhyphenhyphentABQGRR9SjF7_dxAkOnoyeuSIS4k7owaQKYczzLyS8SmeAPhF4pz_w1JZzr6kHfEMJ1s0I-L9v_fuA/s1600/P%C3%B4pa,+Vela+e+Quilha+e+C%C3%A3o+Maior.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgqefwtWtWks1AM0ztcWFWPXH_gStDX6xOR77l1DTDfvnacewV9q39ElryCTCOhyphenhyphentABQGRR9SjF7_dxAkOnoyeuSIS4k7owaQKYczzLyS8SmeAPhF4pz_w1JZzr6kHfEMJ1s0I-L9v_fuA/s1600/P%C3%B4pa,+Vela+e+Quilha+e+C%C3%A3o+Maior.jpg" /></a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhmUUU8atYAyo2JV9ESA8BDFoBgN4rcaVMM6Q2wzQDNgA0ZouF6yrHXtVj_1d0RcAe-zhD4Q3l70ynqgReDUnl2AWK3tN5mnIAGw1c8Xjed3VCV1Iqq9TB-G-zL4vjgZL12WtV4sDd_2BU/s1600/sirius+e+o+pared%C3%A3o+do+navio.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Stellarium</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esse paredão, essa muralha de estrelinhas tímidas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não se apresenta em linha reta, não,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem ao contrário, é como se figurasse madeiras encaixadas,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">madeiras e madeiras formando quase um desencaixe, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">um ziguezague </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de estrelas emparedadas...</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sendo assim,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">podemos compreender muitíssimo bem</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o porquê, a razão das ilustrações antigas mostrarem </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">essa madeira de estrelas figurando a Pôpa de um Navio.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E penso ser interessante enfatizarmos o fato</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de que estamos diante da Pôpa do Navio, realmente,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e não daquilo que poderíamos pensar como a Proa.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Não, é a Pôpa.</span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiF-Qdw_n9uIq7A9huLE6o8RhHOtUafpZAaUVqe73W5ISqviXKMBqck7fADrVJRK4bxEHKRxjtSS0ShwIdMDkTI-Cx2Pyxp5DnNcvXtlJnR8_Att5EMIpPo378On5m485Q2DR31F_zaSwdW/s1600/figura+antigacel4full.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiF-Qdw_n9uIq7A9huLE6o8RhHOtUafpZAaUVqe73W5ISqviXKMBqck7fADrVJRK4bxEHKRxjtSS0ShwIdMDkTI-Cx2Pyxp5DnNcvXtlJnR8_Att5EMIpPo378On5m485Q2DR31F_zaSwdW/s1600/figura+antigacel4full.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></span></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US" style="line-height: 14px;">The image for the "Historical Essay" is taken from<span class="apple-converted-space"> </span></span><a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel.htm" style="text-decoration: none;"><span lang="EN-US" style="line-height: 14px;">Andreas Cellarius,</span><span class="apple-converted-space"><span lang="EN-US" style="line-height: 14px;"> </span></span><i><span lang="EN-US" style="line-height: 14px;">Harmonia macrocosmica,</span></i><span class="apple-converted-space"><span lang="EN-US" style="line-height: 14px;"> </span></span><span lang="EN-US" style="line-height: 14px;">1661</span></a><span lang="EN-US" style="line-height: 14px;">.</span><br /><span lang="EN-US" style="line-height: 14px;"><o:p></o:p></span><a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/images/cel4full.jpg" style="line-height: 14.25pt; text-decoration: none;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/images/cel4full.jpg</a><br /><span lang="EN-US" style="line-height: 14px;"><br /></span><span lang="EN-US" style="line-height: 14px;"><br /></span><span style="line-height: 19.1875px; text-align: start;"><br /></span></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEii3p-aPrnmNirQJ3dfmXwnb4ZZvnRV5ji3Cvky0JNVri9qBQb5FRH621nGWxAJZp51pUd_uELGa6C_UXLoakmw5roGchuv5Rb9sR9UBFsvVknKdEVcA1jP83ztEuqdGnrbWOJ6YQGlNXps/s1600/sch4full.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEii3p-aPrnmNirQJ3dfmXwnb4ZZvnRV5ji3Cvky0JNVri9qBQb5FRH621nGWxAJZp51pUd_uELGa6C_UXLoakmw5roGchuv5Rb9sR9UBFsvVknKdEVcA1jP83ztEuqdGnrbWOJ6YQGlNXps/s1600/sch4full.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></span></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Julius Schiller, <i>Coelum stellatum Christianum</i>, 1627</span></span></div>
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<a href="http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm" style="text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.lindahall.org/events_exhib/exhibit/exhibits/stars/cel_sch.htm</span></span></a></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E podemos também perceber</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o porquê, a razão de o Navio apresentar-se </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">através Pôpa, Quilha e Vela</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Puppis, Carina e Vela -,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e não, nunca, jamais nos apresentar sua Proa....,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">simplesmente porque a Proa não existe...</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e a narração do Mito já nos conta sobre essa realidade</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">através um texto de Richard H. Allen</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">traduzido literalmente por mim</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a partir de</span></span></div>
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<span style="background-color: white;"><span style="background-color: transparent; color: #073763; font-family: Arial, sans-serif; line-height: normal;"><span style="line-height: 18px;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Argo_Navis*.html">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Argo_Navis*.html</a></span></span><span style="background-color: transparent; color: #073763; font-family: Arial, sans-serif; line-height: 13.5pt;"> </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">:</span></span></div>
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<span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">O Mito sobre Jasão e os 50 Argonautas,</span></span></span><br />
<span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">sobre a construção do Argo Navis</span></span></span><br />
<span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e sobre sua Viagem</span></span></span><br />
<span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">nos diz que</span></span></span><br />
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span style="font-family: Arial, sans-serif;">O Navio parece não ter Proa ....................</span><span style="font-family: 'Times New Roman', serif;"><o:p></o:p></span></i></span></span></div>
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span style="font-family: Arial, sans-serif;">Segundo Aratos, a perda da Proa parece haver ocorrido</span><span style="font-family: 'Times New Roman', serif;"><o:p></o:p></span></i></span></span><br />
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;">when Argo pass'd</span></i><span lang="EN-US" style="font-family: 'Times New Roman', serif; font-size: 12pt;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;">Through Bosporus betwixt the justling rocks —</span></i><span lang="EN-US" style="font-family: 'Times New Roman', serif; font-size: 12pt;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;">All Argo stands aloft in sky</span></i><span lang="EN-US" style="font-family: 'Times New Roman', serif; font-size: 12pt;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;">Part moves dim and starless from the prow</span></i><span lang="EN-US" style="font-family: 'Times New Roman', serif; font-size: 12pt;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;">Up to the mast, but all the rest is bright;</span></i><span lang="EN-US" style="font-family: 'Times New Roman', serif; font-size: 12pt;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #7f6000;"><i><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;"><br /></span></i></span></span></div>
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<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;">Quando Argo Navis passou através o Estreito de Bósforo </span></i></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;">e rochas desmoronaram, </span></i></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;">o Navio foi virado e naufragou....; </span></i></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;">e subiu aos céus </span></i></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;">porém sem estrelas apresentando desde a Proa até o mastro.</span></i></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;">... mas todo o resto é brilhante!</span></i><span style="color: #3d85c6; font-weight: bold;"><o:p></o:p></span></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><i><span style="color: #7f6000;"><b><br /></b></span></i></span></div>
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<span style="background-color: white; font-family: Arial, sans-serif;"><span style="color: #073763;">Assim R. H. Allen comenta </span></span><br />
<span style="background-color: white; font-family: Arial, sans-serif;"><span style="color: #073763;">sobre os dizeres de Aratos acerca esta circunstância.</span></span></div>
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<span style="background-color: white;"><span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Aparentemente, as rochas desmoronaram exatamente sobre a Proa </i></span></span></span></div>
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<span style="background-color: white;"><span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>- daí uma explicação mítica sobre seu desaparecimento....</i></span></span></span></div>
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<span style="background-color: white;"><span style="line-height: 19.1875px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i> quando o Navio foi levado aos céus, segundo o Mito.</i></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: #073763; color: #bf9000;"><br /></span><span style="background-color: #073763; color: #bf9000;"><img alt="Carina Navis" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_carina_navis.jpg" height="473" width="640" /></span><span style="background-color: #073763; color: #bf9000;"><br /></span><span style="background-color: white; color: #274e13;"><a href="http://www.aradergalleries.com/detail.php?id=3645">http://www.aradergalleries.com/detail.php?id=3645</a><br /><span style="line-height: normal;">Johann Bayer — Carina Navis</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Podemos pensar em várias circunstâncias</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para nos fazer compreender a razão pela qual o Navio não nos apresenta sua Proa.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Bem, se vemos o Navio a partir de sua Pôpa</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e seguindo em direção mais ao sul,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">podemos pensar que a Proa existe, sim, mas já se encontra</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">desaparecida na 'dobra' do horizonte, digamos assim.</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Porém, podemos também pensar que </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Mito acima tenha vindo até o inconsciente coletivo da antiguidade</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">simplesmente pelo fato de que</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">uma constelação bem mais ao sul não pode ser apreciada,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como um todo, pelos povos moradores do hemisfério norte...</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Daí o fato de que várias ilustrações sobre o Navio</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mostram Pôpa e Quilha (incluindo Canopus, a estrela-alpha Argo Navis)</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- algumas (dependendo da Latitude ao Norte) ainda mostram a Vela...</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">mas nunca mostram a Proa, apenas a induzem.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img src="http://www.ianridpath.com/atlases/urania/urania32.jpg" height="445" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.ianridpath.com/atlases/urania/urania32.jpg" style="text-decoration: none;">http://www.ianridpath.com/atlases/urania/urania32.jpg</a> </span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma outra questão que pode repousar</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre o Mito nos contando que a Proa foi esmagada pelas pedras...,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é o fato de que ...........</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">.......... podemos perceber que existe a vizinhança</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> composta pela imensa constelação do Centauro </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e exatamente no lugar onde a Proa do Navio poderia ter sido inserida</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> podemos ver uma das patas do Centauro </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">escudando nosso Cruzeiro do Sul!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Buscando compreender melhor sobre a questão da ausência de Proa</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> (já manifestada através o Mito) </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">do Navio, </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">pude constatar que Carinae Nebula acontece exatamente no lugar </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">onde a Proa poderia se situar! </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 13.5pt;"><span style="background-color: white;">(Veja em </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">http://oceudomes.blogspot.com.br/2014/05/a-grande-nebulosa-em-carina.html)</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Da mesma forma, </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">constatamos que as chamadas Pleiades do Sul ou Austrais</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">acontecem exatamente no lugar</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">onde a Quilha poderia ter seu término!</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Veja em</span></span></div>
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<span style="background-color: white;"></span></div>
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<span style="background-color: white; line-height: 18px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/05/pleiades-em-touro-e-pleiades-em-carina.html)</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ou seja, quando as Ilustrações do passado </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">mostrando um tanto de fumaça/poeira</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> de pedras desmoronadas por sobre a Proa..., </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">não seria esta 'fumaça', esta poeira,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">a visão aguçada sobre a Grande Nebulosa Carina</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e ratificada sobre as Pleiades do Sul? </span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Será?</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Leia mais sobre o Tema</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Por que não existe Proa em Argo Navis, o Navio?</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acessando meu Trabalho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span></div>
<span style="line-height: 18px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/05/por-que-nao-existe-proa-em-argo-navis-o.html</span></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgTgiycSIhvG2ONo-5WRIUMscmMwgv6OeQm65RTLPxOlW6tvdSsjYoaBYhGxvHKJoaJnxU2TVYkM7lGLVJTnxX03EtQVU6ZyEEiScmEHYuCAF3hfxewrQq_09NktSm2OEYr5W7t-AE8E3E/s1600/on+avio+e+eta+carinae+nebula.jpg" imageanchor="1" style="background-color: white; margin-left: 1em; margin-right: 1em;"><span style="color: #073763;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgTgiycSIhvG2ONo-5WRIUMscmMwgv6OeQm65RTLPxOlW6tvdSsjYoaBYhGxvHKJoaJnxU2TVYkM7lGLVJTnxX03EtQVU6ZyEEiScmEHYuCAF3hfxewrQq_09NktSm2OEYr5W7t-AE8E3E/s1600/on+avio+e+eta+carinae+nebula.jpg" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;">http://media.skysurvey.org/interactive360/index.html</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Programa Sky Survey anotado e marcado por mim no lugar de Eta Carinae Nebula</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Caro Leitor,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Observe as Ilustrações abaixo</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>- em ambas sendo apontado o Objeto Messier 46</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>(que, por sua vez, fica bem próximo ao Objeto Messier 47)</b> -,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e perceba primeiramente que todo o Navio vem envolvido</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pelo braço da Via Lactea que corre de norte a sul;</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e também perceba que</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">os Objetos M46 e M47 encontram-se bem próximos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">à constelação Monoceros, o Unicórnio</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(embora a estrela mais próxima a nos guiar será Sírius!),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">enquanto sabemos que M93 encontra-se bem próximo</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">à constelação Canis Major, o Cão Maior!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Quer dizer,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">esses três Objetos Messier em Puppis</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontram-se já bem ao norte de toda a constelação do Navio</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- ou seja, em situações ainda praticamente bem visíveis</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para os observadores/moradores do hemisfério norte.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É também interessante que possamos perceber</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- observando desde os Objetos Messier 46 e 47</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(ponto bem ao norte de Puppis ou de Argo Navis, o Navio)</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">até as Plêiades do Sul e da Grande Nebulosa Carina</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> (pontos bem ao sul da constelação Carina) -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o quão extensa é a antiga constelação Argo Navis, o Navio,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de tal forma que, infelizmente (a meu ver),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">foi desmembrada em Puppis, Carina e Vela</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o que (a meu ver) </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">descaracterizou-a, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">despiu-a de sua identidade estelar própria, que pena.</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Esta constelação, o Navio, </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">fazia parte do grupo de 48 constelações </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">relacionado por Ptolomeu. </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">La Caille, porém, dividiu o Navio em<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Carina, Vela e Puppis: Quilha, Vela e Popa.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">De qualquer forma,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">eu sou muito feliz por morar no hemisfério sul</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">e poder usufruir da visão maravilhosa</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">do Navio, como um todo!</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><span style="font-family: Arial, Helvetica, sans-serif;">.</span></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi-AAz156KO6nrdyr8GfOrVB4raFKvry186yU0o6lSaPCyx00e2ATpQDZ7J_b2vuWhX586QL1VZfuaSKM5NBTLP34d8L5_jJChJOC-6lUOHVTZOsRbySEy5Tsn9yG_jFNZgxfkomgvPYhE/s1600/a+via+lactea,+com+ilustra%C3%A7%C3%B5es.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi-AAz156KO6nrdyr8GfOrVB4raFKvry186yU0o6lSaPCyx00e2ATpQDZ7J_b2vuWhX586QL1VZfuaSKM5NBTLP34d8L5_jJChJOC-6lUOHVTZOsRbySEy5Tsn9yG_jFNZgxfkomgvPYhE/s1600/a+via+lactea,+com+ilustra%C3%A7%C3%B5es.png" /></span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">ARGO NAVIS, O NAVIO</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o navio no qual Jasão trouxe o Velocino de Ouro para Colquita - e dizem que foi o primeiro navio a ser construído.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações relacionado por Ptolomeu. </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">La Caille, porém, dividiu o Navio em<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Carina, Vela e Puppis: Quilha, Vela e Popa<o:p></o:p></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">Argo Navis</b><span style="line-height: 19.1875px; text-align: start;"> era uma grande </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="line-height: 19.1875px; text-align: start;"> meridional, representava o navio utilizado pelos </span><a href="http://pt.wikipedia.org/wiki/Argonautas" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Argonautas">argonautas</a><span style="line-height: 19.1875px; text-align: start;"> em suas viagens. Foi dividida em </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Carina" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Carina">Carina</a><span style="line-height: 19.1875px; text-align: start;">(quilha), </span><a href="http://pt.wikipedia.org/wiki/Puppis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Puppis">Puppis</a><span style="line-height: 19.1875px; text-align: start;"> (popa) e </span><a href="http://pt.wikipedia.org/wiki/Vela_(constela%C3%A7%C3%A3o)" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Vela (constelação)">Vela</a><span style="line-height: 19.1875px; text-align: start;"> (velame); as </span><a href="http://pt.wikipedia.org/wiki/Designa%C3%A7%C3%A3o_de_Bayer" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Designação de Bayer">designações de Bayer</a><span style="line-height: 19.1875px; text-align: start;">, entretanto, não foram mudadas, de modo que α e β estão em Carina, γ e δ em Vela, ε em Carina, ζ em Puppis e assim por diante. Por outro lado, </span><a href="http://pt.wikipedia.org/wiki/Pyxis" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Pyxis">Pyxis</a><span style="line-height: 19.1875px; text-align: start;">, a constelação da Bússola, embora ocupe uma área que havia sido considerada como os mastros do Argo, possui designações de Bayer próprias.</span></span></span></div>
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<a href="http://pt.wikipedia.org/wiki/Argo_Navis" style="text-decoration: none;"><span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Argo_Navis</span></span></a></div>
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<span style="background-color: white; line-height: 14px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As 88 Constelações, Cartas Celestes</span></span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">PUPPIS, POPA</span></b><span style="color: #073763;"><o:p></o:p></span><br /><b style="color: #073763;"><br /></b><b style="color: #073763;"><br /></b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Posicionamento:<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 6h2m / 8h26m Declinação -11<sup>o</sup>.0 / -50<sup>o</sup>.8<o:p></o:p><br /><br /><br /><b><br /></b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito</b><o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa o navio</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> no qual Jasão trouxe o Velocino de Ouro para Colquita</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> - e dizem que foi o primeiro Navio a ser construído.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p><br /><b><br /></b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação, o Navio, fazia parte do grupo de 48 constelações r</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">elacionado por Ptolomeu. </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Porém, La Caille dividiu o Navio em<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Carina, Vela e Puppis, Quilha, Vela e Popa<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Pôpa é facilmente identificável </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a partir da localização de Canopus, estrela-alpha do Navio Argos </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e situada na parte de Carina, a Quilha,</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> e buscando o padrão de estrelas que ficam ao norte. </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Do ponto de vista de quem está no hemisfério sul, </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é possível se identificar a Popa já muito próxima a Sirius, </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a estrela-alpha do Cão Maior, </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">até chegar a Canopus, a estrela-alpha do Navio).<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Existem alguns aglomerados abertos nesta constelação</span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> sendo que o mais brilhante é M47, visível a olho nu. </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> M46 e M93 são mais pálidos </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém também considerados como objetos interessantes </span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a serem observados. </span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> M46 e M47 situam-se próximos a Sirius </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que atua enquanto ponto de referência, é claro).<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Fronteiras:<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Puppis situa-se entre as constelações </span></span><br />
<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Canis Major, Columba, Pictor, Carina, Vela, Pyxix, Hydra, Monoceros<o:p></o:p></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M46, M47 e M93,</b></span></span><br />
<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></span><br />
<span style="background-color: white;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>EM PUPPIS, A PÔPA DO NAVIO</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b><b>M 46 - Aglomerado Aberto, em Puppis</b><o:p></o:p><br />e</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M 47 - Aglomerado Aberto, em Puppis</b><o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Estes dois Aglomerados podem ser vistos a olho nu </span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e bem esfumaçadamente,<br /> próximos ao Cão Maior e sua estrela-Alpha, Sirius.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> http://www.stellarium.org/pt/</span><br />
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<span style="background-color: white; line-height: 14px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></span></div>
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<span style="background-color: white;">http://www.ipac.caltech.edu/2mass/gallery/m46atlas.jpg</span><br />
<span style="background-color: white;"><a href="https://www.blogger.com/null" name="m81">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
<span style="background-color: white;"><a href="https://www.blogger.com/null" name="m81"><br /></a></span><span style="background-color: white;"><a href="https://www.blogger.com/null" name="m81"><br /></a></span></div>
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<h1>
<span style="background-color: white;">Messier 46</span></h1>
<span style="background-color: white;"><i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M46 (NGC 2437)</i>, type 'f', in <a href="http://messier.obspm.fr/map/Pup.html">Puppis</a></span></center>
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<a href="http://messier.obspm.fr/Jpg/m46.jpg" style="background-color: white;"><img align="right" alt="[m46.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m46.jpg" /></a><br />
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left"><span style="background-color: white;">Right Ascension</span></th><td align="center"><span style="background-color: white;">07 : 41.8 (h:m)</span></td></tr>
<tr><th align="left"><span style="background-color: white;">Declination</span></th><td align="center"><span style="background-color: white;">-14 : 49 (deg:m)</span></td></tr>
<tr><th align="left"><span style="background-color: white;">Distance</span></th><td align="center"><span style="background-color: white;">5.4 (kly)</span></td></tr>
<tr><th align="left"><span style="background-color: white;">Visual Brightness</span></th><td align="center"><span style="background-color: white;">6.0 (mag) </span></td></tr>
<tr><th align="left"><span style="background-color: white;">Apparent Dimension</span></th><td align="center"><span style="background-color: white;">27.0 (arc min)</span></td></tr>
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<span style="background-color: white;"><br /></span><span style="background-color: white;">Discovered 1771 by Charles Messier.</span><br />
<span style="background-color: white;"><br /></span><span style="background-color: white;">Messier 46 (M46, NGC 2437) was the first object <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> discovered after he had published the first edition of <a href="http://messier.obspm.fr/xtra/history/m-cat.html">his list</a> (<a href="http://messier.obspm.fr/m/m001.html">M1</a>-<a href="http://messier.obspm.fr/m/m045.html">M45</a>). He <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M46">added this one</a> to his catalog on February 19, 1771, three days after presenting it to the academy, together with three more Messier objects, <a href="http://messier.obspm.fr/m/m047.html">M47</a>, <a href="http://messier.obspm.fr/m/m048.html">M48</a>, and <a href="http://messier.obspm.fr/m/m049.html">M49</a>.</span><br />
<span style="background-color: white;"><br /></span><span style="background-color: white;">LEIA MAIS</span><br />
<span style="background-color: white;">em</span><br />
<span style="background-color: white;">http://messier.obspm.fr/m/m046.html</span><br />
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 2437 - M 46 - Aglomerado Aberto Puppis</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 07h40m Declinação -14<sup>o</sup>.46<o:p></o:p></span></span></div>
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<span style="background-color: white; line-height: 14px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 6,6 Magnitude fotográfica da mais brilhante estrela 10,8 Distância kpc 1,66 Diâmetro 27’ Tipo Espectral B8<o:p></o:p></span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 46</b> (também conhecido como <b>M46</b> ou <b>NGC 2437</b>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Puppis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Puppis">Puppis</a>. Foi descoberto por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em <a href="http://pt.wikipedia.org/wiki/1771" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1771">1771</a>. Está a cerca de 5 400 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da Terra e é composto por mais de 500 estrelas, sendo que 150 são de magnitude entre 10 e 13. Sua idade é estimada em 300 milhões de anos.<span class="reference" id="cite_ref-seds_1-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> <a href="http://pt.wikipedia.org/wiki/NGC_2438" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 2438">NGC 2438</a> está localizada em Messier 43 perto da sua borda do norte, mas provavelmente não há relação física entre eles visto que NGC 2438 possui uma <a href="http://pt.wikipedia.org/wiki/Velocidade_radial" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Velocidade radial">velocidade radial</a> diferente da do aglomerado.<span class="reference" id="cite_ref-majaess2007_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-majaess2007-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> <span class="reference" id="cite_ref-kiss2008_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-kiss2008-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> Esse caso é um exemplo de coincidência na linha de visão, assim como o caso de <a href="http://pt.wikipedia.org/wiki/NGC_2818" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 2818">NGC 2818</a>.<span class="reference" id="cite_ref-majaess2007_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-majaess2007-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> <span class="reference" id="cite_ref-mermilliod2001_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-mermilliod2001-4" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<span style="line-height: 22.3999996185303px;">Foi o primeiro </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Objeto do céu profundo">objeto do céu profundo</a><span style="line-height: 22.3999996185303px;"> descoberto pelo astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="line-height: 22.3999996185303px;"> após a apresentação da primeira versão de seu </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Catálogo Messier">catálogo</a><span style="line-height: 22.3999996185303px;"> à </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Acad%C3%A9mie_des_sciences" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Académie des sciences">Real Academia de Ciências da França</a><span style="line-height: 22.3999996185303px;">, em 16 de fevereiro de 1771; o </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a><span style="line-height: 22.3999996185303px;"> foi adicionado ao catálogo apenas três dias após a apresentação, juntamente com </span><a href="http://pt.wikipedia.org/wiki/Messier_47" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 47">Messier 47</a><span style="line-height: 22.3999996185303px;">, </span><a href="http://pt.wikipedia.org/wiki/Messier_48" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 48">Messier 48</a><span style="line-height: 22.3999996185303px;"> e </span><a href="http://pt.wikipedia.org/wiki/Messier_49" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 49">Messier 49</a><span style="line-height: 22.3999996185303px;">.</span><span class="reference" id="cite_ref-seds_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 46</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M46a.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 46"><img alt="Messier 46" data-file-height="346" data-file-width="478" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/0b/M46a.jpg/250px-M46a.jpg" height="181" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0b/M46a.jpg/375px-M46a.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/0/0b/M46a.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 46</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1771" style="background: none; color: #0b0080; text-decoration: none;" title="1771">1771</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Puppis" style="background: none; color: #0b0080; text-decoration: none;" title="Puppis">Puppis</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">07<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 41,8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span><span class="reference" id="cite_ref-seds_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-14° 49′<span class="reference" id="cite_ref-seds_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">5400 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> (1700 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,0</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">27'</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">15 anos-luz<span class="reference" id="cite_ref-seds_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">300 milhões de anos<span class="reference" id="cite_ref-seds_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Nº estrelas</td><td style="background-color: #f8f8f8;">500<span class="reference" id="cite_ref-seds_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M46, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 2437.<span class="reference" id="cite_ref-seds_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_46#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 46"><img alt="Messier 46" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Puppis_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Puppis constellation map.png" data-file-height="3409" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Puppis_constellation_map.png/250px-Puppis_constellation_map.png" height="333" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Puppis_constellation_map.png/375px-Puppis_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Puppis_constellation_map.png/500px-Puppis_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 14px;">http://pt.wikipedia.org/wiki/Messier_46</span><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 47</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M47 (NGC 2422)</i>, type 'd', in <a href="http://messier.obspm.fr/map/Pup.html">Puppis</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">07 : 36.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-14 : 30 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.2 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">30.0 (arc min)</td></tr>
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Discovered before 1654 by Giovanni Batista Hodierna.</div>
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Open cluster Messier 47 (M47, NGC 2422) is a coarse, bright cluster which can be glimpsed with the naked eye under good conditions as a dim nebulosity.</div>
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M47 was discovered before 1654 by <a href="http://messier.obspm.fr/xtra/similar/hodierna.html">Hodierna</a> who described it as "a Nebulosa between the two dogs"; this fact, however, remained secret until 1984 when his book came to light. So <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> discovered this cluster independently on February 19, 1771, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M47">described it</a> as cluster of stars brighter than those of apparently neighbored <a href="http://messier.obspm.fr/m/m046.html">M46</a>. But Messier did a sign error when computing the position of M47, so that it was a <a href="http://messier.obspm.fr/missing.html">missing object</a> until 1959 when it was identified by <a href="http://messier.obspm.fr/xtra/Bios/morris.html">T.F. Morris</a> (together with the also missing <a href="http://messier.obspm.fr/m/m048.html">M48</a>). It is interesting that despite Messier's error, <a href="http://messier.obspm.fr/xtra/Bios/cherschel.html">Caroline Herschel</a> observed and identified M47 at least twice in early 1783. Several historians have reported that M47 had been previously identified by<a href="http://messier.obspm.fr/xtra/Bios/thomas.html">Oswald Thomas</a> in 1934, but this is apparently a confusion with that author's identification of M48. As a consequence of Messier's error, <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> also independently rediscovered it on February 4, 1785, and <a href="http://messier.obspm.fr/xtra/similar/herschel.html">gave it the number</a> H VIII.38.</div>
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Messier's erroneous position was also surviving in many catalogs, including John Herschel's GC (as GC 1594) and Dreyer's NGC (NGC 2478), although there was no object, or as <a href="http://messier.obspm.fr/xtra/Bios/jherschel.html">John Herschel</a> (in his Notes on the GC) <a href="http://messier.obspm.fr/Mdes/dm047.html#GC">put it</a>, "This cluster has not since been observed. It is probably a very loose and poor one."</div>
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LEIA MAIS</div>
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http://messier.obspm.fr/m/m047.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgWpRmgE6DN0X8iJ1FAsMaF_nVyBJSHjZ8AjTWTfjptfI77xr_kWPFROk4ojmi7HFSZCBOacDUCy9oMLefs__XaSchh01Kjfv2YliVlT-CUNfDB3pGx8OTO821tg-vUc2JgMs7RsYLwb2U/s1600/M47.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgWpRmgE6DN0X8iJ1FAsMaF_nVyBJSHjZ8AjTWTfjptfI77xr_kWPFROk4ojmi7HFSZCBOacDUCy9oMLefs__XaSchh01Kjfv2YliVlT-CUNfDB3pGx8OTO821tg-vUc2JgMs7RsYLwb2U/s1600/M47.png" /></a></div>
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<span style="background-color: white; line-height: 14px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></span></div>
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<span style="color: #660000;"><b>Messier 47 (NGC 2422, NGC 2478</b></span><span style="color: #252525;">) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Puppis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Puppis">Puppis</a> a 1 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da Terra. Foi descoberto por <a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de <a href="http://pt.wikipedia.org/wiki/1654" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1654">1654</a>, porém a descoberta só foi atribuída a ele em <a href="http://pt.wikipedia.org/wiki/1984" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1984">1984</a>. <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> descoberiu o aglomerado independentemente em <a href="http://pt.wikipedia.org/wiki/19_de_fevereiro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="19 de fevereiro">19 de fevereiro</a> de <a href="http://pt.wikipedia.org/wiki/1771" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1771">1771</a>.</span></div>
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Messier 47 possui um diâmetro de 12 anos-luz e tem uma idade estimada em 78 milhões de anos. Contém cerca de 50 estrelas, sendo que a mais brilhante é de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe</a> B2 e tem uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude</a> de 5,7.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 47</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:MESSIER_047_2MASS.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 47, projeto 2MASS"><img alt="Messier 47, projeto 2MASS" data-file-height="1800" data-file-width="1800" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f1/MESSIER_047_2MASS.jpg/250px-MESSIER_047_2MASS.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f1/MESSIER_047_2MASS.jpg/375px-MESSIER_047_2MASS.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f1/MESSIER_047_2MASS.jpg/500px-MESSIER_047_2MASS.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 47, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1654" style="background: none; color: #0b0080; text-decoration: none;" title="1654">1654</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Puppis" style="background: none; color: #0b0080; text-decoration: none;" title="Puppis">Puppis</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">07<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 36,6<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-14° 30′</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">1600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (490 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">5,2</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">30,0 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">6 anos-luz</td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">78 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td>Nº estrelas</td><td style="background-color: #f8f8f8;">50</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M47, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 2422</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Puppis_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Puppis constellation map.png" data-file-height="3409" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Puppis_constellation_map.png/250px-Puppis_constellation_map.png" height="333" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Puppis_constellation_map.png/375px-Puppis_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d9/Puppis_constellation_map.png/500px-Puppis_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="background-color: white; line-height: 14px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m93atlas.jpg</span></span><br />
<span style="background-color: white; line-height: 14px;"><a href="https://www.blogger.com/null" name="m81" style="line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
<span style="background-color: white; line-height: 14px;"><a href="https://www.blogger.com/null" name="m81" style="line-height: normal;"><br /></a></span><span style="background-color: white; line-height: 14px;"><a href="https://www.blogger.com/null" name="m81" style="line-height: normal;"><br /></a></span></div>
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Messier 93</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M93 (NGC 2447)</i>, type 'g', in <a href="http://messier.obspm.fr/map/Pup.html">Puppis</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">07 : 44.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-23 : 52 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">3.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">22.0 (arc min)</td></tr>
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Discovered by Charles Messier in 1781.</div>
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Messier 93 (M93, NGC 2447) is a nice open star cluster in constellation Puppis.</div>
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As one of the last deepsky objects found by him personally, open cluster M93 was discovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M93">cataloged by him</a> on March 20, 1781.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m093.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiv1ZAFG9ou497lcU6sC51dB6Zk3jR5cP3pU63HgWliNzp8VPYojdpqWb189mriuczJ4q0Sf1CNZVrYKQXpJn71JbE49u6ceggoWoHBNIDhBIgF52_cdfJx6X4XnI_xub_0BSlR85Mp9gc/s1600/M93,+em+Puppis.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiv1ZAFG9ou497lcU6sC51dB6Zk3jR5cP3pU63HgWliNzp8VPYojdpqWb189mriuczJ4q0Sf1CNZVrYKQXpJn71JbE49u6ceggoWoHBNIDhBIgF52_cdfJx6X4XnI_xub_0BSlR85Mp9gc/s1600/M93,+em+Puppis.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><b>Messier 93</b> (also known as <b>M93</b> or <b>NGC 2447</b>) is an <a href="http://en.wikipedia.org/wiki/Open_cluster" style="background-image: none; text-decoration: none;" title="Open cluster">open cluster</a> in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Puppis" style="background-image: none; text-decoration: none;" title="Puppis">Puppis</a>. It was discovered by <a href="http://en.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> in 1782.</span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">M93 is at a distance of about 3,600 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-image: none; text-decoration: none;" title="Light year">light years</a> from Earth and has a spatial radius of some 10 to 12 light years. Its age is estimated at some 100 million years.</span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><a href="http://en.wikipedia.org/wiki/Walter_Scott_Houston" style="background-image: none; text-decoration: none;" title="Walter Scott Houston">Walter Scott Houston</a> described its appearance as follows:<sup class="reference" id="cite_ref-WSH_1-0" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_93#cite_note-WSH-1" style="background-image: none; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Some observers mention the cluster as having the shape of a starfish. With a fair-sized telescope, this is its appearance on a dull night, but [a four-inch refractor] shows it as a typical star-studded galactic cluster.</span></span></div>
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<tr><th colspan="2" style="background: rgb(255, 255, 192); font-size: 15px; text-align: center; vertical-align: top;">Messier 93</th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><a class="image" href="http://en.wikipedia.org/wiki/File:Messier_object_093.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Messier object 093.jpg" data-file-height="300" data-file-width="300" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Messier_object_093.jpg/250px-Messier_object_093.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/f/f0/Messier_object_093.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/f/f0/Messier_object_093.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a></td></tr>
<tr><th colspan="2" style="background: rgb(255, 255, 192); text-align: center; vertical-align: top;">Observation data (J2000.0 <a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">epoch</a>)</th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Right ascension">Right ascension</a></th><td style="vertical-align: top;">07<sup style="font-size: 10px; line-height: 1;">h</sup> 44.6<sup style="font-size: 10px; line-height: 1;">m</sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declination">Declination</a></th><td style="vertical-align: top;">−23° 52′</td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Distance_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Distance (astronomy)">Distance</a></th><td style="vertical-align: top;">3.6 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Light_year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light year">kly</a> (1.1 kpc)</td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a> <small>(V)</small></th><td style="vertical-align: top;">6.0</td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Apparent dimensions <small>(V)</small></th><td style="vertical-align: top;">22.0′</td></tr>
<tr><th colspan="2" style="background: rgb(255, 255, 192); text-align: center; vertical-align: top;">Physical characteristics</th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Radius</th><td style="vertical-align: top;">10</td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Estimated age</th><td style="vertical-align: top;">100 million years<sup class="noprint Inline-Template Template-Fact" style="font-size: 10px; line-height: 1; white-space: nowrap;">[<i><a href="http://en.wikipedia.org/wiki/Wikipedia:Citation_needed" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Wikipedia:Citation needed"><span title="This claim needs references to reliable sources. (February 2007)">citation needed</span></a></i>]</sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Other designations</th><td style="vertical-align: top;">NGC 2447</td></tr>
<tr><td colspan="2" style="background: rgb(255, 255, 192); text-align: center; vertical-align: top;">See also: <a href="http://en.wikipedia.org/wiki/Open_cluster" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Open cluster">Open cluster</a>, <a href="http://en.wikipedia.org/wiki/List_of_open_clusters" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="List of open clusters">List of open cluster</a></td></tr>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Messier_93" style="text-decoration: none;">http://en.wikipedia.org/wiki/Messier_93</a></span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">visite meu Trabalho</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sobre a Antiga Constelação de Argo Navis, o Navio,</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span></span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 14px;">http://sobreargonavis.blogspot.com.br/</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Hemisphaerium Coeli Australe in quo Fixarum loca secundum Eclipticae ductum ad anum 1730 . .</span></h2>
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<a href="http://www.raremaps.com/gallery/detail/35290/Hemisphaerium_Coeli_Australe_in_quo_Fixarum_loca_secundum_Eclipticae_ductum/Doppelmayr.html" style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px; text-decoration: none;"><img alt="Hemisphaerium Coeli Australe in quo Fixarum loca secundum Eclipticae ductum ad anum 1730 . ." src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi0TDoMGyTZ6mq7jzaXWx0RKmsgKVRIRXJXpq2ekaaX40T6hB0xW2VdHEpFWyzJ40aujKuE1hz1mDkr0wva21symtdTqjQHL_TL2djBMjhKyXpZY2_PU0-rE9G9sQ5YKf4PrqVio4d0KHpa/s1260/MAPA+CELESTE+GRANDE.jpg" height="1044" id="Image2_img" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(7, 55, 99); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; visibility: visible;" width="1240" /> </a><span style="color: #0000ee; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">http://www.raremaps.com/gallery/detail/35290/Hemisphaerium_Coeli_Australe_in_quo_Fixarum_loca_secundum_Eclipticae_ductum/Doppelmayr.html</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763; line-height: 18px;">Nice example of Johanne Doppelmayr's map of the Southern Skies, with the constellations shown and the various stars illustrated in gold. Dopplemayr's decorative celestial chart illustrates the southern sky form the south ecliptic pole to ecliptic. The constellations are delineated based upon the catalogue of Johannes Hevelius and include Orion, Scorpio, Taurus, Eridanus and the Southern Cross. The constellations include some unusal additions, including the Peacock, Toucan, and a lovely unicorn called Monoceros.</span></span><br />
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<a href="http://www.sothebys.com/en/auctions/ecatalogue/2013/russian-paintings-l13112/lot.136.html" style="text-decoration: none;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">http://www.sothebys.com/en/auctions/ecatalogue/2013/russian-paintings-l13112/lot.136.html</span></span></a></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">Ivan Konstantinovič Ajvazovskij (1817 - 1900)</span><span lang="EN-US"><br />“Ship in Stormy Sea” 1858</span></span><span lang="EN-US"><o:p></o:p></span></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b>Janine Milward</b></span><br /><div style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 16.8pt;">
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<img alt="Carina Navis" height="473" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_carina_navis.jpg" width="640" /></div>
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<span style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="color: #073763;"><span style="line-height: 22.3999996185303px;">http://www.aradergalleries.com/detail.php?id=3645</span></span></span></div>
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<span style="background-color: white; font-family: Georgia, 'Times New Roman', Times, serif; font-size: 14px; font-weight: bold;"><span style="color: #073763;">Johann Bayer — Carina Navis</span></span><span style="background-color: white; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="color: #073763;"><span style="line-height: 22.3999996185303px;"><br /></span></span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b><br /></b></span><br /><div align="center" class="MsoNormal" style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 18px;">
<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-14219023206265882222014-09-06T08:37:00.003-07:002015-01-04T10:00:58.503-08:00Pisces<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em continuidade aos nossos estudos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">estaremos hoje comentando</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre M74,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o único Objeto Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acolhido pela constelação dos Peixes.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação dos Peixes</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pode ser compreendida como o Cenário</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que acolhe as situações contadas </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">no Mito de Andromeda </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- pois que a Princesa encontra-se acorrentada à uma pedra</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">numa praia dos mares piscianos,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">onde o monstro-marinho, a Baleia Cetus, mora.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">As outras constelações que fazem parte deste Mito</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontram-se nas redondezas:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Cepheus e Cassiopeia (pais de Andromeda),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Perseus e o Cavalo Alado Pegasus.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Boa Leitura e Bons Estudos!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts" style="color: #274e13; text-decoration: none;">https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts</a><br /><span style="color: #274e13;">Andromeda e Perseus - Guido Reni, 1635</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Andrômeda era a filha de Cefeus, rei da Etiópia, e de Cassiopeia. </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">Por causa dos boatos espalhados por Cassiopéia</span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;"> de que a beleza de Andrômeda superava a das Nereidas, </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">Netuno enviou um mostro marinho, Cetus, a Baleia, para devastar aquele país. </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: black; font-family: 'Times New Roman';"></span><span style="font-family: Arial, Helvetica, sans-serif;">Porém, Netuno fez a promessa de libertar o país dessa devastação</span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;"> caso Andromeda fosse oferecida em sacrifício, </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">sendo acorrentada a uma rocha, </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">para ser devorada pelo monstro marinho. </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">No entanto, Perseus soube desse caso </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">e salvou Andrômeda de seu tormento matando o monstro </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">e o transformando em pedra ao lhe mostrar a cara da Medusa. </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Ambos, Perseus e Andrômeda, alçaram vôo alto, sobre Pegasus, o cavalo alado, </span><br style="color: black; font-family: 'Times New Roman';" /><span style="font-family: Arial, Helvetica, sans-serif;">e se dirigiram para o altar onde se casaram.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - CARJ</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">PISCES, OS PEIXES</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Enquanto estavam sentados às margens do Rio Eufrates, Vênus e seu filho, Cupido, viram Tifão, o inimigo dos Deuses, se aproximando. Ambos mergulharam no rio e foram salvos de se afogarem por dois peixes, que mais tarde foram colocados nos céus por Vênus, em agradecimento.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Os babilônios, os assírios e os persas representavam este grupo de estrelas por dois peixes.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Para os egípcios, esse asterismo registrava a aproximação da primavera e da estação da pesca. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">No zodíaco de Denderah, está representado por dois grandes peixes ligados por uma faixa, em meio de um retângulo que simboliza a água. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">No tumulo de Ramsés VI é representado por um único peixe.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Embora não seja uma constelação que apresente estrelas proeminentes, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Peixes faz parte das constelações zodiacais </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">desde os tempos das mais antigas civilizações.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A constelação de Pisces faz fronteira com Áries, Triangulum, Andrômeda, Pegasus, Aquário e Cetus.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Devido à Precessão, o equinócio vernal situa-se em Peixes, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>na linha de sua estrela Omega Piscium.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Segundo o astrônomo Ronaldo Rogério de Freitas Mourão, em sua 6<sup>a</sup>. edição do Atlas Celeste, página 163, podemos ler:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><o:p> </o:p><b><i>Ponto Vernal.</i></b><i> Ponto da esfera celeste, situado na interseção da eclíptica com o equador, na qual o Sol, em seu movimento aparente anual, passa do hemisfério sul para o norte. O ponto vernal serve de origem para as ascensões retas e as longitudes celestes, intervindo desse modo nas definições de tempo. O ponto vernal é habitualmente designado como equinócio da primavera, equinócio vernal, primeiro ponto de Áries.</i></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Excerto da constelação dos Peixes </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- Mario Jaci Monteiro, Cartas Celestes, As Constelações</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> Asterismo </b>nomeado de<b> Circlet, Pequeno Círculo</b>, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">composto pelas estrelas Gamma, Beta, Teta, Iota, 19, Lambda e Kappa Piscium<b><o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Este Pequeno Círculo - um dos dois Peixes </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- marca a proximidade do Ponto Vernal, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">o cruzamento entre as Linhas do Equador celestial e da Eclíptica. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Em lugares de céus escuros e transparentes, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">podemos sempre bem visualizar este Pequeno Círculo, realmente.</span></div>
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LEIA MAIS SOBRE ESTE TEMA,</div>
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acessando minha Postagem</div>
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<a href="https://www.blogger.com/goog_696229657">em</a></div>
<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://oceudomes.blogspot.com.br/2014/07/lua-no-ponto-vernal.html">http://oceudomes.blogspot.com.br/2014/07/lua-no-ponto-vernal.html</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- <span style="line-height: 13.5pt;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M74,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OBJETO MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO PISCES:</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m74atlas.jpg" /></div>
<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;">http://www.ipac.caltech.edu/2mass/gallery/m74atlas.jpg</span></span><br />
<a href="https://www.blogger.com/null" name="m81">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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<h1>
Messier 74</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M74 (NGC 628)</i>, type Sc, in <a href="http://messier.obspm.fr/map/Psc.html">Pisces</a></center>
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<a href="http://messier.obspm.fr/Jpg/m74.jpg"><img align="right" alt="[m74.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m74.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">01 : 36.7 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+15 : 47 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">35000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">10.2x9.5 (arc min)</td></tr>
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Discovered 1780 by Pierre Méchain.</div>
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Messier 74 (M74, NGC 628) is one of the nicest examples of so-called "grand-design" spiral galaxies seen face-on, so that its spiral structure stands out conspicuously. With its comparatively low surface brightness, it is one of the more difficult objects in Messier's catalog, situated in constellation Pisces.</div>
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<a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> found M74 at the end of September 1780. He reported his discovery to his </div>
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friend, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who determined its position and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M74">included it</a> in his catalog on October 18, 1780. It is among the first "Spiral Nebulae" recognized;<a href="http://messier.obspm.fr/xtra/Bios/rosse.html">Lord Rosse</a> lists it as one of 14 "spiral or curvilinear nebulae" discovered before 1850.</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">LEIA MUITO MAIS</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acessando</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://messier.obspm.fr/m/m074.html</span></span><br />
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<a href="http://www.esa.int/Our_Activities/Space_Science/Herschel/Herschel_images_promise_bright_future" style="color: #2d83d5; font-family: 'Lucida Grande', 'Lucida Sans Unicode', Arial, Helvetica, Sans, FreeSans, Jamrul, Garuda, Kalimati; font-size: 12px; margin: 0px; padding: 0px;" target="_blank"><img alt="A galáxia Messier 74 (M74) vista em dois diferentes comprimentos de onda do espectro infravermelho. M74 (conhecida também como NGC 628) é uma galáxia espiral que dista 24 milhões de anos-luz da Terra na constelação de Peixes. As imagens em infravermelho da SPIRE mostram a poeira entre as estrelas, mostrando claramente os braços espirais. Na imagem vemos pontos tênues que são galáxias distantes. Estas galáxias também contem poeira que irradiam no infravermelho, mas como estão bem mais distantes, não conseguimos discernir as estruturas destas galáxias." class="size-medium wp-image-3952" src="http://eternosaprendizes.com/wp-content/uploads/2009/07/ESA_Herschel_SPIRE250_MIPS160_M74_fig3_H-720x540.jpg" height="540" style="border-bottom-left-radius: 4px; border-bottom-right-radius: 4px; border-top-left-radius: 4px; border-top-right-radius: 4px; border: 0px; margin: 0px; padding: 0px;" title="ESA_Herschel_SPIRE250_MIPS160_M74_fig3_H" width="720" /></a><br />
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A galáxia Messier 74 (M74) vista em dois diferentes comprimentos de onda do espectro infravermelho (à esquerda a visão do SPITZER e à direita a imagem do Herschel). A M74 (conhecida também como NGC 628) é uma galáxia espiral que dista 24 milhões de anos-luz da Terra na constelação de Peixes. As imagens em infravermelho da SPIRE mostram a poeira entre as estrelas, mostrando claramente os braços espirais. Na imagem vemos pontos tênues que são galáxias distantes. Estas galáxias também contem poeira que irradiam no infravermelho, mas como estão bem mais distantes, não conseguimos discernir as estruturas destas galáxias.</div>
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<span style="color: #8d8b8b; font-family: Lucida Grande, Lucida Sans Unicode, Arial, Helvetica, Sans, FreeSans, Jamrul, Garuda, Kalimati;"><span style="line-height: 16.7999992370605px;"><a href="http://eternosaprendizes.com/2009/07/18/esaherschel-novas-imagens-prometem-um-futuro-de-descobertas-brilhantes/">http://eternosaprendizes.com/2009/07/18/esaherschel-novas-imagens-prometem-um-futuro-de-descobertas-brilhantes/</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 628 = M74 - Galáxia Espiral</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Galáxia bem grande porém de magnitude 11.0, situada bem próxima à estrela Eta Piscium<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Messier 74</b> (também conhecida como <b>NGC 628</b>)</span></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> na constelação de <a href="http://pt.wikipedia.org/wiki/Pisces" style="background-image: none; color: #274e13; text-decoration: none;" title="Pisces">Pisces</a>.<span class="reference" id="cite_ref-seds_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span> Foi descoberta em setembro de <a href="http://pt.wikipedia.org/wiki/1780" style="background-image: none; color: #274e13; text-decoration: none;" title="1780">1780</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-image: none; color: #274e13; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>. Ele reportou sua descoberta a <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que listou a galáxia em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Catálogo Messier">catálogo</a>.<span class="reference" id="cite_ref-seds_1-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">M74 possui dois braços espirais bem definidos e é usada como protótipo de uma <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Gal%C3%A1xia_espiral_de_grande_desenho&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral de grande desenho (página não existe)">galáxia espiral de grande desenho</a>.<span class="reference" id="cite_ref-seds_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Devido a sua baixa luminosidade, é um dos mais difíceis objetos Messier para se visualizar. É necessário um </span><a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Céu noturno">céu noturno</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em excelentes condições para ver seu núcleo. Sua estrutura em braços espirais começa a ser notada a partir de </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> amadores de 4 polegadas de abertura, embora seus aglomerados estelares azuis possam ser reconhecidos apenas com telescópios de 16 poelagas de abertura. </span><a href="http://pt.wikipedia.org/wiki/Maratona_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Maratona Messier">Maratonistas Messier</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, observadores que tentam visualizar todos os 110 objetos Messier em uma única noite, frequentemente não são capazes de visualizar a galáxia.</span><span class="reference" id="cite_ref-seds_1-7" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13; line-height: 19.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_74">http://pt.wikipedia.org/wiki/Messier_74</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi4KXHJZUyHSWSp2G6GcerD7XtcX_3eXFSukUpqdNtQe2E9nOKRtlPMIVpwNsFTgPkEZoQ1IbyT8wAGxvEDPWpig_UPFcpQ_iYcCwCVZsQs6Oucnm1mCI7__Kjx9Yz7laI24II3dMhDZ4Y/s1600/Messier_74_by_HST.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi4KXHJZUyHSWSp2G6GcerD7XtcX_3eXFSukUpqdNtQe2E9nOKRtlPMIVpwNsFTgPkEZoQ1IbyT8wAGxvEDPWpig_UPFcpQ_iYcCwCVZsQs6Oucnm1mCI7__Kjx9Yz7laI24II3dMhDZ4Y/s1600/Messier_74_by_HST.jpg" height="616" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/galaxy/spiral/2007/41/image/a/" rel="nofollow" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/galaxy/spiral/2007/41/image/a/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="font-family: Arial, Helvetica, sans-serif;">NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration. Acknowledgment: R. Chandar (University of Toledo) and J. Miller (University of Michigan)</span></td></tr>
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<small>Messier 74 em imagem do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></small></td></tr>
<tr><td scope="row" valign="top">Descoberto por</td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span class="reference" id="cite_ref-seds_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Data de descoberta</td><td valign="top">de <a href="http://pt.wikipedia.org/wiki/1780" style="background: none; color: #0b0080; text-decoration: none;" title="1780">1780</a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Dados observacionais (J2000)</b></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pisces" style="background: none; color: #0b0080; text-decoration: none;" title="Pisces">Pisces</a><span class="reference" id="cite_ref-seds_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Tipo</td><td valign="top">SA(s)c<span class="reference" id="cite_ref-ned_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td valign="top">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 36<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 41,8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td valign="top">15° 47′ 01″<span class="reference" id="cite_ref-ned_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Distância</td><td valign="top">30 ± 6 milhões de <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-hendryetal2005_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-hendryetal2005-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><br />
(9,3 ± 1,8 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)</td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background: none; color: #0b0080; text-decoration: none;" title="Desvio para o vermelho">Redshift</a></td><td valign="top">657 km/s<span class="reference" id="cite_ref-ned_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td valign="top">10,0<span class="reference" id="cite_ref-ned_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><td scope="row" valign="top">Dimensões</td><td valign="top">10′,5 × 9′,5<span class="reference" id="cite_ref-ned_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Características físicas</b></th></tr>
<tr><td scope="row" valign="top">Raio</td><td valign="top">~47 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr><td scope="row" valign="top">Número de estrelas</td><td valign="top">100 bilhões<span class="reference" id="cite_ref-APOD_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-APOD-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Outras denominações</b></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 628, <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 1149, PGC 5974.<span class="reference" id="cite_ref-ned_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-ned-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><b>Mapa</b></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 74"><img alt="Messier 74" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Pisces_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Pisces constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Pisces_constellation_map.png/240px-Pisces_constellation_map.png" height="240" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Pisces_constellation_map.png/360px-Pisces_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Pisces_constellation_map.png/480px-Pisces_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></a></div>
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O grande número de regiões HII encontrados na galáxia indicam que o processo de <a href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Formação estelar">formação estelar</a> está vívida. Tais regiões também podem ser visualizadas como pontos em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ultravioleta" style="background: none; color: #0b0080; text-decoration: none;" title="Ultravioleta">ultravioleta</a>. A simetria notável de toda galáxia, possívelmente construída por "ondas de <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Densidade_estelar&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Densidade estelar (página não existe)">densidade estelar</a>", indicam que a galáxia está influenciada por outras <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background: none; color: #0b0080; text-decoration: none;" title="Galáxia">galáxias</a> vizinhas: quando <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Nuvem_interestelar&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Nuvem interestelar (página não existe)">nuvens de gás</a> são afetadas por estas ondas, se arranjam em cristas que se espiralam. Nesse processo, as nuvens de gás podem se fundir com outras, incentivando a formação estelar.<span class="reference" id="cite_ref-seds_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-seds-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<b><span style="color: #660000;">M74 é a galáxia mais brilhante do <a href="http://pt.wikipedia.org/wiki/Grupo_M74" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Grupo M74">Grupo M74</a></span></b><span style="color: #252525;">, um grupo de 5-7 galáxias que também inclui a galáxia espiral </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Gal%C3%A1xia_peculiar&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Galáxia peculiar (página não existe)">peculiar</a><span style="color: #252525;"> </span><a href="http://pt.wikipedia.org/wiki/NGC_660" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 660">NGC 660</a><span style="color: #252525;"> e as galáxias NGC 660, UGC 891, UGC 1195 e UGGA 20.</span><span class="reference" id="cite_ref-nbg_5-0" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-nbg-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span><span style="color: #252525;"> </span><span class="reference" id="cite_ref-garcia1993_6-0" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-garcia1993-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span><span style="color: #252525;"> </span><span class="reference" id="cite_ref-giuricinetal2002_7-0" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-giuricinetal2002-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">7</a></span><span style="color: #252525;"> M74 está a uma distância de aproximadamente 30 milhões de</span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="color: #252525;"> da </span><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Via Láctea">Via Láctea</a><span class="reference" id="cite_ref-hendryetal2005_3-1" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-hendryetal2005-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><span style="color: #252525;"> e contém cerca de 100 bilhões de </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a><span style="color: #252525;">.</span><span class="reference" id="cite_ref-APOD_4-1" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-APOD-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<span class="mw-headline" id="Poss.C3.ADvel_buraco_negro"><span style="font-size: small;">Possível buraco negro</span></span></h3>
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Em <a href="http://pt.wikipedia.org/wiki/22_de_mar%C3%A7o" style="background: none; color: #0b0080; text-decoration: none;" title="22 de março">22 de março</a> de <a href="http://pt.wikipedia.org/wiki/2005" style="background: none; color: #0b0080; text-decoration: none;" title="2005">2005</a>, foi anunciado<span class="reference" id="cite_ref-chandra2005_16-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_74#cite_note-chandra2005-16" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">16</a></span> que o <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">Observatório de raios-X Chandra</a> observou uma luminosa fonte de raios-x (ULX) em M74, irradiando mais energia de raios-X que uma <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrela de nêutrons</a> em intervalos periódicos de cerca de duas horas. Ela tem uma massa estimada de cerca de 10 000 <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a>. Isso é um indicador de um <a href="http://pt.wikipedia.org/wiki/Buraco_negro_de_massa_intermedi%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Buraco negro de massa intermediária">buraco negro de massa intermediária</a>. Esta seria uma classe pouco comum de buracos negros, com tamanho entre os <a href="http://pt.wikipedia.org/wiki/Buraco_negro_estelar" style="background: none; color: #0b0080; text-decoration: none;" title="Buraco negro estelar">buracos negros estelares</a> e os buracos negros maciços localizados no centro de muitas galáxias. Por causa disso, acredita-se que os buracos negros de massa intermediária não são formados de uma única supernova, mas possivelmente de várias delas. A fonte de raios-X é identificada como CXOU J013651.1 154.547.</div>
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LEIA MUITO MAIS, </div>
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acessando</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: normal; text-align: center;">http://pt.wikipedia.org/wiki/Messier_74</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Two supernovae have been discovered in M74:</b></span></div>
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<li><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://messier.obspm.fr/more/m074_sn2002ap.html">Supernova 2002ap</a> was discovered in M74 on January 29, 2002 by Japanese amateur Yoji Hirose when it was at mag 13.7. This type Ib/c supernova brightened up to mag 12.3 between February 5 and 12, 2002, and was classified as a "hypernova," occurring when progenitor stars of at least 40 solar masses explode.</span></li>
<li><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://messier.obspm.fr/more/m074_sn2003gd.html">Supernova 2003gd</a> was found visually in M74 by Bob Evans on June 12.82 UT, in the morning twilight at Australia as it was 13.2 mag bright, and already fading. This supernova was of type II.</span></li>
<li><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://messier.obspm.fr/m/m074.html">http://messier.obspm.fr/m/m074.html</a></span></li>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Supernovae 2002ap and 200</span>3gd in M74</h2>
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<a href="http://messier.obspm.fr/Pics/Jpg/m74sn2002ap.jpg"><img alt="[SN 2002ap, CfA]" border="0" src="http://messier.obspm.fr/Pics/More/m74sn2002ap_s.jpg" /></a> <a href="http://messier.obspm.fr/Pics/Jpg/m74sn2003gd2.jpg"><img alt="[SN 2003gd, M. Schwartz]" border="0" src="http://messier.obspm.fr/Pics/More/m74sn2003gd2s.jpg" /></a></center>
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Images of M74 with the supernovae 2002ap and 2003gd for comparison. The SN 2002ap image was taken by Harvard CfA astronomers with the 1.2-m telescope on Mt. Hopkins, Arizona. The SN 2003gd image was obtained by <a href="http://www.tenagraobservatories.com/">Mike Schwartz</a>.</div>
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<span style="text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://messier.obspm.fr/more/m074_sne.html">http://messier.obspm.fr/more/m074_sne.html</a></span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/8/87/M74_3.6_5.8_8.0_microns_spitzer.png/220px-M74_3.6_5.8_8.0_microns_spitzer.png" height="610" width="640" /></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="background-color: white; font-size: 14px; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_74#mediaviewer/File:M74_3.6_5.8_8.0_microns_spitzer.png">http://pt.wikipedia.org/wiki/Messier_74#mediaviewer/File:M74_3.6_5.8_8.0_microns_spitzer.png</a></span></span></div>
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<span style="background-color: white;">Messier 74, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Spitzer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Spitzer">Telescópio Espacial Spitzer</a></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_74</span></div>
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<b><span style="color: #660000;">O Grupo M74 (também conhecido como o <i>Grupo NGC 628</i>)</span></b><span style="color: #252525;"> é um pequeno </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Grupo_de_gal%C3%A1xias&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Grupo de galáxias (página não existe)">grupo de galáxias</a><span style="color: #252525;"> na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Pisces" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pisces">Pisces</a><span style="color: #252525;">. A </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #252525;"> em visão frontal </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M74" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M74">M74 (NGC 628)</a><span style="color: #252525;"> é o membro mais brilhante dentro do grupo. Outros membros incluem a peculiar </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #252525;"> </span><a href="http://pt.wikipedia.org/wiki/NGC_660" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 660">NGC 660</a><span style="color: #252525;"> e outras pequenas </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia irregular">galáxias irregulares</a><span style="color: #252525;">.</span><span class="reference" id="cite_ref-nbg_3-1" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-nbg-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span><span style="color: #252525;"> </span><span class="reference" id="cite_ref-garcia1993_1-4" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><span style="color: #252525;"> </span><span class="reference" id="cite_ref-giuricinetal2002_2-7" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span class="mw-headline" id="Membros"><span style="font-size: large;">Membros</span></span></h2>
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A tabela abaixo lista todas as galáxias identificadas e confirmadas como membros do grupo pelo Nearby Galaxies Catalog,<span class="reference" id="cite_ref-nbg_3-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-nbg-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o Lyons Groups of Galaxies (LGG) Catalog,<span class="reference" id="cite_ref-garcia1993_1-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> e três listas de grupos criados pelo Nearby Optical Galaxy sample of Giuricin et al.<span class="reference" id="cite_ref-giuricinetal2002_2-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
<table cellpadding="2" class="wikitable" style="background-color: #f9f9f9; border-collapse: collapse; border: 1px solid rgb(170, 170, 170); color: black; font-family: sans-serif; line-height: 22.3999996185303px; margin: 1em 0px; text-align: center;"><caption style="font-weight: bold;"><b>Membros do Grupo M74</b></caption><tbody>
<tr><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Nome</th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_de_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Classificação de Hubble">Tipo</a><span class="reference" id="cite_ref-ned_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-ned-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">A.R.</a> (J2000)<span class="reference" id="cite_ref-ned_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-ned-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Dec.</a> (J2000)<span class="reference" id="cite_ref-ned_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-ned-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Redshift" style="background: none; color: #0b0080; text-decoration: none;" title="Redshift">Redshift</a> (<a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro" style="background: none; color: #0b0080; text-decoration: none;" title="Quilômetro">km</a>/<a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none; color: #0b0080; text-decoration: none;" title="Segundo">s</a>)<span class="reference" id="cite_ref-ned_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-ned-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a><span class="reference" id="cite_ref-ned_4-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-ned-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M74" style="background: none; color: #0b0080; text-decoration: none;" title="M74">Messier 74</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SA(s)c</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 36<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 42<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+15° 47′ 01″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">657</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10,0</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/NGC_660" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 660">NGC 660</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SB(s)a pec</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 43<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 02<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+13° 38′ 42″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">850</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">19,0</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_1176&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 1176 (página não existe)">UGC 1176</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Im</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 40<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+15° 54′ 17″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">630</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">14,4</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_1195&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 1195 (página não existe)">UGC 1195</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Sc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 27<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+13° 58′ 37″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">774</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">13,9</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_1200&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 1200 (página não existe)">UGC 1200</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">IBm</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 48<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+13° 09′ 22″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">808</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">14,0</td></tr>
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Outras possíveis galáxias membros (galáxias listadas em uma ou duas referências citadas acima) incluem as galáxias irregulares <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_891&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 891 (página não existe)">UGC 891</a>, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_1104&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 1104 (página não existe)">UGC 1104</a>, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_1171&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 1171 (página não existe)">UGC 1171</a>, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_1175&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGC 1175 (página não existe)">UGC 1175</a>, e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGCA_20&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="UGCA 20 (página não existe)">UGCA 20</a>.</div>
<table cellpadding="0" cellspacing="2" class="infobox" style="background: rgb(242, 242, 242); border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; margin: 0px 0px 1em 1em; padding: 0.2em; text-align: center; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da;"><b>Grupo M74</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Pisces" style="background: none; color: #0b0080; text-decoration: none;" title="Pisces">Pisces</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 43<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span><span class="reference" id="cite_ref-garcia1993_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <span class="reference" id="cite_ref-giuricinetal2002_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+14° 22′<span class="reference" id="cite_ref-garcia1993_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <span class="reference" id="cite_ref-giuricinetal2002_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td>Número de Membros</td><td style="background-color: #f8f8f8;">5-7<span class="reference" id="cite_ref-nbg_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-nbg-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> <span class="reference" id="cite_ref-garcia1993_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> <span class="reference" id="cite_ref-giuricinetal2002_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td>Membro Brilhante</td><td style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M74" style="background: none; color: #0b0080; text-decoration: none;" title="M74">Messier 74</a><span class="reference" id="cite_ref-giuricinetal2002_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">Grupo <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 628, LGG 29,<span class="reference" id="cite_ref-garcia1993_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><br />
NOGG H 94,<span class="reference" id="cite_ref-giuricinetal2002_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> NOGG P1 84,<span class="reference" id="cite_ref-giuricinetal2002_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span><br />
NOGG P2 87<span class="reference" id="cite_ref-giuricinetal2002_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Grupo_M74">http://pt.wikipedia.org/wiki/Grupo_M74</a></span></div>
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<img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1211/ngc660_gemini_legacy956.jpg" /></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/ap121110.html">http://apod.nasa.gov/apod/ap121110.html</a></span></div>
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<span style="font-size: large;">Polar Ring Galaxy NGC 660 </span><br /><b>Image Credit: </b><a href="http://www.gemini.edu/">Gemini Observatory, AURA</a>, <a href="http://aftar.uaa.alaska.edu/">Travis Rector</a> (<a href="http://www.uaa.alaska.edu/">Univ. Alaska Anchorage</a>)</center>
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<b>Explanation: </b>NGC 660 is featured in <a href="http://www.gemini.edu/node/11896">this cosmic snapshot</a>, a sharp composite of broad and narrow band filter image data from the Gemini North telescope <a href="http://apod.nasa.gov/apod/ap090219.html">on Mauna Kea</a>. Over 20 million light-years away and swimming within the boundaries of the <a href="http://en.wikipedia.org/wiki/Pisces_(constellation)">constellation Pisces</a>, NGC 660's peculiar appearance marks it as <a href="http://apod.nasa.gov/apod/ap070216.html">a polar ring galaxy</a>. A rare galaxy type, polar ring galaxies have a substantial population of stars, gas, and dust <a href="http://apod.nasa.gov/apod/ap990510.html">orbiting in rings</a> nearly perpendicular to the plane of the galactic disk. <a href="http://arxiv.org/abs/astro-ph/0301391">The bizarre-looking configuration</a> could have been caused by the chance capture of material from a passing galaxy by a disk galaxy, with the captured debris eventually strung out in a rotating ring. The violent gravitational interaction would account for the myriad pinkish star forming regions scattered along NGC 660's ring. <a href="http://www.obspm.fr/actual/nouvelle/apr03/prg.en.shtml">The polar ring component</a> can also be used to explore the shape of the galaxy's otherwise unseen <a href="http://www.solstation.com/x-objects/darkhalo.htm">dark matter halo</a> by calculating the <a href="http://chandra.harvard.edu/xray_astro/dark_matter/index.html">dark matter's</a> gravitational influence on the rotation of the ring and disk. Broader than the disk, NGC 660's ring spans over 50,000 light-years.</div>
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<span style="font-size: large;">Hubble Views Polar Ring Galaxy NGC 660</span></h1>
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<img alt="Hubble Views Galaxy NGC 660" src="http://scitechdaily.com/images/Hubble-Views-Galaxy-NGC-660.jpg" height="532" width="640" /></div>
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This new Hubble image shows a peculiar galaxy known as NGC 660, located around 45 million light-years away from us.</div>
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NGC 660 is classified as a “polar ring galaxy”, meaning that it has a belt of gas and stars around its center that it ripped from a near neighbor during a clash about one billion years ago. The first polar ring galaxy was observed in 1978 and only around a dozen more have been discovered since then, making them something of a cosmic rarity.</div>
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Unfortunately, NGC 660’s polar ring cannot be seen in this image, but has plenty of other features that make it of interest to astronomers – its central bulge is strangely off-kilter and, perhaps more intriguingly, it is thought to harbor exceptionally large amounts of dark matter. In addition, in late 2012 astronomers observed a massive outburst emanating from NGC 660 that was around ten times as bright as a supernova explosion. This burst was thought to be caused by a massive jet shooting out of the supermassive black hole at the center of the galaxy.</div>
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Source: Hubble Space Telescope</div>
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<span style="color: #444444; font-family: sans-serif;"><span style="line-height: 19.6000003814697px;"><a href="http://scitechdaily.com/hubble-views-polar-ring-galaxy-ngc-660/">http://scitechdaily.com/hubble-views-polar-ring-galaxy-ngc-660/</a></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/36551</span></div>
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<span style="color: #274e13;"><span style="font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Les Poissons (Pisces) </span><strong style="font-family: Arial, Helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">John Flamsteed</a><span style="font-family: Arial, Helvetica, sans-serif;"> / </span><span style="font-family: Arial, Helvetica, sans-serif;"> </span><a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">MJ Fortin</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/36551/Les_Poissons_Pisces/Flamsteed-Fortin.html</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1104/m74_baixauli_900.jpg" /></div>
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<b>http://apod.nasa.gov/apod/ap110406.html</b></center>
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<b><span style="font-size: large;">M74: The Perfect Spiral </span></b><br /><b>Credit & <a href="http://apod.nasa.gov/apod/lib/about_apod.html#srapply">Copyright</a>: </b><a href="http://www.cienciadirecta.com/">Descubre Foundation</a>, <a href="http://www.caha.es/">Calar Alto Observatory</a>, <a href="http://observatori.uv.es/">OAUV</a>, <a href="http://astro-photographer.org/">DSA</a>, V. Peris (OAUV), J. L. Lamadrid (<a href="http://cefca.es/">CEFCA</a>), <a href="http://pegasusastronomy.com/">J. Harvey</a> (<a href="http://www.starshadows.com/">SSRO</a>), S. Mazlin (SSRO), I. Rodriguez (<a href="http://pixinsight.com/">PTeam</a>), O. L. (PTeam), J. Conejero (<a href="http://pixinsight.com/">PixInsight</a>).</center>
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<b>Explanation: </b>If not perfect, then this <a href="http://www.seds.org/messier/spir.html">spiral galaxy</a> is at least one of the most photogenic. An <a href="http://nedwww.ipac.caltech.edu/level5/March02/Gordon/Gordon2.html">island universe</a> of about 100 billion stars, 32 million light-years away toward the <a href="http://www.allthesky.com/constellations/pisces/constell.html">constellation Pisces</a>, <a href="http://www.seds.org/messier/m/m074.html">M74 presents</a> a gorgeous <a href="http://apod.nasa.gov/apod/ap010427.html">face-on view</a>. Classified as <a href="http://en.wikipedia.org/wiki/Hubble_sequence">an Sc</a> galaxy, the <a href="http://burro.cwru.edu/Academics/Astr222/Galaxies/Spiral/spiral.html">grand design</a> of M74's graceful <a href="http://asterisk.apod.com/viewtopic.php?f=24&t=18005">spiral</a> arms are traced by bright <a href="http://apod.nasa.gov/apod/ap990402.html">blue star clusters</a> and dark <a href="http://apod.nasa.gov/apod/ap071129.html">cosmic dust</a> lanes. The <a href="http://pixinsight.com/gallery/M74-CAHA/en.html">above image</a> covers half the width of the full Moon and was obtained using 19 hours of exposure on the 1.23-meter telescope at <a href="http://www.caha.es/">Calar Alto Observatory</a> in the <a href="http://en.wikipedia.org/wiki/Sierra_de_Los_Filabres">Sierra de Los Filabres</a> mountain range in Spain. <a href="http://hubblesite.org/newscenter/archive/releases/2007/41/image/a/format/zoom/">Spanning</a> about 30,000 light-years across the face of <a href="http://apod.nasa.gov/apod/ap071201.html">M74</a>, it includes exposures recording emission from <a href="http://www.youtube.com/watch?v=XdbGCBrOCak">hydrogen</a> atoms, <a href="http://heritage.stsci.edu/2007/41/supplemental.html">highlighting</a>the reddish glow of the galaxy's large star-forming regions.</div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-44584880138950582862014-09-06T08:36:00.007-07:002015-01-04T09:48:36.414-08:00Perseus<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O nome Perseus é sempre ligado ao nome Andromeda, não é verdade?</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Andromeda é a figura central de seu Mito,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém não seria um Mito com final feliz</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">caso Perseus não salvasse a Princesa Acorrentada</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ambos se apaixonassem e se casassem</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e fossem felizes para todo sempre,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sempre iluminando os céus estrelados</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">do norte!</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>O Mito de Andromeda e Perseus</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>nos céus estrelados:</b></span><br />
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Stellarium 0.11.1 (para a latitude 21s52 e longitude 43w00) - www.stellarium.org<br />trabalhado no Corel Photo-Paint X3 </span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Fronteiras:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação Perseus faz fronteira com Auriga, Camelopardalis, Cassiopéia, Andromeda, Triangulum, Áries e Taurus</span></div>
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Philippe La Hire, <i>Planisphere celeste,</i> 1705<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Andrômeda era a filha de Cefeus, rei da Etiópia, e de Cassiopeia. </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Por causa dos boatos espalhados por Cassiopéia</span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;"> de que a beleza de Andrômeda superava a das Nereidas, </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Netuno enviou um mostro marinho, Cetus, a Baleia, para devastar aquele país. </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;"><br /></span><span style="color: black; font-family: 'Times New Roman'; font-size: small;"></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Porém, Netuno fez a promessa de libertar o país dessa devastação</span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;"> caso Andromeda fosse oferecida em sacrifício, </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">sendo acorrentada a uma rocha, </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">para ser devorada pelo monstro marinho. </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">No entanto, Perseus soube desse caso </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">e salvou Andrômeda de seu tormento matando o monstro </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">e o transformando em pedra ao lhe mostrar a cara da Medusa. </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Ambos, Perseus e Andrômeda, alçaram vôo alto, sobre Pegasus, o cavalo alado, </span><br style="color: black; font-family: 'Times New Roman'; font-size: medium;" /><span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">e se dirigiram para o altar onde se casaram.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg1vElDGoVvLjRf0Rmk0H0YtzhxY5qqxI76mYUW4UMVFlNNTu_FdXka-GGIDfVrIWm4wxOI4mqS7g3iWarKx-C6F4o5yoEUv5Yli8koFJtSI3_9UC0lYPfVcQI5V0nUsZhPn2xpaQpr4SOx/s1600/andromeda,+perseus+-+guido+reni+-+1635.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" height="640" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEg1vElDGoVvLjRf0Rmk0H0YtzhxY5qqxI76mYUW4UMVFlNNTu_FdXka-GGIDfVrIWm4wxOI4mqS7g3iWarKx-C6F4o5yoEUv5Yli8koFJtSI3_9UC0lYPfVcQI5V0nUsZhPn2xpaQpr4SOx/s640/andromeda,+perseus+-+guido+reni+-+1635.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="512" /></span></a></div>
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts" style="color: #274e13; text-decoration: none;">https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts</a><br /><span style="color: #274e13;">Andromeda e Perseus - Guido Reni, 1635</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Enamorados são Andromeda e Perseus</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que entram em cena</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">através nossos comentários </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Messier que são acolhidos por estas duas constelações.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">leia sobre Andromeda e seus Objetos Messier</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre o Mito de Andromeda e Perseus em sua inteireza, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acessando</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com.br/2014/09/m31-m32-e-m110-galaxia-andromeda-e-duas.html">http://oceudomes.blogspot.com.br/2014/09/m31-m32-e-m110-galaxia-andromeda-e-duas.html</a></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e leia sobre Perseus e seus Objetos Messier</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- M34 e M76 -, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nesta Postagem ora sendo apresentada a você.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px;">Imagem invertida em suas cores originais</span><br />
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<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/38529/Perseus/Bayer.html</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Title: </strong>[Perseus]</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="background-color: white;"><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">PERSEUS, O CAMPEÃO</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Posicionamento:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 1h26m / 4h46m Declinação +30<sup>o</sup>.9 / +58<sup>o</sup>.9<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Perseus, era filho de Júpiter e Danae, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">portanto, um semideus </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">a quem Mercúrio deu de presente espada, capa e asas nos pés </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e também o escudo pertencente à Minerva. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O herói matou a Medusa ao cortar sua cabeça </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e mais tarde, salvou Andrômeda,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> com quem se casou e teve alguns filhos. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(Saiba mais sobre o Mito de Andromeda e Perseus,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">acessando meu Trabalho </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> http://sobreandromeda.blogspot.com.br/2013/11/as-constelacoes-que-fazem-parte-do-mito.html)</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Quando retornava para sua casa,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> ele matou acidentalmente seu próprio avô </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e endoideceu de tanta dor, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">mas Júpiter apiedou-se dele </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e o colocou entre as estrelas.<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhKNUwPCBYuYD7U7BPkhsz_S_RUV9Fa11FnnZl8S1UBawGjg809vl2I6clW9F5NPaHf1jOeOqnQS3ZFerDthBu53OFRvawXZtiykXFeNTn7SzEnGQMUQBYWWSg0OO4rP2piU1UJ41TIyzU/s1600/PER+(1).gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhKNUwPCBYuYD7U7BPkhsz_S_RUV9Fa11FnnZl8S1UBawGjg809vl2I6clW9F5NPaHf1jOeOqnQS3ZFerDthBu53OFRvawXZtiykXFeNTn7SzEnGQMUQBYWWSg0OO4rP2piU1UJ41TIyzU/s1600/PER+(1).gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"><a href="http://www.iau.org/static/public/constellations/gif/PER.gif">http://www.iau.org/static/public/constellations/gif/PER.gif</a></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M34 E M76</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO PERSEUS</b></span><br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m34atlas.jpg" /></div>
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http://www.ipac.caltech.edu/2mass/gallery/m34atlas.jpg</div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 34</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M34 (NGC 1039)</i>, type 'd', in <a href="http://messier.obspm.fr/map/Per.html">Perseus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m34.jpg"><img align="right" alt="[m34.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m34.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">02 : 42.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+42 : 47 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.4 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">35.0 (arc min)</td></tr>
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Discovered by Giovanni Batista Hodierna before 1654.</div>
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Open star cluster Messier 34 (M34, NGC 1039) is an intermediate aged open cluster of about 100 stars (according to H.S. Hogg), and lies about 1,400 light years and is scattered over 35 arc minutes, more than the diameter of the full Moon. This angular diameter corresponds to a linear 14 light years; Wallenquist has estimated a little more (42' corresponding to 18.5 light years).</div>
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M34 was probably first found by <a href="http://messier.obspm.fr/xtra/similar/hodierna.html">Giovanni Batista Hodierna</a> before 1654, and independently rediscovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> in on <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M34">August 25, 1764</a>.</div>
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Open cluster M34 can quite easily be found (even with the naked eye under good conditions as a faint nebulous patch) as it lies just north of the line from Algol (Beta Persei) to Gamma Andromedae.</div>
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http://messier.obspm.fr/m/m034.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhCHrIWRGusp9LaPmydbmu7thBl8b8rUh_ZwgHRVHp8SqAANtm9AhRh08gMRo2g8KJ7Bi1XlNG5zUX_kwzoGP8SosU3AY540T26Th8NI6vX-6AOvyvuCjNB8mZi630fNxQIsb4pUE7Kfi8/s1600/m34+-+perseus.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhCHrIWRGusp9LaPmydbmu7thBl8b8rUh_ZwgHRVHp8SqAANtm9AhRh08gMRo2g8KJ7Bi1XlNG5zUX_kwzoGP8SosU3AY540T26Th8NI6vX-6AOvyvuCjNB8mZi630fNxQIsb4pUE7Kfi8/s1600/m34+-+perseus.jpg" /></a></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> http://www.stellarium.org/pt/</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1039 = M34 - Aglomerado Aberto</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Um aglomerado aberto e contendo cerca de 80 estrelas.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Aglomerado Aberto - Perseus<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 03h21m Declinação +48<sup>o</sup>.32<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 2,3 Distância kpc 0,17</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Diâmetro 240’ Tipo Espectral B1<o:p></o:p></span><br />
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 34</b> (também conhecido como <b>M34</b> ou <b>NGC 1039</b>) é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-image: none; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> localizado na constelação de <a href="http://pt.wikipedia.org/wiki/Perseus" style="background-image: none; text-decoration: none;" title="Perseus">Perseus</a>. Foi descoberto por<a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background-image: none; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a> antes de <a href="http://pt.wikipedia.org/wiki/1654" style="background-image: none; text-decoration: none;" title="1654">1654</a> e incluido por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> no seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> em <a href="http://pt.wikipedia.org/wiki/1764" style="background-image: none; text-decoration: none;" title="1764">1764</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A M34 está a uma distância de 1.400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a> e é constituído por 100 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrelas" style="background-image: none; text-decoration: none;" title="Estrelas">estrelas</a>. Abrange cerca de 35 ' no céu, o que equivale a ráio verdadeiro de 7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>. O aglomerado só é visível a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-image: none; text-decoration: none;" title="Olho nu">olho nu</a> em condições muito escuras, fora das luzes da cidade. É bem visto com <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Bin%C3%B3culos" style="background-image: none; text-decoration: none;" title="Binóculos">binóculos</a>.</span><br />
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;">Aglomerado aberto M34</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Giovanni_Battista_Hodierna" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Battista Hodierna">Giovanni Battista Hodierna</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Perseus" style="background: none; color: #0b0080; text-decoration: none;" title="Perseus">Perseus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">02<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42.1<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+42° 46′</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">1.400 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">al</a> (0.4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">5.5</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">35.0′</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">7 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">al</a></td></tr>
<tr style="vertical-align: top;"><td>Nº estrelas</td><td style="background-color: #f8f8f8;">100</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 1039</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 34"><img alt="Messier 34" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Perseus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Perseus constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/250px-Perseus_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/375px-Perseus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/500px-Perseus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_34"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_34</span></a><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://pt.wikipedia.org/wiki/Ficheiro:M34_2mass_atlas.jpg">http://pt.wikipedia.org/wiki/Ficheiro:M34_2mass_atlas.jpg</a></span><br />
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<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://www.ipac.caltech.edu/2mass/gallery/messiercat.html" rel="nofollow">http://www.ipac.caltech.edu/2mass/gallery/messiercat.html</a> Atlas Image [or Atlas Image mosaic] courtesy of 2MASS/UMass/IPAC-Caltech/NASA/NSF.</span></td></tr>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m76atlas.jpg" /><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 76</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Planetary Nebula</a> M76 (NGC 650)</i>, type 3+6, in <a href="http://messier.obspm.fr/map/Per.html">Perseus</a></center>
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<b><span style="font-size: large;">Little Dumbbell Nebula</span></b></center>
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<tr><th align="left">Right Ascension</th><td align="center">01 : 42.4 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+51 : 34 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">3.4 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">10.1 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">2.7x1.8 (arc min)</td></tr>
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Dicovered by Pierre Méchain in 1780.</div>
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Planetary Nebula Messier 76 (M76, NGC 650/651) is one of the faintest Messier Objects, and one of only four planetary nebulae in Messier's catalog, situated in the Eastern part of constellation Perseus.</div>
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M76 was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on September 5, 1780, who reported it to <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who observed it on October 21, 1780, determined its position and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M76">added it to his catalog</a>. While Méchain found it to be a nebula without stars, Messier thought it was composed of small stars with some nebulosity, probably being fooled by foreground or background stars. <a href="http://messier.obspm.fr/xtra/Bios/rosse.html">Lord Rosse</a> erroneously suspected to have detected some spiral structure in this nebula. In 1866, <a href="http://messier.obspm.fr/xtra/Bios/huggins.html">William Huggins</a>, the pioneer of spectroscopy, found its spectrum to be gaseous, showing Nebulium lines. Pioneer astrophotographer <a href="http://messier.obspm.fr/xtra/Bios/roberts.html">Isaac Roberts</a> found that this was not a double, but a single nebula, and first suspected it might be a broad ring seen edgewise. In 1918, <a href="http://messier.obspm.fr/xtra/Bios/curtis.html">Heber D. Curtis</a> correctly classified it as a planetary nebula for the first time.</div>
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M76 is among the fainter Messier objects. It is known under the names <b>Little Dumbbell Nebula</b> (the most common), Cork Nebula, Butterfly Nebula, and Barbell Nebula, and it was given two NGC numbers ..............</div>
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LEIA MAIS</div>
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acessando</div>
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<a href="http://messier.obspm.fr/m/m076.html">http://messier.obspm.fr/m/m076.html</a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiApFvQnLMlCidpKeZhesMWEg-Apk8I_-M8LcaWNUZKOjSzvvEblmsms6MNw4lOmT7s_41GBW5qsOcavZhHdYP_DDqU1gUnaINDWaYTQ3jEPRxOgqj2kQ67xfutaoQpm1Z6A4tzRjRgu6Y/s1600/Perseus.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiApFvQnLMlCidpKeZhesMWEg-Apk8I_-M8LcaWNUZKOjSzvvEblmsms6MNw4lOmT7s_41GBW5qsOcavZhHdYP_DDqU1gUnaINDWaYTQ3jEPRxOgqj2kQ67xfutaoQpm1Z6A4tzRjRgu6Y/s1600/Perseus.jpg" /></a></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> http://www.stellarium.org/pt/</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 650/1 - M 76 - Nebulosa Planetária</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 01h40m Declinação +51<sup>o</sup>.28<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP Dimensão 1,5 Magnitude 20 Magnitude da Estrela associada 17 Distância em anos-luz 15,0</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Uma nebulosa planetária pálida e denominada The Little Dumbbell.</b></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEizhG44qgyKzhM2h2yHztarWb9YAAXS3qIcoA4K7EFZ-bihSuHkDYtnNILiVoxUzO7La0kCnVyRO_brQOMM4KoudQ7-Pa869fPhoCbheCkrQ4Klr_O1Mard1_O_qz0nYE09hsmdb0D2N9U/s1600/m76,+em+Perseus.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEizhG44qgyKzhM2h2yHztarWb9YAAXS3qIcoA4K7EFZ-bihSuHkDYtnNILiVoxUzO7La0kCnVyRO_brQOMM4KoudQ7-Pa869fPhoCbheCkrQ4Klr_O1Mard1_O_qz0nYE09hsmdb0D2N9U/s1600/m76,+em+Perseus.jpg" /></a></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 18px;"> http://www.stellarium.org/pt/</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Pequena Nebulosa do Haltere</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (</span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 76</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 650/651</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) é uma </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> que tem cerca de 1 ano-luz de diametro e está a cerca de 3 a 5 mil anos-luzes da Terra. É reconhecida como uma Nebulosa Planetária assim como seu homônimo mais brilhante, a M27 (a </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa do Haltere">Nebulosa do Haltere</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">).</span><br />
<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">..........................................</span><br />
<span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><br /></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Sua aparência é semelhante à da </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;" title="Nebulosa do Haltere">nebulosa do Haltere</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que justifica seu nome como a "Pequena Nebulosa do Haltere".</span><br />
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<table cellpadding="2" cellspacing="0" class="infobox" style="background: rgb(242, 242, 242); border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 11px; margin: 0px 0px 1em 1em; padding: 0.2em; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Perseus" style="background: none; color: #0b0080; text-decoration: none;" title="Perseus">Perseus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 42<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 24,00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+51° 34′ 31,00″</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">10,1</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">2 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">al</a> (780 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>) <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">2.7 × 1.8 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a> <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Raio">Raio</a></td><td style="background-color: #f8f8f8;">0,617 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">al</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">Magnit. absol.</a></td><td style="background-color: #f8f8f8;">-0,6 (± 0,4</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M76, NGC 650/651</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pequena Nebulosa do Haltere"><img alt="Pequena Nebulosa do Haltere" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Perseus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Perseus constellation map.png" data-file-height="2559" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/250px-Perseus_constellation_map.png" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/375px-Perseus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/09/Perseus_constellation_map.png/500px-Perseus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Pequena_Nebulosa_do_Haltere">http://pt.wikipedia.org/wiki/Pequena_Nebulosa_do_Haltere</a></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em Tempo, Caro Leitor:</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M27, Dumbbell Nebula, a Nebulosa dos Halteres,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pode ser encontrada</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em meu Trabalho sobre</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Vulpecula et Anser, a Raposa e o Ganso,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/08/vulpecula-et-anser-raposa-e-o-ganso.html</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><img alt="File:M76-RL5-DDmin-Gamma-LRGB 883x628.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f0/M76-RL5-DDmin-Gamma-LRGB_883x628.jpg/800px-M76-RL5-DDmin-Gamma-LRGB_883x628.jpg" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://en.wikipedia.org/wiki/File:M76-RL5-DDmin-Gamma-LRGB_883x628.jpg">http://en.wikipedia.org/wiki/File:M76-RL5-DDmin-Gamma-LRGB_883x628.jpg</a></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18.234375px; text-align: start;">Image of planetary nebula M76 (</span><a class="external free" href="http://www.princeton.edu/~rvdb/images/NJP/m76.html" rel="nofollow">http://www.princeton.edu/~rvdb/images/NJP/m76.html</a><span style="line-height: 18.234375px; text-align: start;">) taken by Robert J. Vanderbei.</span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<b><br /></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br /><div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 18px;"><a href="http://www.raremaps.com/gallery/enlarge/36137" style="color: #274e13; text-decoration: none;">http://www.raremaps.com/gallery/enlarge/36137</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<strong>Title: </strong>Andromede, Persee, Le Triangle (Andromeda, Perseus & Triangle)<br />
<strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">MJ Fortin</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-13719549620671445092014-09-06T08:36:00.003-07:002015-01-04T08:37:54.409-08:00Pegasus<div class="MsoNormal">
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<span style="font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Em continuidade aos nossos comentários</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acolhidos pelas constelações</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que fazem parte do Mito de Andromeda,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">por que não tentarmos observar</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M15, o único Objeto Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">na constelação do Cavalo Alado, Pegasus?!</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">O Objeto Messier 15</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">pode ser encontrado bem na fronteira</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">entre a constelações de Pégaso</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e as constelações Delfim e Cavalo Menor</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">- a partir da estrela-epsilon Pegasi, Enif, o nariz do Cavalo Alado,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e a estrela mais brilhante desta constelação.</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="background-color: white;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span style="font-size: large;">O Mito de Andromeda</span></span></b></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Andrômeda era a filha de Cefeus, rei da Etiópia, e de Cassiopeia. Por causa dos boatos espalhados por Cassiopéia de que a beleza de Andrômeda superava a das Nereidas, Netuno enviou um mostro marinho, Cetus, a Baleia, para devastar aquele país. Porém, Netuno fez a promessa de libertar o país dessa devastação caso Andromeda fosse oferecida em sacrifício, sendo acorrentada a uma rocha, para ser devorada pelo monstro marinho. No entanto, Perseus soube desse caso e salvou Andrômeda de seu tormento matando o monstro e o transformando em pedra ao lhe mostrar a cara da Medusa. Ambos, Perseus e Andrômeda, alçaram vôo alto, sobre Pegasus, o cavalo alado, e se dirigiram para o altar onde se casaram.</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts" style="color: #274e13; text-decoration: none;">https://www.facebook.com/MuseoImmaginarioArtisenzaTempo?ref=ts&fref=ts</a><br />Andromeda e Perseus - Guido Reni, 1635</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes - CARJ</span></div>
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<span style="background-color: white;"><span style="color: #660000; font-family: Arial, sans-serif;"><b>PEGASUS, O CAVALO ALADO</b></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;"><b>Posicionamento:</b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h5m / 0h13m Declinação +2<sup>o</sup>.2 / +36<sup>o</sup>.3<o:p></o:p></span></span></div>
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<b><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">O Mito de Pegasus, o Cavalo Alado<o:p></o:p></span></span></b></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Dizem que Pegasus nasceu a partir do sangue da Medusa quando Perseus cortou fora sua cabeça. Foi também cavalgando o Cavalo Alado Pegasus que Perseus pôde salvar Andromeda de sua morte pelo monstro marinho, Cetus, nos mares dos Peixes.</span></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> Mais tarde, o cavalo foi domado e cavalgado por Bellerofonte que se cansou das questões pertinentes à Terra e tentou voar em direção aos céus porém caiu. Pegasus, no entanto, continuou sua cavalgada, entrando no céu e tomando seu lugar entre as estrelas.<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><a href="http://www.raremaps.com/gallery/detail/35069/Pagase_Le_Petit_Cheval_Le_Dauphin_Pegasus_Pisces_and_Equuleus/Flamsteed-Fortin.html" style="text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/35069/Pagase_Le_Petit_Cheval_Le_Dauphin_Pegasus_Pisces_and_Equuleus/Flamsteed-Fortin.html</span></a></span></span><br />
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><strong style="line-height: normal; text-align: start;">Map Maker: </strong><span style="line-height: normal; text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; line-height: normal; text-align: start; text-decoration: none;">John Flamsteed</a><span style="line-height: normal; text-align: start;"> / </span><a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; line-height: normal; text-align: start; text-decoration: none;">MJ Fortin</a></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Detailed star chart of Pegasus, Pisces and Equuleus, from Fortin's <em>Atlas Celeste de Flamsteed </em>. . , published in Paris. </span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">John Flamsteed was the first Astronomer Royal at the London Observatory, winning out over Edmund Halley and Isaac Newton</span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;"><b>Fronteiras:</b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">A constelação de Pegasus faz fronteira com Andrômeda, Lacerta, Cygnus, Vulpecula, Delphinus, Equuleus, Aquário e Peixes</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Pegasus é uma constelação muito fácil de ser reconhecida por apresentar um proeminente quadrado formado por três membros Alpha Pegasi, Markab, Beta Pegasi, Scheat e Gamma Pegasi, Algenib, e ainda acolhendo a estrela Alpha Andromedae, Alpheratz. <o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Este Asterismo é chamado de O Quadrado de Pegasus:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Imagem extraída do Facebook e sem créditos, infelizmente</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD"><b>Markab</b></span><span lang="ES-TRAD"><b>. Alpha Pegasi. </b><o:p></o:p></span></span></div>
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<span lang="PT"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 23h 03,8m - Declinação +15<sup>o</sup> 05’<o:p></o:p></span></span></div>
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<span lang="PT"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,57 - Distância 109 anos-luz<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela branca situada na asa de Pegaso. De Marka, Navio ou Veículo ou também Retornando de Longe. Em outra versão, a Sela, vocábulo árabe para designar o dorso de Pegaso.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">Scheat</span><span lang="EN-US">. Beta Pegasi. Estrela Variável.</span></b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela de amarelo profundo e irregularmente variável (de 2,1 a 3,0) e distante 210 anos-luz, situada na perna esquerda de Pegaso. O Peito, nome árabe.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma das quatro estrelas que compõem o Grande Quadrado do Cavalo Alado (as outras são Alpheratz (ou Sirrah) que Pegasus compartilha com Andrômeda (sua Alpha), a estrela-alpha Pegasi, Markab e a estrela-gamma, Algenib.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="ES-TRAD"><b>Algenib</b></span><span lang="ES-TRAD"><b>. Gamma Pegasi.</b><o:p></o:p></span></span></div>
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<span lang="ES-TRAD"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude 2.84<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma estrela branca situada na ponta da Asa de Pegaso. De Al Janah, a Asa, ou Al Jamb, o Lado. <span lang="PT">Significa Aquele que Carrega. A Asa do Cavalo Alado.<o:p></o:p></span></span></div>
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<span lang="PT"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Alpheratz</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span lang="PT"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Uma estrela situada entre Andrômeda e Pegasus - Alpha Andromedae<o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 00h07,3 - Declinação +28’58<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,15 - Distância 90 anos-luz<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A cabeça de Andrômeda e parte do Cavalo Alado, Pegasus. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> É uma estrela colocada na constelação de Andrômeda</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> mas que possui seu grande simbolismo em relação ao conceito de Andrômeda. <o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M15,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O OBJETO MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO PEGASUS</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O Objeto Messier 15</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">pode ser encontrado bem na fronteira</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">entre a constelações de Pégaso</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e as constelações Delfim e Cavalo Menor</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">- a partir da estrela-epsilon Pegasi, Enif, o nariz do Cavalo Alado,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e a estrela mais brilhante desta constelação.</span></div>
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<span style="color: #073763; font-size: small; font-weight: normal;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi">http://pt.wikipedia.org/wiki/Epsilon_Pegasi</a></span></h1>
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<b>Epsilon Pegasi</b> (ε Peg, ε Pegasi) é a <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrela</a> mais brilhante da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pegasus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pegasus">Pegasus</a>, com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 2,399.<span class="reference" id="cite_ref-saaoc8_59_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-saaoc8_59-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> É conhecida também pelo nome tradicional <b>Enif</b>, que é derivado da palavra árabe para nariz, devido à sua posição na constelação.<span class="reference" id="cite_ref-stars_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-stars-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span> A distância a ela pode ser estimada usando medições de <a href="http://pt.wikipedia.org/wiki/Paralaxe" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Paralaxe">paralaxe</a> da missão <a href="http://pt.wikipedia.org/wiki/Hipparcos" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hipparcos">Hipparcos</a>, dando um valor de 690 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (211 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">parsecs</a>) da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, com uma <a href="http://pt.wikipedia.org/wiki/Margem_de_erro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Margem de erro">margem de erro</a> de 20 anos-luz.<span class="reference" id="cite_ref-simbad_1-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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Epsilon Pegasi é uma estrela <a href="http://pt.wikipedia.org/wiki/Evolu%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Evolução estelar">evoluída</a> que está no estágio de <a href="http://pt.wikipedia.org/wiki/Estrela_supergigante" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela supergigante">supergigante</a>, confome indicado pela <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação estelar">classificação estelar</a> de K2 Ib.<span class="reference" id="cite_ref-simbad_1-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-simbad-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> Estima-se que tenha 12 vezes a<a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massa do Sol</a>.<span class="reference" id="cite_ref-mnras410_1_190_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-mnras410_1_190-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> </div>
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Em algumas ocasiões, o brilho de Epsilon Pegasi aumentou radicalmente, ficando até mais brilhante que <a href="http://pt.wikipedia.org/wiki/Altair_(estrela)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Altair (estrela)">Altair</a>, a estrela mais brilhante da constelação de <a href="http://pt.wikipedia.org/wiki/Aquila" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aquila">Aquila</a>.<span class="reference" id="cite_ref-stars_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-stars-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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Como uma supergigante, Epsilon Pegasi está no fim de sua vida, porém, como sua massa está na divisa entre estrelas destinadas a explodir ou não, não se sabe se irá explodir em uma <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Supernova">supernova</a> ou se tornar uma rara <a href="http://pt.wikipedia.org/wiki/An%C3%A3_branca" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anã branca">anã branca</a> de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Ne%C3%B4nio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Neônio">neônio</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a> com menos da metade do tamanho da Terra.<span class="reference" id="cite_ref-stars_9-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi#cite_note-stars-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">9</a></span></div>
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LEIA MAIS</div>
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em</div>
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<a href="http://pt.wikipedia.org/wiki/Epsilon_Pegasi">http://pt.wikipedia.org/wiki/Epsilon_Pegasi</a></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m15atlas.jpg" /><br />
http://www.ipac.caltech.edu/2mass/gallery/m15atlas.jpg<br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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<h1>
Messier 15</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M15 (NGC 7078)</i>, class IV, in <a href="http://messier.obspm.fr/map/Peg.html">Pegasus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m15.jpg"><img align="right" alt="[m15.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m15.jpg" /></a><br />
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<tr><th align="left">Right Ascension</th><td align="center">21 : 30.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 10 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">33.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.2 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">18.0 (arc min)</td></tr>
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Discovered by Jean-Dominique Maraldi in 1746.<br />
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Globular cluster Messier 15 (M15, NGC 7078) is among the more conspicuous of these great stellar swarms. At a distance of about 33,600 light years, its diameter of 18.0 arc min corresponds to a linear extension of about 175 light-years, and its total visual brightness of 6.2 magnitudes corresponds to an absolute magnitude of -9.17, or roughly 360,000 times that of our sun.<br />
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M15 is perhaps the densest of all (globular) star clusters in our Milky Way galaxy.<br />
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M15 was discovered by <a href="http://messier.obspm.fr/xtra/Bios/maraldi.html">Jean-Dominique Maraldi (Maraldi II, 1709-88)</a> on September 7, 1746 while he was looking for De Chéseaux' comet; he described it as 'A nebulous star, fairly bright and composed of many stars'. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who<a href="http://messier.obspm.fr/xtra/history/m-cat.html#M15">cataloged it on June 3, 1764</a>, and <a href="http://messier.obspm.fr/xtra/similar/bode.html">Johann Elert Bode</a> couldn't make this out and described it as 'nebula without stars,' so that it remained to <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> in 1783 to resolve this fine star cluster.<br />
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LEIA MAIS<br />
acessando<br />
<a href="http://messier.obspm.fr/m/m015.html">http://messier.obspm.fr/m/m015.html</a><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;"><b>NGC 7078 - M 15 - Aglomerado Globular Pegasus</b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 21h29m Declinação +12<sup>o</sup>.05<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 7,0 Diâmetro aparente 9’,4 Tipo Espectral F2<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,44<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 103 Distância kpc 10,5<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) - 107</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 15</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 7078</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pégaso</a>. Foi descobeto pelo astrônomo ítalo-francês <a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Maraldi">Jean-Dominique Maraldi</a> em 1746, e posteriormente incluído pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo</a> de objetos semelhantes a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background: none; color: #0b0080; text-decoration: none;" title="Cometa">cometas</a> em 1764. Com uma idade estimada de 13,2 bilhões de anos, Messier 15 é um dos mais velhos aglomerados globulares conhecidos.</div>
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O aglomerado está a cerca de 33 600 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background: none; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, e tem uma <a href="http://pt.wikipedia.org/wiki/Luminosidade" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade">luminosidade</a> total 360 000 vezes maior do que a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Luminosidade_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Luminosidade solar">luminosidade solar</a>, o que dá ao objeto uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> de -9,2. Messier 15 é um dos aglomerados globulares mais densos conhecidos da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background: none; color: #0b0080; text-decoration: none;" title="Via-Láctea">Via-Láctea</a>. Seu núcleo sofre uma contração conhecida como "<a class="new" href="http://pt.wikipedia.org/w/index.php?title=Colapso_de_n%C3%BAcleo&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Colapso de núcleo (página não existe)">colapso de núcleo</a>"; seu núcleo tem uma densidade estelar elevada, com uma quantidade enorme de estrelas orbitando o que pode ser um <a href="http://pt.wikipedia.org/wiki/Buraco_negro" style="background: none; color: #0b0080; text-decoration: none;" title="Buraco negro">buraco negro</a> central.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_15">http://pt.wikipedia.org/wiki/Messier_15</a></span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/65/Messier_15_Hubble_WikiSky.jpg/800px-Messier_15_Hubble_WikiSky.jpg" /></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_15#mediaviewer/File:Messier_15_Hubble_WikiSky.jpg">http://pt.wikipedia.org/wiki/Messier_15#mediaviewer/File:Messier_15_Hubble_WikiSky.jpg</a></div>
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<a class="extiw" href="http://en.wikipedia.org/wiki/Messier_15" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start; text-decoration: none;" title="en:Messier 15">en:Messier 15</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;"> by </span><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background: none rgb(251, 251, 251); color: #0b0080; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a><span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">; 3.4′ view</span></div>
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<table cellpadding="0" cellspacing="2" class="infobox" style="background: rgb(242, 242, 242); border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; float: right; font-family: sans-serif; font-size: 11px; margin: 0px 0px 1em 1em; padding: 0.2em; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 15</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_15_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 15 pelo Telescópio Espacial Hubble"><img alt="Messier 15 pelo Telescópio Espacial Hubble" data-file-height="4160" data-file-width="4160" src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/65/Messier_15_Hubble_WikiSky.jpg/250px-Messier_15_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Messier_15_Hubble_WikiSky.jpg/375px-Messier_15_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Messier_15_Hubble_WikiSky.jpg/500px-Messier_15_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 15 pelo Telescópio Espacial Hubble</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pegasus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">21<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 29<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 58,38<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">+12° 10′ 00,6″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">33 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (10,3 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,2<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">18',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">88 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">13,2 bilhões de anos</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 7078</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 15"><img alt="Messier 15" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Pegasus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Pegasus constellation map.png" data-file-height="2269" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/1e/Pegasus_constellation_map.png/250px-Pegasus_constellation_map.png" height="222" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1e/Pegasus_constellation_map.png/375px-Pegasus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1e/Pegasus_constellation_map.png/500px-Pegasus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<b>Foi o primeiro aglomerado globular a ter uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a>, Pease I</b>, descoberta por <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Francis_Gladheim_Pease&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Francis Gladheim Pease (página não existe)">Francis Gladheim Pease</a> no <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_Monte_Wilson" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório Monte Wilson">Observatório Monte Wilson</a>, em 1927. Até hoje, conhece-se apenas quatro nebulosas planetárias pertencentes a aglomerados globulares na Via-Láctea.<span class="reference" id="cite_ref-Gillettetal1989_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-Gillettetal1989-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> <span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> </div>
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<span style="color: black; font-family: 'Times New Roman'; line-height: normal;"><a href="http://pt.wikipedia.org/wiki/Messier_15">http://pt.wikipedia.org/wiki/Messier_15</a></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/9/96/M15pease1_%28HST%29.jpg" height="640" width="640" /></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="background-color: white; font-size: 14px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_15#mediaviewer/File:M15pease1_(HST).jpg</span></span></div>
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<span style="background-color: white;">A <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;" title="Nebulosa planetária">nebulosa planetária</a> Pease I, contida em M15, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></div>
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<span style="background-color: white;">HST (WFPC2)</span></div>
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Pease 1: Planetary Nebula in M15</h2>
<i><a href="http://messier.obspm.fr/planetar.html">Planetary Nebula</a> Pease 1</i> (PK 065-27.1, Kuster 648) in globular cluster <a href="http://messier.obspm.fr/m/m015.html"><b>M15</b></a> in <a href="http://messier.obspm.fr/map/Peg.html">Pegasus</a></center>
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<a href="http://messier.obspm.fr/Pics/Jpg/m15_p1cap.jpg"><img align="right" alt="[Pease 1 in M15, Stan Moore]" border="0" src="http://messier.obspm.fr/Pics/More/m15_p1sm.jpg" /></a><br />
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<tr><th align="left">Right Ascension</th><td align="center">21 : 30.02 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+12 : 10.2 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">32.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">15.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">3 (arc seconds)</td></tr>
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Pease 1 was the first planetary nebula found in a globular cluster, in 1928 by <a href="http://messier.obspm.fr/more/m015_pease1.html#pease1928">Francis Gladheim Pease</a>. It had been previously cataloged as a star by <a href="http://messier.obspm.fr/more/m015_pease1.html#kustner1921">Friedrich Kustner (1921)</a>.<br />
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Stan Moore has been able to image Pease 1 in an RGB image obtained with a ST-7 CCD camera on a 12.5-inch RC telescope.<br />
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SAIBA MAIS<br />
sobre Pease 1<br />
acessando<br />
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A Golden Planetary</h2>
<span style="text-align: -webkit-center;">by </span><a href="http://leo.astronomy.cz/" style="text-align: -webkit-center;">Leos Ondra</a><br />
<a href="http://messier.obspm.fr/xtra/leos/pease1.html">http://messier.obspm.fr/xtra/leos/pease1.html</a><br />
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Existem também nove <a href="http://pt.wikipedia.org/wiki/Pulsar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pulsar">pulsares</a>, <a href="http://pt.wikipedia.org/wiki/Estrela_de_n%C3%AAutrons" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela de nêutrons">estrelas de nêutrons</a> remanescentes de <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Supernova">supernovas</a> da época que o aglomerado ainda era jovem. Estas têm as designações PSR 2127+11 A a PSR 2127+11 H. PSR 2127+11 C é um <a href="http://pt.wikipedia.org/wiki/Estrela_bin%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela binária">binário</a> de estrelas de nêutrons. De forma semelhante aos binários de pulsares <a href="http://pt.wikipedia.org/wiki/PSR_1913%2B16" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="PSR 1913+16">PSR 1913+16</a> e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=PSR_1534%2B12&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="PSR 1534+12 (página não existe)">PSR 1534+12</a>, o binário de pulsares de Messier 15 exibe efeitos gravitacionais drásticos e a constatação de alguns efeitos previstos pela <a href="http://pt.wikipedia.org/wiki/Relatividade_geral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Relatividade geral">relatividade geral</a> no sistema são evidentes, como mudanças significativas nos periastros das estrelas de nêutrons, efeitos na luz e emissão de <a href="http://pt.wikipedia.org/wiki/Radia%C3%A7%C3%A3o_gravitacional" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Radiação gravitacional">radiação gravitacional</a>, que causa uma perda energética no binário e consequentemente uma diminuição no período de <a href="http://pt.wikipedia.org/wiki/Rota%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Rotação">rotação</a> dos pulsares e a diminuição no período de suas órbitas.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span class="mw-headline" id="Fonte_de_raios-X"><span style="font-size: small;">Fonte de raios-X</span></span></h2>
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O quarto catálogo "Uhuru" (designada como "4U") contém uma fonte de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raios-x" style="background: none; color: #0b0080; text-decoration: none;" title="Raios-x">raios-x</a> detectada durante o primeiro ano de funcionamento do satélite observatório de raios-X <a href="http://pt.wikipedia.org/wiki/Uhuru" style="background: none; color: #0b0080; text-decoration: none;" title="Uhuru">Uhuru</a>.<span class="reference" id="cite_ref-Forman_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-Forman-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Esta fonte foi catalogada no quarto catálogo "Uhuru" como "4U 2129+12", e é um <a href="http://pt.wikipedia.org/wiki/Bin%C3%A1rio_de_raio_X" style="background: none; color: #0b0080; text-decoration: none;" title="Binário de raio X">sistema binário, emissor de raios-X</a> e de baixa massa. Também foi catalogada como Messier 15 X-1. Além do mais, o <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_de_raios-X_Chandra" style="background: none; color: #0b0080; text-decoration: none;" title="Observatório de raios-X Chandra">observatório de raios-X Chandra</a> detectou outro emissor de raios-X no aglomerado que foi catalogado como Messier 15 X-2. Messier 15 X-1 é a primeira <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Fontes_astron%C3%B4micas_de_raios-X&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Fontes astronômicas de raios-X (página não existe)">fonte astronômica de raios-X</a> detectada na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Pegasus" style="background: none; color: #0b0080; text-decoration: none;" title="Pegasus">Pégaso</a>.<span class="reference" id="cite_ref-White_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_15#cite_note-White-6" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">6</a></span></div>
<a href="http://pt.wikipedia.org/wiki/Messier_15">http://pt.wikipedia.org/wiki/Messier_15</a><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br /><div style="font-family: 'Times New Roman'; font-size: medium; line-height: 18px;">
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<img src="http://www.raremaps.com/maps/medium/38540.jpg" /></div>
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<span style="color: #073763;">http://www.raremaps.com/gallery/detail/38540/_Pegasus/Bayer.html</span></div>
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<span style="color: #073763;"><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span><strong style="font-family: verdana, arial, georgia, sans-serif; font-size: 12px; text-align: start;">Title: </strong><span style="font-family: verdana, arial, georgia, sans-serif; font-size: 12px; text-align: start;">[ Pegasus ]</span></span></div>
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<span style="color: #073763;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Johann Bayer</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><br />
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<!-- Blogger automated replacement: "https://images-blogger-opensocial.googleusercontent.com/gadgets/proxy?url=http%3A%2F%2Fwww.raremaps.com%2Fmaps%2Fmedium%2F35069.jpg&container=blogger&gadget=a&rewriteMime=image%2F*" with "https://blogger.googleusercontent.com/img/proxy/AVvXsEhK3dQ0PW1RlMZExMVZ5OII56FNrakpM_zV0tEKkcoi6gjoe-bVza-Ms2RLqOK6Oykw4UTghZzhyMUcRiH0clUwbEhyEtmFOIqipx9x8R89lBKyM2GGtx0CTsmtikIkrOxjO36s6sPohyVagQlO=" -->Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-7277347020770179182014-09-06T08:35:00.005-07:002015-01-04T08:25:47.181-08:00Orion<div class="MsoNormal">
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Olá!</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Eu sou realmente encantada </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">com os desenhos formados pelas estrelas </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que compõem a constelação Orion:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">podemos ver seu corpanzil, sua cabeça,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> seu braço levantando a clava </span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">e seu outro braço segurando o leão abatido. </span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">Podemos ver seu Cinturão </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">famoso por suas três estrelas óbvias:</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> as chamadas Três Marias</span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"> e que também são conhecidas como </span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">Mintaka, Alnilan e Alnitak. </span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">Podemos ver sua Espada!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">E, com boa visão </span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;">e<b> sempre em lugares de céus escuros e transparentes,</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>podemos ver a olho nu</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b> - <i>ou entrever com visão enviesada</i> - </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>os objetos celestes (esfumaçados) rondando a estrela Alnitak </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como apreciarmos imensamente e sempre a olho nú</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b> os objetos (esfumaçados) que perfazem a Espada de Orion.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Na aparente proximidade da estrela Alnitak </b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>(uma das conhecidas <i>Três Marias</i></b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>formando o Cinturão do Gigante Orion),</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>vamos encontrar o Objeto Messier 78.</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>Na Espada de Orion, vamos encontrar os Objetos Messier</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>M42 e M43!</b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, O Cinturão e a Espada de Orion</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>não somente encantam nossa visão</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>como também encantam nossa Maratona de Objetos Messier.</b></span></div>
<div style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;">
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">É claro, confesso, que sempre podemos ter a boa ajuda</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">de um simpático par de binóculos</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">bem como de um simpático telescópio</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para bem podermos observar com maior nitidez</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">todos estes objetos maravilhosos, em Orion!</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">E sempre podemos nos deleitar com as imagens soberbas</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">realizadas pelas lentes ópticas dos fotógrafos mais profissionais</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">e pelos super-telescópios!</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">A bem da verdade, penso que a constelação do Gigante Orion</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">sempre nos encanta de qualquer maneira que a contemplemos, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">seja através nossa visão desarmada</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> ou através nossa visão por detrás de lentes ópticas poderosas!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.constellation-guide.com/constellation-list/orion-constellation/orion-constellation-2/" rel="attachment wp-att-1784" style="border: none; color: #660000; cursor: pointer; line-height: 21px; margin: 0px; outline: none; padding: 0px; text-decoration: none; vertical-align: baseline;"><img alt="orion constellation,rigel,betelgeuse,orions belt" class=" wp-image-1784 " src="http://www.constellation-guide.com/wp-content/uploads/2011/12/Orion-Constellation.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 102, 102); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; height: auto; margin: 0px auto; max-width: 604px; outline: none; padding: 0px; position: relative; vertical-align: baseline;" title="Orion Constellation" width="475" /></a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Orion constellation, cropped from photo by Hubble, ESA, Akira Fujii</span></div>
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<a href="http://www.constellation-guide.com/constellation-list/orion-constellation/" style="color: #660000; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.constellation-guide.com/constellation-list/orion-constellation/</span></a></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEihj-dMjz50pydhyphenhyphenF8nGtA8HxLKJ6nvk32NdaCw8MGNn-t2-fUHavAEQIXPzmlSmQqvC00_eICFHT9Weu5Lbdnf4XubM8LEh15UVmJoTaZJAt9QLQ6cqia3qgRVYFxOAMOzngIPCWYo1sA/s1600/853px-Orion_above_the_VLT_.png" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEihj-dMjz50pydhyphenhyphenF8nGtA8HxLKJ6nvk32NdaCw8MGNn-t2-fUHavAEQIXPzmlSmQqvC00_eICFHT9Weu5Lbdnf4XubM8LEh15UVmJoTaZJAt9QLQ6cqia3qgRVYFxOAMOzngIPCWYo1sA/s1600/853px-Orion_above_the_VLT_.png" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/thumb/8/8e/Orion_above_the_VLT_.png/853px-Orion_above_the_VLT_.png</span><br />
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;">Description</td><td class="description"><div class="description mw-content-ltr en" dir="ltr" lang="en" style="direction: ltr;">
<span class="language en" title=""><b>English:</b></span> The great hunter Orion hangs above ESO’s Very Large Telescope (VLT), in this stunning, previously unseen, image. As the VLT is in the Southern Hemisphere, Orion is seen here head down, as if plunging towards the Chilean Atacama Desert. At night the four giant 8.2-metre Unit Telescopes of the VLT are all turned skywards to help astronomers in their quest to understand the Universe. The band of the Milky Way, criss-crossed by contrasting dark dust lanes, stretches up over the VLT’s Unit Telescope 3 (Melipal), with the bright star Capella glinting just above the telescope. Up and to the left, Orion’s belt and sword, containing the Orion Nebula, lie between the blue star Rigel and the orange Betelgeuse. The red Rosetta Nebula is seen in the middle part of the Milky Way, while Sirius, the brightest star in the night sky, hangs above the scene. The red patch just above the VLT Unit Telescope 2 (Kueyen) is the California Nebula, nicely offset by the blue of the beautiful Pleiades star cluster a little to the left and above.</div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;">Date</td><td><time class="dtstart" datetime="2009-08-24" style="display: inline;">24 August 2009</time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;">Source</td><td><a class="external text" href="http://www.eso.org/gallery/v/ESOPIA/Paranal/Paranal_Orion_cc_8bit.tif.html" rel="nofollow" style="color: #274e13; text-decoration: none;">ESO</a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.6875px;">Author</td><td>ESO/Y. Beletsky; cropped for article display purposes by <a class="new" href="http://commons.wikimedia.org/w/index.php?title=User:H_Debussy-Jones&action=edit&redlink=1" style="background-image: none; color: #a55858; text-decoration: none;" title="User:H Debussy-Jones (page does not exist)">H Debussy-Jones</a> (<a class="new" href="http://commons.wikimedia.org/w/index.php?title=User_talk:H_Debussy-Jones&action=edit&redlink=1" style="background-image: none; color: #a55858; text-decoration: none;" title="User talk:H Debussy-Jones (page does not exist)">talk</a>) 21:33, 19 November 2009 (UTC)</td></tr>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><b>Mario Jaci Monteiro - As 88 Constelações, Cartas Celestes - CARJ</b></span></span><br />
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<span lang="EN-US"></span>Excerto de </div>
<span style="font-family: Arial, Helvetica, sans-serif; font-size: small;">Mario Jaci Monteiro - As 88 Constelações, Cartas Celestes</span><br />
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<span lang="EN-US"><span lang="EN-US"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US"> </span>ORION, O GIGANTE CAÇADOR</b></span></span></span><br />
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<span lang="EN-US"><span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 4h41m / 6h23m Declinação -11<sup>o</sup>.0 / +23<sup>o</sup>.0<o:p></o:p></span></span></span><br />
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">O Gigante Orion foi criado por Júpiter e Mercúrio, a pedido de Hireus. </span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Ele foi cego por Enopin e Baco </span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">por sua forma de tratar a filha do primeiro, </span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">porém recuperou sua visão </span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">através a exposição de seus olhos ao sol nascente. </span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">E porque ele dizia </span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">que podia eliminar qualquer animal desse mundo,</span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"> o Escorpião lhe picou e Orion morreu.<o:p></o:p></span></span><br />
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Esta é uma constelação muito interessante </span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">e a linha do Equador celestial passa por ela </span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">exatamente em sua estrela Mintaka, Delta Orionis, </span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">que faz parte do famoso Cinturão de Orion,</span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"> mais popularmente conhecido como As Três Marias.<o:p></o:p></span></span><br />
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Orion encontra-se situado entre as constelações Monoceros, Gemini, Taurus, Eridanus e Lepus.<o:p></o:p></span></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiUMcxoXTToZX5LSRCKo8zgaiKlchOFgmdBxKWI2o8EmTF96vRu7zL9yynH5ZF72AonqhijuNY66OGp-BD7j_KCSnWuOMb8n21drDFRh2zJsZ9zDLj5x9KqcnTnXJQI4fGkgxaZs_JJ0EQ/s1600/%D0%94%D1%80%D0%B5%D0%B2%D0%BD%D0%B8%D0%B5_%D1%81%D0%BE%D0%B7%D0%B2%D0%B5%D0%B7%D0%B4%D0%B8%D1%8F_%D0%BD%D0%B0%D0%B4_%D1%82%D0%B5%D0%BB%D0%B5%D1%81%D0%BA%D0%BE%D0%BF%D0%BE%D0%BC_ALMA.jpg" imageanchor="1" style="clear: left; color: #274e13; float: left; margin-bottom: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiUMcxoXTToZX5LSRCKo8zgaiKlchOFgmdBxKWI2o8EmTF96vRu7zL9yynH5ZF72AonqhijuNY66OGp-BD7j_KCSnWuOMb8n21drDFRh2zJsZ9zDLj5x9KqcnTnXJQI4fGkgxaZs_JJ0EQ/s1600/%D0%94%D1%80%D0%B5%D0%B2%D0%BD%D0%B8%D0%B5_%D1%81%D0%BE%D0%B7%D0%B2%D0%B5%D0%B7%D0%B4%D0%B8%D1%8F_%D0%BD%D0%B0%D0%B4_%D1%82%D0%B5%D0%BB%D0%B5%D1%81%D0%BA%D0%BE%D0%BF%D0%BE%D0%BC_ALMA.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-size: 12px; line-height: 16.7999992370605px; margin: 0px; padding: 0px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>http://www.eso.org/public/archives/images/screen/potw1347a.jpg</b></span></span></div>
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<span style="font-size: 12px; line-height: 16.7999992370605px; margin: 0px; padding: 0px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/potw1347a/</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><strong style="margin: 0px; padding: 0px;">Credit: </strong><span style="line-height: 1.4em;">ESO/B. Tafreshi (</span><a href="http://www.twanight.org/tafreshi" style="background-image: url(http://www.eso.org/public/archives/app/i/ext_link2.e3e6349c34f8.gif); background-position: 0% 50%; background-repeat: no-repeat; color: #274e13; line-height: 1.4em; margin: 0px; padding-bottom: 0px; padding-left: 12px !important; padding-right: 0px; padding-top: 0px; text-decoration: none;">twanight.org</a><span style="line-height: 1.4em;">)</span></span></div>
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<span style="line-height: 19.2000007629395px; text-align: start;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Babak Tafreshi, one of the ESO Photo Ambassadors, has captured the antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) in an enthralling image combining the beauty of the southern sky with the amazing dimensions of the biggest astronomical project in the world.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Thousands of stars are revealed to the naked eye in the clear skies over the Chajnantor Plateau. Its dry and transparent night sky is one of the reasons ALMA has been built here. Surprisingly bright in the upper left corner of the picture, there is a tightly packed bunch of young stars, the Pleiades Cluster, which was already known to most ancient civilisations. The constellation of Orion (The Hunter) is clearly visible over the closest of the antennas — the hunter’s belt is formed by the three blue stars just to the left of the red light. According to classic mythology, Orion was a hunter who chased the Pleiades, the beautiful daughters of Atlas. When seen through the thin atmosphere over the Atacama, it almost seems that this epic hunt is really happening.</span></div>
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<b style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 12px; line-height: 16.7999992370605px;">http://www.eso.org/public/images/potw1347a/</b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Minha simples tradução literal </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">para o texto explicativo acima acerca esta belíssima imagem</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> realizada por Babak Tafreshi)</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Milhares de estrelas nos são apresentadas a olho nu nos céus límpidos do Plateau Chajnantor. O céu noturno seco e transparente é uma das razões pelas quais ALMA foi ali construído. Surpreendentemente iluminado no canto esquerdo ao alto da foto encontra-se um aglomerado de estrelas jovens bem compactadas, o Aglomerado das Pleiades (que também era conhecido nas antigas civilizações). A constelação de Orion (O Caçador) é claramente visível e bem próximo às antenas - o Cinturão do Caçador sendo formado peles três estrelas azuladas bem à esquerda da luz vermelha. De acordo com a mitologia clássica, Orion era um caçador que buscava alcançar as Pleiades, as belas filhas de Atlas. Quando visto através a atmosfera delicada do Atacama, nos parece que esse épico de caçada está realmente acontecendo.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
<br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M42 E M43 E M78,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
<div style="color: #073763; line-height: 1.4;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO ORION:</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a constelação do Gigante Caçador, Orion,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não somente é imensa </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como também podemos encontrar </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">estrelas e objetos interessantíssimos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em todo seu corpanzil!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nesta Postagem </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Messier acolhidos por esta constelação, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vamos nos ater às imediações do Cinturão</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e na Espada propriamente dita de Orion:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Asterismo denominado de <b>O Cinturão de Orion</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é composto pelas estrelas Delta, Epsilon e Zeta Orionis.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">É próximo a este Asterismo</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e nas imediações (um tantinho ao norte) da estrela Alnitak,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que encontraremos <b>o Objeto Messier 78</b>.</span></div>
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<div style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;">
<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe um Asterismo denominado de <b>A Espada de Orion</b>, </span></span></div>
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<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">composto pelas estrelas Teta e Iota Orionis.</span></span></div>
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<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Neste Asterismo, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">estaremos encontrando </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>os Objetos Messier</b></span></div>
<div style="font-size: 16px; line-height: 22.3999996185303px;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M42 e M43</b>.</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<img src="http://www.iau.org/static/public/constellations/gif/ORI.gif" /></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://www.iau.org/static/public/constellations/gif/ORI.gif">http://www.iau.org/static/public/constellations/gif/ORI.gif</a></span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="color: #073763; line-height: 1.4;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M42 E M43 E M78,</b></span></div>
<div style="color: #073763; line-height: 1.4;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
<div style="color: #073763; line-height: 1.4;">
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO ORION:</b></span></div>
<div style="color: #073763;">
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<div style="color: #073763;">
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M78</b></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>O Asterismo denominado de O Cinturão de Orion</b></span></div>
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<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é composto pelas estrelas Delta, Epsilon e Zeta Orionis.</span></b></div>
<div style="font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;">
<b><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></b></div>
<div style="font-size: 16px; line-height: 22.3999996185303px;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>É próximo a este Asterismo</b></span></div>
<div style="font-size: 16px; line-height: 22.3999996185303px;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e nas imediações (um tantinho ao norte) da estrela Alnitak,</b></span></div>
<div style="font-size: 16px; line-height: 22.3999996185303px;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>que encontraremos o Objeto Messier 78.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Cingula Orionis</b><b>. Delta e Epsilon Orionis.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Este é o Cinto de Orion.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>O Cinto ou Cinturão de Órion </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">é popularmente conhecido por suas três estrelas </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>compondo As Três Marias </b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b>- Mintaka, Alnitak e Alnilan:<o:p></o:p></b></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.constellation-guide.com/constellation-list/orion-constellation/orions-belt/" rel="attachment wp-att-1796" style="border: none; color: #660000; cursor: pointer; line-height: 21px; margin: 0px; outline: none; padding: 0px; text-decoration: none; vertical-align: baseline;"><img alt="orion's belt,belt of orion,orion constellation,alnitak,alnilam,mintaka" class="size-medium wp-image-1796" src="http://www.constellation-guide.com/wp-content/uploads/2011/12/Orions-Belt-300x199.jpg" height="424" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(102, 102, 102); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; height: auto; margin: 0px auto; max-width: 604px; outline: none; padding: 0px; position: relative; vertical-align: baseline;" title="Orion's Belt" width="640" /></a></span></div>
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<span style="font-size: x-small;"><span style="font-family: Arial, Helvetica, sans-serif;">Orion's Belt: Alnitak, Alnilam, and Mintaka, are the bright bluish stars from east to west (left to right) along the diagonal in this gorgeous cosmic vista. Otherwise known as the Belt of Orion, these three blue supergiant stars are hotter and much more massive than the Sun. They lie about 1,500 light-years away.</span><br /><span style="font-family: Arial, Helvetica, sans-serif;"> Photo: Astrowicht</span></span></div>
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<a href="http://www.constellation-guide.com/constellation-list/orion-constellation/" style="color: #274e13; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: x-small;">http://www.constellation-guide.com/constellation-list/orion-constellation/</span></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Mintaka</b><b>. Delta Orionis. </b></span><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h31,0m - Declinação -00<sup>o</sup> 19’<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 2,48 - Distância 1500 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Uma estrela dupla vagamente variável, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">do branco brilhante ao vileta pálido, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">situada no Cinturão de Orion. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">A Faixa, proveniente do árabe Al Mintakah.<o:p></o:p></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>Alnitak</b><b> - Zeta Orionis - Estrela Tripla</b></span><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h39,7m - Declinação -01<sup>o</sup> 57’<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,79 - Distância 1600 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O Cinto, vocábulo árabe que desgina a cintura do gigante Órion.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span lang="EN-US">Alnilan</span><span lang="EN-US">. Epsilon Orionis. </span>Estrela Dupla</span></b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h35,2 - Declinação -01<sup>o</sup> 13’<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitude visual 1,75 - Distância 1600 anos-luz<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Uma estrela branca e brilhante</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> ocupando a posição central no Cinto de Órion. </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">De Al Nitham, o Colar de Pérolas.</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span><br />
<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt; line-height: 22.3999996185303px;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="line-height: 19px;"><a href="http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.7791666667&declination=0.0800000000&viewAngle=20">http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.7791666667&declination=0.0800000000&viewAngle=20</a></span><br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m78atlas.jpg" /><br />
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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Messier 78</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Starforming Nebula</a> M78 (NGC 2068)</i>, a reflection nebula, with <a href="http://messier.obspm.fr/cluster.html">Open Star Cluster</a>, in <a href="http://messier.obspm.fr/map/Ori.html">Orion</a></center>
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<a href="http://messier.obspm.fr/Jpg/m78.jpg"><img align="right" alt="[m78.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m78.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">05 : 46.7 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+00 : 03 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">8x6 (arc min)</td></tr>
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Discovered 1780 by Pierre Méchain.</div>
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Messier 78 (M78, NGC 2068) is the brightest diffuse reflection nebula in the sky, situated in the rich constellation Orion.</div>
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This object was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> in early 1780. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> added it <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M78">to his catalog</a> on December 17, 1780.</div>
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M78 belongs to the <a href="http://messier.obspm.fr/more/oricloud.html">Orion complex</a>, a large cloud of gas and dust centered on the Orion Nebula <a href="http://messier.obspm.fr/m/m042.html">M42</a>/<a href="http://messier.obspm.fr/m/m043.html">M43</a>, and is about 1,600 light years distant. It is the brightest portion of a vast dust cloud which includes NGC 2071 (northeast, lower right in our image), NGC 2067 (close northwest), and very faint NGC 2064 (southwest), all visible in our image. Together with some other nebulae, including NGC 2024 (Orion B) near Zeta Orionis (sometimes called the Flame Nebula), all these nebulae are associated with the molecular cloud LDN 1630 (from <a href="http://messier.obspm.fr/xtra/supp/cats.html#LDN">Lynds' Catalogue of Dark Nebula</a>), a part of the Orion complex.</div>
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LEIA MUITA MAIS</div>
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em</div>
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<a href="http://messier.obspm.fr/m/m078.html">http://messier.obspm.fr/m/m078.html</a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"> http://www.stellarium.org/pt/</span><br />
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<span lang="EN-US"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"> http://www.stellarium.org/pt/</span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiysq2kDkG26f1KcxIfB4W32LFD5BqvHFQm0xjHjOnBtVlb5HlgkkNVcwMQW0CYpzvnUFn22MJSghyKHMpowxoTW6oUHZYejPkyO3G39YhpDHQTzV5gnotbdRBToV26N0he0Li5k7NDH7Sd/s1600/M42+E+M43+3+E+M78+ORION,+MARIO+JACI.jpg+2.jpg" imageanchor="1" style="color: #660000; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiysq2kDkG26f1KcxIfB4W32LFD5BqvHFQm0xjHjOnBtVlb5HlgkkNVcwMQW0CYpzvnUFn22MJSghyKHMpowxoTW6oUHZYejPkyO3G39YhpDHQTzV5gnotbdRBToV26N0he0Li5k7NDH7Sd/s1600/M42+E+M43+3+E+M78+ORION,+MARIO+JACI.jpg+2.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Extraído de As Constelações, Cartas Celestes - ORION - Mario Jaci Monteiro</span></span><br />
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<span lang="EN-US"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NGC 2068 - M 78 - Orion - Nebulosa de Reflexão - Anel de Barnard</b></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h45m Declinação +00<sup>o</sup>.02</span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NR Dimensão 5,0 Magnitude 20<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância em anos-luz 1,5<o:p></o:p></span><br />
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span><br />
<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt; line-height: 22.3999996185303px;">Editora Vozes, Petrópolis, ano de 1986</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><img alt="Orion constellation map.png" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/250px-Orion_constellation_map.png" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="620" /></span></div>
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<b><span style="color: #660000;">Messier 78 (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC</a> 2068)</span></b> é uma <a href="http://pt.wikipedia.org/wiki/Nebulosa_de_reflex%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Nebulosa de reflexão">nebulosa de reflexão</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Orion_(constela%C3%A7%C3%A3o)" style="background-image: none; color: #0b0080; text-decoration: none;" title="Orion (constelação)">Orion</a>. Foi descoberta por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-image: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> em <a href="http://pt.wikipedia.org/wiki/1780" style="background-image: none; color: #0b0080; text-decoration: none;" title="1780">1780</a> e incluída por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> no seu catálogo de objetos esse mesmo ano.</div>
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M78 é a nebulosa difusa de reflexão mais brilhante de um grupo de nebulosas que inclui <a href="http://pt.wikipedia.org/wiki/NGC_2064" style="background-image: none; color: #0b0080; text-decoration: none;" title="NGC 2064">NGC 2064</a>, <a href="http://pt.wikipedia.org/wiki/NGC_2067" style="background-image: none; color: #0b0080; text-decoration: none;" title="NGC 2067">NGC 2067</a> e <a href="http://pt.wikipedia.org/wiki/NGC_2071" style="background-image: none; color: #0b0080; text-decoration: none;" title="NGC 2071">NGC 2071</a>. M78 é facilmente visível em pequenos telescópios como uma mancha difusa e inclui duas <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> de <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude</a> 10. Estas duas estrelas, <i><a class="new" href="http://pt.wikipedia.org/w/index.php?title=HD_38563A&action=edit&redlink=1" style="background-image: none; color: #a55858; text-decoration: none;" title="HD 38563A (página não existe)">HD 38563A</a></i> e <i><a class="new" href="http://pt.wikipedia.org/w/index.php?title=HD_38563B&action=edit&redlink=1" style="background-image: none; color: #a55858; text-decoration: none;" title="HD 38563B (página não existe)">HD 38563B</a></i>, são responsáveis de fazer a nuvem de pó em M78 visível ao refletir sua <a href="http://pt.wikipedia.org/wiki/Luz" style="background-image: none; color: #0b0080; text-decoration: none;" title="Luz">luz</a>.</div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_78.jpg" style="background-image: none; color: #0b0080; text-decoration: none;" title="Messier 78, ESO"><img alt="Messier 78, ESO" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Messier_78.jpg/250px-Messier_78.jpg" height="242" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Messier_78.jpg/375px-Messier_78.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Messier_78.jpg/500px-Messier_78.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a></div>
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Messier 78, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/ESO" style="background-image: none; color: #0b0080; text-decoration: none;" title="ESO">ESO</a></div>
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Descoberto por</div>
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<a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-image: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a></div>
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Data</div>
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1780</div>
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<b>Dados observacionais (J2000)</b></div>
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Tipo</div>
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<a href="http://pt.wikipedia.org/wiki/Nebulosa_de_reflex%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Nebulosa de reflexão">Nebulosa de reflexão</a></div>
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<a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></div>
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<a href="http://pt.wikipedia.org/wiki/Orion_(constela%C3%A7%C3%A3o)" style="background-image: none; color: #0b0080; text-decoration: none;" title="Orion (constelação)">Orion</a></div>
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<a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></div>
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5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 46<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 00<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></div>
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<a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></div>
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+00° 03′ 00″</div>
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<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></div>
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8,3</div>
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1 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></div>
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8′ × 6′ <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-image: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></div>
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<a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">Messier</a> 78, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 2068</div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-image: none; color: #0b0080; text-decoration: none;" title="Messier 78"><img alt="Messier 78" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="12" /></a></div>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Orion_constellation_map.png" style="background-image: none; color: #0b0080; text-decoration: none;"><img alt="Orion constellation map.png" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/250px-Orion_constellation_map.png" height="258" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/375px-Orion_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/500px-Orion_constellation_map.png 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:Messier 78.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Messier_78.jpg/619px-Messier_78.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_78" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_78</span></a></div>
<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.1875px; padding: 5px; text-align: center; width: 1112px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://www.eso.org/public/images/eso1105a/" rel="nofollow" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/eso1105a/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO/Igor Chekalin</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><br /><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/cf/Cosmic_dust_clouds_in_reflection_nebula_Messier_78.jpg/670px-Cosmic_dust_clouds_in_reflection_nebula_Messier_78.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<a href="http://upload.wikimedia.org/wikipedia/commons/thumb/c/cf/Cosmic_dust_clouds_in_reflection_nebula_Messier_78.jpg/670px-Cosmic_dust_clouds_in_reflection_nebula_Messier_78.jpg" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/thumb/c/cf/Cosmic_dust_clouds_in_reflection_nebula_Messier_78.jpg/670px-Cosmic_dust_clouds_in_reflection_nebula_Messier_78.jpg</span></a></div>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.1875px; padding: 5px; text-align: center; width: 1112px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><a class="external free" href="http://www.eso.org/public/images/eso1219a/" rel="nofollow" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.eso.org/public/images/eso1219a/</span></a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ESO/APEX (MPIfR/ESO/OSO)/T. Stanke et al./Igor Chekalin/Digitized Sky Survey 2</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><br /><img alt="Ficheiro:Messier 078 2MASS Small.jpg" src="http://upload.wikimedia.org/wikipedia/commons/1/1d/Messier_078_2MASS_Small.jpg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></div>
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<a href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_078_2MASS_Small.jpg" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Ficheiro:Messier_078_2MASS_Small.jpg</span></a></div>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="border: 1px solid rgb(170, 170, 170); direction: ltr; line-height: 19.1875px; padding: 5px; text-align: center; width: 1112px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Derivative work of <a class="external text" href="http://www.ipac.caltech.edu/2mass/gallery/messiercat.html" rel="nofollow" style="color: #660000; text-decoration: none;">2MASS Atlas Image Gallery: The Messier Catalog</a></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><br /><img alt="Ficheiro:M78a.jpg" src="http://upload.wikimedia.org/wikipedia/commons/a/ac/M78a.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span><br />
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><a class="external text" href="http://www.ngc7000.org/" rel="nofollow" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ole Nielsen</span></a></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><br /><br /><a href="http://cseligman.com/text/stars/messiernebulae.htm#78" style="color: #660000; text-decoration: none;">http://cseligman.com/text/stars/messiernebulae.htm#78</a></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="78" style="color: #660000; text-decoration: none;"><big><b>M78 (= </b></big></a><big><b><a href="http://cseligman.com/text/atlas/ngc20a.htm#2067" style="color: #660000; text-decoration: none;">NGC 2067</a> and <a href="http://cseligman.com/text/atlas/ngc20a.htm#2068" style="color: #660000; text-decoration: none;">2068</a>)</b></big><br />Discovered (1780) b</span><span style="font-family: Arial, Helvetica, sans-serif;">y <a href="http://cseligman.com/text/atlas/discoverers.htm#mechain" style="color: #660000; text-decoration: none;">Pierre Méchain</a> (Recorded by <a href="http://cseligman.com/text/atlas/discoverers.htm#messier" style="color: #660000; text-decoration: none;">Messier</a> in 1780)<br />An 8th-magnitude reflection nebula in <a href="http://cseligman.com/text/atlas/orion.htm#2068" style="color: #660000; text-decoration: none;">Orion</a> (RA 05 46 45, Dec +00 04 48)<br />Click on the image (below) or the NGC link (above) for more information</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M78 (= <a href="http://cseligman.com/text/atlas/ngc20a.htm#2067" style="color: #660000; text-decoration: none;">NGC 2067</a> and <a href="http://cseligman.com/text/atlas/ngc20a.htm#2068" style="color: #660000; text-decoration: none;">2068</a>) is the bright bluish nebula near the center of the image below. For NGC catalog purposes, M78 is divided into two parts. The brighter region, framed by the semi-circular dark dust lane surrounding the left portion, is <a href="http://cseligman.com/text/atlas/ngc20a.htm#2068" style="color: #660000; text-decoration: none;">NGC 2068</a>. The fainter region, to the right of the dust lane (in this image, to the right), is <a href="http://cseligman.com/text/atlas/ngc20a.htm#2067" style="color: #660000; text-decoration: none;">NGC 2067</a>. The reflection nebula at the top of the image is not considered part of M78, and is referred to as <a href="http://cseligman.com/text/atlas/ngc20a.htm#2071" style="color: #660000; text-decoration: none;">NGC 2071</a>.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><small>(Image credit: T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and AURA/NSF/<a href="http://www.noao.edu/image_gallery/html/im1013.html" style="color: #660000; text-decoration: none;" target="noao">NOAO</a>)</small><br /><a href="http://cseligman.com/text/atlas/ngc20a.htm#2068" style="color: #660000; text-decoration: none;"><img border="1" src="http://cseligman.com/text/stars/m78.jpg" height="894" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="750" /></a></span></div>
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<a href="http://cseligman.com/text/stars/messiernebulae.htm#78" style="color: #660000; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://cseligman.com/text/stars/messiernebulae.htm#78</span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><b><span style="color: #660000;">MESSIER 78 - UM ESPETÁCULO DE FORMAÇÃO DE ESTRELAS</span></b><br /><br /><span style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px;"><img src="http://www.spitzer.caltech.edu/uploaded_files/images/0007/9109/sig11-008_Sm.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; cursor: move; padding: 8px;" /></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://www.spitzer.caltech.edu/images/3658-sig11-008-Making-a-Spectacle-of-Star-Formation-in-Orion#" style="color: #660000; text-decoration: none;">http://www.spitzer.caltech.edu/images/3658-sig11-008-Making-a-Spectacle-of-Star-Formation-in-Orion#</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Making a Spectacle of Star Formation in Orion</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Looking like a pair of eyeglasses only a rock star would wear, this nebula brings into focus a murky region of star formation. NASA's Spitzer Space Telescope exposes the depths of this dusty nebula with its infrared vision, showing stellar infants that are lost behind dark clouds when viewed in visible light.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Best known as Messier 78</b></span><span style="font-family: Arial, Helvetica, sans-serif;">, the two round greenish nebulae are actually cavities carved out of the surrounding dark dust clouds. The extended dust is mostly dark, even to Spitzer's view, but the edges show up in mid-wavelength infrared light as glowing red frames surrounding the bright interiors. Messier 78 is easily seen in small telescopes to the naked eye in the constellation of Orion, just to the northeast of Orion's belt, but looks strikingly different, with dominant, dark swaths of dust. Spitzer's infrared eyes penetrate this dust, revealing the glowing interior of the nebulae.</span></div>
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<span lang="EN-US" style="color: #073763;"><span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Orion and Haase (Lepus the Rabbit) </span></span><strong style="font-family: Arial, Helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1098" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #660000; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">Johann Ehlert Bode</a></span></div>
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<span lang="EN-US"><b style="color: #660000; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">M42 E M43</b></span></div>
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<span lang="EN-US"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>composto pelas estrelas Teta e Iota Orionis.</b></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Neste Asterismo, </b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>estaremos encontrando </b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>os Objetos Messier</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M42 e M43.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Theta Orionis - O Trapézio - Estrelas Duplas</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h32m Declinação - 05<sup>o</sup>.25<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Distância entre estrelas: 8”,922 - 12”,98 - 21”71<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Magnitudes: 6,9 e 6,0 - 6,9 e 5,4 - 6,9 e 6,8<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">AR 05h33m Dec - 5<sup>o</sup>.25<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal;">http://www.nightskyatlas.com/viewer.jsp?rightAscension=5.5883&declination=-5.39&viewAngle=20.0</span></h3>
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<a href="https://www.blogger.com/null" name="m81" style="line-height: normal;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 42</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Starforming Nebula</a> M42 (NGC 1976)</i>, an emission and reflection nebula, with <a href="http://messier.obspm.fr/cluster.html">Open Star Cluster</a>, in <a href="http://messier.obspm.fr/map/Ori.html">Orion</a></center>
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<b><span style="font-size: large;">Orion Nebula</span></b></center>
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<a href="http://messier.obspm.fr/Jpg/m42.jpg"><img align="right" alt="[m42.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m42.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">05 : 35.4 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-05 : 27 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">4.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">85x60 (arc min)</td></tr>
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Nebula possibly discovered 1610 by Nicholas-Claude Fabri de Peiresc.<br />
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Independently found by Johann Baptist Cysatus in 1611.<br />
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Trapezium cluster found as multiple star by Galileo Galilei in 1617.<br />
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The Orion Nebula Messier 42 (M42, NGC 1976) is the brightest starforming, and the brightest diffuse nebula in the sky, and also one of the brightest deepsky objects at all. Shining with the brightness of a star of 4th magnitude, it visible to the naked eye under moderately good conditions, and rewarding in telescopes of every size, from the smallest glasses to the greatest Earth-bound observatories as well as outer-space observatories like the Hubble Space Telescope. It is also a <i>big</i> object in the sky, extending to over 1 degree in diameter, thus covering more than four times the area of the Full Moon.<br />
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As it is so well visible to the naked eye, one may wonder why its nebulous nature was apparently not documented before the invention of the telescope. Only some Central American, Mayan folk tales may be interpreted in a way suggesting that these native Americans may have known of this nebulous object in the sky (<a href="http://messier.obspm.fr/m/m042.html#odell2003">O'Dell 2003</a>, p. 3). However, the brightest stars within the nebula were noted early and cataloged as one bright star of about fifth magnitude: In about 130 AD, <a href="http://messier.obspm.fr/xtra/Bios/ptolemy.html">Ptolemy</a>included it in his catalog, as did <a href="http://messier.obspm.fr/xtra/Bios/tycho.html">Tycho Brahe</a> in the late 16th century, and <a href="http://messier.obspm.fr/xtra/Bios/bayer.html">Johann Bayer</a> in 1603 - the latter cataloging it as Theta Orion in his <i>Uranometria</i>. In 1610, <a href="http://messier.obspm.fr/xtra/Bios/galileo.html">Galileo</a> detected a number of faint stars when first looking at this region with his telescope, but didn't note the nebula. Some years later, on February 4, 1617, Galileo took a closer look at the main star, Theta1, and found it to be triple, at his magnification of 27 or 28x, again not perceiving the nebula.<br />
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The Orion Nebula was probably discovered in late 1610, when <a href="http://messier.obspm.fr/xtra/Bios/peiresc.html">Nicholas-Claude Fabri de Peiresc</a> (1580-1637), a French lawyer, turned his telescope to this region of the sky, and reported of a cloudy nebulosity. This sighting, however, was not published, but only reported in Peiresc's personal documents and brought up only by <a href="http://messier.obspm.fr/m/m042.html#bigourdan1916">Bigourdan (1916)</a>. It was independently found in 1611 by the Jesuit astronomer <a href="http://messier.obspm.fr/xtra/Bios/cysatus.html">Johann Baptist Cysatus</a> (1588-1657) of Lucerne who compared it to a comet he had observed in the year 1618 (<a href="http://messier.obspm.fr/m/m042.html#cysat1619">Cysat 1619</a>). This work also did not get widely known, and opnly turned up by Rudolf Wolf in 1854 (<a href="http://messier.obspm.fr/m/m042.html#wolf1854">Wolf 1854</a>). The <a href="http://messier.obspm.fr/more/m042_hodierna.html">first known drawing of the Orion nebula</a> was created by <a href="http://messier.obspm.fr/xtra/Bios/hodierna.html">Giovanni Batista Hodierna</a>, who included three stars; these are probably Theta1 as well as Theta2A and Theta2B. All these discoveries apparently <a href="http://messier.obspm.fr/more/m042_dis.html">got lost for some time</a>, so that eventually <a href="http://messier.obspm.fr/xtra/Bios/huygens.html">Christian Huygens</a> was longly credited for his independent rediscovery in 1656, e.g. by<a href="http://messier.obspm.fr/xtra/Bios/halley.html">Edmond Halley</a> who included it in his <a href="http://messier.obspm.fr/xtra/similar/halley.html">list of six "nebulae"</a> (<a href="http://messier.obspm.fr/m/m042.html#halley1716">Halley 1716</a>), by <a href="http://messier.obspm.fr/xtra/Bios/demairan.html">Jean-Jacques d'Ortous de Mairan</a> in his <a href="http://messier.obspm.fr/xtra/history/mairan_o.html">nebulae descriptions</a>, by <a href="http://messier.obspm.fr/xtra/Bios/decheseaux.html">Philippe Loys de Chéseaux</a> in <a href="http://messier.obspm.fr/xtra/similar/deches.html">his list</a>, by <a href="http://messier.obspm.fr/xtra/Bios/legentil.html">Guillaume Legentil</a> in his review, and by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>when he <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M42">added it to his catalog</a> on March 4, 1769.<br />
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It is somewhat unusual that the Orion Nebula has found its way into <a href="http://messier.obspm.fr/xtra/history/m-cat.html">Messier's list</a>, together with the bright star clusters <a href="http://messier.obspm.fr/m/m044.html">Praesepe M44</a> and the <a href="http://messier.obspm.fr/m/m045.html">Pleiades M45</a>; Charles Messier usually only included fainter objects which could be easily taken for comets. But in this one night of March 4, 1769, he determined the positions of these wellknown objects, (to say it with Owen Gingerich) `evidently adding these as "frosting" to bring the list to 45', for its first publication in the <i>Memoires de l'Academie</i> for 1771 (published 1774). <a href="http://messier.obspm.fr/m-q&a.html#why_M42-45">One may speculate why</a> he prefered a list of 45 entries over one with 41; a possible reason may be that he wanted to beat <a href="http://messier.obspm.fr/xtra/history/lacaille.html">Lacaille's 1755 catalog</a> of southern objects, which had 42 entries. Messier measured an extra position for a smaller northeastern portion, reported by <a href="http://messier.obspm.fr/xtra/Bios/demairan.html">Jean-Jacques d'Ortous de Mairan</a> previously in 1731 as a separate nebula, which therefore since has the extra Messier number: <a href="http://messier.obspm.fr/m/m043.html">M43</a>.<br />
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As the drawings of the Orion Nebula known to him did so poorly represent Messier's impression, he created a <a href="http://messier.obspm.fr/xtra/history/m-m31_42.html">fine drawing</a> of this Object, in order to "help to recognize it again, provided that it is not subject to change with time" (as Messier states in the <a href="http://messier.obspm.fr/xtra/history/m-cat-i.html">introduction to his catalog</a>).</div>
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LEIA MUITO MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m042.html</div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/2f/Different_Slant_on_Orion_%28495636660%29.jpg/800px-Different_Slant_on_Orion_%28495636660%29.jpg" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion#mediaviewer/File:Different_Slant_on_Orion_(495636660).jpg</span><br />
<div class="mw-mmv-title-para" style="color: #333333; font-family: sans-serif; font-size: 16px; line-height: 1.5em; overflow: visible; padding: 10px 20px 0px; text-overflow: ellipsis;">
<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Different Slant on Orion </span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a href="http://commons.wikimedia.org/wiki/User:Steveblackimages" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="User:Steveblackimages">Steve Black</a> from Las Vegas, NV, USA</span> - <span class="mw-mmv-source"><a class="external text" href="http://www.flickr.com/photos/7634329@N07/495636660/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">Different Slant on Orion</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1976 - M42 - Orion - Nebulosa de Emissão HII Orion</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h43m Declinação -05<sup>o</sup>.25<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária HII Dimensão 30,0 Magnitude 18<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 4 Distância em anos-luz 1,5<o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Grande Nebulosa em Orion, também conhecida como M42, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é uma das mais famosas nebulosas no céu. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> As nuvens de gás e as jovens e quentes estrelas na região formadora de estrelas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> são vicinais à Nebulosa M43, bem menor, e à Nebulosa NGC 1997 e suas amigas, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem como um complexo de nuvens gigantes moleculares invisíveis... </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e tudo isso representando uma pequena fração </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">desta vizinhança galáctica riquíssima em material interestelar. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Dentro desse berçário estelar bem-estudado, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">os astrônomos também identificaram</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> aquilo que parecem ser numerosos sistemas planetários ainda infantes. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Esse glorioso cenário espraia-se por quase dois graus </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ou cerca de 45 anos-luz na Nebulosa de Orion </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> - cuja distância é estimada em 1.500 anos-luz.<o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>NGC 1976 - M 42 - Aglomerado Aberto Trapézio - Órion</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 05h34m Declinação - 05<sup>o</sup>.24<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 2,5 Distância kpc 0,41<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Diâmetro 50’ Tipo Espectral O5<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Grande Nebulosa da Espada de Órion.<o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A Grande Nebulosa na Espada de Orion. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma das mais extensas nebulosas de nossa Galáxia, </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">depois da nebulosa de Eta Carinae. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Situa-se no punhal de Órion e pode ser vista a olho nú,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> bem melhor através um par de binóculos </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e melhor ainda através o telescópio. </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao centro, destaca-se o grupo de estrelas </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">denominado de Eta de Órion, o Trapézio de Órion.<o:p></o:p></span><br />
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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Theta1 Orionis: </h2>
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The Trapezium Cluster in the Orion Nebula M42</h2>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> Trapezium Cluster</i>, in the <a href="http://messier.obspm.fr/m/m042.html">Orion Nebula M42 (NGC 1976)</a>, in <a href="http://messier.obspm.fr/map/Ori.html">Orion</a></center>
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<a href="http://messier.obspm.fr/Pics/More/m42detail.jpg" name="m42detail"><img align="right" alt="[M42 detail, AAT 29]" border="0" src="http://messier.obspm.fr/Pics/More/m42detail.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">05 : 35.4 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-05 : 27 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.6 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">4.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">47 (arc min)</td></tr>
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Discovered by Galileo Galilei in 1617.</div>
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The first recorded observation of a multiple star character of Theta1 Orionis, the bright stellar object in the <a href="http://messier.obspm.fr/m/m042.html">Orion Nebula (M42)</a>, occurred on February 4, 1617, when it was observed and recorded as triple by <a href="http://messier.obspm.fr/xtra/Bios/galileo.html">Galileo Galilei</a> (<a href="http://messier.obspm.fr/more/m042_trapezium.html#galileo1617">Galileo 1617</a>, <a href="http://messier.obspm.fr/more/m042_trapezium.html#fedele1949">Fedele 1949</a>, <a href="http://messier.obspm.fr/more/m042_trapezium.html#ondra1999">Ondra 1999</a>, <a href="http://messier.obspm.fr/more/m042_trapezium.html#mosher2005">Mosher 2005</a>), who did, however, not recognize the Orion Nebula due to unknown reasons.</div>
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With Galileo's observation generally unrecognized, Theta1 Orionis independently revealed as triple star and described by <a href="http://messier.obspm.fr/xtra/Bios/huygens.html">Christiaan Huygens</a> in 1656 (<a href="http://messier.obspm.fr/more/m042_trapezium.html#huygens1659">Huygens 1659</a>). The fourth component, Theta1 Orionis B, was found by <a href="http://messier.obspm.fr/xtra/Bios/picard.html">Abbe Jean Picard</a> in 1673 to complete the "Trapezium." The fourth Trapezium star was independently recovered by Christiaan Huygens in 1684.</div>
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LEIA MAIS</div>
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em</div>
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<a href="http://messier.obspm.fr/more/m042_trapezium.html">http://messier.obspm.fr/more/m042_trapezium.html</a></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.astropix.com/wp/2012/01/25/theta-orionis-the-trapezium/" rel="bookmark" style="color: #660000; text-decoration: none;" title="Permanent Link to Theta Orionis, The Trapezium">Theta Orionis, The Trapezium</a></span></span></h3>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif; line-height: 1.4em; text-align: justify;"><a href="http://www.astropix.com/HTML/SHOW_DIG/Theta_Orionis_The_Trapezium.HTM" style="color: #660000; line-height: 1.4em; text-decoration: none;"><img border="1" src="http://www.astropix.com/wp/wp-content/uploads/2012/01/Trap.JPG" height="427" hspace="10" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; max-width: 100%; padding: 0px; position: relative; text-align: left;" vspace="10" width="640" /></a></span></span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="line-height: 1.4em;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 1.4em;">This is the </span><a href="http://www.astropix.com/HTML/SHOW_DIG/Theta_Orionis_The_Trapezium.HTM" style="color: #660000; line-height: 1.4em; text-decoration: none;">Trapezium, Theta Orionis</a><span style="line-height: 1.4em;">. </span></span></span></span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="line-height: 1.4em;"></span><br /></span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;">Theta Orionis is probably the most famous multiple star system in the entire sky.</span></span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;">Ten of its members can be seen here. There are many more hidden in the dust of the <a href="http://www.astropix.com/HTML/SHOW_DIG/M42_Orion_Nebula.HTM" style="color: #660000; text-decoration: none;">Orion Nebula</a>, which is a factory for star birth.</span></span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;">This is a composite of just 81 seconds of total exposure with 5 x 10 seconds at ISO 1600, 2 x 10 seconds at ISO 400, 1 x 1 second at ISO 400, and 2 x 5 seconds at ISO 400 combined via layer masks in Photoshop into a high-dynamic range image.</span></span></div>
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<span lang="EN-US" style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px;"><a href="http://www.astropix.com/wp/2012/01/" style="color: #660000; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.astropix.com/wp/2012/01/</span></a></span><br />
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1109/orion_spitzerR600h.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br /><a href="http://apod.nasa.gov/apod/ap110917.html" style="color: #660000; text-decoration: none;">http://apod.nasa.gov/apod/ap110917.html</a></span></span><br />
<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><b>Spitzer's Orion </b><br /><b>Credit: </b><a href="http://www.nasa.gov/" style="color: #660000; text-decoration: none;">NASA</a>, <a href="http://spitzer.caltech.edu/" style="color: #660000; text-decoration: none;">JPL-Caltech</a>, T. Megeath (Univ. Toledo, Ohio)</span></span><br />
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<span lang="EN-US"><b>Spitzer's Orion </b><br /><b>Credit: </b><a href="http://www.nasa.gov/">NASA</a>, <a href="http://spitzer.caltech.edu/">JPL-Caltech</a>, T. Megeath (Univ. Toledo, Ohio)</span></center>
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<span lang="EN-US"><b>Explanation: </b>Few cosmic vistas excite the imagination like <a href="http://www.seds.org/messier/m/m042.html">the Orion Nebula</a>, an immense stellar nursery some 1,500 light-years away. <a href="http://www.spitzer.caltech.edu/images/3628-ssc2011-06a-Stars-Adorn-Orion-s-Sword">This stunning false-color view</a> spans about 40 light-years across the region, constructed using <a href="http://coolcosmos.ipac.caltech.edu/cosmic_classroom/ir_tutorial/importance.html">infrared data</a>from the Spitzer Space Telescope. Compared to its <a href="http://apod.nasa.gov/apod/ap110913.html">visual wavelength</a> appearance, the brightest portion of the nebula is likewise centered on Orion's young, massive, hot stars, known as the <a href="http://www.astropix.com/HTML/B_WINTER/TRAPEZ.HTM">Trapezium Cluster</a>. But the infrared image also detects the nebula's many protostars, still in the process of formation, seen here in red hues. In fact, red spots along the dark dusty filament to the left of the bright cluster include the protostar cataloged as HOPS 68, recently <a href="http://www.spitzer.caltech.edu/images/3632-ssc2011-06c-Cosmic-Fountain-of-Crystal-Rain">found to have crystals</a> of the silicate mineral olivine within its <a href="http://arxiv.org/abs/1104.4498">protostellar envelope</a>.</span></div>
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<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Extraído de As Constelações, Cartas Celestes - ORION - Mario Jaci Monteiro</span></span></div>
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<span lang="EN-US"><span style="color: #660000;">A <b><a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Nebulosa">nebulosa</a> de Órion</b> ou <b>nebulosa de Orião</b>, também descrita como <b>M42</b> ou <b>NGC 1976</b>,</span><span style="color: #252525;"> de acordo com a nomenclatura <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Astronomia">astronômica</a>, é uma <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> difusa que se encontra entre 1500 e 1800 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sistema Solar">Sistema Solar</a>, e situada a sul do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/%C3%93rion_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Órion (constelação)">Cinto de Órion</a>.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> . Foi descoberta por <a href="http://pt.wikipedia.org/wiki/Nicolas-Claude_Fabri_de_Peiresc" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nicolas-Claude Fabri de Peiresc">Nicolas-Claude Fabri de Peiresc</a> em 1610 (anteriormente havia sido classificada como estrela - Theta Orionis). Existem muitas outras (fracas) nebulosas ao redor da nebulosa Orion e existem muitas formações de estrelas na região. A nebulosa Orion é, provavelmente, a nebulosa mais ativamente estudada do céu. O seu nome provém da sua localização na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> <a href="http://pt.wikipedia.org/wiki/Orion_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Orion (constelação)">Orion</a>. Possui 25 anos-luz de <a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a>, uma<a href="http://pt.wikipedia.org/wiki/Densidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Densidade">densidade</a> de 600 <a href="http://pt.wikipedia.org/wiki/%C3%81tomo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Átomo">átomos</a>/cm³ e <a href="http://pt.wikipedia.org/wiki/Temperatura" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Temperatura">temperatura</a> de 70 <a href="http://pt.wikipedia.org/wiki/Kelvin" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kelvin">K</a>. Trata-se de uma região de <a href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Formação estelar">formação estelar</a>: em seu interior as estrelas estão nascendo e começando a brilhar constantemente. Há uma enorme concentração de poeira estelar e de gases nessa região, o que sugere a existência de <a href="http://pt.wikipedia.org/wiki/%C3%81gua" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Água">água</a>, pela junção de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Hidrog%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hidrogênio">hidrogênio</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Oxigênio">oxigênio</a>.</span></span></div>
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<span lang="EN-US">É uma das <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosas</a> mais brilhantes, e pode ser observada a <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Simples_vista&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="Simples vista (página não existe)">simples vista</a> sobre o céu noturno. Fica a 1.270±76 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>,<span class="reference" id="cite_ref-apj667_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion#cite_note-apj667-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> e possui um diâmetro aproximado de 24 anos-luz. Os textos mais antigos denominam-na <i><b>Ensis</b></i>, palavra <a href="http://pt.wikipedia.org/wiki/Latim" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Latim">latina</a> que significa "espada", nome que também recebe a estrela <a href="http://pt.wikipedia.org/wiki/Eta_Orionis" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Eta Orionis">Eta Orionis</a>, que desde a Terra se vê muito próxima à nebulosa.<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></span></div>
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<span lang="EN-US">A nebulosa de Órion é um dos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objeto_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Objeto astronômico">objetos astronômicos</a> mais fotografados, examinados, e investigados.<span class="reference" id="cite_ref-successor_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion#cite_note-successor-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span> Dela obteve-se informação determinante a respeito da <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_de_estrelas" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Formação de estrelas">formação de estrelas</a> e <a href="http://pt.wikipedia.org/wiki/Planeta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Planeta">planetas</a> a partir de nuvens de poeira e gás em colisão. Os astrônomos observaram nas suas entranhas <a href="http://pt.wikipedia.org/wiki/Disco_protoplanet%C3%A1rio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Disco protoplanetário">discos protoplanetários</a>, <a href="http://pt.wikipedia.org/wiki/An%C3%A3_marrom" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anã marrom">anãs castanhas</a>, fortes turbulências no movimento de partículas de gás e efeitos fotoionizantes perto de estrelas muito massivas próximas à nebulosa.</span></div>
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<span lang="EN-US">LEIA MUITO MAIS</span></div>
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<span lang="EN-US">em</span></div>
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<span lang="EN-US"><span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion">http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion</a></span></span></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; font-size: 15px; text-align: center;"><b>Nebulosa de Órion</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Different_Slant_on_Orion_(495636660).jpg" style="background: none; color: #0b0080; text-decoration: none;" title="{{{legenda}}}"><img alt="{{{legenda}}}" data-file-height="4814" data-file-width="4941" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/2f/Different_Slant_on_Orion_%28495636660%29.jpg/250px-Different_Slant_on_Orion_%28495636660%29.jpg" height="244" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2f/Different_Slant_on_Orion_%28495636660%29.jpg/375px-Different_Slant_on_Orion_%28495636660%29.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2f/Different_Slant_on_Orion_%28495636660%29.jpg/500px-Different_Slant_on_Orion_%28495636660%29.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Nebulosa de Órion</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;">Nicolas-Claude Peiresc</td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;">1610</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_emiss%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Nebulosa de emissão">nebulosa de emissão</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Orion_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Orion (constelação)">Orion</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">05<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 32<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 49<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-05° 25′</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">4,0</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">média de 1 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">85,0 × 60,0 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">Messier</a> 42, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 1976</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa de Órion"><img alt="Nebulosa de Órion" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Orion_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Orion constellation map.png" data-file-height="2639" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/250px-Orion_constellation_map.png" height="258" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/375px-Orion_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/500px-Orion_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span lang="EN-US"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion">http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion</a></span></span></span></div>
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<span lang="EN-US"><span style="background-color: white;"><span style="color: #252525; font-family: sans-serif; line-height: 17.3185615539551px;">Desenho da nebulosa de Órion realizado por Messier em 1771, </span></span></span></div>
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<span lang="EN-US"><span style="background-color: white;"><span style="color: #252525; font-family: sans-serif; line-height: 17.3185615539551px;">publicado no seu trabalho </span><i style="color: #252525; font-family: sans-serif; line-height: 17.3185615539551px;">Mémoires de l'Académie Royale</i><span style="color: #252525; font-family: sans-serif; line-height: 17.3185615539551px;"> </span></span></span></div>
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<span lang="EN-US">Charles Messier</span></div>
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<span lang="EN-US"><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.................... e </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, que apercebeu-se da sua existência em </span><a href="http://pt.wikipedia.org/wiki/4_de_mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="4 de março">4 de março</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/1769" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1769">1769</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, observando também três das estrelas do cúmulo do Trapézio, embora a descoberta destas três estrelas seja atribuída a </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Galileu" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galileu">Galileu</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1617" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1617">1617</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, apesar de não poder observar a nebulosa (possivelmente devido ao limitado campo de visão do seu primitivo </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópio</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">). Charles Messier publicou a primeira edição do seu </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Catálogo Messier">catálogo de objetos astronômicos</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1774" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1774">1774</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><span class="reference" id="cite_ref-13" style="bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion#cite_note-13" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">13</a></span><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> A nebulosa de Órion foi designada neste catálogo como M42, por ser o objeto número 42 de tal lista em ser descoberto.</span></span></div>
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<span lang="EN-US"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://cseligman.com/text/atlas/ngc19a.htm#1976">http://cseligman.com/text/atlas/ngc19a.htm#1976</a><br /><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="42" style="color: black;"><big><b>M42 (= </b></big></a><big style="color: black;"><b><a href="http://cseligman.com/text/atlas/ngc19a.htm#1976">NGC 1976</a>) -- The Orion Nebula</b></big><br /><span style="color: black;">Discovered (Nov 24, 1610) by </span><a href="http://cseligman.com/text/atlas/discoverers.htm#peiresc" style="color: black;">Nicolas Peiresc</a><br /><span style="color: black;">Earliest known drawing (sometime before 1654) by </span><a href="http://cseligman.com/text/atlas/discoverers.htm#hodierna" style="color: black;">Giovanni Hodierna</a><span style="color: black;"> (list I, #5)</span><br /><span style="color: black;">Recorded (Mar 4, 1769) by </span><a href="http://cseligman.com/text/atlas/discoverers.htm#messier" style="color: black;">Messier</a><br /><span style="color: black;">A 4th-magnitude emission nebula (and star cluster) in </span><a href="http://cseligman.com/text/atlas/orion.htm#1976" style="color: black;">Orion</a><span style="color: black;"> (RA 05 35 17, Dec -05 23 25)</span><br /><span style="color: black;">Click on the image (below) or the NGC link (above) for more information</span><br /><small style="color: black;">(Image credits: <a href="http://hubblesite.org/newscenter/archive/releases/2006/01/fastfacts/" target="apod">NASA</a>, ESA, M. Robberto (STScI/ESA) and The Hubble Space Telescope Orion Treasury Project Team)</small><br /><a href="http://cseligman.com/text/atlas/ngc19a.htm#1976" style="color: black;"><img border="1" src="http://cseligman.com/text/stars/m42.jpg" height="750" width="750" /></a><br /><a href="http://cseligman.com/text/atlas/ngc19a.htm#1976" style="color: black;">http://cseligman.com/text/atlas/ngc19a.htm#1976</a><a href="http://www.blogger.com/blogger.g?blogID=7155777971455253706" name="43" style="color: black;"><br /><big><b>M43 (= </b></big></a><big style="color: black;"><b><a href="http://cseligman.com/text/atlas/ngc19a.htm#1982">NGC 1982</a>)</b></big><br /><span style="color: black;">Discovered (1731) by </span><a href="http://cseligman.com/text/atlas/discoverers.htm#mairan" style="color: black;">Jean-Jacques Mairan</a><span style="color: black;"> (Recorded by </span><a href="http://cseligman.com/text/atlas/discoverers.htm#messier" style="color: black;">Messier</a><span style="color: black;"> in 1769)</span><br /><span style="color: black;">A 7th-magnitude emission nebula in </span><a href="http://cseligman.com/text/atlas/orion.htm#1982" style="color: black;">Orion</a><span style="color: black;"> (RA 05 35 31, Dec -05 16 03)</span><br /><span style="color: black;">A portion of the Orion nebula (see </span><a href="http://cseligman.com/text/stars/messiernebulae.htm#42" style="color: black;">M42</a><span style="color: black;">, above) separated from the main portion by a dark lane.</span><br /><span style="color: black;">Click on the image (below) or the NGC link (above) for more information</span><br /><small style="color: black;">(Image credits: <a href="http://hubblesite.org/newscenter/archive/releases/2006/01/fastfacts/" target="apod">NASA</a>, ESA, M. Robberto (STScI/ESA) and The Hubble Space Telescope Orion Treasury Project Team)</small><br /><a href="http://cseligman.com/text/atlas/ngc19a.htm#1982" style="color: black;"><img border="1" src="http://cseligman.com/text/stars/m43.jpg" height="741" width="750" /></a></span></span></span></div>
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<span lang="EN-US"><a href="https://www.blogger.com/null" name="m81"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
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Messier 43</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Starforming Nebula</a> M43 (NGC 1982)</i>, </span></center>
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<span lang="EN-US">an emission and reflection nebula, with <a href="http://messier.obspm.fr/cluster.html">Open Star Cluster</a>, in <a href="http://messier.obspm.fr/map/Ori.html">Orion</a></span></center>
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<span lang="EN-US"><br /><b><span style="font-size: large;">De Mairan's Nebula, Companion of the Orion Nebula</span></b><br /><b><span style="font-size: large;"><br /></span></b><div>
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<tr><th align="left">Right Ascension</th><td align="center">05 : 35.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-05 : 16 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.0 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">20x15 (arc min)</td></tr>
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<span lang="EN-US">Discovered before 1731 by Jean-Jacques Dortous de Mairan.</span></div>
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<span lang="EN-US">Messier 43 (M43, NGC 1982) is the companion of the Great Orion Nebula, <a href="http://messier.obspm.fr/m/m042.html">M42</a>. It is separated from the great nebula by an impressive, turbulent dark lane, and is lying 7 arcmin north of the Trapezium Cluster.</span></div>
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<span lang="EN-US">M43 was <a href="http://messier.obspm.fr/Mdes/dm043.html#DeMairan">first reported</a> by <a href="http://messier.obspm.fr/xtra/Bios/demairan.html">de Mairan</a> in 1731 as a "brilliance surrounding a star" which he thought was "very similar to the atmosphere of our Sun, if it were dense enough and extensive enough to be visible in telescopes at a similar distance" (<a href="http://messier.obspm.fr/m/m043.html#demairan1733">De Mairan 1733</a>). <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included in his <a href="http://messier.obspm.fr/xtra/history/m-m31_42.html">fine drawing of the Orion Nebula</a>, and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M43">assigned it</a> an extra catalog number, M43, on March 4, 1769. </span></div>
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<span lang="EN-US">Moreover, <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> took it into his list with the number H III.1, although normally he careful avoided to <a href="http://messier.obspm.fr/xtra/similar/herschel.html">assign his numbers</a> to Messier Objects. In his 1811 paper, Herschel states to have observed it as early as March 4, 1774, and cataloged it on November 3, 1783. M43 shows up on the first deep photograph of the Orion Nebula, taken on March 14, 1882 by <a href="http://messier.obspm.fr/xtra/Bios/draper.html">Henry Draper</a>.</span></div>
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<span lang="EN-US">LEIA MAIS</span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://messier.obspm.fr/m/m043.html">http://messier.obspm.fr/m/m043.html</a></span></span></div>
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<span lang="EN-US"><a href="http://annesastronomynews.com/annes-image-of-the-day-star-forming-region-messier-43/"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-image-of-the-day-star-forming-region-messier-43/</span></a></span></div>
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<span lang="EN-US"><strong style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 43, a star-forming region in Orion</span></strong></span></div>
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<span lang="EN-US"><span style="border: 0px; color: #073763; font-family: Arial, Helvetica, sans-serif; margin: 0px; outline: 0px; padding: 0px;"><a href="http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/messier-43/" rel="attachment wp-att-10318" style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><img alt="NGC 1982, De Mairan's Nebula" class="aligncenter size-full wp-image-10318" src="http://annesastronomynews.com/wp-content/uploads/2012/02/Messier-43.jpg" style="border: none; display: block; margin: 0px auto; max-width: 100%; outline: 0px; padding: 0px;" width="1024" /></a></span></span></div>
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<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Image Credit: <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px;">NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team.</em></span></span></div>
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<span lang="EN-US"><span style="border: 0px; margin: 0px; outline: 0px; padding: 0px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 43 (also known as NGC 1982 or De Mairan’s Nebula</b>, after its discoverer Jean-Jacques Dortous de Mairan) is a star-forming (H II) region of some 3 light-years across that lies about 1,600 light-years away from Earth in the Orion Arm of our Milky Way galaxy, in the constellation of Orion (the Hunter).</span></span></span></div>
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<span lang="EN-US"><a href="http://annesastronomynews.com/annes-image-of-the-day-star-forming-region-messier-43/"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://annesastronomynews.com/annes-image-of-the-day-star-forming-region-messier-43/</span></a></span></div>
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<span lang="EN-US"><span style="color: black; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /><br /><br /><br /><span style="color: #660000;"><br /></span></b></span><span style="color: #660000;"><b style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 43</b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (também conhecido como </span><b style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">M43</b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, </span><b style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Nebulosa De Mairan</b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, e </span><b style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 1982</b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">)</span></span><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é uma </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Região HII">região HII</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Orion_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Orion (constelação)">Orion</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Foi descoberto por </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Jean-Jacques_De_Mairan_Dortous&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Jean-Jacques De Mairan Dortous (página não existe)">Jean-Jacques De Mairan Dortous</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> antes de </span><a href="http://pt.wikipedia.org/wiki/1731" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1731">1731</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> . De Mairan da nebulosa é parte da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Nebulosa_de_Orion" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa de Orion">nebulosa de Orion</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> , separada da nebulosa principal por uma faixa de </span><a href="http://pt.wikipedia.org/wiki/Poeira" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Poeira">poeira</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> . É parte do maior complexo da </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Nuvem_Molecular_de_Orion&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nuvem Molecular de Orion (página não existe)">Nuvem Molecular de Orion</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /><br />........................................</b></span></span></span></div>
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<span lang="EN-US"><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">A </span><a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa">nebulosa</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> foi registrada pela primeira vez por </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Jean-Jacques_d%27Ortous_de_Mairan&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Jean-Jacques d'Ortous de Mairan (página não existe)">Jean-Jacques d'Ortous de Mairan</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em 1731, descrita por ele como um "brilho envolvendo uma estrela" e que era "muito semelhante à </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Atmosfera_Solar&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Atmosfera Solar (página não existe)">atmosfera Solar</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, se fosse suficientemente densa e extensa para ser visível em </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Telescópio">telescópios</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> a uma distância semelhante." O astrônomo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">incluiu-o em um desenho da </span><a href="http://pt.wikipedia.org/wiki/Nebulosa_de_%C3%93rion" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Nebulosa de Órion">nebulosa de Órion</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e também o incluiu em seu </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Catálogo Messier">catálogo</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> como sua entrada número 43 (M43) em 4 de março de 1769.</span></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; font-size: 15px; text-align: center;"><b>Messier 43</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M43_HST.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="{{{legenda}}}"><img alt="{{{legenda}}}" data-file-height="5024" data-file-width="5024" src="http://upload.wikimedia.org/wikipedia/commons/thumb/9/93/M43_HST.jpg/250px-M43_HST.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/M43_HST.jpg/375px-M43_HST.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/93/M43_HST.jpg/500px-M43_HST.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 43</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;">Jean-Jacques d'Ortous de Mairan</td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;">1731</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Regi%C3%A3o_HII" style="background: none; color: #0b0080; text-decoration: none;" title="Região HII">Região HII</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Orion_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Orion (constelação)">Orion</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">05<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 35,6<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-05° 16′</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">9,0</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">Magnit. absol.</a></td><td style="background-color: #f8f8f8;"> ?</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">1 600 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">20′x15′ <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #e0e0ff; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M43, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 1982, Nebulosa De Mairan</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 43"><img alt="Messier 43" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Orion_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Orion constellation map.png" data-file-height="2639" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/250px-Orion_constellation_map.png" height="258" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/375px-Orion_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Orion_constellation_map.png/500px-Orion_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span lang="EN-US"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /><a href="http://pt.wikipedia.org/wiki/Messier_43">http://pt.wikipedia.org/wiki/Messier_43</a></span></span></span><br />
<span lang="EN-US"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></span><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="color: black;"><img alt="The Orion Nebula" src="http://imgsrc.hubblesite.org/hu/db/images/hs-2006-01-a-1280_wallpaper.jpg" /></span></span></span><br />
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<span lang="EN-US"><span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Thousands of stars are forming in the cloud of gas and dust known as the Orion nebula. More than 3,000 stars of various sizes appear in this image. Some of them have never been seen in visible light.<o:p></o:p></span></span></span></div>
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<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US">Credit:</span></b><span lang="EN-US"> </span><a href="http://www.nasa.gov/"><span lang="EN-US">NASA</span></a><span lang="EN-US">,</span><a href="http://www.spacetelescope.org/"><span lang="EN-US">ESA</span></a><span lang="EN-US">, M. Robberto (</span><a href="http://www.stsci.edu/"><span lang="EN-US">Space Telescope Science Institute</span></a><span lang="EN-US">/</span><a href="http://www.spacetelescope.org/"><span lang="EN-US">ESA</span></a><span lang="EN-US">) and the Hubble Space</span></span></span></div>
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<span lang="EN-US"><span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Telescope Orion Treasury Project Team</span></span></span></div>
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<span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US"><a href="http://hubblesite.org/gallery/wallpaper/pr2006001a/titles/true/">http://hubblesite.org/gallery/wallpaper/pr2006001a/titles/true/</a></span><span lang="EN-US"><o:p></o:p></span></span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b>Janine Milward</b></span><br /><div>
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<img src="http://www.ianridpath.com/atlases/urania/urania29.jpg" /></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://www.ianridpath.com/atlases/urania/urania29.jpg</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span lang="EN-US"><b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">Com um abraço estrelado,</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">Janine Milward</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">VISITE MINHA PÁGINA</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">DA TERRA AO CÉU E AO INFINITO</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><b><span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></b><span style="font-size: 13.5pt;"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span lang="EN-US"><span class="text_exposed_show" style="display: inline; line-height: 18px; text-align: left;"><a href="http://www.astrophotogallery.org/messier-catalog/p11180-m42-narrow-band.html"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.astrophotogallery.org/messier-catalog/p11180-m42-narrow-band.html</span></a></span></span></span></div>
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<span lang="EN-US"><span lang="EN-US"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.photopost.com/">Photo Sharing Gallery by PhotoPost</a><br />Copyright © 2012 All Enthusiast, Inc.</span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.astrophotogallery.org/m1264-alexw.html" style="background-image: none; display: block; text-align: left; text-decoration: none !important;">AlexW </a><a href="http://www.astrophotogallery.org/m1264-alexw.html" style="background-image: none; display: block; text-align: left; text-decoration: none !important;"> Location: Silver City, NM, USA </a><a href="http://www.astrophotogallery.org/m1264-alexw.html" style="background-image: none; display: block; text-align: left; text-decoration: none !important;"> <b>M42 Narrow Band </b>Target: M42 (Orion Nebula) Scope: 12.5" RCOS Imaging: 14x15s Lum; 10x15s each Ha (R), OIII (G), SII (B)Processing: PixInsight Objective: Trapezium stars and faint nebula together learn PixInsight </a></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-77545622811157839422014-09-06T08:35:00.001-07:002015-01-04T08:14:49.882-08:00Ophiucus<div class="MsoNormal">
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Olá!</span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Nossa visita</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> através a constelação do Serpentário, Ophiucus,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acontecerá em</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">M9, M10, M12, M14, M19, M62 e M107, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">os Objetos Messier em Ophiucus.</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Ophiucus, o Serpentário, Aquele que Segura a Serpente,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">é uma constelação bem interessante</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">porém composta de estrelas não muito proeminentes</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">- e, da mesma forma, assim acontece </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">com a constelação da Serpente, ou seja, Serpens Cauda e Serpens Caput.</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">No entanto, em lugares de céus escuros e transparentes</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">e, de preferência, em noites de ausência de iluminação da Lua,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">podemos observar algumas estrelas pertencentes </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">aos desenhos estelares de Ophiucus e de Serpens!</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">É bem interessante percebermos o fato de que</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">a imensa figura estelar do Serpentário segurando a Serpente</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">- é uma constelação tripla, digamos assim! -,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">se posiciona bem próxima, porém mais ao norte,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">das constelações do Escorpião e do Sagitário</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">e, portanto, </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">bem próxima do ponto que nos leva ao centro da Galáxia.</span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Saiba sobre os Objetos Messier encontrados em Serpens,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- Serpens Cauda e Serpens Caput -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">acessando nosso Trabalho em</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m5-e-m16-os-objetos-messier-em-serpens.html</span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhbhzw1oFXUR6oS7nFSwFvnREzmWi6KXzcusSieA4Wv-vdorVGu3DINLHz-_ieSfNfsy6PO-zYFmz8vNzomeTFOAOIuPWcNIhfCL9vDVlO-EQVfb1PVkMaxsFCG-51X8tcnfbhOtBw49wA/s1600/M12.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhbhzw1oFXUR6oS7nFSwFvnREzmWi6KXzcusSieA4Wv-vdorVGu3DINLHz-_ieSfNfsy6PO-zYFmz8vNzomeTFOAOIuPWcNIhfCL9vDVlO-EQVfb1PVkMaxsFCG-51X8tcnfbhOtBw49wA/s1600/M12.png" /></a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif; line-height: 18px;">http://www.stellarium.org/pt/</span></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; margin-left: 1em; margin-right: 1em;"><br /><br /><img src="http://www.raremaps.com/maps/medium/34480.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: center;">E também estaremos encontrando as constelações Scorpius, Sagittarius, Scutum, Aquila, Hercules Corona Borealis, Libra<o:p></o:p></span><br />
<br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; text-align: center;" />
<a href="http://www.raremaps.com/gallery/detail/34480/Ophiuchus_and_Serpent/Jamieson.html" style="background-color: white; color: #274e13; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; text-align: center; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/34480/Ophiuchus_and_Serpent/Jamieson.html</span></a><br />
<div class="productDetailItem" style="background-color: white; border: 0px; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; margin-bottom: 1em; padding: 0px 0px 10px; text-align: center;">
<span style="font-family: Arial, Helvetica, sans-serif;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1372" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-decoration: none;">Alexander Jamieson</a></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OPHIUCUS, OFIÚCO<o:p></o:p></b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>ou Serpentarius, aquele que Segura a Serpente</b><o:p></o:p></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Ascensão Reta 15h58m / 18h42m Declinação +14<sup>o</sup>.3 / -30<sup>o</sup>.1<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><b>Mito:</b><o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Hercules, quando criança, estrangulou duas serpentes enviadas por Juno para matá-lo enquanto dormia em seu berço. Esta constelação também foi chamada de Esculapius, o pai da medicina.</span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;"><b>Fronteiras:</b><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Ophiucus situa-se entre as constelações Serpens Cauda e Serpens Caput (e todas três acabam formando um conjunto imenso de situações entrelaçadas), e também Scorpius, Sagittarius, Scutum, Aquila, Hercules Corona Borealis, Libra</span><span style="color: #0f243e; font-size: 11pt;"><o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><b>Algumas Informações Interessantes acerca esta Constelação:</b></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Quando o Zodíaco foi originalmente nomeado, </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">a Eclíptica não passava pelo Ofiúco, </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">de forma que esta constelação não foi incluída. </span><br /><span style="font-family: Arial, Helvetica, sans-serif;"> Hoje em dia, sim, em função da precessão, </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Ofiúco recebe a passagem da linha da Eclíptica </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">e o Sol passa um bom tempo aqui </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">depois de ter adentrado a Cabeça do Escorpião </span></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">e passado ao largo de sua estrela Alpha, Antares.</span></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /><br /><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ophiuchus*.html" style="text-decoration: none;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ophiuchus*.html</a></span></span></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.amazon.com/dp/0486210790/ref=rdr_ext_tmb" style="text-decoration: none;">http://www.amazon.com/dp/0486210790/ref=rdr_ext_tmb</a></span></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><span lang="EN-US">- </span><b><span lang="EN-US">Richard Hinckley Allen, Star Names, Their Lore and Meaning</span></b><span lang="EN-US">, Dover Publications, Inc, New York, USA <o:p></o:p></span></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Segundo Allen, em seu livro Star Names, Their Lore and Meaning – fantástico livro e já em domínio público </span></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"><br /></span></span><span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">– e traduzindo literalmente, de forma simples e sintética, </span></span><br />
<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">por mim, Janine:<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">Ophiucus vel Serpentarius, o Serpentário</span></b></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> – não Ophiucus Serpentarius, é Ofiuco em italiano, Schlangentrager em alemão e Serpentaire em francês.<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">...........................<o:p></o:p></span></span><br />
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">…. (Porém) o Serpentário foi normalmente identificado com Asclepios ou Aesculapius, a quem o Rei James I descreveu como “um curador que mais tarde foi feito deus”, com cujas adoradas serpentes eram sempre associados como símbolos de prudência, renovação, sabedoria e o poder de descobrir ervas curadoras. Educado por seu pai Apollo – ou pelo Centauro Quíron -, Aesculapius foi o primeiro em sua profissão e o cirurgião do navio Argo. Quando a famosa viagem terminou, ele estava tão treinado em sua prática que ele pôde até trazer mortos à vida – entre esses, Hippolytus.<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">....................<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Sucessivas operações e inúmeras e notáveis curas – e especialmente a tentativa de reviver Órion morto -, levaram Plutão (que temia pela continuidade de seu reino) induzir Júpiter a atingir Aesculapius com um raio e colocá-lo dentre as constelações.<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Ophiucus também foi associado a Caecius, o Cego, assassinado por Hercules e celebrado por Dante no Inferno. Na verdade, diz-se que o Herói foi atribuído a estas estrelas por Hyginus e nomeou-as com seu nome: uma confusão que pode ter vindo à tona em função das fronteiras entre essas duas constelações – por serem mal-definidas, primeiramente, ou pela similaridade de seus mitos originais em relação a Izhdubar e o dragão Tiamat.<o:p></o:p></span></span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">.......................................<o:p></o:p></span></span></div>
<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span></span><span style="background-color: white;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ophiuchus*.html" style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px; text-decoration: none;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ophiuchus*.html</a></span><br />
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<span style="background-color: white;"><img src="http://www.iau.org/static/public/constellations/gif/OPH.gif" /></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M9, M10, M12, M14, M19, M62 E M107</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO OPHIUCUS</b></span></div>
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http://www.ipac.caltech.edu/2mass/gallery/m9atlas.jpg<br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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Messier 9</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M9 (NGC 6333)</i>, class VIII, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">17 : 19.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-18 : 31 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">25.8 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">12.0 (arc min)</td></tr>
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Discovered 1764 by Charles Messier.</div>
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Globular cluster Messier 9 (M9, NGC 6333) is one of the original discoveries of <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M9">cataloged it</a> on May 28, 1764, and described it as "Nebula without star" of 3' diameter. It was first resolved into stars by <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a>about 20 years later.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m009.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiEF5SmvAMVLqUQT68JzgfOO4CThJDuoODjXnIlfpH2Bxg7WsrMcayblsMyj-Mn_FN8LVUJ8vNNHSvWIY3dxG9bGczUsNGdT_763urQJe4IruvdtwNyzqEE1Jzhg3iT28D6IhV2qdkYPYs/s1600/m9+e+m107.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiEF5SmvAMVLqUQT68JzgfOO4CThJDuoODjXnIlfpH2Bxg7WsrMcayblsMyj-Mn_FN8LVUJ8vNNHSvWIY3dxG9bGczUsNGdT_763urQJe4IruvdtwNyzqEE1Jzhg3iT28D6IhV2qdkYPYs/s1600/m9+e+m107.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M 9 - NGC 6333 - Ophiucus - Aglomerado</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h18m Declinação -18<sup>o</sup>.30<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 7,6 Tipo A7<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<table cellpadding="0" cellspacing="2" class="infobox" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; line-height: 19.1875px; margin: 0px 0px 1em 1em; padding: 0.2em; text-align: center; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 9</span></b></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_9_Hubble_WikiSky_wfpc2_patched.jpg" style="background-image: none; text-decoration: none;" title="Messier 9 visto pelo Telescópio Espacial Hubble."><img alt="Messier 9 visto pelo Telescópio Espacial Hubble." src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/250px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg" height="640" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/375px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/500px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="640" /></a><br />Messier 9 visto pelo Telescópio Espacial Hubble.</span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Descoberto por</span></td><td><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Charles Messier</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><a href="http://pt.wikipedia.org/wiki/1764" style="background-image: none; text-decoration: none;" title="1764"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">1764</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dados observacionais (J2000)</span></b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Constelação</span></a></td><td><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; text-decoration: none;" title="Ophiuchus"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiuchus</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">VII</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; text-decoration: none;" title="Ascensão reta"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Asc. reta</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 19<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 11,78<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Declinação"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Declinação</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">-18° 30′ 58,5″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">25 800 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-image: none; text-decoration: none;" title="Ano-luz">anos-luz</a> (7,9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-image: none; text-decoration: none;" title="Parsec">kpc</a>)</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; text-decoration: none;" title="Magnitude aparente"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnit. apar.</span></a></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">8,42<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background-image: none; text-decoration: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Dimensões</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">12',0</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2"><b><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Características físicas</span></b></td></tr>
<tr style="vertical-align: top;"><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Raio</span></td><td><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">45 anos-luz</span></td></tr>
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<tr style="vertical-align: top;"><td colspan="2"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; text-decoration: none;" title="New General Catalogue">NGC</a> 6333</span></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b style="line-height: 19.1875px; text-align: start;">Messier 9</b><span style="line-height: 19.1875px; text-align: start;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="New General Catalogue">NGC 6333</a><span style="line-height: 19.1875px; text-align: start;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="line-height: 19.1875px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Estrela">estrelas</a><span style="line-height: 19.1875px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="line-height: 19.1875px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Ophiuchus">Ofiúco</a><span style="line-height: 19.1875px; text-align: start;">. Foi descoberto pelo francês </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="line-height: 19.1875px; text-align: start;"> em 1764 e é um dos aglomerados globulares próximos ao centro da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Via-Láctea">Via-Láctea</a><span style="line-height: 19.1875px; text-align: start;">, a uma distância de 5 500 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="line-height: 19.1875px; text-align: start;">. Está a uma distância de cerca de 25 800 anos-luz em relação à </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; line-height: 19.1875px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="line-height: 19.1875px; text-align: start;">.</span></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Messier 9</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_9_Hubble_WikiSky_wfpc2_patched.jpg" style="background: none;" title="Messier 9 visto pelo Telescópio Espacial Hubble."><img alt="Messier 9 visto pelo Telescópio Espacial Hubble." data-file-height="4000" data-file-width="4000" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/250px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/375px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Messier_9_Hubble_WikiSky_wfpc2_patched.jpg/500px-Messier_9_Hubble_WikiSky_wfpc2_patched.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />Messier 9 visto pelo Telescópio Espacial Hubble.</span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Descoberto por</span></span></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; line-height: 22.3999996185303px;" title="Charles Messier"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Charles Messier</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Data</span></span></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; line-height: 22.3999996185303px;" title="1764"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">1764</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Dados observacionais (J2000)</span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 22.3999996185303px;" title="Constelação"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Constelação</span></a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; line-height: 22.3999996185303px;" title="Ophiuchus"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Ophiuchus</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Tipo</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">VII</span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 22.3999996185303px;" title="Ascensão reta"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Asc. reta</span></a></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">17<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 19<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 11,78<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background: none;">1</a></span></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 22.3999996185303px;" title="Declinação"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Declinação</span></a></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">-18° 30′ 58,5″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background: none;">1</a></span></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Distância</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">25 800 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none;" title="Ano-luz">anos-luz</a> (7,9 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none;" title="Parsec">kpc</a>)</span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 22.3999996185303px;" title="Magnitude aparente"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Magnit. apar.</span></a></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">8,42<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_9#cite_note-simbad-1" style="background: none;">1</a></span></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Dimensões</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">12',0</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Características físicas</span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Raio</span></span></td><td style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">45 anos-luz</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;">Outras denominações</span></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none;" title="New General Catalogue">NGC</a> 6333</span></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 22.3999996185303px;" title="Messier 9"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><img alt="Messier 9" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 22.3999996185303px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_9</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.ipac.caltech.edu/2mass/gallery/m10atlas.jpg</span><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
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Messier 10</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M10 (NGC 6254)</i>, class VII, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m10.jpg"><img align="right" alt="[m10.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m10.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">16 : 57.1 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-04 : 06 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">14.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">20.0 (arc min)</td></tr>
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Discovered 1764 by Charles Messier.</div>
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Messier 10 (M10, NGC 6254) is one of the bright globulars populating constellation Ophiuchus.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m010.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEik2dxcAokXE7Q9xnBO6_laP_mkpfm6PGgRVXBgZUTSNE9hcAEo5QBp1I4QGPpBIeh4yEere00jPVneWDh9V79OVYlG_5MEL5EgLw8fA8QydeuTN_AGKBDdDAMkUzmR3Z26T7JXcaxSN9U/s1600/m10,+m12,+m14.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEik2dxcAokXE7Q9xnBO6_laP_mkpfm6PGgRVXBgZUTSNE9hcAEo5QBp1I4QGPpBIeh4yEere00jPVneWDh9V79OVYlG_5MEL5EgLw8fA8QydeuTN_AGKBDdDAMkUzmR3Z26T7JXcaxSN9U/s1600/m10,+m12,+m14.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M 10 - NGC 6254 - Ophiucus - Aglomerado Estelar Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h56 Declinação -04<sup>o</sup>.05<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,5 Tipo AG</span></div>
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<span lang="PT" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Na parte ao sul do Ophiúco existem, entre partes adoráveis da Via Láctea, Nuvens de Estrelas e Nebulosas Escuras. Próximo à estrela Alya, Theta Serpentis, é possível se observar a olho nú uma imensa nuvem escura no formato de um Cachimbo, é a Nebulosa do Cachimbo. Quando observamos esta região e sua vizinhança fazendo parte da Via Láctea em Sagitário, estamos olhando em direção ao centro de nossa Galáxia.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h56m Declinação -04<sup>o</sup>.05<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 7,3 Diâmetro aparente 16’,2 Tipo Espectral G1<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,17<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Número conhecido de Variáveis 3 Distância kpc 6,2<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_10#mediaviewer/File:Messier_10_Hubble_WikiSky.jpg</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 10 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a> - <a class="external text" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=16.952488111678985&de=-4.099788817522698&angle=0.05795360204325173&projection=tan&rotation=5.362764724205696&survey=astrophoto&img_id=60475&width=4200&height=4200&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=zoom" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">Wikisky's snapshot tool</a></span></span></div>
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<b>Messier 10</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6254</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ofiúco</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 29 de maio de 1764, que catalogou o sistema como o décimo objeto de <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">sua lista</a>. Messier descreveu o aglomerado como uma <a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa">nebulosa</a> sem estrelas, embora anos mais tarde, <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de<a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, tenha descoberto que o sistema era formado por milhares de estrelas distintas.</div>
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O aglomerado tem um diâmetro angular de cerca de 20 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>, cerca de dois terços do diâmetro angular da <a href="http://pt.wikipedia.org/wiki/Lua" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lua">Lua</a> na abóbada celeste, correspondendo a um diâmetro real de 80 anos-luz. Sua distância da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> é de cerca de 14 300 anos-luz.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 10</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_10_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 10 visto pelo Telescópio Espacial Hubble."><img alt="Messier 10 visto pelo Telescópio Espacial Hubble." data-file-height="4200" data-file-width="4200" src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/67/Messier_10_Hubble_WikiSky.jpg/250px-Messier_10_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/67/Messier_10_Hubble_WikiSky.jpg/375px-Messier_10_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/67/Messier_10_Hubble_WikiSky.jpg/500px-Messier_10_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 10 visto pelo Telescópio Espacial Hubble.</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;">VII</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">16<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 57<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 08,99<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_10#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-04° 05′ 57,6″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_10#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">14 300 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (4,4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,4<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_10#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">20',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Massa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa">Massa</a></td><td style="background-color: #f8f8f8;">2,25 x 10<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">5</span> <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background: none; color: #0b0080; text-decoration: none;" title="Massa solar">massas solares</a><span class="reference" id="cite_ref-apj522_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_10#cite_note-apj522-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">41,6 anos-luz</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6254</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 10"><img alt="Messier 10" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="line-height: 22.3999996185303px;"><a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span><br />
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<h1>
Messier 12</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M12 (NGC 6218)</i>, class IX, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m12.jpg"><img align="right" alt="[m12.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m12.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">16 : 47.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-01 : 57 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">16.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">16.0 (arc min)</td></tr>
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Discovered by Charles Messier in 1764.</div>
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Messier 12 (M12, NGC 6218) is nearly a twin of its apparent neighbor, <a href="http://messier.obspm.fr/m/m010.html">M10</a>, and is only slightly larger and an idea fainter. Nevertheless, it was once believed to be an intermediate type between globular and dense open clusters (like <a href="http://messier.obspm.fr/m/m011.html">M11</a>), as it is not very concentrated - Harlow Shapley included M12 in his concentration class IX. It is, e.g., notably much less concentrated toward the center than M10 (of class VII). At its distance of about 16,000 light years, the apparent diameter of M12 of 16.0 arc minutes corresponds to about 75 light years. This stellar swarm is approaching us at 16 km/sec.</div>
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LEIA MAIS</div>
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http://messier.obspm.fr/m/m012.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEik2dxcAokXE7Q9xnBO6_laP_mkpfm6PGgRVXBgZUTSNE9hcAEo5QBp1I4QGPpBIeh4yEere00jPVneWDh9V79OVYlG_5MEL5EgLw8fA8QydeuTN_AGKBDdDAMkUzmR3Z26T7JXcaxSN9U/s1600/m10,+m12,+m14.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEik2dxcAokXE7Q9xnBO6_laP_mkpfm6PGgRVXBgZUTSNE9hcAEo5QBp1I4QGPpBIeh4yEere00jPVneWDh9V79OVYlG_5MEL5EgLw8fA8QydeuTN_AGKBDdDAMkUzmR3Z26T7JXcaxSN9U/s1600/m10,+m12,+m14.png" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span></div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M 12 - NGC 6218 - Ophiucus - Aglomerado Estelar Globular</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,7 Tipo AG</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 16h46m Declinação -01<sup>o</sup> 55<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 7,6 Diâmetro aparente 21’,5 Tipo Espectral F8<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 14,07<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Número conhecido de Variáveis 1 Distância kpc 7,4<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Velocidade Radial (km/s) -16<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_12#mediaviewer/File:M12_Hubble.jpg</span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">M12 Hubble</span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author">ESA/Hubble & NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/potw1113a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/potw1113a/</a></span></span></div>
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<b>Messier 12</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6218</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ofiúco</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 30 de maio de 1764.</div>
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Localizado a cerca de 3° de distância de <a href="http://pt.wikipedia.org/wiki/Messier_10" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 10">Messier 10</a> na abóbada celeste, o sistema está a cerca de 16 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e têm um diâmetro espacial de cerca de 75 anos-luz. As estrelas mais brilhantes do aglomerado têm <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 12,0. É pouco denso em relação a outros aglomerado globular e o sistema foi por muito tempo classificado como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a>. Tem <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 6,7 e não é visível a <a class="mw-disambig" href="http://pt.wikipedia.org/wiki/Olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a>, mas visível com <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> ou <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 12</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M12_Hubble.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 12 pelo Telescópio Espacial Hubble"><img alt="Messier 12 pelo Telescópio Espacial Hubble" data-file-height="3708" data-file-width="3899" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/50/M12_Hubble.jpg/250px-M12_Hubble.jpg" height="238" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/50/M12_Hubble.jpg/375px-M12_Hubble.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/50/M12_Hubble.jpg/500px-M12_Hubble.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 12 pelo Telescópio Espacial Hubble</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">16<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 47<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 14,52<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_12#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-01° 56′ 52,1″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_12#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">16 000 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (4,2 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">7,68</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">16',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6218</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 12"><img alt="Messier 12" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 14</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M14 (NGC 6402)</i>, class VIII, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m14.jpg"><img align="right" alt="[m14.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m14.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">17 : 37.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-03 : 15 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">30.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">11.0 (arc min)</td></tr>
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Discovered by Charles Messier in 1764.</div>
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Messier 14 (M14, NGC 6402) is a slightly elliptically shaped stellar swarm, about 100 light years across and about 30,000 light years away; older determinations have given values between 64,000 ly (Shapley) and 23,000 (Mallas/Kreimer) to 24,000 ly (Glyn Jones, Kinman, Becvar); the Sky Catalogue 2000.0 had 38,000 ly. Shapley assigned it an ellipticity of 9, extended in position angle 110 deg. While its bright main body about only about 3 arc minutes in angular diameter, the cluster's outlayers reach out to a total apparent diameter of 11.7 arc min. It lacks a dense central condensation (Burnham), as its concentration class VIII indicates. Its apparent visual brightness of 7.6 visual magnitudes corresponds to an absolute magnitude of -9.12, or to a luminosity about 400,000 times that of our sun - so while, because of its greater distance, it is apparently dimmer than the two other great Ophiuchus clusters, <a href="http://messier.obspm.fr/m/m010.html">M10</a> and <a href="http://messier.obspm.fr/m/m012.html">M12</a>, it is intrinsically much more luminous.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m014.html</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">M 14 - NGC 6402 - Ophiucus - Aglomerado Estelar Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h36m Declinação -03<sup>o</sup>.14<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 7,8 Tipo AG<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #274e13; font-family: Arial, sans-serif;"><span style="font-size: 15px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_14#mediaviewer/File:M14HunterWilson.jpg</span></span></div>
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<span style="background-color: white;"><span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">M14HunterWilson</span></span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a href="http://commons.wikimedia.org/wiki/User:Hewholooks" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="User:Hewholooks">Hewholooks</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Obra do próprio</span></span></span></div>
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<b>Messier 14</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC 6402</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ofiúco</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764.</div>
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A uma distância de cerca de 30 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, o aglomerado contém várias centenas de milhares de estrelas. Com uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de 7,6, o aglomerado pode ser facilmente observável de <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a>. <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">Telescópios</a> amadores podem revelar algumas das estrelas mais brilhantes do aglomerado, de magnitude aparente 14. A cerca de 3° a sudoeste do aglomerado situa-se na abóbada celeste outro aglomerado globular mais pálido, <a href="http://pt.wikipedia.org/wiki/NGC_6366" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 6366">NGC 6366</a>.</div>
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A <a href="http://pt.wikipedia.org/wiki/Luminosidade" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Luminosidade">luminosidade</a> total do aglomerado corresponde a 400 000 vezes a do <a href="http://pt.wikipedia.org/wiki/Sol" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Sol">Sol</a>, que corresponde a uma <a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a> de -9,12. A forma do aglomerado apresenta-se como uma <a href="http://pt.wikipedia.org/wiki/Elipsoide" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Elipsoide">elipsoide</a>, e mede cerca de 100 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em seu <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Semi-eixo_maior" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Semi-eixo maior">semi-eixo maior</a>.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 14</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M14HunterWilson.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 14 por um telescópio amador"><img alt="Messier 14 por um telescópio amador" data-file-height="850" data-file-width="1032" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/30/M14HunterWilson.jpg/250px-M14HunterWilson.jpg" height="206" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/30/M14HunterWilson.jpg/375px-M14HunterWilson.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/30/M14HunterWilson.jpg/500px-M14HunterWilson.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 14 por um telescópio amador</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;">VIII</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 37<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 36,15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_14#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-03° 14′ 45,3″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_14#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">30 300 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (9,3 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">8,32<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_14#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">11',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">50 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6402</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 14"><img alt="Messier 14" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="line-height: 22.3999996185303px;">http://www.ipac.caltech.edu/2mass/gallery/m19atlas.jpg</span><br />
<span style="line-height: 22.3999996185303px;"><a href="https://www.blogger.com/null" name="m81" style="background-color: white; line-height: normal;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></span></div>
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Messier 19</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M19 (NGC 6273)</i>, class VIII, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">17 : 02.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-26 : 16 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">28.0 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">17.0 (arc min)</td></tr>
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Discovered by Charles Messier in 1764.</div>
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Messier 19 (M19, NGC 6273) is the most oblate known globular cluster, being about ellipticity E3-E4. Shapley found it at ellipticity 6, corresponding E4, elongated at position angle 15 deg. He estimated that there could be counted twice as many stars along the major axis as along the minor. This deformation of the cluster from the globular shape may have to do with its proximity to the Galactic Center: While about 28,000 light years away from our Solar System, it is quite near to the Galactic Center, only about 5,200 light years away. It is located nine degrees above the galactic plane (i.e., at a galactic latitude of 9 deg North) and slightly west og the Galactic Center, as seen from Earth; it is perhaps very slightly more remote from us than the center of the <a href="http://messier.obspm.fr/more/mw.html">Milky Way</a>. M19 is receding from us at 146 km/sec.</div>
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LEIA MAIS</div>
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http://messier.obspm.fr/m/m019.html</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjRlXSty3IcDekIuaLWdevEDarezuo6-p8m2KZCofAmMoNkTw5RE7Uw78laxSNYY22M0sKoy3O90wSDcoH6pdHOmv5Sc4bDPTCDNEwBPNQaoqnSUNtY6a8sWiUYl9Rbzo68OAFzCUvbiQQ/s1600/m19+e+m62.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjRlXSty3IcDekIuaLWdevEDarezuo6-p8m2KZCofAmMoNkTw5RE7Uw78laxSNYY22M0sKoy3O90wSDcoH6pdHOmv5Sc4bDPTCDNEwBPNQaoqnSUNtY6a8sWiUYl9Rbzo68OAFzCUvbiQQ/s1600/m19+e+m62.png" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 6273 - M 19 - Aglomerado Globular Ophiucus</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h01m Declinação -26<sup>o</sup>.14<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 8,3 Diâmetro aparente 5’,3 Tipo Espectral F2<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância kpc 6,9 Velocidade Radial (km/s) + 102</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 17h10m Declinação -26<sup>o</sup>.14<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude visual integral 6,9 Tipo AG<o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img alt="Ficheiro:M19HunterWilson.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/38/M19HunterWilson.jpg/600px-M19HunterWilson.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 156.140625px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://commons.wikimedia.org/wiki/User:Hewholooks" style="background-image: none; text-decoration: none;" title="User:Hewholooks">Hewholooks</a></span><br />
<h1 class="firstHeading" id="firstHeading" lang="pt" style="background-image: none; border-bottom-color: rgb(170, 170, 170); border-bottom-style: solid; border-bottom-width: 1px; font-weight: normal; line-height: 1.2em; margin: 0px 0px 0.1em; overflow: hidden; padding-bottom: 0px; padding-top: 0px; position: relative;">
<span dir="auto"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">M19HunterWilson.</span></span></h1>
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<a href="http://pt.wikipedia.org/wiki/Messier_19" style="text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_19</span></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Messier 19</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; text-decoration: none;" title="New General Catalogue">NGC 6273</a>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> de <a href="http://pt.wikipedia.org/wiki/Estrela" style="background-image: none; text-decoration: none;" title="Estrela">estrelas</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-image: none; text-decoration: none;" title="Ophiuchus">Ofiúco</a>. Foi descoberto pelo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 1764, que o adicionou ao seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo de objetos</a> de aparência semelhante a <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-image: none; text-decoration: none;" title="Cometa">cometas</a>.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Messier 19 é o mais oblato dos aglomerados globulares conhecidos. Está a uma distância de cerca de 28 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-image: none; text-decoration: none;" title="Sistema Solar">Sistema Solar</a>, e está bastante próximo ao Centro Galáctico, com apenas cerca de 5.200 anos-luz de distância.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">É um dos aglomerados globulares mais <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Esferoide_oblato" style="background-image: none; text-decoration: none;" title="Esferoide oblato">oblatos</a> (achatados) conhecidos. Essa deformidade pode estar relacionado à proximidade do aglomerado ao <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea#N.C3.BAcleo" style="background-image: none; text-decoration: none;" title="Via-Láctea">centro galáctico</a>: embora esteja a cerca de 28 000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a>da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a>, está apenas a 5 200 do núcleo da Via-Láctea, ou cerca de 9° acima do núcleo galáctico na<a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; text-decoration: none;" title="Esfera celeste">esfera celeste</a>. Afasta-se radialmente do <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-image: none; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> a uma velocidade aproximada de 146 km/s.<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_19#cite_note-seds-2" style="background-image: none; text-decoration: none;">2</a></span></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 19</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_19_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 11 pelo Telescópio Espacial Hubble"><img alt="Messier 11 pelo Telescópio Espacial Hubble" data-file-height="1480" data-file-width="1480" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/46/Messier_19_Hubble_WikiSky.jpg/250px-Messier_19_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/46/Messier_19_Hubble_WikiSky.jpg/375px-Messier_19_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/46/Messier_19_Hubble_WikiSky.jpg/500px-Messier_19_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 11 pelo Telescópio Espacial Hubble</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1764" style="background: none; color: #0b0080; text-decoration: none;" title="1764">1764</a></td></tr>
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<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;">VII</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 02<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 37,69<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_19#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-26° 16′ 04,6″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_19#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">28 000 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (8,6 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">7,47<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_19#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">17',0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">70 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080;" title="Anos-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6273</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 19"><img alt="Messier 19" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="https://www.blogger.com/null" name="m81"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 62</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M62 (NGC 6266)</i>, class IV, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m62.jpg"><img align="right" alt="[m62.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m62.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">17 : 01.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-30 : 07 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">22.5 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">15.0 (arc min)</td></tr>
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Discovered 1771 by Charles Messier.</div>
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Messier 62 (M62, NGC 6266) is one of the most irregularly shaped globular clusters, as was first reported by Herschel. This deformation may be a result of the fact that M62 is one of the closest of Messier's globulars to the Galactic center (only about 6100 light years), so that it is deformed by tidal forces. Its central condensation is obviously displaced from the center, to the lower right in our image (SE).</div>
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From its apparent size and magnitude, M62 is very similar to its neighbor, <a href="http://messier.obspm.fr/m/m019.html">M19</a>. Physically, they are a bit less similar because their distances are somewhat different different: M62 is at 22,500, M19 at 28,400 light years, according to <a href="http://www.physics.mcmaster.ca/~harris/Databases.html">W.E. Harris' database</a>. M62 appears at a diameter of 15 arc minutes, about half of the Full Moon, corresponding to a linear extennsion of about 100 light-years.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m062.html</div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M62</b><o:p></o:p></span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhMFTH6c9h08j55j86ILSKsJQA2z86BwI2RT_xOHbAb8XhQv2lWLWIbZUx5egh8ngbn5BZtvt1vcy9O9xSOKVJ6iPUibnRUUt_bcj3IjHJxZbRhGrAHm0QqHOMm5gk5zKs_xB_gTOyhVFbm/s1600/M62_3.6_5.8_8.0_microns_spitzer.png" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhMFTH6c9h08j55j86ILSKsJQA2z86BwI2RT_xOHbAb8XhQv2lWLWIbZUx5egh8ngbn5BZtvt1vcy9O9xSOKVJ6iPUibnRUUt_bcj3IjHJxZbRhGrAHm0QqHOMm5gk5zKs_xB_gTOyhVFbm/s640/M62_3.6_5.8_8.0_microns_spitzer.png" height="625" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
<tr><td class="tr-caption" style="font-size: 13px;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><span style="line-height: 19.1875px; text-align: start;">Image of the M62 star cluster in infrared at 3.6 (blue), 4.5 (green) and 8.0 µm. The image has been made by myself (Médéric Boquien) from the public image archive of the Spitzer Space Telescope (courtesy NASA/JPL-Caltech).</span></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi descoberto pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; text-decoration: none;" title="Charles Messier">Charles Messier</a> em 7 de junho de 1771, embora ele tenha tomado sua posição na <a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; text-decoration: none;" title="Esfera celeste">esfera celeste</a> apenas em 4 de junho de 1779, quando listou em seu <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo</a>. <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-image: none; text-decoration: none;" title="Urano (planeta)">Urano</a>, foi o primeiro a resolver suas estrelas mais brilhantes.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">É um dos <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-image: none; text-decoration: none;" title="Aglomerado globular">aglomerados globulares</a> mais irregulares que se conhece. Sua deformação, relatada primeiramente por Herschel, é o resultado das <a href="http://pt.wikipedia.org/wiki/For%C3%A7a_de_mar%C3%A9" style="background-image: none; text-decoration: none;" title="Força de maré">forças de maré</a> do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Via-L%C3%A1ctea#N.C3.BAcleo" style="background-image: none; text-decoration: none;" title="Via-Láctea">núcleo da Via-Láctea</a>; o aglomerado está apenas 6 100 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; text-decoration: none;" title="Anos-luz">anos-luz</a> do centro galáctico, um dos aglomerados globulares do <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; text-decoration: none;" title="Catálogo Messier">catálogo Messier</a>mais próximos da região central da Via-Láctea.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Está a uma distância de 22 500 anos-luz em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; text-decoration: none;" title="Terra">Terra</a>, e seu diâmetro aparente de 15 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-image: none; text-decoration: none;" title="Minuto de arco">minutos de grau</a>, metade do diâmetro aparente da <a href="http://pt.wikipedia.org/wiki/Fases_da_Lua" style="background-image: none; text-decoration: none;" title="Fases da Lua">Lua Cheia</a>, corresponde a um diâmetro real de 100 anos-luz.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">Contém 89 <a href="http://pt.wikipedia.org/wiki/Estrela_vari%C3%A1vel" style="background-image: none; text-decoration: none;" title="Estrela variável">estrelas variáveis</a> conhecidas, a maior parte variáveis <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/RR_Lyrae" style="background-image: none; text-decoration: none;" title="RR Lyrae">RR Lyrae</a>. Seu núcleo é extremamente denso;possívelmente o núcleo sofreu no passado um colapso de núcleo, de modo semelhante ao encontrado nos aglomerados <a href="http://pt.wikipedia.org/wiki/Messier_15" style="background-image: none; text-decoration: none;" title="Messier 15">Messier 15</a>, <a href="http://pt.wikipedia.org/wiki/Messier_30" style="background-image: none; text-decoration: none;" title="Messier 30">Messier 30</a> e <a href="http://pt.wikipedia.org/wiki/Messier_70" style="background-image: none; text-decoration: none;" title="Messier 70">Messier 70</a>. Contém vários <a href="http://pt.wikipedia.org/wiki/Bin%C3%A1rio_de_raio_X" style="background-image: none; text-decoration: none;" title="Binário de raio X">binários de raios X</a>, consequência da alta <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Densidade_estelar&action=edit&redlink=1" style="background-image: none; text-decoration: none;" title="Densidade estelar (página não existe)">densidade estelar</a> de seu núcleo; tais binários de raios-X são consequência de quase-colisões entre estrelas</span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_62_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 62 pelo Telescópio Espacial Hubble.NASA/STScI/WikiSky"><img alt="Messier 62 pelo Telescópio Espacial Hubble.NASA/STScI/WikiSky" data-file-height="2000" data-file-width="2000" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Messier_62_Hubble_WikiSky.jpg/250px-Messier_62_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Messier_62_Hubble_WikiSky.jpg/375px-Messier_62_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Messier_62_Hubble_WikiSky.jpg/500px-Messier_62_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 62 pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a>.<br />
<a href="http://pt.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=STScI&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="STScI (página não existe)">STScI</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=WikiSky&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="WikiSky (página não existe)">WikiSky</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1771" style="background: none; color: #0b0080; text-decoration: none;" title="1771">1771</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 01<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 12,6<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-30° 06′ 44,5″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">22 500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (6 900 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">7,39<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">15 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">Classe</a></td><td style="background-color: #f8f8f8;">IV<span class="reference" id="cite_ref-seds_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">50<span class="reference" id="cite_ref-seds_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M62, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6266, GCl 51.<span class="reference" id="cite_ref-simbad_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_62#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." This is the stated policy of 2MASS.</a><br />
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Messier 107</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M107 (NGC 6171)</i>, class X, in <a href="http://messier.obspm.fr/map/Oph.html">Ophiuchus</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">16 : 32.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-13 : 03 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">20.9 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">13.0 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1782.</div>
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Messier 107 (M107, NGC 6171) is another <a href="http://messier.obspm.fr/addition.html">additional object</a> found by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> in April, 1782. Herewith, it is probably the <a href="http://messier.obspm.fr/xtra/history/m-cat.html#m107">Messier object</a> which was the latest to be <a href="http://messier.obspm.fr/xtra/history/dis-tab.html">discovered</a>. Eventually, <a href="http://messier.obspm.fr/xtra/Bios/hogg.html">Helen Sawyer Hogg</a> added it to the Messier Catalog in 1947, together with <a href="http://messier.obspm.fr/m/m105.html">M105</a> and <a href="http://messier.obspm.fr/m/m106.html">M106</a>, although it appears probable that already Méchain had intended to add it to a future edition of <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>'s list. <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a>, who had independently discovered it on May 12, 1793,<a href="http://messier.obspm.fr/xtra/similar/herschel.html">cataloged</a> this object as H VI.40; Herschel was the first observer to resolve this globular cluster into stars.</div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiEF5SmvAMVLqUQT68JzgfOO4CThJDuoODjXnIlfpH2Bxg7WsrMcayblsMyj-Mn_FN8LVUJ8vNNHSvWIY3dxG9bGczUsNGdT_763urQJe4IruvdtwNyzqEE1Jzhg3iT28D6IhV2qdkYPYs/s1600/m9+e+m107.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiEF5SmvAMVLqUQT68JzgfOO4CThJDuoODjXnIlfpH2Bxg7WsrMcayblsMyj-Mn_FN8LVUJ8vNNHSvWIY3dxG9bGczUsNGdT_763urQJe4IruvdtwNyzqEE1Jzhg3iT28D6IhV2qdkYPYs/s1600/m9+e+m107.png" /></a></div>
<span style="font-family: Arial, Helvetica, sans-serif;">Excerto da Carta Celeste Ophiucus - Mario Jaci Monteiro</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 1.4;"><b>M107</b><o:p></o:p></span><br />
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<b>Messier 107</b> (também conhecido como <b>M107</b> ou <b>NGC 6171</b>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> pouco denso localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> <a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a>. Situa-se perto do <a href="http://pt.wikipedia.org/wiki/Plano_gal%C3%A1ctico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Plano galáctico">plano galáctico</a>em uma distância de 20.000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>.<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span></div>
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Foi descoberto em abril de <a href="http://pt.wikipedia.org/wiki/1782" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1782">1782</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a> e é provavelmente o último objeto Messier a ser descoberto. <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a> o descobriu, de forma independente, em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/12_de_Maio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="12 de Maio">12 de Maio</a> de <a href="http://pt.wikipedia.org/wiki/1793" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1793">1793</a> e finalmente, em <a href="http://pt.wikipedia.org/wiki/1947" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1947">1947</a>, <a href="http://pt.wikipedia.org/wiki/Helen_Sawyer_Hogg" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Helen Sawyer Hogg">Helen Sawyer Hogg</a> adiciona Messier 107, juntamente com <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M105" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M105">M105</a> e <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M106" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="M106">M106</a> ao <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo Messier</a>.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-4" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span><br />
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 107</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_107_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular Messier 107"><img alt="Aglomerado globular Messier 107" data-file-height="4200" data-file-width="4200" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/42/Messier_107_Hubble_WikiSky.jpg/250px-Messier_107_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/42/Messier_107_Hubble_WikiSky.jpg/375px-Messier_107_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/42/Messier_107_Hubble_WikiSky.jpg/500px-Messier_107_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
<a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">Aglomerado globular</a> Messier 107</td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1782" style="background: none; color: #0b0080; text-decoration: none;" title="1782">1782</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Ophiuchus" style="background: none; color: #0b0080; text-decoration: none;" title="Ophiuchus">Ophiuchus</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">16<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 32<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 31.91<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-13° 03′ 13.1″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">20.000 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> (6.4 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">+8.85<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">13′.0</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">39.5 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a><span class="reference" id="cite_ref-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/New_general_catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New general catalogue">NGC</a> 6171, GCl 44<span class="reference" id="cite_ref-simbad_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_107#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Ophiuchus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Ophiuchus constellation map.png" data-file-height="2559" data-file-width="2269" src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/250px-Ophiuchus_constellation_map.png" height="282" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/375px-Ophiuchus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bc/Ophiuchus_constellation_map.png/500px-Ophiuchus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjbtsoitfirVsAWE6VivyhqyIPoSXuv5oSxJ1WfLqvAR-LcWHEOCZlAWNZV1jIxlZlEuK3p1gChNzhjV4HuXm08gweAqgq49_H0WjEKYyOpZSEpmLZkWDsGNkP8vnvGAy5HntFN_1zW8F4g/s1600/600px-Messier_107_Hubble_WikiSky.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjbtsoitfirVsAWE6VivyhqyIPoSXuv5oSxJ1WfLqvAR-LcWHEOCZlAWNZV1jIxlZlEuK3p1gChNzhjV4HuXm08gweAqgq49_H0WjEKYyOpZSEpmLZkWDsGNkP8vnvGAy5HntFN_1zW8F4g/s1600/600px-Messier_107_Hubble_WikiSky.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></td></tr>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 1.4;"><a href="http://pt.wikipedia.org/wiki/Messier_107" style="text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_107</a></span><span style="background-color: white; font-family: candara, trebuchet, arial, sans-serif; text-align: start;"><br />...................</span></div>
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<span style="background-color: white; font-family: candara, trebuchet, arial, sans-serif; text-align: start;">Messier 107 foi descoberto por Pierre Méchain em Abril de 1782 e foi acrescentado à lista dos sete Objectos de Messier Adicionais que não tinham sido originariamente incluídos na versão final do catálogo, publicada no ano anterior. Em 12 de Maio de 1783, este objecto foi re-descoberto independentemente por William Herschel, que conseguiu, pela primeira vez, resolver o enxame globular em estrelas individuais. Mas foi apenas em 1947 que tomou o seu lugar no catálogo de Messier como M107, o que o tornou no mais recente enxame estelar a ser acrescentado a esta famosa lista.</span></div>
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<span style="background-color: white; text-align: start;"><span style="font-family: candara, trebuchet, arial, sans-serif;">http://www.cienciahoje.pt/index.php?oid=46379&op=all</span></span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiw1a0F9uY66ir6ARMXkabpfmD3FJelfgfZYSPZ1Xk2in9L5011l2_Wb0DJnxvOBy8lsPza9yxrWbvoDiDCCoIPxh1IKR0zCjDfJe5GtCQfjYQ6BeLIozmt9AsiQusD5jhmm-dnl2uZ2aR9/s1600/eso1048a+m107.jpg" imageanchor="1" style="margin-left: auto; margin-right: auto; text-decoration: none;"><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiw1a0F9uY66ir6ARMXkabpfmD3FJelfgfZYSPZ1Xk2in9L5011l2_Wb0DJnxvOBy8lsPza9yxrWbvoDiDCCoIPxh1IKR0zCjDfJe5GtCQfjYQ6BeLIozmt9AsiQusD5jhmm-dnl2uZ2aR9/s640/eso1048a+m107.jpg" height="584" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(127, 96, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
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<span lang="EN-US" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">The globular cluster Messier 107, also known as NGC 6171, is located about 21 000 light-years away in the constellation of Ophiuchus. Messier 107 is about 13 arcminutes across, which corresponds to about 80 light-years at its distance. As is typical of globular clusters, a population of thousands of old stars in Messier 107 is densely concentrated into a volume that is only about twenty times the distance between our Sun and its nearest stellar neighbour, Alpha Centauri, across. This image was created from exposures taken through blue, green and near-infrared filters, using the Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at La Silla Observatory, Chile.<o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><strong><span lang="EN-US">Credit:</span></strong><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;">ESO/ESO Imaging Survey</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Saiba mais</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Sobre a Constelação Ophiucus,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>O Serpentário</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acessando meus Trabalhos em</span></div>
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<span style="line-height: 22.3999996185303px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://sobreophiucuseserpens.blogspot.com.br/</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><div class="MsoNormal" style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
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<a href="http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg" style="text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">http://www.aai.ee/muuseum/Uranomeetria/Pictures/Web/Reissig_W_011.jpg</span></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-75037683931814404192014-09-06T08:34:00.003-07:002015-01-04T08:10:34.769-08:00Monoceros<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nesta Postagem, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">estaremos comentando sobre o único Objeto Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontrado na constelação Monoceros, o Unicórnio:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M50.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Estivemos comentando sobre os Objetos Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontrados em constelações bem próximas ao Monoceros</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Orion</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m42-m43-e-m78-os-objetos-messier-na.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Canis Majoris</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m41-o-unico-objeto-messier-na.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Puppis </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/10/m46-m47-m93-os-objetos-messier-em.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Gemi</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m35-o-unico-objeto-messier-na.html</span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ni</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ainda estaremos, em breve,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">trazendo ao Caro Leitor,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nossos comentários sobre os Objetos Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontrados em Lepus e em Hydra</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(constelações também vicinais ao Unicórnio).</span></div>
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<br />
<br />
<img src="http://www.raremaps.com/maps/medium/37703.jpg" /><br />
<span style="background-color: white;"><span style="color: #073763;">http://www.raremaps.com/gallery/detail/37703/The_January_February_and_March_Sky_Cancer_Perseus_Gemini_Taurus/Burritt.html</span></span><br />
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<span style="background-color: white;"><span style="color: #073763;"><strong>Title: </strong>[The January, February & March Sky -- Cancer, Perseus, Gemini, Taurus, Orion, Monceros, Canis Major, Lepus, Argo Navis, Hydra, Perseus, Lynx, etc.]</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/808" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">Elijah J. Burritt</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Monoceros apresenta-se de maneira a ser bem divisado</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pois que se insere entre as constelações Canis Majoris e Canis Minoris</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Cão Maior e Cão Menor -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, certamente, as duas estrelas-alpha dessas constelações</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Sírius e Procyum, respectivamente -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">atuam enquanto boas guias para bem encontrarmos o Unicórnio.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Aliás, o Objeto Messier 50</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pode ser encontrado bem próximo à maravilhosa Sirius.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEifzN_JHDvVqwcgsBWr1Rixmq-jwxUvimGzaxbZhT88IPCmXmbkxKJ71WZ_ahmgnLLN1yNg_AZgjKizQYDvRUWhdfRKaWTUtep-jToCUqyFHBYjyvvRNnL2pFda0gwqb8-TsakHm6ZJ1Gc/s1600/M50+aproximado+e+com+ilustra%C3%A7%C3%A3o.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEifzN_JHDvVqwcgsBWr1Rixmq-jwxUvimGzaxbZhT88IPCmXmbkxKJ71WZ_ahmgnLLN1yNg_AZgjKizQYDvRUWhdfRKaWTUtep-jToCUqyFHBYjyvvRNnL2pFda0gwqb8-TsakHm6ZJ1Gc/s1600/M50+aproximado+e+com+ilustra%C3%A7%C3%A3o.png" /></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Monoceros é uma constelação que vem sendo bem comentada</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em função de acolher </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a maravilhosa Nebulosa Roseta</span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #274e13;">NGC 2237 + 2244 - A Nebulosa Rosette<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #274e13;">NGC 2237 é uma nebulosa difusa circundando o aglomerado aberto NGC 2244. A Nebulosa Rosette é difícil de ser observada visualmente mas a parte central do aglomerado pode ser resolvida facilmente através binóculos. O aglomerado é fisicamente conectado à nebulosa: é possível que duas estrelas muito quentes que fazem parte deste aglomerado tenham ‘varrido’ a região central da nebulosa e a deixado sem gás - o que poderia ser a razão da aparência da Nebulosa Rosette, como se fosse um anel.</span></span><br />
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<span style="background-color: white; color: #274e13;"><span style="font-family: Arial, sans-serif;"> 6<sup>a</sup>. Edição do Atlas Celeste</span><span style="font-family: "Arial","sans-serif";"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13;"><span style="font-family: Arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span><span style="font-family: "Arial","sans-serif";"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/8/86/Rosette_nebula_s.jpg/800px-Rosette_nebula_s.jpg" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Nebulosa_Roseta#mediaviewer/File:Rosette_nebula_s.jpg</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Rosette nebula s</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author" style="background-color: white;"><a class="extiw" href="http://en.wikipedia.org/wiki/Special:Contributions/Nwright6302" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Special:Contributions/Nwright6302">Nwright6302</a></span></span></div>
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<span style="background-color: white;">A Nebulosa Roseta (H-Alpha)</span></div>
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<span style="background-color: white;"><a class="extiw" href="http://en.wikipedia.org/wiki/Rosette_nebula" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Rosette nebula">Rosette nebula</a>. Original text: These images are released into the public domain for private use or for use in the promotion of the IPHAS survey. If any image or images are redisplayed or reproduced, please accompany the image or images with the following acknowledgement: "Image based on data obtained as part of <a class="extiw" href="http://en.wikipedia.org/wiki/The_INT_Photometric_H-Alpha_Survey" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:The INT Photometric H-Alpha Survey">the INT Photometric H-Alpha Survey</a> of the Northern Galactic Plane, prepared by Nick Wright, University College London, on behalf of the IPHAS Collaboration".</span></div>
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Mario Jaci Monteiro - As Constelações, Cartas Celestes</div>
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<span style="background-color: white; color: #660000;"><b><span lang="EN-US" style="font-family: Arial, sans-serif;"> </span><span style="font-family: Arial, sans-serif;">MONOCEROS, O UNICÓRNIO</span></b></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 5h54m / 8h8m Declinação -11<sup>o</sup>.0 / +11<sup>o</sup>.9<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">História:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Constelação adicionada por Bartschius, 1624.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Fronteiras:</span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Monoceros faz fronteira com Canis Minor, Gemini, Orion, Lepus, Canis Major, Puppis e Hydra<o:p></o:p></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><br /></span></span><span style="background-color: white;"><span style="color: #073763;"><a href="https://www.blogger.com/goog_1846066287"><br /></a></span></span><br />
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<span style="background-color: white; color: #274e13;"><span style="font-family: Arial, sans-serif;"> 6<sup>a</sup>. Edição do Atlas Celeste</span><span style="font-family: "Arial","sans-serif";"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13;"><span style="font-family: Arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span><span style="font-family: "Arial","sans-serif";"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #274e13; font-family: Arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span><br />
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<span style="background-color: white;"><img src="http://www.iau.org/static/public/constellations/gif/MON.gif" /></span><br />
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<span style="background-color: white;"><a href="https://www.blogger.com/goog_1846066287">http://www.iau.org/static/public/constellations/gif/MON.gif</a></span></div>
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<a href="http://www.ipac.caltech.edu/2mass/gallery/m50atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m50atlas.jpg</a><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 50</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M50 (NGC 2323)</i>, type 'e', in <a href="http://messier.obspm.fr/map/Mon.html">Monoceros</a></center>
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<a href="http://messier.obspm.fr/Jpg/m50.jpg"><img align="right" alt="[m50.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m50.jpg" /></a><br />
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<tr><th align="left">Right Ascension</th><td align="center">07 : 03.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-08 : 20 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">3.2 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">16.0 (arc min)</td></tr>
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Possibly discovered by G.D. Cassini before 1711. Discovered independently by Charles Messier in 1772.<br />
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Open cluster Messier 50 (M50, NGC 2323) is a pretty and considerably bright object located in a rich part of stars and nebulae in constellation Monoceros, near its border to Canis Major.<br />
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This cluster was <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M50">discovered</a> on April 5, 1772 by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, but possibly <a href="http://messier.obspm.fr/xtra/Bios/cassini.html">G.D. Cassini</a> had already discovered it before 1711, according to a report by his son, <a href="http://messier.obspm.fr/xtra/Bios/cassini2.html">Jacques Cassini</a>, in his book of 1740, Elements of Astronomy.<br />
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LEIA MAIS<br />
em<br />
http://messier.obspm.fr/m/m050.html<br />
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<b><span style="color: #660000;">Messier 50</span></b><span style="color: #252525;"> é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado estelar aberto</a><span style="color: #252525;"> localizado a 3 200 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="color: #252525;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/Monoceros" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Monoceros">Monoceros</a><span style="color: #252525;">. Possivelmente foi descoberto por </span><a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Cassini" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Cassini">Giovanni Domenico Cassini</a><span style="color: #252525;">antes de </span><a href="http://pt.wikipedia.org/wiki/1711" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1711">1711</a><span style="color: #252525;">. Em </span><a href="http://pt.wikipedia.org/wiki/5_de_abril" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="5 de abril">5 de abril</a><span style="color: #252525;"> de </span><a href="http://pt.wikipedia.org/wiki/1772" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1772">1772</a><span style="color: #252525;"> </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525;"> o descobriu independentemente.</span></div>
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Messier 50 tem um raio de 10 anos-luz e uma idade estimada em 78 milhões de anos. Possui cerca de 200 estrelas, sendo que a mais brilhante é de <a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_estelar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação estelar">classe</a> B e tem uma<a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude</a> de 9,0 ou 7,85.</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 50</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_object_50.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 50, projeto 2MASS"><img alt="Messier 50, projeto 2MASS" data-file-height="1500" data-file-width="1300" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/3f/Messier_object_50.jpg/250px-Messier_object_50.jpg" height="288" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/3f/Messier_object_50.jpg/375px-Messier_object_50.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/3f/Messier_object_50.jpg/500px-Messier_object_50.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 50, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Cassini" style="background: none; color: #0b0080; text-decoration: none;" title="Giovanni Domenico Cassini">Giovanni Domenico Cassini</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1711" style="background: none; color: #0b0080; text-decoration: none;" title="1711">1711</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Monoceros" style="background: none; color: #0b0080; text-decoration: none;" title="Monoceros">Monoceros</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">07<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 03,2<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-08° 20′</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">3200 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (1000 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">5,9</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">16,0 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">10</td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">78 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td>Nº estrelas</td><td style="background-color: #f8f8f8;">200</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 2323</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 50"><img alt="Messier 50" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Monoceros_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Monoceros constellation map.png" data-file-height="1989" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a2/Monoceros_constellation_map.png/250px-Monoceros_constellation_map.png" height="194" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a2/Monoceros_constellation_map.png/375px-Monoceros_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a2/Monoceros_constellation_map.png/500px-Monoceros_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;">http://pt.wikipedia.org/wiki/Messier_50</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><br /><div class="MsoNormal" style="font-size: 16px; line-height: 22.3999996185303px;">
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal; text-align: start;">
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">COM UM ABRAÇO ESTRELADO,</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Janine Milward</span></span><br />
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-26089026635650058082014-09-06T08:33:00.003-07:002015-01-04T08:08:39.274-08:00Lyra<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Olá!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Devo confessar que sou imensamente apaixonada</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">pela constelação da Lira!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Eu admiro profundamente sua delicadeza,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">seu desenho suave tecido por estrelas suaves</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e a presença inequívoca da belíssima Vega, estrela-alpha Lyrae!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Não podemos nos esquecer que Vega é uma das três estrelas</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">que perfazem o chamado Grande Triângulo do Verão</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(ou do Norte, para nós, do hemisfério sul, </span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">pois que acontece nos tempos do nosso Inverno!).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">juntamente com Altair, estrela-alpha Aquilae, e Deneb, estrela-alpha Cygnus.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Estaremos, em outros Trabalhos, comentando sobre</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">os Objetos Messier acolhidos pela constelação Cygnus</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- veja em </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m29-e-m39-os-objetos-messier-em-cygnus.html -,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">porém não encontramos nenhum desses Objetos em Aquila</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- mas, ao invés da Águia, estaremos comentando também</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">sobre o Objeto Messier encontrado em Vulpecula, a Raposa,</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- veja em </span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://oceudomes.blogspot.com.br/2014/09/m27-o-unico-objeto-messier-em-vulpecula.html -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(constelação que se encontra entre Cygnus e Aquila!),</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e esse Objeto é a famosa Dumbbell Nebula, M27.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">A Lyra é cantada, em prosa e em verso e em imagens e em ilustrações,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ora como uma lira, ora como um violino;</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">ora como um abutre, Vultur Cadens; ora como um tear!</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Sempre que escutamos o nome Lyra,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">nossa mente nos leva diretamente para a belíssima Nebulosa do Anel,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">não é verdade?</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Estaremos neste Trabalho, Caro Leitor,</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">comentando um tantinho sobre</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">os Objetos Messier acolhidos por Lyra:</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">M56 e M57.</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/detail/31398op/_Lyra_Stars_Heightened_in_Gold/Bayer.html</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: normal; text-align: start;">Map Maker:</span><strong style="line-height: normal; text-align: start;"> </strong><span style="line-height: normal; text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/247" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; line-height: normal; text-align: start; text-decoration: none;">Johann Bayer</a></span></div>
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<b>Ah, A Lira!</b><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">A Lira é uma constelação sempre maravilhosa e nos trazendo seu encantamento, seja através a observação a olho nú, ou através binóculos e telescópios.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A Lira, enquanto um instrumento musical, pode sempre estar nos apresentando apenas um dos instrumentos de sua grande orquestra....; ou pode sempre estar nos apresentando alguns ou mesmo (quase) todos os instrumentos/objetos celestiais de sua grande orquestra..;. e ainda o maestro apontando seu super telescópio para poder amealhar outros demais instrumentos/objetos celestes que aguardam serem revelados ao público sempre disposto a aplaudir a doce musicalidade advinda dessa belíssima constelação dos céus estrelados do norte! </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O simples e singular instrumento musical da Lira acontece quando a observamos a olho nú e nos deixamos encantar pela delicada música realizada através de suas cordas tremulantes sendo dedilhadas pelo mito de Orpheu. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns ou mesmo (quase) todos os instrumentos/objetos celestiais de sua grande orquestra acontece quando a observamos através simpáticos telescópios, de menor ou de maior potência. Surgem objetos celestes admiráveis, fundamentalmente entra em cena a belíssima e sempre tão buscada e observada Nebulosa do Anel!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O maestro regendo a grande orquestra e ainda revelando mais e mais instrumentos/objetos celestiais que aguardam por seus momentos de entrada..., acontece quando os super telescópios e a tecnologia cada vez mais avançada das várias formas de fotografia são direcionados para esta constelação! Aglomerados e Galáxias entram em cena e tomam seus lugares.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Eu diria que, nesta orquestra dos céus, o lugar do solista é ocupado pela estonteante Nebulosa do Anel que vai sendo revelada mais e mais em seus profundos segredos que repousam em seu interior aparentemente vazio e que vai se enchendo de estrelas, pouco a pouco - quanto mais avançadamente a astronomia caminha, mais profundamente investiga e traz à luz objetos celestiais ainda nem sonhados em nossa vã filosofia...! Talvez possamos pensar que o maestro seja representado pela segunda mais brilhante estrela dos céus do norte e a quinta mais brilhante estrela de todos os céus: Vega.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Você e eu, Amantes das Estrelas, somos o público e nos posicionamos ansiosamente diante do belíssimo espetáculo apresentado no palco dos céus estrelados!</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Excerto de meu Trabalho</div>
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acessado em</div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://sobrelyra.blogspot.com/2011/10/observacao-olho-nu-ou-atraves-binoculos.html" style="color: #274e13; text-decoration: none;">http://sobrelyra.blogspot.com/2011/10/observacao-olho-nu-ou-atraves-binoculos.html</a></span></span></div>
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<strong>Object Names:</strong> Ring Nebula, M57</div>
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<strong>Image Type:</strong> Astronomical</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> The <a href="http://heritage.stsci.edu/" style="color: #993333;">Hubble Heritage</a> Team (<a href="http://www.aura-astronomy.org/" style="color: #993333;">AURA</a>/<a href="http://www.stsci.edu/" style="color: #993333;">STScI</a>/<a href="http://www.nasa.gov/" style="color: #993333;">NASA</a>)</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/1999/01/image/a/format/web_print/</span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Carta Celeste realizada por Mario Jaci Monteiro</span></span></div>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(invertido do branco original do papel por Janine)</span></span></div>
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<span style="font-family: Arial, sans-serif;"><b><span style="color: #660000;">LYRA, A LIRA</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Posicionamento:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Ascensão Reta 18h12m / 19h26m Declinação +25<sup>o</sup>.6 / +47<sup>o</sup>.7<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Mito:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Mercúrio encontrou o casco de uma tartaruga no Rio Nilo e descobriu que, depois que a carne havia sido consumida, poderia tocar as entranhas do animal e produzir música. Ele fez uma lira com três cordas e ofertou a Orfeu, o filho de Caliope, que encantava feras, pedras e pássaros com sua música. Depois que Orfeu foi degolado pelas mulheres da Trácia, Júpiter colocou a lira nos céus, a pedido de Apolo e das Musas. Esta constelação também foi chamada de Vultur Cadens, pelos antigos.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Algumas Informações Interessantes acerca esta Constelação:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">A Lira foi uma das primeiras constelações a serem descritas.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Fronteiras:<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="color: #073763;">Hercules Vulpecula, Cygnus, Draco</span><span style="color: #0f243e; font-size: 11pt;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<img src="http://www.iau.org/static/public/constellations/gif/LYR.gif" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.iau.org/static/public/constellations/gif/LYR.gif</span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M56 E M57,</b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA CONSTELAÇÃO DA LIRA:</b></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m56atlas.jpg" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m56atlas.jpg</span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 56</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M56 (NGC 6779)</i>, class X, in <a href="http://messier.obspm.fr/map/Lyr.html">Lyra</a></center>
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<a href="http://messier.obspm.fr/Jpg/m56.jpg"><img align="right" alt="[m56.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m56.jpg" /></a><br />
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<tr><th align="left">Right Ascension</th><td align="center">19 : 16.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+30 : 11 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">32.9 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">8.8 (arc min)</td></tr>
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Discovered by Charles Messier in 1779.<br />
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Messier 56 (M56, NGC 6779) is located about half-way between Beta Cygni (Albireo) and Gamma Lyrae. It is one of the less bright Messier globulars, especially lacking the bright core which most globulars have. Nevertheless it is not too difficult to resolve, even at its rather large distance. This led to its classification in concentration class X.<br />
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LEIA MAIS<br />
em<br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://messier.obspm.fr/m/m056.html</span><br />
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M56 - NGC 6779 - Aglomerado Globular</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 19h16m35.5s Declinação +30d11m04s</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">M56 possui a magnitude 8.3 e a dimensão de 7”, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">portanto bastante brilhante e grande, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">um tanto irregular, rica e bem condensada,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> podendo ser encontrada a 3.8<sup>o</sup>. NW de Albireo, a estrela Beta Cygni. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Porque a Via Láctea passa extremamente próxima a este objeto, </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">isso pode ser considerado tanto um problema quanto uma bênção: </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">o problema acontece pelo fato de não deixar que M56 se apresente</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> através seu devido valor de brilho e de dimensão;</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> a bênção acontece através o fato de M56 se situar</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> em um lugar de extrema riqueza dos céus estrelados.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/73/Messier_56_Hubble_WikiSky.jpg/800px-Messier_56_Hubble_WikiSky.jpg" /></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Messier_56#mediaviewer/File:Messier_56_Hubble_WikiSky.jpg</span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="background-color: white; font-size: 1.2em; max-width: 60%;">Messier 56 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="background-color: white;"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=19.2765815&de=30.1841766&angle=0.060215&projection=tan&rotation=-30.3162&survey=astrophoto&img_id=60454&width=4320&height=4320&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=zoom" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<b>Messier 56</b> (também conhecido como <b>NGC 6779</b> ou <b>M56</b>) é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> localizado na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Lyra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lyra">Lyra</a> a 32 900 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>. Foi descoberto por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> em <a href="http://pt.wikipedia.org/wiki/1779" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1779">1779</a>. Possui um raio de 42,5 anos-luz e uma dimensão aparente de 8,8 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a>.<span class="reference" id="cite_ref-seds_2-5" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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O <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi uma das descobertas originais do astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que o viu pela primeira vez em 23 de janeiro de 1779, descrevendo-o como uma "nebulosa sem estrelas". Suas estrelas mais brilhantes foram <a href="http://pt.wikipedia.org/wiki/Resolu%C3%A7%C3%A3o_de_imagem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Resolução de imagem">resolvidas</a> pela primeira vez por <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, em 1784.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 56</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_56_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 56 pelo Telescópio Espacial Hubble.NASA/STScI/WikiSky"><img alt="Messier 56 pelo Telescópio Espacial Hubble.NASA/STScI/WikiSky" data-file-height="4320" data-file-width="4320" src="http://upload.wikimedia.org/wikipedia/commons/thumb/7/73/Messier_56_Hubble_WikiSky.jpg/250px-Messier_56_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/73/Messier_56_Hubble_WikiSky.jpg/375px-Messier_56_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/73/Messier_56_Hubble_WikiSky.jpg/500px-Messier_56_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 56 pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a>.<br />
<a href="http://pt.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=STScI&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="STScI (página não existe)">STScI</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=WikiSky&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="WikiSky (página não existe)">WikiSky</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1779" style="background: none; color: #0b0080; text-decoration: none;" title="1779">1779</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Lyra" style="background: none; color: #0b0080; text-decoration: none;" title="Lyra">Lyra</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">19<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 16<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 35,6<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">30° 11′ 00,5″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">32 900 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (10 100 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">8,3<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">8,8 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-seds_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">Classe</a></td><td style="background-color: #f8f8f8;">X<span class="reference" id="cite_ref-seds_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">42,5<span class="reference" id="cite_ref-seds_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M56, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6779, GCl 110.<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_56#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 56"><img alt="Messier 56" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/14px-Locator_Dot2.gif" height="14" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="14" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Lyra_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Lyra constellation map.png" data-file-height="2409" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/29/Lyra_constellation_map.png/250px-Lyra_constellation_map.png" height="337" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/29/Lyra_constellation_map.png/375px-Lyra_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/29/Lyra_constellation_map.png/500px-Lyra_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><strong>Credit: </strong><a href="http://www.stsci.edu/~bond/" style="text-decoration: none;">H. Bond</a> et al., <a href="http://heritage.stsci.edu/commonpages/infoindex/ourproject/moreproject.html" style="text-decoration: none;">Hubble Heritage Team</a> (<a href="http://www.stsci.edu/" style="text-decoration: none;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="text-decoration: none;">AURA</a>), <a href="http://www.nasa.gov/" style="text-decoration: none;">NASA</a></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 57</h1>
<i><a href="http://messier.obspm.fr/nebula.html">Planetary Nebula</a> M57 (NGC 6720)</i>, type 4+3, in <a href="http://messier.obspm.fr/map/Lyr.html">Lyra</a></center>
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<br /><b><span style="font-size: large;">Ring Nebula</span></b><br /><b><br /></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m57.jpg"><img align="right" alt="[m57.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m57.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">18 : 53.6 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+33 : 02 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">2.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">8.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">1.4x1.0 (arc min)</td></tr>
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Discovered by Antoine Darquier de Pellepoix in 1779.</div>
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The famous ring nebula Messier 57 (M57, NGC 6720) is often regarded as the prototype of a planetary nebula, and a showpiece in the northern hemisphere summer sky.</div>
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Recent research has confirmed that it is, most probably, actually a ring (torus) of bright light-emitting material surrounding its central star, and not a spherical (or ellipsoidal) shell, thus coinciding with an early assumption by <a href="http://messier.obspm.fr/xtra/Bios/jherschel.html">John Herschel</a>. Viewed from this equatorial plane, it would thus more resemble the Dumbbell Nebula <a href="http://messier.obspm.fr/m/m027.html">M27</a> or the Little Dumbbell Nebula <a href="http://messier.obspm.fr/m/m076.html">M76</a> than its appearance we know from here: We happen to view it from near one pole.</div>
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M57 was the second planetary nebula to be discovered (in January 1779), 15 years after the first one, <a href="http://messier.obspm.fr/m/m027.html">M27</a>. <a href="http://messier.obspm.fr/xtra/Bios/darquier.html">Antoine Darquier de Pellepoix (Darquier)</a>, who discovered the Ring Nebula only a few days before <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> found and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M57">cataloged it</a>, described it as "a dull nebula, but perfectly outlined; as large as Jupiter and looks like a fading planet." This comparison to a planet may have influenced <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a>, who found the objects of this type resembling the planet newly discovered by him, Uranus, and introduced the name <i>"Planetary Nebulae"</i>. Herschel described M57 as "a perforated nebula, or ring of stars;" this was the first mention of the ring shape. Oddly, the inventor of the name "Planetary Nebula" did not count this most prominent representative in this object class, but described it as a "curiosity of the heavens", a peculiar object. Herschel also identified some of the superimposed stars, and correctly assumed that "none [of them] seems to belong to it."</div>
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M57 is very easy to locate as it is situated between Beta and Gamma Lyrae, at about one-third the distance from Beta to Gamma. It can be seen with binoculars as an almost stellar object, difficult to identify just because of its small apparent diameter. In smaller amateur telescopes, the ring becomes apparent at about 100 magnification, with a darker middle; a 12th-mag star is east of the planetary nebula, about 1' of the center. If ever color is notable, the Ring Nebula appears slightly greenish, not unexpected because most of its light is emitted in few green spectral lines. Even in small scopes, a slight ellipticity can be noted, with major axis in a position angle of about 60 deg. With increasing aperture and under good condition, more and more detail becomes visible, but even in large instruments, the central star will be apparent only under exceptionally good conditions, or with the help of filters. In large instruments, several very faint foreground or background stars can be glimpsed within the nebula's extension under very good conditions.</div>
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Of the neighboring stars, <a href="http://www.seds.org/~spider/spider/Vars/betaLyr.html">Beta Lyrae (Sheliak)</a> is a notable eclipsing binary, with components of spectral type B7 and A8, varying between mag 3.4 and 4.4 with a period of 12.91 days. Gamma Lyrae (Sulaphat, Arabic for "Tortoise") is a giant of spectral type B9 III and mag 3.2 with a mag 12 companion at 13.8" distance in position angle 300 deg. The 0.4' small and 14.4-mag faint galaxy IC 1296 is situated just 4' NW of M57 and can be found with large instruments.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m057.html</div>
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<b><span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;">M57 - NGC 5720 - A Nebulosa do Anel</span></b></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 18h53m35 Declinação +33<sup>o</sup>.01 m4</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Tipo Nebulosa Planetária NP Dimensão 1,2 Magnitude 18</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude da Estrela associada 15 Distância em anos-luz 5,0<b></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A um terço da distância entre as estrelas Beta e Gamma Lyrae, encontra-se a maravilhosa Nebulosa do Anel, NGC 6720, M57, descoberta em 1772 embora sua forma aparentemente anular tenha sido revelado mais tarde, por William Herschel em suas observações.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Sua magnitude é de 9 e sua dimensão é de 2.5”. <b></b></span></div>
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<span lang="PT" style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta é uma das mais familiares nebulosas planetárias. </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Telescópios mostram sua forma um tanto indefinida em suas extremidades, com uma abertura escura ao centro acolhendo pálidas estrelas bem como, através lentes potentes, uma estrela também pálida se revela. <span lang="PT">É uma estrela azul-anã, muito quente. A intensa radiação dessa estrela é absorvida pela nebulosa e re-emitida na região visível. </span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O espectro da nebulosa e da estrela central é puramente gasoso. Embora pareça oval para nossos olhos, é supostamente quase circular porém visto obliquamente. Esta nebulosa pode ser visualizada através telescópios pequenos.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Surgindo pela morte de estrela parecidas com o Sol, as nebulosas planetárias representam a breve porém gloriosa fase final da evolução estelar. Os envoltórios gasosos são ionizados por uma fonte central extremamente quente, o núcleo colapsado de uma estrela que esgotou todo o combustível por fusão nuclear.</span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 11pt;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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Mapping the Ring Nebula's Structure</h2>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2013/13/image/e/format/web_print/</span></span></div>
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This illustration depicts a sideways view of the Ring Nebula, as deduced by astronomers using new Hubble observations. The doughnut-shaped feature in the center of the graphic is the main ring. The lobes above and below the ring comprise a football-shaped structure that pierces the ring. Dense knots of gas are embedded along the ring's inner rim.</div>
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<strong>Object Names:</strong> Ring Nebula, M57, NGC 6720</div>
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<strong>Image Type:</strong> Illustration</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> <a href="http://www.nasa.gov/" style="color: #993333;">NASA</a>, <a href="http://www.spacetelescope.org/" style="color: #993333;">ESA</a>, and A. Feild (<a href="http://www.stsci.edu/" style="color: #993333;">STScI</a>)</div>
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<span style="font-family: arial, sans-serif; font-size: x-small;"><span style="line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2013/13/image/e/</span></span></div>
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<span style="color: #660000;">A <b>Nebulosa do Anel</b> (também conhecida por <b>M57</b> ou <b>NGC 6720</b>)</span><span style="color: #252525;">, fica a 2.300 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a>, na <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Lyra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lyra">Lira</a>. Está entre os mais notáveis exemplos de <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a>. Foi descoberta por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Antoine_Darquier_de_Pellepoix" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Antoine Darquier de Pellepoix">Antoine Darquier de Pellepoix</a> em <a href="http://pt.wikipedia.org/wiki/1779" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1779">1779</a>. Esse nome é porque seus gases parecem um anel ou as pétalas de uma rosa cósmica.</span></div>
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<span style="font-family: 'Linux Libertine', Georgia, Times, serif; line-height: 1.3;">..................................................</span></div>
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<span style="font-family: 'Linux Libertine', Georgia, Times, serif; line-height: 1.3;">Descoberta e visualização</span></div>
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<span style="line-height: 22.3999996185303px;"><br />Pode ser visto com</span><span style="line-height: 22.3999996185303px;"> </span><a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Binóculo">binóculos</a><span style="line-height: 22.3999996185303px;"> </span><span style="line-height: 22.3999996185303px;">como um objeto quase estelar, difícil de identificar como uma nebulosa planetária devido ao seu diâmetro aparente pequeno. Nos pequenos</span><span style="line-height: 22.3999996185303px;"> </span><a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Telescópio">telescópios</a><span style="line-height: 22.3999996185303px;"> </span><span style="line-height: 22.3999996185303px;">amadores, o anel se torna evidente a uma magnificação 100. Em instrumentos ópticos mais potentes, é possível identificar uma cor esverdeada; a maior parte de suas</span><span style="line-height: 22.3999996185303px;"> </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Linha_espectral" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Linha espectral">linhas espectrais</a><span style="line-height: 22.3999996185303px;"> </span><span style="line-height: 22.3999996185303px;">estão no</span><span style="line-height: 22.3999996185303px;"> </span><a href="http://pt.wikipedia.org/wiki/Comprimento_de_onda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Comprimento de onda">comprimento de onda</a><span style="line-height: 22.3999996185303px;"> </span><span style="line-height: 22.3999996185303px;">ao redor do verde devido à dupla ionização do</span><span style="line-height: 22.3999996185303px;"> </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Oxig%C3%AAnio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Oxigênio">oxigênio</a><span style="line-height: 22.3999996185303px;"> </span><span style="line-height: 22.3999996185303px;">presente nos gases que formam a nebulosa.</span><span class="reference" id="cite_ref-seds_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span>Messier 57 foi a segunda <a href="http://pt.wikipedia.org/wiki/Nebulosa_planet%C3%A1ria" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa planetária">nebulosa planetária</a> a ser descoberta na história, em 1779, 15 anos após a primeira, a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Haltere" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Nebulosa do Haltere">nebulosa do Haltere</a> (M27). <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Antoine_Darquier_de_Pellepoix" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Antoine Darquier de Pellepoix">Antoine Darquier de Pellepoix</a> descobriu a nebulosa pouco dias antes de <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> redescobrir o objeto independentemente, descrevendo-o como uma "nebulosa ordinária, mas perfeitamente definida, tão grande quanto <a href="http://pt.wikipedia.org/wiki/J%C3%BApiter_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Júpiter (planeta)">Júpiter</a> quanto ao diâmetro aparente e parece-se como um planeta tênue." Esta comparação a um planeta pode ter influenciado <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Herschel">William Herschel</a>, descobridor de <a href="http://pt.wikipedia.org/wiki/Urano_(planeta)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Urano (planeta)">Urano</a>, que associou esses objetos como o mais novo planeta descoberto por ele e introduziu a denominação "nebulosa planetária". Descreveu-a como uma "nebulosa perfurada", ou um "anel de estrelas", a primeira menção histórica de seu formato de um anel. Entretanto, o inventor do nome "nebulosa planetária" não classificou a nebulosa como tal, mas descerveu-a como "uma curiosidade dos céus", um objeto peculiar.<span class="reference" id="cite_ref-seds_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-seds-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; font-size: 15px; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Nebulosa do Anel</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M57_The_Ring_Nebula.JPG" style="background: none;" title="Nebulosa do Anel, Telescópio Espacial Hubble"><img alt="Nebulosa do Anel, Telescópio Espacial Hubble" data-file-height="1241" data-file-width="1215" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/13/M57_The_Ring_Nebula.JPG/250px-M57_The_Ring_Nebula.JPG" height="255" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/13/M57_The_Ring_Nebula.JPG/375px-M57_The_Ring_Nebula.JPG 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/13/M57_The_Ring_Nebula.JPG/500px-M57_The_Ring_Nebula.JPG 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />Nebulosa do Anel, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Dados observacionais (J2000)</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Constelação"><span style="color: black; font-family: Times New Roman; font-size: small;">Constelação</span></a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Lyra" style="background: none;" title="Lyra"><span style="color: black; font-family: Times New Roman; font-size: small;">Lyra</span></a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ascensão reta"><span style="color: black; font-family: Times New Roman; font-size: small;">Asc. reta</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">18<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 53<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 35,079<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-simbad-1" style="background: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Declinação"><span style="color: black; font-family: Times New Roman; font-size: small;">Declinação</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">+33° 01′ 45,03″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-simbad-1" style="background: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Magnitude aparente"><span style="color: black; font-family: Times New Roman; font-size: small;">Magnit. apar.</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">8,8<span class="reference" id="cite_ref-Murdin2000_2-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-Murdin2000-2" style="background: none;">2</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: black; font-family: Times New Roman; font-size: small;">Distância</span></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">2 300 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none;" title="Ano-luz">al</a> (700 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none;" title="Parsec">pc</a>)<span class="reference" id="cite_ref-ODelletal2002_3-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-ODelletal2002-3" style="background: none;">3</a></span> <span class="reference" id="cite_ref-Harrisetal2007_4-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-Harrisetal2007-4" style="background: none;">4</a></span> <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none;" title="Ano-luz">anos-luz</a></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: black; font-family: Times New Roman; font-size: small;">Dimensões</span></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">1,9 x 1,9 <span class="reference" id="cite_ref-ODelletal2002_3-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-ODelletal2002-3" style="background: none;">3</a></span> <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none;" title="Minuto de arco">minutos de arco</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Características físicas</span></td></tr>
<tr style="vertical-align: top;"><td><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Raio" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Raio"><span style="color: black; font-family: Times New Roman; font-size: small;">Raio</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">1,3 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none;" title="Ano-luz">al</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Magnitude absoluta"><span style="color: black; font-family: Times New Roman; font-size: small;">Magnit. absol.</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">-0,2</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #a0d8a0; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Outras denominações</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none;" title="Catálogo Messier">Messier</a> 57, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none;" title="New General Catalogue">NGC</a> 6720,<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Anel#cite_note-simbad-1" style="background: none;">1</a></span></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Nebulosa do Anel"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Nebulosa do Anel" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Lyra_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Lyra constellation map.png" data-file-height="2409" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/29/Lyra_constellation_map.png/250px-Lyra_constellation_map.png" height="337" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/29/Lyra_constellation_map.png/375px-Lyra_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/29/Lyra_constellation_map.png/500px-Lyra_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></span></a></div>
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http://pt.wikipedia.org/wiki/Nebulosa_do_Anel</div>
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Compass and Scale Image for Ring Nebula (HST only)</h2>
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<span style="background-color: white;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://hubblesite.org/newscenter/archive/releases/2013/13/image/d/format/web_print/</span></span></div>
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<strong>Object Names:</strong> Ring Nebula, M57, NGC 6720</div>
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<strong>Image Type:</strong> Astronomical/Illustration</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> <a href="http://www.nasa.gov/" style="color: #993333;">NASA</a>, <a href="http://www.spacetelescope.org/" style="color: #993333;">ESA</a>, and Z. Levay (<a href="http://www.stsci.edu/" style="color: #993333;">STScI</a>)</div>
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<span style="font-family: arial, sans-serif; font-size: x-small;"><span style="line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2013/13/image/d/</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b>Janine Milward</b></span><br /><div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b><br /></b></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b><br /></b></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 16.8pt;"><b><br /></b></span><span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 16.8pt;"><img src="http://www.ianridpath.com/atlases/urania/urania14.jpg" /></span></span><br /><div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">http://www.ianridpath.com/atlases/urania/urania14.jpg</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-84660002134516686102014-09-06T08:32:00.007-07:002015-01-04T08:05:15.476-08:00Lepus<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Sempre que nossa visão é atraída, irresistívelmente atraída,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">pelo Gigante Orion nos céus estrelados,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é certo que também podemos divisar</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">as estrelinhas que compõem a figura de Lepus, a Lebre,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem aos pés do Caçador</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e diante do Rio dos céus estrelados, Eridanus.</span></div>
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http://www.raremaps.com/gallery/detail/36717/LEridan_Orion_et_Le_Lievre/Flamsteed-Fortin.html</div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Title: </strong>L'Eridan, Orion et Le Lievre</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><strong>Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1260" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">John Flamsteed</a> / <a href="https://www.raremaps.com/gallery/browse/creator_id/1454" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; text-decoration: none;">MJ Fortin</a></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A bem da verdade, a figura do Gigante Caçador </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é inteiramente centralizadora de vários outros Asterismos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que fazem parte do Mito em torno a Orion.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação Taurus e as Pleiades, M45:</span><br />
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<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #073763; font-family: Arial, Helvetica, sans-serif;">De acordo com a mitologia clássica, </span><br />
<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #073763; font-family: Arial, Helvetica, sans-serif;">Orion era um caçador que buscava alcançar as Pleiades, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #073763; font-family: Arial, sans-serif;">as belas filhas de Atlas.<span class="apple-converted-space"> </span></span><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">As Pleiades ou Atlântidas eram as sete filhas de Atlas e Pleione, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background: white; color: #073763;">seis das quais podem ser vistas a olho nu e uma invisível ou “perdida”. </span><o:p></o:p></span></div>
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<span style="background: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Elas eram as companheiras virgens de Diana </span><br />
<span style="background: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e foram levadas para o céu para escaparem do Gigante Orion </span><br />
<span style="background: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">que as importunava. <o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">..........................</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Diana pode ser considerada como a versão romana para Artemis.</span><br />
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<span style="color: #073763;">Constelações Scorpius:</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">...... lenda conta que, tendo (Artemis) ela se apaixonado perdidamente pelo jovem </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Orion_(mitologia)" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Orion (mitologia)">Orion</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, e se dispondo a consorciá-lo, o seu enciumado irmão Apolo impediu o enlace mediante uma grande perfídia: achando-se em uma praia, em sua companhia, desafiou-a a atingir, com a sua flecha, um ponto negro que indicava a tona da água, e que mal se distinguia, devido à grande distância. Ártemis, toda vaidosa, prontamente retesou o arco e atingiu o alvo, que logo desapareceu no abismo no mar, fazendo-se substituir por espumas ensanguentadas. Era Orion que ali nadava, fugindo de um imenso escorpião criado por Apolo para persegui-lo. Ao saber do desastre, Ártemis, cheia de desespero, conseguiu, do pai, que a vítima e o escorpião fossem transformados em </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Quando a de Órion se põe, a de escorpião nasce, sempre o perseguindo, mas sem nunca alcançar.</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><br /></span><span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525;"><a href="http://pt.wikipedia.org/wiki/%C3%81rtemis">http://pt.wikipedia.org/wiki/%C3%81rtemis</a></span></span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: Arial, Helvetica, sans-serif;">............................................</span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525;"><br /></span></span><span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763;">Neste relato mais acima,</span></span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">penso que podemos incluir no cenário voltado para o Mito de Orion,</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a constelação do rio dos céus estrelados, Eridanus,</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem como a constelação do Navio</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- ambas constelações suprindo as questões voltadas para as águas</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(do Rio e do mar).</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E não podemos nos esquecer das presenças próximas</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de Cetus, a Baleia, o Monstro Marinho,</span></span><br />
<span style="background-color: white; line-height: 22.3999996185303px; text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e de Pisces, os Peixes.</span></span><br />
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<span style="color: #444444; font-family: Arial, Helvetica, sans-serif;"><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: Arial, sans-serif;">Outra versão é a de que Órion tentou violentar a deusa Ártemis. A fim de castigá-lo, Ártemis mandou um escorpião gigantesco morder-lhe o calcanhar, matando-o. Pelo serviço prestado à deusa, o escorpião foi transformado em constelação, simbolizando a raiva de Artemis por ter sido ameaçada de estupro ou, segundo algumas versões, por ter tido sua oferta afetiva e sexual rejeitada. .</span><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/%C3%93rion_(mitologia)"><span style="color: #376307; mso-bidi-font-size: 11.0pt; text-decoration: none; text-underline: none;">http://pt.wikipedia.org/wiki/%C3%93rion_(mitologia)</span><o:p></o:p></a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;"> </span><span style="color: #073763; line-height: 22.3999996185303px;">Richard Hinckley Allen, </span><span style="color: #073763; line-height: 22.3999996185303px;">em seu famoso e importantíssimo livro</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">Star Names — Their Lore and Meaning -,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">nos fala bem sobre </span></div>
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<span style="line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;">ESCORPIÃO E ÓRION:</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><i><span style="color: #666666;">..</span><span style="color: #444444;">. Aratos said:</span></i></span></div>
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<span style="color: #444444; font-family: Arial, Helvetica, sans-serif;"><i>When the Scorpion comes</i></span></div>
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<span style="color: #444444; font-family: Arial, Helvetica, sans-serif;"><i>Orion flies to utmost end of earth.</i></span></div>
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<span style="color: #444444; font-family: Arial, Helvetica, sans-serif;">Quando o Escorpião chega,</span></div>
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<span style="color: #444444; font-family: Arial, Helvetica, sans-serif;">Orion desaparece no final da terra.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Orion*.html" style="color: #376307; text-decoration: none;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Orion*.html</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">....................................</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">E ainda, em termos do cenário acolhendo Orion e seu Mito,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">podemos incluir as constelações Canis Major e Canis Minor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- os cães que acompanham o Caçador -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e, certamente, Lepus, a Lebre.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>E é bem aos pés ligeiros de Lepus,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>que encontraremos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>M79, o único Objeto Messier</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nesta constelação.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">LEPUS, O COELHO, A LEBRE</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 4h54m / 6h9m Declinação -11<sup>o</sup>.0 / +27<sup>o</sup>.1<o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Um jovem rapaz da Ilha de Leros muito queria um coelho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> e encomendou um mais distante - pois nenhum podia ser encontrado na ilha. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Os outros habitantes também quiseram possuir um coelho... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de tal forma que os animais se multiplicaram tanto</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> que não havia suficiente comida para eles, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que devoraram o milho nos campos.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Então, os habitantes se juntaram e deram cabo dos coelhos.<o:p></o:p></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 79</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M79 (NGC 1904)</i>, class V, in <a href="http://messier.obspm.fr/map/Lep.html">Lepus</a></center>
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<a href="http://messier.obspm.fr/Jpg/m79.jpg"><img align="right" alt="[m79.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m79.jpg" /></a><br />
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">05 : 24.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-24 : 33 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">42.1 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">9.6 (arc min)</td></tr>
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Discovered 1780 by Pierre Méchain.<br />
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Globular cluster Messier 79 (M79, NGC 1904) is a nice globular cluster in an unusual place for this kind of objects, in the hemisphere opposite to the Galactic Center, in the inconspicuous constellation Lepus.<br />
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M79 was found by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on October 26, 1780, and reported his discovery to his friend and colleague, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who determined its position and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M79">included it in his catalog</a> on December 17, 1780. It was first resolved into stars and recognized as a globular cluster by <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> in about 1784.<br />
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LEIA MAIS<br />
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http://messier.obspm.fr/m/m079.html<br />
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<span style="color: #660000;"><b>Messier 79</b> (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC</a> 1904)</span><span style="color: #252525;"> é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> localizado a mais de sessenta mil <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> de distância na direção da <a href="http://pt.wikipedia.org/wiki/Lepus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lepus">constelação da Lebre</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de +7,7, uma declinação de -24º 31' 27" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 5 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a>, 24 <a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a> e 10,6 <a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a>.</span></div>
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O aglomerado globular NGC 1904 foi descoberto em <a href="http://pt.wikipedia.org/wiki/1780" style="background: none; color: #0b0080; text-decoration: none;" title="1780">1780</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>.</div>
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Supõe-se estar associado com a galáxia anã de Canis Maior.</div>
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<span style="line-height: 22.3999996185303px;">A </span><a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Nebulosa">nebulosa</a><span style="line-height: 22.3999996185303px;"> foi descoberta pelo astrômomo francês </span><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a><span style="line-height: 22.3999996185303px;"> em 26 de outubro de 1780, sendo </span><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Catálogo Messier">catalogado</a><span style="line-height: 22.3999996185303px;"> pelo seu colega de observatório, </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="line-height: 22.3999996185303px;">, em 17 de dezembro daquele ano. </span><a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; line-height: 22.3999996185303px; text-decoration: none;" title="William Herschel">William Herschel</a><span style="line-height: 22.3999996185303px;"> foi o primeiro a resolver suas estrelas mais brilhantes em 1784.</span><span class="reference" id="cite_ref-seds_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-seds-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span></div>
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LEIA MAIS</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 79</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier79.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 79, projeto 2MASS"><img alt="Messier 79, projeto 2MASS" data-file-height="330" data-file-width="330" src="http://upload.wikimedia.org/wikipedia/commons/thumb/3/37/Messier79.jpg/250px-Messier79.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/3/37/Messier79.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/3/37/Messier79.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 79, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/26_de_outubro" style="background: none; color: #0b0080; text-decoration: none;" title="26 de outubro">26 de outubro</a> <a href="http://pt.wikipedia.org/wiki/1780" style="background: none; color: #0b0080; text-decoration: none;" title="1780">1780</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Lepus" style="background: none; color: #0b0080; text-decoration: none;" title="Lepus">Lepus</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background: none; color: #0b0080; text-decoration: none;" title="Aglomerado globular">Aglomerado globular</a> V<span class="reference" id="cite_ref-hcob849_11_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-hcob849_11-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">05<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 24<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 10,59<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-simbad-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-24° 31′ 27,3″<span class="reference" id="cite_ref-simbad_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-simbad-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">41 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">kal</a><span class="reference" id="cite_ref-apj657_1_286_3-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-apj657_1_286-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> (13 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">8,7'</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">11,7 bilhões de anos<span class="reference" id="cite_ref-mnras385_4_1998_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-mnras385_4_1998-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M79, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 1904, GCl 10<span class="reference" id="cite_ref-simbad_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_79#cite_note-simbad-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 79"><img alt="Messier 79" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Lepus_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Lepus constellation map.png" data-file-height="1709" data-file-width="1789" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a9/Lepus_constellation_map.png/250px-Lepus_constellation_map.png" height="239" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a9/Lepus_constellation_map.png/375px-Lepus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a9/Lepus_constellation_map.png/500px-Lepus_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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<dl style="font-family: sans-serif; font-size: 16px; line-height: 22.3999996185303px; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;"><div style="text-align: center;">
"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</a></span></span></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><br /><div class="MsoNormal" style="font-size: 16px; line-height: 22.3999996185303px;">
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<b><br /></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal; margin-left: 1em; margin-right: 1em;">
<img alt="Lepus" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_lepus.jpg" height="469" width="640" /></div>
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<span style="color: #073763;"><span style="font-family: Georgia, Times New Roman, Times, serif;"><span style="font-size: 14px;">http://www.aradergalleries.com/detail.php?id=3655</span></span></span></div>
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<span style="color: #073763;"><span style="font-family: Georgia, 'Times New Roman', Times, serif; font-size: 14px;">Johann Bayer — Lepus</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-64957324296190809832014-09-06T08:32:00.003-07:002015-01-04T08:02:13.665-08:00Leo<div class="MsoNormal">
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação do garboso Leão</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">é verdadeiramente muito interessante</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não somente por causa do desenho de suas estrelas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">figurando o rei dos animais dos céus estrelados</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como também,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ao longo dos tempos,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">foi nos revelando objetos</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(bem como Objetos Messier ora comentados)</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que realizaram-se enquanto galáxias,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">enquanto Grupos de galáxias,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">enquanto fusão desses Grupos</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e ainda enquanto fazendo parte</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- como Galáxia Anã denominada Leo I ou Regulus Dwarf -</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de nosso chamado Grupo Local!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entrou em cena Leo II</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- que </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">encontra-se ainda além o Grupo Leo I</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que é bem mais próximo),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém ambos situam-se numa mesma região.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entrou em cena Leo III.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entraram em cena Aglomerados de galáxias.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entrou em cena o Superaglomerado Leo.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, e bem recentemente (agora, em setembro de 2014!),</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">entrou em cena Laniakea,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nosso novo endereço dentre as estrelas do céu que nos protege,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">esse Céu Imensurável!</span><br />
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<img alt="Leo" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_uranometria05.jpg" height="477" width="640" /></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://www.aradergalleries.com/detail.php?id=1668">http://www.aradergalleries.com/detail.php?id=1668</a></span></span></div>
<span style="font-family: Georgia, 'Times New Roman', Times, serif;"><span style="color: #073763;">Johann Bayer — Leo</span></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O garboso Leão dos céus estrelados</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">com toda certeza, sempre nos revela mais e mais segredos</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e nos confirma nossa mente que vai acompanhando</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">a revelação de que,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">quanto mais nos aprofundamos no passado</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mais conhecemos nosso presente</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e mais concordamos</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que existe mais, bem mais, entre a Terra e o céu</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">que nossa simples mente possa imaginar!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Da Terra ao Céu e ao Infinito:</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">Os desenhos formados pelas estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> - As Constelações - </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">são como janelas que se abrem para a infinitude do universo </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> entre o céu e a terra..., </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como percebendo que o caos, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vagarosamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">vai se tornando Cosmos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> e este por nossa mente sendo conscientizado.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Quer dizer, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">nossa mente é tão infinita quanto infinito é o Cosmos.<o:p></o:p></span></div>
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<img alt="Leo constellation map.png" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/de/Leo_constellation_map.png/240px-Leo_constellation_map.png" height="498" width="640" /></div>
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<a href="http://pt.wikipedia.org/wiki/Leo_A">http://pt.wikipedia.org/wiki/Leo_A</a><br />
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><i><br /></i></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><i><br /></i></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><i><br /></i></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nossa Postagem estará trazendo um tantinho de informações</span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>sobre</b></span><br />
<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M65, M66, M95, M96 e M105</b></span><br />
<b style="color: #660000;"><span style="font-family: Arial, Helvetica, sans-serif;">os Objetos Messier em Leão</span></b><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M65 e M66 foram descobertos por Charles Messier <o:p></o:p></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e catalogados em março de 1780.<o:p></o:p></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M95 e M96 foram descobertos por Pierre Mechain, </b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>em 1781,</b><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> e logo foram incluídos por Messier </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(colega de observatório) </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em seu Catálogo.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, M105, descoberto por Mechain,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> não foi incluído no Catálogo Messier<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- por alguma razão que desconhecemos -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e somente assim aconteceu em 1947, </span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">como um objeto adicional.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Vamos encontrar Objetos Messier</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">no corpo central e nas proximidades da cauda</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">do Leão, o garboso rei dos animais dos céus estrelados!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Nas proximidades da cauda do Leão,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vamos encontrar <b>M65 e M66 e ainda NGC 3628</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>formando o famoso Leo Triplet ou Grupo M66.</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No corpo do Leão,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">vamos encontrar <b>M95 e M96 e M105,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>formando o Grupo M96 </b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e acolhendo ainda outras galáxias menos significativas.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>O Grupo M96 vem sendo conhecido como Grupo Leo I</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e, por causa da proximidade entre este Grupo M96 e o Grupo M66,</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ambos tornaram-se subgrupos pertencentes ao Grupo Leo I.</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">E ainda, pelo fato da proximidade da estrela-alpha Leonis, Regulus,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e todo seu brilho, no céu estrelado,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>algumas vezes o Grupo Leo I é conhecido como Regulus Dwarf.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Bright Star Regulus near the Leo 1 Dwarf Galaxy </b><br /><b>Credit & <a href="http://www.rc-astro.com/copyright.html" style="color: #274e13; text-decoration: none;">Copyright</a>: </b><a href="http://www.rc-astro.com/about.html" style="color: #274e13; text-decoration: none;">Russell Croman</a></span></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>The star on the upper left is so bright it is sometimes hard to notice the galaxy on the lower right. Both the star, <a href="http://en.wikipedia.org/wiki/Regulus" style="color: #274e13; text-decoration: none;">Regulus</a>, and the galaxy, <a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)" style="color: #274e13; text-decoration: none;">Leo I</a>, can be found within one degree of each other toward the constellation of Leo. <a href="http://www.astro.uiuc.edu/~kaler/sow/regulus.html" style="color: #274e13; text-decoration: none;">Regulus</a> is part of a<a href="http://homepage.univie.ac.at/peter.wienerroither/pwafods/10084+1158.htm" style="color: #274e13; text-decoration: none;">multiple star system</a>, with a close companion <a href="http://apod.nasa.gov/apod/ap970219.html" style="color: #274e13; text-decoration: none;">double star</a> visible to the upper right of the young <a href="http://observe.arc.nasa.gov/nasa/space/stellardeath/stellardeath_1ai.html" style="color: #274e13; text-decoration: none;">main sequence</a> star. Leo I is a <a href="http://www.astro.uu.se/~ns/review.html" style="color: #274e13; text-decoration: none;">dwarf spheroidal galaxy</a> in the <a href="http://www.seds.org/messier/more/local.html" style="color: #274e13; text-decoration: none;">Local Group</a> of galaxies dominated by our <a href="http://apod.nasa.gov/apod/ap980523.html" style="color: #274e13; text-decoration: none;">Milky Way Galaxy</a> and <a href="http://apod.nasa.gov/apod/ap051222.html" style="color: #274e13; text-decoration: none;">M31</a>. Leo I is thought to be the most distant of the <a href="http://www.astro.uu.se/~ns/mwsat.html" style="color: #274e13; text-decoration: none;">several known small satellite galaxies</a> orbiting our <a href="http://apod.nasa.gov/apod/ap971229.html" style="color: #274e13; text-decoration: none;">Milky Way Galaxy</a>. Regulus is located about 75 <a href="http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html" style="color: #274e13; text-decoration: none;">light years</a> away, in contrast to Leo 1 which is located about 800,000 light years awa</span><span style="font-family: 'Times New Roman';">y.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Leia, Caro Leitor,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">alguns excertos de textos mais abaixo apresentados:</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i><b>O Grupo M96 (também conhecido como Grupo Leo I)</b> </i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>é um grupo de galáxias </i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>na constelação do Leão e contém entre 8 e 24 galáxias, </i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>incluindo Objetos Messier.</i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Esse grupo é um dos muitos grupos</i></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i> que se situam dentro do Superaglomerado Virgo</i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>(quer dizer, o Superaglomerado Local).</i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(minha tradução simples e direta para o texto encontrado</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mais abaixo, em inglês, e extraído de <a href="http://en.wikipedia.org/wiki/Leo_I_Group" style="background-color: white; line-height: 19px; text-decoration: none;">http://en.wikipedia.org/wiki/Leo_I_Group</a><span style="background-color: white; line-height: 19px;">)</span></span><br />
<span style="color: #073763;"><span style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><br /></span><span style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><br /></span><span style="background-color: white; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><i>O Grupo M96 pode ser fisicamente relacionado ao Grupo M66</i></span></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><i>e estes podem ser considerados praticamente na mesma distância</i></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><i>e situados praticamente próximos no céu.</i></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 19px;">(minha tradução simples e direta para um trecho extraído de</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><a href="http://messier.seds.org/more/m096gr.html">http://messier.seds.org/more/m096gr.html</a>)</span><br />
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<b><i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Leo I é um Grupo grande e proeminente e consistido,</span></i></b><br />
<b><i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> predominantemente, </span></i></b></div>
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<b><i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de galaxias espirais em Leão.</span></i></b></div>
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<b><i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Leo I consiste de dois principais subgrupos:</span></i></b></div>
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<b><i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Grupo M66 e o Grupo M96.</span></i></b></div>
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<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O primeiro situa-se a cerca de 35 milhões de anos-luz </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e é centrado através galáxias espirais M65, M66 e parte de NGC3628, </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e também conhecido como Leo Triplet.</span></i><br />
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<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Não muito distante do Grupo M66 </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e quase fisicamente relacionado a este, </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">encontra-se o Grupo M96, bem maior e dominado por M96,</span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> a cerca de 41 milhões de anos-luz,</span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> M95 e M101 e NGC 3384. </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Outros membros menos significativos incluem ......</span></i></div>
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<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">...........................................................</span></i></div>
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<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></i></div>
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<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em função do fato de que Leo I encontra-se bem próximo </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">à estrela Regulus</span></i></div>
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<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">no céu </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(tornando o estudo do mesmo mais dificultado </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">por causa da luz dessa estrela luminosa), </span></i><br />
<i><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">algumas vezes Leo I é conhecido como Regulus Dwarf ....</span></i></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(minha tradução simples e direta para o texto encontrado</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">mais abaixo, em inglês, e extraído de <a href="http://www.daviddarling.info/encyclopedia/L/Leo_I.html" style="line-height: 22.3999996185303px;">http://www.daviddarling.info/encyclopedia/L/Leo_I.html</a>)</span></div>
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<img src="http://www.allthesky.com/constellations/leo/bigm.jpg" /></div>
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<a href="http://www.allthesky.com/constellations/leo/">http://www.allthesky.com/constellations/leo/</a></div>
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<a href="http://www.allthesky.com/copyright.html" style="font-style: italic;" target="_parent">© all photographs</a><span style="color: white; font-style: italic;"> taken by </span><a href="mailto:credner@allthesky.de" style="font-style: italic;">Till Credner</a><span style="color: white; font-style: italic;"> and </span><a href="mailto:kohle@allthesky.de" style="font-style: italic;">Sven Kohle</a></div>
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<a href="http://www.allthesky.com/constellations/leo/">http://www.allthesky.com/constellations/leo/</a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>O Grupo Leo I é um grupo de galáxias muito famoso em função do fato </i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>de que contém muitas galáxias brilhantes. </i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>Á direita, encontra-se o subgrupo M96 </i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>e,</i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>à esquerda, encontra-se o subgrupo M66</i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>e ambos esses subgrupos são interconectados através NGC 3489,</i></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><i>que encontra-se entre eles.</i></span></div>
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<h1 style="border: 1px solid rgb(102, 102, 204); font-family: 'Century Gothic', Monaco, Avantgarde, 'URW Gothic L', sans-serif; font-size: 29px; font-weight: normal; margin: 0px 62.671875px; position: relative;">
<span style="color: #274e13;">The Leo I Group</span></h1>
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<span style="color: #274e13;">The Leo I group is a very famous group of galaxies because it contains a lot of bright galaxies. On the right is the M96 subgroup and on the left is the M66 subgroup which are connected to each other via NGC 3489 which lies between them.</span></div>
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<span style="color: #274e13;"><img alt="The Leo I Group" src="http://www.atlasoftheuniverse.com/galgrps/leoi.gif" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; cursor: move; padding: 8px;" width="640" /></span></div>
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<span style="font-size: 14px; line-height: 22.3999996185303px; text-align: start;"><span style="color: #274e13; font-family: sans-serif;"><a href="http://www.atlasoftheuniverse.com/galgrps/leoi.html">http://www.atlasoftheuniverse.com/galgrps/leoi.html</a></span></span></div>
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<span style="color: #274e13;"><span lang="EN-US" style="font-family: Arial, sans-serif;"><br /></span><span lang="EN-US" style="font-family: Arial, sans-serif;"><br /></span><span lang="EN-US" style="font-family: Arial, sans-serif;"><img src="http://upload.wikimedia.org/wikipedia/commons/5/5e/Local_supercluster.jpg" height="620" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; cursor: move; padding: 8px;" width="640" /></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><a href="http://pt.wikipedia.org/wiki/Superaglomerado_de_gal%C3%A1xias#mediaviewer/Ficheiro:Local_supercluster.jpg">http://pt.wikipedia.org/wiki/Superaglomerado_de_gal%C3%A1xias#mediaviewer/Ficheiro:Local_supercluster.jpg</a></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="color: #274e13; font-size: 1.2em; max-width: 60%;">Local supercluster</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte" style="color: #274e13;"><span class="mw-mmv-author">NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://en.wikipedia.org/wiki/Image:Local_supercluster.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://en.wikipedia.org/wiki/Image:Local_supercluster.jpg</a> / <a class="external free" href="http://heasarc.nasa.gov/docs/cosmic/local_supercluster.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;">http://heasarc.nasa.gov/docs/cosmic/local_supercluster.html</a></span></span></div>
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<span style="color: #274e13;"><b style="font-size: 16px;"><br /></b><b style="font-size: 16px;"><br /></b></span><br />
<span style="color: #274e13;"><b style="font-size: 16px;"><br /></b></span><span style="color: #274e13;"><b style="font-size: 16px;"><br /></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe também o chamado <b>Grupo Leo II</b>.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Grupo Leo II encontra-se ainda além o Grupo Leo I</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(que é bem mais próximo),</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">porém ambos situam-se numa mesma região.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entrou em cena Leo III.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entraram em cena Aglomerados de galáxias.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, entrou em cena o Superaglomerado Leo.</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com o tempo, e bem recentemente (agora, em setembro de 2014!),</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">entrou em cena Laniakea,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nosso novo endereço dentre as estrelas do céu que nos protege,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">esse Céu Imensurável!</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<b><span style="color: #660000;"><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Leo B</span><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (ou </span><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Leo II</span></span></b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><b><span style="color: #660000;">)</span></b><span style="color: #252525;"> é uma </span></span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_an%C3%A3_esferoidal" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia anã esferoidal">galáxia anã esferoidal</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> a proximadamente 690.000 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> de distância na direção da </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Leo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Leo">Leo</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;">. A partir de Outubro de 2008, é uma das 24 galáxias satélites conhecidas da </span><a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Via Láctea">Via Láctea</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;">.</span><span class="reference" id="cite_ref-toll08_4-0" style="bottom: 1ex; color: #252525; font-family: sans-serif; font-weight: normal; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Leo_II#cite_note-toll08-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> A partir de 2007, acredita-se que Leo II tenha um núcleo com um raio de 178 ± 13 pc e uma maré com raio de 632 ± 32 pc.</span><span class="reference" id="cite_ref-5" style="bottom: 1ex; color: #252525; font-family: sans-serif; font-weight: normal; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Leo_II#cite_note-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> Ela foi descoberta em </span><a href="http://pt.wikipedia.org/wiki/1950" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1950">1950</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> por </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Robert_G._Harrington&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Robert G. Harrington (página não existe)">Robert G. Harrington</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> e </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Albert_George_Wilson&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Albert George Wilson (página não existe)">Albert George Wilson</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;">, do </span><a class="new" href="http://pt.wikipedia.org/w/index.php?title=Obasevat%C3%B3rio_Monte_Wilson&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Obasevatório Monte Wilson (página não existe)">Monte Wison</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> e </span><a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_Palomar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Observatório Palomar">Observatório Palomar</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Calif%C3%B3rnia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Califórnia">Califórnia</a><span style="color: #252525; font-family: sans-serif; font-weight: normal; line-height: 22.3999996185303px; text-align: start;">.</span></div>
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<span style="line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://pt.wikipedia.org/wiki/Leo_II">http://pt.wikipedia.org/wiki/Leo_II</a></span></span></div>
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<span style="color: #660000;"><b style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Leo A</b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (também conhecida como </span><b style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Leo III</b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">)</span></span><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_irregular" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Galáxia irregular">galáxia irregular</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/Leo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Leo">Leo</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e faz parte do </span><a href="http://pt.wikipedia.org/wiki/Grupo_Local" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Grupo Local">Grupo Local</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Ela fica a aproximadamente 2,25 milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span></div>
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<span style="color: #274e13; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Leo_A">http://pt.wikipedia.org/wiki/Leo_A</a></span></span><br />
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<span style="color: #274e13; font-size: large;">Local Group</span></h1>
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<span style="color: #274e13;"><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;">A collection of more than 40 galaxies, spread across a volume of space some 10 million light-years in diameter, of which our own </span><a href="http://www.daviddarling.info/encyclopedia/G/Galaxy.html" style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start; text-decoration: none;">Milky Way Galaxy</a><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;"> and the </span><a href="http://www.daviddarling.info/encyclopedia/A/Andromeda.html" style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start; text-decoration: none;">Andromeda Galaxy</a><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;"> are the dominant and central members. Both these two giant spirals have retinues of </span><a href="http://www.daviddarling.info/encyclopedia/S/satellite_galaxy.html" style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start; text-decoration: none;">satellite galaxies</a><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;">, which together account for most of the membership of the Local Group.</span></span></div>
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<span style="color: #274e13;"><img alt="Local Group" src="http://www.daviddarling.info/images/Local_Group.jpg" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; cursor: move; padding: 8px;" width="640" /></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: small; font-weight: normal;"><a href="http://www.daviddarling.info/encyclopedia/L/LocalGroup.html">http://www.daviddarling.info/encyclopedia/L/LocalGroup.html</a></span></h1>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><br /></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Veja em</b></span></div>
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<span style="color: #274e13;"><a href="http://www.nightskyatlas.com/catAbell.jsp?id=LEO">http://www.nightskyatlas.com/catAbell.jsp?id=LEO</a></span></div>
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<span style="color: #073763; font-size: large;">Galaxy Clusters of Leo - The Night Sky Atlas</span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b>uma imensa lista (o Catálogo Abell)</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b> de Aglomerados de Galáxias</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: small;"><b>na constelação do Leão</b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiStOZ0-MyRw6Yuj7qRD32y0CgQDPbTKgJh6Zil2-lG1B7r464ZHCenMiD5MII7S7g-9gnteVAYHz0yp9UHhCzjH_X7NbbV-zSkaISxez0jRZnOqXUDnkWxumMFTEPjH4-46Sl7S1I5xiY/s1600/abell+clusters.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiStOZ0-MyRw6Yuj7qRD32y0CgQDPbTKgJh6Zil2-lG1B7r464ZHCenMiD5MII7S7g-9gnteVAYHz0yp9UHhCzjH_X7NbbV-zSkaISxez0jRZnOqXUDnkWxumMFTEPjH4-46Sl7S1I5xiY/s1600/abell+clusters.png" height="266" width="640" /></a></div>
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<a href="http://www.nightskyatlas.com/catAbell.jsp?id=LEO">http://www.nightskyatlas.com/catAbell.jsp?id=LEO</a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Existe <b>o Superaglomerado Leo</b>,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">não exatamente considerado famoso</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em função de sua distância a cerca de 440 milhões de anos-luz de nós</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e, a esta distância, é difícil de ser visualizado em função</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">das galáxias que se encontram em primeiro plano.</span></div>
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<img alt="The closest superclusters" src="http://www.atlasoftheuniverse.com/nearsc.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<div style="text-align: center;">
<span style="font-family: Arial, Helvetica, sans-serif;">http://www.atlasoftheuniverse.com/nearsc.html</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>CÉU IMENSURÁVEL</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Laniakea</b></span></div>
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<b><span style="color: #660000;">Laniakea é um <a href="http://pt.wikipedia.org/wiki/Superaglomerado_de_gal%C3%A1xias" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Superaglomerado de galáxias">Superaglomerado de galáxias</a>, onde a <a href="http://pt.wikipedia.org/wiki/Via_L%C3%A1ctea" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Via Láctea">Via Láctea</a>, o <a href="http://pt.wikipedia.org/wiki/Sistema_Solar" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Sistema Solar">Sistema Solar</a> e a <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Terra">Terra</a> estão localizados</span></b><span style="color: #252525;">. Foi definido em setembro de 2014, quando astrônomos da Universidade do Havaí, liderados por R. Brent Tully, publicaram um novo método de definir superaglomerados de acordo com as velocidades relativas de </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">Galáxias</a><span style="color: #252525;">. Essa nova definição de superaglomerados locais engloba o anteriormente caracterizado </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Superaglomerado_de_virgem" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Superaglomerado de virgem">Superaglomerado de Virgem</a><span style="color: #252525;"> como um apêndice de Laniakea.</span></div>
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O superaglomerado de Laniakea abrange 100,000 galáxias ao longo de 520 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Anos-luz">Anos-luz</a>. No centro do superaglomerado, há um ponto gravitacional central denominado <a href="http://pt.wikipedia.org/wiki/Grande_Atrator" style="background: none; color: #0b0080; text-decoration: none;" title="Grande Atrator">Grande Atrator</a>, que atrai todas as galáxias do superaglomerado, fazendo com que o movimento de cada galáxia seja direcionado para esse centro de massa.</div>
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A palavra Laniakea significa "paraíso imensurável" em havaiano. <span class="reference" id="cite_ref-NRAO-2014-09-03_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Laniakea#cite_note-NRAO-2014-09-03-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Laniakea">http://pt.wikipedia.org/wiki/Laniakea</a></span></span></div>
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<img alt="" class="vox-lazy-load lazy-loaded" data-dim="755x504" data-imgkey="37958316:standard:44" src="http://cdn0.vox-cdn.com/uploads/chorus_image/image/37962938/lanikea_map.0.0_standard_755.0.png" data-original="http://cdn0.vox-cdn.com/uploads/chorus_image/image/37962938/lanikea_map.0.0_standard_755.0.png" data-overlay="c-warm" data-ratio="1.5" style="background-color: #f1f3f2; border: 0px; box-sizing: border-box; color: #4c4e4d; display: block; font-family: 'Alright Sans', sans-serif; font-size: 15px; line-height: 25.0000514984131px;" /></div>
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<figcaption class="p-caption" style="background-color: #f1f3f2; border-bottom-color: rgb(217, 214, 215); border-bottom-style: solid; border-bottom-width: 1px; box-sizing: border-box; color: #979797; display: table; font-family: 'Alright Sans', sans-serif; font-size: 0.8em; padding: 1em 5px 0.75em; text-align: start; width: 755px;"><span class="p-caption__text" style="box-sizing: border-box; display: table-cell;"><span style="background-color: white;"><span style="color: #073763;">A new study in Nature finds that the Milky Way is part of a broader supercluster of 100,000 galaxies known as Laniakea.</span></span></span></figcaption><a href="http://www.vox.com/2014/9/4/6105631/map-galaxy-supercluster-laniakea-milky-way">http://www.vox.com/2014/9/4/6105631/map-galaxy-supercluster-laniakea-milky-way</a><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">VEJA O VÍDEO</span></div>
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<span class="watch-title " dir="ltr" id="eow-title" style="background: transparent; border: 0px; margin: 0px; padding: 0px;" title="Laniakea: Our home supercluster"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Laniakea: Our home supercluster</span></span></h1>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.youtube.com/watch?v=rENyyRwxpHo#t=235">http://www.youtube.com/watch?v=rENyyRwxpHo#t=235</a></span><br />
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<div style="background-color: white;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mais comentários sobre </span></div>
<div style="background-color: white;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>a Constelação do Leão</b></span></div>
<div style="background-color: white;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">podem ser encontrados em meu Trabalho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">em</span></div>
<div style="background-color: white;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Da Terra ao Céu e ao Infinito</b></span></div>
<div style="background-color: white;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/leo-o-leao.html">http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/leo-o-leao.html</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - Cartas Celestes, As Constelações - CARJ</span></div>
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<tr><td><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilqJDMWExPq7CNKpvgOhUP7V59tEyPXHdeKjYjpwdRFzledNNONwzuPOLzEvztoAs0bA1zgdkUUq_HG1Y36waZ-Fg3ZKckNTJ06s6m43raQpH3ZzrHr48UYbXwiDWMHZdB3Qr5hCF-5sl9/s1600/alfabeto+grego%252C+conven%25C3%25A7%25C3%25B5es+e+uso+da+carta+celeste.jpg" imageanchor="1" style="color: #274e13; margin-left: auto; margin-right: auto; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilqJDMWExPq7CNKpvgOhUP7V59tEyPXHdeKjYjpwdRFzledNNONwzuPOLzEvztoAs0bA1zgdkUUq_HG1Y36waZ-Fg3ZKckNTJ06s6m43raQpH3ZzrHr48UYbXwiDWMHZdB3Qr5hCF-5sl9/s640/alfabeto+grego%252C+conven%25C3%25A7%25C3%25B5es+e+uso+da+carta+celeste.jpg" height="422" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #faf2d9; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(191, 144, 0); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></span></a></td></tr>
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<span style="line-height: 11px;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></span></div>
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<span style="line-height: 11px;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;"> - excerto -</span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #660000;"><b>LEO, O LEÃO</b></span><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 9h18m / 11h56m Declinação -6<sup>o</sup>.4 / +33<sup>o</sup>.3<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esta constelação do Zodíaco representa o Leão de Neméia</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> que se originava da Lua e que foi degolado por Hércules.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Constelação das primeiras conhecidas dos babilônios que, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">como todos os povos da antiguidade, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">associavam o Leão ao Sol. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O Leão é, realmente, a mais notável de todas as constelações zodiacais, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">já que o Sol encontrava-se neste asterismo no solstício do verão, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">na época em que esse asterismo foi instituído. </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Realmente, esta antiga constelação era reconhecida por muitas civilizações antigas, incluindo aquelas na Babilônia, no Egito e na Grécia.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Para os egípcios, a entrada do Sol no asterismo do Leão</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> correspondia às inundações do Nilo </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e servia, portanto, como importante referência à atividade agrícola, </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">pois a inundação trazia a fertilidade das margens do Nilo.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Leo situa-se entre as constelações Virgo, Coma Berenices, Ursa Major, Leo Minor, Câncer, Hydra, Sextans, Crater<span style="color: #0f243e;"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;"> 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">de autoria de Ronaldo Rogério de Freitas Mourão</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">Editora Vozes, Petrópolis, ano de 1986</span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhJ504KBjtYyPWgb-jdYyLjK2S6QzVWPcef619lujIgbVIO3-GeVObTWh8JL43gV3t9TtJxX-mand55BYeFtIDmsOgvE4l7dKrzCalc8pciZBuSqj00Ud3CG5yNyAkRqXBcr2DAY9z11lc/s1600/LEO.gif" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhJ504KBjtYyPWgb-jdYyLjK2S6QzVWPcef619lujIgbVIO3-GeVObTWh8JL43gV3t9TtJxX-mand55BYeFtIDmsOgvE4l7dKrzCalc8pciZBuSqj00Ud3CG5yNyAkRqXBcr2DAY9z11lc/s1600/LEO.gif" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #faf2d9; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<a href="http://www.iau.org/static/public/constellations/gif/LEO.gif" style="color: #274e13; text-decoration: none;"><span style="font-family: Arial, Helvetica, sans-serif;">http://www.iau.org/static/public/constellations/gif/LEO.gif</span></a></div>
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<b>Caro Leitor,</b><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Vamos encontrar Objetos Messier</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>no corpo central e nas proximidades da cauda</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>do Leão, o garboso rei dos animais dos céus estrelados!</b></span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Nas proximidades da cauda do Leão,</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>vamos encontrar M65 e M66 e ainda NGC 3628</b></span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>formando o famoso Leo Triplet ou Grupo M66.</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>No corpo do Leão,</b></span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>vamos encontrar M95 e M96 e M105,</b></span></div>
<div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>formando o Grupo M96 </b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>e acolhendo ainda outras galáxias menos significativas.</b></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/a/a8/LeoCC.jpg" height="640" width="427" /></div>
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<span style="color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://en.wikipedia.org/wiki/Leo_(constellation)#mediaviewer/File:LeoCC.jpg">http://en.wikipedia.org/wiki/Leo_(constellation)#mediaviewer/File:LeoCC.jpg</a></span></span></div>
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<span style="background-color: white;"><span style="color: #073763;"><span style="font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">The constellation Leo as it can be seen by the naked eye (the bright object in the centre of the picture is the planet Jupiter). </span><a class="external text" href="http://www.allthesky.com/constellations/leo.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">AlltheSky.com</a></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><b> OBJETOS MESSIER</b></span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><b>NAS PROXIMDADES DA CAUDA DO LEÃO</b></span></span></div>
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<span style="color: #660000;"><b>- M65 E M66 -</b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEigHtVTcoiJ_lmt5D0_58R_M6VGdYJtgu5dBeMvPCQf2yUBQ2I995UCz_HKgb7PAhiBvMwDIyHvDQS4vD7lSbA004zZ_Nls5GaJrdfYfczA5jwgCzV7w_8ww3WlXsQ9Ukt3VAiu9mRjmg4/s1600/leo+-+parte+traseira.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEigHtVTcoiJ_lmt5D0_58R_M6VGdYJtgu5dBeMvPCQf2yUBQ2I995UCz_HKgb7PAhiBvMwDIyHvDQS4vD7lSbA004zZ_Nls5GaJrdfYfczA5jwgCzV7w_8ww3WlXsQ9Ukt3VAiu9mRjmg4/s1600/leo+-+parte+traseira.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro -</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">excerto da Carta Celeste sobre a constelação do Leão</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Cartas Celestes, As Constelações</span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m65atlas.jpg" /></div>
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<a href="http://www.ipac.caltech.edu/2mass/gallery/m65atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m65atlas.jpg</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 65</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M65 (NGC 3623)</i>, type Sa, in <a href="http://messier.obspm.fr/map/Leo.html">Leo</a><b><span style="font-size: large;">in the Leo Triplett</span></b><br /><b><br /></b></center>
<a href="http://messier.obspm.fr/Jpg/m65.jpg"><img alt="[m65.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m65.jpg" style="text-align: right;" /></a><br />
<table border="2" cellpadding="5" cellspacing="0" style="text-align: center;"><tbody>
<tr><th align="left">Right Ascension</th><td>11 : 18.9 (h:m)</td></tr>
<tr><th align="left">Declination</th><td>+13 : 05 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td>35000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td>9.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td>8x1.5 (arc min)</td></tr>
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Discovered 1780 by Charles Messier.</div>
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Messier 65 (M65, NGC 3623), together with its neighbors <a href="http://messier.obspm.fr/m/m066.html">M66</a> and <a href="http://messier.obspm.fr/xtra/ngc/n3628.html">NGC 3628</a>, forms a most conspicuous triplet of galaxies, the <a href="http://messier.obspm.fr/more/m066gr.html">Leo Triplett or M66 group</a>, located at a distance of about 35 million light years.</div>
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Although it is close to and thus under the gravitational influence of its neighbors, M65 looks like a very "normal" Sa type spiral and seems to have felt little influence. It has a prominent central lense and tightly wound spiral arms, plus a prominent dust lane marking the facing edge. The luminous disk is dominated by a smooth old stellar population. Near the lane, some knots are visible, which, according to <i>J.D. Wray</i>, may be associated with star forming regions. The lane may hide regions of star formation usually associated with such features in spiral galaxies.</div>
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Our image of M65 was obtained by <a href="http://www.aao.gov.au/images/general/malin.html">David Malin</a> with the <a href="http://www.aao.gov.au/">Anglo Australian Telescope</a>; interested readers may obtain <a href="http://messier.obspm.fr/more/m065_image.html">more detailed information on our image</a>.</div>
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M65, together with its neighbor, M66, has been discovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M65">cataloged it</a> on March 1, 1780, describes it as "very faint nebula without stars." Because of a dubious error, <a href="http://messier.obspm.fr/xtra/Bios/smyth.html">Admiral Smyth</a> has <a href="http://www.seds.org/messier/Mdes/dm065.html#smyth">assigned</a> this discovery of M65 and M66 (and <a href="http://messier.obspm.fr/m/m068.html">M68</a>) to <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a>, a view which was adopted by <a href="http://messier.obspm.fr/xtra/Bios/kgj.html">Kenneth Glyn Jones</a> somewhen in the 1960s, and consequently, in many sources, despite the fact that Messier doesn't acknowledge such a prior sighting, which he did in all other cases.</div>
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Halton Arp includes M65 in his entry number 317 of his <a href="http://messier.obspm.fr/xtra/supp/m-arp.html">Catalogue of Peculiar Galaxies</a>, which denotes the Leo Triplett.</div>
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<a href="https://www.blogger.com/goog_2014696277">L</a>EIA MAIS</div>
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<a href="http://www.ipac.caltech.edu/2mass/gallery/m66atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m66atlas.jpg</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 66</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M66 (NGC 3627)</i>, type Sb, in <a href="http://messier.obspm.fr/map/Leo.html">Leo</a><b><span style="font-size: large;">in the Leo Triplett</span></b><br /><b><br /></b><b><br /></b></center>
<a href="http://messier.obspm.fr/Jpg/m66.jpg"><img alt="[m66.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m66.jpg" style="text-align: right;" /></a><br />
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<tr><th align="left">Right Ascension</th><td>11 : 20.2 (h:m)</td></tr>
<tr><th align="left">Declination</th><td>+12 : 59 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td>35000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td>8.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td>8x2.5 (arc min)</td></tr>
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Discovered 1780 by Charles Messier.</div>
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Messier 66 (M66, NGC 3627), together with its neighbors <a href="http://messier.obspm.fr/m/m065.html">M65</a> and <a href="http://messier.obspm.fr/xtra/ngc/n3628.html">NGC 3628</a>, forms a most conspicuous triplet of galaxies, the <a href="http://messier.obspm.fr/more/m066gr.html">Leo Triplett or M66 group</a>, located at a distance of about 35 million light years.</div>
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M66 is considerably larger than its neighbor, <a href="http://messier.obspm.fr/m/m065.html">M65</a>, and has a well developed but not well defined central bulge, and is therefore classified Sb. Obviously its spiral arms are deformed, probably because of the encounters with its neighbors. They seem to be distorted and displaced above the plane of the galaxy. Note how one of the spiral arms seems to pass over the left side of the central bulge. Much dust is visible here, as well as a few pink nebulae, signs of star formation, near the end of one of the arms.</div>
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This image was obtained by <a href="http://www.aao.gov.au/images/general/malin.html">David Malin</a> with the 3.9-meter <a href="http://www.aao.gov.au/">Anglo Australian Telescope</a>; interested readers may obtain <a href="http://messier.obspm.fr/more/m066_image.html">more detailed information on this image</a>.</div>
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Together with its neighbor M65, M66 has been discovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M66">cataloged it</a> on March 1, 1780, remarks that he missed these two objects in 1773, when a comet passed between them on November 1 to 2, 1773, probably because of the light of the comet. Because of a dubious error, <a href="http://messier.obspm.fr/xtra/Bios/smyth.html">Admiral Smyth</a> has <a href="http://www.seds.org/messier/Mdes/dm066.html#smyth">assigned</a> this discovery of M65 and M66 (and <a href="http://messier.obspm.fr/m/m068.html">M68</a>) to <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a>, a view which was adopted by <a href="http://messier.obspm.fr/xtra/Bios/kgj.html">Kenneth Glyn Jones</a> somewhen in the 1960s, and consequently, in many modern sources, despite the fact that Messier doesn't acknowledge such a prior sighting, which he did in all other cases.</div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span style="font-size: large;">The Leo Triplet (also known as the M66 Group)</span></span></b><span style="color: #274e13; font-size: 16px;"> is a small </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Group_of_galaxies" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Group of galaxies">group of galaxies</a><span style="color: #274e13; font-size: 16px;"> about </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E22_m" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="1 E22 m">35 million</a><span style="color: #274e13; font-size: 16px;"> </span><a href="http://en.wikipedia.org/wiki/Light-year" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Light-year">light-years</a><span style="color: #274e13; font-size: 16px;"> away</span><sup class="reference" id="cite_ref-5" style="color: #274e13; font-size: 16px; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-5" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[5]</a></sup><span style="color: #274e13; font-size: 16px;"> in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Constellation">constellation</a><span style="color: #274e13; font-size: 16px;"> </span><a href="http://en.wikipedia.org/wiki/Leo_(constellation)" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Leo (constellation)">Leo</a><span style="color: #274e13; font-size: 16px;">. </span></span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #274e13; font-size: 16px;">This galaxy group consists of the </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Spiral_galaxies" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Spiral galaxies">spiral galaxies</a><span style="color: #274e13; font-size: 16px;"> </span><a href="http://en.wikipedia.org/wiki/Messier_65" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Messier 65">M65</a><span style="color: #274e13; font-size: 16px;">, </span><a href="http://en.wikipedia.org/wiki/Messier_66" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="Messier 66">M66</a><span style="color: #274e13; font-size: 16px;">, and </span><a href="http://en.wikipedia.org/wiki/NGC_3628" style="background-image: none; color: #274e13; font-size: 16px; text-decoration: none;" title="NGC 3628">NGC 3628</a><span style="color: #274e13; font-size: 16px;">.</span></b></span></div>
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<span class="mw-headline" id="Members" style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Members</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">The table below lists galaxies that have been consistently identified as group members in the Nearby Galaxies Catalog,<sup class="reference" id="cite_ref-nbg_3-1" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-nbg-3" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[3]</a></sup> the Lyons Groups of Galaxies (LGG) Catalog,<sup class="reference" id="cite_ref-garcia1993_1-5" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-garcia1993-1" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[1]</a></sup> and the group lists created from the Nearby Optical Galaxy sample of Giuricin et al.<sup class="reference" id="cite_ref-giuricinetal2002_2-6" style="line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-giuricinetal2002-2" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></div>
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<table cellpadding="2" class="wikitable" style="border-collapse: collapse; border: 1px solid rgb(170, 170, 170); color: #073763; font-size: 16px; line-height: 19.2000007629395px; margin: 1em 0px; text-align: center;"><caption style="font-weight: bold;"><b><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Members of the Leo Triplet</span></b></caption><tbody>
<tr><th style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Name</span></th><th style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Galaxy_morphological_classification" style="background-image: none; color: #274e13; text-decoration: none;" title="Galaxy morphological classification">Type</a><sup class="reference" id="cite_ref-ned_6-0" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-ned-6" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[6]</a></sup></span></th><th style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Right_Ascension" style="background-image: none; color: #274e13; text-decoration: none;" title="Right Ascension">R.A.</a> (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-image: none; color: #274e13; text-decoration: none;" title="J2000">J2000</a>)<sup class="reference" id="cite_ref-ned_6-1" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-ned-6" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[6]</a></sup></span></th><th style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-image: none; color: #274e13; text-decoration: none;" title="Declination">Dec.</a> (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-image: none; color: #274e13; text-decoration: none;" title="J2000">J2000</a>)<sup class="reference" id="cite_ref-ned_6-2" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-ned-6" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[6]</a></sup></span></th><th style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Redshift" style="background-image: none; color: #274e13; text-decoration: none;" title="Redshift">Redshift</a> (km/<a href="http://en.wikipedia.org/wiki/Second" style="background-image: none; color: #274e13; text-decoration: none;" title="Second">s</a>)<sup class="reference" id="cite_ref-ned_6-3" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-ned-6" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[6]</a></sup></span></th><th style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Apparent_Magnitude" style="background-image: none; color: #274e13; text-decoration: none;" title="Apparent Magnitude">Apparent Magnitude</a><sup class="reference" id="cite_ref-ned_6-4" style="font-weight: normal; line-height: 1em; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_Triplet#cite_note-ned-6" style="background-image: none; color: #274e13; text-decoration: none; white-space: nowrap;">[6]</a></sup></span></th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Messier_65" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 65"><span style="font-family: Arial, Helvetica, sans-serif;">M65</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">SAB(rs)a</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">11<sup style="line-height: 1em;">h</sup> 18<sup style="line-height: 1em;">m</sup> 56.0<sup style="line-height: 1em;">s</sup></span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">+13° 05′ 32″</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">807 ± 3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">10.3</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Messier_66" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 66"><span style="font-family: Arial, Helvetica, sans-serif;">M66</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">SAB(s)b</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">11<sup style="line-height: 1em;">h</sup> 20<sup style="line-height: 1em;">m</sup> 15.0<sup style="line-height: 1em;">s</sup></span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">+12° 59′ 30″</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">727 ± 3</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">9.7</span></td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_3628" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 3628"><span style="font-family: Arial, Helvetica, sans-serif;">NGC 3628</span></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">SAb pec</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">11<sup style="line-height: 1em;">h</sup> 20<sup style="line-height: 1em;">m</sup> 17.0<sup style="line-height: 1em;">s</sup></span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">+13° 35′ 23″</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">843 ± 1</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">9.4</span></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;">2011 August 3</span><br /><a href="http://apod.nasa.gov/apod/image/1108/leotriplet_vst_4000.jpg" style="color: #073763; text-decoration: none;"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/1108/leotriplet_vst_900.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #faf2d9; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></span></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">The Leo Triplet Galaxies from VST </span></b><br /><b style="color: #274e13;">Image Credit: </b><a href="http://www.eso.org/" style="color: #274e13; text-decoration: none;">ESO</a><span style="color: #274e13;">, </span><a href="http://www.eso.org/public/images/eso1119c/" style="color: #274e13; text-decoration: none;">INAF-VST</a><span style="color: #274e13;">, </span><a href="http://www.astro-wise.org/~omegacam/index.shtml" style="color: #274e13; text-decoration: none;">OmegaCAM</a><span style="color: #274e13;">;</span><br /><i style="color: #274e13;">Acknowledgement: </i><a href="http://www.astro.rug.nl/~omegacen/" style="color: #274e13; text-decoration: none;">OmegaCen</a><span style="color: #274e13;">, </span><a href="http://www.astro-wise.org/" style="color: #274e13; text-decoration: none;">Astro-WISE</a><span style="color: #274e13;">, </span><a href="http://www.rug.nl/sterrenkunde/index" style="color: #274e13; text-decoration: none;">Kapteyn I.</a></span></center>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>This popular group is famous as the <a href="http://en.wikipedia.org/wiki/Leo_Triplet" style="color: #274e13; text-decoration: none;">Leo Triplet</a> - a gathering of three magnificent galaxies in one field of view. <a href="http://data.whicdn.com/images/4888787/tumblr_l7w5s18RbI1qctvlmo1_400_large.jpg" style="color: #274e13; text-decoration: none;">Crowd pleasers</a> when imaged with even modest telescopes, these galaxies can be introduced individually as <b>NGC 3628 (left), <a href="http://www.youtube.com/watch?v=IFcUNHJb_ic" style="color: #274e13; text-decoration: none;">M66</a>(bottom right), and M65 (top right)</b>. All three are large <a href="http://cassfos02.ucsd.edu/public/tutorial/Galaxies.html" style="color: #274e13; text-decoration: none;">spiral galaxies</a>. They tend to look dissimilar because their <a href="http://asterisk.apod.com/viewtopic.php?f=24&t=18005" style="color: #274e13; text-decoration: none;">galactic</a> disks are tilted at different angles to our line of sight. <a href="http://apod.nasa.gov/apod/ap050408.html" style="color: #274e13; text-decoration: none;">NGC 3628</a> is seen <a href="http://apod.nasa.gov/apod/ap010510.html" style="color: #274e13; text-decoration: none;">edge-on</a>, with obscuring dust lanes cutting across the plane of the galaxy, while the disks <a href="http://apod.nasa.gov/apod/ap101113.html" style="color: #274e13; text-decoration: none;">of M66</a> and <a href="http://apod.nasa.gov/apod/ap070601.html" style="color: #274e13; text-decoration: none;">M65 are</a> both inclined enough to show off their spiral structure. <a href="http://www.youtube.com/watch?v=xNBQTpdOFMk" style="color: #274e13; text-decoration: none;">Gravitational interactions</a> between galaxies in the group have also left <a href="http://apod.nasa.gov/apod/ap070727.html" style="color: #274e13; text-decoration: none;">telltale</a> signs, including the <a href="http://apod.nasa.gov/apod/ap030607.html" style="color: #274e13; text-decoration: none;">warped</a> and inflated disk of NGC 3628 and the drawn out spiral arms of <a href="http://apod.nasa.gov/apod/ap100413.html" style="color: #274e13; text-decoration: none;">M66</a>. This <a href="http://www.eso.org/public/images/eso1126a/" style="color: #274e13; text-decoration: none;">gorgeous deep view</a> of the region was taken by the new <a href="http://en.wikipedia.org/wiki/VLT_Survey_Telescope" style="color: #274e13; text-decoration: none;">VLT Survey Telescope</a> (VST) and spans about one degree (two full moons) on the sky. The field covers over 500 thousand <a href="http://chandra.harvard.edu/photo/cosmic_distance.html" style="color: #274e13; text-decoration: none;">light-years</a> at the trio's estimated distance of 30 million light-years.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://apod.nasa.gov/apod/ap110803.html">http://apod.nasa.gov/apod/ap110803.html</a></span></div>
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<h1>
The Leo Triplett (M66 group)</h1>
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<a href="http://messier.seds.org/Pics/More/m65-66mw.jpg" style="font-family: 'Times New Roman'; line-height: normal; text-align: start;"><img alt="[m65-66mw.jpg]" border="0" src="http://messier.seds.org/Pics/More/m65-66mw.jpg" style="text-align: right;" /></a><span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"></span><br />
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<span style="color: black; font-family: 'Times New Roman'; line-height: normal; text-align: start;"><span style="color: black; font-family: 'Times New Roman';">This small group of galaxies consists of the Messier objects </span><a href="http://messier.seds.org/m/m065.html">M65</a><span style="color: black; font-family: 'Times New Roman';"> (NGC 3623) and </span><a href="http://messier.seds.org/m/m066.html">M66</a><span style="color: black; font-family: 'Times New Roman';"> (NGC 3627) as well as the edge-on spiral </span><a href="http://messier.seds.org/xtra/ngc/n3628.html">NGC 3628</a><span style="color: black; font-family: 'Times New Roman';">. These three galaxies, the heart of the M66 group, form a beautiful and photogenic group which is frequently referred to as the Leo Triplett; Halton Arp has included this group as number 317 in his </span><a href="http://messier.seds.org/xtra/supp/m-arp.html">Catalogue of Peculiar Galaxies</a><span style="color: black; font-family: 'Times New Roman';"> (M66 is also Arp 16). Lying at a distance of some 35 million light years, it is probably physically related to the </span><a href="http://messier.seds.org/more/m096gr.html">M96 group</a><span style="color: black; font-family: 'Times New Roman';">.</span></span></div>
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The slightly more distant S0 or "early" Sa galaxy NGC 3593 is probably another member of the group, not in out image.</div>
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Our image was obtained by the German amateur <i>Michael Weiland</i> of the <i><a href="http://spider.seds.org/ig/ig.html">Interessengemeinschaft Astronomie</a></i> at the University of Constance.</div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://messier.seds.org/more/m066gr.html">http://messier.seds.org/more/m066gr.html</a></span></span><br />
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<a href="https://www.blogger.com/null" name="objlist" style="background-color: black; color: #ccccc0; font-family: 'Times New Roman'; line-height: normal; text-align: start;"></a></div>
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<h3>
Object list is sorted on RA or Longitude</h3>
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<pre><strong>
Row Object Name EquB1950.0 Object Velocity/Redshift Mag./ Separ. Number of Row
No. (* => Essential Note) RA DEC Type km/s z Qual Filter arcmin Refs Notes Phot Posn Vel/z Diam Assoc Images Spectra No.
</strong><a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=55565&objname=1&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">1 </a> MESSIER 065 11h16m19.3s +13d21m58s G 807 0.002692 10.25 ... <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Ref_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 388</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Note_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 10</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Photo_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 90</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Posn_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 6</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=z_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 11</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Diam_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 8</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Assoc_id&objid=55565&objname=MESSIER%20065&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 1</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/imgdata?objname=MESSIER+065&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/NEDspectra?objname=MESSIER+065&extend=never&detail=0&preview=1&numpp=20&refcode=ANY&bandpass=ANY&line=ANY&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=55565&objname=1&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">1 </a>
<a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=259317&objname=2&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">2 </a> *ARP 317 11h17m04.7s +13d28m09s GGroup 800 0.002668 ... ... <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Ref_id&objid=259317&objname=ARP%20317&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 31</a> 0 0 0 <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=z_id&objid=259317&objname=ARP%20317&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 2</a> 0 0 <a href="http://ned.ipac.caltech.edu/cgi-bin/imgdata?objname=ARP+317&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/NEDspectra?objname=ARP+317&extend=never&detail=0&preview=1&numpp=20&refcode=ANY&bandpass=ANY&line=ANY&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=259317&objname=2&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">2 </a>
<a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=55566&objname=3&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">3 </a> *MESSIER 066 11h17m38.4s +13d15m56s G 727 0.002425 9.65 ... <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Ref_id&objid=55566&objname=MESSIER%20066&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 917</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Note_id&objid=55566&objname=MESSIER%20066&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 26</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Photo_id&objid=55566&objname=MESSIER%20066&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 281</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Posn_id&objid=55566&objname=MESSIER%20066&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 10</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=z_id&objid=55566&objname=MESSIER%20066&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 14</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Diam_id&objid=55566&objname=MESSIER%20066&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 8</a> 0 <a href="http://ned.ipac.caltech.edu/cgi-bin/imgdata?objname=MESSIER+066&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/NEDspectra?objname=MESSIER+066&extend=never&detail=0&preview=1&numpp=20&refcode=ANY&bandpass=ANY&line=ANY&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=55566&objname=3&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">3 </a>
<a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=55567&objname=4&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">4 </a> NGC 3628 11h17m40.3s +13d51m49s G 843 0.002812 10.2B ... <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Ref_id&objid=55567&objname=NGC%203628&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 527</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Note_id&objid=55567&objname=NGC%203628&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 27</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Photo_id&objid=55567&objname=NGC%203628&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 190</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Posn_id&objid=55567&objname=NGC%203628&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 10</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=z_id&objid=55567&objname=NGC%203628&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 10</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Diam_id&objid=55567&objname=NGC%203628&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table" target="ned_dw"> 11</a> 0 <a href="http://ned.ipac.caltech.edu/cgi-bin/imgdata?objname=NGC+3628&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/NEDspectra?objname=NGC+3628&extend=never&detail=0&preview=1&numpp=20&refcode=ANY&bandpass=ANY&line=ANY&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">Retrieve</a> <a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=55567&objname=4&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1" target="ned_dw">4 </a></pre>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=Arp+317&extend=yes&out_csys=Equatorial&out_equinox=B1950.0&obj_sort=RA+or+Longitude&zv=z&zv_breaker=10000.0">http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=Arp+317&extend=yes&out_csys=Equatorial&out_equinox=B1950.0&obj_sort=RA+or+Longitude&zv=z&zv_breaker=10000.0</a></span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>AS GALÁXIAS NGC 3628 </b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>E MESSIER 65 E 66</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000; font-size: x-small;">NGC 3628</span></b><span style="color: #274e13;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #274e13;"> localizada a cerca de trinta e cinco milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #274e13;"> (aproximadamente 10,73 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-image: none; color: #274e13; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="color: #274e13;">) de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Le%C3%A3o" style="background-image: none; color: #274e13; text-decoration: none;" title="Constelação de Leão">constelação de Leão</a><span style="color: #274e13;">. Possui uma</span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #274e13; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #274e13;"> de 9,6, uma declinação de +13º 35' 20" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #274e13; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #274e13;"> de 11 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #274e13; text-decoration: none;" title="Hora">horas</a><span style="color: #274e13;">, 20 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #274e13; text-decoration: none;" title="Minuto">minutos</a><span style="color: #274e13;"> e 16,9 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #274e13; text-decoration: none;" title="Segundo">segundos</a><span style="color: #274e13;">.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">A galáxia NGC 3628 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/8_de_Abril" style="background-image: none; color: #274e13; text-decoration: none;" title="8 de Abril">8 de Abril</a> de <a href="http://pt.wikipedia.org/wiki/1784" style="background-image: none; color: #274e13; text-decoration: none;" title="1784">1784</a> por <a href="http://pt.wikipedia.org/wiki/William_Herschel" style="background-image: none; color: #274e13; text-decoration: none;" title="William Herschel">William Herschel</a>.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 19.2000007629395px;">http://pt.wikipedia.org/wiki/NGC_3628</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjZ9YEomVc5mBSQAibbJRrJAaCrLnO9VPEblH-ojGCLmYu10sY9NRBdDT4rZV7xW_93BTfwuMCmbsd0mbiJxj427vBdT2WpykY8NdAFpzqrW-zN3BoGytDXZPboQZbLHUp5e5AnwZxOe88/s1600/800px-NGC3628_Zoom.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjZ9YEomVc5mBSQAibbJRrJAaCrLnO9VPEblH-ojGCLmYu10sY9NRBdDT4rZV7xW_93BTfwuMCmbsd0mbiJxj427vBdT2WpykY8NdAFpzqrW-zN3BoGytDXZPboQZbLHUp5e5AnwZxOe88/s1600/800px-NGC3628_Zoom.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #faf2d9; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></span></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 19.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Ficheiro:NGC3628_Zoom.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Ficheiro:NGC3628_Zoom.jpg</a></span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Descrição</span></td><td class="description"><div class="description mw-content-ltr en" dir="ltr" lang="en" style="direction: ltr;" xml:lang="en">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span class="language en" title="">English:</span> NGC3628 Spiral Galaxy in Leo 11H20',+13°36') At 35.000.000 yl distant, this galaxy belong to the M66 - M65 group. a huge dust band is twisted because of attractions forces between them and dark it. 80'Luminance - 20'RGB- Bin.2X2 - STL11K - C14</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">04/10/08</span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><span class="int-own-work" style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Obra do próprio</span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><a href="http://commons.wikimedia.org/wiki/User:Fryns" style="background-image: none; color: #274e13; text-decoration: none;" title="User:Fryns"><span style="font-family: Arial, Helvetica, sans-serif;">Fryns</span></a></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b style="color: #660000;">Messier 65</b><span style="color: #660000;"><b> (</b></span><span style="color: #274e13;"><b><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 3623</a>)</b> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia">galáxia</a> <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">espiral</a> na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-image: none; color: #274e13; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Leo" style="background-image: none; color: #274e13; text-decoration: none;" title="Leo">Leo</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #274e13; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 11 <a href="http://pt.wikipedia.org/wiki/Horas" style="background-image: none; color: #274e13; text-decoration: none;" title="Horas">horas</a>, 18 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Minutos" style="background-image: none; color: #274e13; text-decoration: none;" title="Minutos">minutos</a> e 55.9 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Segundos" style="background-image: none; color: #274e13; text-decoration: none;" title="Segundos">segundos</a>, e uma <a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-image: none; color: #274e13; text-decoration: none;" title="Declinação">declinação</a> de +13º 05' 37".</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Junto com <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M66" style="background-image: none; color: #274e13; text-decoration: none;" title="M66">M66</a> e <a href="http://pt.wikipedia.org/wiki/NGC_3628" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 3628">NGC 3628</a>, formam o famoso <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Trio_Leo" style="background-image: none; color: #274e13; text-decoration: none;" title="Trio Leo">Trio Leo</a>, um pequeno <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Grupo_de_gal%C3%A1xias&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Grupo de galáxias (página não existe)">grupo de galáxias</a>.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia">galáxia</a> <b>M65</b> foi descoberta por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a>, em <a href="http://pt.wikipedia.org/wiki/1780" style="background-image: none; color: #274e13; text-decoration: none;" title="1780">1780</a>.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> foi descoberta pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a>, descobrindo na mesma ocasião <a href="http://pt.wikipedia.org/wiki/Messier_66" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 66">Messier 66</a>. Ambos foram<a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Catálogo Messier">catalogados</a> em 1 de março de 1780 e Messier descreveu M65 como uma "<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-image: none; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosa</a> muito tênue sem estrelas". Ao descrever a descoberta da galáxia, <a href="http://pt.wikipedia.org/wiki/William_Henry_Smyth" style="background-image: none; color: #274e13; text-decoration: none;" title="William Henry Smyth">William Henry Smyth</a> atribuiu erroneamente a descoberta de M65, M66 e <a href="http://pt.wikipedia.org/wiki/Messier_68" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 68">M68</a> ao amigo e colega de observatório de Messier, <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-image: none; color: #274e13; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, erro propagado historicamente mesmo em livros mais recentes.<span class="reference" id="cite_ref-seds_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_65#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></div>
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<span class="mw-headline" id="Caracter.C3.ADsticas" style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="font-size: small;">Características</span></span></h2>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia">galáxia</a>, juntamente com <a href="http://pt.wikipedia.org/wiki/Messier_66" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 66">Messier 66</a> e <a href="http://pt.wikipedia.org/wiki/NGC_3628" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 3628">NGC 3628</a>, formam um grupo galáctico, conhecido como o <a href="http://pt.wikipedia.org/wiki/Trio_do_Le%C3%A3o" style="background-image: none; color: #274e13; text-decoration: none;" title="Trio do Leão">Trio do Leão</a>, localizado a cerca de 35 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #274e13; text-decoration: none;" title="Terra">Terra</a>.</span></b><span style="color: #274e13;"> Embora esteja próximo de suas companheiras de grupo, ou seja, está ligada gravitacionalmente com os outros membros de seu grupo, a galáxia praticamente não tem alterações significativas em sua estrutura. Seu conjunto de braços é denso e seu </span><a href="http://pt.wikipedia.org/wiki/N%C3%BAcleo_gal%C3%A1ctico" style="background-image: none; color: #274e13; text-decoration: none;" title="Núcleo galáctico">núcleo galáctico</a><span style="color: #274e13;"> é lenticular e denso. Seu diâmetro aparente na </span><a href="http://pt.wikipedia.org/wiki/Esfera_celeste" style="background-image: none; color: #274e13; text-decoration: none;" title="Esfera celeste">esfera celeste</a><span style="color: #274e13;"> é de 8,5 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-image: none; color: #274e13; text-decoration: none;" title="Minuto de arco">minutos de grau</a><span style="color: #274e13;">, o que corresponde a um diâmetro real de 87 000 anos-luz.</span><span class="reference" id="cite_ref-seds_1-1" style="bottom: 1ex; color: #274e13; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_65#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Uma de suas principais características é a <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Nuvem_interestelar&action=edit&redlink=1" style="background-image: none; color: #274e13; text-decoration: none;" title="Nuvem interestelar (página não existe)">nuvem interestelar</a> que obscurece parcialmente a luminosidade da galáxia. Seu <a href="http://pt.wikipedia.org/wiki/Disco_gal%C3%A1ctico" style="background-image: none; color: #274e13; text-decoration: none;" title="Disco galáctico">disco</a> é constituído por uma população estelar velha, embora em sua borda seja possível visualizar lguns pontos azuis onda há <a href="http://pt.wikipedia.org/wiki/Forma%C3%A7%C3%A3o_estelar" style="background-image: none; color: #274e13; text-decoration: none;" title="Formação estelar">formação estelar</a>.<span class="reference" id="cite_ref-seds_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_65#cite_note-seds-1" style="background-image: none; color: #274e13; text-decoration: none;">1</a></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 19.2000007629395px;"><a href="http://pt.wikipedia.org/wiki/Messier_65">http://pt.wikipedia.org/wiki/Messier_65</a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">http://upload.wikimedia.org/wikipedia/commons/2/2a/Messier_65_Hubble_WikiSky.jpg</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Descrição</span></td><td class="description"><div class="description mw-content-ltr en" dir="ltr" lang="en" style="direction: ltr;">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span class="language en" title=""><b>English:</b></span> <a class="extiw" href="http://en.wikipedia.org/wiki/Messier_65" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Messier 65">en:Messier 65</a> spiral galaxy by <a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Hubble Space Telescope">en:Hubble Space Telescope</a>; 2.45′ view</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><time class="dtstart" datetime="2008-09-05" style="display: inline;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">5 de setembro de 2008</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; color: #274e13; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=11.315283115956627&de=13.095362894493123&angle=0.04080128137285874&projection=tan&rotation=-18.13684824546109&survey=astrophoto&img_id=60572%3Aall&width=1480&height=1480&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=zoom" rel="nofollow" style="color: #274e13; text-decoration: none;">[1]</a></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background-image: none; color: #274e13; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background-image: none; color: #274e13; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background-image: none; color: #274e13; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_perm" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Permissão</span></td><td><div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
<span style="font-family: Arial, Helvetica, sans-serif;">PD-HUBBLE</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">The 1st of March 1780 was a particularly productive night for Charles Messier. Combing the constellation of Leo for additions to his grand astronomical catalogue, he struck on not one, but two, new objects.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">One of those objects is seen here: Messier 65. <em style="border: 0px; margin: 0px; outline: 0px; padding: 0px; vertical-align: baseline;">"Nebula discovered in Leo: It is very faint and contains no star,"</em> he jotted down in his notebook. But he was wrong — as we now know, Messier 65 is a spiral galaxy containing billions upon billions of stars.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">All Messier saw was a faint diffuse light, nothing like the fine detail here, so we can forgive his mistake. If he had had access to a telescope like Hubble, he could have spied these stunning, tightly wound purple spiral arms and dark dust lanes, encircling a bright centre crammed with stars.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Almost exactly 233 years later in March of this year, one of the stars within Messier 65 <a href="http://messier.seds.org/more/m065_sn2013am.html" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">went supernova</a> (not seen in this image), rivalling the rest of the entire galaxy in brightness. This, the first Messier supernova of 2013, is now fading, and the serene beauty of M65 is returning.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://www.spacetelescope.org/" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">ESA/Hubble</a> & <a href="http://www.nasa.gov/" style="border: 0px; color: #274e13; margin: 0px; outline: 0px; padding: 0px; text-decoration: none; vertical-align: baseline;">NASA</a></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Supernova appears in M65</b></span></div>
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<b><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">BY MARK ARMSTRONG</span></b></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>ASTRONOMY NOW</b></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Posted: 17 April 2013</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">A very young core-collapse supernova burst forth on 21st March in the bright Messier galaxy Messier 65, surprisingly the first supernova to be discovered in that galaxy, raising hopes of a spectacular and pretty rare chance for amateur observers to follow its rise to brightness.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Read more http://www.astronomynow.com/news/n1304/17m65supernova/#.UyHYrj9dWL_</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Messier 66</span><span style="color: #274e13;"> (</span><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-image: none; color: #274e13; text-decoration: none;" title="New General Catalogue">NGC 3627</a></b><span style="color: #274e13;"><b>) </b>é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #274e13;"> localizada a cerca de trinta e cinco milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #274e13;"> (aproximadamente 10,73 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-image: none; color: #274e13; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="color: #274e13;">) de distância na direção da</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Le%C3%A3o" style="background-image: none; color: #274e13; text-decoration: none;" title="Constelação de Leão">constelação de Leão</a><span style="color: #274e13;">.</span><span class="reference" id="cite_ref-4" style="bottom: 1ex; color: #274e13; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_66#cite_note-4" style="background-image: none; color: #274e13; text-decoration: none;">4</a></span><span style="color: #274e13;"> Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #274e13; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #274e13;"> de 8,9, uma declinação de +12º 59' 28" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-image: none; color: #274e13; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #274e13;"> de 11 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-image: none; color: #274e13; text-decoration: none;" title="Hora">horas</a><span style="color: #274e13;">, 20 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-image: none; color: #274e13; text-decoration: none;" title="Minuto">minutos</a><span style="color: #274e13;"> e 15,1 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-image: none; color: #274e13; text-decoration: none;" title="Segundo">segundos</a><span style="color: #274e13;">.</span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">A galáxia NGC 3627 foi descoberta em <a href="http://pt.wikipedia.org/wiki/1780" style="background-image: none; color: #274e13; text-decoration: none;" title="1780">1780</a> por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a>.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 19.2000007629395px;">http://pt.wikipedia.org/wiki/Ficheiro:Messier_66_in_the_Leo_Triplet_(captured_by_the_Hubble_Space_Telescope).jpg</span></div>
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<table cellpadding="4" class="toccolours vevent mw-content-ltr" style="background-color: white; border: 1px solid rgb(170, 170, 170); color: #073763; direction: ltr; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 19.2000007629395px; padding: 5px; text-align: center; width: 1348px;"><tbody>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Descrição</span></td><td class="description"><div style="line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em;">
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a class="extiw" href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Hubble Space Telescope">Hubble</a> has snapped this view of <a class="extiw" href="http://en.wikipedia.org/wiki/Messier_66" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Messier 66">Messier 66</a>, the largest "player" of the <a class="extiw" href="http://en.wikipedia.org/wiki/Leo_Triplet" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Leo Triplet">Leo Triplet</a>, and a <a class="extiw" href="http://en.wikipedia.org/wiki/galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="en:galaxy">galaxy</a> with an unusual anatomy: it displays asymmetric spiral arms and an apparently displaced core. The peculiar anatomy is most likely caused by the gravitational pull of the other two members of the trio.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">The unusual <a class="extiw" href="http://en.wikipedia.org/wiki/spiral_galaxy" style="background-image: none; color: #274e13; text-decoration: none;" title="en:spiral galaxy">spiral galaxy</a>, Messier 66, is located at a distance of about 35 million light-years in the constellation of <a class="extiw" href="http://en.wikipedia.org/wiki/Leo_(constellation)" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Leo (constellation)">Leo</a>. Together with <a class="extiw" href="http://en.wikipedia.org/wiki/Messier_65" style="background-image: none; color: #274e13; text-decoration: none;" title="en:Messier 65">Messier 65</a> and <a class="extiw" href="http://en.wikipedia.org/wiki/NGC_3628" style="background-image: none; color: #274e13; text-decoration: none;" title="en:NGC 3628">NGC 3628</a>, Messier 66 is the member of the Leo Triplet, a trio of interacting spiral galaxies, part of the larger Messier 66 group. Messier 66 wins in size over its fellow triplets — it is about 100 000 light-years across.</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">This is a composite of images obtained through the following filters: 814W (near infrared), 555W (green) and H-alpha (showing the glowing of the hydrogen gas). They have been combined so to represent the real colors of the galaxy.</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Data</span></td><td><time class="dtstart" datetime="2010-04-08" style="display: inline;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">8 de abril de 2010</span></time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Origem</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a class="external free" href="http://www.spacetelescope.org/images/html/heic1006a.html" rel="nofollow" style="color: #274e13; text-decoration: none;">http://www.spacetelescope.org/images/html/heic1006a.html</a> (<a class="external text" href="http://www.spacetelescope.org/images/large/heic1006a.jpg" rel="nofollow" style="color: #274e13; text-decoration: none;">direct link</a>)</span></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 192.140625px;"><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Autor</span></td><td><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">NASA, ESA and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration</span></td></tr>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a> foi descoberta pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a>, descobrindo na mesma ocasião <a href="http://pt.wikipedia.org/wiki/Messier_65" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 65">Messier 65</a>. Ambos foram<a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-image: none; color: #274e13; text-decoration: none;" title="Catálogo Messier">catalogados</a> em 1 de março de 1780. Ao descrever a descoberta da galáxia, <a href="http://pt.wikipedia.org/wiki/William_Henry_Smyth" style="background-image: none; color: #274e13; text-decoration: none;" title="William Henry Smyth">William Henry Smyth</a> atribuiu erroneamente a descoberta de M65, M66 e <a href="http://pt.wikipedia.org/wiki/Messier_68" style="background-image: none; color: #274e13; text-decoration: none;" title="Messier 68">M68</a> ao amigo e colega de observatório de Messier, <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-image: none; color: #274e13; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, erro propagado historicamente mesmo em livros mais recentes.<span class="reference" id="cite_ref-seds_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_66#cite_note-seds-5" style="background-image: none; color: #274e13; text-decoration: none;">5</a></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><b>A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-image: none; color: #274e13; text-decoration: none;" title="Galáxia">galáxia</a>, juntamente com <span class="selflink">Messier 66</span> e <a href="http://pt.wikipedia.org/wiki/NGC_3628" style="background-image: none; color: #274e13; text-decoration: none;" title="NGC 3628">NGC 3628</a>, formam um grupo galáctico, conhecido como o <a href="http://pt.wikipedia.org/wiki/Trio_do_Le%C3%A3o" style="background-image: none; color: #274e13; text-decoration: none;" title="Trio do Leão">Trio do Leão</a></b>, localizado a cerca de 35 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-image: none; color: #274e13; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-image: none; color: #274e13; text-decoration: none;" title="Terra">Terra</a>. A galáxia é maior do que sua companheira de grupo, M65, e tem um <a href="http://pt.wikipedia.org/wiki/N%C3%BAcleo_gal%C3%A1ctico" style="background-image: none; color: #274e13; text-decoration: none;" title="Núcleo galáctico">núcleo galáctico</a> bem desenvolvido mas não muito definido. Seus braços parecem ser distorcidos e estão deslocados acima do <a href="http://pt.wikipedia.org/wiki/Plano_gal%C3%A1ctico" style="background-image: none; color: #274e13; text-decoration: none;" title="Plano galáctico">plano galáctico</a>.<span class="reference" id="cite_ref-seds_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_66#cite_note-seds-5" style="background-image: none; color: #274e13; text-decoration: none;">5</a></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Até o momento, quatro <a href="http://pt.wikipedia.org/wiki/Supernova" style="background-image: none; color: #274e13; text-decoration: none;" title="Supernova">supernova</a> foram encontradas na galáxia: SN 1973R, uma <a href="http://pt.wikipedia.org/wiki/Supernova_tipo_II" style="background-image: none; color: #274e13; text-decoration: none;" title="Supernova tipo II">supernova tipo II</a> que alcançou a <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-image: none; color: #274e13; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> 15, descoberta em 12 de dezembro de 1973; SN 1989B, descoberta em 31 de janeiro de 1989, alcançando a magnitude aparente 12,2; SN 1997bs, uma supernova tipo IIn descoberta por astrônomos no <a href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_Lick" style="background-image: none; color: #274e13; text-decoration: none;" title="Observatório Lick">observatório Lick</a>, alcançando a magnitude aparente 17; e SN 2009hd, descoberta por Berto Monard em 2 de julho de 2009, alcançando a magnitude aparente 15,8.<span class="reference" id="cite_ref-seds_5-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_66#cite_note-seds-5" style="background-image: none; color: #274e13; text-decoration: none;">5</a></span></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro -</span><br />
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">excerto da Carta Celeste sobre a constelação do Leão</span><br />
<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Cartas Celestes, As Constelações</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b> OBJETOS MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b> NO CENTRO DO CORPO DO LEÃO</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>- M95, M96 e M105</b></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m95atlas.jpg" /></div>
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http://www.ipac.caltech.edu/2mass/gallery/m95atlas.jpg</div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 95</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M95 (NGC 3351)</i>, type SBb, in <a href="http://messier.obspm.fr/map/Leo.html">Leo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m95.jpg"><img alt="[m95.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m95.jpg" style="text-align: right;" /></a><br />
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<tr><th align="left">Right Ascension</th><td>10 : 44.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td>+11 : 42 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td>38000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td>9.7 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td>4.4x3.3 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.</div>
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Messier 95 (M95, NGC 3351) is a beautiful barred spiral galaxy situated in constellation Leo, and one of the fainter Messier Objects.</div>
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<a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> discovered M95, together with <a href="http://messier.obspm.fr/m/m096.html">M96</a>, March 20, 1781. Consequently, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included it in <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M95">his catalog</a> on March 24, 1781.</div>
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M95 is a barred spiral of type SBb, or SB(r)ab according to de Vaucouleurs' classification, with nearly circular arms. Alan Sandage, in the <i>Hubble Atlas of Galaxies</i>, calls it a "typical ringed galaxy". Its overall appearance is quite similar to <a href="http://messier.obspm.fr/m/m091.html">M91</a>except that M95 has more pronounced spiral structure.</div>
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M95 is a member of the <a href="http://messier.obspm.fr/more/m096gr.html">Leo I or M96 group</a>, which also contains M96, <a href="http://messier.obspm.fr/m/m105.html">M105</a> and a number of fainter galaxies.</div>
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<a href="http://messier.obspm.fr/m/m095.html">http://messier.obspm.fr/m/m095.html</a></div>
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<a href="http://www.ipac.caltech.edu/2mass/gallery/m96atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m96atlas.jpg</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a>
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<h1>
Messier 96</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> M96 (NGC 3368)</i>, type Sa, in <a href="http://messier.obspm.fr/map/Leo.html">Leo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m96.jpg"><img alt="[m96.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m96.jpg" style="text-align: right;" /></a><br />
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<tr><th align="left">Right Ascension</th><td>10 : 46.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td>+11 : 49 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td>38000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td>9.2 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td>6x4 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.</div>
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Messier 96 (M96, NGC 3368) is a conspicuous spiral galaxy in constellation Leo.</div>
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M96 is the brightest member of the Leo I group of galaxies, which is therefore also called the <a href="http://messier.obspm.fr/more/m096gr.html">M96 group</a>, and also includes <a href="http://messier.obspm.fr/m/m095.html">M95</a>, <a href="http://messier.obspm.fr/m/m105.html">M105</a> as well as a number of fainter galaxies.</div>
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<a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> discovered M96, together with M95, on March 20, 1781. Consequently, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included it in <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M96">his catalog</a> on March 24, 1781. It was among the first spirals that have been discovered, and listed by <a href="http://messier.obspm.fr/xtra/Bios/rosse.html">Lord Rosse</a> as one of 14 "spiral nebulae" discovered to 1850.</div>
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<a href="http://messier.obspm.fr/m/m096.html">http://messier.obspm.fr/m/m096.html</a></div>
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<span style="font-size: small; font-weight: normal;"><a href="http://www.ipac.caltech.edu/2mass/gallery/m105atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m105atlas.jpg</a></span></h1>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a></div>
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Messier 105</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Elliptical Galaxy</a> M105 (NGC 3379)</i>, type E1, in <a href="http://messier.obspm.fr/map/Leo.html">Leo</a></center>
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<a href="http://messier.obspm.fr/Jpg/m105.jpg"><img alt="[m105.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m105.jpg" style="text-align: right;" /></a><br />
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<tr><th align="left">Right Ascension</th><td>10 : 47.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td>+12 : 35 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td>38000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td>9.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td>2.0 (arc min)</td></tr>
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Discovered by Pierre Méchain in 1781.</div>
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Messier 105 (M105, NGC 3379) is the brightest elliptical galaxy in the Leo I or <a href="http://messier.obspm.fr/more/m096gr.html">M96 group</a> of galaxies, and as such approximately 38 million light years distant. It is of type E1, and often studied as a typical representative of elliptical galaxies; e.g., J.D. Wray's <i>Color Atlas of Galaxies</i> states: "This elliptical galaxy is a photometric standard for surface brightness distribution," and mentions the uniformity of color over the entire range of luminosity.</div>
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<a href="http://messier.obspm.fr/more/m105_hst.html">Investigations with the Hubble Space Telescope</a> of the central region of M105 have revealed that this galaxy contains a massive central object of about 50 million solar masses.</div>
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M105 was discovered by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> on March 24, 1781, even 3 days earlier than <a href="http://messier.obspm.fr/m/m101.html">M101</a>, but due to unknown reasons, although probably intended, not included in <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>'s published list. Méchain described this object in <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m105">his letter of May 6, 1783</a>. This <a href="http://messier.obspm.fr/addition.html">additional object</a> was included <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M105">in the Messier Catalog</a> by <a href="http://messier.obspm.fr/xtra/Bios/hogg.html">Helen B. Sawyer Hogg</a> in 1947, together with <a href="http://messier.obspm.fr/m/m106.html">M106</a> and <a href="http://messier.obspm.fr/m/m107.html">M107</a>. <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> had observed it on March 11, 1784, and <a href="http://messier.obspm.fr/xtra/similar/herschel.html">assigned it</a> his number H I.17.</div>
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<a href="http://messier.obspm.fr/m/m105.html">http://messier.obspm.fr/m/m105.html</a></div>
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The M96 group of galaxies</h1>
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<a href="http://messier.seds.org/Pics/Jpg/m96gr.jpg"><img alt="[M96 Group]" border="0" src="http://messier.seds.org/Pics/More/m96gr_s.jpg" style="text-align: right;" /></a><br />
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This conspicuous <a href="http://messier.seds.org/g-group.html">group of galaxies</a> contains 3 Messier objects (<a href="http://messier.seds.org/m/m095.html">M95</a>, <a href="http://messier.seds.org/m/m096.html">M96</a>, and <a href="http://messier.seds.org/m/m105.html">M105</a>), plus a larger number of fainter galaxies (including NGCs 3299, 3377, 3384, 3412 and 3489 as well as UGC 5889, which is also called NGC 3377A in the Sky Catalogue 2000.0). The Sc galaxy NGC 3389, which is in the same field and close to M105, is probably a background galaxy, as its redshift corresponds to a receding velocity of 1138 km/sec, whereas the members of the Leo I group have radial velocities of only 449..766 km/sec.</div>
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In our image on the right hand side, M95 is in the lower right corner, while M96 is in the lower middle, and M105 is the bright elliptical galaxy above and left of the picture's center, together with its fainter neighbors NGC 3384 and faint NGC 3889.</div>
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The M96 group may be physically related to the <a href="http://messier.seds.org/more/m066gr.html">M66 group</a> which is roughly at the same distance and situated rather nearby in the sky.</div>
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LEIA MAIS</div>
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<a href="http://messier.seds.org/more/m096gr.html">http://messier.seds.org/more/m096gr.html</a></div>
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<img src="http://www.allthesky.com/constellations/leo/bigm.jpg" /></div>
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<a href="http://www.allthesky.com/constellations/leo/">http://www.allthesky.com/constellations/leo/</a></div>
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<a href="http://www.allthesky.com/copyright.html" style="font-style: italic;" target="_parent">© all photographs</a><span style="color: white; font-style: italic;"> taken by </span><a href="mailto:credner@allthesky.de" style="font-style: italic;">Till Credner</a><span style="color: white; font-style: italic;"> and </span><a href="mailto:kohle@allthesky.de" style="font-style: italic;">Sven Kohle</a></div>
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<a href="http://www.allthesky.com/constellations/leo/">http://www.allthesky.com/constellations/leo/</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;"><span style="font-size: large;"><span style="line-height: 22.3999996185303px; text-align: start;">The </span><span style="line-height: 22.3999996185303px; text-align: start;">M96 Group</span><span style="line-height: 22.3999996185303px; text-align: start;"> (also known as the </span><i style="line-height: 22.3999996185303px; text-align: start;">Leo I Group</i><span style="line-height: 22.3999996185303px; text-align: start;">)</span></span></span><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;"> is a </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Group_of_galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 16px; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Group of galaxies">group of galaxies</a><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;"> in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 16px; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;"> </span><a href="http://en.wikipedia.org/wiki/Leo_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 16px; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Leo (constellation)">Leo</a><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;">. This group contains between 8 and 24 galaxies, including three </span><a href="http://en.wikipedia.org/wiki/Messier_object" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 16px; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier object">Messier objects</a><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;">.</span><sup class="reference" id="cite_ref-garcia1993_1-3" style="color: #252525; font-size: 16px; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-giuricinetal2002_2-5" style="color: #252525; font-size: 16px; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup><sup class="reference" id="cite_ref-nbg_4-0" style="color: #252525; font-size: 16px; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-nbg-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup><sup class="reference" id="cite_ref-fouqueetal1992_3-1" style="color: #252525; font-size: 16px; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-fouqueetal1992-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;"> The group is one of many groups that lies within the </span><a href="http://en.wikipedia.org/wiki/Virgo_Supercluster" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 16px; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Virgo Supercluster">Virgo Supercluster</a><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;"> (i.e. the </span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Local_Supercluster" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 16px; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Local Supercluster">Local Supercluster</a><span style="color: #252525; font-size: 16px; line-height: 22.3999996185303px; text-align: start;">).</span><sup class="reference" id="cite_ref-tully1982_5-0" style="color: #252525; font-size: 16px; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-tully1982-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></b></span></div>
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<span style="line-height: 19px;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><a href="http://en.wikipedia.org/wiki/Leo_I_Group" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Leo_I_Group</a></b></span></span></div>
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<img alt="Local supercluster-ly.jpg" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Local_supercluster-ly.jpg/400px-Local_supercluster-ly.jpg" height="620" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; padding: 8px; text-align: -webkit-center;" width="640" /><br />
<span style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: -webkit-center;">http://en.wikipedia.org/wiki/Local_Supercluster#mediaviewer/File:Local_supercluster-ly.jpg</span><br />
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Local supercluster-ly</span></div>
<div class="mw-mmv-credit" style="background-color: white; color: #333333; font-family: sans-serif; font-size: 16px; line-height: 1.5em; overflow: hidden; padding: 5px 20px; text-align: center; text-overflow: ellipsis; white-space: nowrap;">
<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">NASA</span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/Image:Local_supercluster-ly.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:Image:Local supercluster-ly.jpg">English wikipedia</a></span></span></div>
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<table cellspacing="3" class="infobox" style="background-color: #f9f9f9; border-spacing: 3px; border: 1px solid rgb(170, 170, 170); clear: right; color: black; font-family: sans-serif; font-size: 12px; line-height: 1.5em; margin: 0.5em 0px 0.5em 1em; padding: 0.2em; text-align: center; width: 22em;"><tbody>
<tr><th colspan="2" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; font-size: 15px; text-align: center; vertical-align: top;"><span style="font-size: small;">M96 Group</span></th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><span style="font-size: small;"><a class="image" href="http://en.wikipedia.org/wiki/File:AnttlersM95-m96.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="AnttlersM95-m96.jpg" data-file-height="700" data-file-width="960" src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/a1/AnttlersM95-m96.jpg/350px-AnttlersM95-m96.jpg" height="255" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a1/AnttlersM95-m96.jpg/525px-AnttlersM95-m96.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a1/AnttlersM95-m96.jpg/700px-AnttlersM95-m96.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="350" /></a></span><br />
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<span style="font-size: small;"><a href="http://en.wikipedia.org/wiki/Messier_95" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 95">M95</a> (left) and <a href="http://en.wikipedia.org/wiki/Messier_96" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 96">M96</a> (right). Credit:Scott Anttila.</span></div>
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<tr><th colspan="2" style="background: rgb(235, 224, 70); text-align: center; vertical-align: top;"><span style="font-size: small;">Observation data (<a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">Epoch</a> <a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="J2000">J2000</a>)</span></th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constellation">Constellation(s)</a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Leo_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Leo (constellation)">Leo</a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Right ascension">Right ascension</a></th><td style="vertical-align: top;"><span style="font-size: small;"><sup class="reference" id="cite_ref-garcia1993_1-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-garcia1993-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-giuricinetal2002_2-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declination">Declination</a></th><td style="vertical-align: top;"><span style="font-size: small;"><sup class="reference" id="cite_ref-garcia1993_1-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-garcia1993-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-giuricinetal2002_2-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
<tr><th colspan="2" style="background: rgb(235, 224, 70); text-align: center; vertical-align: top;"><span style="font-size: small;">Other designations</span></th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><span style="font-size: small;">Leo I Group,<sup class="reference" id="cite_ref-fouqueetal1992_3-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-fouqueetal1992-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup> <a href="http://en.wikipedia.org/wiki/Lyons_Groups_of_Galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Lyons Groups of Galaxies">LGG</a> 217,<sup class="reference" id="cite_ref-garcia1993_1-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-garcia1993-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> NOGG H 507,<sup class="reference" id="cite_ref-giuricinetal2002_2-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup><br />NOGG P1 498,<sup class="reference" id="cite_ref-giuricinetal2002_2-3" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup> NOGG P2 507<sup class="reference" id="cite_ref-giuricinetal2002_2-4" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></span></td></tr>
</tbody></table>
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<table cellpadding="2" class="wikitable" style="background-color: #f9f9f9; border-collapse: collapse; border: 1px solid rgb(170, 170, 170); color: black; font-family: sans-serif; line-height: 22.3999996185303px; margin: 1em 0px; text-align: center;"><caption style="font-weight: bold;"><b>Members of the M96 Group</b></caption><caption style="font-weight: bold;"><b><br /></b></caption><tbody>
<tr><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Name</th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Galaxy_morphological_classification" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galaxy morphological classification">Type</a><sup class="reference" id="cite_ref-ned_6-0" style="font-weight: normal; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ned-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Right_Ascension" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Right Ascension">R.A.</a> (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="J2000">J2000</a>)<sup class="reference" id="cite_ref-ned_6-1" style="font-weight: normal; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ned-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declination">Dec.</a> (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="J2000">J2000</a>)<sup class="reference" id="cite_ref-ned_6-2" style="font-weight: normal; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ned-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Redshift" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Redshift">Redshift</a> (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/Kilometer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Kilometer">km</a>/<a href="http://en.wikipedia.org/wiki/Second" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Second">s</a>)<sup class="reference" id="cite_ref-ned_6-3" style="font-weight: normal; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ned-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Apparent_Magnitude" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Apparent Magnitude">Apparent Magnitude</a><sup class="reference" id="cite_ref-ned_6-4" style="font-weight: normal; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ned-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Messier_95" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 95"><b>M95</b></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SB(r)b</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 43<sup style="line-height: 1;">m</sup> 57.7<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+11° 42′ 14″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">778 ± 4</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">11.4</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Messier_96" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 96"><b>M96</b></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SAB(rs)ab</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 46<sup style="line-height: 1;">m</sup> 45.7<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+11° 49′ 12″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">897 ± 4</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10.1</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/Messier_105" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 105"><b>M105</b></a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">E1</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 47<sup style="line-height: 1;">m</sup> 49.6<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+12° 34′ 54″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">911 ± 2</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10.2</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_3299&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="NGC 3299 (page does not exist)">NGC 3299</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SAB(s)dm</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 36<sup style="line-height: 1;">m</sup> 23.8<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+12° 42′ 27″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">641 ± 6</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">13.3</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_3377" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 3377">NGC 3377</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">E5.5</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 47<sup style="line-height: 1;">m</sup> 42.4<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+13° 59′ 08″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">665 ± 2</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">11.2</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://en.wikipedia.org/wiki/NGC_3384" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 3384">NGC 3384</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SB(s)0</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 48<sup style="line-height: 1;">m</sup> 16.9<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+12° 37′ 46″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">704 ± 2</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10.9</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_3412&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="NGC 3412 (page does not exist)">NGC 3412</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SB(s)0</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10<sup style="line-height: 1;">h</sup> 50<sup style="line-height: 1;">m</sup> 53.3<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+13° 24′ 44″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">841 ± 2</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">11.5</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="new" href="http://en.wikipedia.org/w/index.php?title=NGC_3489&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="NGC 3489 (page does not exist)">NGC 3489</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SAB(rs)0</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">11<sup style="line-height: 1;">h</sup> 00<sup style="line-height: 1;">m</sup> 18.6<sup style="line-height: 1;">s</sup></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+13° 54′ 04″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">677 ± 2</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">11.1</td></tr>
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<b><span style="color: #660000;"><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">The </span><a href="http://en.wikipedia.org/wiki/Leo_Triplet" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Leo Triplet">Leo Triplet</a><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, which includes the spiral galaxies </span><a href="http://en.wikipedia.org/wiki/Messier_65" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 65">M65</a><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, </span><a href="http://en.wikipedia.org/wiki/Messier_66" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Messier 66">M66</a><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, and </span><a href="http://en.wikipedia.org/wiki/NGC_3628" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="NGC 3628">NGC 3628</a><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">,</span><sup class="reference" id="cite_ref-garcia1993_1-5" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-garcia1993-1" style="background: none; text-decoration: none; white-space: nowrap;">[1]</a></sup><sup class="reference" id="cite_ref-giuricinetal2002_2-7" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background: none; text-decoration: none; white-space: nowrap;">[2]</a></sup><sup class="reference" id="cite_ref-nbg_4-2" style="font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-nbg-4" style="background: none; text-decoration: none; white-space: nowrap;">[4]</a></sup></span></b><span style="font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"><b><span style="color: #660000;"> is located physically near the M96 Group</span><span style="color: #252525;">.</span></b></span><sup class="reference" id="cite_ref-ferrareseetal00_7-0" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ferrareseetal00-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> </span></div>
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<span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Some group identification algorithms actually identify the Leo Triplet at part of the M96 Group.</span><sup class="reference" id="cite_ref-giuricinetal2002_2-8" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup><sup class="reference" id="cite_ref-fouqueetal1992_3-3" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-fouqueetal1992-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup><span style="color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> The two groups may actually be separate parts of a much larger group.</span><sup class="reference" id="cite_ref-ferrareseetal00_7-1" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#cite_note-ferrareseetal00-7" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup></div>
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<a href="https://www.blogger.com/goog_2014696295"><br /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group">http://en.wikipedia.org/wiki/Leo_I_Group</a></span></div>
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<span style="line-height: 19px;"><b>LEIA MAIS SOBRE O GRUPO LEO</b></span></div>
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<span style="line-height: 19px;"><b>acessando</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: 19px;"><a href="http://www.beskeen.com/gallery/galaxy/m95m96m105.shtml" style="color: #274e13; text-decoration: none;">http://www.beskeen.com/gallery/galaxy/m95m96m105.shtml</a></span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/a/a1/AnttlersM95-m96.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><a href="http://en.wikipedia.org/wiki/Leo_I_Group#mediaviewer/File:AnttlersM95-m96.jpg">http://en.wikipedia.org/wiki/Leo_I_Group#mediaviewer/File:AnttlersM95-m96.jpg</a></span></div>
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">AnttlersM95-m96</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">Original uploader was <a class="extiw" href="http://en.wikipedia.org/wiki/User:Anttler" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="en:User:Anttler">Anttler</a> at <a class="external text" href="http://en.wikipedia.org/" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">en.wikipedia</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="text-align: start;"><span style="color: #660000;"><b>M95 and M96</b></span><span style="color: #252525;"> are both </span></span><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Spiral_galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Spiral galaxies">spiral galaxies</a><span style="color: #252525; text-align: start;"> 20 million light-years from Earth. Though they are visible as fuzzy objects in small telescopes, their structure is only visible in larger instruments. M95 is a </span><a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a><span style="color: #252525; text-align: start;">. M105 is about a degree away from the M95/M96 pair; it is an </span><a href="http://en.wikipedia.org/wiki/Elliptical_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-align: start; text-decoration: none;" title="Elliptical galaxy">elliptical galaxy</a><span style="color: #252525; text-align: start;"> of the 9th magnitude, also about 20 million light-years from Earth.</span><sup class="reference" id="cite_ref-FOOTNOTERidpathTirion2001166-168_1-6" style="color: #252525; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_(constellation)#cite_note-FOOTNOTERidpathTirion2001166-168-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://en.wikipedia.org/wiki/Leo_(constellation)">http://en.wikipedia.org/wiki/Leo_(constellation)</a></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">Messier 95 (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC</a> 3351)</span></b><span style="color: #252525;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #252525;"> localizada a cerca de trinta e oito milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525;"> (aproximadamente 11,65 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="color: #252525;">) de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_Le%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação de Leão">constelação de Leão</a><span style="color: #252525;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525;"> de 9,7, uma declinação de +11º 42' 13" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525;"> de 10 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a><span style="color: #252525;">, 43 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a><span style="color: #252525;"> e 57,7 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a><span style="color: #252525;">.</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A galáxia NGC 3351 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/20_de_Mar%C3%A7o" style="background: none; color: #0b0080; text-decoration: none;" title="20 de Março">20 de Março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background: none; color: #0b0080; text-decoration: none;" title="1781">1781</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>.</span></div>
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<span style="color: black; line-height: normal; text-align: center;"><span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://pt.wikipedia.org/wiki/Messier_95">http://pt.wikipedia.org/wiki/Messier_95</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhJxrq6inaLai0oFn0DBMlQILHPTpBENGG36r18yESQ90xb2VY1xXn3tXuB5GhnwdMZ7_t1yB8jey9Iayz0DN_ZyqJQr8A13nKuZm9MYIcyXMz2oSmd-evG9n4oNK30K4IJVg3Sdg-1CuU/s1600/800px-The_VLT_goes_lion_hunting.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhJxrq6inaLai0oFn0DBMlQILHPTpBENGG36r18yESQ90xb2VY1xXn3tXuB5GhnwdMZ7_t1yB8jey9Iayz0DN_ZyqJQr8A13nKuZm9MYIcyXMz2oSmd-evG9n4oNK30K4IJVg3Sdg-1CuU/s1600/800px-The_VLT_goes_lion_hunting.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_95#mediaviewer/Ficheiro:The_VLT_goes_lion_hunting.jpg">http://pt.wikipedia.org/wiki/Messier_95#mediaviewer/Ficheiro:The_VLT_goes_lion_hunting.jpg</a></span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">The VLT goes lion hunting</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">ESO</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/potw1212a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.eso.org/public/images/potw1212a/</a></span></span></div>
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<b><span style="color: #660000;">Messier 96 (<a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="New General Catalogue">NGC</a> 3368)</span></b><span style="color: #252525;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_espiral" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia espiral">galáxia espiral</a><span style="color: #252525;"> localizada a cerca de trinta e oito milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="color: #252525;"> (aproximadamente 11,65 </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="color: #252525;">) de distância na direção da </span><a href="http://pt.wikipedia.org/wiki/Leo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Leo">constelação do Leão</a><span style="color: #252525;">. Possui aproximadamente cem mil anos-luz de </span><a href="http://pt.wikipedia.org/wiki/Di%C3%A2metro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Diâmetro">diâmetro</a><span style="color: #252525;">, uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525;"> de 9,3, uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_absoluta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude absoluta">magnitude absoluta</a><span style="color: #252525;"> de -21,1, uma declinação de +11º 49' 25" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="color: #252525;"> de 10 </span><a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a><span style="color: #252525;"> 46 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto">minutos</a><span style="color: #252525;"> 45,9 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">segundos</a><span style="color: #252525;">.</span></div>
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A galáxia NGC 3368 foi descoberta em <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/20_de_Mar%C3%A7o" style="background: none; color: #0b0080; text-decoration: none;" title="20 de Março">20 de Março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background: none; color: #0b0080; text-decoration: none;" title="1781">1781</a> por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, na mesma ocasião descobriu-se a galáxia vizinha <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/M95" style="background: none; color: #0b0080; text-decoration: none;" title="M95">M95</a>. Esta galáxia pertence ao<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Grupo_de_Gal%C3%A1xias_Le%C3%A3o_I" style="background: none; color: #0b0080; text-decoration: none;" title="Grupo de Galáxias Leão I">Grupo de Galáxias Leão I</a>.</div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_96">http://pt.wikipedia.org/wiki/Messier_96</a></span></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiRLFJlX_bQCWONctHftkSRApq8pVsmw97jB-jp8wilLUPpdn_t_pStdBQPlp13WLcA0XQJ7ravnQOotJgKGhZ-d-0qydXFzLIJFqgTKbATzGXEzLgd_7MA7uKarzavGwjBxCNfZQmnnLI/s1600/800px-NGC_3368_ESO.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiRLFJlX_bQCWONctHftkSRApq8pVsmw97jB-jp8wilLUPpdn_t_pStdBQPlp13WLcA0XQJ7ravnQOotJgKGhZ-d-0qydXFzLIJFqgTKbATzGXEzLgd_7MA7uKarzavGwjBxCNfZQmnnLI/s1600/800px-NGC_3368_ESO.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_96#mediaviewer/Ficheiro:NGC_3368_ESO.jpg">http://pt.wikipedia.org/wiki/Messier_96#mediaviewer/Ficheiro:NGC_3368_ESO.jpg</a></span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">NGC 3368 ESO</span><a class="mw-mmv-license cc-license" href="http://creativecommons.org/licenses/by/3.0" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="_blank">CC BY 3.0</a></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">ESO/Oleg Maliy</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.eso.org/public/images/potw1143a/" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://www.eso.org/public/images/potw1143a/</a></span></span></div>
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<span style="color: #660000;"><b>Messier 105 (também conhecida como M105 e NGC 3379)</b></span><span style="color: #252525;"> é uma <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a> na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Leo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Leo">Leo</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">declinação</a> de +12° 34' 54" e uma<a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 10 <a href="http://pt.wikipedia.org/wiki/Horas" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Horas">horas</a>, 47 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Minutos" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minutos">minutos</a> e 49.6 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Segundos" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundos">segundos</a>.</span></div>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia">galáxia</a> <b>M105</b> foi descoberta por <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, em <a href="http://pt.wikipedia.org/wiki/24_de_mar%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="24 de março">24 de março</a> de <a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1781">1781</a>.</div>
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A <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_el%C3%ADptica" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia elíptica">galáxia elíptica</a> situa-se a uma distância de aroximadamente 38 milhões de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> em relação à <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e é a galáxia elíptica mais brilhante de seu grupo galáctico, o <a href="http://pt.wikipedia.org/wiki/Grupo_M96" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grupo M96">grupo M96</a>.<span class="reference" id="cite_ref-seds_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_105#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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Sua região central contém um <a href="http://pt.wikipedia.org/wiki/Buraco_negro_supermaci%C3%A7o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Buraco negro supermaciço">buraco negro supermaciço</a> com massa equivalente a 50 milhões de vezes a <a href="http://pt.wikipedia.org/wiki/Massa_solar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Massa solar">massa solar</a>. Se afasta radialmente da Terra a uma velocidade de 752 km/s.<span class="reference" id="cite_ref-seds_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_105#cite_note-seds-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></div>
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<span style="color: #252525; font-family: sans-serif;"><span style="line-height: 22.3999996185303px;"><a href="http://pt.wikipedia.org/wiki/Messier_105">http://pt.wikipedia.org/wiki/Messier_105</a></span></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif;"><br /></span><span lang="EN-US" style="font-family: Arial, sans-serif;"><br /></span><span lang="EN-US" style="font-family: Arial, sans-serif;"><img src="http://upload.wikimedia.org/wikipedia/commons/5/5e/Local_supercluster.jpg" height="620" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><a href="http://pt.wikipedia.org/wiki/Superaglomerado_de_gal%C3%A1xias#mediaviewer/Ficheiro:Local_supercluster.jpg">http://pt.wikipedia.org/wiki/Superaglomerado_de_gal%C3%A1xias#mediaviewer/Ficheiro:Local_supercluster.jpg</a></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Local supercluster</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author">NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://en.wikipedia.org/wiki/Image:Local_supercluster.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://en.wikipedia.org/wiki/Image:Local_supercluster.jpg</a> / <a class="external free" href="http://heasarc.nasa.gov/docs/cosmic/local_supercluster.html" rel="nofollow" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;">http://heasarc.nasa.gov/docs/cosmic/local_supercluster.html</a></span></span></div>
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<span style="color: #660000; font-size: large;">Local Group</span></h1>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;">A collection of more than 40 galaxies, spread across a volume of space some 10 million light-years in diameter, of which our own </span><a href="http://www.daviddarling.info/encyclopedia/G/Galaxy.html" style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start; text-decoration: none;">Milky Way Galaxy</a><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;"> and the </span><a href="http://www.daviddarling.info/encyclopedia/A/Andromeda.html" style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start; text-decoration: none;">Andromeda Galaxy</a><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;"> are the dominant and central members. Both these two giant spirals have retinues of </span><a href="http://www.daviddarling.info/encyclopedia/S/satellite_galaxy.html" style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start; text-decoration: none;">satellite galaxies</a><span style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; text-align: start;">, which together account for most of the membership of the Local Group.</span></div>
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<tr><td><img alt="Local Group" src="http://www.daviddarling.info/images/Local_Group.jpg" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></td></tr>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small; font-weight: normal;">http://www.daviddarling.info/encyclopedia/L/LocalGroup.html</span></h1>
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<b><span style="background-color: white; color: #073763;"><span style="font-size: large;">galaxy</span></span></b></div>
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<b><span style="background-color: white; color: #073763;"><span style="font-size: large;">dec.</span></span></b></div>
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<b><span style="background-color: white; color: #073763;"><span style="font-size: large;">abs.<br />mag.</span></span></b></div>
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<b><span style="background-color: white; color: #073763;"><span style="font-size: large;">diameter<br />(lt. yr.)</span></span></b></div>
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<b><span style="background-color: white; color: #073763;"><span style="font-size: large;">rad. vel.<br />(km/s)*</span></span></b></div>
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<b><span style="background-color: white; color: #073763;"><span style="font-size: large;">distance<br />(lt. yr.)</span></span></b></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">Leo II</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">11:13.5</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">+22:10</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">dSph</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">-10.2</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">3,000</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">+36</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">670,000</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">Leo I</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">10:08.5</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">+12:18</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">dE3</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">-12.0</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">3,000</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">+60</span></span></div>
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<span style="background-color: white; color: #073763;"><span style="font-size: large;">820,000</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#mediaviewer/File:Ugc5470.jpg">http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#mediaviewer/File:Ugc5470.jpg</a></span><br />
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Ugc5470</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">Scott Anttila<a class="new" href="http://commons.wikimedia.org/w/index.php?title=User:Anttler&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="User:Anttler (page does not exist)">Anttler</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Own work</span></span></span></div>
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<span dir="auto">Leo I (dwarf galaxy)</span></h1>
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<a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#mw-navigation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"></a><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#p-search" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"></a></div>
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<tr><th colspan="2" style="background: rgb(102, 204, 0); font-size: 15px; text-align: center; vertical-align: top;">Leo I</th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><a class="image" href="http://en.wikipedia.org/wiki/File:Ugc5470.jpg" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Ugc5470.jpg" data-file-height="667" data-file-width="1000" src="http://upload.wikimedia.org/wikipedia/commons/thumb/2/29/Ugc5470.jpg/250px-Ugc5470.jpg" height="167" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/29/Ugc5470.jpg/375px-Ugc5470.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/29/Ugc5470.jpg/500px-Ugc5470.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a><br />
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Leo I appears as a faint patch to the right of the bright star, <a href="http://en.wikipedia.org/wiki/Regulus" style="background: none; color: #0b0080; text-decoration: none;" title="Regulus">Regulus</a>.</div>
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<tr><th colspan="2" style="background: rgb(102, 204, 0); text-align: center; vertical-align: top;">Observation data (<a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)#Julian_years_and_J2000" style="background: none; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">J2000</a> <a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background: none; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">epoch</a>)</th></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background: none; color: #0b0080; text-decoration: none;" title="Constellation">Constellation</a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Leo_(constellation)" style="background: none; color: #0b0080; text-decoration: none;" title="Leo (constellation)">Leo</a></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background: none; color: #0b0080; text-decoration: none;" title="Right ascension">Right ascension</a></th><td style="vertical-align: top;">10<sup style="line-height: 1;">h</sup> 08<sup style="line-height: 1;">m</sup> 27.4<sup style="line-height: 1;">s</sup><sup class="reference" id="cite_ref-ned_1-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background: none; color: #0b0080; text-decoration: none;" title="Declination">Declination</a></th><td style="vertical-align: top;">+12° 18′ 27″<sup class="reference" id="cite_ref-ned_1-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Redshift" style="background: none; color: #0b0080; text-decoration: none;" title="Redshift">Redshift</a></th><td style="vertical-align: top;">285 ± 2 km/<a href="http://en.wikipedia.org/wiki/Second" style="background: none; color: #0b0080; text-decoration: none;" title="Second">s</a><sup class="reference" id="cite_ref-ned_1-2" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Cosmic_distance_ladder" style="background: none; color: #0b0080; text-decoration: none;" title="Cosmic distance ladder">Distance</a></th><td style="vertical-align: top;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/1_E21_m" style="background: none; color: #0b0080; text-decoration: none;" title="1 E21 m">820 ± 70</a> <a href="http://en.wikipedia.org/wiki/Light-year" style="background: none; color: #0b0080; text-decoration: none;" title="Light-year">kly</a> (250 ± 20<a href="http://en.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)<sup class="reference" id="cite_ref-karachentsevetal2004_2-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-karachentsevetal2004-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup><sup class="reference" id="cite_ref-Karachentsevetal2006_3-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-Karachentsevetal2006-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Galaxy_morphological_classification" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy morphological classification">Type</a></th><td style="vertical-align: top;">E;dSph<sup class="reference" id="cite_ref-ned_1-3" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Angular_diameter" style="background: none; color: #0b0080; text-decoration: none;" title="Angular diameter">Apparent dimensions</a> <small title="in visual light">(V)</small></th><td style="vertical-align: top;">9′.8 × 7′.4<sup class="reference" id="cite_ref-ned_1-4" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background: none; color: #0b0080; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a> <small title="in visual light">(V)</small></th><td style="vertical-align: top;">11.2<sup class="reference" id="cite_ref-ned_1-5" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background: inherit; vertical-align: top;">Notable features</th><td style="vertical-align: top;">Milky Way satellite</td></tr>
<tr><th colspan="2" style="background: rgb(102, 204, 0); text-align: center; vertical-align: top;">Other designations</th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="Uppsala General Catalogue">UGC</a> 5470,<sup class="reference" id="cite_ref-ned_1-6" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> <a href="http://en.wikipedia.org/wiki/Principal_Galaxies_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="Principal Galaxies Catalogue">PGC</a> 29488,<sup class="reference" id="cite_ref-ned_1-7" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> <a href="http://en.wikipedia.org/wiki/David_Dunlap_Observatory_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="David Dunlap Observatory Catalogue">DDO</a> 74,<sup class="reference" id="cite_ref-ned_1-8" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup>A1006,<sup class="reference" id="cite_ref-ned_1-9" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> Harrington-Wilson #1,<sup class="reference" id="cite_ref-ned_1-10" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup> Regulus Dwarf<sup class="reference" id="cite_ref-ned_1-11" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-ned-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><td colspan="2" style="background: rgb(102, 204, 0); text-align: center; vertical-align: top;">See also: <a href="http://en.wikipedia.org/wiki/Galaxy" style="background: none; color: #0b0080; text-decoration: none;" title="Galaxy">Galaxy</a>, <a href="http://en.wikipedia.org/wiki/List_of_galaxies" style="background: none; color: #0b0080; text-decoration: none;" title="List of galaxies">List of galaxies</a></td></tr>
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<b>Leo I</b> is a <a href="http://en.wikipedia.org/wiki/Dwarf_spheroidal_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Dwarf spheroidal galaxy">dwarf spheroidal galaxy</a> in the <a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constellation">constellation</a> <a href="http://en.wikipedia.org/wiki/Leo_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Leo (constellation)">Leo</a>. At about 820,000 <a href="http://en.wikipedia.org/wiki/Light-year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light-year">light-years</a> distant, it is a member of the <a href="http://en.wikipedia.org/wiki/Local_Group" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Local Group">Local Group</a> of galaxies and is thought to be one of the most distant satellites of the <a href="http://en.wikipedia.org/wiki/Milky_Way" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Milky Way">Milky Way</a> galaxy. It was discovered in 1950 by <a href="http://en.wikipedia.org/wiki/Albert_George_Wilson" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Albert George Wilson">Albert George Wilson</a> on <a href="http://en.wikipedia.org/wiki/Photographic_plate" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Photographic plate">photographic plates</a> of the <a href="http://en.wikipedia.org/wiki/National_Geographic_Society_%E2%80%93_Palomar_Observatory_Sky_Survey" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="National Geographic Society – Palomar Observatory Sky Survey">National Geographic Society – Palomar Observatory Sky Survey</a>, which were taken with the 48-inch <a href="http://en.wikipedia.org/wiki/Schmidt_camera" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Schmidt camera">Schmidt camera</a> at <a href="http://en.wikipedia.org/wiki/Palomar_Observatory" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Palomar Observatory">Palomar Observatory</a>.<sup class="reference" id="cite_ref-SEDS_4-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-SEDS-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup><sup class="reference" id="cite_ref-Bergh_5-0" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-Bergh-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></div>
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<span class="mw-headline" id="Regulus"><span style="font-size: large;">Regulus</span></span></h2>
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Leo I is located only 12 <a href="http://en.wikipedia.org/wiki/Minute_of_arc" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minute of arc">arc minutes</a> from <a href="http://en.wikipedia.org/wiki/Regulus" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Regulus">Regulus</a>, the brightest star in the constellation. For that reason, the galaxy is sometimes called the <i>Regulus Dwarf</i>. Scattered light from the star makes studying the galaxy more difficult, and it was not until the 1990s that it was detected visually.<sup class="reference" id="cite_ref-SEDS_4-1" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-SEDS-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup><sup class="reference" id="cite_ref-Bergh_5-5" style="line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)#cite_note-Bergh-5" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></div>
<span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><a href="http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)">http://en.wikipedia.org/wiki/Leo_I_(dwarf_galaxy)</a></span><br />
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjtGEJJ7nvGzn-TWADsKUrmS7b6rqXp_z4FRCOg1vFY-t4LByBNSamK5OLmo4totGKX9j-W7zCuN23-sosKD0P7JmnrfnDflaQFvu4wmwl7J48E1jfrsbYrS1RplbXYGcvwZMUOR1S-1la_/s1600/leo1_aao_big.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjtGEJJ7nvGzn-TWADsKUrmS7b6rqXp_z4FRCOg1vFY-t4LByBNSamK5OLmo4totGKX9j-W7zCuN23-sosKD0P7JmnrfnDflaQFvu4wmwl7J48E1jfrsbYrS1RplbXYGcvwZMUOR1S-1la_/s1600/leo1_aao_big.jpg" height="468" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></div>
<span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif; font-size: 16px;"><a href="http://apod.nasa.gov/apod/ap991003.html">http://apod.nasa.gov/apod/ap991003.html</a></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Nearby Dwarf Galaxy Leo I </b><br /><b>Credit & Copyright: </b>David Malin (<a href="http://www.aao.gov.au/" style="color: #274e13; text-decoration: none;">AAO</a>), <a href="http://www.aao.gov.au/local/www/dfm/rights.html" style="color: #274e13; text-decoration: none;">AATB</a></span></center>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Explanation: </b>Leo I is a <a href="http://www.astro.uu.se/~ns/review.html" style="color: #274e13; text-decoration: none;">dwarf spheroidal galaxy</a> in the <a href="http://www.seds.org/messier/more/local.html" style="color: #274e13; text-decoration: none;">Local Group</a> of galaxies dominated by our <a href="http://apod.nasa.gov/apod/ap980523.html" style="color: #274e13; text-decoration: none;">Milky Way Galaxy</a> and <a href="http://apod.nasa.gov/apod/ap971101.html" style="color: #274e13; text-decoration: none;">M31</a>. Leo I is thought to be the most distant of the <a href="http://www.astro.uu.se/~ns/mwsat.html" style="color: #274e13; text-decoration: none;">eleven known small satellite galaxies</a> orbiting our <a href="http://apod.nasa.gov/apod/ap971229.html" style="color: #274e13; text-decoration: none;">Milky Way Galaxy</a>. Besides the <a href="http://apod.nasa.gov/apod/ap980124.html" style="color: #274e13; text-decoration: none;">LMC</a>and the <a href="http://apod.nasa.gov/apod/ap980125.html" style="color: #274e13; text-decoration: none;">SMC</a>, all Milky Way satellite galaxies are <a href="http://www.astro.uu.se/~ns/dsph.html" style="color: #274e13; text-decoration: none;">small, dim, dwarf spheroidals</a>, including the closest galaxy - the <a href="http://apod.nasa.gov/apod/ap970329.html" style="color: #274e13; text-decoration: none;">Sagittarius Dwarf</a>. Leo I is more distant than most of them, thought to be about 250 kpc away. Although very little star-forming gas is visible in <a href="http://www.aao.gov.au/local/www/dfm/aat051.html" style="color: #274e13; text-decoration: none;">Leo I</a>, analysis of <a href="http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1999ApJ...514..665G" style="color: #274e13; text-decoration: none;">star ages shows</a> that stars have formed as recently as a billion years ago.</span></div>
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<span style="color: #660000; font-size: large;">Leo I</span></h1>
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<span style="line-height: 22.3999996185303px;">A large, prominent group of predominantly </span><a href="http://www.daviddarling.info/encyclopedia/S/spiralgal.html" style="color: #274e13; line-height: 22.3999996185303px; text-decoration: none;">spiral galaxies</a><span style="line-height: 22.3999996185303px;"> in </span><a href="http://www.daviddarling.info/encyclopedia/L/Leo_constellation.html" style="color: #274e13; line-height: 22.3999996185303px; text-decoration: none;">Leo</a><span style="line-height: 22.3999996185303px;">. </span></div>
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<li style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px; margin: 0px 0px 0.25em; padding: 0px; text-align: center;"><b>It consists of two main subgroups: the M66 Group and the M96 Group.</b> The former lies about 35 million light-years away and is centered on the interacting spirals M65 (NGC 3623), M66 (NGC 3627), and the edge-on NGC 3628, also known as the Leo Triplet (see accompanying photo). Not far from the M66 Group, and almost certainly physically related to it, is the much larger M96 group dominated by M96 itself, about 41 million light-years away, M95, M105, and NGC 3384. Fainter members of the M96 Group include NGCs 3299, 3377, 3377A, 3384, 3412, and 3489. The slightly more distant S0 or early Sa galaxy NGC 3593 is probably also a member.</li>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"><br /></span></div>
<li style="color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 16px; line-height: 22.3999996185303px; margin: 0px 0px 0.25em; padding: 0px; text-align: center;">A <a href="http://www.daviddarling.info/encyclopedia/D/dwarf_spheroidal.html" style="color: #274e13; text-decoration: none;">dwarf spheroidal</a> (dE3) galaxy that, at a distance of about 880,000 light-years, is the most remote satellite galaxy of the Milky Way and hence also a member of the <a href="http://www.daviddarling.info/encyclopedia/L/LocalGroup.html" style="color: #274e13; text-decoration: none;">Local Group</a>. Discovered in 1950, it has a diameter of about 6,000 light-years. Because it lies close to<a href="http://www.daviddarling.info/encyclopedia/R/Regulus.html" style="color: #274e13; text-decoration: none;">Regulus</a> in the sky (making study of it difficult in the bright star's light) it is sometimes known as the <strong>Regulus Dwarf</strong>, and also catalogued as DDO 74, UGC 5470, and Harrington-Wilson 1.</li>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.daviddarling.info/encyclopedia/L/Leo_I.html">http://www.daviddarling.info/encyclopedia/L/Leo_I.html</a></span><br />
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The Leo I Group</h1>
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The Leo I group is a very famous group of galaxies because it contains a lot of bright galaxies. On the right is the M96 subgroup and on the left is the M66 subgroup which are connected to each other via NGC 3489 which lies between them.</div>
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<img alt="The Leo I Group" src="http://www.atlasoftheuniverse.com/galgrps/leoi.gif" height="480" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(250, 242, 217); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(241, 194, 50); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></div>
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<span style="color: #073763; font-size: 14px; line-height: 22.3999996185303px; text-align: start;"><span style="color: #252525; font-family: sans-serif;"><a href="http://www.atlasoftheuniverse.com/galgrps/leoi.html">http://www.atlasoftheuniverse.com/galgrps/leoi.html</a></span></span></div>
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The Galaxies of the Leo I Group</h2>
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This is a list of the main galaxies in the Leo I group. This group contains twelve galaxies with a diameter above thirty thousand light years.</div>
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<tr><td style="vertical-align: middle;"><pre><span style="font-size: large;"><span style="color: #073763;"> 1 2 3 4 5 6 7 8 9
Name Equatorial Blue Type Size Size RV Other
Coordinates Mag (') kly km/s Names
RA Dec
NGC 3239 10 25.1 +17 10 11.7 Irr 4.5 45 1078
NGC 3299 10 36.4 +12 42 14.1 SBd 1.9 20 977
PGC 31877 10 42.0 +12 20 16.8 S0 0.6 5 1116
</span><b><span style="color: #660000;">M95 10 44.0 +11 42 10.5 SBb 7.6 75 1117 NGC 3351
M96 10 46.8 +11 49 10.1 SBa 7.8 80 1237 NGC 3368</span></b><span style="color: #073763;">
PGC 83339 10 46.9 +13 00 17.3 Irr 1.2 10 1171
NGC 3377A 10 47.4 +14 04 14.3 SBm 1.8 20 905 UGC 5889
PGC 83341 10 47.5 +13 53 17.5 Sc 0.5 5 909
NGC 3377 10 47.7 +13 59 11.1 E 4.4 45 1026
</span><b><span style="color: #660000;">M105 10 47.8 +12 35 10.2 E 5.1 50 1217 NGC 3379</span></b><span style="color: #073763;">
NGC 3384 10 48.3 +12 38 10.8 E 5.4 55 1066
PGC 32348 10 48.9 +14 07 16.1 E? 0.8 10 973
UGC 5923 10 49.1 +06 55 14.1 Sa 0.9 10 1061
NGC 3412 10 50.9 +13 25 11.4 S0 3.7 40 1191
NGC 3489 11 00.3 +13 54 11.1 S0 3.5 35 1031
NGC 3593 11 14.6 +12 49 11.8 S0 5.2 55 969
</span><span style="color: #660000;"><b>M65 11 18.9 +13 06 10.2 SBa 9.1 95 1146 NGC 3623
M66 11 20.2 +13 00 9.6 SBb 8.7 90 1066 NGC 3627</b>
</span><span style="color: #073763;">NGC 3628 11 20.3 +13 35 10.3 Sb 12.9 130 1184
IC 2787 11 23.3 +13 38 16.0 Sc 0.8 10 1081
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<span style="color: #073763; line-height: 22.3999996185303px; text-align: start;"><span style="font-family: sans-serif;"><a href="http://www.atlasoftheuniverse.com/galgrps/leoi.html">http://www.atlasoftheuniverse.com/galgrps/leoi.html</a></span></span></div>
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<tr><th colspan="2" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">Properties of the Leo I Group</span></th></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="font-size: large;">Equatorial Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">RA=11h00m Dec=+13°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="font-size: large;">Galactic Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">l=235° b=+60°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="font-size: large;">Supergalactic Coordinates</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">L=95° B=-25°</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="font-size: large;">Distance to the centre of the group</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">35 million light years</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="font-size: large;">Number of large galaxies in the group</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">12</span></td></tr>
<tr><td style="border: 1px solid rgb(0, 102, 204); vertical-align: middle;"><span style="font-size: large;">Alternative names for the group</span></td><td class="center" style="border: 1px solid rgb(0, 102, 204); text-align: center; vertical-align: middle;"><span style="font-size: large;">M66/M96 Group</span></td></tr>
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<span style="font-family: sans-serif; font-size: 16px; line-height: 22.3999996185303px; text-align: start;"><a href="http://www.atlasoftheuniverse.com/galgrps/leoi.html">http://www.atlasoftheuniverse.com/galgrps/leoi.html</a></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">Existe também o chamado </span><span style="color: #660000;">Grupo Leo II</span><span style="color: #073763;">.</span></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>O Grupo Leo II encontra-se ainda além o Grupo Leo I</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>(que é bem mais próximo),</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>porém ambos situam-se numa mesma região.</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">Com o tempo, entrou em cena </span><span style="color: #660000;">Leo III</span><span style="color: #073763;">.</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">Com o tempo, entraram em cena </span><span style="color: #660000;">Aglomerados de galáxias</span><span style="color: #073763;">.</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">Com o tempo, entrou em cena o </span><span style="color: #660000;">Superaglomerado Leo</span><span style="color: #073763;">.</span></b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Com o tempo, e bem recentemente (agora, em setembro de 2014!),</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">entrou em cena </span><span style="color: #660000;">Laniakea</span><span style="color: #073763;">,</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">nosso novo endereço</span><span style="color: #073763;"> dentre as estrelas do céu que nos protege,</span></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #073763;">esse </span><span style="color: #660000;">Céu Imensurável</span><span style="color: #073763;">!</span></b></span></div>
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<span style="color: #073763;">S<span style="font-family: Arial, Helvetica, sans-serif;"><b>AIBA BEM MAIS</b></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>SOBRE A CONSTELAÇÃO DO LEÃO</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>acessando meu Trabalho</b></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>em</b></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><a href="http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/leo-o-leao.html">http://daterraaoceueaoinfinito.blogspot.com.br/2013/08/leo-o-leao.html</a></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><span style="line-height: 18px;">...............................................</span></span><br style="background-color: white; color: #073763; font-family: Arial, Tahoma, Helvetica, FreeSans, sans-serif; font-size: 14px; line-height: 19.6000003814697px;" /><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><span style="line-height: 18px;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><span style="line-height: 18px;"><br /></span></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif; font-size: 14px; line-height: 19.6000003814697px;"><span style="line-height: 18px;"><br /></span></span><br />
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><br /><div class="MsoNormal" style="font-size: 16px; line-height: 22.3999996185303px;">
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><div style="font-family: 'Times New Roman'; font-size: medium; line-height: 18px;">
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<span style="color: #073763;"><span style="font-family: Arial, Helvetica, sans-serif;">Title: [The April, May & June Sky -- Virgo</span><span style="font-family: verdana, arial, georgia, sans-serif;">, Leo, Libra, Leo Minor, Ursa Major, Argo Navis, The Centaur, Hydra, Crater, Curvus Noctus, Boots, Bernices Hair, Asterion . . . ] </span></span><span style="color: #073763; font-family: verdana, arial, georgia, sans-serif;">Map Maker: </span><a href="https://www.raremaps.com/gallery/browse/creator_id/808" style="background-color: white; border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: verdana, arial, georgia, sans-serif; text-decoration: none;">Elijah J. Burritt</a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-62686343940275143642014-09-06T08:32:00.001-07:002016-01-19T03:46:31.693-08:00Hydra<div class="MsoNormal">
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<span style="border-left-color: rgb(255, 255, 255); border-left-style: solid; border-left-width: 0px; border-right-color: rgb(255, 255, 255); border-right-style: solid; border-right-width: 0px; display: block; font-stretch: normal; padding: 0.5em 15px;"><a href="http://oceudomes.blogspot.com.br/2016/01/o-serpenteado-de-estrelinhas-formando.html" style="background-color: transparent; color: #783f04; font-size: 22px; font-stretch: normal; text-decoration: none;">O serpenteado de estrelinhas formando a constelação Hydra, </a></span><span style="border-left-color: rgb(255, 255, 255); border-left-style: solid; border-left-width: 0px; border-right-color: rgb(255, 255, 255); border-right-style: solid; border-right-width: 0px; display: block; font-stretch: normal; padding: 0.5em 15px;"><a href="http://oceudomes.blogspot.com.br/2016/01/o-serpenteado-de-estrelinhas-formando.html" style="background-color: transparent; color: #783f04; font-size: 22px; font-stretch: normal; text-decoration: none;">a Hidra Fêmea, </a></span><span style="border-left-color: rgb(255, 255, 255); border-left-style: solid; border-left-width: 0px; border-right-color: rgb(255, 255, 255); border-right-style: solid; border-right-width: 0px; display: block; font-stretch: normal; padding: 0.5em 15px;"><a href="http://oceudomes.blogspot.com.br/2016/01/o-serpenteado-de-estrelinhas-formando.html" style="background-color: transparent; color: #783f04; font-size: 22px; font-stretch: normal; text-decoration: none;">e acolhendo seus três Objetos Messier</a></span></h2>
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<span style="font-family: arial, helvetica, sans-serif;">Olá!</span><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span><div align="left" class="MsoNormal" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 16.8pt; margin-bottom: 0.0001pt;">
<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: Arial, sans-serif; font-size: 12pt;">Caro Leitor,</span><span style="font-family: Arial, sans-serif; font-size: 12pt;"><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">a constelação da Hidra Fêmea, Hydra, é composta por estrelinhas bem tímidas</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">- com a boa exceção de sua estrela-alpha Alphard! -,</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">que vão desenhando a figura de um longo corpo<o:p></o:p></span></span></div>
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<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: Arial, sans-serif; font-size: 12pt;">enrolando-se</span><span style="font-family: Arial, sans-serif; font-size: 12pt;"> <span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">e enredilhando-se e serpenteando<o:p></o:p></span></span></div>
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<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: Arial, sans-serif; font-size: 12pt;"> através um longo espaço dos céus estrelados!</span><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></div>
<div align="left" class="MsoNormal" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; line-height: 16.8pt; margin-bottom: 0.0001pt;">
<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: Arial, sans-serif; font-size: 12pt;">- quase como que realizando uma linha divisória</span><span style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></div>
<span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; font-family: Arial, sans-serif; font-size: 12pt;"> entre algumas constelações do Zodíaco</span><span style="font-family: Arial, sans-serif; font-size: 12pt;"><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">- Virgem, Leão e Caranguejo -</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">(com o Corvo e a Taça e o Sextante colados ao corpo da Hidra</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">voltado para o norte)</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">e constelações mais ao sul</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">- Centauro, Lobo, Navio (Quilha, Popa e Vela)</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">(com as constelações Máquina Pneumática (Antlia) e Bússola (Pyxis)</span><br /><span style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">coladas ao corpo da Hidra voltado para o sul)!</span><br /></span></div>
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<br /><span style="font-family: arial, helvetica, sans-serif;">É sempre uma emoção podermos visualizar a Hydra por inteiro e a olho nú...,</span><br /><span style="font-family: arial, helvetica, sans-serif;">afinal, é maior constelação em termos de área ocupada!</span><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span><span style="font-family: arial, helvetica, sans-serif;">No entanto, é sempre importante que estejamos sob céus escuros e transparentes</span><br /><span style="font-family: arial, helvetica, sans-serif;">e em noites de ausência de Lua</span><b style="font-family: arial, helvetica, sans-serif;">!</b><br /><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span><br /><div class="separator" style="clear: both; text-align: center;">
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<span style="font-family: arial, helvetica, sans-serif;">Stellarium</span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>É sempre bem interessante que possamos divisar</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>a Cabeça da Hidra</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>que se posiciona um tantinho ao sul da tímida constelação do Caranguejo</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>- onde podemos também divisar a olho nú, usando nossa visão enviesada,</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>a Colmeia de Abelhas ou Presépio ou Objeto Messier 44 ou Manjedoura</b></span></div>
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<span style="color: #073763; font-family: arial, helvetica, sans-serif;"><b>ou Berçário de Estrelas!</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Stellarium</span></div>
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<b><span style="font-family: arial, sans-serif;">A Cabeça da Hydra</span><span style="font-family: arial, sans-serif;"> é considerada como um Asterismo </span></b></div>
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<span style="font-family: arial, sans-serif;"><b>formado pelas estrelas Epsilon, Delta, Zeta, Ro, Eta, Sigma </b></span></div>
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<span style="font-family: arial, sans-serif;"><b>e suas magnitudes vão desde quase 4,</b></span></div>
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<span style="font-family: arial, sans-serif;"><b>passando por 5 e por 6 e 12 e ainda além.<o:p></o:p></b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Certamente, após termos divisado o objeto celeste Presépio</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>e, um tantinho ao sul, o Asterismo formando a cabeça da Hidra,</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>nos deixamos encantar diante de</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>o coração da Hydra sugerido pela estrela-alpha Hydrae, Alphard,</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>maravilhosamente amarelada/alaranjada e esmaecida </b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>- porém a mais brilhante</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>de toda esta longa constelação!</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span><span style="font-family: arial, helvetica, sans-serif;"><br /></span><span style="font-family: arial, helvetica, sans-serif;"><br /></span><br /><div class="separator" style="clear: both; text-align: center;">
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<span style="font-family: arial, helvetica, sans-serif;">Stellarium</span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Como você poderá perceber,</span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Caro Leitor,</span><br /><span style="font-family: arial, helvetica, sans-serif;">a constelação da Hydra é composta por estrelinhas bem tímidas</span><br /><span style="font-family: arial, helvetica, sans-serif;">- com a boa exceção de sua estrela-alpha Alphard, é claro! -,</span><br /><span style="font-family: arial, helvetica, sans-serif;">que vão desenhando a figura de um longo corpo enrolando-se</span><br /><span style="font-family: arial, helvetica, sans-serif;">e enredilhando-se através um longo espaço dos céus estrelados!</span><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span><span style="font-family: arial, helvetica, sans-serif;">Porém, certamente a Hydra nos surpreende imensamente</span><br /><span style="font-family: arial, helvetica, sans-serif;">pelo fato de acolher Objetos Celestes tão inusitados, digamos assim,</span><br /><span style="font-family: arial, helvetica, sans-serif;">como o Fantasma de Júpiter e como a Dança Cósmica!</span><br /><span style="font-family: arial, helvetica, sans-serif;">(Confira em nossas Postagens anteriores:</span><br /><span style="font-family: arial, helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com.br/2016/01/o-fantasma-de-jupiter-ngc-3242.html" style="color: #274e13; text-decoration: none;">http://oceudomes.blogspot.com.br/2016/01/o-fantasma-de-jupiter-ngc-3242.html</a></span><br /><span style="font-family: arial, helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com.br/2016/01/a-danca-cosmica-realizada-pela.html" style="color: #274e13; text-decoration: none;">http://oceudomes.blogspot.com.br/2016/01/a-danca-cosmica-realizada-pela.html</a> )</span><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span><span style="font-family: arial, helvetica, sans-serif;"><b>Nesta Postagem,</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>estaremos comentando </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>sobre a constelação da Hydra e suas estrelas</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>e seus Objetos Messier </b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>(M48, M68 e M83)</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Boa Observação e Bons Estudos!</span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Janine Milward</span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><a href="http://www.raremaps.com/gallery/detail/28800/Hydra_Stars_heightened_in_gold/Hevelius.html" style="color: #274e13; text-decoration: none;">http://www.raremaps.com/gallery/detail/28800/Hydra_Stars_heightened_in_gold/Hevelius.html</a></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><strong style="text-align: start;">ap Maker: </strong><span style="text-align: start;"></span><a href="https://www.raremaps.com/gallery/browse/creator_id/2813" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; text-align: start; text-decoration: none;">Johannes Hevelius</a></span></div>
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<span style="font-family: 'helvetica neue', helvetica, arial, sans-serif;"><span style="line-height: 21px;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></span></div>
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<span style="font-family: arial, sans-serif;"><span style="color: #660000;"><b>HYDRA, </b></span></span></div>
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<span style="font-family: arial, sans-serif;"><span style="color: #660000;"><b>A HIDRA FÊMEA</b></span><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Ascensão Reta 8h8m / 14h58m Declinação +6<sup>o</sup>.8 / -35<sup>o</sup>.3<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Esta constelação representa a serpente marinha encontrada pelo Corvo </span><br /><span style="font-family: arial, sans-serif;">e usada como desculpa para que não tenha podido trazer a água na Taça </span><br /><span style="font-family: arial, sans-serif;">na missão solicitada por Apollo.<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Hydra é a mais longa constelação no céu </span><br /><span style="font-family: arial, sans-serif;">e também a maior em termos de área ocupada.<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;"> A cabeça da Hydra surge acima do equador em direção à constelação de Câncer, </span><br /><span style="font-family: arial, sans-serif;">o Caranguejo, </span><br /><span style="font-family: arial, sans-serif;">e seu corpo de cobra vai serpenteando através o céu do sul, </span><br /><span style="font-family: arial, sans-serif;">começando em Câncer e tendo o Leão ao norte, </span><br /><span style="font-family: arial, sans-serif;">depois o Sextante e então a Taça e o Corvo e ainda Virgem </span><br /><span style="font-family: arial, sans-serif;">até terminar sua cauda fina em Libra, a Balança. </span><br /><span style="font-family: arial, sans-serif;">Ao sul, a Hydra faz seus encontros com o Cão Menor, </span><br /><span style="font-family: arial, sans-serif;">o Monoceros, a Popa do Navio, o Peixe Austral, Antlia e o Centauro.<o:p></o:p></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">http://en.wikipedia.org/wiki/File:HydraCC.jpg</span></div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_desc" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.688px;">Description</td><td class="description"><div class="description mw-content-ltr en" dir="ltr" lang="en" style="direction: ltr;">
<span class="language en" title=""><b>English:</b></span> Photography of the constellation Hydra, the water snake</div>
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<span class="language de" title="Deutsch"><b>Deutsch:</b></span> Fotografie des Sternbildes Hydra, der Wasserschlange</div>
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<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_date" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.688px;">Date</td><td><time class="dtstart" datetime="2004-03-14" style="display: inline;">14 March 2004</time></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_src" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.688px;">Source</td><td><span class="int-own-work">Own work</span>: <a class="external text" href="http://www.allthesky.com/constellations/visualconstellations.html" rel="nofollow" style="color: #274e13; text-decoration: none;">AlltheSky.com</a></td></tr>
<tr style="vertical-align: top;"><td class="fileinfo-paramfield" id="fileinfotpl_aut" style="font-weight: bold; padding-right: 0.4em; text-align: right; width: 191.688px;">Author</td><td><a href="http://commons.wikimedia.org/wiki/User:Till_Credner" style="background-image: none; color: #0b0080; text-decoration: none;" title="User:Till Credner">Till Credner</a></td></tr>
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http://www.iau.org/static/public/constellations/gif/HYA.gif<br /><br /><br /><br /><br /></div>
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<span style="color: #660000; font-family: arial, sans-serif;"><b>Estrelas e objetos interessantes, em Hydra:</b><o:p></o:p></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Stellarium</span></div>
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<b><span style="font-family: arial, sans-serif;">A Cabeça da Hydra</span><span style="font-family: arial, sans-serif;"> é considerada como um Asterismo formado pelas estrelas Epsilon, Delta, Zeta, Ro, Eta, Sigma </span></b></div>
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<span style="font-family: arial, sans-serif;"><b>e suas magnitudes vão desde quase 4,</b></span></div>
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<span style="font-family: arial, sans-serif;"><b> passando por 5 e por 6 e 12 e ainda além.<o:p></o:p></b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>(Repare, Caro Leitor, que este Asterismo situa-se</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>imediatamente abaixo do belíssimo Presépio, em Cancer).</b></span></div>
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Stellarium</div>
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<span lang="EN-US" style="font-family: arial, sans-serif;"><b>Alphard</b></span><span lang="EN-US" style="font-family: arial, sans-serif;"><b>. Alpha Hidrae</b><o:p></o:p></span></div>
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<span lang="PT" style="font-family: arial, sans-serif;">Ascensão Reta 09h 26,6m - Declinação - 08<sup>o</sup> 35’<o:p></o:p></span></div>
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<span lang="PT" style="font-family: arial, sans-serif;">Magnitude visual 2,16 - distância 94 anos-luz<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Uma estrela laranja no pescoço da Hidra. De Al Fard al Shuja, A Estrela Solitária na Serpente. Freqüentemente chama de O Coração da Hidra.<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;"><b>U Hydrae - Estrela Variável Irregular</b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Ascensão Reta 10h35m Declinação -13<sup>o</sup>.07<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;"><b>R Hydrae - Estrela Variável</b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Ascensão Reta 13h26m Declinação -23<sup>o</sup>.01<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Magnitudes: Max 3,5 Min 10,9 Período 387,0<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;"><b>W Hydrae - Estrela Variável</b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Ascensão Reta 13h46m Declinação -28<sup>o</sup>.07<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Magnitudes: Max 6,5 Min 8,0 Período 380,0<o:p></o:p></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste</span><span style="font-family: arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></span></div>
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<span style="color: #274e13; font-family: arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-family: georgia, 'times new roman', times, serif; font-size: 14px;">"Hydra constellation map" por Hydra_constellation_map.png: Torsten Brongerderivative work: Kxx (talk) - Hydra_constellation_map.png. Licenciado sob CC BY-SA 3.0, via Wikimedia Commons - https://commons.wikimedia.org/wiki/File:Hydra_constellation_map.svg#/media/File:Hydra_constellation_map.svg</span></div>
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<span style="color: #660000; font-family: arial, helvetica, sans-serif;"><b>OS OBJETOS MESSIER</b></span><br /><span style="color: #660000; font-family: arial, helvetica, sans-serif;"><b>EM HYDRA</b></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="color: #274e13; text-decoration: none;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 48</h1>
<i><a href="http://messier.obspm.fr/cluster.html" style="color: #274e13; text-decoration: none;">Open Cluster</a> M48 (NGC 2548)</i>, type 'f', in <a href="http://messier.obspm.fr/map/Hya.html" style="color: #274e13; text-decoration: none;">Hydra</a></center>
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<tr><th align="left">Right Ascension</th><td align="center">08 : 13.8 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-05 : 48 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">1.5 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.5 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">54.0 (arc min)</td></tr>
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<br />Discovered 1771 by Charles Messier.<br /><br />Open cluster Messier 48 (M48, NGC 2548) is a conspicuous open cluster in the head of the extended constellation Hydra, almost on its border to Monoceros.<br /><br />This open cluster was discovered by <a href="http://messier.obspm.fr/xtra/history/biograph.html" style="color: #274e13; text-decoration: none;">Charles Messier</a> and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M48" style="color: #274e13; text-decoration: none;">cataloged by him</a> on February 19, 1771. However, as he did an error in data reduction, he gave a wrong position in his catalog so that the object was <a href="http://messier.obspm.fr/missing.html" style="color: #274e13; text-decoration: none;">missing</a> until <a href="http://messier.obspm.fr/xtra/Bios/thomas.html" style="color: #274e13; text-decoration: none;">Oswald Thomas</a>identified it in 1934, and independently <a href="http://messier.obspm.fr/xtra/Bios/morris.html" style="color: #274e13; text-decoration: none;">T.F. Morris</a> in 1959. The identification of M48 by Oswald Thomas was confused by some historians, who have claimed erroneously instead that he had identified M47. As M48 was lost, two independent rediscoveries occurred: First, <a href="http://messier.obspm.fr/xtra/Bios/bode.html" style="color: #274e13; text-decoration: none;">Johann Elert Bode</a> apparently found it in or before 1782, and second, <a href="http://messier.obspm.fr/xtra/Bios/cherschel.html" style="color: #274e13; text-decoration: none;">Caroline Herschel</a> independently <a href="http://messier.obspm.fr/xtra/similar/cher.html" style="color: #274e13; text-decoration: none;">rediscovered it</a> in 1783; this latter discovery was published by Caroline's famous brother, <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html" style="color: #274e13; text-decoration: none;">William Herschel</a>, who included it in <a href="http://messier.obspm.fr/xtra/similar/herschel.html" style="color: #274e13; text-decoration: none;">his catalog</a> as H VI.22 on February 1, 1786.<br /><br />.................................................<br />LEIA MAIS<br />em<br /><a href="http://messier.obspm.fr/m/m048.html" style="color: #274e13; text-decoration: none;">http://messier.obspm.fr/m/m048.html</a><br /><br /><br /><br /><br /><br /><div class="separator" style="clear: both;">
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<span style="font-family: arial, helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span lang="PT" style="color: #660000; font-family: arial, sans-serif;"><b>M 48 NGC 2548 Aglomerado Aberto</b></span><span lang="PT" style="font-family: arial, sans-serif;"><o:p></o:p></span></div>
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<span lang="PT" style="font-family: arial, sans-serif;">Um aglomerado aberto bem pálido porém grande</span><br /><span lang="PT" style="font-family: arial, sans-serif;"> e que pode ser resolvido através um par de binóculos.<o:p></o:p></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste</span><span style="font-family: arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></span></div>
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<span style="color: #274e13; font-family: arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<b>Messier 48</b>, também denominado <b>M48</b> e <b>NGC 2548</b>, é um <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado estelar aberto">aglomerado aberto</a> localizado a cerca de mil e quinhentos <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> de distância na direção da <a href="http://pt.wikipedia.org/wiki/Hydra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hydra">constelação da Hidra</a>. Possui uma <a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a> de +5,8, uma <a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">declinação</a> de -05º 45' 02" e uma <a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">ascensão reta</a> de 08 <a href="http://pt.wikipedia.org/wiki/Hora" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hora">horas</a> 13 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos</a> 43,1 <a href="http://pt.wikipedia.org/wiki/Segundo_de_arco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo de arco">segundos</a>.</div>
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Foi descoberto a <a href="http://pt.wikipedia.org/wiki/19_de_fevereiro" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="19 de fevereiro">19 de Fevereiro</a> de <a href="http://pt.wikipedia.org/wiki/1771" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1771">1771</a> por <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>. Trata-se de um objeto relativamente conspícuo e pode ser observado a <a href="http://pt.wikipedia.org/wiki/Vis%C3%A3o#A_olho_nu" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Visão">olho nu</a> sob boas condições. A sua idade é estimada em 300 milhões de <a href="http://pt.wikipedia.org/wiki/Ano" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ano">anos</a>.</div>
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<table cellpadding="0" cellspacing="2" class="infobox" style="background: rgb(242, 242, 242); border-collapse: collapse; border: 1px solid rgb(170, 170, 170); clear: right; color: #252525; font-family: sans-serif; font-size: 11px; margin: 0px 0px 1em 1em; padding: 0.2em; width: 250px;"><tbody>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 48</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_object_048.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 48, projeto 2MASS"><img alt="Messier 48, projeto 2MASS" data-file-height="1400" data-file-width="1000" height="350" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Messier_object_048.jpg/250px-Messier_object_048.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Messier_object_048.jpg/375px-Messier_object_048.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Messier_object_048.jpg/500px-Messier_object_048.jpg 2x" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a><br />Messier 48, projeto <a href="http://pt.wikipedia.org/wiki/2MASS" style="background: none; color: #0b0080; text-decoration: none;" title="2MASS">2MASS</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1771" style="background: none; color: #0b0080; text-decoration: none;" title="1771">1771</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Hydra" style="background: none; color: #0b0080; text-decoration: none;" title="Hydra">Hydra</a></td></tr>
<tr style="vertical-align: top;"><td>Tipo</td><td style="background-color: #f8f8f8;">I,2,r / I,3,r</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 13<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 43,18<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-5° 45' 1,6"</td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">1500 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a> (460 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">5,5</td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">54'</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">23 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a></td></tr>
<tr style="vertical-align: top;"><td>Idade estimada</td><td style="background-color: #f8f8f8;">300 milhões de anos</td></tr>
<tr style="vertical-align: top;"><td>Nº estrelas</td><td style="background-color: #f8f8f8;">80</td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">NGC 2548, C 0811-056, [KPR2004b] 189</td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 48"><img alt="Messier 48" data-file-height="15" data-file-width="15" height="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="15" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Hydra_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Hydra constellation map.png" data-file-height="1419" data-file-width="2559" height="139" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Hydra_constellation_map.png/250px-Hydra_constellation_map.png" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Hydra_constellation_map.png/375px-Hydra_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Hydra_constellation_map.png/500px-Hydra_constellation_map.png 2x" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a></div>
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<br /><a href="http://pt.wikipedia.org/wiki/Messier_48" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_48</a><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><br /><img src="http://www.ipac.caltech.edu/2mass/gallery/m68atlas.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br /><div>
<a href="http://www.ipac.caltech.edu/2mass/gallery/m68atlas.jpg" style="color: #274e13; text-decoration: none;">http://www.ipac.caltech.edu/2mass/gallery/m68atlas.jpg</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="color: #274e13; text-decoration: none;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 68</h1>
<i><a href="http://messier.obspm.fr/cluster.html" style="color: #274e13; text-decoration: none;">Globular Cluster</a> M68 (NGC 4590)</i>, class X, in <a href="http://messier.obspm.fr/map/Hya.html" style="color: #274e13; text-decoration: none;">Hydra</a></center>
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<a href="http://messier.obspm.fr/Jpg/m68.jpg" style="color: #274e13; text-decoration: none;"><img align="right" alt="[m68.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m68.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a><br /><table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">12 : 39.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-26 : 45 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">33.3 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">11.0 (arc min)</td></tr>
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<br /><br />Discovered 1780 by Charles Messier.<br /><br />Messier 68 (M68, NGC 4590) is a beautiful globular cluster situated in an unusual place for such objects, in the hemisphere opposite to the Galactic Center.<br />.....................................<br /><br />LEIA MAIS em<br /><br /><a href="http://messier.obspm.fr/m/m068.html" style="color: #274e13; text-decoration: none;">http://messier.obspm.fr/m/m068.html</a><br /><br /><br /><br /><div class="separator" style="clear: both;">
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgMoUBBLyBp5NNxUIUlL_nN_-Vloq8QDItZKL6TNSifIQ2Jdyq341sOnYpFqBtNQJ9hsqX7fFUVmxe6e7F8IvVGUtD-fJ4q_FLleGRnbJSKU5bizkkFHp4YxmMU29OfMl4nFxRKdg02VO0/s1600/m+68+..png" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgMoUBBLyBp5NNxUIUlL_nN_-Vloq8QDItZKL6TNSifIQ2Jdyq341sOnYpFqBtNQJ9hsqX7fFUVmxe6e7F8IvVGUtD-fJ4q_FLleGRnbJSKU5bizkkFHp4YxmMU29OfMl4nFxRKdg02VO0/s1600/m+68+..png" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-family: arial, helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: arial, sans-serif;"><b><span style="color: #660000;">NGC 4590 - M 68 - Aglomerado Globular Hydra</span></b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Ascensão Reta 12h38m Declinação -26<sup>o</sup>.38<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Magnitude fotográfica global 9,1 Diâmetro aparente 9’8 Tipo Espectral A6<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Distância kpc 11,5 Velocidade Radial (km/s) -111<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Situado a 3<sup>o</sup>. ao sul, cerca de 1<sup>o</sup>. a leste de Beta Corvii </span><br /><span style="font-family: arial, sans-serif;">e próximo de uma estrela de magnitude 5.</span><br /><span style="font-family: arial, sans-serif;"> Com magnitude visual de 7,5 e um diametro de 3’,</span><br /><span style="font-family: arial, sans-serif;">torna-se um objeto interessante para ser visto </span><br /><span style="font-family: arial, sans-serif;">com um telescópio de 5cm de abertura.</span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste</span><span style="font-family: arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></span></div>
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<span style="color: #274e13; font-family: arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="color: #274e13; font-family: arial, sans-serif;"><span style="line-height: 22.4px;"><a href="http://pt.wikipedia.org/wiki/Messier_68#mediaviewer/File:Messier_68_Hubble_WikiSky.jpg" style="color: #274e13; text-decoration: none;">http://pt.wikipedia.org/wiki/Messier_68#mediaviewer/File:Messier_68_Hubble_WikiSky.jpg</a></span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 68 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=12.6577842&de=-26.74335&angle=0.0553424&projection=tan&rotation=-38.5669&survey=astrophoto&img_id=60446&width=4000&height=4000&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=zoom" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<span style="font-size: 14px;"> </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a> foi descoberto pelo astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que o <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogou</a> em 9 de abril de 1780. Ao descrever a descoberta do aglomerado, <a href="http://pt.wikipedia.org/wiki/William_Henry_Smyth" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="William Henry Smyth">William Henry Smyth</a> atribuiu erroneamente a descoberta do objeto e também de <a href="http://pt.wikipedia.org/wiki/Messier_65" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 65">Messier 65</a> e <a href="http://pt.wikipedia.org/wiki/Messier_66" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier 66">Messier 66</a> ao amigo e colega de observatório de Messier, <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>.<span class="reference" id="cite_ref-seds_2-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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É vista como uma "mancha nebulosa" em <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Binóculo">binóculos</a> e suas estrelas mais brilhantes podem ser resolvidas com <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores de 4 polegadas de abertura ou mais. Telescópios de 6 polegadas de abrtura conseguem distinhuir seu halo, com 11 minutos de grau de diâmetro, e com 12 polegadas de abertura é possível distinguir as estrelas de seu núcleo.<span class="reference" id="cite_ref-seds_2-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 68</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_68_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 68 pelo Telescópio Espacial Hubble.NASA/STScI/WikiSky"><img alt="Messier 68 pelo Telescópio Espacial Hubble.NASA/STScI/WikiSky" data-file-height="4000" data-file-width="4000" height="250" src="http://upload.wikimedia.org/wikipedia/commons/thumb/c/c0/Messier_68_Hubble_WikiSky.jpg/250px-Messier_68_Hubble_WikiSky.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/c0/Messier_68_Hubble_WikiSky.jpg/375px-Messier_68_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/c0/Messier_68_Hubble_WikiSky.jpg/500px-Messier_68_Hubble_WikiSky.jpg 2x" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a><br />Messier 68 pelo <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a>.<br /><a href="http://pt.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="NASA">NASA</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=STScI&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="STScI (página não existe)">STScI</a>/<a class="new" href="http://pt.wikipedia.org/w/index.php?title=WikiSky&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="WikiSky (página não existe)">WikiSky</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1780" style="background: none; color: #0b0080; text-decoration: none;" title="1780">1780</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Hydra" style="background: none; color: #0b0080; text-decoration: none;" title="Hydra">Hydra</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">12<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 39<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 28,0<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background: none; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">-26° 44′ 38,6″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">33 300 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (10 200 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">9,67<span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">11 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-seds_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background: none; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">Classe</a></td><td style="background-color: #f8f8f8;">X<span class="reference" id="cite_ref-seds_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">53<span class="reference" id="cite_ref-seds_2-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M68, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 4590, GC1 20.<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_68#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 68"><img alt="Messier 68" data-file-height="15" data-file-width="15" height="12" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="12" /></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Hydra_constellation_map.png" style="background: none; color: #0b0080; text-decoration: none;"><img alt="Hydra constellation map.png" data-file-height="1419" data-file-width="2559" height="139" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Hydra_constellation_map.png/250px-Hydra_constellation_map.png" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Hydra_constellation_map.png/375px-Hydra_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Hydra_constellation_map.png/500px-Hydra_constellation_map.png 2x" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a><br /></div>
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<a href="http://www.ipac.caltech.edu/2mass/gallery/m83atlas.jpg" style="color: #274e13; text-decoration: none;">http://www.ipac.caltech.edu/2mass/gallery/m83atlas.jpg</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="color: #274e13; text-decoration: none;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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Messier 83</h1>
<i><a href="http://messier.obspm.fr/galaxy.html" style="color: #274e13; text-decoration: none;">Spiral Galaxy</a> M83 (NGC 5236)</i>, type SABc, in <a href="http://messier.obspm.fr/map/Hya.html" style="color: #274e13; text-decoration: none;">Hydra</a></center>
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<b><span style="font-size: medium;">Southern Pinwheel</span></b></center>
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<a href="http://messier.obspm.fr/Jpg/m83.jpg" style="color: #274e13; text-decoration: none;"><img align="right" alt="[m83.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m83.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a><br /><table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">13 : 37.0 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">-29 : 52 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">15000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">7.6 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">11x10 (arc min)</td></tr>
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<br /><br />Discovered 1752 by Abbe Nicholas Louis de la Caille.<br /><br />Messier 83 (M83, NGC 5236) is one of the most conspicuous spiral galaxies in the sky. Situated in constellation Hydra, it is the southernmost galaxy in Messier's catalog.<br /><br />M83 was discovered by <a href="http://messier.obspm.fr/xtra/Bios/lacaille.html" style="color: #274e13; text-decoration: none;">Abbe Nicholas Louis de la Caille</a> at the Cape of Good Hope on February 23, 1752; it was <a href="http://messier.obspm.fr/xtra/history/lacaille.html" style="color: #274e13; text-decoration: none;">his object</a> Lacaille I.6. Thus it became the first galaxy to be discovered beyond the <a href="http://messier.obspm.fr/more/local.html" style="color: #274e13; text-decoration: none;">Local Group</a>, and the third of all galaixes, after <a href="http://messier.obspm.fr/m/m031.html" style="color: #274e13; text-decoration: none;">M31</a> and <a href="http://messier.obspm.fr/m/m032.html" style="color: #274e13; text-decoration: none;">M32</a>. It was next <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M83" style="color: #274e13; text-decoration: none;">cataloged</a> by <a href="http://messier.obspm.fr/xtra/history/biograph.html" style="color: #274e13; text-decoration: none;">Charles Messier</a> on February 17, 1781; from his mid-northern location in Paris (at 49 degrees Northern latitude), it is such a difficult object that he stated that: "One is only able with the greatest concentration to see it at all." The present author can confirm it is one of the most difficult Messier objects from South Germany. Due to this fact, older Northern-compiled catalogs tended to underestimate its brightness considerably; e.g., Becvar has it at a mere 10.1 mag only.<br /><br />Early 19th century Australian observer <a href="http://messier.obspm.fr/xtra/Bios/dunlop.html" style="color: #274e13; text-decoration: none;">James Dunlop</a> has it as No. 628 in <a href="http://messier.obspm.fr/xtra/similar/dunlop.html" style="color: #274e13; text-decoration: none;">his catalog</a>. Its spiral structure was noted and sketched by <a href="http://messier.obspm.fr/xtra/Bios/lassell.html" style="color: #274e13; text-decoration: none;">William Lassell</a> who described it as a "three-branched spiral."<br />................................<br /><br />LEIA MAIS<br />em<br /><a href="http://messier.obspm.fr/m/m083.html" style="color: #274e13; text-decoration: none;">http://messier.obspm.fr/m/m083.html</a><br /><br /><br /><br /><div class="separator" style="clear: both;">
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjVEbiPIZgKAcleIZTbgOrTdlMZgA-0RxN9CKDmEv5AlJvYahy8p6ey7AjrwZPe8Bg9lBy_mQheTj_14GqRevFmGRULamxlOGSb7gKtxB7QyIp30VStBUDhQ4Ln_t8l173152WZ8_zpjFE/s1600/m+83..png" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjVEbiPIZgKAcleIZTbgOrTdlMZgA-0RxN9CKDmEv5AlJvYahy8p6ey7AjrwZPe8Bg9lBy_mQheTj_14GqRevFmGRULamxlOGSb7gKtxB7QyIp30VStBUDhQ4Ln_t8l173152WZ8_zpjFE/s1600/m+83..png" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" /></a></div>
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<span style="font-family: arial, helvetica, sans-serif;">http://www.stellarium.org/pt/</span><br /><span style="font-family: arial, helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: arial, sans-serif;"><b><span style="color: #660000;">NGC 5236 - M 83 - Galáxia Hydra</span></b><o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Ascensão Reta 13h36 Declinação - 29<sup>o</sup>.46<o:p></o:p></span></div>
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<span style="font-family: arial, sans-serif;">Tipo S - Galáxia Espiral Magnitude fotográfica aparente 7,00</span></div>
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<span style="font-family: arial, sans-serif;">Dimensões Angulares 13 X 12 Distância (milhões de anos-luz) 8,0</span></div>
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<span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">M 83 - NGC 5236 - Galáxia Espiral Barrada<o:p></o:p></span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"><br /></span></div>
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<span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">Uma das mais brilhantes e mais belas galáxias do céu do sul. </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"> Seus braços em espiral elegantemente curvados </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">criam a impressão de um movimento dinâmico e giratório</span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"> em nuvens de estrelas que circundam o centro dessa ilha no universo.<o:p></o:p></span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"><br /></span></div>
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<span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">A coloração alaranjada da barra e da região central </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">indicam a predominância de estrelas antigas, </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">esfriadas e ainda estrelas avermelhadas. </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"> Em seus braços espiralados, a cor predominante </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">é o azul das estrelas jovens, quentes e muito massivas </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">que foram formadas recentemente</span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"> e que estão realizando uma evolução rápida. </span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;">Nuvens imensas de hidrogenio interestelar ionizado brilham do vermelho ao rosa.</span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif;"> Existem berços de novas estrelas que nascem aqui em grande número.<span style="font-size: 11pt;"><o:p></o:p></span></span><br /><span lang="PT" style="color: #0f243e; font-family: arial, sans-serif; font-size: 11pt;"><br /></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste</span><span style="font-family: arial, sans-serif;"><o:p></o:p></span></span></div>
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<span style="color: #274e13;"><span style="font-family: arial, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></span></div>
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<span style="color: #274e13; font-family: arial, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<br /><br /><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg/1280px-Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br /><br /><br /><a href="http://en.wikipedia.org/wiki/Messier_83#mediaviewer/File:Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Messier_83#mediaviewer/File:Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg</a><br /><div class="mw-mmv-title-para" style="color: #333333; font-family: sans-serif; line-height: 1.5em; overflow: hidden; padding: 10px 20px 0px; text-overflow: ellipsis; white-space: nowrap;">
<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Hubble view of barred spiral galaxy Messier 83</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgement: William Blair (Johns Hopkins University)</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/heic1403a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/heic1403a/</a></span></span></div>
<span style="color: #555555; font-family: sans-serif; line-height: 24px;">This new Hubble image shows the scatterings of bright stars and thick dust that make up spiral galaxy Messier 83, otherwise known as the Southern Pinwheel Galaxy. One of the largest and closest barred spirals to us, this galaxy is dramatic and mysterious; it has hosted a large number of supernova explosions, and appears to have a double nucleus lurking at its core.</span><br /><span style="color: #555555; font-family: sans-serif; line-height: 24px;"><br /></span><span style="color: #555555; font-family: sans-serif; line-height: 24px;"><br /></span><span style="color: #555555; font-family: sans-serif; line-height: 24px;"><br /></span><b style="color: #252525; font-family: sans-serif; line-height: 22.4px; text-align: start;">Messier 83</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> (also known as the </span><b style="color: #252525; font-family: sans-serif; line-height: 22.4px; text-align: start;">Southern Pinwheel Galaxy</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">, </span><b style="color: #252525; font-family: sans-serif; line-height: 22.4px; text-align: start;">M83</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> or </span><b style="color: #252525; font-family: sans-serif; line-height: 22.4px; text-align: start;">NGC 5236</b><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">) is a </span><a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a><sup class="reference" id="cite_ref-7" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> approximately 15 million </span><a href="http://en.wikipedia.org/wiki/Light-year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Light-year">light-years</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> away in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"></span><a href="http://en.wikipedia.org/wiki/Hydra_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Hydra (constellation)">Hydra</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">. It is one of the closest and brightest </span><a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxies</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> in the sky, making it visible with </span><a href="http://en.wikipedia.org/wiki/Binoculars" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Binoculars">binoculars</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">. Six </span><a href="http://en.wikipedia.org/wiki/Supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Supernova">supernovae</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> (</span><a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_1923A&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="SN 1923A (page does not exist)">SN 1923A</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">, </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_1945B&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="SN 1945B (page does not exist)">SN 1945B</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">, </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_1950B&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="SN 1950B (page does not exist)">SN 1950B</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">, </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_1957D&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="SN 1957D (page does not exist)">SN 1957D</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">,</span><a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_1968L&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="SN 1968L (page does not exist)">SN 1968L</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> and </span><a class="new" href="http://en.wikipedia.org/w/index.php?title=SN_1983N&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="SN 1983N (page does not exist)">SN 1983N</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">) have been observed in M83.</span><br /><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">.....................................</span><br /><a href="http://en.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> discovered M83 on February 23, 1752 at the </span><a href="http://en.wikipedia.org/wiki/Cape_of_Good_Hope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Cape of Good Hope">Cape of Good Hope</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">.</span><sup class="reference" id="cite_ref-jones1991_8-0" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-jones1991-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[8]</a></sup><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> </span><a href="http://en.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;"> added it to his catalogue of nebulous objects (now known as the </span><a href="http://en.wikipedia.org/wiki/Messier_object" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.4px; text-align: start; text-decoration: none;" title="Messier object">Messier Catalogue</a><span style="color: #252525; font-family: sans-serif; line-height: 22.4px;">) in March 1781.</span><sup class="reference" id="cite_ref-jones1991_8-1" style="color: #252525; font-family: sans-serif; line-height: 1; text-align: start; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-jones1991-8" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[8]</a></sup><br /><br /><br /><table cellspacing="3" class="infobox" style="background-color: #f9f9f9; border-spacing: 3px; border: 1px solid rgb(170, 170, 170); clear: right; color: black; font-family: sans-serif; font-size: 12px; line-height: 1.5em; margin: 0.5em 0px 0.5em 1em; padding: 0.2em; width: 22em;"><tbody>
<tr><th colspan="2" style="background: rgb(102, 204, 0); font-size: 15px; text-align: center; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Messier_object" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Messier object">Messier</a> 83</th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><a class="image" href="http://en.wikipedia.org/wiki/File:Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Hubble view of barred spiral galaxy Messier 83.jpg" data-file-height="2602" data-file-width="4000" height="163" src="http://upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg/250px-Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg/375px-Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d5/Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg/500px-Hubble_view_of_barred_spiral_galaxy_Messier_83.jpg 2x" style="background: rgb(255, 255, 255); border-radius: 0px; border: none; box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="250" /></a><br /><div>
<a href="http://en.wikipedia.org/wiki/Hubble_Space_Telescope" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hubble Space Telescope">Hubble</a> view of <a href="http://en.wikipedia.org/wiki/Barred_spiral_galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Barred spiral galaxy">barred spiral galaxy</a> Messier 83<sup class="reference" id="cite_ref-1" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></div>
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<tr><th colspan="2" style="background: rgb(102, 204, 0); text-align: center; vertical-align: top;">Observation data (<a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)#Julian_years_and_J2000" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">J2000</a> <a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">epoch</a>)</th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constellation">Constellation</a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Hydra_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hydra (constellation)">Hydra</a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Right ascension">Right ascension</a></th><td style="vertical-align: top;">13<sup style="font-size: 10px; line-height: 1;">h</sup> 37<sup style="font-size: 10px; line-height: 1;">m</sup> 00.9<sup style="font-size: 10px; line-height: 1;">s</sup><sup class="reference" id="cite_ref-ned_2-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declination">Declination</a></th><td style="vertical-align: top;">−29° 51′ 57″<sup class="reference" id="cite_ref-ned_2-1" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Redshift" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Redshift">Redshift</a></th><td style="vertical-align: top;">513 ± 2 km/<a href="http://en.wikipedia.org/wiki/Second" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Second">s</a><sup class="reference" id="cite_ref-ned_2-2" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Cosmic_distance_ladder" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Cosmic distance ladder">Distance</a></th><td style="vertical-align: top;"><div style="line-height: inherit; margin-bottom: 0.5em; margin-top: 0.5em;">
15.21 <a href="http://en.wikipedia.org/wiki/Light-year" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light-year">Mly</a> (4.61<a href="http://en.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">Mpc</a>)</div>
<sup class="reference" id="cite_ref-Sandage2006_3-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-Sandage2006-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Galaxy_morphological_classification" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galaxy morphological classification">Type</a></th><td style="vertical-align: top;">SAB(s)c<sup class="reference" id="cite_ref-ned_2-3" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Angular_diameter" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Angular diameter">Apparent dimensions</a> <small title="in visual light">(V)</small></th><td style="vertical-align: top;">12′.9 × 11′.5<sup class="reference" id="cite_ref-ned_2-4" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a> <small title="in visual light">(V)</small></th><td style="vertical-align: top;">7.54<sup class="reference" id="cite_ref-SIMBAD-M83_4-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-SIMBAD-M83-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup><sup class="reference" id="cite_ref-GAXEL_5-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-GAXEL-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup></td></tr>
<tr><th colspan="2" style="background: rgb(102, 204, 0); text-align: center; vertical-align: top;">Other designations</th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 5236,<sup class="reference" id="cite_ref-ned_2-5" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup> UGCA 366,<sup class="reference" id="cite_ref-ned_2-6" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup> <a href="http://en.wikipedia.org/wiki/Principal_Galaxies_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Principal Galaxies Catalogue">PGC</a> 48082,<sup class="reference" id="cite_ref-ned_2-7" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-ned-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup>Southern Pinwheel Galaxy<sup class="reference" id="cite_ref-simbad_6-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_83#cite_note-simbad-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></td></tr>
<tr><td colspan="2" style="background: rgb(102, 204, 0); text-align: center; vertical-align: top;">See also: <a href="http://en.wikipedia.org/wiki/Galaxy" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galaxy">Galaxy</a>, <a href="http://en.wikipedia.org/wiki/List_of_galaxies" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="List of galaxies">List of galaxies</a></td></tr>
</tbody></table>
<a href="http://en.wikipedia.org/wiki/Messier_83" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Messier_83</a><br /><br /><br /><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/b/b1/Star_birth_in_Messier_83_%28captured_by_the_Hubble_Space_Telescope%29.jpg/800px-Star_birth_in_Messier_83_%28captured_by_the_Hubble_Space_Telescope%29.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><br /><a href="http://en.wikipedia.org/wiki/Messier_83#mediaviewer/File:Star_birth_in_Messier_83_(captured_by_the_Hubble_Space_Telescope).jpg" style="color: #274e13; text-decoration: none;">http://en.wikipedia.org/wiki/Messier_83#mediaviewer/File:Star_birth_in_Messier_83_(captured_by_the_Hubble_Space_Telescope).jpg</a><br /><div class="mw-mmv-title-para" style="color: #333333; font-family: sans-serif; line-height: 1.5em; overflow: visible; padding: 10px 20px 0px; text-overflow: ellipsis;">
<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Star birth in Messier 83 (captured by the Hubble Space Telescope)</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">NASA, ESA, and the Hubble Heritage Team (STScI/AURA)</span> - <span class="mw-mmv-source"><a class="external free" href="http://hubblesite.org/newscenter/archive/releases/2009/29/image/b/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://hubblesite.org/newscenter/archive/releases/2009/29/image/b/</a> (<a class="external text" href="http://imgsrc.hubblesite.org/hu/db/images/hs-2009-29-b-full_jpg.jpg" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">direct link</a>)</span></span></div>
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<span style="font-family: arial, helvetica, sans-serif;">Portion of M83 by Hubble</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-source" style="font-family: arial, helvetica, sans-serif;"></span></span></div>
<div class="mw-mmv-image-desc" style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; line-height: 1.5em; margin-bottom: 0.5em; margin-top: 0.4em; padding-left: 20px; text-align: start;">
<span style="font-family: arial, helvetica, sans-serif;">Nicknamed the Southern Pinwheel, M83 is undergoing more rapid star formation than our own Milky Way galaxy, especially in its nucleus. The sharp "eye" of the Wide Field Camera 3 (WFC3) has captured hundreds of young star clusters, ancient swarms of globular star clusters, and hundreds of thousands of individual stars, mostly blue supergiants and red supergiants. The image, taken in August 2009, provides a close-up view of the myriad stars near the galaxy's core, the bright whitish region at far right. WFC3's broad wavelength range, from ultraviolet to near-infrared, reveals stars at different stages of evolution, allowing astronomers to dissect the galaxy's star-formation history. The image reveals in unprecedented detail the current rapid rate of star birth in this famous "grand design" spiral galaxy. The newest generations of stars are forming largely in clusters on the edges of the dark dust lanes, the backbone of the spiral arms. These fledgling stars, only a few million years old, are bursting out of their dusty cocoons and producing bubbles of reddish glowing hydrogen gas. The excavated regions give a colorful "Swiss cheese" appearance to the spiral arm. Gradually, the young stars' fierce winds (streams of charged particles) blow away the gas, revealing bright blue star clusters. These stars are about 1 million to 10 million years old. The older populations of stars are not as blue. A bar of stars, gas, and dust slicing across the core of the galaxy may be instigating most of the star birth in the galaxy's core. The bar funnels material to the galaxy's center, where the most active star formation is taking place. The brightest star clusters reside along an arc near the core. The remains of about 60 supernova blasts, the deaths of massive stars, can be seen in the image, five times more than known previously in this region. WFC3 identified the remnants of exploded stars. By studying these remnants, astronomers can better understand the nature of the progenitor stars, which are responsible for the creation and dispersal of most of the galaxy's heavy elements. M83, located in the Southern Hemisphere, is often compared to M51, dubbed the Whirlpool galaxy, in the Northern Hemisphere. Located 15 million light-years away in the constellation Hydra, M83 is two times closer to Earth than M51.</span></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><br /></span><br /><div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal;">
<img alt="Hydra" height="478" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_hydra.jpg" style="background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></div>
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<a href="http://www.aradergalleries.com/detail.php?id=3638" style="color: #274e13; text-decoration: none;">http://www.aradergalleries.com/detail.php?id=3638</a></div>
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<span style="font-family: georgia, 'times new roman', times, serif; font-size: 14px;"><span style="color: #073763;">Johann Bayer — Hydra</span></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>- as constelações -</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b> são como janelas que se abrem para a infinitude do universo </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>e que possibilitam nossa mente </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>a ir percebendo que existe mais, bem mais, entre o céu e a terra... </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>vagarosamente,</b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b> vai se tornando Cosmos </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>e sendo por nossa mente conscientizado. </b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Quer dizer, </b></span><br /><span style="font-family: arial, helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>COM UM ABRAÇO ESTRELADO,<o:p></o:p></b></span></div>
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<span style="font-family: arial, helvetica, sans-serif;"><b>Janine Milward</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: arial, helvetica, sans-serif;"><b>VISITE MINHA PÁGINA</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: arial, helvetica, sans-serif;"><b>DA TERRA AO CÉU E AO INFINITO</b><o:p></o:p></span></div>
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<span style="color: #660000; font-family: "arial" , "helvetica" , sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><b>Janine Milward</b></span><br />
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<img alt="Hydra" src="http://www.aradergalleries.com/maps/images/158_Bayer/br_hydra.jpg" height="478" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" width="640" /></div>
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<a href="http://www.aradergalleries.com/detail.php?id=3638" style="color: #274e13; text-decoration: none;">http://www.aradergalleries.com/detail.php?id=3638</a></div>
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<span style="font-family: "georgia" , "times new roman" , "times" , serif; font-size: 14px;"><span style="color: #073763;">Johann Bayer — Hydra</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: "arial" , "helvetica" , sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: "arial" , "helvetica" , sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: "arial" , "helvetica" , sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">COM UM ABRAÇO ESTRELADO,</span></div>
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<span style="font-family: "arial" , "helvetica" , sans-serif;">Janine Milward</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-9817073758808584262014-09-06T05:43:00.001-07:002015-01-04T07:44:00.260-08:00Hercules<br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Gosto muitíssimo de observar</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">um grupo de estrelas</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">bem ao meu norte,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">entre a Coroa Boreal e a Lira</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(e sempre o Grande Triângulo do Norte</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">composto pelas estrelas alpha da Lira, do Cisne e da Águia</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- Vega, Deneb e Altair, respectivamente -</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">nos atrai a atenção... )</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e tornando mais fácil, digamos assim,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">observarmos esse grupo de estrelas..</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> estrelas que formam uma figura meio desengonçada...</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">apresentando Hercules, o Homem Ajoelhado.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em Hercules, estaremos encontrando </span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o Objeto Messier 13</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- considerado o Aglomerado Globular mais famoso dos céus do norte.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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http://www.stellarium.org/pt/</div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US"> </span>HERCULES, O HOMEM AJOELHADO</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 15h47m / 18h56m Declinação +3<sup>o</sup>.9 / +51<sup>o</sup>.3<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Mito:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação foi colocada no céu como recordação dos trabalhos </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">realizados por Hércules</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> (sendo que os Doze Trabalhos do herói são representados pelas doze constelações do Zodíaco). </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Entretanto, existem outros relatos de que, durante a guerra entre os Deuses e os Titãs, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">os primeiros se situaram em uma parte dos céus que quase tombou com o peso caso Atlas e Hercules não tivessem segurado! </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Então, Hércules foi colocado no céu em comemoração a esse seu serviço.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Próximo à estrela Upsilon Herculis, situa-se o Apex Solar. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Nosso sistema solar está, de fato, em movimento em relação à galáxia da Via Láctea. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Seu movimento próprio traduz-se por um deslocamento aparente das estrelas. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> A velocidade relativa do Sol em direção ao Apex</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> é da ordem de 20 quilometros por segundo.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Fronteiras:</b><o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ophiucus, Aquila, Sagitta, Vulpecula, Lyra, Draco, Bootes, Corona Borealis, Serpens</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><img src="http://www.iau.org/static/public/constellations/gif/HER.gif" /><br />
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http://www.iau.org/static/public/constellations/gif/HER.gif<br />
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m13atlas.jpg" /><br />
http://www.ipac.caltech.edu/2mass/gallery/m13atlas.jpg<br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a><br />
<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a><a href="https://www.blogger.com/null" name="m81" style="background-color: white;"><br /></a><br />
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Messier 13</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M13 (NGC 6205)</i>, class V, in <a href="http://messier.obspm.fr/map/Her.html">Hercules</a></center>
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<br /><b><span style="font-size: large;">Hercules Globular Cluster</span></b><br /><b><span style="font-size: large;"><br /></span></b><b><br /></b></center>
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<a href="http://messier.obspm.fr/Jpg/m13.jpg"><img align="right" alt="[m13.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m13.jpg" /></a></div>
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">16 : 41.7 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+36 : 28 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">25.1 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.8 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">20.0 (arc min)</td></tr>
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Discovered by Edmond Halley in 1714.</div>
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Messier 13 (M13, NGC 6205), also called the 'Great globular cluster in Hercules', is one of the most prominent and best known globulars of the Northern celestial hemisphere.</div>
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It was discovered by <a href="http://messier.obspm.fr/xtra/Bios/halley.html">Edmond Halley</a> in 1714, who noted that 'it shows itself to the naked eye when the sky is serene and the Moon absent.' According to <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M13">cataloged it</a> on June 1, 1764, it is also reported in <a href="http://messier.obspm.fr/xtra/Bios/bevis.html">John Bevis</a>' "English" <i>Celestial Atlas</i>.</div>
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LEIA MAIS</div>
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em</div>
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http://messier.obspm.fr/m/m013.html</div>
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http://www.stellarium.org/pt/</div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/a/af/Cumulo-globular-m13.JPG/1024px-Cumulo-globular-m13.JPG" /></div>
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http://pt.wikipedia.org/wiki/Grande_Aglomerado_Globular_de_H%C3%A9rcules#mediaviewer/File:Cumulo-globular-m13.JPG</div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Cumulo-globular-m13</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="new" href="http://commons.wikimedia.org/w/index.php?title=User:Portscan&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="User:Portscan (página não existe)">Portscan</a></span> - <span class="mw-mmv-source"><span class="int-own-work">Obra do próprio</span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><span style="color: #660000;"><b>NGC 6205 - M 13 - Aglomerado Globular Hercules</b></span><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 16h41 Declinação +36<sup>o</sup>.30<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,4 Diâmetro aparente 12’,9 Tipo Espectral F6<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 13,85<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 10 Distância kpc 6,3 <o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) - 241<o:p></o:p></span></span><br />
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Este é considerado o aglomerado globular mais familiar do céu do norte. </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Mesmo a olho nu é visível como uma lastro pequeno e fosforescente </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">e é um dos objetos favoritos a serem observados através o telescópio. </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">O aglomerado contém cerca de 1 milhão de estrelas </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">e estima-se que tenha cerca de 10 mil milhões anos </span></span><br />
<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">e sua distância é de 34.000 anos-luz.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/60/Heart_of_M13_Hercules_Globular_Cluster.jpg/800px-Heart_of_M13_Hercules_Globular_Cluster.jpg" /></div>
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<span style="background-color: white;"><span style="color: #073763;">http://en.wikipedia.org/wiki/Messier_13</span></span></div>
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<span class="mw-mmv-title" original-title="File name" style="font-size: 1.2em; max-width: 60%;">Heart of M13 Hercules Globular Cluster</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Heart_of_M13_Hercules_Globular_Cluster.jpg" style="background: none; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Public Domain</a></div>
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<span class="mw-mmv-source-author" original-title="Author and source information"><span class="mw-mmv-author">ESA/Hubble and NASA</span> - <span class="mw-mmv-source"><a class="external free" href="http://www.spacetelescope.org/images/potw1011a/" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://www.spacetelescope.org/images/potw1011a/</a></span></span></div>
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<span style="background-color: #fbfbfb; color: #555555; font-family: sans-serif; font-size: 16px; line-height: 24px; text-align: start;">This image, taken by the Advanced Camera for Surveys on the Hubble Space Telescope, shows the core of the great globular cluster Messier 13 and provides an extraordinarily clear view of the hundreds of thousands of stars in the cluster, one of the brightest and best known in the sky. Just 25 000 light-years away and about 145 light-years in diameter, Messier 13 has drawn the eye since its discovery by Edmund Halley, the noted British astronomer, in 1714. The cluster lies in the constellation of Hercules and is so bright that under the right conditions it is even visible to the unaided eye. As Halley wrote: “This is but a little Patch, but it shews it self to the naked Eye, when the Sky is serene and the Moon absent.” Messier 13 was the target of a symbolic Arecibo radio telescope message that was sent in 1974, communicating humanity’s existence to possible extraterrestrial intelligences. However, more recent studies suggest that planets are very rare in the dense environments of globular clusters. This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys on the Hubble Space Telescope. Data through a blue filter (F435W) are coloured blue, data through a red filter (F625W) are coloured green and near-infrared data (through the F814W filter) are coloured red. The exposure times are 1480 s, 380 s and 567 s respectively and the field of view is about 2.5 arcminutes across</span></div>
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<img src="http://upload.wikimedia.org/wikipedia/commons/b/b6/Trouvelot_-_Star_clusters_in_Hercules_-_1877.jpg" /></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="line-height: 24px; max-width: 60%;"><span style="color: #333333; font-family: sans-serif;">http://pt.wikipedia.org/wiki/Grande_Aglomerado_Globular_de_H%C3%A9rcules#mediaviewer/File:Trouvelot_-_Star_clusters_in_Hercules_-_1877.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Trouvelot - Star clusters in Hercules - 1877</span><a class="mw-mmv-license" href="http://commons.wikimedia.org/wiki/File:Trouvelot_-_Star_clusters_in_Hercules_-_1877.jpg" style="background: none; color: #0b0080; font-size: 0.9em; padding: 0px 10px; text-align: right; text-decoration: none;" target="">Domínio público</a></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/%C3%89tienne_L%C3%A9opold_Trouvelot" style="background: none; color: #0b0080; text-decoration: none;" title="en:Étienne Léopold Trouvelot">Étienne Léopold Trouvelot</a></span> - <span class="mw-mmv-source"><a class="external free" href="http://digitalgallery.nypl.org/nypldigital/id?TROUVELOT_014" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">http://digitalgallery.nypl.org/nypldigital/id?TROUVELOT_014</a></span></span></div>
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Esboço de M13, desenhado por <a class="new" href="http://pt.wikipedia.org/w/index.php?title=%C3%89tienne_L%C3%A9opold_Trouvelot&action=edit&redlink=1" style="background: none; color: #a55858; text-decoration: none;" title="Étienne Léopold Trouvelot (página não existe)">Étienne Léopold Trouvelot</a> em 1877</div>
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Star cluster Messier 13 in Hercules. From a study made in June, 1877. (Plate XIV from The Trouvelot Astronomical Drawings 1881)</div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 13</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (</span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">M13</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">), also designated </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6205</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> and sometimes called the </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Great Globular Cluster in Hercules</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> or the </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Hercules Globular Cluster</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">, is a </span><a href="http://en.wikipedia.org/wiki/Globular_cluster" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Globular cluster">globular cluster</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> of about 300,000 stars in the </span><a href="http://en.wikipedia.org/wiki/Constellation" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constellation">constellation</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> of </span><a href="http://en.wikipedia.org/wiki/Hercules_(constellation)" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Hercules (constellation)">Hercules</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span></div>
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M13 was discovered by <a href="http://en.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Edmond Halley">Edmond Halley</a> in 1714, and catalogued by <a href="http://en.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a> on June 1, 1764.</div>
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It is located at <a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Right ascension">right ascension</a> 16<sup style="line-height: 1;">h</sup> 41.7<sup style="line-height: 1;">m</sup> and <a href="http://en.wikipedia.org/wiki/Declination" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declination">declination</a> +36° 28'. With an <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Apparent magnitude">apparent magnitude</a> of 5.8, it is barely visible with the <a href="http://en.wikipedia.org/wiki/Naked_eye" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Naked eye">naked eye</a> on a very clear night. Its diameter is about 23 arc minutes and it is readily viewable in small telescopes. Nearby is NGC 6207, a 12th magnitude edge-on galaxy that lies 28 arc minutes directly north east. A small galaxy, IC 4617, lies halfway between NGC 6207 and M13, north-northeast of the large globular cluster's center.</div>
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<tr><th colspan="2" style="background: rgb(255, 255, 192); font-size: 15px; text-align: center; vertical-align: top;">Messier 13</th></tr>
<tr><td colspan="2" style="text-align: center; vertical-align: top;"><a class="image" href="http://en.wikipedia.org/wiki/File:Heart_of_M13_Hercules_Globular_Cluster.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Heart of M13 Hercules Globular Cluster.jpg" data-file-height="3018" data-file-width="3018" src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/60/Heart_of_M13_Hercules_Globular_Cluster.jpg/250px-Heart_of_M13_Hercules_Globular_Cluster.jpg" height="640" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/60/Heart_of_M13_Hercules_Globular_Cluster.jpg/375px-Heart_of_M13_Hercules_Globular_Cluster.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/60/Heart_of_M13_Hercules_Globular_Cluster.jpg/500px-Heart_of_M13_Hercules_Globular_Cluster.jpg 2x" style="border: none; vertical-align: middle;" width="640" /></a><br />
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The heart of Hercules Globular Cluster;<br />
<span style="font-size: smaller;">Credit: ESA/Hubble and NASA</span></div>
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<tr><th colspan="2" style="background: rgb(255, 255, 192); text-align: center; vertical-align: top;">Observation data (<a class="mw-redirect" href="http://en.wikipedia.org/wiki/J2000" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="J2000">J2000</a> <a href="http://en.wikipedia.org/wiki/Epoch_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Epoch (astronomy)">epoch</a>)</th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Shapley%E2%80%93Sawyer_Concentration_Class" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Shapley–Sawyer Concentration Class">Class</a></th><td style="vertical-align: top;">V<sup class="reference" id="cite_ref-hcob849_11_1-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-hcob849_11-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[1]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Constellation" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constellation">Constellation</a></th><td style="vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Hercules_(constellation)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Hercules (constellation)">Hercules</a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Right_ascension" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Right ascension">Right ascension</a></th><td style="vertical-align: top;">16<sup style="font-size: 10px; line-height: 1;">h</sup> 41<sup style="font-size: 10px; line-height: 1;">m</sup> 41.24<sup style="font-size: 10px; line-height: 1;">s</sup><sup class="reference" id="cite_ref-aj140_6_1830_2-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-aj140_6_1830-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Declination" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declination">Declination</a></th><td style="vertical-align: top;">+36° 27′ 35.5″<sup class="reference" id="cite_ref-aj140_6_1830_2-1" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-aj140_6_1830-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[2]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a class="mw-redirect" href="http://en.wikipedia.org/wiki/Distance_(astronomy)" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Distance (astronomy)">Distance</a></th><td style="vertical-align: top;">22.2 <a href="http://en.wikipedia.org/wiki/Light-year#Distances_in_light-years" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Light-year">kly</a> (6.8 <a href="http://en.wikipedia.org/wiki/Parsec#Parsecs_and_kiloparsecs" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Parsec">kpc</a>)<sup class="reference" id="cite_ref-aj139_2_476_3-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-aj139_2_476-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[3]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Apparent_magnitude" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Apparent magnitude">Apparent magnitude</a><small>(V)</small></th><td style="vertical-align: top;">+5.8<sup class="reference" id="cite_ref-simbad_4-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-simbad-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Apparent dimensions<small>(V)</small></th><td style="vertical-align: top;">20 <a href="http://en.wikipedia.org/wiki/Minute_of_arc" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Minute of arc">arcmins</a></td></tr>
<tr><th colspan="2" style="background: rgb(255, 255, 192); text-align: center; vertical-align: top;">Physical characteristics</th></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Mass</th><td style="vertical-align: top;"><span class="nowrap" style="white-space: nowrap;">6<span style="margin-left: 0.25em; margin-right: 0.15em;">×</span>10<sup style="font-size: 10px; line-height: 1;">5</sup></span><sup class="reference" id="cite_ref-leonard_5-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-leonard-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[5]</a></sup> <a href="http://en.wikipedia.org/wiki/Solar_mass" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Solar mass">M<sub style="font-size: 10px; line-height: 1;">☉</sub></a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Radius</th><td style="vertical-align: top;">84 ly<sup class="reference" id="cite_ref-6" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[6]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;"><a href="http://en.wikipedia.org/wiki/Metallicity" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Metallicity">Metallicity</a></th><td style="vertical-align: top;">–1.33<sup class="reference" id="cite_ref-mnras404_3_1203_7-0" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-mnras404_3_1203-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup> <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Log_10" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Log 10">dex</a></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Estimated age</th><td style="vertical-align: top;">11.65 <a class="mw-redirect" href="http://en.wikipedia.org/wiki/Gigayear" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Gigayear">Gyr</a><sup class="reference" id="cite_ref-mnras404_3_1203_7-1" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-mnras404_3_1203-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[7]</a></sup></td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Notable features</th><td style="vertical-align: top;">one of the best-known clusters of the northern hemisphere</td></tr>
<tr><th scope="row" style="background-attachment: inherit; background-clip: inherit; background-image: inherit; background-origin: inherit; background-position: inherit; background-repeat: inherit; background-size: inherit; vertical-align: top;">Other designations</th><td style="vertical-align: top;">NGC 6205<sup class="reference" id="cite_ref-simbad_4-1" style="font-size: 10px; line-height: 1; unicode-bidi: -webkit-isolate;"><a href="http://en.wikipedia.org/wiki/Messier_13#cite_note-simbad-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">[4]</a></sup></td></tr>
<tr><td class="noprint" colspan="2" style="background: rgb(255, 255, 192); text-align: center; vertical-align: top;">See also: <a href="http://en.wikipedia.org/wiki/Globular_cluster" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Globular cluster">Globular cluster</a>, <a href="http://en.wikipedia.org/wiki/List_of_globular_clusters" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="List of globular clusters">List of globular clusters</a></td></tr>
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<div style="background-color: white; margin-bottom: 0.5em; margin-top: 0.5em; text-align: start;">
<span style="color: #252525; font-family: sans-serif;"><span style="font-size: 14px; line-height: 22.3999996185303px;">http://en.wikipedia.org/wiki/Messier_13</span></span></div>
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<span style="background-color: white;"><span style="color: #073763;">http://pt.wikipedia.org/wiki/Grande_Aglomerado_Globular_de_H%C3%A9rcules#mediaviewer/File:Messier_13_Hubble_WikiSky.jpg</span></span></div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 13 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=16.6945&de=36.461775&angle=0.0549531&projection=tan&rotation=19.53317&survey=astrophoto&img_id=60444&width=4000&height=4000&img_borders=0&interpolation=bicubic&jpeg_quality=0.8&max_preview_size=800&show_params=1&mouse_action=move" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m92atlas.jpg" /></div>
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<span style="background-color: white;"><span style="color: #073763;">http://www.ipac.caltech.edu/2mass/gallery/m92atlas.jpg</span></span></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a></div>
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<h1>
Messier 92</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Globular Cluster</a> M92 (NGC 6341)</i>, class IV, in <a href="http://messier.obspm.fr/map/Her.html">Hercules</a></center>
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<a href="http://messier.obspm.fr/Jpg/m92.jpg"><img align="right" alt="[m92.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m92.jpg" /></a></div>
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<tr><th align="left">Right Ascension</th><td align="center">17 : 17.1 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+43 : 08 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">26.7 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">6.4 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">14.0 (arc min)</td></tr>
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Discovered 1777 by Johann Elert Bode.</div>
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Globular cluster Messier 92 (M92, NGC 6341) is one of the more conspicuous globular clusters. Situated in constellation Hercules, it is nevertheless second only within that constellation, after bright <a href="http://messier.obspm.fr/m/m013.html">M13</a>.<br />
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M92 is one of the original discoveries of <a href="http://messier.obspm.fr/xtra/Bios/bode.html">Johann Elert Bode</a>, who found it on December 27, 1777. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> independently rediscovered it and <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M92">cataloged it</a> on March 18, 1781, the same day as he cataloged another 8 objects, all of them Virgo Cluster galaxies (<a href="http://messier.obspm.fr/m/m084.html">M84</a>-<a href="http://messier.obspm.fr/m/m091.html">M91</a>). It was <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> who first resolved it into stars in 1783.</div>
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LEIA MAIS </div>
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em</div>
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http://messier.obspm.fr/m/m092.html</div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white;"><b><span style="color: #660000;">NGC 6341 - M 92 - Aglomerado Globular</span></b><span style="color: #073763;"><o:p></o:p></span></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Ascensão Reta 17h16m Declinação + 34<sup>o</sup>.10<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude fotográfica global 6,9 Diâmetro aparente 12’,3 Tipo Espectral F1<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Magnitude média das 25 mais brilhantes estrelas (excluindo as 5 mais brilhantes) 13,96<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Número conhecido de Variáveis 16 Distância kpc 7,9<o:p></o:p></span></span></div>
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<span style="font-family: Arial, sans-serif;"><span style="background-color: white; color: #073763;">Velocidade Radial (km/s) - 118</span></span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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http://pt.wikipedia.org/wiki/Messier_92#mediaviewer/File:Messier_92_Hubble_WikiSky.jpg</div>
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<span class="mw-mmv-title" original-title="Nome do ficheiro" style="font-size: 1.2em; max-width: 60%;">Messier 92 Hubble WikiSky</span></div>
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<span class="mw-mmv-source-author" original-title="Autor e informação sobre a fonte"><span class="mw-mmv-author"><a class="extiw" href="http://en.wikipedia.org/wiki/NASA" style="background: none; color: #0b0080; text-decoration: none;" title="en:NASA">en:NASA</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/STScI" style="background: none; color: #0b0080; text-decoration: none;" title="en:STScI">en:STScI</a>, <a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a></span> - <span class="mw-mmv-source"><a class="extiw" href="http://en.wikipedia.org/wiki/WikiSky" style="background: none; color: #0b0080; text-decoration: none;" title="en:WikiSky">en:WikiSky</a>'s snapshot tool - <a class="external autonumber" href="http://server1.sky-map.org/snapshot?img_size=&img_res=&ra=17.285412165446733&de=43.135748659866834&angle=0.05822981366459627&projection=tan&rotation=-28.412301297434507&survey=astrophoto&img_id=60476&width=4200&height=4200&img_borders=0&interpolation=bicubic2&jpeg_quality=0.95&max_preview_size=800&show_params=1&mouse_action=zoom" rel="nofollow" style="background: none; color: #0b0080; text-decoration: none;">[1]</a></span></span></div>
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<b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">Messier 92</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> (também conhecido como </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">M92</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> ou </span><b style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">NGC 6341</b><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">) é um </span><a href="http://pt.wikipedia.org/wiki/Aglomerado_globular" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Aglomerado globular">aglomerado globular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> localizado na </span><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Constelação">constelação</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> de </span><a href="http://pt.wikipedia.org/wiki/H%C3%A9rcules_(constela%C3%A7%C3%A3o)" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Hércules (constelação)">Hercules</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> a 26 700 </span><a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Ano-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> da </span><a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Terra">Terra</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Foi descoberto por</span><a href="http://pt.wikipedia.org/wiki/Johann_Elert_Bode" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Johann Elert Bode">Johann Elert Bode</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1777" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1777">1777</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> e redescoberto independentemente por </span><a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Charles Messier">Charles Messier</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;"> em </span><a href="http://pt.wikipedia.org/wiki/1781" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="1781">1781</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">. Possui um raio de 54,5 anos-luz e uma dimensão aparente de 14,0 </span><a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background-attachment: initial; background-clip: initial; background-color: white; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px; text-align: start;">.</span><span class="reference" id="cite_ref-seds_2-4" style="background-color: white; bottom: 1ex; color: #252525; font-family: sans-serif; height: 0px; line-height: 1; position: relative; text-align: start; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-seds-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><b>Messier 92</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Messier_92_Hubble_WikiSky.jpg" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 92, Telescópio Espacial Hubble"><img alt="Messier 92, Telescópio Espacial Hubble" data-file-height="4200" data-file-width="4200" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/43/Messier_92_Hubble_WikiSky.jpg/250px-Messier_92_Hubble_WikiSky.jpg" height="250" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/43/Messier_92_Hubble_WikiSky.jpg/375px-Messier_92_Hubble_WikiSky.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/43/Messier_92_Hubble_WikiSky.jpg/500px-Messier_92_Hubble_WikiSky.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br />
Messier 92, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></td></tr>
<tr style="vertical-align: top;"><td>Descoberto por</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Johann_Elert_Bode" style="background: none; color: #0b0080; text-decoration: none;" title="Johann Elert Bode">Johann Elert Bode</a></td></tr>
<tr style="vertical-align: top;"><td>Data</td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1777" style="background: none; color: #0b0080; text-decoration: none;" title="1777">1777</a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Dados observacionais (J2000)</b></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação">Constelação</a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/H%C3%A9rcules_(constela%C3%A7%C3%A3o)" style="background: none; color: #0b0080; text-decoration: none;" title="Hércules (constelação)">Hercules</a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">Asc. reta</a></td><td style="background-color: #f8f8f8;">17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 17<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 07,4<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Declinação</a></td><td style="background-color: #f8f8f8;">43° 08′ 09,4″<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Distância</td><td style="background-color: #f8f8f8;">26 700 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background: none; color: #0b0080; text-decoration: none;" title="Ano-luz">anos-luz</a><span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span> (8 200 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background: none; color: #0b0080; text-decoration: none;" title="Parsec">pc</a>)</td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnit. apar.</a></td><td style="background-color: #f8f8f8;">6,3<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
<tr style="vertical-align: top;"><td>Dimensões</td><td style="background-color: #f8f8f8;">14,0 <a href="http://pt.wikipedia.org/wiki/Minuto_de_arco" style="background: none; color: #0b0080; text-decoration: none;" title="Minuto de arco">minutos de arco</a><span class="reference" id="cite_ref-seds_2-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Classe_de_Concentra%C3%A7%C3%A3o_de_Shapley%E2%80%93Sawyer" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classe de Concentração de Shapley–Sawyer">Classe</a></td><td style="background-color: #f8f8f8;">IV<span class="reference" id="cite_ref-seds_2-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Características físicas</b></td></tr>
<tr style="vertical-align: top;"><td>Raio</td><td style="background-color: #f8f8f8;">54,5<span class="reference" id="cite_ref-seds_2-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><b>Outras denominações</b></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;">M92, <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none; color: #0b0080; text-decoration: none;" title="New General Catalogue">NGC</a> 6341, GC1 59.<span class="reference" id="cite_ref-simbad_1-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_92#cite_note-simbad-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Hercules_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;"><img alt="Hercules constellation map.png" data-file-height="2839" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/46/Hercules_constellation_map.png/250px-Hercules_constellation_map.png" height="277" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/46/Hercules_constellation_map.png/375px-Hercules_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/46/Hercules_constellation_map.png/500px-Hercules_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></a></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br /><div style="color: black; font-family: 'Times New Roman'; font-size: medium; line-height: normal; margin: 0px;">
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,<o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;">Janine Milward<b><o:p></o:p></b></span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-81791406919423276622014-09-06T05:41:00.005-07:002015-01-04T07:34:28.245-08:00Gemini<br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Em continuidade aos nossos Trabalhos</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Visitando os Objetos Messier,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">estaremos comentando um tantinho</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre M35,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">o único Objeto Messier na constelação Gemini.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiL18ZUL4Tn5ZToivm3Q3Fjg6YqIcowO2NYmSU1m5a8Y2Gu0dcsWEOhCT61fWCwkZ0_-R2qBx8cJuJ4ZNWCjOUU69WOL0kWoN8om4OOJgFJqXWInfpg9glfj0YayJ_8QhWyUBlG0KxUt_w/s1600/M35+aproximado.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiL18ZUL4Tn5ZToivm3Q3Fjg6YqIcowO2NYmSU1m5a8Y2Gu0dcsWEOhCT61fWCwkZ0_-R2qBx8cJuJ4ZNWCjOUU69WOL0kWoN8om4OOJgFJqXWInfpg9glfj0YayJ_8QhWyUBlG0KxUt_w/s1600/M35+aproximado.jpg" /></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<b><span style="color: #660000;">CASTOR E POLLUX</span></b></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; margin-left: 1em; margin-right: 1em;"><a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgaeui6BQGq7IjgEHt_prJHt14Y5xfEnQoVHu8gGAPDFOYkSP6jpUcFWWG3kDrH9irvRZ4Zg3tdwYMvWov2A1FK6BnLu8-4MwYiPNL7xykadhPN0DJ2sJFbUh3zyHqYPyi5eZ95cgdJB-E/s1600/castor_and_pollux_by_zerolexa-d55ja88.jpg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgaeui6BQGq7IjgEHt_prJHt14Y5xfEnQoVHu8gGAPDFOYkSP6jpUcFWWG3kDrH9irvRZ4Zg3tdwYMvWov2A1FK6BnLu8-4MwYiPNL7xykadhPN0DJ2sJFbUh3zyHqYPyi5eZ95cgdJB-E/s1600/castor_and_pollux_by_zerolexa-d55ja88.jpg" height="428" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="640" /></a></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;">http://zerolexa.deviantart.com/art/Castor-and-Pollux-311628680</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; font-size: x-small;"><span style="line-height: 16.1200008392334px; text-align: left;">Antoine Coysevox</span><span style="line-height: 16.1200008392334px; text-align: left;"> [French Baroque Era Sculptor, 1640-1720)</span></span></div>
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<i><span lang="EN-US" style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">The conception of a sky couple for these stars has been universal from remote antiquity, but our Latin title dates only from classical times, varied by </span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"><span lang="EN-US">Gemelli</span></span><span lang="EN-US" style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">, which is still the Italian name.</span></i></div>
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<span lang="EN-US" style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;"><span style="line-height: 22.3999996185303px;"> </span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Gemini*.html" style="color: #274e13; line-height: 22.3999996185303px; text-decoration: none;">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Gemini*.html</a></span></div>
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<span style="line-height: 22.3999996185303px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="larger"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: #274e13; text-decoration: none;" target="index"><span style="color: #274e13;">Star Names, </span><span class="small" style="color: #274e13;">Their Lore and Meaning</span></a></span></span></span></div>
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<span style="line-height: 22.3999996185303px;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span class="larger"><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: #274e13; text-decoration: none;" target="index"><span class="small" style="color: #274e13;"> </span></a></span></span></span><a href="http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/home.html" style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px; text-decoration: none;" target="index">by <span class="larger">Richard Hinckley Allen </span></a></div>
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<span lang="EN-US"><span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>Os Gêmeos</b></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">(minha tradução literal)</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">A concepção de um casal celeste </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">para estas estrelas tem sido universal </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">desde a mais remota antigüidade</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> – porém nosso nome em latim data somente desde os tempos clássicos</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">O Mito e sua representação pictórica</span></b></span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilMwTP7eYOJUS5v6Fy0gRQFdzBOuD7M7hMt9GniDIhMkrF8rEWv8ZA8UZJfp9K4paE3GQytakdjoP0syU2qELCK0cKDQlcS5IMtNxkMfzhKw_3YSkUt4wsitrkjVCUSscW_FndFzmR-OE/s1600/191-av-renascimento-da-vinci.jpeg" imageanchor="1" style="color: #274e13; margin-left: 1em; margin-right: 1em; text-decoration: none;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEilMwTP7eYOJUS5v6Fy0gRQFdzBOuD7M7hMt9GniDIhMkrF8rEWv8ZA8UZJfp9K4paE3GQytakdjoP0syU2qELCK0cKDQlcS5IMtNxkMfzhKw_3YSkUt4wsitrkjVCUSscW_FndFzmR-OE/s1600/191-av-renascimento-da-vinci.jpeg" height="640" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative;" width="483" /></span></a></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #274e13;">“LEDA E O CISNE”, de Leonardo Da Vinci, em cópia do século 16</span></b></span></span></div>
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<span style="text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;"> - Leda é a esposa de Tíndaro, rei de Esparta, seduzida por Zeus transfigurado em um cisne, do qual gerou dois ovos, um com os gêmeos Castor e Pólux e outro com as gêmeas Helena e Clitemnestra. Conservada pela Galleria Borghese, em Roma, esta é uma cópia realizada por um discípulo direto de Leonardo Da Vinci (1452-1519), provavelmente Cesare da Sesto. A obra original do gênio, feita sobre painéis de madeira entre 1510 e 1515, foi vista pela última vez em 1691, num castelo francês, em mau estado de conservação. Além da desaparecida pintura com Leda em pé, cercada pela libidinosa figura do cisne, é provável, segundo os desenhos originais conservados, que Da Vinci tenha pintado também a mulher ajoelhada, obra da qual restaram apenas cópias de alta qualidade. - </span></span></span></div>
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<span style="color: #274e13;"><span style="text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span></span><span style="text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><b>See more at:</b></span></span></span></div>
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<span style="text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #274e13;"> http://bravonline.abril.com.br/materia/guia-do-renascimento-para-o-seculo-21#sthash.HOb4Qtgq.dpuf</span></span></span></div>
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<span style="text-align: start;"><span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">Caros Leitores,</span></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Esse é um Mito bem interessante</span><span style="font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">, realmente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">pois que Leda, a mãe, trouxe à luz dois pares de gêmeos</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- sendo que, <i>aparentemente</i>, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Castor e Clitemnestra eram filhos do marido de Leda, o Rei Tíndaro,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">enquanto Pollux e Helena eram filhos de Júpiter</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(que transmutou-se num Cisne</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"> - para fugir dos olhos atentos de Juno, sua mulher -</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e fazer amor e emprenhar Leda).</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">O tema de amor entre Leda e o Cisne</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">tem sido sempre motivação de inspiração pictórica</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">e para ser cantado em prosa e verso</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">bem como para a formulação de conceitos na psicanálise!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">........................</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Em lugares de céus escuros e transparentes,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sempre podemos acompanhar a Lua e os Planetas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">visitando as várias estrelas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">que compõem esta imensa constelação</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- pena que quase sempre Lua e Planetas</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">não se aproximem muito das estrelas-alpha e beta Gemini,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Castor e Pollux,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">duas estrelas ponteadoras dos céus estrelados!</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">.....................................</span><br />
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<span style="font-family: Arial, Helvetica, sans-serif;">Quando do meu nascimento,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">o Sol estava passando entre as estrelas epsilon e zeta Gemini, </span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">Mebsuta e Mekbuda, respectivamente,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- e coincindindo com o momento do Afélio, que bom.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Gostaria de lhe chamar a atenção,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Caro Leitor,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">para o fato de que M35 se situar bem próximo à Linha da Eclíptica</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- e esse fato pode sempre fazer acontecerem passagens em Conjunção </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">de Lua e de Planetas em relação a este Objeto Messier único</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">na constelação dos Gêmeos Castor e Pollux.</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">(Na Ilustração abaixo, perceba</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">a proximidade de Mercúrio e de Urano</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">em relação a M35)</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhLVyT3VN-B0n30XOKC31R-IBXN7w-CliFz1VdaMcM9pbWW8gjWYcQJzVN0djHeQpcWqNGphejw6K_ML4vsXqzKQKItFvKUIwMT9n8hYACweYknd8WjuvHdCNkksf5hlCuZyj5-8TeaawE/s1600/me.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhLVyT3VN-B0n30XOKC31R-IBXN7w-CliFz1VdaMcM9pbWW8gjWYcQJzVN0djHeQpcWqNGphejw6K_ML4vsXqzKQKItFvKUIwMT9n8hYACweYknd8WjuvHdCNkksf5hlCuZyj5-8TeaawE/s1600/me.png" height="480" width="640" /></a></div>
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<span style="color: black; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: normal;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: normal;"><span style="color: #073763;">E se você bem perceber, Caro Leitor,</span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; line-height: normal;"><span style="color: #073763;">verá que o momento do Solstício</span></span></div>
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- de inverno para o hemisfério sul e de verão para o hemisfério norte -</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acontece bem na pontinha de um pé de Castor</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(segundo a Ilustração do Programa Stellarium)</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e sob o testemunho do Objeto Messier ora sendo estudado,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">M35!</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;">Acessando meu Trabalho em</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://oceudomes.blogspot.com.br/2014/06/inverno-e-verao-entram-em-cena-amanha.html">http://oceudomes.blogspot.com.br/2014/06/inverno-e-verao-entram-em-cena-amanha.html</a>,</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;">você encontrará informações sobre o Tema Solstícios e Equinócios.</span><br />
<span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="font-family: Arial, Helvetica, sans-serif;"><br /></span><br />
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<span style="color: black; font-family: Arial, Helvetica, sans-serif; font-size: small; line-height: normal;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - Cartas Celestes, As Constelações </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="line-height: 18px;">Apoio: CARJ/MEC/CAPES/PADCT-SPEC</span></span></div>
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<span style="background-color: white; color: #660000; font-family: Arial, Helvetica, sans-serif;"><b><span lang="EN-US"> </span>GEMINI, OS GÊMEOS</b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Posicionamento:<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 5h57m / 8h6m Declinação +10<sup>o</sup>.0 / +35<sup>o</sup>.4<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esta constelação representa Castor e Pollux, os filhos gêmeos de Leda e Júpiter.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>Algumas Informações Interessantes acerca esta Constelação:</b><o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A origem deste asterismo prende-se à coincidência </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">de estar o sol nesta região do céu no período posterior às inundações do Nilo, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">precedendo a época da germinação e anunciando a fecundidade. </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Inscrições existentes no túmulo de Ramsés VI, do século XIIII AC, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">mostram dois brotos de plantas no lugar dos Gêmeos: </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e à semelhança desta representação, no Atlas Celeste de Bayer,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Pollux é encontrado armado de uma foice.<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Na antiguidade, a constelação dos Gêmeos foi freqüentemente representada </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">pela figura de duas estrelas sobre um navio,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> pois Castor e Pollux são considerados </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">divindades protetoras dos marinheiros e viajantes.<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">A constelação Gemini situa-se entre Câncer, Lyinx, Auriga, Taurus, Orion, Monóceros e Canes Minor</span><br />
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,<o:p></o:p></span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<a href="http://www.iau.org/static/public/constellations/gif/GEM.gif">http://www.iau.org/static/public/constellations/gif/GEM.gif</a></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>M35,</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O OBJETO MESSIER</b></span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>NA DIREÇÃO DA CONSTELAÇÃO GEMINI:</b></span></div>
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<a href="http://www.ipac.caltech.edu/2mass/gallery/m35atlas.jpg">http://www.ipac.caltech.edu/2mass/gallery/m35atlas.jpg</a></div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;"> "Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation."</a></div>
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<h1>
Messier 35</h1>
<i><a href="http://messier.obspm.fr/cluster.html">Open Cluster</a> M35 (NGC 2168)</i>, type 'e', in <a href="http://messier.obspm.fr/map/Gem.html">Gemini</a></center>
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<a href="http://messier.obspm.fr/Jpg/m35.jpg"><img align="right" alt="[m35.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m35.jpg" /></a><br />
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<tr><th align="left">Right Ascension</th><td align="center">06 : 08.9 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+24 : 20 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">2.8 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">5.3 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">28.0 (arc min)</td></tr>
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Discovered by Philippe Loys de Chéseaux 1745-46.<br />
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Independently discovered by John Bevis before 1750.<br />
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The discovery of M35 is usually assigned to <a href="http://messier.obspm.fr/xtra/similar/deches.html">Philippe Loys de Chéseaux</a> who observed and cataloged it in 1745 or 1746. It is also printed in <a href="http://messier.obspm.fr/xtra/Bios/bevis.html">John Bevis</a>' <a href="http://messier.obspm.fr/more/m035_bevis.html"><i>Uranographia Britannica</i></a> which was completed in 1750, so that this astronomer must have discovered it independently before this time, maybe or maybe not before De Chéseaux. <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a>, who <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M35">cataloged it</a> on August 30, 1764, acknowledges Bevis' discovery.<br />
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LEIA MUITO MAIS<br />
em<br />
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.stellarium.org/pt/</span></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 2168 - M 35 - Aglomerado Aberto</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 06h07m Declinação +24<sup>o</sup>.21<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Magnitude fotográfica global 5,6 Magnitude fotográfica da mais brilhante estrela 9,0<o:p></o:p></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Distância kpc 0,87 Diâmetro 29’ Tipo Espectral B5<o:p></o:p></span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Esplêndido aglomerado aberto, visível a olho nu,</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> a dois graus a noroeste de Eta Geminorum, o Pé Estirado. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> Formado por mais de 600 estrelas, está situado à distância de 1.500 anos-luz. </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um bom par de binóculos, </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">são percebidas algumas estrelas </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e com um bom telescópio, cerca de 300!<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; text-align: left; text-indent: 47.2000007629395px;">6</span><sup style="font-family: Arial, Helvetica, sans-serif; text-align: left; text-indent: 47.2000007629395px;">a</sup><span style="font-family: Arial, Helvetica, sans-serif; text-align: left; text-indent: 47.2000007629395px;">. Edição do </span><span style="font-family: Arial, Helvetica, sans-serif; text-align: left; text-indent: 47.2000007629395px;">Atlas Celeste </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; text-indent: 47.2000007629395px;">de autoria de </span><span style="font-family: Arial, Helvetica, sans-serif; text-indent: 47.2000007629395px;">Ronaldo Rogério de Freitas Mourão</span><span style="font-family: Arial, Helvetica, sans-serif; text-indent: 47.2000007629395px;">,</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif; text-indent: 47.2000007629395px;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - excerto da Carta Celeste dos Gêmeos </span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">- As Constelações, Cartas Celestes - CARJ</span></div>
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<span style="color: #660000;"><b>Messier 35 (também conhecido como M35 ou NGC 2168)</b></span><span style="color: #252525;"> é um <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> localizado na <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_de_G%C3%AAmeos" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Constelação de Gêmeos">constelação de Gêmeos</a>. Foi descoberto por <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Philippe Loys de Chéseaux">Philippe Loys de Chéseaux</a> em<a href="http://pt.wikipedia.org/wiki/1745" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1745">1745</a> e independentemente redescoberto por <a href="http://pt.wikipedia.org/wiki/John_Bevis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Bevis">John Bevis</a> antes de <a href="http://pt.wikipedia.org/wiki/1750" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="1750">1750</a>.</span></div>
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M35 está a uma distância de cerca de 2800 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a> da <a href="http://pt.wikipedia.org/wiki/Terra" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Terra">Terra</a> e tem um diâmetro de cerca de 24 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Anos-luz">anos-luz</a>. O aglomerado tem uma idade entre 95 e 110 milhões de anos e contém algumas <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Estrelas" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Estrelas">estrelas</a> que já abandonaram a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Seq%C3%BC%C3%AAncia_principal" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Seqüência principal">seqüência principal</a>.</div>
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A descoberta do <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Aglomerado aberto">aglomerado aberto</a> é geralmente creditada ao astrônomo suíço-francês <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a> em 1745 ou 1746. Também estava presente na<i>Uranographia Britannica</i>, de <a href="http://pt.wikipedia.org/wiki/John_Bevis" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="John Bevis">John Bevis</a>, publicada em 1750. É possível que Bevis tenha descoberto objeto antes de de Chéseaux, mas não há registros comprovatórios.<a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>, que o <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catalogou</a> em 30 de agosto de 1764, creditou a descoberta do aglomerado a Bevis.<span class="reference" id="cite_ref-seds_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_35#cite_note-seds-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Pode ser visualizado mesmo a <a href="http://pt.wikipedia.org/wiki/Olho_nu" style="background: none; color: #0b0080; text-decoration: none;" title="Olho nu">olho nu</a> em um <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a> com boas condições. Um <a href="http://pt.wikipedia.org/wiki/Bin%C3%B3culo" style="background: none; color: #0b0080; text-decoration: none;" title="Binóculo">binóculo</a> pode observar as estrelas mais brilhantes do aglomerado e <a href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio" style="background: none; color: #0b0080; text-decoration: none;" title="Telescópio">telescópios</a> amadores de baixa magnificação são os melhores instrumentos ópticos para a sua observação</div>
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<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; font-size: 15px; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Messier 35</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: black; color: white; font-size: x-small; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;"><a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:M35atlas.jpg" style="background: none;" title="Aglomerado aberto Messier 35"><img alt="Aglomerado aberto Messier 35" data-file-height="1196" data-file-width="1501" src="http://upload.wikimedia.org/wikipedia/commons/thumb/1/12/M35atlas.jpg/250px-M35atlas.jpg" height="199" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/12/M35atlas.jpg/375px-M35atlas.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/12/M35atlas.jpg/500px-M35atlas.jpg 2x" style="border: none; vertical-align: middle;" width="250" /></a><br /><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none;" title="Aglomerado aberto">Aglomerado aberto</a> Messier 35</span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: black; font-family: Times New Roman; font-size: small;">Descoberto por</span></td><td style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Philippe_Loys_de_Ch%C3%A9seaux" style="background: none;" title="Philippe Loys de Chéseaux"><span style="color: black; font-family: Times New Roman; font-size: small;">Philippe Loys de Chéseaux</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="color: black; font-family: Times New Roman; font-size: small;">Data</span></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/1745" style="background: none;" title="1745"><span style="color: black; font-family: Times New Roman; font-size: small;">1745</span></a></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Dados observacionais (J2000)</span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Constelação"><span style="color: black; font-family: Times New Roman; font-size: small;">Constelação</span></a></td><td style="background-color: #f8f8f8;"><a href="http://pt.wikipedia.org/wiki/Gemini_(constela%C3%A7%C3%A3o)" style="background: none;" title="Gemini (constelação)"><span style="color: black; font-family: Times New Roman; font-size: small;">Gemini</span></a></td></tr>
<tr style="vertical-align: top;"><td><span style="color: black; font-family: Times New Roman; font-size: small;">Tipo</span></td><td style="background-color: #f8f8f8;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Aglomerado_aberto" style="background: none;" title="Aglomerado aberto"><span style="color: black; font-family: Times New Roman; font-size: small;">Aglomerado aberto</span></a></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ascensão reta"><span style="color: black; font-family: Times New Roman; font-size: small;">Asc. reta</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">06<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 09.1<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span><span class="reference" id="cite_ref-simbad_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_35#cite_note-simbad-1" style="background: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Declinação"><span style="color: black; font-family: Times New Roman; font-size: small;">Declinação</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">+24° 21′<span class="reference" id="cite_ref-simbad_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_35#cite_note-simbad-1" style="background: none;">1</a></span></span></td></tr>
<tr style="vertical-align: top;"><td><span style="color: black; font-family: Times New Roman; font-size: small;">Distância</span></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">2800 <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none;" title="Anos-luz">anos-luz</a></span></td></tr>
<tr style="vertical-align: top;"><td><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Magnitude aparente"><span style="color: black; font-family: Times New Roman; font-size: small;">Magnit. apar.</span></a></td><td style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;">5.30</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #6295da; text-align: center;"><span style="color: black; font-family: Times New Roman; font-size: small;">Outras denominações</span></td></tr>
<tr style="vertical-align: top;"><td colspan="2" style="background-color: #f8f8f8;"><span style="color: black; font-family: Times New Roman; font-size: small;"><a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background: none;" title="New General Catalogue">NGC</a> 2168<span class="reference" id="cite_ref-simbad_1-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_35#cite_note-simbad-1" style="background: none;">1</a></span></span></td></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Messier 35"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Messier 35" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif" height="15" style="border: none; vertical-align: middle;" width="15" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Gemini_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Gemini constellation map.png" data-file-height="2269" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/58/Gemini_constellation_map.png/250px-Gemini_constellation_map.png" height="222" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/58/Gemini_constellation_map.png/375px-Gemini_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/58/Gemini_constellation_map.png/500px-Gemini_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="250" /></span></a></div>
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<a href="http://pt.wikipedia.org/wiki/Messier_35">http://pt.wikipedia.org/wiki/Messier_35</a><br />
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<a href="http://pt.wikipedia.org/wiki/Messier_35#mediaviewer/File:M35atlas.jpg">http://pt.wikipedia.org/wiki/Messier_35#mediaviewer/File:M35atlas.jpg</a></div>
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<span style="background-color: white;">Aglomerado aberto Messier 35</span></div>
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<span style="background-color: white;">Image of M35 Credit: Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.</span></div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
<div style="line-height: 16.8pt; margin: 0cm;">
<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br /><div style="font-family: 'Times New Roman'; font-size: medium; line-height: 18px;">
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<img src="http://www.raremaps.com/maps/large/31708.jpg" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background: rgb(255, 255, 255); border-bottom-left-radius: 0px; border-bottom-right-radius: 0px; border-top-left-radius: 0px; border-top-right-radius: 0px; border: 1px solid rgb(7, 55, 99); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px;" /><span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://www.raremaps.com/gallery/enlarge/31708</span></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif;"><strong>Title: </strong>Gemini </span><strong style="color: #274e13; font-family: Arial, Helvetica, sans-serif;">Map Maker: </strong><a href="https://www.raremaps.com/gallery/browse/creator_id/1372" style="border-bottom-color: rgb(255, 255, 255); border-bottom-style: solid; border-bottom-width: 0px; color: #274e13; font-family: Arial, Helvetica, sans-serif; text-decoration: none;">Alexander Jamieson</a></div>
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<span style="color: #274e13; font-family: Arial, Helvetica, sans-serif; line-height: 20px;">http://www.raremaps.com/gallery/detail/31708/Gemini/Jamieson.html</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">Com um abraço estrelado,</span><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<span style="color: #660000; font-family: Arial, sans-serif; font-size: 13.5pt;">Janine Milward</span><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 13.5pt;">VISITE MINHA PÁGINA</span><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 13.5pt;">DA TERRA AO CÉU E AO INFINITO</span><span style="font-size: 13.5pt;"><o:p></o:p></span></div>
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<span style="font-family: Arial, sans-serif; font-size: 13.5pt;">http://daterraaoceueaoinfinito.blogspot.com.br/</span></div>
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Janine Milwardhttp://www.blogger.com/profile/11201650743829208536noreply@blogger.comtag:blogger.com,1999:blog-8331511920586323989.post-90880298901565726712014-09-06T05:41:00.001-07:002015-01-04T05:15:21.763-08:00Draco<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Olá!</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Draco, o Dragão, é uma constelação que se posiciona</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">no semi-entorno do Polo Norte</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e por esta razão,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">dificilmente pode ser observada em sua inteireza</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">no Brasil.</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(Na região onde moro, o sudeste,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">consigo apenas visualizar o asterismo que forma a cabeça do Dragão</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span style="color: #073763;">e composto pelas estrelas </span><span style="color: #073763;"> Beta, Gamma, Xi e Omega Draconis).</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">No entanto, confeccionei uma Ilustração do Stellarium</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">para apresentar Draco </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">(não completo e visto em horizonte norte bem baixo, realmente)</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> a partir do ponto-de-vista</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">da cidade de Manaus, bem ao norte brasileiro,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">capital do belíssimo e imenso Estado do Amazonas.</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiVvZ3Uyl7sPgJzFSzH-3KF1kJGcIqSIINb0VtLZN3VFlS6ugXoI0QfshSickqtvqspQLAcDkGgJy_MeNGzaW5jDZgBfgTcZWMaLytOHtjmhubEAVqDxSbYlzZygeOiyhWPvDfto3ZOCxw/s1600/M102,+aproximada+e+ocm+ilustra%C3%A7%C3%B5es.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiVvZ3Uyl7sPgJzFSzH-3KF1kJGcIqSIINb0VtLZN3VFlS6ugXoI0QfshSickqtvqspQLAcDkGgJy_MeNGzaW5jDZgBfgTcZWMaLytOHtjmhubEAVqDxSbYlzZygeOiyhWPvDfto3ZOCxw/s1600/M102,+aproximada+e+ocm+ilustra%C3%A7%C3%B5es.png" /></span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></div>
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<a href="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhp9gB6Gj-8TX83ycINydE0dLHYc6Zgk0t755lRI6vwOxeDp1vOmEBS679RJ_qlGKEmwtheNBpnbX8Zk3PL2II7X0rhRirCQS5YCyf34cVKRVfr7BGEGaFyT0ba0L_ZpxLoIIz7mzRPCTE/s1600/m102.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><img border="0" src="https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhp9gB6Gj-8TX83ycINydE0dLHYc6Zgk0t755lRI6vwOxeDp1vOmEBS679RJ_qlGKEmwtheNBpnbX8Zk3PL2II7X0rhRirCQS5YCyf34cVKRVfr7BGEGaFyT0ba0L_ZpxLoIIz7mzRPCTE/s1600/m102.png" /></span></a></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; line-height: 22.3999996185303px;">http://www.stellarium.org/pt/</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">O título desta Postagem</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>M102, Objeto Messier em Draco (?) </b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ou NGC 5866, Galáxia do Fuso/do Eixo?</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b>ou ainda</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><b> ..... uma duplicata de M101, em Ursa Major?</b></span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">pode nos trazer, em um primeiro momento,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">alguma surpresa e uma indagação de seu porquê !?!</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Ao longo desta Postagem,</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">o Caro Leitor</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">haverá de encontrar situações informativas:</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- comentário </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">citando apenas NGC 5866, </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"> </span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">(sem mencionar M102), </span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">em pequeno trecho mais abaixo compilado</span><br />
<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">do astrônomo Ronaldo Rogério de Freitas Mourão:</span><br />
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">NGC 5866 - Galáxia</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma galáxia observada de lado </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e mostrando uma banda estreita e escura ao longo de seu equador.</span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span><span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">- cartas celestes não mencionando nem NGC 5866 e nem M102</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(Ilustrações em cartas celestes realizadas por</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">Mario Jaci Monteiro e por IAU)</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- Imagens realizadas por Nasa/Esa</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">apresentando a Galáxia Lenticular como NGC 5866</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">e não mencionando M102</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">(e ainda Imagem apresentada por Apod)</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- ilustrações advindas do Programa Stellarium</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">apresentando M102 - NGC 5866 como um mesmo objeto celeste</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"><br /></span></span><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">- a imagem realizada por Two Micron All Sky Survey</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;">nos apresenta o Objeto Messier 102</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> seguido de um ponto de interrogação entre-parênteses</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><span style="background-color: white;"> (denotando a dúvida/controvérsia acerca este objeto celeste).</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://www.ipac.caltech.edu/2mass/gallery/m102atlas.jpg</span><br />
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</span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"><br />- Situações não muito bem explicadas, dúvidas, duplo êrro, não-verificação,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e até situações bem controversas</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> acerca trabalhos realizados por Messier e Mechain,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> sugerem que o objeto observado e catalogado foi, na verdade,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> a galáxia lenticular NCG 5866, denominada Galáxia do Fuso/do Eixo... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e ainda incluindo a possibilidade de engano,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> ou seja,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;"> de que o objeto que teria sido nomeado enquanto M102 </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">seria uma possível duplicata do Objeto Messier 101, em Ursa Maior... </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">Ao final, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">parece que tanto Messier quanto Mechain observaram NGC 5866 no passado </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">e, portanto, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">este objeto acabou sendo listado </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">como o item perdido (no Catálogo Messier).<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">Leia mais abaixo, Caro Leitor,<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">trechos de comentários e explicações<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">sobre estas situações tão controversas<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; mso-themecolor: text2; mso-themeshade: 128;">extraídos dos Sites:</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">http://messier.obspm.fr/m/m102.html</span><br />
<span style="text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span></span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">http://messier.obspm.fr/m/ngc5866.html</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif; text-align: start;">http://pt.wikipedia.org/wiki/Messier_102</span><br />
<span style="text-align: start;"><span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e</span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Grupo_NGC_5866</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Se você quiser saber mais e mais</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">sobre o Catálogo Messier,</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">acesse</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span><br />
<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com um abraço estrelado,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Janine Milward</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Mario Jaci Monteiro - As Constelações, Cartas Celestes</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">DRACO, O DRAGÃO</span></b><span style="color: #073763;"><o:p></o:p></span></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> Situa-se em semi-torno do Pólo Norte</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ascensão Reta 9h18m / 21hom Declinação +47<sup>o</sup>.7 / - 86<sup>o</sup>.0<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Draco representa o dragão que guardava as maçãs douradas no jardim das Hesperides </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e somente Hercules (a constelação vizinha) poderia abater o Dragão. <o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">De acordo com outro mito, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">poderia ser ou o dragão jogado pelos gigantes em Minerva, na guerra com os Deuses, </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">ou a serpente Python degolada por Apollo após o Dilúvio.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br /></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Draco é uma das mais antigas constelações catalogadas </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">e era conhecida dos Egípcios, dos Gregos, dos Chineses e dos Árabes </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">através vários diferentes nomes.<o:p></o:p></span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">O Dragão é um conjunto de estrelas que forma uma longa fileira sinuosa. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Com a Cabeça voltada para Vega, ele circunda a Ursa Menor</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"> e separa as duas Ursas. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Ainda encontraremos fronteiras do Dragão com Bootes, Hercules, Lyra e Cepheus. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Um pequeno pedaço da fronteira de Dragão </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">situa-se muito próximo ao pólo norte celestial. </span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;"><br />A estrela Alpha do Dragão atuava como estrela polar em 2.700 AC.<o:p></o:p></span><br />
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">- 6a. Edição do Atlas Celeste</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="color: #073763; font-family: Arial, Helvetica, sans-serif;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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<img src="http://www.iau.org/static/public/constellations/gif/DRA.gif" /><br />
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http://www.iau.org/static/public/constellations/gif/DRA.gif</div>
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<img src="http://www.ipac.caltech.edu/2mass/gallery/m102atlas.jpg" /></div>
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http://www.ipac.caltech.edu/2mass/gallery/m102atlas.jpg</div>
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<a href="https://www.blogger.com/null" name="m81" style="background-color: white;">"Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation." </a></div>
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<h1>
Messier 102</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Galaxy</a> M102</i>(<a href="http://messier.obspm.fr/m/m101.html">M101</a> or <a href="http://messier.obspm.fr/m/ngc5866.html">NGC 5866</a>)</center>
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<a href="http://messier.obspm.fr/Jpg/m102.jpg"><img alt="[m102.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/m102.jpg" /></a></center>
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Evidently, Messier 102 (M102) is the last possibly "<a href="http://messier.obspm.fr/missing.html">missing</a>", or doubty, Messier object. This means that, based on the observation record of his friend, <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a>, <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> included this object <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M102">in his catalog</a> without verifying before publication, and it happens that Méchain's published position is erroneous. Two opinions on the identity of this object are common:<br />
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<li>M102 might be a duplication of the <i><a href="http://messier.obspm.fr/galaxy.html">Spiral Galaxy</a> <a href="http://messier.obspm.fr/m/m101.html">M101 (NGC 5457)</a></i> in <a href="http://messier.obspm.fr/map/UMa.html">Ursa Major</a>, due to a possible error of either the catalog author Messier, or its `discoverer' Méchain, a view brought up by Méchain in a <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m102">letter of May 1783</a>.</li>
<li>Perhaps more probably (<a href="http://messier.obspm.fr/m/m102d.html">due to historical evidence</a>), M102 may be the <i><a href="http://messier.obspm.fr/galaxy.html">Lenticular Galaxy</a> <a href="http://messier.obspm.fr/m/ngc5866.html">NGC 5866</a></i> in <a href="http://messier.obspm.fr/map/Dra.html">Draco</a>, also sometimes called the <i>Spindle Galaxy</i>, as Messier's catalog description indicates, together with the position he added later by hand in his personal copy.</li>
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The authors of this page think that there is sufficient evidence that both Méchain and Messier have probably observed NGC 5866 in context of this catalog entry. Therefore, it should be considered to take this last missing object back into the catalog.<br />
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Please note our discussion of <a href="http://messier.obspm.fr/m/m102d.html">more details on this topic</a>.<br />
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NGC 5866 / Messier 102 ?</h1>
<i><a href="http://messier.obspm.fr/galaxy.html">Lenticular (S0) Galaxy</a> NGC 5866 (M102 ?)</i>, type S0_3, in <a href="http://messier.obspm.fr/map/Dra.html">Draco</a></center>
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<br /><b><span style="font-size: large;">Spindle Galaxy</span></b><br /><b><br /></b><b><br /></b></center>
<a href="http://messier.obspm.fr/Jpg/ngc5866.jpg"><img align="right" alt="[ngc5866.jpg]" border="0" src="http://messier.obspm.fr/JpgSm/ngc5866.jpg" /></a><br />
<table border="2" cellpadding="5" cellspacing="0"><tbody>
<tr><th align="left">Right Ascension</th><td align="center">15 : 06.5 (h:m)</td></tr>
<tr><th align="left">Declination</th><td align="center">+55 : 46 (deg:m)</td></tr>
<tr><th align="left">Distance</th><td align="center">45000 (kly)</td></tr>
<tr><th align="left">Visual Brightness</th><td align="center">9.9 (mag) </td></tr>
<tr><th align="left">Apparent Dimension</th><td align="center">5.2x2.3 (arc min)</td></tr>
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Discovered probably either by Pierre Méchain or by Charles Messier in 1781.<br />
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Independently discovered by William Herschel in 1788.<br />
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NGC 5866 is a beautiful lenticular galaxy in Northern constellation Draco, which is seen almost exactly edge-on, showing a prominent dust lane along its equatorial plane. It is prominent for being a good candidate for <a href="http://messier.obspm.fr/m/m102.html">Messier Object 102</a>, i.e., Messier 102 (M102).<br />
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NGC 5866 was probably first seen by <a href="http://messier.obspm.fr/xtra/history/pmechain.html">Pierre Méchain</a> in March 1781, or by <a href="http://messier.obspm.fr/xtra/history/biograph.html">Charles Messier</a> shortly after that time. Therefore, NGC 5866 is possibly <a href="http://messier.obspm.fr/m/m102.html">M102</a>, although Pierre Méchain <a href="http://messier.obspm.fr/xtra/history/pm-lett.html#m102">disclaimed the discovery</a> two years later. Pierre Méchain's first observing report caused Messier to include it as <a href="http://messier.obspm.fr/xtra/history/m-cat.html#M102">entry No. 102</a> in his catalog, without giving a position or further verification. Soon after, Messier added a position measurement for this object (or entry) to his personal copy of the catalog, probably shortly after publication, and still in 1781. There is evidence that Charles Messier has probably observed NGC 5866 when measuring this position, as this is almost exactly 5 degrees preceding (west) of the actual position of the object: Very probably a data reduction error of some kind. Nevertheless, this subject is still somewhat dubious and therefore <a href="http://messier.obspm.fr/m/m102d.html">controversial</a>. If, despite this evidence, it should be true that neither Méchain nor Messier have observed NGC 5866, it was probably first seen by <a href="http://messier.obspm.fr/xtra/Bios/wherschel.html">William Herschel</a> when independently discovering it in 1788; William Herschel determined its position on May 5, 1788. As the possible earlier sightings by Méchain and Messier did not result in a published position for this object, this galaxy bears <a href="http://messier.obspm.fr/xtra/similar/herschel.html">Herschel's number H I.215</a>.<br />
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<img alt="Finder Chart for M102 (also shown M51 and M101)" src="https://blogger.googleusercontent.com/img/proxy/AVvXsEi0cR_WPjkM_5bFNDEQAUD37gUUT_rgmPFO3zVRX3P-Z4eCoqYgEhdiwqONW1IT3O4NsJAwhVRT9xp8XWEN-oyeui8KCyATcrMPDSQTCPdivNnCEidxF8h09kkej-aZpQygKPgEqwJjxcqvLexiZT3Mz_zKHSmns7e_BLuK_FkcoSdJoRd5i58=" /><br />
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<b><span style="font-family: Arial, sans-serif; font-size: 12pt;"><a href="http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy"><span lang="EN-US" style="color: blue; mso-ansi-language: EN-US; mso-bidi-font-size: 11.0pt;">Messier 102 - M102 - NGC 5866 - Spindle Galaxy (Lenticular Galaxy)</span></a></span></b><b><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 12pt;"><o:p></o:p></span></b></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">M102 is a galaxy catalogued by Charles Messier that hasn't been explicitly identified. It was Pierre Mechain who made the original observation in March 1781 before passing the information onto Messier, who catalogued it without verification. However, Mechain himself believed M102 was an error and wrote a letter on the May 6, 1783 expressing his view that the object was in fact a duplicate entry of</span><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;"> </span><span style="font-family: Arial, sans-serif; font-size: 9.5pt;"><a href="http://freestarcharts.com/index.php/20-guides/messier/251-messier-101-m101-the-pinwheel-galaxy-spiral-galaxy"><span lang="EN-US" style="color: blue; mso-ansi-language: EN-US; mso-bidi-font-size: 11.0pt;">M101</span></a></span><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">. The story does not end there, historical evidence based on Messier description of the galaxy combined with its co-ordinates suggest that M102 could well be lenticular galaxy NGC 5866, also known as the Spindle galaxy. A number of other possible candidates have been suggested but it seems both Messier and Mechain have observed NGC 5866 in the past and therefore we list it as the missing item.<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">The Spindle galaxy (mag. +9.9) is located at the southern edge of the far northern constellation of Draco. It's positioned four degrees southwest of star Iota Draconis (</span><span style="font-family: Arial, sans-serif; font-size: 9.5pt;">ι</span><span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;"> Dra - mag. +3.3). Directly west of NGC 5866 are the seven stars that form the famous "Plough" or "Big Dipper" asterism of Ursa Major.<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;">NGC 5866 is a challenging binocular object but easier to spot with small scopes. It's best seen from the Northern Hemisphere during the months of April, May and June. From latitudes of 35N or greater, the galaxy is circumpolar and therefore never sets.<o:p></o:p></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;"><a href="http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy" style="font-family: 'Times New Roman'; font-size: medium; line-height: normal;">http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy</a></span></div>
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<span lang="EN-US" style="font-family: Arial, sans-serif; font-size: 9.5pt;"><i><span style="color: #073763;">(Minha, Janine, tradução simples e direta da primeira parte do texto acima)</span></i></span></div>
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<span style="font-family: Arial, sans-serif;"><i><span style="color: #073763;">M102 é uma galáxia catalogada por Charles Messier mas que não foi explicitamente identificada. Pierre Mechain foi quem originalmente observou-a em março de 1781 e ainda antes de passar esta informação para Messier – que catalogou a galáxia sem verificação. No entanto, Mechain acreditou que M102 foi um erro e escreveu uma carta datada de 6 de maio de 1783, expressando sua visão de que o objeto era, de fato, uma duplicata catalogada de M101. A história não termina aí, pois que evidências históricas baseadas na descrição de Messier sobre a galáxia combinaram com as coordenadas sugeridas que M102 poderia bem ser a galáxia lenticular NCG 5866, também conhecida como galáxia do Fuso ou do Eixo. Um número de outros possíveis candidatos foi sugerido porém parece que tanto Messier quanto Mechain observaram NGC 5866 no passado e, portanto, este objeto acabou sendo listado como o item perdido (no Catálogo Messier).</span></i><o:p></o:p></span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">LEIA MAIS SOBRE M102 - NGC 5866</span></b></div>
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<a href="http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy">http://freestarcharts.com/index.php/20-guides/messier/321-messier-102-m102-ngc-5866-spindle-galaxy-lenticular-galaxy</a></div>
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<span style="background-color: white; font-family: Arial, Helvetica, sans-serif;"><b><span style="color: #660000;">NGC 5866 - Galáxia</span></b></span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">Uma galáxia observada de lado </span></div>
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<span style="background-color: white; color: #073763; font-family: Arial, Helvetica, sans-serif;">e mostrando uma banda estreita e escura ao longo de seu equador.<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">- 6<sup>a</sup>. Edição do Atlas Celeste<o:p></o:p></span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt;">de autoria de Ronaldo Rogério de Freitas Mourão,</span></div>
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<span style="color: #0f243e; font-family: Arial, sans-serif; font-size: 11pt; line-height: 22.3999996185303px;">Editora Vozes, Petrópolis, ano de 1986</span></div>
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http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/format/web_print/</div>
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<strong>Object Name:</strong> NGC 5866</div>
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<strong>Image Type:</strong> Astronomical</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> <a href="http://www.nasa.gov/" style="color: #993333;">NASA</a>, <a href="http://www.spacetelescope.org/" style="color: #993333;">ESA</a>, and The <a href="http://heritage.stsci.edu/" style="color: #993333;">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/" style="color: #993333;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="color: #993333;">AURA</a>)</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Acknowledgment:</span> W. Keel (University of Alabama, Tuscaloosa)</div>
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<span style="font-family: arial, sans-serif; font-size: x-small;"><span style="line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/</span></span></div>
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<span style="color: #660000;"><br /></span><span style="color: #660000;"><br /></span><span style="color: #660000;"><br /></span><span style="color: #660000;"><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">NGC 5866</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> ou </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">Galáxia do Fuso</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;"> (e possivelmente </span><b style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">Messier 102</b><span style="background-color: white; font-family: sans-serif; line-height: 22.3999996185303px;">)</span></span><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> é uma </span><a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_lenticular" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Galáxia lenticular">galáxia lenticular</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> localizada a cerca de quarenta milhões de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Anos-luz" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Anos-luz">anos-luz</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> (aproximadamente 12,26</span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Megaparsec" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Megaparsec">megaparsecs</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">) de distância na direção da </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o_do_Drag%C3%A3o" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px;" title="Constelação do Dragão">constelação do Dragão</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Possui uma </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de 9,9, uma declinação de +55º 45' 47" e uma </span><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Ascensão reta">ascensão reta</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> de 15</span><a href="http://pt.wikipedia.org/wiki/Hora" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Hora">horas</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">, 06 </span><a href="http://pt.wikipedia.org/wiki/Minuto" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Minuto">minutos</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;"> e 29,3 </span><a href="http://pt.wikipedia.org/wiki/Segundo" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Segundo">segundos</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">. Contudo, devido à razões históricas, existe a possibilidade de Messier 102 ser uma duplicata de </span><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_101" style="background: none rgb(255, 255, 255); color: #0b0080; font-family: sans-serif; line-height: 22.3999996185303px; text-decoration: none;" title="Messier 101">Messier 101</a><span style="background-color: white; color: #252525; font-family: sans-serif; line-height: 22.3999996185303px;">.</span><br />
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Messier 102 tem sido considerado um objeto perdido por muito tempo e frequentemente tem sido tomado como uma duplicação de <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_101" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 101">Messier 101</a> no <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Catálogo Messier">catálogo de objetos do céu profundo</a> do astrônomo francês <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background: none; color: #0b0080; text-decoration: none;" title="Charles Messier">Charles Messier</a>. Por outro lado, evidências históricas dão conta que M102 poderia ser a galáxia <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5866" style="background: none; color: #0b0080; text-decoration: none;" title="NGC 5866">NGC 5866</a>.<span class="reference" id="cite_ref-seds_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Em meados de 1781, Messier e seu assitente, <a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background: none; color: #0b0080; text-decoration: none;" title="Pierre Méchain">Pierre Méchain</a>, empreenderam um grande projeto com o intuito de descobrir e catalogar novos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background: none; color: #0b0080; text-decoration: none;" title="Objetos do céu profundo">objetos do céu profundo</a>: em abril daquele ano, ambos já tinham verificado as posições de 100 objetos. A data limite para novas adições ao anuário astronômico francês <i><a href="http://pt.wikipedia.org/wiki/Connaissance_des_temps" style="background: none; color: #0b0080; text-decoration: none;" title="Connaissance des temps">Connaissance des temps</a></i> estava se aproximando e Messier adicionou outros três objetos descobertos por Méchain, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_101" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 101">Messier 101</a>, 102 e <a href="http://pt.wikipedia.org/wiki/Messier_103" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 103">103</a>, sem a devida verificação de suas posições. A versão impressa do catálogo contém uma única posição para M101 e M102 e apenas as descrições para M103 são fornecidas. Contudo, Messier adicionou as posições de ambos os objetos em sua cópia pessoal e sempre houve consenso sobre a identidade de M101 e M103.<span class="reference" id="cite_ref-seds_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Cerca de dois anos depois, Méchain retratou sua descoberta e afirmou que sua observação tinha sido um erro, uma observação duplicada de M101. Em 6 de maio de 1783, escreveu uma carta a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Jacob_Bernoulli" style="background: none; color: #0b0080; text-decoration: none;" title="Jacob Bernoulli">Jacob Bernoulli</a> onde descreve suas observações de "nebulosas" que não estavam na edição do catálogo de 1781. Com base nessa carta,<a href="http://pt.wikipedia.org/wiki/Helen_Sawyer_Hogg" style="background: none; color: #0b0080; text-decoration: none;" title="Helen Sawyer Hogg">Helen Sawyer Hogg</a> em 1947 e <a href="http://pt.wikipedia.org/wiki/Owen_Gingerich" style="background: none; color: #0b0080; text-decoration: none;" title="Owen Gingerich">Owen Gingerich</a> em 1953 adicionaram os objetos <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Messier_104" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 104">M104</a> a <a href="http://pt.wikipedia.org/wiki/Messier_109" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 109">M109</a> na versão moderna do catálogo.<span class="reference" id="cite_ref-seds_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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GC 5866 foi sugerido pela primeira vez como candidato ao objeto perdido em 1917 por <a href="http://pt.wikipedia.org/wiki/Camille_Flammarion" style="background: none; color: #0b0080; text-decoration: none;" title="Camille Flammarion">Camille Flammarion</a>, que havia adquirido as cópias pessoais de Messier. Além disso, outro fato torna NGC 5866 bom candidato para M102: situado próximo a ele, cerca de 1 grau ao sul, situa-se a estrela de magnitude aparente 5,25 HR 5635, adequada para ajudar a encontrar o objeto. Portanto, é uma boa candidata para ser a "estrela de magnitude 6" mencionada na descrição de Méchain e Messier: não há nenhuma estrela útil nas vizinhanças de M101 no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background: none; color: #0b0080; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-seds_4-7" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Ainda mais importante para a identificação de M102 é a evidência histórica que Charles Messier provavelmente tenha observado NGC 5866 na tentativa de verificar o objeto M102. Em sua cópia pessoal do catálogo, o astrônomo francês acrescentou posições aproximadas para ambos os objetos M102 e M103, provavelmente logo após a sua publicação em 1781. Estas posições só foram publicadas novamente por Flammarion em 1921.<span class="reference" id="cite_ref-seds_4-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Porém, novamente há erros na descrição do astrônomo francês: não há nenhum objeto óbvio perto da posição descrita por Messier. Mas considerando válido que a referência a "Omicron" seria um erro de impressão e que na verdade seria "Theta", existe de fato um objeto que está situado quase exatamente 5 graus da descrição dada inicialmente por Messier: NGC 5866.<span class="reference" id="cite_ref-seds_4-9" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Messier usava cotidianamente <a href="http://pt.wikipedia.org/wiki/Carta_celeste" style="background: none; color: #0b0080; text-decoration: none;" title="Carta celeste">cartas celestes</a> com grades de linhas com divisões a cada 5 graus e pode ter ocorrido um erro na rotulação do objeto. O astrônomo francês tinha cometido um erro semelhante na redução de dados para o cálculo da posição de um outro objeto ausente, <a href="http://pt.wikipedia.org/wiki/Messier_48" style="background: none; color: #0b0080; text-decoration: none;" title="Messier 48">M48</a>, que também tinha um desvio de 5 graus.<span class="reference" id="cite_ref-seds_4-10" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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Portanto, parece provável que Charles Messier tenha observado NGC 5866 quando media a posição de M102, objeto que ele provavelmente poderia localizar sem muita dificuldade por causa da descrição acurada de Méchain, mas devido a algum erro reducional, foi plotado exatamente 5 graus a oeste de sua posição correta.<span class="reference" id="cite_ref-seds_4-11" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-seds-4" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></div>
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<table border="0" cellpadding="3" class="infobox_v2" style="background: rgb(249, 249, 249); border: 1px solid rgb(170, 170, 170); clear: right; color: black; font-family: sans-serif; font-size: 12px; line-height: 1.1em; margin: 0px 0px 0.5em 1em; padding: 2px; width: 20em;"><tbody>
<tr><th class="" colspan="2" style="background-color: #99c9e6; font-size: 16px; text-align: center; vertical-align: top;"><span class="" style="font-weight: normal;"><span style="font-family: Times New Roman; font-size: small;">NGC 5866 (possivelmente Messier 102)</span></span></th></tr>
<tr><td colspan="2" style="text-align: center;"><div class="center" style="width: 280px;">
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:File-Ngc5866_hst_big.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; margin-left: auto; margin-right: auto;"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="" data-file-height="3756" data-file-width="3190" src="http://upload.wikimedia.org/wikipedia/commons/thumb/5/5c/File-Ngc5866_hst_big.png/280px-File-Ngc5866_hst_big.png" height="330" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5c/File-Ngc5866_hst_big.png/420px-File-Ngc5866_hst_big.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5c/File-Ngc5866_hst_big.png/560px-File-Ngc5866_hst_big.png 2x" style="border: none; margin-left: auto; margin-right: auto; vertical-align: middle;" width="280" /></span></a></div>
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<small><span style="font-family: Times New Roman; font-size: small;">NGC 5866, <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Telesc%C3%B3pio_Espacial_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Telescópio Espacial Hubble">Telescópio Espacial Hubble</a></span></small></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Descoberto por</span></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Pierre_M%C3%A9chain" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Pierre Méchain"><span style="color: black; font-family: Times New Roman; font-size: small;">Pierre Méchain</span></a></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Dados observacionais (J2000)</span></span></th></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Constelação"><span style="color: black; font-family: Times New Roman; font-size: small;">Constelação</span></a></td><td valign="top"><a href="http://pt.wikipedia.org/wiki/Draco" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Draco"><span style="color: black; font-family: Times New Roman; font-size: small;">Draco</span></a></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Tipo</span></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">S0<span class="reference" id="cite_ref-ned_1-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ascensão reta"><span style="color: black; font-family: Times New Roman; font-size: small;">Asc. reta</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">15<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">h</span> 06<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">m</span> 29.5<span style="bottom: 1ex; height: 0px; position: relative; vertical-align: baseline;">s</span><span class="reference" id="cite_ref-ned_1-1" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Declinação"><span style="color: black; font-family: Times New Roman; font-size: small;">Declinação</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">+55° 45′ 48″<span class="reference" id="cite_ref-ned_1-2" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Distância</span></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">50 ± 3 <a href="http://pt.wikipedia.org/wiki/Ano-luz" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Ano-luz">Mal</a> (15,3 ± 0,7 <a href="http://pt.wikipedia.org/wiki/Parsec" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Parsec">Mpc</a><span class="reference" id="cite_ref-tonryetal2001_2-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-tonryetal2001-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">2</a></span> )</span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Desvio_para_o_vermelho" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Desvio para o vermelho"><span style="color: black; font-family: Times New Roman; font-size: small;">Redshift</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">672 ± 9 km/<a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Segundo">s</a><span class="reference" id="cite_ref-ned_1-3" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Magnitude aparente"><span style="color: black; font-family: Times New Roman; font-size: small;">Magnit. apar.</span></a></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">10,7<span class="reference" id="cite_ref-ned_1-4" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><td scope="row" valign="top"><span style="font-family: Times New Roman; font-size: small;">Dimensões</span></td><td valign="top"><span style="font-family: Times New Roman; font-size: small;">4′,7 x 1′,9<span class="reference" id="cite_ref-ned_1-5" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Outras denominações</span></span></th></tr>
<tr><td colspan="2" style="text-align: center;" valign="top"><span style="font-family: Times New Roman; font-size: small;">Galáxia do Fuso,<span class="reference" id="cite_ref-simbad_3-0" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-simbad-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">3</a></span> <a href="http://pt.wikipedia.org/wiki/Uppsala_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Uppsala General Catalogue">UGC</a> 9723,<span class="reference" id="cite_ref-ned_1-6" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span> <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Principal_Galaxies_Catalogue&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Principal Galaxies Catalogue (página não existe)">PGC</a> 53933<span class="reference" id="cite_ref-ned_1-7" style="bottom: 1ex; height: 0px; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Messier_102#cite_note-ned-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;">1</a></span></span></td></tr>
<tr><th colspan="2" style="background-color: #99c9e6; text-align: center; vertical-align: top;"><span style="font-family: Times New Roman; font-size: small;"><span style="font-weight: normal;">Mapa</span></span></th></tr>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Locator_Dot2.gif" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;" title="Messier 102"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Messier 102" data-file-height="15" data-file-width="15" src="http://upload.wikimedia.org/wikipedia/commons/thumb/e/e2/Locator_Dot2.gif/12px-Locator_Dot2.gif" height="12" srcset="//upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/e/e2/Locator_Dot2.gif 2x" style="border: none; vertical-align: middle;" width="12" /></span></a></div>
<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Draco_constellation_map.png" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial;"><span style="color: black; font-family: Times New Roman; font-size: small;"><img alt="Draco constellation map.png" data-file-height="2839" data-file-width="2559" src="http://upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Draco_constellation_map.png/240px-Draco_constellation_map.png" height="266" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Draco_constellation_map.png/360px-Draco_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f0/Draco_constellation_map.png/480px-Draco_constellation_map.png 2x" style="border: none; vertical-align: middle;" width="240" /></span></a></div>
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http://pt.wikipedia.org/wiki/Messier_102<br />
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<span style="background-color: white;"><span style="color: #073763;">Hubble Sees Galaxy on Edge</span></span></h1>
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<img src="http://imgsrc.hubblesite.org/hu/db/images/hs-2006-24-a-xlarge_web.jpg" /></div>
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http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/format/xlarge_web/</div>
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<strong>Object Name:</strong> NGC 5866</div>
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<strong>Image Type:</strong> Astronomical</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Credit:</span> <a href="http://www.nasa.gov/" style="color: #993333;">NASA</a>, <a href="http://www.spacetelescope.org/" style="color: #993333;">ESA</a>, and The <a href="http://heritage.stsci.edu/" style="color: #993333;">Hubble Heritage</a> Team (<a href="http://www.stsci.edu/" style="color: #993333;">STScI</a>/<a href="http://www.aura-astronomy.org/" style="color: #993333;">AURA</a>)</div>
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<span class="import" style="font-weight: bold; line-height: 18.2000007629395px;">Acknowledgment:</span> W. Keel (University of Alabama, Tuscaloosa)</div>
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<span style="font-family: arial, sans-serif; font-size: x-small;"><span style="line-height: 18.2000007629395px;">http://hubblesite.org/newscenter/archive/releases/2006/24/image/a/</span></span></div>
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<b><span style="color: #660000;">O Grupo NGC 5866 é um pequeno <a class="new" href="http://pt.wikipedia.org/w/index.php?title=Grupo_de_gal%C3%A1xias&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Grupo de galáxias (página não existe)">grupo de galáxias</a> na direção da <a href="http://pt.wikipedia.org/wiki/Constela%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Constelação">constelação</a> de <a href="http://pt.wikipedia.org/wiki/Draco" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="Draco">Draco</a>. O grupo está nomeado como <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5866" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; text-decoration: none;" title="NGC 5866">NGC 5866</a></span></b><span style="color: #252525;">, pois ela é galáxia com maior </span><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">magnitude aparente</a><span style="color: #252525;"> no grupo, embora alguns catálogos de grupos de galáxias listam </span><a href="http://pt.wikipedia.org/wiki/NGC_5907" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5907">NGC 5907</a><span style="color: #252525;"> como o membro mais brilhante.</span><span class="reference" id="cite_ref-garcia1993_1-5" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span><span style="color: #252525;"> </span><span class="reference" id="cite_ref-giuricinetal2002_2-7" style="bottom: 1ex; color: #252525; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-giuricinetal2002-2" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<span class="mw-headline" id="Membros" style="font-family: 'Linux Libertine', Georgia, Times, serif; font-size: large; line-height: 1.3;">Membros</span></div>
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A tabela abaixo lista todas as <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xias" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxias">galáxias</a> identificadas e confirmadas como membros do grupo pelo Nearby Galaxies Catalog,<span class="reference" id="cite_ref-nbg_3-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-nbg-3" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">3</a></span> o Lyons Groups of Galaxies (LGG) Catalog,<span class="reference" id="cite_ref-garcia1993_1-6" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-garcia1993-1" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">1</a></span> e três listas de grupos criados pelo Nearby Optical Galaxy sample of Giuricin et al.<span class="reference" id="cite_ref-giuricinetal2002_2-8" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-giuricinetal2002-2" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">2</a></span></div>
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<table cellpadding="2" class="wikitable" style="background-color: #f9f9f9; border-collapse: collapse; border: 1px solid rgb(170, 170, 170); color: black; font-family: sans-serif; font-size: 14px; line-height: 22.3999996185303px; margin: 1em 0px; text-align: center;"><caption style="font-weight: bold;"><b>Membros do Grupo NGC 5866</b></caption><tbody>
<tr><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;">Nome</th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Classifica%C3%A7%C3%A3o_de_Hubble" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Classificação de Hubble">Tipo</a><span class="reference" id="cite_ref-ned_4-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Ascens%C3%A3o_reta" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Ascensão reta">R.A.</a> (J2000)<span class="reference" id="cite_ref-ned_4-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Declina%C3%A7%C3%A3o" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Declinação">Dec.</a> (J2000)<span class="reference" id="cite_ref-ned_4-2" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Redshift" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Redshift">Redshift</a> (<a href="http://pt.wikipedia.org/wiki/Quil%C3%B4metro" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Quilômetro">km</a>/<a href="http://pt.wikipedia.org/wiki/Segundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Segundo">s</a>)<span class="reference" id="cite_ref-ned_4-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th><th style="background: rgb(239, 239, 239); border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/Magnitude_aparente" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Magnitude aparente">Magnitude</a><span class="reference" id="cite_ref-ned_4-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ned-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none; white-space: nowrap;">4</a></span></th></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a class="mw-redirect" href="http://pt.wikipedia.org/wiki/NGC_5866" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5866">NGC 5866</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">S0</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 06<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 29.5<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+55° 45′ 48″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">672 ± 9</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">10.7</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/NGC_5879" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5879">NGC 5879</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SA(rs)bc</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 09<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 46.8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+57° 00′ 01″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">772 ± 5</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">12.4</td></tr>
<tr><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;"><a href="http://pt.wikipedia.org/wiki/NGC_5907" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5907">NGC 5907</a></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">SA(s)c</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">h</span> 15<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">m</span> 53.8<span style="bottom: 1ex; height: 0px; line-height: 1; position: relative; vertical-align: baseline;">s</span></td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">+56° 19′ 44″</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">667 ± 3</td><td style="border: 1px solid rgb(170, 170, 170); padding: 0.2em;">11.1</td></tr>
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Outros possíveis membros (galáxias listadas com uma ou duas de algumas referências acima) incluem <a class="new" href="http://pt.wikipedia.org/w/index.php?title=NGC_5866B&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="NGC 5866B (página não existe)">NGC 5866B</a>, <a href="http://pt.wikipedia.org/wiki/NGC_5963" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="NGC 5963">NGC 5963</a>, <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_9776&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="UGC 9776 (página não existe)">UGC 9776</a> e <a class="new" href="http://pt.wikipedia.org/w/index.php?title=UGC_9816&action=edit&redlink=1" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #a55858; text-decoration: none;" title="UGC 9816 (página não existe)">UGC 9816</a>.</div>
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<span class="mw-headline" id="Grupos_pr.C3.B3ximos">Grupos próximos</span></h2>
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O Grupo NGC 5866 está localizado ao noroeste do <a href="http://pt.wikipedia.org/wiki/Grupo_M101" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grupo M101">Grupo M101</a> (que contém a <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Catavento" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Catavento">Galáxia do Catavento (M101)</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_sat%C3%A9lite" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia satélite">galáxias satélites</a> e companheiras) e o <a href="http://pt.wikipedia.org/wiki/Grupo_M51" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Grupo M51">Grupo M51</a> (que contém a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Rodamoinho" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Rodamoinho">Galáxia do Rodamoinho (M51)</a>, a<a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_do_Girassol" style="background-attachment: initial; background-clip: initial; background-color: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #0b0080; text-decoration: none;" title="Galáxia do Girassol">Galáxia do Girassol (M63)</a> e algumas outras galáxias)<span class="reference" id="cite_ref-ferrareseetal00_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ferrareseetal00-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> . As distâncias para estes três grupos (como determinadas pelas distâncias para os membros individuais) são similares, com sugestões de que o Grupo M51, o Grupo M101 e o Grupo NGC 5866 são atualmente parte de um grande, e solta, larga estrutura.<span class="reference" id="cite_ref-ferrareseetal00_5-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Grupo_NGC_5866#cite_note-ferrareseetal00-5" style="background: none; color: #0b0080; text-decoration: none; white-space: nowrap;">5</a></span> Contudo, a maior parte de métodos para identificação (incluindo por referências citadas acima) têm estes três grupos como grupos separados.</div>
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http://pt.wikipedia.org/wiki/Grupo_NGC_5866</div>
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<br /><a href="http://apod.nasa.gov/apod/image/0606/ngc5866_hst_big.jpg"><img alt="See Explanation. Clicking on the picture will download
the highest resolution version available." src="http://apod.nasa.gov/apod/image/0606/ngc5866_hst.jpg" /></a></center>
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<b>http://apod.nasa.gov/apod/ap060612.html</b></center>
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<b>Edge-On Galaxy NGC 5866 </b><br /><b>Credit: </b><a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, and The <a href="http://heritage.stsci.edu/">Hubble Heritage</a> <a href="http://heritage.stsci.edu/commonpages/infoindex/ourproject/moreproject.html">Team</a> (<a href="http://www.stsci.edu/resources/">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>); <b>Acknowledgment: </b><a href="http://www.astr.ua.edu/keel/billkeel.html">W. Keel</a> (<a href="http://www.astr.ua.edu/">U. Alabama</a>)</center>
<b>Explanation: </b>Why is this galaxy so thin? Many disk galaxies are actually just as thin as NGC 5866, <a href="http://hubblesite.org/newscenter/newsdesk/archive/releases/2006/24/">pictured above</a>, but are not <a href="http://apod.nasa.gov/apod/ap010510.html">seen edge-on</a> from our vantage point. One galaxy that is situated edge-on is our own <a href="http://apod.nasa.gov/apod/ap050605.html">Milky Way Galaxy</a>. Classified as a <a href="http://apod.nasa.gov/apod/ap020408.html">lenticular galaxy</a>, NGC 5866 has numerous and complex dust lanes appearing dark and red, while many of the bright stars in the disk give it a more blue underlying hue. The blue disk of young stars can be seen extending past the <a href="http://apod.nasa.gov/apod/ap990919.html">dust</a> in the extremely thin galactic plane, while the bulge in the disk center appears tinged more orange from the older and redder stars that likely exist there. Although similar in mass to our Milky Way Galaxy, light takes about 60,000 <a href="http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html">years</a> to cross <a href="http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...20311002K">NGC 5866</a>, about 30 percent less than light takes to cross our own Galaxy. In general, many disk galaxies are very thin because the gas that <a href="http://en.wikipedia.org/wiki/Galaxy_formation_and_evolution">formed them</a> collided with itself as it rotated about the gravitational center. Galaxy <a href="http://en.wikipedia.org/wiki/NGC_5866">NGC 5866</a> lies about 44 million light years distant toward the constellation of the Dragon (<a href="http://www.astronomical.org/portal/modules/wfsection/article.php?articleid=34">Draco</a>).</div>
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<span style="color: #660000; font-family: Arial, Helvetica, sans-serif;"><b>O CATÁLOGO MESSIER</b></span></div>
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O <b>Catálogo Messier</b> é um <a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Catálogo astronômico">catálogo astronômico</a> composto por 110 <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu profundo">objetos do céu profundo</a>, compilado pelo <a href="http://pt.wikipedia.org/wiki/Astronomia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Astronomia">astrônomo</a> <a href="http://pt.wikipedia.org/wiki/Fran%C3%A7a" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="França">francês</a> <a href="http://pt.wikipedia.org/wiki/Charles_Messier" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Charles Messier">Charles Messier</a> entre 1764 e 1781.<span class="reference" id="cite_ref-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-1" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">1</a></span>Originalmente com o nome "<i>Catalogue des Nébuleuses et des amas d'Étoiles, que l'on découvre parmi les Étoiles fixes sur l'horizon de Paris</i>" (<i>Catálogo de Nebulosas e Aglomerados Estelares Observados entre as Estrelas Fixas sobre o Horizonte de Paris</i>), foi construído com objetivo de identificar objetos do céu profundo, como<a href="http://pt.wikipedia.org/wiki/Nebulosa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa">nebulosas</a>, <a href="http://pt.wikipedia.org/wiki/Aglomerado_estelar" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Aglomerado estelar">aglomerados estelares</a> e <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia">galáxias</a> que poderiam ser confundidos com <a href="http://pt.wikipedia.org/wiki/Cometa" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa">cometas</a>, objetos de brilho fraco e difusos no <a href="http://pt.wikipedia.org/wiki/C%C3%A9u_noturno" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Céu noturno">céu noturno</a>.<span class="reference" id="cite_ref-inic_2-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-inic-2" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">2</a></span></div>
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Antes de Messier, vários outros astrônomos elaboraram catálogos semelhantes, como a lista de seis objetos de <a href="http://pt.wikipedia.org/wiki/Edmond_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Edmond Halley">Edmond Halley</a>,<span class="reference" id="cite_ref-3" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-3" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">3</a></span> o catálogo de <a href="http://pt.wikipedia.org/wiki/William_Derham" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="William Derham">William Derham</a>, baseado no catálogo de estrelas de <a href="http://pt.wikipedia.org/wiki/Johannes_Hevelius" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Johannes Hevelius">Johannes Hevelius</a>, o <i>Prodomus Astronomiae</i>, o Catálogo das Nebulosas do Sul de <a href="http://pt.wikipedia.org/wiki/Nicolas_Louis_de_Lacaille" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nicolas Louis de Lacaille">Nicolas Louis de Lacaille</a>, de 1755, bem como as listas de<a href="http://pt.wikipedia.org/wiki/Giovanni_Domenico_Maraldi" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Giovanni Domenico Maraldi">Giovanni Domenico Maraldi</a> e <a href="http://pt.wikipedia.org/wiki/Guillaume_Le_Gentil" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Guillaume Le Gentil">Guillaume Le Gentil</a> e <a href="http://pt.wikipedia.org/wiki/Jean-Philippe_de_Ch%C3%A9seaux" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Jean-Philippe de Chéseaux">Jean-Philippe de Chéseaux</a>. Os diferentes objetos do catálogo são designados pela letra M seguida de um número, que corresponde à ordem cronológica das descobertas ou inclusões: assim, <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">M1</a> corresponde ao primeiro objeto catalogado, enquanto que a <a href="http://pt.wikipedia.org/wiki/Gal%C3%A1xia_de_Andr%C3%B4meda" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Galáxia de Andrômeda">galáxia de Andrômeda</a>, conhecida desde a <a href="http://pt.wikipedia.org/wiki/Idade_M%C3%A9dia" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Idade Média">Idade Média</a>, é apenas o objeto M31. Os objetos do catálogo, conhecidos como "Objetos Messier", também constam em outros catálogos mais recentes, como o <a href="http://pt.wikipedia.org/wiki/New_General_Catalogue" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="New General Catalogue">New General Catalogue</a> (NGC).</div>
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<span class="mw-headline" id="Hist.C3.B3ria">História</span></h2>
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<a class="image" href="http://pt.wikipedia.org/wiki/Ficheiro:Crab_Nebula.jpg" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;"><img alt="" class="thumbimage" data-file-height="3864" data-file-width="3864" height="220" src="http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/220px-Crab_Nebula.jpg" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/330px-Crab_Nebula.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/00/Crab_Nebula.jpg/440px-Crab_Nebula.jpg 2x" style="-webkit-box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; background-attachment: initial; background-clip: initial; background-color: #f2eee4; background-image: initial; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; border-radius: 0px; border: 1px solid rgb(204, 204, 204); box-shadow: rgba(0, 0, 0, 0.2) 0px 0px 0px; padding: 8px; position: relative; vertical-align: middle;" width="220" /></a><br /><div class="thumbcaption" style="border: none; font-size: 12px; line-height: 1.4em; padding: 3px; text-align: left;">
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A <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">nebulosa do Caranguejo</a> (M1), a primeira entrada do Catálogo Messier</div>
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Messier foi motivado a elaborar o catálogo enquanto estava à procura do <a href="http://pt.wikipedia.org/wiki/Cometa_Halley" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Cometa Halley">cometa Halley</a> em 1758.<span class="reference" id="cite_ref-4" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-4" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">4</a></span> <span class="reference" id="cite_ref-buscab_5-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-buscab-5" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">5</a></span> Segundo os cálculos orbitais de <a href="http://pt.wikipedia.org/wiki/Joseph-Nicolas_Delisle" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Joseph-Nicolas Delisle">Joseph-Nicolas Delisle</a>, chefe do<a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Observat%C3%B3rio_astron%C3%B4mico" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Observatório astronômico">observatório astronômico</a> onde ele trabalhava, Halley reapareceria na <a href="http://pt.wikipedia.org/wiki/Taurus" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Taurus">constelação do Touro</a>.<span class="reference" id="cite_ref-Delisle_6-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-Delisle-6" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">6</a></span> Enquanto observava o céu noturno à procura de Halley, descobriu independentemente outro cometa<span class="reference" id="cite_ref-cometas_7-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-cometas-7" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">7</a></span> e um objeto de aparência semelhante, mas que não se movia em relação às estrelas vizinhas, sendo o primeiro <a class="mw-redirect" href="http://pt.wikipedia.org/wiki/Objetos_do_c%C3%A9u_profundo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Objetos do céu profundo">objeto do céu profundo</a>descoberto pelo astrônomo francês. Esse objeto é conhecido atualmente como a <a href="http://pt.wikipedia.org/wiki/Nebulosa_do_Caranguejo" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Nebulosa do Caranguejo">Nebulosa do Caranguejo</a>, o <a href="http://pt.wikipedia.org/wiki/Remanescente_de_supernova" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="Remanescente de supernova">remanescente</a> da <a href="http://pt.wikipedia.org/wiki/SN_1054" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none;" title="SN 1054">supernova de 1054</a>.<span class="reference" id="cite_ref-crab_nebula_8-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-crab_nebula-8" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">8</a></span></div>
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Com o objetivo de não mais confundir esses objetos difusos e fixos com cometas, Messier decidiu procurar outros objetos que poderiam enganar a si próprio e a outros astrônomos e decidiu incluí-los em um catálogo que descrevesse suas posições exatas e características.<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-0" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span> Segundo o próprio astrônomo:</div>
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<dl style="font-family: sans-serif; font-size: 16px; line-height: 22.3999996185303px; margin-bottom: 0.5em; margin-top: 0.2em; text-align: start;"><dd style="line-height: 1.5em; margin-bottom: 0.1em; margin-left: 1.6em; margin-right: 0px;"><div style="text-align: center;">
"O que me levou a construir o catálogo foi a descoberta da nebulosa I acima do chifre sul de Touro em 12 de setembro de 1758, enquanto observava o cometa daquele ano. Esta nebulosa tinha tamanha semelhança com um cometa em sua forma e brilho e me esforcei para encontrar os outros, de modo que os astrônomos não mais confundissem estas mesmas nebulosas com cometas."<span class="reference" id="cite_ref-ca.C3.A7adordecometas_9-1" style="bottom: 1ex; height: 0px; line-height: 1; position: relative; unicode-bidi: -webkit-isolate; vertical-align: baseline;"><a href="http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier#cite_note-ca.C3.A7adordecometas-9" style="background-attachment: initial; background-clip: initial; background-image: none; background-origin: initial; background-position: initial; background-repeat: initial; background-size: initial; color: #274e13; text-decoration: none; white-space: nowrap;">9</a></span></div>
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SAIBA MUITO MAIS, acessando</div>
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<span style="font-family: Arial, Helvetica, sans-serif;">http://pt.wikipedia.org/wiki/Cat%C3%A1logo_Messier</span></div>
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<span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><span style="font-size: 16px; line-height: 22.3999996185303px;"><br /></span><span style="font-size: 16px; line-height: 22.3999996185303px;"></span><br /><div class="MsoNormal" style="font-size: 16px; line-height: 22.3999996185303px;">
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Os desenhos formados pelas estrelas</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> - AS CONSTELAÇÕES - </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>são como janelas que se abrem para a infinitude do universo </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>e que possibilitam nossa mente a ir percebendo que existe mais, bem mais,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> entre o céu e a terra..., </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>bem como percebendo que o caos, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vagarosamente,</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>vai se tornando Cosmos</b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b> e este por nossa mente sendo conscientizado.<o:p></o:p></b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Quer dizer, </b></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>nossa mente é tão infinita quanto infinito é o Cosmos.</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Com um abraço estrelado,</b><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span><br /><div>
<span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><span style="font-family: Arial, Helvetica, sans-serif;"><b><br /></b></span><br /><div style="font-family: 'Times New Roman'; font-size: medium; line-height: 18px;">
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<span style="font-family: Arial, Helvetica, sans-serif;">Alguns dados apresentados neste Trabalho<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">devem requerer do Caro Leitor</span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">alguma pequena retificação.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Obrigada por sua compreensão.<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">Visitando os Sites abaixo,<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"> você conseguirá informações atualizadas e preciosas<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">sobre os Objetos Celestiais de seu interesse:<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;">NASA/IPAC EXTRAGALACTIC DATABASE –<o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://ned.ipac.caltech.edu/forms/byname.html" style="color: #274e13; text-decoration: none;">http://ned.ipac.caltech.edu/forms/byname.html</a><o:p></o:p></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><em><span lang="EN-US">NASA/IPAC Extragalactic Database (NED) -</span></em><span class="apple-converted-space"><i><span lang="EN-US"> </span></i></span><em><span lang="EN-US"> operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.</span></em><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">THE NIGHT SKY ATLAS<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.nightskyatlas.com/index.jsp" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.nightskyatlas.com/index.jsp</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">The night sky atlas creates images of any part of the night sky, allowing easy location of any object. Detailed chart images show all stars visible to the naked eye, the constellations, Messier objects, and names of the brightest stars.<o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><span lang="EN-US">The</span><span class="apple-converted-space"><span lang="EN-US"> </span></span><span lang="EN-US">Internet STELLAR DATABASE</span><span lang="EN-US"><o:p></o:p></span></span></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><a href="http://www.stellar-database.com/" style="color: #274e13; text-decoration: none;"><span lang="EN-US">http://www.stellar-database.com/</span></a><span lang="EN-US"><o:p></o:p></span></span></div>
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<span lang="EN-US"><span style="font-family: Arial, Helvetica, sans-serif;">- stars within 75 light-years. (Plus some of the more well-known "name brand" stars farther away.)</span></span></div>
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<b><span style="font-family: Arial, Helvetica, sans-serif;">COM UM ABRAÇO ESTRELADO,</span></b></div>
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<span style="font-family: Arial, Helvetica, sans-serif;"><b>Janine Milward</b></span></div>
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