https://arolstar52-zhtest.hf.space/index.php?action=history&feed=atom&title=NGC_2080 NGC 2080 - 版本历史 2026-07-19T04:41:53Z 本wiki上该页面的版本历史 MediaWiki 1.43.9 https://arolstar52-zhtest.hf.space/index.php?title=NGC_2080&diff=162742&oldid=prev imported>InternetArchiveBot：​Add 1 book for verifiability (20250707)) #IABot (v2.0.9.5) (GreenC bot 2025-07-08T00:32:44Z <p>Add 1 book for verifiability (20250707)) #IABot (v2.0.9.5) (<a href="/index.php?title=User:GreenC_bot&amp;action=edit&amp;redlink=1" class="new" title="User:GreenC bot（页面不存在）">GreenC bot</a></p> <p><b>新页面</b></p><div>{{Infobox nebula<br /> | image = NGC2080.jpg<br /> |caption = A [[Hubble Space Telescope|HST]] image of a Star-forming region NGC 2080.<br /> | credit = [[NASA]]/[[ESA]]<br /> | name = [[New General Catalogue|NGC]] 2080<br /> | type = 發射星雲<br /> | epoch = J2000.0<br /> | ra = {{RA|05|39|44.2}}<br /> | dec = {{DEC|-69|38|44}}<br /> | dist_ly = 160,000<br /> | appmag_v = <br /> | size_v = <br /> | constellation = [[劍魚座]]<br /> | radius_ly = <br /> | absmag_v = <br /> | notes = <br /> | names = ESO 057-EN012, &lt;br&gt;h 2950, GC 1278<br /> }}<br /> {{NGCInfoBox|NGCID=NGC 2080|發現者=約翰·弗里德里希·威廉·赫歇爾|發現日期=1834年12月-日|其他編號=ESO 57-EN12|曆元=J2000.0|赤經=5時39分44.2秒<br /> |赤緯=-69°38&#039;44&quot;|星座=剑鱼座|星體=發射星雲|星等=|表面亮度=|藍等=}}<br /> <br /> &#039;&#039;&#039;NGC 2080&#039;&#039;&#039; 又稱鬼頭星雲，是位於[[劍魚座]][[大麥哲倫星系]][[蜘蛛星雲]]南部的恆星形成區和發射星雲。大麥哲倫星雲是[[銀河系]]的[[衛星星系]]，距離[[地球]]168,000光年&lt;ref name=&quot;objects&quot;&gt;{{cite book |title = 300 Astronomical Objects: A Visual Reference to the Universe |url = https://archive.org/details/300astronomicalo0000wilk |last1=Wilkins |first1=Jamie |last2=Dunn |first2 = Robert |publisher = Firefly Books |date = 2006 |edition = 1st |location=Buffalo, New York |isbn = 978-1-55407-175-3}}&lt;/ref&gt;。<br /> <br /> NGC 2080由[[約翰·赫歇爾]]於1834年發現&lt;ref&gt;{{cite web |url = http://messier.seds.org/xtra/ngc/lmc_more.html |title = More LMC objects |publisher = SEDS |last1 = Frommert |first1 = Hartmut |last2 = Kronberg |first2 = Christine |date = 19 April 2006 |access-date = 7 May 2012}}&lt;/ref&gt;。鬼頭星雲的直徑為50[[光年]]&lt;ref&gt;{{Cite APOD |title = Halloween and the Ghost Head Nebula |date = 31 October 2001 |access-date = 7 May 2012}}&lt;/ref&gt;，因擁有的兩個明顯的白色斑塊而得名，被稱為“鬼眼”。西部斑塊稱為A1，其中心有一個氣泡，是由其所含的年輕大質量恆星產生的。東部的區域稱為A2，由新形成的星團中的幾顆年輕恆星組成，但它們仍然被其起源的塵埃雲所遮蔽。由於兩組塵埃雲都沒有因恆星輻射而消散，天文學家推斷這兩組恆星都是在過去10,000年內形成的。這些[[恆星]]開始在星雲中形成一個氣泡，噴湧出被稱為[[恆星風]]的物質&lt;ref&gt;{{cite web |url = http://www.spacetelescope.org/news/heic0114/ |title = Painting with oxygen and hydrogen |date = 18 October 2001 |publisher = [[ESA]] |access-date = 7 May 2012}}&lt;/ref&gt;。<br /> <br /> ==參考資料==<br /> {{reflist}}<br /> <br /> {{剑鱼座恒星}}<br /> {{NGCReference|2080}}<br /> {{Catalogs|NGC=2080}}</div> imported>InternetArchiveBot