集信:M42proplyds.jpg
M42proplyds.jpg (510×381點影、戟𡱩集信:13kB、矯MIME:image/jpeg)
集信尼得留於威其迷𠫾阿・古門吧伮固体得使用於各預案恪。 𠳒描寫𧵑集信在張模寫得顯示𨑜低。
DescriptionM42proplyds.jpg |
A Hubble Space Telescope view of a small portion of the Orion Nebula, captured by the Wide Field and Planetary Camera 2, reveals five young stars. Four of the stars are surrounded by gas and dust trapped as the stars formed, but were left in orbit about the star. These are possibly protoplanetary disks, or proplyds, that might evolve on to agglomerate planets. The proplyds which are closest to the hottest stars of the parent star cluster are seen as bright objects, while the object farthest from the hottest stars is seen as a dark object. The field of view is only 0.14 light-years across. The Orion Nebula star-birth region is 1500 light-years away, in the direction of the constellation Orion the Hunter. العربية: صورة هابل لأقراص الكواكب الأولية في سديم الجبار، وهو «حضانة نجمية» تمتد على مدى سنوات ضوئية من المحتمل أن تكون مشابهة جدًا للسديم الأولي الذي تشكلت منه الشمس. |
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Date | ||||
Source | http://hubblesite.org/newscenter/archive/releases/1994/24/image/b/ (direct link) | |||
Author | C.R. O'Dell/Rice University; NASA | |||
Permission (Reusing this file) |
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Items portrayed in this file
depicts English
inception English
29 December 1993
歷史集信
扨𠓨𣈜/𣇞抵䀡內容集信在時點妬。
𣈜/𣇞 | 形䀡𠓀 | 戟櫸 | 成員 | 描寫 | |
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現在 | 18:11、𣈜21𣎃12𢆥2009 | 510×381 (13kB) | wikimediacommons>Tryphon | Original image, from http://imgsrc.hubblesite.org/hu/db/images/hs-1994-24-b-full_jpg.jpg. |
張使用集信
張𢖖󠄁使用集信尼:
特性形
集信尼貯通信補充、固体得添自𣛠影技術數或𣛠𢭯得使用抵造或數化𣜿。
裊集信㐌得𢯢𢷮𬧺貝狀態班頭、𠬠數枝節固体空反映𣹓𨁥集信㐌𢯢𢷮。
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