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描述 The explosion of a massive star blazes with the light of 200 million Suns in this NASA/ESA Hubble Space Telescope image. The arrow at top right points to the stellar blast, called a supernova. The supernova is so bright in this image that it easily could be mistaken for a foreground star in our Milky Way Galaxy. And yet, this supernova, called SN 2004dj, resides far beyond our galaxy. Its home is in the outskirts of NGC 2403, a galaxy located 11 million light-years from Earth. Although the supernova is far from Earth, it is the closest stellar explosion discovered in more than a decade.
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来源 http://www.spacetelescope.org/images/opo0423a/
作者 NASA, ESA, A.V. Filippenko (University of California, Berkeley), P. Challis (Harvard-Smithsonian Center for Astrophysics), et al.
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This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

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当前2010年5月25日 (二) 17:362010年5月25日 (二) 17:36版本的缩略图3,880 × 3,952(3.04 MB)TryphonOriginal size, from http://hubblesite.org/newscenter/archive/releases/2004/23/image/a/ (http://imgsrc.hubblesite.org/hu/db/images/hs-2004-23-a-full_jpg.jpg).
2006年8月20日 (日) 15:582006年8月20日 (日) 15:58版本的缩略图785 × 800(129 KB)Bgvr{{Information |Description=NGC 2403 |Source=http://hubblesite.org/newscenter/newsdesk/archive/releases/2004/23/image/ |Date=August 17, 2004 |Author=NASA, ESA, and A. Filippenko (University of California, Berkeley) |Permission=Material credited to STScI on

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