File:Bright Supernova Sn2006gy.jpg

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English: This artist's illustration shows what SN 2006gy may have looked like if viewed at a close distance. The fireworks-like material in white shows the explosion of an extremely massive star. This debris is pushing back two lobes of cool, red gas that were expelled in a large eruption from the star before it exploded. The green, blue and yellow regions in these lobes shows where gas is being heated in a shock front as the explosion material crashes into it and pushes it backwards. Most of the optical light generated by the supernova is thought to come from debris that has been heated by radioactivity, but some likely comes from the shocked gas.
Date (released)
Source http://solarsystem.nasa.gov/multimedia/display.cfm?Category=Planets&IM_ID=9947; see also http://chandra.harvard.edu/photo/2007/sn2006gy/
Author Illustration: NASA/CXC/M.Weiss; X-ray: NASA/CXC/UC Berkeley/N.Smith et al.; IR: Lick/UC Berkeley/J.Bloom & C.Hansen

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current17:49, 30 January 2013Thumbnail for version as of 17:49, 30 January 20132,025 × 2,504 (542 KB)Stas1995 (talk | contribs)User created page with UploadWizard

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