File:SN 1006.jpg

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English: Chandra's image of SN 1006 shows X-rays from multimillion degree gas (red/green) and high-energy electrons (blue). In the year 1006 a "new star" appeared in the sky and in just a few days it became brighter than the planet Venus. We now know that the event heralded not the appearance of a new star, but the cataclysmic death of an old one. It was likely a white dwarf star that had been pulling matter off an orbiting companion star. When the white dwarf mass exceeded the stability limit (known as the Chandrasekhar limit), it exploded. Material ejected in the supernova produced tremendous shock waves that heated gas to millions of degrees and accelerated electrons to extremely high energies.
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来源 https://www.flickr.com/photos/25053835@N03/2940666879/in/photolist-5tRFP6-avs4hH-6JHxst-ehJDeH-7owauz-4NC1Me-cMi4E1-7Dhfo3-avrgBx-eokkqh-7DhH5q-8ajz1T-75AgWF-dHvEBe-cXXbgy-dGNSPX-dGNSzH-dGUk8S-dGUjTd-dGUjDU-avKM2D-afkfBd-8kNJEu-cE13Vs-cE1423-cE148S-cE145f-cE13YJ-drZjvP-7MTuTd-ffWzke-9Uhs6J-dWHrNy-dWHrLE-dWBNu6-dWBNU2-dWBNrv-dWBNAR-dWHrzb-dWBNwn-dWHrv1-dWBNGi-dWHrJy-dWBNLB-dWHrDW-da9SvS-9E412Y-7DeD7V-5B6PNC-dWHrdb-dWHrkd
作者 Smithsonian Institution

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本图原来发表于Flickr，作者为Smithsonian Institution，网址为https://www.flickr.com/photos/25053835@N03/2940666879；经FlickreviewR于2013-08-04 19:51:24审查后，确认本图以No known copyright restrictions释出，相容于维基共享资源。然而上述的授权条款与来源处不同，因而无法确定本页所提供的授权条款是否有效。
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