File:A disc of rocky debris from a disrupted planetesimal (geminiann17003a).jpg
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摘要
| 描述 |
English: A disc of rocky debris from a disrupted planetesimal surrounds white dwarf plus brown dwarf binary star. The white dwarf is the burned-out core of a star that was probably similar to the Sun, the brown dwarf is only ~60 times heavier than Jupiter, and the two stars go around each other in only a bit over two hours. |
| 日期 | 2017年2月23日, 13:58:00 (上傳日期) |
| 來源 | A disc of rocky debris from a disrupted planetesimal |
| 作者 | International Gemini Observatory/NOIRLab/NSF/AURA/UCL/University of Warwick/University of Sheffield//Mark Garlick |
| 其他版本 |
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This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
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| 目前 | 2023年10月22日 (日) 23:05 | | 4,500 × 6,000（3.01 MB） | OptimusPrimeBot | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann17003a.jpg via Commons:Spacemedia |
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