File:Dustiest Star Could Harbor a Young Earth (gemini0506a).tiff
Summary
| Description |
English: Artist's conception of a possible collision around BD +20 307 that might have created some of the dust observed in the recent Gemini/ Keck observations. The collisions responsible for this dust could range in size from the largest known asteroids (approximated here) to planets the size of the Earth or Mars. |
| Date | 20 July 2005 (upload date) |
| Source | Dustiest Star Could Harbor a Young Earth |
| Author | NOIRLab |
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Licensing
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This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab). Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. |
  This file is licensed under the Creative Commons Attribution 4.0 International license.
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