File:Numerical simulation of possible surface temperatures on Proxima b (synchronous rotation).ogv
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[edit]DescriptionNumerical simulation of possible surface temperatures on Proxima b (synchronous rotation).ogv |
English: A numerical simulation of possible surface temperatures on Proxima b performed with the Laboratoire de Météorologie Dynamique's Planetary Global Climate Model. Here it is hypothesised that the planet possesses an Earth-like atmosphere and that it is covered by an ocean (the dashed line is the frontier between the liquid and icy oceanic surface). Two models exist for the planet's rotation. Here the planet is in synchronous rotation (like the Moon around the Earth), and is seen as a distant observer would do during one full orbit. |
Date | |
Source | http://www.eso.org/public/videos/eso1629b/ |
Author | ESO/M. Kornmesser |
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[edit]This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts 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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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 02:14, 26 August 2016 | 17 s, 1,280 × 720 (5.7 MB) | Quantanew (talk | contribs) | User created page with UploadWizard |
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