File:Numerical simulation of possible surface temperatures on Proxima b (synchronous rotation).ogv

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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.
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Source http://www.eso.org/public/videos/eso1629b/
Author ESO/M. Kornmesser

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Date/TimeThumbnailDimensionsUserComment
current02:14, 26 August 201617 s, 1,280 × 720 (5.7 MB)Quantanew (talk | contribs)User created page with UploadWizard

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Format Bitrate Download Status Encode time
VP9 720P 829 kbps Completed 10:01, 5 September 2018 24 s
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VP9 480P 351 kbps Completed 10:01, 5 September 2018 16 s
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VP9 360P 186 kbps Completed 10:01, 5 September 2018 11 s
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VP9 240P 109 kbps Completed 10:01, 5 September 2018 9.0 s
Streaming 240p (VP9) 109 kbps Completed 07:21, 6 February 2024 1.0 s
WebM 360P 512 kbps Completed 13:54, 9 February 2017 22 s
Streaming 144p (MJPEG) 823 kbps Completed 12:16, 16 November 2023 1.0 s

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