File:Numerical simulation of possible surface temperatures on Proxima b (3 2 resonance).ogv

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Original file ‎(Ogg Theora video file, length 17 s, 1,920 × 1,080 pixels, 6.12 Mbps, file size: 12.54 MB)

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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 a so-called 3:2 resonance (a natural frequency for the orbit), 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, 1,920 × 1,080 (12.54 MB)Quantanew (talk | contribs)User created page with UploadWizard

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VP9 1080P 2.07 Mbps Completed 10:01, 5 September 2018 42 s
Streaming 1080p (VP9) 2.07 Mbps Completed 12:31, 27 March 2024 1.0 s
VP9 720P 869 kbps Completed 10:01, 5 September 2018 25 s
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WebM 360P 512 kbps Completed 13:50, 9 February 2017 29 s
Streaming 144p (MJPEG) 859 kbps Completed 12:15, 16 November 2023 2.0 s

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