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

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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. Another model is that it is trapped in a so-called synchronous rotation.

Two additional papers about Proxima b's possibility for habitability are described at proximacentauri.info.
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Source Numerical simulation of possible surface temperatures on Proxima b (3:2 resonance)
Author ESO
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Date/TimeThumbnailDimensionsUserComment
current06:03, 17 May 201817 s, 1,920 × 1,080 (3.92 MB)ComputerHotline (talk | contribs)Imported media from https://cdn.eso.org/videos/hd_1080p25_broadcast/eso1629h.avi

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Format Bitrate Download Status Encode time
VP9 1080P 1.94 Mbps Completed 10:01, 5 September 2018 43 s
Streaming 1080p (VP9) 1.94 Mbps Completed 12:31, 27 March 2024 1.0 s
VP9 720P 883 kbps Completed 10:01, 5 September 2018 26 s
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VP9 480P 485 kbps Completed 10:01, 5 September 2018 23 s
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VP9 240P 159 kbps Completed 10:00, 5 September 2018 13 s
Streaming 240p (VP9) 159 kbps Completed 07:21, 6 February 2024 1.0 s
WebM 360P 417 kbps Completed 06:03, 17 May 2018 10 s
Streaming 144p (MJPEG) 858 kbps Completed 12:15, 16 November 2023 2.0 s

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