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File:Computer simulation of star formation in MACS1149-JD1 (eso1815c).webm

Original file ‎(WebM audio/video file, VP8, length 34 s, 1,920 × 1,080 pixels, 1.39 Mbps overall, file size: 5.6 MB)

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English: This computer graphics movie shows the probable star formation history in the galaxy MACS1149-JD1. The self-gravity of matter creates filamentary structures and the density at the intersections of the filaments increases. Around 200 million years after the Big Bang, active star formation ignites in the high density regions, which leads to the formation of galaxies. The gas in the galaxy is blown off by active stellar wind and supernovae, then the gas returns to the galaxy and causes another burst of star formation.
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Source Computer simulation of star formation in MACS1149-JD1
Author ALMA (ESO/NAOJ/NRAO)
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Date/TimeThumbnailDimensionsUserComment
current06:16, 30 May 201834 s, 1,920 × 1,080 (5.6 MB)ComputerHotline (talk | contribs)Imported media from https://cdn.eso.org/videos/hd_1080p25_broadcast/eso1815c.avi

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Format Bitrate Download Status Encode time
VP9 1080P 1.08 Mbps Completed 14:13, 22 August 2018 1 min 20 s
Streaming 1080p (VP9) 1.08 Mbps Completed 21:04, 5 February 2024 1.0 s
VP9 720P 468 kbps Completed 14:13, 22 August 2018 50 s
Streaming 720p (VP9) 468 kbps Completed 03:40, 7 February 2024 1.0 s
VP9 480P 215 kbps Completed 14:13, 22 August 2018 37 s
Streaming 480p (VP9) 214 kbps Completed 23:27, 24 January 2024 1.0 s
VP9 360P 109 kbps Completed 14:12, 22 August 2018 22 s
Streaming 360p (VP9) 109 kbps Completed 14:54, 5 February 2024 1.0 s
VP9 240P 59 kbps Completed 14:12, 22 August 2018 19 s
Streaming 240p (VP9) 58 kbps Completed 17:14, 12 December 2023 1.0 s
WebM 360P 456 kbps Completed 06:16, 30 May 2018 19 s
Streaming 144p (MJPEG) 504 kbps Completed 11:06, 2 November 2023 3.0 s

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