File:Size Comparison Between PSR B1509-58 and Crab Nebula.ogv

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Size_Comparison_Between_PSR_B1509-58_and_Crab_Nebula.ogv ‎(Ogg Theora video file, length 7.0 s, 720 × 480 pixels, 847 kbps, file size: 725 KB)

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Summary[edit]

Description
English: This animation shows how radio jets may be suppressed in the micro- quasar GRS 1915. Material is being pulled from a red companion star into a black hole via a blue, rapidly rotating disk. The animation begins with a jet blowing material away from the black hole. Later, when the disk is heated by powerful radiation from close to the black hole, a wind is driven off the disk. As the wind strengthens, the jet apparently is shut down because the wind deprives the jet of material that would otherwise have fuelled it.
Date
Source CHANDRA Photo Album
Author B1509-58 (NASA/CXC/SAO/P.Slane, et al.); Crab (NASA/CXC/SAO/F.Seward et al.)
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Licensing[edit]

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current08:25, 2 May 20107.0 s, 720 × 480 (725 KB)Originalwana (talk | contribs){{Information |Description={{en|1=This animation shows how radio jets may be suppressed in the micro- quasar GRS 1915. Material is being pulled from a red companion star into a black hole via a blue, rapidly rotating disk. Th

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Transcode status

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Format Bitrate Download Status Encode time
VP9 480P 242 kbps Completed 19:29, 19 October 2018 10 s
Streaming 480p (VP9) Not ready Unknown status
VP9 360P 126 kbps Completed 19:29, 19 October 2018 6.0 s
Streaming 360p (VP9) Not ready Unknown status
VP9 240P 76 kbps Completed 19:29, 19 October 2018 4.0 s
Streaming 240p (VP9) 76 kbps Completed 03:27, 16 December 2023 0.0 s
WebM 360P 513 kbps Completed 15:56, 9 February 2017 10 s
Streaming 144p (MJPEG) 950 kbps Completed 04:15, 18 November 2023 1.0 s

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