File:MUSE — Running through the 3D data of NGC 4650A.ogv

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Original file(Ogg multiplexed audio/video file, Theora/Vorbis, length 2 min 33 s, 1,280 × 720 pixels, 788 kbps overall, file size: 14.39 MB)

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English: This view shows how the new MUSE instrument on ESO’s Very Large Telescope gives a three-dimensional view of a distant galaxy. For each part of the galaxy the light has been split up into its component colours — revealing not only the motions of different parts of the galaxy but also clues to its chemical composition and other properties. At certain wavelengths the emission from the rotating disc around the galaxy is clearly seens, as well as the different velocities of different parts of the disc.

During the subsequent analysis the astronomer can move through the data and study different views of the object at different wavelengths, just like tuning a television to different channels at different frequencies. In this sequence the slices at different wavelengths are presented in sequence and the speed is adjusted to highlight the glow from star formation regions in the disc.

This picture is based on data on the polar ring galaxy NGC 4650A that were obtained soon after the instrument achieved first light in early 2014.
Date
Source ESO
Author ESO/MUSE consortium/R. Bacon

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Date/TimeThumbnailDimensionsUserComment
current21:18, 5 March 20142 min 33 s, 1,280 × 720 (14.39 MB)Originalwana (talk | contribs)User created page with UploadWizard

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VP9 720P 294 kbps Completed 11:35, 2 September 2018 2 min 23 s
Streaming 720p (VP9) Not ready Unknown status
VP9 480P 133 kbps Completed 11:35, 2 September 2018 1 min 55 s
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VP9 360P 68 kbps Completed 11:34, 2 September 2018 1 min 11 s
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WebM 360P 503 kbps Completed 02:57, 1 February 2017 2 min 12 s
Streaming 144p (MJPEG) 491 kbps Completed 10:30, 10 November 2023 5.0 s
Stereo (Opus) 1 kbps Completed 02:01, 10 November 2023 1.0 s
Stereo (MP3) 128 kbps Completed 02:00, 10 November 2023 3.0 s

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