File:Warped Space and Time Around Colliding Black Holes.webm

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Original file(WebM audio/video file, VP8/Vorbis, length 1 min 14 s, 1,920 × 1,080 pixels, 2.13 Mbps overall, file size: 18.75 MB)

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Description
English: This computer simulation shows the warping of space and time around two colliding black holes observed by LIGO on September 14, 2015. LIGO detected gravitational waves generated by this black hole merger—humanity's first contact with gravitational waves and black-hole collisions. Gravitational waves are ripples in the shape of space and flow of time.

The colored surface is the space of our universe, as viewed from a hypothetical, flat, higher-dimensional universe, in which our own universe is embedded. Our universe looks like a warped two-dimensional sheet because one of its three space dimensions has been removed. Around each black hole, space bends downward in a funnel shape, a warping produced by the black hole's huge mass.

Near the black holes, the colors depict the rate at which time flows. In the green regions outside the holes, time flows at its normal rate. In the yellow regions, it is slowed by 20 or 30 percent. In the red regions, time is hugely slowed. Far from the holes, the blue and purple bands depict outgoing gravitational waves, produced by the black holes' orbital movement and collision.

Our universe's space, as seen from the hypothetical higher-dimensional universe, is dragged into motion by the orbital movement of the black holes, and by their gravity and by their spins. This motion of space is depicted by silver arrows, and it causes the plane of the orbit to precess gradually, as seen in the video.

The upper left numbers show time, as measured by a hypothetical person near the black holes (but not so near that time is warped). The bottom portion of the movie shows the waveform, or wave shape, of the emitted gravitational waves.

The gravitational waves carry away energy, causing the black holes to spiral inward and collide. The movie switches to slow motion as the collision nears, and is paused at the moment the black holes' surfaces (their "horizons") touch. At the pause, space is enormously distorted. After the pause, again seen in slow motion, the shapes of space and time oscillate briefly but wildly, and then settle down into the quiescent state of a merged black hole. Returning to fast motion, we see the gravitational waves from the collision, propagating out into the universe.

The collision and wild oscillations constitute a "storm" in the fabric of space and time—an enormously powerful but brief storm. During the storm, the power output in gravitational waves is far greater than the luminosity of all the stars in our observable universe put together. In other words, this collision of two black holes, each the size of a large city on Earth, is the most powerful explosion that astronomers have ever seen, aside from our universe's birth in the Big Bang.

This simulation was created by the SXS (Simulating eXtreme Spacetimes) Project (http://www.black-holes.org).

Credit: SXS
Date
Source YouTube: Warped Space and Time Around Colliding Black Holes – View/save archived versions on archive.org and archive.today
Author LIGO Lab Caltech : MIT

Licensing

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This video, screenshot or audio excerpt was originally uploaded on YouTube under a CC license.
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attribution
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
Attribution: LIGO Lab Caltech : MIT
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
This file, which was originally posted to YouTube: Warped Space and Time Around Colliding Black Holes – View/save archived versions on archive.org and archive.today, was reviewed on 25 August 2016 by reviewer INeverCry, who confirmed that it was available there under the stated license on that date.

File history

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Date/TimeThumbnailDimensionsUserComment
current20:21, 25 August 20161 min 14 s, 1,920 × 1,080 (18.75 MB)بدارين (talk | contribs)Imported media from https://www.youtube.com/watch?v=1agm33iEAuo

Transcode status

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Format Bitrate Download Status Encode time
VP9 1080P 1.9 Mbps Completed 11:47, 26 October 2018 3 min 38 s
Streaming 1080p (VP9) Not ready Unknown status
VP9 720P 963 kbps Completed 11:46, 26 October 2018 2 min 11 s
Streaming 720p (VP9) Not ready Unknown status
VP9 480P 533 kbps Completed 11:45, 26 October 2018 1 min 38 s
Streaming 480p (VP9) Not ready Unknown status
VP9 360P 322 kbps Completed 11:45, 26 October 2018 1 min 10 s
Streaming 360p (VP9) Not ready Unknown status
VP9 240P 189 kbps Completed 11:44, 26 October 2018 1 min 2 s
Streaming 240p (VP9) 185 kbps Completed 04:45, 5 December 2023 1.0 s
WebM 360P 508 kbps Completed 20:23, 25 August 2016 1 min 19 s
Streaming 144p (MJPEG) 817 kbps Completed 14:55, 18 November 2023 4.0 s
Stereo (Opus) 1 kbps Completed 02:59, 13 November 2023 1.0 s
Stereo (MP3) 128 kbps Completed 01:58, 13 November 2023 2.0 s

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