File:GRB 080916C Fermi observation translated to music.webm

From Wikimedia Commons, the free media repository
Jump to navigation Jump to search

Original file(WebM audio/video file, VP9/Opus, length 3 min 47 s, 556 × 720 pixels, 255 kbps overall, file size: 6.9 MB)

Captions

Captions

Add a one-line explanation of what this file represents

Summary[edit]

Description
English: A gamma-ray burst, the most energetic explosions in the universe, converted to music. Made by Sylvia Zhu (music) and Judy Racusin (animation)

Every photon has its own energy and frequency; the higher the energy, the higher the frequency. Some photons have just the right frequencies for us to see them as different colors, while others — such as the gamma rays studied by the Fermi LAT — are much too energetic to be seen with our eyes. Sound waves have frequencies too, and similarly, we can hear some of them as musical notes. So what happens if we convert high-energy photons into musical notes?

Gamma-ray bursts (GRBs) are some of the most powerful explosions in the universe. GRB 080916C was a particularly energetic burst that occurred in September 2008. The brightest part of it lasted less than a minute, during which the LAT detected hundreds of gamma rays from the extremely-distant explosion; when we converted the data to music, we slowed the rates down by a factor of five times to hear the individual gamma rays better.

In translating the gamma-ray measurements into musical notes we assigned the photons to be “played” by different instruments (harp, cello, or piano) based on the probabilities that they came from the burst. This particular conversion is a fairly simple one; We built this on work done by other members of the LAT team (Luca Baldini and Alex Drlica-Wagner) who explored converting our data into music in different ways.

In the beginning of the song, before the burst starts, the harp plucks out a few lonely notes. After about half a minute, the piano joins in on top of the harp background, and the notes begin to pile on more and more rapidly. The cello enters the scene as the burst begins in earnest.

We created an accompanying animation to help see what is happening. The top panel shows each individual gamma-ray. The colors refer to low (red), medium (blue) and high (green) quality gamma-rays (played by harp, cello and piano respectively). The energy of the gamma-ray is on the y-axis (higher energy gamma-rays are towards the top of the plot) and the arrival time of the gamma-rays are on the x-axis (later arriving gamma-rays are further to the right). The vertical white line tells you where the music is currently playing. The bottom panel shows the number of gamma-rays (which is the number of notes played) in each time slice.

By converting gamma rays into musical notes, we have a new way of representing the data and listening to the universe.
Date (released)
Source https://blogs.nasa.gov/GLAST/2012/06/21/post_1340301006610/; https://www.youtube.com/watch?v=2wvPe9OA1qA
Author NASA/Fermi Science Team/Sylvia Zhu (music) and Judy Racusin (animation)

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.)
Warnings:

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current06:25, 22 June 20193 min 47 s, 556 × 720 (6.9 MB)Huntster (talk | contribs)Imported media from uploads:c2dad7ca-94b3-11e9-b6cb-0242c0a8950f

Transcode status

Update transcode status
Format Bitrate Download Status Encode time
VP9 720P 215 kbps Completed 06:26, 22 June 2019 1 min 20 s
Streaming 720p (VP9) 99 kbps Completed 14:30, 27 March 2024 1.0 s
VP9 480P 170 kbps Completed 06:26, 22 June 2019 1 min 26 s
Streaming 480p (VP9) 54 kbps Completed 06:25, 12 March 2024 1.0 s
VP9 360P 149 kbps Completed 06:26, 22 June 2019 1 min 7 s
Streaming 360p (VP9) Not ready Unknown status
VP9 240P 136 kbps Completed 06:26, 22 June 2019 46 s
Streaming 240p (VP9) 20 kbps Completed 23:29, 21 December 2023 0.0 s
WebM 360P 129 kbps Completed 06:26, 22 June 2019 43 s
Streaming 144p (MJPEG) 1 Mbps Completed 16:12, 13 November 2023 9.0 s
Stereo (Opus) 115 kbps Completed 08:14, 23 November 2023 7.0 s
Stereo (MP3) 128 kbps Completed 06:32, 3 November 2023 7.0 s

Metadata