File:KSC-04-S-00343 (ksc 110104 swiftexplained).webm

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KSC-04-S-00343_(ksc_110104_swiftexplained).webm (WebM audio/video file, VP9/Opus, length 1 min 48 s, 320 × 212 pixels, 293 kbps overall, file size: 3.79 MB)

Captions

Captions

Mysterious and fleeting, gamma-ray bursts come from galaxies so far away that they take billions of years to reach us.

Summary

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Description
English: Mysterious and fleeting, gamma-ray bursts come from galaxies so far away that they take billions of years to reach us. NASA's new satellite called Swift will be able to quickly slew around and investigate these dynamic beacons of light, which scientists have speculated signal birth cries when block holes are formed_ Gamma ray bursts are a flash of gamma rays and then there's x-ray and optical emission that fades away quickly on minute-time scales. It lasts for hours and days after that, but it is brightest right after the burst. No other previous mission has been able to look at that spot in the sky quickly enough to see the really bright emission a few minutes fter the burst, and that's what's unique about Swift. Swift will also be able to relay the position of the GRB to scientists on the ground in less than one minute_ There are many theories about what causes gamma-ray bursts or GRB's: one is the Collapsar Model where the collapse of the core of a massive star forms a black hole. Another model is the Binary Merge Theory where two neutron stars, or a neutron star and a black hole merge in a violent explosion. The Swift team expects to detect and analyze 100 bursts a year. When not catching gamma-ray bursts, Swift will conduct an all-sky survey, which will be 20 times more sensitive than previous measurements. The operation center for swift is at the PSU 'Penn State University.' Managed by NASA's Goddard Space Flight Center in Greenbelt, Maryland, Swift was built in partnership with national laboratories, universities, and international partners such as Italy and the United Kingdom.
Date Taken on 4 November 2004
Source
This image or video was catalogued by Kennedy Space Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: ksc_110104_swiftexplained.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
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Author NASA Kennedy Space Center
Keywords
InfoField
afterglow; midex; early_universe; astronomy; gamma_ray_burst; observatory; multi-wavelength; blastwave; grb; ultraviolet; survey; X-ray; telescope; optical; swift

Licensing

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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
current16:41, 7 May 20241 min 48 s, 320 × 212 (3.79 MB)OptimusPrimeBot (talk | contribs)Imported media from http://images-assets.nasa.gov/video/ksc_110104_swiftexplained/ksc_110104_swiftexplained~orig.mp4

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Format Bitrate Download Status Encode time
VP9 240P 202 kbps Completed 17:42, 7 May 2024 1 min 44 s
WebM 360P 415 kbps Completed 17:42, 7 May 2024 22 s
QuickTime 144p (MJPEG) 825 kbps Completed 17:39, 8 November 2024 4.0 s

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