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Neil Gehrels Swift Observatory

NASA's Neil Gehrels Swift Observatory is a rapidly repointing, multiwavelength telescope built to detect gamma-ray bursts and study their afterglows. Its Burst Alert Telescope, X-Ray Telescope, and Ultraviolet/Optical Telescope work together to locate transient events and begin follow-up observations within minutes.

Neil Gehrels Swift Observatory
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Identity

Aliases
SwiftSwift Gamma-Ray Burst ExplorerSwift Gamma-ray Observatory
Name
Neil Gehrels Swift Observatory
Status
active

Details

Astronauts
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Description
NASA's Neil Gehrels Swift Observatory is a rapidly repointing, multiwavelength telescope built to detect gamma-ray bursts and study their afterglows. Its Burst Alert Telescope, X-Ray Telescope, and Ultraviolet/Optical Telescope work together to locate transient events and begin follow-up observations within minutes.
Destination
Low Earth orbit for rapid multiwavelength detection and follow-up of gamma-ray bursts and other transient cosmic events using gamma-ray, X-ray, ultraviolet, and optical telescopes
Launch Site
Outcome
Swift remains an active time-domain observatory after more than two decades. It has localized and characterized gamma-ray bursts, supported rapid international follow-up, and expanded its observing program to supernovae, tidal-disruption events, novae, active galaxies, and other transient sources.
Programs
Start Date
2004-11-20
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Creation Time
July 18, 2026 at 14:52:46 UTC
Updated Time
August 22, 2026 at 13:43:37 UTC

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Neil Gehrels Swift Observatory Swift Swift Gamma-Ray Burst Explorer Swift Gamma-ray Observatory
Space Stations
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