Swift satellite

E1027636

The Swift satellite is a NASA space observatory launched in 2004 to detect and rapidly observe gamma-ray bursts and other high-energy astrophysical phenomena across multiple wavelengths.

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Swift satellite canonical 1

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Predicate Object
instanceOf artificial satellite
space observatory
space telescope
abbreviation BAT
UVOT
XRT
alternativeName Swift satellite
capability automatic distribution of burst coordinates to ground observers
onboard burst localization
rapid autonomous slewing to new targets
collaboration Italy
United Kingdom
United States
countryOfOrigin United States
fieldOfView large field of view for BAT
formerName Swift Gamma-Ray Burst Explorer
fullName Neil Gehrels Swift Observatory
fundingAgency NASA
hasInstrument Burst Alert Telescope
Ultraviolet/Optical Telescope
X-Ray Telescope
launchCountry United States
launchDate 2004-11-20
launchSite Cape Canaveral Air Force Station Space Launch Complex 17A
launchVehicle Delta II 7320-10C
linked to: Delta II
manufacturer Spectrum Astro
mass approximately 1500 kilograms
missionType gamma-ray burst observatory
multi-wavelength astronomy observatory
namedAfter Neil Gehrels
observes X-ray sources
gamma-ray bursts
optical sources
ultraviolet sources
operator NASA
orbitInclination about 20.6 degrees
orbitPeriod about 96 minutes
orbitType low Earth orbit
primaryObjective detection of gamma-ray bursts
rapid follow-up observations of gamma-ray bursts
scienceFocus cosmology using gamma-ray bursts
high-energy astrophysics
transient astrophysical phenomena
spaceAgency NASA Goddard Space Flight Center
status operational (as of mid-2020s)
wavelengthCoverage X-ray
gamma-ray
optical
ultraviolet

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Ultraviolet/Optical Telescope platform Swift satellite