Cosmic Origins Spectrograph

E46137

The Cosmic Origins Spectrograph is a highly sensitive ultraviolet spectrograph on the Hubble Space Telescope designed to study the origins and evolution of galaxies, stars, and the intergalactic medium.


Statements (47)
Predicate Object
instanceOf Hubble Space Telescope instrument
space telescope instrument
spectrograph
ultraviolet spectrograph
abbreviation COS
countryOfOrigin United States
dataProduct ultraviolet spectra
designedFor faint astronomical sources
high-sensitivity ultraviolet spectroscopy
developedBy Ball Aerospace
Center for Astrophysics and Space Astronomy
University of Colorado Boulder
developedForAgency NASA Goddard Space Flight Center
hasSpectralChannel FUV channel
NUV channel
improvesUpon Space Telescope Imaging Spectrograph sensitivity in FUV
installedBy Space Shuttle mission STS-125
installedDuringMission Hubble Servicing Mission 4
launchVehicle Space Shuttle Atlantis
missionRole study intergalactic medium
study origins and evolution of galaxies
study star formation and evolution
observes active galactic nuclei
hot stars
intergalactic gas
interstellar gas
quasars
operator NASA
partOf Hubble Space Telescope
platform low Earth orbit via Hubble Space Telescope
primaryScienceBand 115–205 nm (FUV)
replacedInstrument Corrective Optics Space Telescope Axial Replacement
scienceTheme chemical enrichment of the universe
cosmic origins
cosmic web
galaxy formation and evolution
scientificObjective measure absorption lines in spectra of distant objects
probe large-scale structure of the universe
study baryonic content of the universe
study circumgalactic medium
study interstellar medium
secondaryScienceBand 170–320 nm (NUV)
spectralResolution low resolution
medium resolution
telescopeFocus HST Science Instrument Bay
wavelengthRange far-ultraviolet
near-ultraviolet

Referenced by (2)
Subject (surface form when different) Predicate
Hubble Space Telescope
hasInstrument
STS-125
installedInstrument

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