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.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Cosmic Origins Spectrograph canonical | 9 |
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
Hubble Space Telescope instrument
ⓘ
space telescope instrument ⓘ spectrograph ⓘ ultraviolet spectrograph ⓘ |
| abbreviation | COS ⓘ |
| countryOfOrigin |
United States of America
ⓘ
surface form:
United States
|
| dataProduct | ultraviolet spectra ⓘ |
| designedFor |
faint astronomical sources
ⓘ
high-sensitivity ultraviolet spectroscopy ⓘ |
| developedBy |
Ball Aerospace
ⓘ
Laboratory for Atmospheric and Space Physics ⓘ
surface form:
Center for Astrophysics and Space Astronomy
University of Colorado Boulder ⓘ |
| developedForAgency |
Goddard Space Flight Center
ⓘ
surface form:
NASA Goddard Space Flight Center
|
| hasSpectralChannel |
FUV channel
ⓘ
NUV channel ⓘ |
| improvesUpon | Space Telescope Imaging Spectrograph sensitivity in FUV ⓘ |
| installedBy |
STS-125
ⓘ
surface form:
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 (COSTAR)
ⓘ
surface form:
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 |
Hubble Space Telescope
ⓘ
surface form:
HST Science Instrument Bay
|
| wavelengthRange |
far-ultraviolet
ⓘ
near-ultraviolet ⓘ |
Referenced by (9)
Full triples — surface form annotated when it differs from this entity's canonical label.
Hubble Space Telescope science instruments
→
fourthGenerationInstruments
→
Cosmic Origins Spectrograph
ⓘ