Far Infrared Absolute Spectrophotometer

E1036260

The Far Infrared Absolute Spectrophotometer (FIRAS) was a key instrument on NASA’s COBE satellite designed to precisely measure the spectrum of the cosmic microwave background, confirming its near-perfect blackbody nature.

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Statements (49)

Predicate Object
instanceOf cosmic microwave background instrument
far‑infrared spectrometer
space telescope instrument
spectrophotometer
abbreviation FIRAS NERFINISHED
associatedAward 2006 Nobel Prize in Physics NERFINISHED
blackbodyFitQuality deviations less than parts in 10^5
confirmed near‑perfect blackbody spectrum of the cosmic microwave background
constrained Compton y‑distortion of the CMB
chemical potential (mu) distortions of the CMB
spectral distortions of the cosmic microwave background
contributedTo establishing the Big Bang model of cosmology
precision determination of the CMB spectrum
cosmologicalParameterMeasured CMB monopole temperature
countryOfOrigin United States of America
surface form: United States
dataRelease COBE FIRAS data products
dataUsage constraints on reionization and structure formation models
tests of early‑universe energy release
fieldOfView about 7 degrees
found no significant deviation from a perfect blackbody spectrum
frequencyRange approximately 30 GHz to 3000 GHz
fullName Far Infrared Absolute Spectrophotometer NERFINISHED
hostedBy NASA Goddard Space Flight Center (project management) NERFINISHED
launchDate 1989-11-18
launchSite Vandenberg Air Force Base NERFINISHED
launchVehicle Delta 5920-8 NERFINISHED
locatedOn COBE payload module NERFINISHED
measuredCMBTemperature approximately 2.725 K
measurementType absolute spectrophotometry
differential radiometry
mission COBE mission NERFINISHED
operator NASA
primaryObjective measure the spectrum of the cosmic microwave background radiation
test the blackbody nature of the cosmic microwave background
referenceSource external calibrator at controlled temperature
on‑board blackbody calibrators
scanStrategy full‑sky coverage over mission lifetime
scienceDiscipline astrophysics
cosmology
spacecraft COBE NERFINISHED
Cosmic Background Explorer NERFINISHED
spectralResolution about 0.5 cm^-1
status decommissioned
teamLead John C. Mather NERFINISHED
temperatureMeasurementAccuracy about 0.1 mK relative to a 2.7 K blackbody
usedTechnique Fourier transform spectroscopy
polarizing Michelson interferometer
verifiedPredictionOf standard hot Big Bang theory
wavelengthRange approximately 0.1 cm to 1 cm

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Cosmic Background Explorer instrument Far Infrared Absolute Spectrophotometer