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The first orbiting astronomical infrared telescope system Its development and performanceThe Infrared Astronomical Satellite (IRAS) was launched on January 25, 1983, and has provided astronomers with their first extended views of the universe in the 8 to 120 micron wavelength region. The infrared telescope system is one of several United States contributions to this international project sponsored by the U.S.A., The Netherlands, and the U.K. This telescope employs four bands of detectors cooled to 2.4 K to achieve a noise equivalent flux density in the 10 to the -18th to 10 to the -19th watts/sq cm range and will operate for approximately eleven months before depletion of its supply of superfluid helium. This paper describes major problems, early flight results, and technical lessons learned during the course of the telescope's development and flight operations.
Document ID
19850043245
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Conrad, A. G.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Irace, W. R.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Subject Category
Spacecraft Instrumentation
Meeting Information
Meeting: Instrumentation in astronomy V
Location: London
Start Date: September 7, 1983
End Date: September 9, 1983
Sponsors: SPIE and ISOE
Accession Number
85A25396
Distribution Limits
Public
Copyright
Other

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