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SIRTF - Capabilities for planetary scienceMajor research areas of the Space Infrared Telescope Facility (SIRTF) are discussed which include Kuiper-belt comets, IR spectroscopy of comets, and circumstellar planetary debris disks. SIRTF instrumentation will include the infrared array camera (IRAC) and multiband imaging photometer (MIP). The IRAC uses large area, 2D infrared array detectors to provide wide-field (7 arcmin) and diffraction-limited imaging over the spectral region from 2 to 30 microns. The MIP will provide background-limited imaging and photometry over the wavelength range from 30 to 200 microns, wide-field, high resolution imaging from 50 to 120 microns, and broad band photometry and mapping from 200 to 700 microns.
Document ID
19920062672
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Cruikshank, D. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Werner, M. W.
(NASA Ames Research Center Moffett Field; JPL, Pasadena, CA, United States)
Backman, D. E.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1992
Publication Information
Publication: Advances in Space Research
Volume: 12
Issue: 11, N
ISSN: 0273-1177
Subject Category
Astronomy
Accession Number
92A45296
Distribution Limits
Public
Copyright
Other

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