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The 7.5- to 13.5-micron spectrum of SaturnA medium-resolution spectrum of Saturn in the 7.5-13.5 micron range is presented. The observed low brightness temperature between 9 and 11 microns of about 100-105 K rules out gaseous NH3 as the dominant absorber in this spectral range. Absorption features due to PH3 may be present around 10 microns and cloud particles could be an important source of opacity in this wavelength range. There are strong indications of a temperature inversion in the upper atmosphere, including high brightness temperature in the 7.7-micron CH4 band, and possible emission from C2H6 around 12 microns.
Document ID
19740049179
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Gillett, F. C.
(Kitt Peak National Observatory Tucson, Ariz., United States)
Forrest, W. J.
(California, University San Diego, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 187
Subject Category
Space Sciences
Accession Number
74A31929
Funding Number(s)
CONTRACT_GRANT: NGL-05-005-003
Distribution Limits
Public
Copyright
Other

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