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Ammonia in the atmospheres of Saturn and JupiterA profile and equivalent width for the 6451.1-A feature of the 6450-A band of ammonia at the equator and south pole of Saturn have been measured. Estimates for the NH3 abundance at the center of the disk which vary from 0.4 to 5 m-am, depending upon the atmospheric model used, lead to uncertainties in the NH3/H2 ratio which are greater than a factor of 10. Half-widths for theoretical line profiles computed from models in which the NH3 absorption occurs at a pressure level of 1.0 atm agree with the observed profiles. NH3/H2 ratios have been obtained which range from 0.00001 to 0.00002 for Jupiter.
Document ID
19800053759
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smith, W. H.
(Washington University St. Louis, Mo., United States)
Macy, W.
(Hawaii, University Honolulu, Hawaii, United States)
Cochran, W.
(McDonald Observatory; Texas, University Austin, Tex., United States)
Date Acquired
August 10, 2013
Publication Date
April 1, 1980
Publication Information
Publication: Icarus
Volume: 42
Subject Category
Lunar And Planetary Exploration
Accession Number
80A37929
Funding Number(s)
CONTRACT_GRANT: NGR-44-012-152
CONTRACT_GRANT: NGL-12-001-057
CONTRACT_GRANT: NSG-7334
Distribution Limits
Public
Copyright
Other

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