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Oblateness, radius, and mean stratospheric temperature of Neptune from the 1985 August 20 occultationThe oblateness and equatorial radius of Neptune at the 1-microbar pressure level, together with the position angle of the projected spin axis, are the goals of a general oblate atmosphere model for Neptune employing a data ensemble obtained from the occultation of a bright IR star that provided accurate measurements of the limb position at these and several other stations. The observed reduction in central flash intensity is explained by a 150-135 K temperature decrease as pressure rises from 1 to 400 microbar. Attention is given to the implications of these oblateness results for models of the Neptune interior.
Document ID
19880035887
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hubbard, W. B.
(Arizona, University Tucson, United States)
Nicholson, Philip D.
(Cornell University Ithaca, NY, United States)
Lellouch, Emmanuel
(Arizona Univ. Tucson, AZ, United States)
Sicardy, Bruno
(Arizona Univ. Tucson, AZ, United States)
Brahic, Andre
(Paris Observatoire, Meudon, France)
Vilas, Faith
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 13, 2013
Publication Date
December 1, 1987
Publication Information
Publication: Icarus
Volume: 72
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
88A23114
Funding Number(s)
CONTRACT_GRANT: NSG-7045
CONTRACT_GRANT: NSF AST-78-27879
CONTRACT_GRANT: NGL-05-002-140
Distribution Limits
Public
Copyright
Other

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