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Volatile processes in Triton's atmosphere and surfaceA basic model for latitudinal transport of nitrogen is reviewed focusing on its limitations and some complications associated with surface and atmospheric physics. Data obtained by 1989 Voyager encounter with the Neptune system revealed the complexity in the pure nitrogen transport which is caused by the nonuniform albedo of the frosts. It is concluded that Triton is similar to Mars in terms of the complexity of volatile transport and to understand Triton's surface-atmosphere system, Mars may be a very good analog.
Document ID
19920062662
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lunine, J. I.
(Arizona, University Tucson, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1992
Publication Information
Publication: Advances in Space Research
Volume: 12
Issue: 11
ISSN: 0273-1177
Subject Category
Lunar And Planetary Exploration
Accession Number
92A45286
Funding Number(s)
CONTRACT_GRANT: NAGW-1039
Distribution Limits
Public
Copyright
Other

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