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Physical state of volatiles on the surface of tritonSeveral possible configurations for volatiles on Triton are assessed. It is concluded that the simplest volatile configuration which best satisfies the constraints with the least number of ad hoc assumptions is N2 and CH4 both in solid forms, perhaps partly as a microscopic mixture, but more probably as a disequilibrium assemblage, nonuniformly distributed. Thermodynamic equilibrium is then limited by seasonal transport and the finite diffusion time of CH4 in crystalline N2. Although a nitrogen ocean cannot be excluded, it requires very restrictive assumptions.
Document ID
19860027101
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lunine, J. I.
(Arizona, University Tucson, United States)
Stevenson, D. J.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
September 19, 1985
Publication Information
Publication: Nature
Volume: 317
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Accession Number
86A11839
Funding Number(s)
CONTRACT_GRANT: NAGW-185
CONTRACT_GRANT: NSF AST-82-06173
CONTRACT_GRANT: NAGW-450
Distribution Limits
Public
Copyright
Other

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