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Triton's global heat budgetInternal heat flow from radioactive decay in Triton's interior along with absorbed thermal energy from Neptune total 5 to 20 percent of the isolation absorbed by Triton, thus comprising a significant fraction of Triton's surface energy balance. These additional energy inputs can raise Triton's surface temperature between about 0.5 and 1.5 K above that possible with absorbed sunlight alone, resulting in an increase of about a factor of about 1.5 to 2.5 in Triton's basal atmospheric pressure. If Triton's internal heat flow is concentrated in some areas, as is likely, local effects such as enhanced sublimation with subsequent modification of albedo could be quite large. Furthermore, indications of recent global albedo change on Triton suggest that Triton's surface temperature and pressure may not now be in steady state, further suggesting that atmospheric pressure on Triton was as much as ten times higher in the recent past.
Document ID
19910046525
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Brown, R. H.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Johnson, T. V.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Goguen, J. D.
(JPL Pasadena, CA, United States)
Schubert, G.
(California, University Los Angeles, United States)
Ross, M. N.
(Aerospace Corp. Space Sciences Laboratory, Los Angeles, CA, United States)
Date Acquired
August 14, 2013
Publication Date
March 22, 1991
Publication Information
Publication: Science
Volume: 251
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
91A31148
Distribution Limits
Public
Copyright
Other

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