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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 insolation 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 approx. 0.5 to 1.5 K above that possible with absorbed sunlight alone, resulting in a factor of approx. 1.5 to 2.5 increase in Triton's basal atmospheric pressure. If Triton's internal heatflow 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 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 10 times higher in the recent past.
Document ID
19910013705
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Brown, R. H.
(Jet Propulsion Lab. California Inst. of Tech., Pasadena., United States)
Johnson, T. V.
(Jet Propulsion Lab. California Inst. of Tech., Pasadena., United States)
Goguen, J. D.
(Jet Propulsion Lab. California Inst. of Tech., Pasadena., United States)
Schubert, Gerald
(California Univ. Los Angeles., United States)
Ross, Martin N.
(Aerospace Corp. Los Angeles, CA., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1991
Subject Category
Space Radiation
Report/Patent Number
NASA-CR-188178
NAS 1.26:188178
Report Number: NASA-CR-188178
Report Number: NAS 1.26:188178
Accession Number
91N23018
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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