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Thermal state of an ice shell on EuropaThe thickness of the ice shell presently hypothesized for Europa, which is decoupled from a silicate core by a liquid water layer, is calculated as a function of colatitude and longitude under suitable assumptions for two plausible ice rheology behaviors: that of Maxwell type, and that of generalized flow-law rheology. Due to the dissipation rate's pronounced temperature dependence, virtually all tidal dissipation is found to concentrate in the lowest few kilometers of the shell. While for some parameter choices an insulating regolith that raises the near-surface temperature by more than a few tens of degrees C may stabilize the shell against polar wander, a modest regolith may enhance the probability of such wander's occurrence through the reduction of the shell's retarding friction.
Document ID
19900024509
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ojakangas, Gregory W.
(California Inst. of Tech. Pasadena, CA, United States)
Stevenson, David J.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
October 1, 1989
Publication Information
Publication: Icarus
Volume: 81
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
90A11564
Funding Number(s)
CONTRACT_GRANT: NAGW-185
CONTRACT_GRANT: NAGW-944
Distribution Limits
Public
Copyright
Other

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