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Internal structure of Io and the global distribution of its topographyA global topography is presently calculated for two multilayer Io models in which dissipation occurs in a viscous asthenosphere and a solid mantle: (1) a 'thermal swell' model, in which topography and heat flow are positively correlated, and (2) a 'differentiated lithosphere' model, in which topography and heat flow are negatively correlated. Both the polar topography and the hypsometric distribution of elevations in the differentiated lithosphere model are better matched with observations than the thermal swell model. The shift of the equatorial basin-swell pattern indicates a recent zonal rotation of about 25 deg for Io's lithosphere.
Document ID
19900049448
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ross, M. N.
(Aerospace Corp. Space Sciences Laboratory, Los Angeles, CA, United States)
Schubert, G.
(California, University Los Angeles, United States)
Spohn, T.
(Muenster, Universitaet Federal Republic of Germany, United States)
Gaskell, R. W.
(JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
June 1, 1990
Publication Information
Publication: Icarus
Volume: 85
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
90A36503
Distribution Limits
Public
Copyright
Other

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