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Internal structure and shape of MimasThe observed triaxial ellipsoid shape of Mimas, in conjunction with a mean density of 1137 kg/cu cm, is presently used as the basis of hydrostatic equilibrium and nonhydrostatic models of internal structure whose outer layers are sufficiently strong to support part of the tidal load. Such plausible internal structures are consistent with the shape and density constraints as (1) a two-layer model in hydrostatic equilibrium, (2) a hydrostatic model with four layers of equal depth, and (3) a nonhydrostatic constant-density model with an elastic lithosphere; these models admit either homogeneous or heterogeneous accretion, as well as either a cold thermal history or melting and differentiation.
Document ID
19880067580
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ross, M. N.
(California Univ. Los Angeles, CA, United States)
Schubert, G.
(California, University Los Angeles, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1988
Publication Information
Publication: Icarus
Volume: 75
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0019-1035
Accession Number
88A54807
Funding Number(s)
CONTRACT_GRANT: NSG-7315
Distribution Limits
Public
Copyright
Other

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