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The moment of inertia and isostasy of MarsThe systematic and large deviation of the gravitational equipotential surface (EPS) of Mars from a spheroid of revolution suggests a description of Mars in terms of a spheroid nearly in isostatic equilibrium with an extra mass in the Tharsis region. The displacement from Mars and the shape of the spheroid are calculated by using this description and a Mars gravity model. The EPS is represented as a contour map of its height above the spheroid. This representation provides the first clear demonstration that the Hellas depression coincides with a depression in the EPS. The disequilibrium contribution of Tharsis to the coefficient J2 of the second-degree harmonics of gravitational potential of Mars is estimated to be (126 + or - 5) times 10 to the minus 6th. The optical flattening and dynamic flattening calculated on this basis are in substantially better agreement than are those calculated in the usual way.
Document ID
19770038697
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Reasenberg, R. D.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 10, 1977
Publication Information
Publication: Journal of Geophysical Research
Volume: 82
Subject Category
Lunar And Planetary Exploration
Accession Number
77A21549
Funding Number(s)
CONTRACT_GRANT: NGR-22-009-804
CONTRACT_GRANT: NAS1-9702
Distribution Limits
Public
Copyright
Other

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