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Past obliquity oscillations of Mars - The role of the Tharsis upliftThe paper deals with possible ancient variations of the obliquity of Mars. Consideration of data on internal differentiation, Tharsis uplift and crustal phenomena, mantle convection, and eigenfrequencies and mean motion suggest that (1) differentiation with core formation decreased the primeval spin precession constant (alpha) by 4-5%, driving it through resonance with the j = 2 orbital term; (2) a combination of geophysical processes caused alpha to drift back and forth through resonance with the j = 2 orbital term during part of Mars' history; (3) this situation was turned off by the Tharsis uplift, which drove alpha away from j = 2 resonance and possibly through the j = 26 resonance. The consequences of such events for the planet's obliquity are analyzed. Various types of motions are calculated, demonstrating the sensitivity of the obliquity to passage through resonance with such minor orbital terms.
Document ID
19790039085
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ward, W. R.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Burns, J. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Toon, O. B.
(Cornell University Ithaca, N.Y., United States)
Date Acquired
August 9, 2013
Publication Date
January 10, 1979
Publication Information
Publication: Journal of Geophysical Research
Volume: 84
Subject Category
Lunar And Planetary Exploration
Accession Number
79A23098
Funding Number(s)
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NGR-22-007-269
Distribution Limits
Public
Copyright
Other

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