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Mars secular obliquity change due to the seasonal polar capsThere is a weak positive feedback mechanism between the astronomy and meteorology of Mars. The mechanism is this: the seasonal waxing and waning polar caps cause small changes in Mars' dynamical flattening. Because the changes in flattening are out of phase with the sun, there is a net annual solar torque on the planet which increases the angle between the equatorial and orbital phanes. On the basis of Viking observations of the present climate and simple atmospheric models of past climates, these seasonal shifts of mass between the atmosphere and polar caps are capable of secularly increasing Mars' obliquity by about 1 or 2 deg since the origin of the solar system. Thus, the climate, driven largely by the axial tilt, reacts back on the planet and slightly enhances the seasons on Mars as time progresses. More sophisticated models will probably not change this result much; therefore this mechanism probably produced only minor changes in Mars' climate. It causes negligible changes in the axial tilt and climate of the earth.
Document ID
19920044142
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Rubincam, David P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 15, 2013
Publication Date
February 25, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: E2, F
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
92A26766
Distribution Limits
Public
Copyright
Other

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