The rotation of Mars

Details The rotation of Mars The rotation of Mars

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.6231r&link_type=abstract

Journal of Geophysical Research, vol. 84, Oct. 10, 1979, p. 6231-6240.

Physics

Geophysics

11

Mars (Planet), Planetary Rotation, Planetology, Astronomical Models, Equations Of Motion, Geophysics, Nutation, Precession, Mars, Rotation, Mathematical Models, Viking Probes, Precession, Nutation, Geophysics, Equations Of Motion, Parameters, Obliquity, Coordinate Systems, Analysis

Scientific paper

A new model of the rotation of Mars is presented that is designed to support the analysis of radio metric data from the Viking landers and possible future Mars-lander missions. The precession and nutation are represented by series that include all terms causing a maximum Mars surface displacement of at least 1 cm after 10 years. The precession rate is estimated from Mars physical constants to be (7.58 in. + or - 0.03 in.)/yr based on Reasenberg's (1977) model of the mass distribution of Mars. Some geophysical effects that may cause Mars surface displacements larger than 1-cm criterion are also discussed.

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