The moment of inertia of Mars

Details The moment of inertia of Mars The moment of inertia of Mars

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979georl...6..194k&link_type=abstract

Geophysical Research Letters, vol. 6, Mar. 1979, p. 194-196.

Physics

16

Mars (Planet), Moments Of Inertia, Planetary Rotation, Planetology, Gravitational Effects, Mass Distribution, Oblate Spheroids, Topography, Moments Of Inertia, Hypotheses, Mars, Domes, Tharsis, Montes, Mathematical Models, Asymmetry, Gravitational Potential, Topography, Mass

Scientific paper

The nonhydrostatic contribution to the oblateness is calculated based on the single assumption that nonhydrostatic contributions to the moments-of-inertia are axially symmetric about the principal axis in the direction of the Tharsis dome. The correction to J2 is thereby -2(J22), in numerical value equal to that obtained by Reasenberg by a more complicated technique. The resulting C/(M x (square of R)) is 0.365. The error in these values depends entirely on the extent to which mass irregularities depart from axial symmetry around Tharsis, which plausibly would not be great.

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