A model of Venusian global topography has been obtained by fitting an eighteenth‐degree harmonic series to Pioneer Venus orbiter radar altimeter data. The mean radius is (6051.45±0.04) km. The corresponding mean density is (5244.8±0.5) kg m −3 . The center of figure is displaced from the center of mass by (0.339±0.088) km towards (6.6±10.1)°N, (148.8±7.7)°E. The figure of Venus is distinctly triaxial, but the orientation and magnitudes of the principal topographic axes correlate rather poorly with the gravitational principal axes. However, the higher‐degree harmonics of topography and gravity are significantly correlated. The topographic variance spectrum of Venus is very similar in form to those of the moon, Mars, and especially Earth. We suggest that this spectral similarity simply reflects a statistical balance between constructional and degradational geomorphic processes. Venus and Earth are particularly similar (and differ from the moon and Mars) in that the larger bodies both exhibit a significant low degree‐deficit (relative to the extrapolated trend of the higher harmonics).
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Bills et al. (1985) studied this question.
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