The relief of the crust-mantle boundary and strain-compression stresses in the crust of Venus

Details The relief of the crust-mantle boundary and strain-compression stresses in the crust of Venus The relief of the crust-mantle boundary and strain-compression stresses in the crust of Venus

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..182m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Feb. 1989, p. 182-190. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Compression Loads, Planetary Crusts, Planetary Mantles, Planetary Structure, Venus (Planet), Gravitational Fields, Green'S Functions, Planetary Geology, Spherical Harmonics, Strain Rate, Topography

Scientific paper

A joint analysis of the topography and nonequilibrium part of the gravitational field of the Venus was carried out for spherical harmonics with n = 3-18. The characteristics of the crust-mantle boundary and of the strain-compression stresses in the crust were revealed for a series of realistic models of Venus with allowance for the asthenosphere. In general, the crust-mantle boundary of Venus is sufficiently smooth. The stresses vary from + 600 bars (strain) to - 700 bars (compression) as a function of the model of the planet's interior.

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