Astronomy and Astrophysics – Astronomy
Scientific paper
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.
Marchenkov Konstantin I.
Zharkov Vladimir Naumovich
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