Models of the Internal Structure of the Earth-like Venus

A working model of the Venusian interior (radial distribution of the density, pressure, gravitational acceleration, and velocities of compressional and shear seismic waves) has been constructed based on observational data and general experience of geophysics. Corrections for the influence of the pla...

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Bibliographic Details
Published in:Solar system research 2020, Vol.54 (1), p.20-27
Main Authors: Gudkova, T. V., Zharkov, V. N.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics and Astroparticles
Astrophysics and Cosmology
Observations and Techniques
Physics
Physics and Astronomy
Planetology
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Summary:A working model of the Venusian interior (radial distribution of the density, pressure, gravitational acceleration, and velocities of compressional and shear seismic waves) has been constructed based on observational data and general experience of geophysics. Corrections for the influence of the planetary interior anelasticity on the value of the model Love number k 2 were calculated. The equilibrium figure parameters of Venus were determined.
ISSN:0038-0946
1608-3423
DOI:10.1134/S0038094620010049