Dynamical evolution of the rotation of venus

Details Dynamical evolution of the rotation of venus Dynamical evolution of the rotation of venus

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988em%26p...43..275s&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 43, Dec. 1988, p. 275-287.

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Computation

5

Computational Astrophysics, Planetary Evolution, Planetary Rotation, Spin Dynamics, Venus (Planet), Atmospheric Tides, Hamiltonian Functions, Planetary Cores, Planetary Mantles, Runge-Kutta Method, Venus Atmosphere

Scientific paper

The evolution of the spin angular velocity and the obliquity of Venus are calculated using the step-variable Runge-Kutta method of 7th order. Also, seven sets of the probable Cytherean spin evolution are obtained. The results suggest that Venus could have been captured in a spin-orbit resonant state by the gravitational torque of the earth on the permanent deformation of Venus.

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