The evolution of the translational-rotational motion of a viscoelastic planet in a central force field

Details The evolution of the translational-rotational motion of a viscoelastic planet in a central force field The evolution of the translational-rotational motion of a viscoelastic planet in a central force field

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..861v&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, July-Aug. 1988, p. 861-867. In Russian.

Astronomy and Astrophysics

Astronomy

1

Planetary Evolution, Planetary Rotation, Translational Motion, Viscoelasticity, Canonical Forms, Energy Dissipation, Solar System

Scientific paper

The averaging method has been applied to obtain approximate equations describing the evolution of translation-rotational motion of a viscoelastic planet in the plane case. The equations are written down in the form using known Delaunay-Andoyer canonical variables. The described motion of a deformed planet in presence of energy dissipation can serve to simulate the tidal phenomena in the motion of a planet of the solar system.

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