Evolution of the motion of a viscoelastic planet with reverse rotation in the gravitational field of two point masses

Details Evolution of the motion of a viscoelastic planet with reverse rotation in the gravitational field of two point masses Evolution of the motion of a viscoelastic planet with reverse rotation in the gravitational field of two point masses

Publishing date

May 1988

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..358l&link_type=abstract

Journals

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, May-June 1988, p. 358-365. In Russian.

Science

Physics

Additional info 3

Earth-Venus Trajectories, Gravitational Fields, Orbital Resonances (Celestial Mechanics), Planetary Evolution, Planetary Rotation, Translational Motion, Hamiltonian Functions, Orbit Calculation, Orbit Perturbation, Solar System

Type

Scientific paper

Abstract

An analysis is made of the evolution of the translational-rotational motion of a viscoelastic planet moving in the field of two point masses. A model is developed for the sun-moon-Venus system. The analysis is based on an averaging scheme for investigating resonance regimes in two-frequency oscillatory systems. The results are pertinent to the study of nonlinear resonant processes in the solar system, including the commensurability between the axial and orbital motions of planets.

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