Physics
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kosis..29..201m&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 29, Mar.-Apr. 1991, p. 201-211. In Russian.
Physics
Gravitational Fields, Natural Satellites, Orbit Perturbation, Planetary Orbits, Center Of Mass, Equations Of Motion, Inclination, Motion Stability, Viscoelasticity
Scientific paper
This paper examines the mechanism for a slow change in the inclination of a satellite's orbital plane caused by the action of dissipative forces arising in a deformable planet. It is shown that, in the case of a nonrotating planet, the change in the orbital plane inclination can occur both toward the equator of the planet and away from the equator. Rotation of the planet affects the inclination of the satellite orbital plane, leading to an eventual coincidence of the satellite orbital plane of with the equatorial plane of the planet.
Markov Iu. G.
Miniaev I. S.
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