Physics
Scientific paper
Dec 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kosis..32...89m&link_type=abstract
Kosmicheskie Issledovaniia, Tom 32, Vyp. 6, p. 89 - 98
Physics
3
Celestial Mechanics: Planetary System
Scientific paper
Translational-rotational motion of a system, consisting of a deformable planet and a satellite, in the field of an attracting centre is considered. Approximate equations of motion are obtained in canonical variables. It is shown that during the tidal evolution, the satellite orbit is tending toward a circular one, and the orbit's radius is monotonously decreasing. Qualitative conclusions on the evolution of the characteristics of the system are given.
Markov Yu. G.
Minyaev I. S.
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