The space case of the problem of a deformable planet-satellite in the field of an attracting centre.

Physics

Scientific paper

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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.

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