Dissipative evolution of translational-rotational motion of the system comprising a deformable planet and its satellite.

Details Dissipative evolution of translational-rotational motion of the system comprising a deformable planet and its satellite. Dissipative evolution of translational-rotational motion of the system comprising a deformable planet and its satellite.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999kosis..37..306k&link_type=abstract

Kosmicheskie Issledovaniia, Tom 37, No. 3, p. 306 - 311

Computer Science

Celestial Mechanics: Motions, Celestial Mechanics: Planets, Celestial Mechanics: Planetary Satellites

Scientific paper

Approximate (averaged) equations are derived from the obtained exact equations of translational-rotational motion of a system comprising a deformable planet and its satellite. Slow evolution of inclinations and rotations on time intervals that significantly exceed the periods of precession and nutation of the orbital plane is studied by means of these approximate equations.

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