One effect in the resonant motion of deformable planets in the limited three-body problem.

Details One effect in the resonant motion of deformable planets in the limited three-body problem. One effect in the resonant motion of deformable planets in the limited three-body problem.

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cosre..31..351l&link_type=abstract

Cosmic Res., Vol. 31, No. 4, p. 351 - 357

Physics

Planets: Motions, Planets: Three-Body Problem, Three-Body Problem: Restricted

Scientific paper

Translational-rotational motions of two deformable planets are investigated in the limited three-body problem. It is confirmed that tidal evolution creates a tendency to commensurability between the mean angular velocities of the rotational and orbital motions. It is found that there is an effect in which the symmetry axis of a dynamically deformable planet deviates from the line joining the centers of mass of the planets through a small angle proportional to the parameters that determine the viscoelastic properties of the planet.

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