An effect in the resonance motion of deformable planets in the restricted three-body problem

Details An effect in the resonance motion of deformable planets in the restricted three-body problem An effect in the resonance motion of deformable planets in the restricted three-body problem

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kosis..31....3l&link_type=abstract

Kosmicheskie Issledovaniya, vol. 31, p. 3

Physics

Three Body Problem, Planetary Orbits, Orbital Resonances (Celestial Mechanics), Planetary Rotation, Angular Velocity, Viscoelasticity

Scientific paper

The translational-rotational motion of two deformable planets in the restricted three-body problem is analyzed. The results confirm that tidal evolution results in a trend toward commensurability between the mean angular velocities of rotational and orbital motions. An effect is discovered whereby the axis of symmetry of a dynamically stretched planet deviates from the line connecting the centers of mass of the planets by a small angle proportional to the parameters that determine the viscoelastic properties of the planet.

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