Resonance phenomena accompanying evolution of translational-rotational motion of viscoelastic planet

Details Resonance phenomena accompanying evolution of translational-rotational motion of viscoelastic planet Resonance phenomena accompanying evolution of translational-rotational motion of viscoelastic planet

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rpsct...1...47v&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 47 (SEE N87-29547 24-12) Transl. into ENGLISH from Kosmicheskiye Issle

Physics

Dynamic Stability, Planetary Rotation, Resonance, Translational Motion, Viscoelasticity, Equations Of Motion, Planetary Orbits

Scientific paper

Resonance phenomena in the translational-rotational motion of a viscoelastic planet are investigated theoretically on the basis of equations of motion derived by Vil'ke (1984). It is shown that, in the presence of resonances, the evolution rate of the rotational motion of the planet can be sharply reduced; i.e., the planet will remain for a sufficiently long time in the state of resonance rotation. However, the orbital evolution continues to proceed, and the system ultimately leaves the resonance regime.

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