Resonance phenomena in the evolution of the translational-rotational motion of a viscoelastic planet

Details Resonance phenomena in the evolution of the translational-rotational motion of a viscoelastic planet Resonance phenomena in the evolution of the translational-rotational motion of a viscoelastic planet

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..148v&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, Jan.-Feb. 1987, p. 148-152. In Russian.

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.

Affiliated with

Also associated with

No associations

Rating

Resonance phenomena in the evolution of the translational-rotational motion of a viscoelastic planet does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Resonance phenomena in the evolution of the translational-rotational motion of a viscoelastic planet, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resonance phenomena in the evolution of the translational-rotational motion of a viscoelastic planet will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1623973