Evolution and resonances in the rotational motion of a viscoelastic planet in an elliptical orbit

DOI10.1016/0021-8928(91)90016-NzbMath0803.70006OpenAlexW2040543065MaRDI QIDQ1314032

E. V. Sinitsyn

Publication date: 2 March 1994

Published in: Journal of Applied Mathematics and Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0021-8928(91)90016-n

zbMATH Keywords

method of averagingeccentricityKelvin-Voigt modelmany-parameter modelstable resonant rotation

Mathematics Subject Classification ID

Celestial mechanics (70F15) Dynamical problems in solid mechanics (74Hxx)

Cites Work

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• On fluid flow between rotating surfaces
• The causes of the shimmy phenomenon
• Evolution of the rotational motion of a viscoelastic sphere in a central Newtonian force field
• Motion of a visco-elastic sphere in a central Newtonian force field
• A Nonlinear Theory of Viscoelasticity for Application to Elastomers
• On the motion of a satellite about its center of mass under the action of gravitational moments

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