Evolution of the rotational motion of a viscoelastic sphere in a central Newtonian force field

DOI10.1016/0021-8928(85)90121-2zbMath0598.70014OpenAlexW1985016736MaRDI QIDQ1079965

V. G. Vil'ke, Yu. G. Markov, Sergey A. Kopylov

Publication date: 1985

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(85)90121-2

zbMATH Keywords

averagingcircular orbitmethod of separation of motionsapproximate equationscentral Newtonian force fieldhomogeneous isotropic elastic spheremotion of a viscoelastic sphererotary motion of the sphere in canonical Andoyer variablestidal hump

Mathematics Subject Classification ID

Free motion of a rigid body (70E15) Dynamics of a system of particles, including celestial mechanics (70F99) Celestial mechanics (70F15) Materials of strain-rate type and history type, other materials with memory (including elastic materials with viscous damping, various viscoelastic materials) (74D99)

Related Items (4)

Sensitivity of the Euler-Poinsot tensor values to the choice of the body surface triangulation mesh ⋮ Keeping a solar sail near the triangular libration point of a dumbbell-shaped or binary asteroid ⋮ Stationary solutions in a model three-body problem ⋮ Evolution and resonances in the rotational motion of a viscoelastic planet in an elliptical orbit

Cites Work

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• On libration points near a gravitating and rotating triaxial ellipsoid
• On stability of an autonomous Hamiltonian system with two degrees of freedom under first-order resonance

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