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

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

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985primm..49...25v&link_type=abstract

Prikladnaia Matematika i Mekhanika (ISSN 0032-8235), vol. 49, Jan.-Feb. 1985, p. 25-34. In Russian.

Physics

2

Celestial Mechanics, Gravitational Fields, Planetary Rotation, Rotating Spheres, Viscoelasticity, Canonical Forms, Evolution (Development), Isotropic Media

Scientific paper

The paper examines the motion of a viscoelastic sphere (a planet) whose center of mass moves in circular orbit in a central Newtonian force field. The method of separation of motions and averaging is used to obtain approximate equations describing the rotational motion of the sphere in canonical variables, and the evolution of this motion is analyzed.

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