The use of the Laplace method in the theory of Iapetus' motion

Details The use of the Laplace method in the theory of Iapetus' motion The use of the Laplace method in the theory of Iapetus' motion

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66.1311g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Nov.-Dec. 1989, p. 1311-1318. In Russian.

Astronomy and Astrophysics

Astronomy

Iapetus, Laplace Equation, Orbital Mechanics, Perturbation, Saturn (Planet), Dione, Gravitational Effects, Rhea (Astronomy), Secular Variations, Sun, Titan

Scientific paper

The Laplace method is used to calculate perturbations in the coordinates of Iapetus, taking into account both long-period and secular perturbations due to Saturn's oblateness and the gravitational attracting forces of the sun, Titan, Rhea, and Dione, as well as short-period perturbations due to the sun and Titan. A numerical analysis of the findings obtained is presented.

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