A method in the theory of planetary-satellite motion

Details A method in the theory of planetary-satellite motion A method in the theory of planetary-satellite motion

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..842a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, July-Aug. 1989, p. 842-849. In Russian.

Astronomy and Astrophysics

Astronomy

4

Equations Of Motion, Natural Satellites, Planetary Orbits, Satellite Orbits, Differential Equations, Gravitation Theory, Liapunov Functions, Trigonometric Functions

Scientific paper

A coordinate method for the construction of the analytical theory of planetary satellite motion is presented. The method is based on an intermediate orbit which includes all of the inequalities due to the influence of the second zonal harmonic of the planetary attraction potential. The method makes it possible to construct the gravitational theory of satellite motion in a purely trigonometric form.

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