A general theory of motion for the eight major satellites of Saturn. I - Equations and method of resolution

Details A general theory of motion for the eight major satellites of Saturn. I - Equations and method of resolution A general theory of motion for the eight major satellites of Saturn. I - Equations and method of resolution

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...243..263d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 1, March 1991, p. 263-275.

Astronomy and Astrophysics

Astronomy

20

Equations Of Motion, Orbit Perturbation, Orbital Resonances (Celestial Mechanics), Saturn Satellites, Galilean Satellites, Space Exploration, Voyager 2 Spacecraft, Saturn, Satellites, Theoretical Studies, Motion, Calculations, Mimas, Techniques, Resonance, Equations Of Motion, Parameters, Eccentricity, Orbital Elements, Procedure, Astronomy, Enceladus, Tethys, Dione, Rhea, Titan, Hyperion, Iapetus

Scientific paper

A new method to construct an analytical theory of motion of Saturn's satellites is presented. It is an extension of the methods already used by Duriez (1979) and Laskar (1984) to construct a general planetary theory, using the same formalism to deal with the multiple resonances occurring in the saturnian system. The present goal is to obtain accurate representations of motions, adequate to future space observations. Thus, great care is taken in the construction of the models, which remains completely analytical with respect to physical parameters and constants of motion. Some preliminary results are given, which indicate good agreement with previous theories.

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