Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....91..233c&link_type=abstract
Astronomy and Astrophysics, vol. 91, no. 1-2, Nov. 1980, p. 233-246. In French.
Astronomy and Astrophysics
Astrophysics
23
Celestial Mechanics, Gravitational Effects, Lunar Orbits, Orbit Perturbation, Selenology, Differential Equations, Earth-Moon System, Equations Of Motion
Scientific paper
The planetary perturbations of the moon are analyzed by the ELP-1900 solution methods with planetary expressions for the inverses of the distances between the earth and planets based on Bretagnon (1980). The equations of motion in the rotating system referred to the ecliptic of the date determine four force functions acting on the moon; an expression is derived for direct actions, in which the planetary portion depends on the powers of inverse distances between the barycenter of the earth-moon system. In indirect cases, the planetary part depends on the solution for the solar orbit around the barycenter, expressed by the developments of the six elliptic elements in the Bretagnon theory.
Chapront Jean
Chapront-Touze Michelle
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