Physics
Scientific paper
Nov 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982m%26p....27..257m&link_type=abstract
Moon and the Planets, vol. 27, Nov. 1982, p. 257-284.
Physics
20
Celestial Mechanics, Earth Orbits, Hamiltonian Functions, Libration, Lunar Rotation, Center Of Mass, Lunar Gravitation, Numerical Integration, Perturbation Theory
Scientific paper
This paper presents a new theory of the libration of the moon, completely analytical with respect to the harmonic coefficients of the lunar gravity field. This field is represented through its third degree harmonics for the torque due to the earth (second degree for the torque due to the sun). The orbital motion of the moon is described by the ELP 2000 solution (Chapront-Touze, 1980) of the main problem of lunar theory. The physical libration variables are obtained as Poisson series and comparisons with the results of Eckhardt (Eckhardt, 1981) and Migus (Migus, 1980) are presented.
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