Direct perturbations of the planets on the moon's motion Results and comparisons

Details Direct perturbations of the planets on the moon's motion Results and comparisons Direct perturbations of the planets on the moon's motion Results and comparisons

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983cemec..30...21s&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 30, May 1983, p. 21-29.

Computer Science

Celestial Mechanics, Moon, Orbit Perturbation, Perturbation Theory, Planet Ephemerides, Accuracy, Truncation Errors

Scientific paper

Using the method of Standaert (1980), a first-order theory for the direct perturbations of the planets on the motion of the moon is computed whose goal is the achievement of an internal accuracy of the order of one meter for all periodic terms of period less than 2000 years. A comparison of the present results with those of Chapront (1980) supports the accuracy claimed, which is better than that of Brown (1897) by three orders of magnitude. Part of the second-order perturbation in the planetary masses has also been computed for the first time.

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