Planetary perturbations of the Moon in ELP 2000 View Full Text


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Article Info

DATE

1982-01

AUTHORS

Jean Chapront, Michelle Chapront-Touze

ABSTRACT

A new solution for the planetary perturbations of the Moon is being built in the frame of ELP 2000, using Bretagnon's planetary theories, and achieved at the first order. It contains the two actions commonly distinguished: direct and indirect. The internal precision of computation is 2×10−6 arcsec. First-order planetary perturbations, in the direct case (Venus & Mars), have been compared to Standaert's solution. The major discrepancy reaches 70 cm in the longitude of Venus. Perturbations of the second order with respect to planetary masses, have been undertaken and illustrations are given. Finally, new values for the perigee and node motions are proposed. More... »

PAGES

83-94

References to SciGraph publications

  • 1980-11. Direct perturbations of the planets on the Moon's motion in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1982-02. Theorie des planetes inferieures in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1982-01. Comments about the direct perturbations of Venus and Mars on the Moon's motion in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1982-01. Perturbations by the oblateness of the Earth and by the planets in the motion of the Moon in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1982-01. Progress in the analytical theories for the orbital motion of the Moon in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/bf01233187

    DOI

    http://dx.doi.org/10.1007/bf01233187

    DIMENSIONS

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