Perturbations due to the shape of the Moon in lunar theory View Full Text


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Article Info

DATE

1980-11

AUTHORS

J. Henrard

ABSTRACT

We compute the perturbations on the motion of the Moon due to its shape. The accuracy is estimated at 1″.10−5 in longitude and latitude and 5 parts in 1011 in distance.

PAGES

335-341

References to SciGraph publications

  • 1969-03. Canonical transformations depending on a small parameter in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1979-05. A new solution to the Main Problem of Lunar Theory in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • Journal

    Author Affiliations

    Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/bf01306908

    DOI

    http://dx.doi.org/10.1007/bf01306908

    DIMENSIONS

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