Abstract
A new solution for planetary perturbations in the orbital motion of the Moon has been constructed, and is intended to be substitued to the previous one, computed twenty years ago. We present here the results of our computations and comparisons to ELP2000-82B planetary perturbations solution and to the JPL numerical integrations.
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© 2001 Springer Science+Business Media Dordrecht
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Bidart, P. (2001). MPP01, A New Solution for Moon’s Planetary Perturbations. Comparisons to Numerical Integrations. In: Pretka-Ziomek, H., Wnuk, E., Seidelmann, P.K., Richardson, D.L. (eds) Dynamics of Natural and Artificial Celestial Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1327-6_22
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DOI: https://doi.org/10.1007/978-94-017-1327-6_22
Publisher Name: Springer, Dordrecht
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