Volume 366, Number 1, January IV 2001
|Page(s)||351 - 358|
|Section||Atomic, molecular, and nuclear data|
|Published online||15 January 2001|
MPP01, a new solution for planetary perturbations in the orbital motion of the Moon
DANOF -UMR 8630, Observatoire de Paris, 61 avenue de l'Observatoire, 75014 Paris, France
Accepted: 3 November 2000
We present in this paper MPP01, a new solution for the planetary perturbations in the orbital motion of the Moon. Comparisons of the semi-analytical solution ELP2000-82B to numerical integrations of the Jet Propulsion Laboratory and to LLR observations have shown deficiencies resulting mainly from planetary perturbations series established twenty years ago. The publication of a new planetary solution VSOP2000 and the progresses in numerical tools have contributed to improve the precision of the MPP01 solution. Comparisons between MPP01 and the ELP2000-82B solution for planetary perturbations show differences which are mainly due to the long periodic terms of the solution.
Key words: celestial mechanics, stellar dynamics / Moon / solar system: general
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.