The use of LLR observations (1969-2006) for the determination of the celestial coordinates of the pole

Details The use of LLR observations (1969-2006) for the determination of the celestial coordinates of the pole The use of LLR observations (1969-2006) for the determination of the celestial coordinates of the pole

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jsrs.meet..123z&link_type=abstract

"Proceedings of the "Journées Systèmes de Référence Spatio-temporels 2007". Observatoire de Paris, 17-19 September 2007. Editor:

Physics

Scientific paper

Analysis of Lunar Laser ranging observations allows to determine a number of parameters related to the dynamics of the Earth-Moon system. It also contributes to the determination of the Earth Orientation Parameters (EOP) such as precession-nutation, polar motion and UT1. Here, we focus on the determination of the precession-nutation corrections DX, DY to the conventional model for the coordinates of the CIP (Celestial Intermediate Pole) in the GCRS (Geocentric Celestial Reference System), which are used in this study, instead of the classical parameters determined in previous works.

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