Abstract
The emplacement of retroreflectors on the Moon by Apollo astronauts and the Russian Lunakhod spacecraft marked the inception of lunar laser ranging (LLR) and provided a natural laboratory for the study of general relativity. Continuing acquisition of increasingly accurate LLR data has provided enhanced sensitivity to general relativity parameters. Two relativistic effects are investigated in this paper: (1) The Nordtvedt effect, yielding a test of the strong equivalence principle, would appear as a distortion of the geocentric lunar orbit in the direction of the Sun. The inclusion of recent LLR data limits the size of any such effect to 3 ± 4 cm. The sensitivities to the various PPN quantities are also highlighted. (2) The geodetic precession of the lunar perigee is predicted by general relativity as a consequence of the motion of the Earth-Moon system about the Sun; its theoretical magnitude is 19.2 mas/yr. Analysis presented here confirms this value and determines this quantity to a 2% level.
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