High Precision Lunar Tracking For Laser Ranging
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Laser ranging to lunar surface retro-reflectors has provided a valuable source of data for the investigation of the lunar orbit, the earth's orientation in space, general relativity, and many other aspects of solar system dynamics.1,2,3 Due to the moon's relatively large distance, and the requirement to keep the beam from the relatively low-power laser very narrow, acquiring this data type requires very accurate telescope pointing and tracking capabilities. The nominal requirement is to keep the telescope on target within approximately 1 arc-sec of its predicted location for at least several minutes. An expansion of this requirement and the methods we have used to accomplish this high precision pointing are presented. Difficulties encountered and a few future goals of automating the McDonald station are also discussed.
[1] J. Derral Mulholland,et al. Scientific Achievements From Ten Years of Lunar Laser Ranging (Paper 80R0466) , 1980 .
[2] P. Shelus,et al. MLRS: A Lunar/Artificial Satellite Laser Ranging Facility at the McDonald Observatory , 1985, IEEE Transactions on Geoscience and Remote Sensing.
[3] Peter John Shelus. Fundamental coordinate ties using laser ranging data , 1985 .