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Long-term degradation of optical devices on the Moon
Authors:TW Murphy Jr  EG Adelberger  CD Hoyle  EL Michelsen  CW Stubbs
Institution:a University of California, San Diego, Dept. of Physics, La Jolla, CA 92093-0424, United States
b University Washington, Dept. of Physics, Seattle, WA 98195-1560, United States
c Massachusetts Institute of Technology, Dept. of Physics, Cambridge, MA 02139, United States
d Humboldt State University, Dept. of Physics and Astronomy, Arcata, CA 95521-8299, United States
e Apache Point Observatory, Sunspot, NM 88349-0059, United States
f Harvard University, Dept. of Physics, Cambridge, MA 02318, United States
Abstract:Forty years ago, Apollo astronauts placed the first of several retroreflector arrays on the lunar surface. Their continued usefulness for laser ranging might suggest that the lunar environment does not damage optical devices. However, new laser ranging data reveal that the efficiency of the three Apollo reflector arrays is now diminished by a factor of 10 at all lunar phases and by an additional factor of 10 when the lunar phase is near full Moon. These deficits did not exist in the earliest years of lunar ranging, indicating that the lunar environment damages optical equipment on the timescale of decades. Dust or abrasion on the front faces of the corner-cube prisms may be responsible, reducing their reflectivity and degrading their thermal performance when exposed to face-on sunlight at full Moon. These mechanisms can be tested using laboratory simulations and must be understood before designing equipment destined for the Moon.
Keywords:Moon  Surface  Instrumentation  Experimental techniques
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