Long-term degradation of optical devices on the Moon

被引:71
作者
Murphy, T. W., Jr. [1 ]
Adelberger, E. G. [2 ]
Battat, J. B. R. [3 ]
Hoyle, C. D. [4 ]
McMillan, R. J. [5 ]
Michelsen, E. L. [1 ]
Samad, R. L. [1 ]
Stubbs, C. W. [6 ]
Swanson, H. E. [2 ]
机构
[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[2] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[3] MIT, Dept Phys, Cambridge, MA 02139 USA
[4] Humboldt State Univ, Dept Phys & Astron, Arcata, CA 95521 USA
[5] Apache Point Observ, Sunspot, NM 88349 USA
[6] Harvard Univ, Dept Phys, Cambridge, MA 02318 USA
关键词
Moon; Surface; Instrumentation; Experimental techniques;
D O I
10.1016/j.icarus.2010.02.015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 reflectivicy 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. (C) 2010 Elsevier Inc. All rights reserved.
引用
收藏
页码:31 / 35
页数:5
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