The apache point observatory lunar laser-ranging operation: Instrument description and first detections

被引:94
作者
Murphy, T. W., Jr. [1 ]
Adelberger, E. G. [2 ]
Battat, J. B. R. [3 ]
Carey, L. N. [4 ]
Hoyle, C. D. [5 ]
LeBlanc, P. [1 ]
Michelsen, E. L. [1 ]
Nordtvedt, K. [6 ]
Orin, A. E. [1 ]
Strasburg, J. D. [7 ]
Stubbs, C. W. [8 ]
Swanson, H. E. [2 ]
Williams, E. [1 ]
机构
[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[2] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[5] Humboldt State Univ, Dept Phys & Astron, Arcata, CA 95521 USA
[6] NW Anal, Bozeman, MT USA
[7] Pacific NW Natl Lab, Richland, WA USA
[8] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
基金
美国国家科学基金会;
关键词
D O I
10.1086/526428
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A next-generation lunar laser-ranging apparatus using the 3.5 m telescope at the Apache Point Observatory in southern New Mexico has begun science operation. The Apache Point Observatory Lunar Laser-ranging Operation (APOLLO) has achieved 1 mm range precision to the moon, which should lead to approximately 1 order-of-magnitude improvements in several tests of fundamental properties of gravity. We briefly outline the scientific goals, and then give a detailed discussion of the APOLLO instrumentation.
引用
收藏
页码:20 / 37
页数:18
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