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Development of a 170-mm hollow corner cube retroreflector for the future lunar laser ranging |
Yun He(何芸)1,2,3, Qi Liu(刘祺)1,3, Jing-Jing He(何静静)2, Ming Li(黎明)4, Hui-Zong Duan(段会宗)1,3, Hsien-Chi Yeh(叶贤基)1,3, Jun Luo(罗俊)1 |
1 TianQin Research Center for Gravitational Physics, Sun Yat-sen University, Zhuhai 519000, China;
2 MOE Key Laboratory of Fundamental Physical Quantities Measurement, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China;
3 School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519000, China;
4 DFH Satellite Co., Ltd., Beijing 100094, China |
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Abstract Over the past 50 years, lunar laser ranging has made great contributions to the understanding of the Earth-Moon system and the tests of general relativity. However, because of the lunar libration, the Apollo and Lunokhod corner-cube retroreflector (CCR) arrays placed on the Moon currently limit the ranging precision to a few centimeters for a single photon received. Therefore, it is necessary to deploy a new retroreflector with a single and large aperture to improve the ranging precision by at least one order of magnitude. Here we present a hollow retroreflector with a 170-mm aperture fabricated using hydroxide-catalysis bonding technology. The precisions of the two dihedral angles are achieved by the mirror processing with a sub-arc-second precision perpendicularity, and the remaining one is adjusted utilizing an auxiliary optical configuration including two autocollimators. The achieved precisions of the three dihedral angles are 0.10 arc-second, 0.30 arc-second, and 0.24 arc-second, indicating the 68.5% return signal intensity of ideal Apollo 11/14 based on the far field diffraction pattern simulation. We anticipate that this hollow CCR can be applied in the new generation of lunar laser ranging.
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Received: 24 June 2018
Revised: 16 July 2018
Accepted manuscript online:
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PACS:
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07.60.-j
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(Optical instruments and equipment)
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07.07.Df
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(Sensors (chemical, optical, electrical, movement, gas, etc.); remote sensing)
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04.80.Cc
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(Experimental tests of gravitational theories)
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Fund: Project supported by the National Natural Science Foundation of China (Grant Nos. 11655001 and 11605065). |
Corresponding Authors:
Qi Liu
E-mail: liuq239@mail.sysu.edu.cn
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Cite this article:
Yun He(何芸), Qi Liu(刘祺), Jing-Jing He(何静静), Ming Li(黎明), Hui-Zong Duan(段会宗), Hsien-Chi Yeh(叶贤基), Jun Luo(罗俊) Development of a 170-mm hollow corner cube retroreflector for the future lunar laser ranging 2018 Chin. Phys. B 27 100701
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[1] |
Murphy T, Adelberger E, Strasburg J, Stubbs C and Nordtvedt K 2004 Nucl. Phys. B (Proc. Suppl.) 134 155
|
[2] |
Murphy T 2013 Rep. Prog. Phys. 76 076901
|
[3] |
Merkowitz S 2010 Living Rev. Relativ. 13 7
|
[4] |
Murphy T, Adelberger E, Battat J, Carey L, Hoyle C, Leblanc P, Michelsen E, Nordtvedt K, Orin A, Strasburg J, Stubbs C, Swanson H and Williams E 2008 Publ. Astron. Soc. Pac. 120 20
|
[5] |
Turyshev S G, Williams J G, Folkner W M, Gutt G M, Baran R T, Hein R C, Somawardhana R P, Lipa J A and Wang S 2013 Exp. Astron. 36 105
|
[6] |
Currie D, DellAgnello S and Monache G 2011 Acta Astronaut. 68 667
|
[7] |
Murphy T, Adelberger E, Battat J, Hoyle C, McMillan R, Michelsen E, Samad R, Stubbs C and Swanson H 2010 Icarus 208 31
|
[8] |
Currie D, DellAgnello S, Monache G, Behr B and Williams J 2013 Nucl. Phys. B (Proc. Suppl.) 243-244 218
|
[9] |
Araki H, Kashima S, Noda H, Kunimori H, Chiba K, Mashiko H, Kato H, Otsubo T, Matsumoto Y, Tsuruta S, Asari K, Hanada H, Yasuda S, Utsunomiya S and Takino H 2016 Earth Planets Space 68 101
|
[10] |
Wing W H 2003 Opt. Commun. 220 1-6
|
[11] |
Otsubo T, Kunimori H, Noda H and Hanada H 2010 Adv. Space Res. 45 733
|
[12] |
Preston A and Merkowitz S 2013 Appl. Opt. 52 8676
|
[13] |
Preston A and Merkowitz S 2014 Opt. Eng. 53 065107
|
[14] |
Burke J, Oreb B, Platt B and Nemati 2005 Proc. SPIE 5869 58690W
|
[15] |
Oreb B, Burke J, Netterfield R, Seckold J, Leistner A, Gross M and Dligatch S 2006 Proc. SPIE 6292 629202
|
[16] |
Burke J, Green K, Raouf N, Seckold J and Oreb B 2008 Proc. SPIE 7013 701351
|
[17] |
Gwo D 1998 Proc. SPIE 3435 136
|
[18] |
Gwo D, Wang S, Bower K, Davidson D, Ehrersberger P, Huff L, Romero E, Sullivan M, Triebes K and Lipa J 2003 Adv. Space Res. 32 1401
|
[19] |
Ciocci E, Martini M, Contessa S, Procelli L, Mastrofini M, Currie D, Monache G and DellAgnello S 2017 Adv. Space Res. 60 1300
|
[20] |
He Y, Liu Q, Tian W, Duan H, Yeh H, Fan S and Li Y 2017 J. Deep Space Exploration 4 130 (in Chinese)
|
[21] |
He Y, Liu Q, Duan H, Yeh H and Li Y 2016 Proceedings of the 20$th International Workshop on Laser Ranging, October 9-14, 2016, Potsdam, Germany
|
[22] |
He Y, Liu Q, Duan H, He J, Jiang Y and Yeh H 2018 Res. Astron. Astrophys. accepted
|
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