The GMT Telescope Metrology System: easing the complexity of initial and operational alignment and increasing observing efficiency

被引:1
|
作者
Sitarski, Breann [1 ]
Rakich, Andrew [2 ]
Chiquito, Hugo [1 ]
Rosenthal, Wylie [1 ]
Pires, Priscila [3 ]
Thompson, Peter [1 ]
Aguayo, Francisco [1 ]
Schoenell, William [1 ]
Schurter, Patricio [1 ]
Brossus, Glenn [1 ]
Conan, Rodolphe [1 ]
Bouchez, Antonin [1 ]
Angeli, George [1 ]
Beifus, Keath [1 ]
Lam, King-Ming [1 ]
Gardner, Paul [1 ]
Thomas, David [1 ]
机构
[1] GMTO Corp, 465 N Halstead St,Suite 250, Pasadena, CA 91107 USA
[2] Mersenne Opt Consulting, 41 Rimu Rd, Paraparaumu 5032, New Zealand
[3] Univ Sao Paulo, Dept Astron, IAG, BR-05508900 Sao Paulo, Brazil
来源
关键词
3D metrology; telescope alignment; pointing models; absolute distance interferometry; differential distance measuring interferometry; active optics;
D O I
10.1117/12.2560681
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Giant Magellan Telescope will be a 25.4-m visible and infrared telescope at Las Campanas Observatory. The optical design consists of 7 8.4-m primary mirror segments that reflect light to 7 secondary mirror segments in a doubly segmented direct Gregorian configuration. Each mirror pair must be coaligned and co-boresighted. During operations, the alignment of the optical components will deflect due to variations in temperature, gravity-induced structure flexure of the mount, and, on a scale relevant to phasing, vibrations. The doubly segmented nature and size of the GMT will create a novel set of challenges for initial assembly, integration, and verification and maintaining high-precision alignment of the optical elements during operations. GMT is developing a Telescope Metrology System (TMS) that uses 3D laser metrology systems to decrease the complexity of alignment and increase observatory efficiency. This paper discusses the 4 subsystems of TMS as well as their operational modes.
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页数:18
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