Volume 42 Issue 5
Feb.  2014
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Wang Fuguo, Yang Fei, Zhang Jingxu. TMT tertiary mirror passive support system conceptual design[J]. Infrared and Laser Engineering, 2013, 42(5): 1269-1274.
Citation: Wang Fuguo, Yang Fei, Zhang Jingxu. TMT tertiary mirror passive support system conceptual design[J]. Infrared and Laser Engineering, 2013, 42(5): 1269-1274.

TMT tertiary mirror passive support system conceptual design

  • Received Date: 2012-09-11
  • Rev Recd Date: 2012-10-15
  • Publish Date: 2013-05-25
  • TMT(Thirty Meter Telescope) was a Ritchey Chrtien optical-infrared thirty meter telescope with 3.594 m2.568 m ellipse flat one and 1 800 kg weight. The tertiary mirror system reflected the light coming from the secondary mirror(M2S) to the science instruments which mounted on the telescope Nasmyth platforms. It had tracking and slewing functions. Tertiary mirror support system included axial support system and lateral support system. Based on the mirror surface figure error requirements, the paper proposed axial support system used 18 point whiffletree structure with surface figure RMS of 118.5 nm after optimum. The surface figure RMS can reach 4.7 nm by the lateral support, and the surface figure RMS was less than 77 nm by axial and lateral support. Based on this support program, the mirror support structure is designed to satisfy weighted and volume requirements.
  • [1] Silva David R, George Angeli, Corinne Boyer, et al. Thirty meter telescope: observatory software requirements, architecture, and preliminary implementation strategies[C]// SPIE, 2008, 7019: 789974-789992.
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    [3] Luc Simard, David Crampton, Brent Ellerbroek, et al. The TMT instrumentation program[C]// SPIE, 2010, 7735:857187-85192.
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    [5] Larry Stepp. Thirty meter telescope project update[C]//SPIE, 2012, 8444: 928006-928019.
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    [8] Jerry Nelson, Sanders Gary H. The status of the thirty meter telescope project[C]//SPIE, 2008, 7012: 788238-788245.
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    [10] Ellerbroek Brent L, Adkins Sean M, Andersen David R, et al. TMT adaptive optics program status report[C]//SPIE, 2012, 8447: 927046-927054.
    [11] Wang Fuguo, Yang hongbo, Yang Fei, et al. Optimization and analysis for the axis support points position of the large aperture mirrors[J]. Infrared and Laser Engineering, 2007, 36(6): 877-880. (in Chinese)王富国, 杨洪波, 杨飞, 等. 大口径主镜轴向支撑点位置优化分析[J]. 红外与激光工程, 2007, 36(6): 877-880.
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    [14] Zhang Dongge, Zhuo Renshan, Li Yaobin. Surrogate models based optimization methods for the axial support points of the primary mirror[J]. Infrared and Laser Engineering, 2012, 41(2): 409-414. (in Chinese)张东阁, 卓仁善, 李耀彬. 反射镜轴向支撑位置优化的代理模型方法[J] 红外与激光工程, 2012, 41(2): 409-414.
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    [16] Cho Myung K. Performance Prediction of the TMT Tertiary Mirror Support System[C]//SPIE, 2008, 7018: 169.
    [17] Kaercher H J, Peter Eisentraeger, Martin S. Mechanical principles of large mirror supports[C]//SPIE, 2010, 7733: 77332O-1-12.
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    [20] Wang Baoxu, Wu Fan, Jiang Shilei, et al. Opto-mechanical analysis and structure optimization of infrared cassegrain optical system[J]. Infrared and Laser Engineering, 2012, 41(7): 1872-1878. (in Chinese)汪宝旭, 伍凡, 蒋世磊, 等. 卡式红外光学系统光机分析与结构优化[J]. 红外与激光工程, 2012, 41(7): 1872-1878.
    [21] Fan Lili, Zhang Jingxu, Jiang Hao, et al. Design of primary mirror support of equatorial telescope[J]. Infrared and Laser Engineering, 2011, 40(3):476-479. (in Chinese)范李立, 张景旭, 姜皓, 等. 极轴式望远镜主镜支撑设计[J]. 红外与激光工程, 2011, 40(3): 476-479.
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TMT tertiary mirror passive support system conceptual design

  • 1. Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences,Changchun 130033,China

Abstract: TMT(Thirty Meter Telescope) was a Ritchey Chrtien optical-infrared thirty meter telescope with 3.594 m2.568 m ellipse flat one and 1 800 kg weight. The tertiary mirror system reflected the light coming from the secondary mirror(M2S) to the science instruments which mounted on the telescope Nasmyth platforms. It had tracking and slewing functions. Tertiary mirror support system included axial support system and lateral support system. Based on the mirror surface figure error requirements, the paper proposed axial support system used 18 point whiffletree structure with surface figure RMS of 118.5 nm after optimum. The surface figure RMS can reach 4.7 nm by the lateral support, and the surface figure RMS was less than 77 nm by axial and lateral support. Based on this support program, the mirror support structure is designed to satisfy weighted and volume requirements.

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