26 June 2006 TMT telescope structure system: design and development
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Abstract
The Thirty Meter Telescope (TMT) project has chosen a reference configuration with the telescope elevation axis above the primary mirror. The TMT telescope design has a segmented primary mirror, with 738 segments, nominally 1.2 m across corners, and it uses an articulated tertiary mirror to feed science light to predefined instrument positions on two large Nasmyth platforms. This paper outlines the development of the telescope structural design to meet the motion requirements related to the image quality error budget. The usage of opto-structural performance evaluation tools such as Merit Function Routine are described in addition with the optimization techniques used during the telescope structure design development.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kei Szeto, Kei Szeto, Scott Roberts, Scott Roberts, Simon Sun, Simon Sun, Larry Stepp, Larry Stepp, Jerry Nelson, Jerry Nelson, Mike Gedig, Mike Gedig, Nathan Loewen, Nathan Loewen, Dominic Tsang, Dominic Tsang, } "TMT telescope structure system: design and development", Proc. SPIE 6267, Ground-based and Airborne Telescopes, 62672Q (26 June 2006); doi: 10.1117/12.669731; https://doi.org/10.1117/12.669731
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