Experimental study of breakaway system for the fast-steering secondary mirror prototype of GMT
Author
Lee, Won GiKim, Sanghyuk
Han, Jeong-Yeol
Jeong, Ueejeong
Kim, Chang-Hee
Lee, Sungho
Moon, Bong-Kon
Park, Chan
Park, Byeong-Gon
Cho, Myung K.
Dribusch, Christoph
Jun, Youra
Ryu, Jieun
Poczulp, Gary
Liang, Ming
Moon, Il-Kwon
Lee, Chan-Hee
Kim, Ho-Sang
Gardner, Paul
Bernier, Robert
Groark, Frank
Chiquito, Hugo
Kim, Yunjong
Affiliation
Univ ArizonaIssue Date
2018Keywords
Extremely Large TelescopeGiant Magellan Telescope
Fast-steering Secondary Mirror
Breakaway System
Tip-Tilt
Metadata
Show full item recordPublisher
SPIE-INT SOC OPTICAL ENGINEERINGCitation
Yunjong Kim, Wongi Lee, Chanhee Lee, Myung K. Cho, Christoph Dribusch, Sungho Lee, Sanghyuk Kim, Chang-Hee Kim, Ueejeong Jeong, Jeong-Yeol Han, Bong-Kon Moon, Chan Park, Byeong-Gon Park, Youra Jun, Jieun Ryu, Gary Poczulp, Ming Liang, Il-Kwon Moon, Ho-Sang Kim, Paul Gardner, Robert Bernier, Frank Groark, and Hugo Chiquito "Experimental study of breakaway system for the fast-steering secondary mirror prototype of GMT ", Proc. SPIE 10706, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III, 107064A (10 July 2018); doi: 10.1117/12.2311779; https://doi.org/10.1117/12.2311779Rights
© 2018 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Fast-steering Secondary Mirror (FSM) of Giant Magellan Telescope (GMT) consists of seven 1.1 m diameter circular segments with an effective diameter of 3.2 m, which are conjugated 1:1 to the seven 8.4 m segments of the primary. Each FSM segment contains a tip-tilt capability for fast guiding to attenuate telescope wind shake and mount control jitter by adapting axial support actuators. Breakaway System (BAS) is installed for protecting FSM from seismic overload or other unknown shocks in the axial support. When an earthquake or other unknown shocks come in, the springs in the BAS should limit the force along the axial support axis not to damage the mirror. We tested a single BAS in the lab by changing the input force to the BAS in a resolution of 10 N and measuring the displacement of the system. In this paper, we present experimental results from changing the input force gradually. We will discuss the detailed characteristics of the BAS in this report.ISSN
97815106196549781510619661
Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2311779
