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서지반출
Performance Analysis for Mirrors of 30 cm Cryogenic Space Infrared Telescope
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  • Performance Analysis for Mirrors of 30 cm Cryogenic Space Infrared Telescope
  • Performance Analysis for Mirrors of 30 cm Cryogenic Space Infrared Telescope
저자명
Park. Kwi-Jong,Moon. Bong-Kon,Lee. Dae-Hee,Jeong. Woong-Seob,Nam. Uk-Won,Park. Young-Sik,Pyo. Jeong-Hyun,Han. Won-Yong
간행물명
Journal of astronomy and space sciences
권/호정보
2012년|29권 3호|pp.321-328 (8 pages)
발행정보
한국우주과학회
파일정보
정기간행물|ENG|
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기타
이 논문은 한국과학기술정보연구원과 논문 연계를 통해 무료로 제공되는 원문입니다.
서지반출

기타언어초록

We have designed a 30 cm cryogenic space infrared telescope for astronomical observation. The telescope is designed to observe in the wavelength range of 0.5~2.1 ${mu}m$, when it is cooled down to 77 K. The result of the preliminary design of the support structure and support method of the mirror of a 30 cm cryogenic space infrared telescope is shown in this paper. As a Cassegrain prescription, the optical system of a 30 cm cryogenic space infrared telescope has a focal ratio of f/3.1 with a 300 mm primary mirror (M-1) and 113 mm secondary mirror (M-2). The material of the whole structure including mirrors is aluminum alloy (Al6061-T6). Flexures that can withstand random vibration were designed, and it was validated through opto-mechanical analysis that both primary and secondary mirrors, which are assembled in the support structure, meet the requirement of root mean square wavefront error < ${lambda}/8$ for all gravity direction. Additionally, when the M-1 and flexures are assembled by bolts, the effect of thermal stress occurring from a stainless steel bolt when cooled and bolt torque on the M-1 was analyzed.