Presentation + Paper
29 August 2022 Development of a wide field telescope for the NSOS-α
Author Affiliations +
Abstract
The design of the Near Space Optical Survey-alpha (NSOS-α) telescope, encouraged by Korea Astronomy and Space Science Institute (KASI) aims to discover and catalog near-Earth asteroids, especially Potentially Hazardous Asteroids (PHAs). To achieve this goal, an optical telescope with a 1.5m class primary mirror and a 5 square degree field of view will be installed and operated at Cerro Tololo Inter-American Observatory (CTIO) in Chile. The wide field telescope is under development and being designed by a collaboration between KASI and the NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab). A prime focus configuration was adopted and designed with a seven element wide field corrector (WFC). The main mechanical design philosophy was scaled, modified, and revised based on the Korea Microlensing Telescope Network (KMTNet). The NSOS-α telescope will be the first dedicated observation facility for asteroid survey in the southern hemisphere using a 1.5-meter class telescope. In this paper, a summary of the optical and mechanical assemblies designed for the NSOS-α telescope will be addressed.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Myung Cho, Hong-Suh Yim, Jaemann Kyeong, Gary Poczulp, Jung Hyun Jo, Myung-Jin Kim, Ming Liang, Ellie Hileman, and Sungki Cho "Development of a wide field telescope for the NSOS-α", Proc. SPIE 12188, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation V, 1218813 (29 August 2022); https://doi.org/10.1117/12.2629307
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KEYWORDS
Telescopes

Mirrors

3D modeling

Computer aided design

Solid modeling

Optical instrument design

Cameras

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