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10 July 2018 LUVOIR thermal architecture (Conference Presentation)
Jonathan W. Arenberg, John Pohner, George Harpole, Jason Hylan, Julie A. Crooke, Bryan D. Matonak, Matthew R. Bolcar, Sang A. Park
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Proceedings Volume 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave; 1069814 (2018) https://doi.org/10.1117/12.2312375
Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States
Abstract
LUVOIR is one of the four large missions being studied for the Astro 2020 decadal review. The LUVOIR observatory is a large, ~9-15m diameter, serviceable concept. The observatory must be highly stable, low 10’s of picometers/10s of minutes and has cold, less than 100K detectors, and warm mirrors, 270K. This paper discusses the evolution of the thermal architecture and discusses the trades evaluated to arrive at the current concept. The next steps in the development will be discussed.
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Jonathan W. Arenberg, John Pohner, George Harpole, Jason Hylan, Julie A. Crooke, Bryan D. Matonak, Matthew R. Bolcar, and Sang A. Park "LUVOIR thermal architecture (Conference Presentation)", Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 1069814 (10 July 2018); https://doi.org/10.1117/12.2312375
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KEYWORDS
Observatories
Mirrors
Sensors
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