Presentation + Paper
10 October 2023 PRIMA space telescope cryocooling system
Weibo Chen, Bradley Moore, Michael DiPirro, Peter Shirron, Michael Petach
Author Affiliations +
Abstract
The PRobe far Infrared Mission for Astrophysics (PRIMA) is a mission concept for a NASA cryogenic observatory in an Earth-Sun L2 halo orbit, designed to reveal how abundant elements are built up in galaxies over cosmic time. To achieve the target sensitivity in the wavelength range of 25 to at least 200 microns, its wideband spectrometer and multiband spectrophotometric imager/polarimeter need to operate at 0.1 K, and its primary mirror and relay optics need to be at 4.5 K. To meet these cooling needs, the PRIMA study team is designing a cryogen-free cooling system with a combination of passive radiators and thermal shields, a hybrid mechanical cooler and a continuous Adiabatic Demagnetization Refrigerator system. The PRIMA mechanical cooler is slightly modified JWST Mid-Infrared Instrument (MIRI) cooler that uses 3He as the working fluid in its JT stage. This paper first discusses the overall thermal requirements and the system's thermal architecture and then describes the main thermal subsystems in the cryocooling chain. Finally, the paper presents compressor and 3He Joule-Thomson (JT) effect test results to validate the predicted performance of PRIMA’s 4.5 K mechanical cryocooler.
Conference Presentation
(2023) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Weibo Chen, Bradley Moore, Michael DiPirro, Peter Shirron, and Michael Petach "PRIMA space telescope cryocooling system", Proc. SPIE 12687, Infrared Sensors, Devices, and Applications XIII, 1268705 (10 October 2023); https://doi.org/10.1117/12.2675697
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KEYWORDS
Cryogenics

Design and modelling

Telescopes

Cryocoolers

Thermal analysis

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