Open Access
23 January 2021 Cryocooling technologies for the Origins Space Telescope
Michael J. DiPirro, Peter Shirron, Mark Kimball, James Tuttle, Amir Jahromi, David Glaister, Jeffrey Olson, Michael Petach, Mark Zagarola
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Abstract

The Origins Space Telescope’s (Origins) significant improvement over the scientific capabilities of prior infrared missions is based on its cold telescope (4.5 K) combined with low-noise far-IR detectors and ultrastable mid-IR detectors. A small number of new technologies will enable Origins to approach the fundamental sensitivity limit imposed by the natural sky background and deliver groundbreaking science. This paper describes a robust plan to mature the Origins mission, enabling cryocooler technology from current state-of-the-art (SOA) to Technology Readiness Level (TRL) 5 by 2025 and to TRL 6 by mission Preliminary Design Review. Entry TRLs corresponding to today’s SOA are 4 or 5, depending on the technology in question.

CC BY: © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
Michael J. DiPirro, Peter Shirron, Mark Kimball, James Tuttle, Amir Jahromi, David Glaister, Jeffrey Olson, Michael Petach, and Mark Zagarola "Cryocooling technologies for the Origins Space Telescope," Journal of Astronomical Telescopes, Instruments, and Systems 7(1), 011008 (23 January 2021). https://doi.org/10.1117/1.JATIS.7.1.011008
Received: 19 June 2020; Accepted: 9 December 2020; Published: 23 January 2021
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CITATIONS
Cited by 8 scholarly publications.
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KEYWORDS
Cryocoolers

Space telescopes

Telescopes

Magnetism

Sensors

James Webb Space Telescope

Space operations

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