Paper
18 August 2005 Cooling large space telescopes to 4 kelvin
Author Affiliations +
Abstract
To obtain sky background limited viewing in the mid and far infrared, cooling the telescope itself is required. In the past the lowest temperatures have been achieved using stored cryogen systems. Due to weight constraints and the desire for long life observatories, stored cryogen coolers will be replaced by passive coolers, mechanical coolers and solid state coolers. Some of the challenges and opportunities presented by these large cold telescopes and cryogenic cooling systems are described with emphasis on telescopes that require temperatures below 6 K.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael DiPirro "Cooling large space telescopes to 4 kelvin", Proc. SPIE 5899, UV/Optical/IR Space Telescopes: Innovative Technologies and Concepts II, 58990W (18 August 2005); https://doi.org/10.1117/12.613949
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KEYWORDS
Space telescopes

Telescopes

Cryocoolers

Cryogenics

Space operations

Mirrors

Observatories

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