Abstract
We examine three possible design approaches for radiative cooling of multiple-aperture missions of the sort required for space IR interferometry, particularly those to be sent out to 5 AU which are aimed at detecting extrasolar terrestrial planets.
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– Individually cooled free-flyers (c.f. MOFFIT): This approach offers adapt-able geometry but access to a limited fraction of the sky, perhaps less than half from elliptical trans-asteroid orbits.
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– Large semi-independent sunshade: This may allow free-flyers access to more of the sky but has many technical challenges.
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– Structurally-linked individually-protected telescopes: This concept can offer protection of the beam lines from all stray light and gives good sky cover-age, but geometry changes may be difficult, limiting its applications to general astronomy.
A possible solution to the last problem is suggested. A unit design based on the PRISM studies at NASA Marshall Space Flight Center is outlined, together with a mission scenario
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References
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© 1997 Springer Science+Business Media Dordrecht
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Hawarden, T.G. (1997). Passive Cooling of Infrared Interferometers in Space. In: Eiroa, C., Alberdi, A., Thronson, H., De Graauw, T., Schalinski, C.J. (eds) Infrared Space Interferometry: Astrophysics & the Study of Earth-Like Planets. Astrophysics and Space Science Library, vol 215. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5468-0_27
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DOI: https://doi.org/10.1007/978-94-011-5468-0_27
Publisher Name: Springer, Dordrecht
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