Development of a 4K Sorption Cooler for ESA’s Darwin Mission: System-Level Design Considerations

Author:

Burger J. F.,ter Brake H. J. M.,Holland H. J.,Venhorst G.,Hondebrink E.,Meijer R. J.,Veenstra T. T.,Rogalla H.,Coesel M.,Lozano-Castello D.,Sirbi A.

Publisher

Springer US

Reference18 articles.

1. Darwin — The InfraRed Space Interferometer, The search for Terrestrial Exoplanets and High Resolution Imaging of the Universe, Concept and Feasibility Study Report, ESA-SCI (2000).

2. Queloz D. Planets outside the solar system: Theory and observations, eds. J.M. Mariotti and D. Alloin, Kluwer (1999), pp. 107.

3. Charbonneau D., Brown T.M., Latham D.W., Mayor M, “Detection of planetary transits across a sun-like star,” The Astrophysics Journal, vol. 529 (2000), pp. L45–L48.

4. Collaudin B., Rando N., “Cryogenics in space: a review of the missions and of the technologies,” Cryogenics, vol. 40 (2000), pp. 797–819.

5. Wade L.A., Lindensmith C.A., “Low-power, zero-vibration 5 K sorption coolers for astrophysics instruments,” Adv. in Cryogenic Engineering (2002), pp. 47.

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