Cockell, C.S.; Léger, A.; Fridlund, M.; Herbst, T.M.; Kaltenegger, L.; Absil, O.; Beichman, C.; Benz, W.; Blanc, M.; Brack, A.; Chelli, A.; Colangeli, L.; Cottin, H.; Foresto, F. Coudé du; Danchi, W.C.; Defrère, D.; Herder, J.-W. den; Eiroa, C.; Greaves, J.; Henning, T.; Johnston, K.J.; Jones, H.; Labadie, L.; Lammer, H.; Launhardt, R.; Lawson, P.; Lay, O.P.; LeDuigou, J.-M.; Liseau, R.; Malbet, F.; Martin, S.R.; Mawet, D.; Mourard, D.; Moutou, C.; Mugnier, L.M.; Ollivier, M.; Paresce, F.; Quirrenbach, A.; Rabbia, Y.D.; Raven, J.A.; Rottgering, H.J.A.; Rouan, D.; Santos, N.C.; Selsis, F.; Serabyn, E.; Shibai, H.; Tamura, M.; Thiébaut, E.; Westall, F. and White, G.J.
Darwin — a mission to detect and search for life on extrasolar planets.
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The discovery of extrasolar planets is one of the greatest achievements of modern astronomy. The detection of planets that vary widely in mass demonstrates that extrasolar planets of low mass exist. In this paper, we describe a mission, called Darwin, whose primary goal is the search for, and characterization of, terrestrial extrasolar planets and the search for life. Accomplishing the mission objectives will require collaborative science across disciplines, including astrophysics, planetary sciences, chemistry, and microbiology. Darwin is designed to detect rocky planets similar to Earth and perform spectroscopic analysis at mid-infrared wavelengths (6–20 μm), where an advantageous contrast ratio between star and planet occurs. The baseline mission is projected to last 5 years and consists of approximately 200 individual target stars. Among these, 25–50 planetary systems can be studied spectroscopically, which will include the search for gases such as CO2, H2O, CH4, and O3. Many of the key technologies required for the construction of Darwin have already been demonstrated, and the remainder are estimated to be mature in the near future. Darwin is a mission that will ignite intense interest in both the research community and the wider public.
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