The DARWIN project |
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| Authors: | A Léger J M Mariotti B Mennesson M Ollivier J L Puget D Rouan J Schneider |
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| Institution: | (1) I.A.S., C.N.R.S., Université Paris XI, Bât 121, 91405 Orsay, Cedex, France |
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| Abstract: | Angel and co-workers have proposed to detect exoplanets around nearby stars in the infrared (6–17  m) and to analyze their spectra, searching for H2O, CO2, CH4, NH3, and O3 spectral features. The presence or absence of CO2 would indicate either a strong similarity or difference with Solar telluric planet atmospheres. Water would indicate a habitable planet, and O3 would reveal significant photosynthesis activity, due to the presence of carbon chemistry based life. Like these authors, we suggest an infrared nulling interferometer pointing to the star and working as a coronograph. Our main contribution is to propose an observatory made of four to five 1-meter class telescopes observing from about 4 to 5 AU to avoid the Solar Zodiacal Light (ZL) background at 10m instead of four 8-meter ones observing from the Earth vicinity. This allows the mission to be feasible in thenear future. The concept, named DARWIN, is under consideration by the European Space Agency for its Horizon 2000 Plus program. |
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