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21 February 2003Darwin ground-based European Nulling Interferometer Experiment (GENIE)
Philippe Gondoin,1 Olivier Absilhttps://orcid.org/0000-0002-4006-6237,2 C. V. Malcolm Fridlund,1 Christian Erd,1 Roland H. den Hartog,1 Nicola Rando,1 Andreas Glindemann,3 Bertrand Koehler,3 Rainer Wilhelm,3 Anders Karlsson,1 L. Labadie,1 I. Mann,1 Anthony J. Peacock,1 Andrea Richichi,3 Zoran Sodnik,1 Massimo Tarenghi,3 Sergio Volonte4
1European Space Agency (Netherlands) 2Observatoire de Paris-Meudon (France) 3European Southern Observatory (Germany) 4European Space Agency (France)
Darwin is one of the most challenging space projects ever
considered by the European Space Agency (ESA). Its principal
objectives are to detect Earth-like planets around nearby stars and to characterize their atmospheres. Darwin is conceived as a space
"nulling interferometer" which makes use of on-axis destructive
interferences to extinguish the stellar light while keeping the
off-axis signal of the orbiting planet. Within the frame of the Darwin program, the European Space Agency (ESA) and the European Southern Observatory (ESO) intend to build a ground-based technology
demonstrator called GENIE (Ground based European Nulling
Interferometry Experiment). Such a ground-based demonstrator built
around the Very Large Telescope Interferometer (VLTI) in Paranal will
test some of the key technologies required for the Darwin Infrared Space Interferometer. It will demonstrate that nulling interferometry can be achieved in a broad mid-IR band as a precursor to the next phase of the Darwin program. The present paper will describe the objectives and the status of the project.
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Philippe Gondoin, Olivier Absil, C. V. Malcolm Fridlund, Christian Erd, Roland H. den Hartog, Nicola Rando, Andreas Glindemann, Bertrand Koehler, Rainer Wilhelm, Anders Karlsson, L. Labadie, I. Mann, Anthony J. Peacock, Andrea Richichi, Zoran Sodnik, Massimo Tarenghi, Sergio Volonte, "Darwin ground-based European Nulling Interferometer Experiment (GENIE)," Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); https://doi.org/10.1117/12.458573