Title:
Nulling interferometry for the DARWIN mission: experimental demonstration of the concept in the thermal infrared with high levels of rejection
Authors:
Ollivier, Marc; Mariotti, Jean-Marie; Sekulic, Predrag; Michel, Guy; Leger, Alain M.; Bouchareine, Patrick; Brunaud, Jacqueline; Coude du Foresto, Vincent; Mennesson, Bertrand P.; Borde, Pascal J.; Amy-Klein, A.; Vanlerberghe, A.; Lagage, Pierre-Olivier; Artzner, Guy E.; Malbet, Fabien
Affiliation:
AA(Max-Planck-Institut fuer Astronomie and Univ. Paris-Sud) AB(Observatoire de Paris-Meudon) AC(Univ. Paris-Sud) AD(Observatoire de Paris-Meudon) AE(Univ. Paris-Sud) AH(Observatoire de Paris-Meudon) AK(Univ. Paris-Nord) AM(CEA Saclay) AN(Univ. Paris-Nord)
Journal:
Proc. SPIE Vol. 4006, p. 354-358, Interferometry in Optical Astronomy, Pierre J. Lena; Andreas Quirrenbach; Eds. (SPIE Homepage)
Publication Date:
07/2000
Origin:
SPIE
Abstract Copyright:
(c) 2000 SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Bibliographic Code:
2000SPIE.4006..354O

Abstract

Present projects of space interferometers dedicated to the detection and analysis of extrasolar planets (DARWIN in Europe, TPF in the United States) are based on the nulling interferometry concept. This concept has been proposed by Bracewell in 1978 but has never been demonstrated with high values of rejection, in the thermal infrared range, where the planet detection should be performed (6 - 18 micrometers ). We have thus built a two-beam laboratory interferometer to validate this concept in a monochromatic case (at 10 micrometers ). The keypoint of our interferometer is the use of optical filtering by pinhole and optical fibers to clean the interfering beams. We present in this paper the principle of the experimental setup, its realization, and the first measurements of rejection it allowed. We also present the future developments of this interferometer.