Optical design, modelling and tolerancing of a Fizeau interferometer dedicated to astrometry.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Instrumentation: Interferometers, Telescopes, Astrometry

Scientific paper

Space-based interferometers dedicated to wide-angle astrometry would dramatically increase the accuracy of angular measurements fundamental to a wide range of astrophysical problems. The proposed Global Astrometric Interferometer for Astrophysics (GAIA), a continuously rotating instrument comprising two or three interferometers, will reach the 5-20μas level on more than 35 million objects. The necessary wide field-of-view for such a precision could be obtained with a Fizeau interferometer. We designed and modelled a 2.6m baseline interferometer with two 40cm apertures, and overall dimensions compatible with the size of the Ariane V payload shroud. It has a ~1degree diffraction limited field-of-view. The response of the optical system to small perturbations on each optical element is given in terms of fringe visibility, which is shown to depend mainly on sub-aperture spot separation. The robustness of the design to thermal, mechanical and manufacturing errors is discussed.

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