A field rotator dedicated to compensate for the celestial field rotati
on has been designed and built for the Grand Interferometre a 2 Telesc
opes (GI2T) by the Laboratoire d'Astronomie Spatiale (LAS). In each in
terferometric arm, we introduce a three-reflection optics rotatable ar
ound ?he axis of the optical train. Since the visibility of the interf
erence fringe pattern is mostly sensitive to the differential instrume
ntal polarization, this device must fulfill not only optomechanical re
quirements but also polarization constraints. For this purpose, three
metallic reflections at small incidences are preferred to classical K-
prisms (such as Dove or Koenig-Abbe prisms) and coatings optimization
leads to protected silver mirrors. (C) 1998 Society of Photo-Optical i
nstrumentation Engineers.