  The measurement of the integrated optical polarization of weakly
gravitationally lensed galaxies can provide considerable constraints on lens
models. The method outlined depends on fact that the orientation of the
direction of optical polarization is not affected by weak gravitational
lensing. The angle between the semi-major axis of the imaged galaxy and the
direction of integrated optical polarization thus informs one of the distortion
produced by the gravitational lensing. Although the method depends on the
polarimetric measurement of faint galaxies, large telescopes and improved
techniques should make such measurements possible in the near future.
