  It is suggested that gravity waves could, in several cases, be detected by
means of already (or shortly to be) available technology, independently of
current efforts of detection. The present is a follow-up on a recently
suggested detection strategy based on gravity-wave-induced deviations of null
geodesics. The new development is that a way was found to probe the waves close
to the source, where they are several orders of magnitude larger than on the
Earth. The effect translates into apparent shifts in stellar angular positions
that could be as high as $10^{-7}$ arcsec, which is just about the present
theoretical limit of detectability. (Calculation improved; results unchanged.)
