  We present the first EVN parallax measurements of 6.7 GHz methanol masers in
star forming regions of the Galaxy. The 6.7 GHz methanol maser transition is a
very valuable astrometric tool, for its large stability and confined velocity
spread, which makes it ideal to measure proper motions and parallaxes. Eight
well-studied massive star forming regions have been observed during five EVN
sessions of 24 hours duration each and we present here preliminary results for
five of them. We achieve accuracies of up to 51 $\mu$as, which still have the
potential to be proved by more ideal observational circumstances.
