  We present the lightcurves of two microlensing events from the MACHO Project
data that are likely to be due to lenses with masses similar to Jupiter's mass.
Although the MACHO Project survey data are not sufficient to definitively
establish the identification of planetary mass lenses in these cases,
observations by microlensing follow-up networks such as GMAN and PLANET should
be able to definitively determine the planetary nature of similar events which
may occur in the near future.
