  We investigate the ability of ground based gravitational wave observatories
to detect gravitational wave lensing events caused by stellar mass lenses. We
show that LIGO and Virgo possess the sensitivities required to detect lenses
with masses as small as $\sim 30 M_\odot$ provided that the gravitational wave
is observed with a signal-to-noise ratio of $\sim30$. Third generation
observatories will allow detection of gravitational wave lenses with masses of
$\sim 1 M_\odot$. Finally, we discuss the possibility of lensing by multiple
stars, as is the case if the gravitational radiation is passing through
galactic nucleus or a dense star cluster.
