Current experiments allow the possibility of gluino masses below about
600 MeV if the lifetime of the gluino is longer than 100 psec. If the
mass and lifetime are in this window, then photoproduction of pairs o
f gluino-gluon bound states can provide a means to observe them. The c
ross section is large enough that the window can be fully explored, up
to lifetimes exceeding a microsecond, at high luminosity electron acc
elerators.