  Does the Galaxy contain sources of micro-FRB, lower energy events resembling
the known FRB but detectable only at Galactic distances? The answer to this
question is essential to determining the nature of FRB sources. At typical
($10$ kpc) Galactic distances a burst would be about 117 dB brighter than at a
"cosmological" ($z = 1$) distance. The radiation of Galactic micro-FRB, if they
exist, could be detected after Lunar reflection, or an upper bound on their
rate set, by a modest (20 m at 1.4 GHz) radio telescope staring at the Moon. It
would have all-sky sensitivity. The delay between detection of direct (by
STARE2 or dipoles) and Lunar-scattered radiation would restrict a burst's
position to a narrow arc.
