  We discuss the prospects for detecting nu_{mu,tau} and nu_{tau}neutrinos from
Type II supernovas using the novel detector at the Supernova Burst Observatory
(SNBO) or OMNIS that is being designed for an underground laboratory in the
USA. This detector would collect ~2000 flavor selected events from a Galactic
supernova and could probe neutrino mass down to a few eV, as well as the
dynamics of the supernova process. We believe this is essential to further our
understanding of the neutrino section of elementary particle physics.
