2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/182189The rate of gravitational collapse (type II) supernovae in our galaxy is uncertain by a factor of three or more. One way to determine the galactic supernova rate is through a radiogeochemical experiment (for example, the molybdenum-technetium experiment) that would integrate the neutrino flux over several million years. While such a measurement is designed to integrate the flux over the entire galaxy, nearby star-forming regions could skew the results. We model the flux from a recently identified such region, the Scorpius-Centaurus OB association, and compare with the flux from the rest of the galaxy.8 pages, no figures; corrected typo, added 2 references; now uses elsart.clsAstrophysicsNuclear Theorytext