The difference in absolute magnitude between two objects is related to their fluxes by the flux-magnitude relation. FA FB = 2.51(MB − MA) A distant galaxy contains a supernova with an absolute magnitude of −19. If this supernova were placed next to our Sun (M = 4.8) and you observed them both from the same distance, how much more flux would the supernova emit than the Sun? Fsupernova FSun =