  We show that the recently-discovered orbits of massive stars with closest
approach of ~10^3 Schwarzschild radii from SgrA*, allow winds from these stars
to provide the required mass deposition rate near the black hole horizon. The
observed luminosity of SgrA* does not require viscous transport of angular
momentum, as long as the total wind mass loss rate reaches ~10^{-6} solar
masses per year from the close-in stars. The specific orbits of the nearest
stars should cause modulation of the radio and infrared flux from SgrA* on a
timescale of years in a predictable fashion.
