  We compute the effects on the temperature and precise spectrum of Hawking
radiation from a Schwarzschild black hole when the emitted object is taken to
be spatially extended. We find that in the low-momentum regime, the power
emitted is exponentially suppressed for sufficiently large radiated objects, or
sufficiently small black holes, though the temperature of emission is
unchanged. We numerically determine the magnitude of this suppression as a
function of the size and mass of the object and the black hole, and discuss the
implications for various extended objects in nature.
