  Non-commutative corrections to the classical expression for the fuzzy sphere
area are found out through the asymptotic expansion for its heat kernel trace.
As an important consequence, some quantum gravity deviations in the luminosity
of black holes must appear. We calculate these deviations for a static,
spherically symmetric, black-hole with a horizon modeled by a fuzzy sphere. The
results obtained could be verified through the radiation of black holes formed
in the Large Hadron Collider (LHC).
