  Within the scenario of large extra dimensions, the Planck scale is lowered to
values soon accessible. Among the predicted effects, the production of TeV mass
black holes at the {\sc LHC} is one of the most exciting possibilities. Though
the final phases of the black hole's evaporation are still unknown, the
formation of a black hole remnant is a theoretically well motivated
expectation. We analyze the observables emerging from a black hole evaporation
with a remnant instead of a final decay. We show that the formation of a black
hole remnant yields a signature which differs substantially from a final decay.
We find the total transverse momentum of the black hole event to be
significantly dominated by the presence of a remnant mass providing a strong
experimental signature for black hole remnant formation.
