  We find a new, non-commutative geometry inspired, solution of the coupled
Einstein-Maxwell field equations describing a variety of charged,
self-gravitating objects, including extremal and non-extremal black holes. The
metric smoothly interpolates between deSitter geometry, at short distance, and
Reissner-Nordstroem geometry far away from the origin. Contrary to the ordinary
Reissner-Nordstroem spacetime there is no curvature singularity in the origin
neither "naked" nor shielded by horizons. We investigate both the Hawking
process and pair creation in this new scenario.
