We consider the spacetimes corresponding to static global monopoles with in
terior boundaries corresponding to a black hole horizon and analyse the beh
aviour of the appropriate ADM mass as a function of the horizon radius r(H)
. We find that for small enough rH, this mass is negative as in the case of
the regular global monopoles, but that for large enough rH the mass become
s positive, encountering an intermediate value for which we have a black ho
le with zero ADM mass.