Massless black holes can be understood as bound states of a (positive-
mass) extreme a = root 3 black hole and a singular object with opposit
e (i.e., negative) mass with vanishing Arnowitt-Deser-Misner (total) m
ass but nonvanishing gravitational field. Supersymmetric balance of fo
rces is crucial for the existence of this kind of bound states and exp
lains why the system does not move at the speed of light. We also expl
ain how supersymmetry allows for negative mass as long as it is never
isolated but in bound states of total non-negative mass.