We apply linear perturbation theory to the study of the universality a
nd criticality first observed by Choptuik in gravitational collapse. S
ince these are essentially nonlinear phenomena our approach provides a
rough approximation. In spite of this, universal behavior of the fina
l black hole mass is observed with an exponent only slightly higher th
an the observed value of 0.367. The universal behavior is based on the
unique form that in-falling perturbations on black holes have at the
horizon.