We present new broadband optical photometry of Centaurs and Kuiper Bel
t objects from the Keek 10 m, the University of Hawaii 2.2 m, and the
Cerro Tololo InterAmerican Observatory (CTIO) 1.5 m telescopes. These
objects are believed to represent large protocomets in different stage
s of dynamical evolution. We find a wide dispersion in the optical col
ors of the objects, indicating nonuniform surface properties. The colo
r dispersion must be understood in the context of the expected steady
reddening due to bombardment by the ubiquitous flux of cosmic rays. We
describe a model in which the dispersion is produced by stochastic co
llisional resurfacing. While non-unique, this model provides a plausib
le match to the observed color spread. (C) 1996 American Astronomical
Society.