  I review recent developments in numerical relativity, focussing on progress
made in 3D black hole evolution. Progress in development of black hole initial
data, apparent horizon boundary conditions, adaptive mesh refinement, and
characteristic evolution is highlighted, as well as full 3D simulations of
colliding and distorted black holes. For true 3D distorted holes, with Cauchy
evolution techniques, it is now possible to extract highly accurate,
nonaxisymmetric waveforms from fully nonlinear simulations, which are verified
by comparison to pertubration theory, and with characteristic techniques
extremely long term evolutions of 3D black holes are now possible. I also
discuss a new code designed for 3D numerical relativity, called Cactus, that
will be made public.
