Relaxation in a kaon condensate proceeds through nonequilibrium weak r
eactions, which includes the kaon-induced Urea and the modified Urea r
eactions. The kinetics of a K- condensate is considered semiclassicall
y starting from a small seed of a condensate with the assumption that
the system is in thermal equilibrium. It is shown that the temporal ev
olution to the K--condensed phase in the kinetic regime is divided int
o several characteristic time intervals as a result of the interplay b
etween the two major weak processes. The implications for the dynamica
l evolution of newly-born neutron stars are briefly discussed.