  We study interaction of rotating higher dimensional black holes with a brane
in space-times with large extra dimensions. We demonstrate that a rotating
black hole attached to a brane can be stationary only if the null Killing
vector generating the black hole horizon is tangent to the brane world-sheet.
The characteristic time when a rotating black hole with the gravitational
radius $r_0$ reaches this final stationary state is $T\sim
r_0^{p-1}/(G\sigma)$, where $G$ is the higher dimensional gravitational
coupling constant, $\sigma$ is the brane tension, and $p$ is the number of
extra dimensions.
