  We present a practical method for calculating the gravitational self-force,
as well as the electromagnetic and scalar self forces, for a particle in a
generic orbit around a Kerr black hole. In particular, we provide the values of
all the regularization parameters needed for implementing the (previously
introduced) {\it mode-sum regularization} method. We also address the
gauge-regularization problem, as well as a few other issues involved in the
calculation of gravitational radiation-reaction in Kerr spacetime.
