  We study scattering and capture of particles by a rotating black hole in the
five-dimensional spacetime described by the Myers-Perry metric. The equations
of geodesic motion are integrable, and allow us to calculate capture conditions
for a free particle sent towards a black hole from infinity. We introduce a
three-dimensional impact parameter describing asymptotic initial conditions in
the scattering problem for a given initial velocity. The capture surface in
impact parameter space is a sphere for a non-rotating black hole, and is
deformed for a rotating black hole. We obtain asymptotic expressions that
describe such deformations for small rotational parameters, and use numerical
calculations to investigate the arbitrary rotation case, which allows us to
visualize the capture surface as extremal rotation is approached.
