  The Painleve-Gullstrand coordinates provide a convenient framework for
presenting the Schwarzschild geometry because of their flat constant-time
hypersurfaces, and the fact that they are free of coordinate singularities
outside r=0. Generalizations of Painleve-Gullstrand coordinates suitable for
the Kerr geometry have been presented by Doran and Natario. These coordinate
systems feature a time coordinate identical to the proper time of
zero-angular-momentum observers that are dropped from infinity. Here, the
methods of Doran and Natario are extended to the five-dimensional rotating
black hole found by Myers and Perry. The result is a new formulation of the
Myers-Perry metric. The properties and physical significance of these new
coordinates are discussed.
