  We construct exact solutions describing the motion of rotating thin shells in
a fully backreacted five-dimensional rotating black hole spacetime. The radial
equation of motion follows from the Darmois-Israel junction conditions, where
both interior and exterior geometries are taken to be equal angular momenta
Myers-Perry solutions. We show that rotation generates anisotropic pressures
and momentum along the shell. Gravitational collapse scenarios including
rotation are analyzed and a new class of stationary solutions is introduced.
Energy conditions for the matter shell are briefly discussed.
