  A black hole casts a shadow as an optical appearance because of its strong
gravitational field. We study the shadow cast by the five-dimensional
Myers-Perry black hole with equal rotation parameters. We demonstrate that the
null geodesic equations can be integrated that allows us to investigate the
shadow cast by a black hole. The shadow of a black hole is found to be a dark
zone covered by deformed circle. Interestingly, the shapes of the black hole
shadow are more distorted and size decreases for larger black hole spins.
Interestingly, it turns out that, for fixed values of rotation parameter, the
shadow is slightly smaller and less deformed than for its four-dimensional Kerr
black counterpart. Further, the shadow of the five-dimensional Kerr black hole
is concentric deformed circles. The effect of rotation parameter on the shape
and size of a naked singularity shadow is also analyzed.
