  Gravitational redshift is being generally calculated without considering the
rotation of a body. Neglecting the rotation, the geometry of space time can be
described by using the spherically symmetric Schwarzschild geometry. Rotation
has great effect on general relativity, which gives new challenges on
gravitational redshift. When rotation is taken into consideration spherical
symmetry is lost and off diagonal terms appear in the metric. The geometry of
space time can be then described by using the solutions of Kerr family. In the
present paper we will discuss the gravitational redshift for rotating body by
using Kerr metric. The numerical calculations has been done under Newtonian
approximation of angular momentum. The variation of gravitational redshift from
equatorial to non - equatorial region has been calculated and its implications
are discussed in detail.
