  In this paper, we study the spin precession frequency of a test gyroscope
attached to a stationary observer in the five dimensional rotating Kaluza-Klein
black hole (RKKBH). We derive the conditions under which the test gyroscope
moves along a timelike trajectory in this geometry and the regions where the
spin precession frequency diverges. The magnitude of the gyroscope precession
frequency around KK black hole diverges at two spatial locations outside the
event horizon. However in the static case, the behavior of the Lense Thirring
frequency of a gyroscope around KK black hole is much like an ordinary
Schwarzschild black hole. Since a rotating Kaluza-Klein black hole is a
generalization of Kerr-Newman black hole, we present two mass-independent
schemes to distinguish these two spacetimes.
