The Lagrangian equations of motion for massive spinning test particles (tops)
moving on a gravitational background using general relativity are presented.
The paths followed by tops are nongeodesic.An exact solution for themotion of
tops on a Schwarzschild background which allows for superluminal propagation
of tops is studied. It is shown that the solution becomes relevant for particles
with small masses, such as neutrinos. This general result is used to calculate the
necessary condition to produce superluminal motion in part of the trajectory
of a small mass particle in a weak gravitational field. The condition for
superluminal motion establishes a relation between the mass, energy and total
angular momentum of the particle.