  We present a derivation of the equation of motion for a test-particle in the
framework of the nonsymmetric gravitational theory. Three possible couplings of
the test-particle to the non-symmetric gravitational field are explored. The
equation of motion is found to be similar in form to the standard geodesic
equation of general relativity, but with an extra antisymmetric force term
present. The equation of motion is studied for the case of a static,
spherically symmetric source, where the extra force term is found to take the
form of a Yukawa force.
