  In this work, we perform a detailed analysis of the equatorial motion of the
charged test particles in Kerr-Newman-Taub-NUT spacetime. By working out the
orbit equation in the radial direction, we examine possible orbit types. We
investigate the conditions for existence of bound orbits in
causality-preserving region as well as the conditions for existence of circular
orbits for charged and uncharged particles. We also study the effect of NUT
parameter on Newtonian orbits. Finally, we give exact analytical solutions of
equations of equatorial motion for a charged test particle.
