  We investigate the (electro-)geodesic structure of the Majumdar-Papapetrou
solution representing static charged black holes in equilibrium. We assume only
two point sources, imparting thus the spacetime axial symmetry. We study
electrogeodesics both in and off the equatorial plane and explore the stability
of circular trajectories via geodesic deviation equation. In contrast to the
classical Newtonian situation, we find regions of spacetime admitting two
different angular frequencies for a given radius of the circular
electrogeodesic. We look both at the weak- and near-field limits of the
solution. We use analytic as well as numerical methods in our approach.
