We consider geodesic equations for a black hole solution in the Randall-Sundrum II scenario presented in [1]. This solution is a generalization of the Schwarzschild one and has the mathematical form of the Reissner-Nördstrom solution, but with an additional "tidal charge" instead of the electric charge. We examine the behavior of geodesic parameters and show that the solution does not contradict the observational data and does not predict any fundamentally new effects. A more serious restriction on the "tidal charge" value can be extracted from the circular orbit equation. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.