  This study is purposed to derive the equation of motion for geodesics in
vicinity of spacetime of a (2 + 1)-dimensional charged BTZ black hole. In this
paper, we solve geodesics for both massive and massless particles in terms of
Weierstrass elliptic and Kleinian sigma hyper-elliptic functions. Then we
determine different trajectories of motion for particles in terms of conserved
energy and angular momentum and also using effective potential.
