  In this article we study the geodesic motion of test particles and light in
the Einstein-Maxwell-Dilaton-Axion black hole spacetime. We derive the
equations of motion and present their solutions in terms of the Weierstra{\ss}
$\wp$-, $\sigma$- and $\zeta$-functions. With the help of parametric diagrams
and effective potentials we analyze the geodesic motion and give a list of all
possible orbit types.
