  We consider Reissner-Nordstrom solutions in quasi-topological gravity,
obtaining exact solutions to the field equations yielding charged
quasi-topological black holes. We study their thermodynamic behaviour over a
range of parameters that yield ghost-free and stable space times. We find that
a sufficiently negative quasi-topological parameter can yield black holes with
2 horizons, even for zero charge. We discuss the thermodynamic stability for
the class of solutions we obtain. We also describe the structure of exact
charged solutions to $k^{th}$ order quasi-topological gravity.
