  We considered the generation of gravitational waves by the binary system
associated with a wormhole. In the Newtonian limit, the gravitational potential
of a wormhole requires the effective mass of the wormhole taking into account
radial tension effects. This definition allows us to derive gravitational wave
production in homogeneous and heterogeneous binary systems. Therefore, we
studied gravitational waves generation by orbiting wormhole-wormhole and
wormhole-black hole binary systems before coalescence. Cases involving negative
mass require more careful handling. We also calculated the energy loss to
gravitational radiation by a particle orbiting around the wormhole and by a
particle moving straight through the wormhole mouth, respectively.
