  We present HST WFPC2 images of Stephan's Quintet which encompass three
interacting galaxies and their associated tidal features. These deep,
three-color (B, V, I) images indicate recent, massive stellar system formation
in various regions within the compact group environment. We have identified
star cluster candidates (SCC) both within the interacting galaxies and in the
tidal debris. We compare the SCC colors with stellar population synthesis
models in order to constrain cluster ages, and compare the pattern of formation
of SCC in different regions to the inferred dynamical history of the group.
