1. Introduction
2. Observations and Reductions
3. Derivation of Cluster Properties
3.1. Extinction, Age, and Metallicity
3.2. Masses
3.3. Velocities
4. Cluster Kinematics: Two Populations?
4.1. Origin of the Disk
4.2. Non-Disk Clusters
5. Discussion
5.1. Environment of the Clusters
5.2. Star/Cluster Formation Rates
5.3. Metallicities
6. Comparison of NGC 3256 with Other Merging Galaxies
7. Summary and Conclusions