We present radial velocity measurements for globular clusters in M60, a giant elliptical galaxy in the Virgo Cluster. Target globular cluster candidates were selected using Washington photometry based on deep 16 -->' × 16 -->' images taken at the KPNO 4 m telescope and using VI photometry derived from Hubble Space Telescope WFPC2 archival images. The spectra of the target objects were obtained with the Multi-Object Spectrograph at the Canada-France-Hawaii Telescope. We have measured the radial velocities of 111 objects in the field of M60: 93 globular clusters (72 blue globular clusters with 1.0 ≤ C– -->T1 T1 + 27−25 km s−1, which is in good agreement with the velocity of the nucleus of M60 ( -->vgal = 1056 km s−1). Combining our results with data from the literature, we present a master catalog of radial velocities for 121 globular clusters in M60. The velocity dispersion of the clusters in the master catalog is found to be 234 -->+ 13−14 km s−1 for the entire sample, 223 -->+ 13−16 km s−1 for 83 blue globular clusters, and 258 -->+ 21−31 km s−1 for 38 red globular clusters.