Enigmatic lunar seismograms recorded during the Apollo 17 mission in 1972 have so far precluded the identification of shear‐wave arrivals and hence the construction of a comprehensive elastic model of the shallow lunar subsurface. Here, for the first time, we extract shear‐wave information from the Apollo active seismic data using a novel waveform analysis technique based on spatial seismic wavefield gradients. The star‐like recording geometry of the active seismic experiment lends itself surprisingly well to compute spatial wavefield gradients and rotational ground motion as a function of time. These observables, which are new to seismic exploration in general, allowed us to identify shear waves in the complex lunar seismograms, and to derive a new model of seismic compressional and shear‐wave velocities in the shallow lunar crust, critical to understand its lithology and constitution, and its impact on other geophysical investigations of the Moon's deep interior.