We refine the newly developed seismicity catalog of the Apollo 17 Lunar Seismic Profiling Experiment using quality control algorithms, and speculate on the source mechanisms of thousands of catalogued events using cross-correlation and calculation of event and waveform properties. We first sort these events into two types – “repeating’ or “isolated’ – based on whether or not the event shares similar waveforms with at least one other event. Repeating events are characterized by minimal time between signal onset and maximum, a prevalence during early sunrise, a periodicity consistent with the diurnal cycle, and a preferential direction due east, coincident with the Lunar Module. Isolated events, on the other hand, are distributed throughout the lunar day, originate from a wide variety of directions, and are characterized by a more gradual increase in amplitude. Many repeating events are likely caused by thermal expansion of the Lunar Module or its trapped volatiles, while most isolated events may be caused by thermal fracturing of rock or sliding of regolith along crater slopes. Across both the repeating and isolated events, we pinpoint 43 moonquakes whose time-of-day and waveform characteristics are consistent with thermally-induced fracture of several boulders at the Apollo 17 site. Future lunar missions, particularly those sensitive to ground motion, should be aware of thermally-induced, repeating seismic signals caused by nearby boulders and structures.