Existing models for large-magnitude, right-lateral slip on the San Gregorio-Hosgri fault system imply much more deformation of the onshore block in the Santa Maria basin than is supported by geologic data. This problem is resolved by a model in which dextral slip on this fault system increases gradually from 0-10 km near Point Arguello to ~150 km at Cape San Martin, but such a model requires abandoning the cross-fault tie between Point Sal and Point Piedras Blancas, which requires 90-100 km of right-lateral slip on the southern Hosgri fault. We collected stratigraphic and detrital zircon data from Miocene clastic rocks overlying Jurassic basement at both localities to determine if either section contained unique characteristics that could establish how far apart they were in the early Miocene. Our data indicate that these basins formed in the early Miocene during a period of widespread transtensional basin formation in the central Coast Ranges, and they filled with sediment derived from nearby pre-Cenozoic basement rocks. Although detrital zircon data do not indicate a unique source component in either section, they establish the maximum depositional age of the previously undated Point Piedras Blancas section to be 18 Ma. We also show that detrital zircon trace-element data can be used to discriminate between zircons of oceanic crust and arc affinity of the same age, a potentially useful tool in future studies of the California Coast Ranges. Overall, we find no characteristics in the stratigraphy and provenance of the Point Sal and Point Piedras Blancas sections that are sufficiently unique to prove whether they were far apart or close together in the early Miocene, making them of questionable utility as piercing points. ranging from as great as 80-180 km (e.g., Graham and Dickinson, 1978; Clark et al., 1984; Burnham, 1998; Dickinson et al., 2005) to as little as 4-5 km (Sedlock and Hamilton, 1991; Sorlien et al., 1999). Widely variable estimates of the total amount of slip have widely different implications for the role of the fault in deformation of the central California Coast Ranges and for the degree of seismic hazard it poses (e.g., Hanson et al., 2004; Dickinson et al., 2005). The San Gregorio-Hosgri fault system forms the western boundary of a triangular area of the central California Coast Ranges that is bounded to the east by the San Andreas Fault and to the south by the western Transverse Ranges (Fig. 1). The eastern part of this region is underlain by Cretaceous granitic and metamorphic rocks of the Salinian block, offset from southern California by the San Andreas Fault, together with their Cretaceous and early Cenozoic sedimentary cover (e.g., Page et al., 1979; Barbeau et al., 2005; Sharman et al., 2013). The western part is underlain by Mesozoic Franciscan complex and Jurassic ophiolites of the Nacimiento block, juxtaposed with the Salinian block along the Nacimiento fault (Fig. 1) sometime in the Cretaceous or early Cenozoic (e.g., Dickinson, 1983; Vedder et al., 1983; Jacobson et al., 2011). Mes...