STRATIGRAPHIC ANALYSIS OF THE LATE MIOCENE BOLEO FORMATION, SANTA ROSALIA BASIN, BAJA CALIFORNIA SUR, MEXICO
We document doubling of thickness of sediments toward the SE between Mantos 3 and 2, and a lateral change to conglomerate-dominated facies in the SE-most section (Arroyo Purgatorio). Inverse grading, general absence of cross bedding, and rare erosional scours in conglomeratic facies support an alluvial fan setting for proximal deposits in the SE. The coarse alluvial-fan facies pass laterally to the NW into fine-grained, rhythmically laminated mud, silt and sand which we tentatively interpret as tidal rhythmites, consistent with a marginal-marine model proposed by Conly et al. (2006). The southeast-ward increase of stratigraphic thickness can be attributed to an increase in the rate of production of accommodation space closer to the sediment source, which we infer was due to fault-controlled tilting and increased subsidence toward the SE during deposition. The observed pattern can be explained by deposition in a pull-apart basin that was bounded by NW-striking transform faults on the NE and SW margins of the basin, and tilted southeast toward a NW-dipping normal fault. The lack of marine fossils likely can likely be explained by a high rate of siliciclastic input, and/or chemical toxins produced by active volcanism and geothermal activity. Future study of micropaleontology and fault kinematics may provide more insight into the controls on deposition of the Boleo Formation.