Origin and evolution of ore-forming fluids of San Dimas deposits

The San Dimas district is a world-class Ag/Au deposit, developed as a telescoped Eocene-Oligocene Ag/Au mineralization located in the Sierra Madre Occidental (SMO) of western Mexico. San Dimas exhibits multiple mineralization events during different magmatic and tectonic episodes from Late Cretaceous to early Oligocene. The well-preserved magmatic-hydrothermal system provides an excellent opportunity to determine the source of silver and gold, the evolution of the hydrothermal fluids, and the controls on the mineralization precipitation. Mineralogical, fluid inclusions, stable and noble gases isotope analyses suggest that the San Dimas deposit consist of two different mineralization styles: 1) Ag-dominant mesothermal Eocene veins that occurred at temperatures > 300ºC developed at ca. 3 km depth, associated to the final stages of intrusion of the Piaxtla batholith, and 2) epithermal low sulfidation Au-dominant Oligocene veins which were developed at 250ºC, at shallower depths (