HIGH-TEMPERATURE HYDROTHERMAL ACTIVITY BENEATH THE CERRO ESCORIAL VOLCANO, NW ARGENTINA, AS SAMPLED BY AN EXPLOSIVE VOLCANIC ERUPTION
A small (<=0.6 km3) dacitic ignimbrite was erupted from the Cerro Escorial vent at 0.46 +/- 0.01 Ma, followed by extrusion of a viscous andesitic flow at 0.34 +/- 0.03 Ma. Along with pumice blocks, the poorly-welded ignimbrite contains a variety of lithic clasts, including basement granite, supracrustal sedimentary rocks, and fragments of the volcanic edifice. In addition, pebble-sized clasts of quartz were found in the deposit. Some of the clasts consist of poly-crystalline aggregates, but most are single crystals with a form suggestive of hydrothermal vein growth. Primary and pseudosecondary fluid inclusions contained within these clasts are of three types: (1) dark, vapor-rich inclusions; (2) highly concentrated aqueous brines with a high proportion of daughter minerals; (3) internally decrepitated inclusions. Preliminary microthermometric investigations of the brine inclusions show only partial dissolution of daughter minerals by 600 degrees C, suggesting entrapment under two-phase (liquid plus vapor) magmatic-hydrothermal conditions. The internally decrepitated inclusions provide evidence for rapid depressurization, likely during eruption from depth. The quartz clasts and fluid inclusions thus appear to represent quenched samples of a deep-seated magmatic-hydrothermal system, perhaps analogous to fossil hydrothermal systems exposed in porphyry-type ore deposits. Unlike fossil systems, however, these samples are pristine and have not been overprinted by later, lower-temperature hydrothermal events. Further detailed study should elucidate early high-temperature magmatic-hydrothermal processes in such systems.