157 Geochemistry (Posters)
Tuesday, 6 November 2012
9:00 AM - 6:00 PM
Hall B
MICROTHERMOMETRY OF FLUID INCLUSIONS IN THE EMPIRE MOUNTAINS SKARNS, SIERRA NEVADA, CA: IMPLICATIONS FOR FLUID δ18O VALUES AND ORE FORMATION
Paper number: 157-7
Program: Technical Sessions
Time: 9:00 AM – 6:00 PM
Authors
-
Jade Star LackeyPomona College, Claremont, CA
-
Megan D'ErricoStanford University, Stanford, CA
-
Jaime BarnesThe University of Texas at Austin, Austin, TX
Abstract
Primary fluid inclusions in the Empire Mountain skarns and associated alteration zones are used to examine the thermal history of the hydrothermal system and to evaluate the isotopic composition of skarn-forming fluids. Microthermometry of primary fluid inclusion assemblages within late stage, grossular garnets yield homogenization temperatures of 310–325 °C; early andradite garnets lack discernible primary fluid inclusion assemblages. Primary inclusions in euhdral quartz, including samples from the Empire Mine homogenize at 215–255°C. Using δ18O values of garnet and quartz, and homogenization temperatures as minimums, calculated δ18O values of water in equilibrium with minerals are as follows: red garnet ~ 0.5–1.0‰, beige garnet ~4.3‰, and quartz = –1.7 to –6.5‰. Initial waters had low δ18O values that increased during growth of beige garnet, which suggests greater proportion of magmatic or metamorphic water input. Early meteoric water infiltration into the hydrothermal system was facilitated by the extensive brecciation caused by a shallow, hot intruding magma. Late stage alteration and ore formation was accompanied by the resumption of an increased proportion of meteoric water infiltration.