T80 Investigations of Hydrothermal Systems: Advances and Challenges
Monday, 23 September 2019
8:00 AM - 12:00 PM
Room 222BC, North Building
FLUID EVOLUTION IN THE GEYSERS GEOTHERMAL SYSTEM, CALIFORNIA: EVIDENCE FROM FLUID INCLUSION AND SECONDARY ION MASS SPECTROMETRY (SIMS) OXYGEN ISOTOPE ANALYSES OF VEIN QUARTZ
Paper number: T80-14
Program: Technical Sessions
Time: 11:15 AM – 11:30 AM
Authors
-
John R. BowmanUniversity of Utah, Salt Lake City, UT
-
Joseph N. MooreUniversity of Utah, Salt Lake, UT
-
John ValleyUniversity of Wisconsin-Madison, Madison, WI
-
Kouki KitajimaUniversity of Wisconsin-Madison, Madison, WI
-
Mark WaltersMiddletown, CA
Abstract
Vein quartz contains two-phase vapor-rich inclusions and liquid-rich inclusions containing up to 13 solid phases at room temperature. Calculated salinities range from 0 to ~47 weight percent NaCl equivalent based on ice-melting or halite dissolution temperatures. Total homogenization temperatures range from 220 to 385oC. In general, both temperature and salinity decrease with time through successively later generations of vein quartz. The paleo liquid-dominated reservoir was highly stratified with regards to salinity with hypersaline fluid inclusions occurring only at depth, within the pluton and surrounding hornfels. Coeval hypersaline fluid inclusions and vapor-rich fluid inclusions in vein quartz intergrown with high-temperature minerals (biotite, amphibole, tourmaline) suggest that fluid immiscibility occurred early in the evolution of the system and continued as the system evolved.
Vein quartz δ18O ranges from +21.4‰ to +4.3‰. Individual core samples exhibit variations of up to 16.9‰, and up to 8.9‰ in single crystals. Overall, maximum δ18O of vein quartz decreases as the pluton is approached. Within the system as a whole, and within individual crystals, quartz δ18O values decrease with time.
The spatial correlation of fluid inclusion and SIMS data allows calculation of the δ18O values of the water from which the vein quartz precipitated. Calculated δ18O values for the early deep hypersaline waters are as high as +10‰, consistent with either formation waters or extensively boiled magmatic fluids. Paragenetically later, lower temperature and less saline fluids have δ18O(H2O) values as low as -1‰. The decrease in δ18O of the fluid, coupled with decreases in homogenization temperatures and salinities of the inclusions over time, is interpreted as the result of the progressive incursion of meteoric water into the paleo liquid-dominated reservoir.
Geological Society of America Abstracts with Programs. Vol. 51, No. 5
doi: 10.1130/abs/2019AM-337561
© Copyright 2019 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.