A two-stage fluid history for the Orocopia Schist and associated rocks related to flat subduction and exhumation,southeastern California |
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| Authors: | Gregory J Holk Marty Grove Carl E Jacobson Gordon B Haxel |
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| Institution: | 1. Department of Geological Sciences and the Institute for Integrated Research in Materials, Environments, and Societies, California State University, Long Beach, CA, USAgholk@csulb.edu;3. Department of Geological Sciences, Green Earth Sciences, Stanford University, Stanford, CA, USA;4. Department of Geological and Atmospheric Sciences, Iowa State University, Ames, IA, USA;5. Department of Earth and Space Sciences, West Chester University of Pennsylvania, West Chester, PA, USA;6. Geology Program, School of Earth Sciences and Environmental Sustainability, Northern Arizona University, Flagstaff, AZ, USA |
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| Abstract: | ABSTRACTStable isotopes combined with pre-existing 40Ar/39Ar thermochronology at the Gavilan Hills and Orocopia Mountains in southeastern California record two stages of fluid–rock interaction: (1) Stage 1 is related to prograde metamorphism as Orocopia Schist was accreted to the base of the crust during late Cretaceous–early Cenozoic Laramide flat subduction. (2) Stage 2 affected the Orocopia Schist and is related to middle Cenozoic exhumation along detachment faults. There is no local evidence that schist-derived fluids infiltrated structurally overlying continental rocks. Mineral δ18O values from Orocopia Schist in the lower plate of the Chocolate Mountains fault and Gatuna normal fault in the Gavilan Hills are in equilibrium at 490–580°C with metamorphic water (δ18O = 7–11‰). Phengite and biotite δD values from the Orocopia Schist and upper plate suggest metamorphic fluids (δD ~ –40‰). In contrast, final exhumation of the schist along the Orocopia Mountains detachment fault (OMDF) in the Orocopia Mountains was associated with alteration of prograde biotite and amphibole to chlorite (T ~ 350–400°C) and the influx of meteoric-hydrothermal fluids at 24–20 Ma. Phengites from a thin mylonite zone at the top of the Orocopia Schist and alteration chlorites have the lowest fluid δD values, suggesting that these faults were an enhanced zone of meteoric fluid (δD < –70‰) circulation. Variable δD values in Orocopia Schist from structurally lower chlorite and biotite zones indicate a lesser degree of interaction with meteoric-hydrothermal fluids. High fluid δ18O values (6–12‰) indicate low water–rock ratios for the OMDF. A steep thermal gradient developed across the OMDF at the onset of middle Cenozoic slip likely drove a more vigorous hydrothermal system within the Orocopia Mountains relative to the equivalent age Gatuna fault in the Gavilan Hills. |
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| Keywords: | stable isotopes flat subduction exhumation meteoric-hydrothermal fluids |
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