Abstract
Establishing the depths of magma accumulation is critical to understanding how magmas evolve and erupt, but developing methods to constrain these pressures is challenging. We apply the new rhyolite-MELTS phase-equilibria geobarometer—based on the equilibrium between melt, quartz, and two feldspars—to matrix glass compositions from Peach Spring Tuff (Arizona–California–Nevada, USA) high-silica rhyolite. We compare the results to those from amphibole geothermobarometry, projection of glass compositions onto the haplogranitic ternary, and glass SiO2 geobarometry. Quartz + 2 feldspar rhyolite-MELTS pressures span a relatively small range (185–230 MPa), consistent with nearly homogeneous crystal compositions, and are similar to estimates based on projection onto the haplogranitic ternary (250 ± 50 MPa) and on glass SiO2 (255–275 MPa). Amphibole geothermobarometry gives much wider pressure ranges (temperature-independent: ~65–300 MPa; temperature-dependent: ~75–295 MPa; amphibole-only: ~80–950 MPa); average Anderson and Smith (Am Mineral 80:549–559, 1995) + Blundy and Holland (Contrib Miner Petrol 104:208–224, 1990) or Holland and Blundy (Contrib Miner Petrol 116:433–447, 1994—Thermometer A, B) pressures are most similar to phase-equilibria results (~220, 210, 190 MPa, respectively). Crystallization temperatures determined previously with rhyolite-MELTS (742 °C), Zr-in-sphene (769 ± 20 °C), and zircon saturation (770–780 °C) geothermometry are similar, but temperatures from amphibole geothermometry (~450–955 °C) are notably different; the average Anderson and Smith + Holland and Blundy (1994—Thermometer B; ~710 °C) temperature is most consistent with previous estimates. The rhyolite-MELTS geobarometer effectively culls glass compositions affected by alteration or analytical issues; Peach Spring glass compositions that yield pressure estimates reveal a tight range of plausible Na2O and K2O contents, suggesting that low Na2O and high K2O contents of many Peach Spring samples are due to alteration. Use of altered whole-pumice compositions in rhyolite-MELTS simulations is likely the cause of the incorrect crystallization sequence reported previously for Peach Spring compositions. Using the rhyolite-MELTS geobarometer, we estimate a more realistic composition for Peach Spring Tuff high-silica rhyolite, and the calculated composition finds close matches with some analyzed rocks and results in the expected sequence of crystallization.
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Acknowledgments
Support for this work was provided by NSF grants (EAR-0948528, EAR-1151337, EAR-1321806) and a Vanderbilt University Discovery Grant to Gualda, NSF grants (EAR-0948734, EAR-132942) to Ghiorso, an NSF grant (EAR-0911726) to Miller and Gualda, and a Vanderbilt University Summer Research Program (VUSRP) grant to McCracken.
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Communicated by Gordon Moore.
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Table S 1 Peach Spring high-silica rhyolite glass composition, method of analysis, and highest saturation level achieved with rhyolite-MELTS geobarometry. (XLS 166 kb)
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Table S 2 Compositions of Peach Spring amphibole and feldspar crystals analyzed by EMP. Average plagioclase edge compositions were used for amphibole–plagioclase geothermometry. (XLS 217 kb)
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Table S 3 Pressure estimates from rhyolite-MELTS geobarometry upon application of each of the five phase saturation conditions. (PDF 166 kb)
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Figure S 1 Plots of pressure-, temperature-, and plagioclase-dependent cation substitutions (recalculated using the method of Holland and Blundy (1994); see Figure 1 in main text for plots using amphibole formulas recalculated using the 13eCNK method of Robinson et al. (1982) in amphiboles from Peach Spring high-silica rhyolites. (PDF 237 kb)
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Figure S 2 Backscattered electron images, elemental maps, and cathodoluminescence images of Peach Spring amphibole, feldspar, and quartz crystals. (PDF 3016 kb)
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Pamukcu, A.S., Gualda, G.A.R., Ghiorso, M.S. et al. Phase-equilibrium geobarometers for silicic rocks based on rhyolite-MELTS—Part 3: Application to the Peach Spring Tuff (Arizona–California–Nevada, USA). Contrib Mineral Petrol 169, 33 (2015). https://doi.org/10.1007/s00410-015-1122-y
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DOI: https://doi.org/10.1007/s00410-015-1122-y