189 D28. Petrology, Igneous (Posters)

Tuesday, 6 November 2018
9:00 AM - 6:30 PM
Halls J-K

DETERMINATION OF FERRIC-FERROUS RATIO IN PYROXENES WITH X-RAY ABSORPTION SPECTROSCOPY

Paper number: 189-13
Program: Technical Sessions
Time: 9:00 AM – 6:30 PM

Authors

Abstract

Iron is the most abundant multivalent element in the Earth’s crust, and is commonly used as an indicator of oxygen fugacity in geologic systems. Oxygen fugacity is a principle component of phase equilibria of a chemical system, and the redox state of sample can be used to ascribe provenance and interpret the petrogenesis of a rock. Despite its importance, few methods are sensitive to Fe valence state, and the predominant method, Mossbauer spectroscopy, requires a bulk sample for analysis. Because of the limitations of Mossbauer spectroscopy, calibrations using X-ray absorption spectroscopy (XAS) continue to develop, because its 1×1 mm spot size permits analyses on the same scales as other probes. Multivariate models that utilize full spectral ranges of XAS have proven to accurately predict redox ratios in spite of the polarization of the synchrotron beam, even in anisotropic minerals. Though these models have been established for garnets, amphiboles, and glasses, several other geologically significant mineral groups remain to be calibrated. In particular, pyroxenes are widely used in thermobarometry and occur in a wide variety of terrestrial and extraterrestrial environments. Further, pyroxenes can be chemically zoned or exsolved, so their redox ratios provide insights into the behavior of iron partitioning under the crystallization or recrystallization conditions of the pyroxene. Fe-XAS data collected from a set of 70 pyroxenes in this study and predicted using multivariate analysis show a strong correlation with true ferric-ferrous ratio from Mossbauer spectroscopy. The resultant prediction model is far more accurate than that determined from the pre-edge region alone.

Geological Society of America Abstracts with Programs. Vol. 50, No. 6

doi: 10.1130/abs/2018AM-319797

© Copyright 2018 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.