1Molly C. McCanta,2,3M. Darby Dyar,4,5Stephen R. Sutton,6Sarah E. Roberts,7,8Cai R. Ytsma
American Mineralogist 110, 1597-1613 Link to Article [https://doi.org/10.2138/am-2024-9602]
1Department of Earth, Environment, and Planetary Sciences, University of Tennessee, 1621 Cumberland Avenue, Knoxville, Tennessee 37996, U.S.A.
2Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, Arizona 85719, U.S.A.
3Department of Astronomy, Mount Holyoke College, 50 College Street, South Hadley, Massachusetts 01075, U.S.A.
4Center for Advanced Radiation Sources, University of Chicago, Chicago, Illinois 60637, U.S.A.
5Department of the Geophysical Sciences, University of Chicago, Chicago, Illinois 60637, U.S.A.
6Corning Glass, Corning, New York 14830, U.S.A.
7Cai Consulting, Glasgow, Scotland, U.K.
8Institute of Health Informatics, University College London, Gower Street, London WC1E 6BT, U.K.
Copyright: The Mineralogical Society of America
Iron redox works well for constraining oxygen fugacity () in terrestrial igneous materials due to the relatively high of the Earth’s atmosphere, crust, and upper mantle , where there are large changes in Fe2+/Fe3+ with relatively small changes in . At values <QFM, Fe redox becomes less sensitive, and analytical uncertainties may make it difficult to determine differences between samples. The valence change between Cr2+ and Cr3+ occurs at lower values than for iron, potentially making it a more sensitive oxybarometer for materials equilibrated under reducing conditions. The current approach to measuring from X-ray absorption (XAS) measurements derives Cr valence first from the 1s → 4s transition and then uses that redox couple to estimate as a function of temperature and composition. Here, that method is compared to an alternate approach of predicting directly from the spectra of experimentally homogenized glasses of geological relevance without an intermediate step of attempting to discern Cr2+/Cr3+. In this study, partial least-squares (PLS) multivariate (MVA) regression models were trained on the whole XAS energy spectral range, and accuracy was quantified using root mean square error (RMSE). MVA results showed significantly higher accuracy (RMSE-C of ±0.75 log units) for predicting ΔIW relative to known experimental conditions relative to the two-step method, which yielded RMSE-C of ±2.75 to ±7.65 log units for our data set vs. those of Berry and O’Neill (2004) and Berry et al. (2006), respectively. The MVA results calibrate a new Cr oxybarometer for use in low- glasses with a cross-validated (RMSE-CV) accuracy of ±0.84 log units relative to a standard oxygen buffer. Finally, the new Cr oxybarometer was applied to lunar glasses, both volcanic and impact metamorphosed, to assess the range in oxidation conditions the materials experienced during formation. Lunar volcanic glasses cluster ∼IW±1, close to that of previous studies while agglutinates and lunar impact melts record a wide range of values using Cr oxybarometry.