The oxidation state of chromium in basaltic silicate melts
| dc.contributor.author | O'Neill, Hugh | |
| dc.contributor.author | Berry, Andrew | |
| dc.date.accessioned | 2022-11-02T23:32:02Z | |
| dc.date.issued | 2021 | |
| dc.date.updated | 2021-11-28T07:26:18Z | |
| dc.description.abstract | Cr3+/Cr2+ in melts in the systems CaO-MgO-Al2O3-SiO2 ± Na2O ± K2O doped with Cr added as 0.5 wt% Cr2O3 were determined as a function of oxygen fugacity (fO2) at 1400 °C by XANES spectroscopy of their quenched glasses, using the intensity of the shoulder on the Cr K-edge due to the 1 s → 4 s transition. The addition of Na and K to the system CMAS increases Cr3+/Cr2+ at constant temperature and fO2, in good agreement with the predictions from the “ideal optical basicity”. The new results have been combined with previous results to calibrate a model for Cr3+/Cr2+ in silicate melts as a function of temperature, pressure and melt composition: log10(Cr3+/Cr2+) = 1/4 ΔQFM + 3031/T − 2.26 + (843P – 158 P2)/T + ∑cZXZ. where XZ are the mole fractions of the oxide components Z defined on the single-cation basis and ∑cZXZ = 2.00 XNaO0.5 + 1.00 (XMgO + XFe2+O) + 0.37 (XAlO1.5 + XFe3+O1.5) + 2.12 XKO0.5 + 2.44 XCaO + 3.69 XTiO2, T is temperature in K, P is pressure in GPa, and ΔQFM is the difference between the fO2 of the silicate melt and the Quartz-Fayalite-Magnetite buffer at 105 Pa, given by log10fO2(QFM) = 8.58–25050/T, relative to the conventional standard state of pure O2 at 105 Pa. The effect of pressure is markedly non-linear, so the model should not be extrapolated above 4 GPa. Combining this model with the similar one for Fe3+/Fe2+ in silicate melts gives: log10(Cr3+/Cr2+) = log10(Fe3+/Fe2+) + 3031/T − 0.9 + (1317P – 219 P2)/T + ∑jZXZ. where ∑jZXZ = 1.00 (XMgO + XFe2+O) + 0.37 (XAlO1.5 + XFe3+O1.5) −1.59 XKO0.5 + 0.04 XCaO + 3.69 XTiO2. High Cr2+/∑Cr in silicate melts is promoted by high temperature and low pressure, as well as low Fe3+/∑Fe. For a parental MORB melt composition at 1250 °C (1523 K), 105 Pa, with Fe3+/∑Fe = 0.10, the model predicts Cr2+/ΣCr = 0.27. The effect of pressure is very large: the Cr2+/ΣCr in the above example would drop to 0.03 at 2 GPa and 1250 °C. The Cr2+ present in Fe3+-containing melts at magmatic temperatures decreases on cooling because of the electron exchange reaction: Cr2+ + Fe3+ = Cr3+ + Fe2+. | en_AU |
| dc.description.sponsorship | Part of this work was performed at the Australian National Beamline Facility with support from the Australian Synchrotron Research Program, which was funded by the Commonwealth of Australia under the Major National Research Facilities Program. | en_AU |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 0016-7037 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/277971 | |
| dc.language.iso | en_AU | en_AU |
| dc.publisher | Pergamon Press Ltd. | en_AU |
| dc.rights | © 2021 The authors | en_AU |
| dc.source | Geochimica et Cosmochimica Acta | en_AU |
| dc.title | The oxidation state of chromium in basaltic silicate melts | en_AU |
| dc.type | Journal article | en_AU |
| local.bibliographicCitation.lastpage | 320 | en_AU |
| local.bibliographicCitation.startpage | 304 | en_AU |
| local.contributor.affiliation | O'Neill, Hugh, College of Science, ANU | en_AU |
| local.contributor.affiliation | Berry, Andrew, College of Science, ANU | en_AU |
| local.contributor.authoruid | O'Neill, Hugh, u8101317 | en_AU |
| local.contributor.authoruid | Berry, Andrew, u9715689 | en_AU |
| local.description.embargo | 2099-12-31 | |
| local.description.notes | Imported from ARIES | en_AU |
| local.identifier.absfor | 370302 - Inorganic geochemistry | en_AU |
| local.identifier.absfor | 370503 - Igneous and metamorphic petrology | en_AU |
| local.identifier.absseo | 280107 - Expanding knowledge in the earth sciences | en_AU |
| local.identifier.ariespublication | a383154xPUB19866 | en_AU |
| local.identifier.citationvolume | 306 | en_AU |
| local.identifier.doi | 10.1016/j.gca.2021.03.024 | en_AU |
| local.identifier.scopusID | 2-s2.0-85107701350 | |
| local.publisher.url | https://www.sciencedirect.com/ | en_AU |
| local.type.status | Published Version | en_AU |
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