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Apatite: A new redox proxy for silicic magmas?

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journal contribution
posted on 2019-02-18, 12:04 authored by AJ Miles, CM Graham, CJ Hawkesworth, MR Gillespie, RW Hinton, GD Bromiley
The oxidation states of magmas provide valuable information about the release and speciation of volatile elements during volcanic eruptions, metallogenesis, source rock compositions, open system magmatic processes, tectonic settings and potentially titanium (Ti) activity in chemical systems used for Ti-dependent geothermometers and geobarometers. In this paper we explore the use of Mn in apatite as an oxybarometer in intermediate and silicic igneous rocks. Increased Mn concentrations in apatite in granitic rocks from the zoned Criffell granitic pluton (southern Scotland) correlate with decreasing Fe2O3 (Fe3+ 24 ) and Mn in the whole-rock and likely reflect increased Mn2+/Mn3+ and greater compatibility of Mn2+ 25 relative to Mn3+ in apatite under reduced conditions. Fe3+/Fe2+ 26 ratios in biotites have previously been used to calculate oxygen fugacities (fO2) in the outer zone granodiorites and inner zone granites where redox conditions have been shown to change from close to the magnetite hematite buffer to close to the nickel-nickel oxide buffer respectively (Stephens et al., 1985). This trend is apparent in apatite Mn concentrations from a range of intermediate to silicic volcanic rocks that exhibit varying redox states and are shown to vary linearly and negatively with log fO2, such that log fO2 = -0.0022(±0.0003) Mn (ppm) – 9.75(±0.46) Variations in the Mn concentration of apatites appear to be largely independent of differences in the Mn concentration of the melt. Apatite Mn concentrations may therefore provide an independent oxybarometer that is amenable to experimental calibration, with major relevance to studies on detrital mineral suites, particularly those containing a record of early Earth redox conditions, and on the climatic impact of historic volcanic eruptions.

Funding

AM is grateful to NERC for a CASE studentship and acknowledges the support of the British Geological Survey for a BUFI grant to meet the costs of analytical work. NERC is also thanked for use of the Edinburgh Ion Microprobe Facility.

History

Citation

Geochimica et Cosmochimica Acta, 2014, 132, pp. 101-119

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Geology

Version

  • AM (Accepted Manuscript)

Published in

Geochimica et Cosmochimica Acta

Publisher

Elsevier, Meteoritical Society, Geochemical Society

issn

0016-7037

Acceptance date

2014-01-29

Copyright date

2014

Available date

2019-02-18

Publisher version

https://www.sciencedirect.com/science/article/pii/S0016703714000842?via=ihub

Notes

Supplementary data associated with this article can be found, in the online version, at http://dx.doi.org/10.1016/j.gca.2014.01.040.

Language

en

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