Using synchrotron radiation to determine the oxidation state of uranium in magmas
File(s)
Author(s)
Halse, Helen
Type
Thesis
Abstract
Young igneous rocks from a range of tectonic settings exhibit various Uranium-series (Useries) disequilibria. The U-series systematics of Mid-ocean-ridge basalts (MORBs) have been attributed to mantle melting, while those of arc basalts are widely thought to be slab fluid signatures. Mid-ocean-ridge and arc U-series models generally assume that U4+ is the
only oxidation state relevant to mantle melting processes, however the potential for the stabilisation of U5+ and/or U6+ has recently been proposed for some arc lavas.
To determine the oxidation state of U in geological melts, and to assess the relative stabilities of U4+, U5+, and U6+ under mantle conditions, X-ray absorption near edge structure (XANES) spectra were recorded from synthetic analogues, including an Fe-bearing MORB composition. Spectra were collected from quenched glasses equilibrated at 1400 °C and oxygen fugacities (fO2s) between logfO2 = -18 and +4.7 (QFM-11.7 to QFM+11), and from equivalent high temperature melts using a custom designed XAS furnace. Spectra were collected at both the U L3- and M4-edges, as the variation of the M4-edge spectral line-shape could be unambiguously linked to oxidation state changes in the glasses, while the higher energy of the L3-edge was better suited to in situ studies.
The variation of the XANES spectra as a function of fO2 allowed U5+ to be identified as a major component in both the MORB glasses and their original melts, and a methodology was developed to accurately quantify their U oxidation state proportions. The proportion of U4+ was found to be highly sensitive to fO2 at conditions relevant to mantle melting, with U5+/ΣU varying between ~0.1 and 0.5 between QFM-1 and QFM+2 and pressures equivalent to mantle depths of ≥ 15 km. U-series models assuming melting of a variably oxidised mantle wedge can produce a wide range of U-series signatures that are consistent with many arc basalts. In contrast, the stability of even small proportions of U5+ in the melt may present a problem for those models currently attributing the 230Th excesses of MORBs to mantle
melting in the spinel lherzolite field.
only oxidation state relevant to mantle melting processes, however the potential for the stabilisation of U5+ and/or U6+ has recently been proposed for some arc lavas.
To determine the oxidation state of U in geological melts, and to assess the relative stabilities of U4+, U5+, and U6+ under mantle conditions, X-ray absorption near edge structure (XANES) spectra were recorded from synthetic analogues, including an Fe-bearing MORB composition. Spectra were collected from quenched glasses equilibrated at 1400 °C and oxygen fugacities (fO2s) between logfO2 = -18 and +4.7 (QFM-11.7 to QFM+11), and from equivalent high temperature melts using a custom designed XAS furnace. Spectra were collected at both the U L3- and M4-edges, as the variation of the M4-edge spectral line-shape could be unambiguously linked to oxidation state changes in the glasses, while the higher energy of the L3-edge was better suited to in situ studies.
The variation of the XANES spectra as a function of fO2 allowed U5+ to be identified as a major component in both the MORB glasses and their original melts, and a methodology was developed to accurately quantify their U oxidation state proportions. The proportion of U4+ was found to be highly sensitive to fO2 at conditions relevant to mantle melting, with U5+/ΣU varying between ~0.1 and 0.5 between QFM-1 and QFM+2 and pressures equivalent to mantle depths of ≥ 15 km. U-series models assuming melting of a variably oxidised mantle wedge can produce a wide range of U-series signatures that are consistent with many arc basalts. In contrast, the stability of even small proportions of U5+ in the melt may present a problem for those models currently attributing the 230Th excesses of MORBs to mantle
melting in the spinel lherzolite field.
Version
Open Access
Date Issued
2014-06
Date Awarded
2014-12
Copyright Statement
Attribution NoDerivatives 4.0 International Licence (CC BY-ND)
Advisor
Berry, Andrew
Sponsor
Imperial College London
Natural History Museum (London, England)
Diamond Light Source (Firm)
Publisher Department
Earth Science and Engineering
Publisher Institution
Imperial College London
Qualification Level
Doctoral
Qualification Name
Doctor of Philosophy (PhD)