he stability of V0 implies oxygen fugacities ≥9 log units below the Iron-Wustite buffer, suggesting a hydrogendominated atmosphere. This is supported by wt%-levels of hydrogen in gasses released by crushing, by Raman spectroscopy, and by the presence of VH2 among the vanadium balls. The oxide assemblage formed at 1400–1200 °C; the solution of hydrogen in the metal could lower the melting point of vanadium to these temperatures. These assemblages probably resulted from reaction between differentiated mafic melts and mantle-derived CH4+H2 fluids near the crust-mantle boundary, and they record the most reducing magmatic conditions yet documented on Earth.
Extreme reduction: Mantle-derived oxide xenoliths from a hydrogen-rich environment / W.L. Griffin, S.E.M. Gain, F. Cámara, L. Bindi, J. Shaw, O. Alard, M. Saunders, J.-X. Huang, V. Toledo, S.Y. O'Reilly. - In: LITHOS. - ISSN 0024-4937. - STAMPA. - 358-359:(2020), pp. 1-8.
Extreme reduction: Mantle-derived oxide xenoliths from a hydrogen-rich environment
L. BindiMembro del Collaboration Group
;
2020
Abstract
he stability of V0 implies oxygen fugacities ≥9 log units below the Iron-Wustite buffer, suggesting a hydrogendominated atmosphere. This is supported by wt%-levels of hydrogen in gasses released by crushing, by Raman spectroscopy, and by the presence of VH2 among the vanadium balls. The oxide assemblage formed at 1400–1200 °C; the solution of hydrogen in the metal could lower the melting point of vanadium to these temperatures. These assemblages probably resulted from reaction between differentiated mafic melts and mantle-derived CH4+H2 fluids near the crust-mantle boundary, and they record the most reducing magmatic conditions yet documented on Earth.| File | Dimensione | Formato | |
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