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http://www.sciencedirect.com/science/article/pii/S1674987114000590
Authors:Maria-Luce Frezzotti    Jacques L.R.Touret
Affiliation:1. Department of Earth and Environmental Sciences, University Milano Bicocca, P.za Della Scienza 4, 20126 Milano, Italy
2. Mineralogy, Université Pierre et Marie Curie, 4 Place Jussieu, 75272 Paris Cedex O5, France
Abstract:This paper reviews the origin and evolution of fluid inclusions in ultramafic xenoliths, providing a framework for interpreting the chemistry of mantle fluids in the different geodynamic settings. Fluid inclusion data show that in the shallow mantle, at depths below about 100 km, the dominant fluid phase is CO2 ± brines, changing to alkali-, carbonate-rich (silicate) melts at higher pressures. Major solutes in aqueous fluids are chlorides, silica and alkalis (saline brines; 5–50 wt.% NaCl eq.). Fluid inclusions in peridotites record CO2 fluxing from reacting metasomatic carbonate-rich melts at high pressures, and suggest significant upper-mantle carbon outgassing over time. Mantle-derived CO2 (±brines) may eventually reach upper-crustal levels, including the atmosphere, independently from, and additionally to magma degassing in active volcanoes.
Keywords:Fluid inclusion  Peridotite  Mantle metasomatism  Carbonate-rich melt  CO2  Saline brine
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