Abstract
Volatiles can be transferred from slabs to wedge asthenosphere either by silicate melts of by hydrous fluids. Experiments defining the nature of these agents, and expected ratios of transported elements, are not well-constrained, especially for fluids. Phase equilibria of basaltic slab material and probable geotherms suggest that slabs devolatilize or melt, or both, at depths shallower than the average 136 km beneath arc fronts. Volatiles probably are transported into immediately overlying asthenosphere and then carried by flow beneath arcs. Simple addition of probable fluid to MORB or OIB-type asthenosphere cannot explain observed H2O and K2O to asthenosphere and more complicated histories of melt generation; the melts generated at 100–140 km beneath arcs bear little chemical relation to arc basalts. Volatiles thus must pass numerous “filters” before they emerge in arc volcanics.
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Eggler, D.H. (1989). Influence of H2O And CO2 on Melt and Fluid Chemistry in Subduction Zones. In: Hart, S.R., Gülen, L. (eds) Crust/Mantle Recycling at Convergence Zones. NATO ASI Series, vol 258. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0895-6_11
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DOI: https://doi.org/10.1007/978-94-009-0895-6_11
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