Abstract
Bending of oceanic plates at subduction zones results in extension and widespread normal faulting1 in the upper, brittle part of the slab2,3. Detailed seismic surveys at trenches reveal that this part of the oceanic plate could be pervasively hydrated for several kilometres below the crust–mantle boundary4,5,6,7. Similarly, heat-flow surveys indicate active fluid circulation within the slab8. Yet, the mechanisms that enable fluids to percolate to such depths in spite of their natural buoyancy remain unclear. Here we use two-dimensional numerical experiments to show that stress changes induced by the bending oceanic plate produce subhydrostatic or even negative pressure gradients along normal faults, favouring downward pumping of fluids. The fluids then react with the crust and mantle surrounding the faults and are stored in the form of hydrous minerals. We suggest that this process is the dominant mechanism of deep slab hydration, although it may be locally aided by the enhancement in porosity due to prefailure dilatancy9, pre-existing cracks10 and migrating fluid-filled cracks11. Our results have implications for the transport of water into the deeper parts of the mantle12, and for further clarifying the seismic anisotropy of slabs13.
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Acknowledgements
This work was supported by SNF Research Grants 200021-113672/1, 200021-113672/1 and 200021-116381/1, ETH Research Grants TH-12/05-3 and TH-0807-3 and ETH account 0-12422-97. M.F. thanks N. Mancktelow for discussion about tectonic pressure effects on fluid flow in subducting slabs. M. Spiegelman contributed to clarify the basic concepts of this work. D. May improved the English of the manuscript.
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M.F. designed the study, carried out and analysed the numerical experiments and wrote the paper. T.V.G. developed the numerical code and analysed the numerical experiments. L.B. contributed to the concept development. All authors discussed the results and commented on the paper.
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Faccenda, M., Gerya, T. & Burlini, L. Deep slab hydration induced by bending-related variations in tectonic pressure. Nature Geosci 2, 790–793 (2009). https://doi.org/10.1038/ngeo656
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DOI: https://doi.org/10.1038/ngeo656
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