Journal article
Subduction zone fluxes of halogens and noble gases in seafloor and forearc serpentinites
MA Kendrick, M Honda, T Pettke, M Scambelluri, D Phillips, A Giuliani
Earth and Planetary Science Letters | ELSEVIER | Published : 2013
Abstract
Serpentinites form by hydration of ultramafic lithologies in a range of seafloor and shallow subduction zone settings. Serpentinites are recognised as major reservoirs of fluid mobile elements and H2O in subducting oceanic lithosphere, and together with forearc serpentinites formed in the mantle wedge, provide critical information about shallow-level volatile fluxes during subduction. The current study provides new Cl, as well as the first comprehensive Br, I and noble gas analyses reported for seafloor and forearc chrysotile-lizardite serpentinites. The samples were recovered from IODP drilling campaigns of mid-ocean ridge, passive margin and forearc settings (n=17), and ophiolites in the I..
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Awarded by Australian Research Council
Funding Acknowledgements
Stanislav Szczepanski is thanked for technical assistance in the University of Melbourne noble gas laboratory. Dr Mark Kendrick is the recipient of an Australian Research Council QEII Fellowship (Project no. DP 0879451). This research used samples provided by the Deep Sea Drilling Project and Ocean Drilling Program, which are funded by agencies of the participating countries under management of Joint Oceanographic Institutions (JOI), Inc. Drs Jaime Barnes and Hirochika Sumino are gratefully acknowledged for their insightful reviews that improved the focus of this manuscript.