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Contributions of slab fluid and sediment melt components to magmatism in the Mariana Arc–Trough system: Evidence from geochemical compositions and Sr,Nd, and noble gas isotope systematics
Authors:Yasuo Ikeda  Keisuke Nagao  Teruaki Ishii  Daisuke Matsumoto  Robert J Stern  Hiroo Kagami  Makoto Arima  Sherman H Bloomer
Affiliation:1. Department of Earth Science, Hokkaido University of Education, Kushiro, Hokkaido, Japan;2. Geochemical Research Center, Graduate School of Science, University of Tokyo, Tokyo, Japan;3. Ocean Research Institute, University of Tokyo, Nakano, Japan;4. Geosciences Department, University of Texas at Dallas, Richardson, TX, USA;5. Graduate School of Science and Technology, Niigata University, Niigata, Japan;6. Graduate School of Environment and Information Sciences, Yokohama National University, Yokohama, Japan;7. Department of Geoscience, Oregon State University, Corvallis, OR, USA
Abstract:This study presents new major and trace element, mineral, and Sr, Nd, and noble gas isotope geochemical analyses of basalts, gabbro, and clinopyroxenite from the Mariana Arc (Central Islands and Southern Seamount provinces) including the forearc, and the Mariana Trough (Central Graben and Spreading Ridge). Mantle source compositions beneath the Mariana Arc and the Mariana Trough indicate a mantle source that is depleted in high field strength elements relative to MORB (mid‐oceanic ridge basalt). Samples from the Mariana Arc, characterized by high ratios of Ba/Th, U/Th, 84Kr/4He and 132Xe/4He, are explained by addition of fluid from the subducted slab to the mantle wedge. Correlations of noble gas data, as well as large ion lithophile elements, indicate that heavy noble gases (Ar, Kr, and Xe) provide evidence for fluid fluxing into the mantle wedge. On the other hand, major elements and Sr, Nd, He, and Ne isotopic data of basalts from the Mariana Trough are geochemically indistinguishable from MORB. Correlations of 3He/4He and 40Ar/36Ar in the Mariana Trough samples are explained by mixing between MORB and atmosphere. One sample from the Central Graben indicates extreme enrichment in 20Ne/22Ne and 21Ne/22Ne, suggesting incorporation of solar‐type Ne in the magma source. Excess 129Xe is also observed in this sample suggesting primordial noble gases in the mantle source. The Mariana Trough basalts indicate that both fluid and sediment components contributed to the basalts, with slab‐derived fluids dominating beneath the Spreading Ridge, and that sediment melts, characterized by high La/Sm and relatively low U/Th and Zr/Nb, dominate in the source region of basalts from the Central Graben.
Keywords:basalt  fluid  mantle source  Mariana Arc  Mariana Trough  noble gas isotopes  sediment  Sr–  Nd isotopes                                            Sr‐Nd同                                            
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