Genesis of ultra-high-Ni olivine in high-Mg andesite lava triggered by seamount subduction

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作者
Tatsuji Nishizawa
Hitomi Nakamura
Tatiana Churikova
Boris Gordeychik
Osamu Ishizuka
Satoru Haraguchi
Takashi Miyazaki
Bogdan Stefanov Vaglarov
Qing Chang
Morihisa Hamada
Jun-Ichi Kimura
Kenta Ueki
Chiaki Toyama
Atsushi Nakao
Hikaru Iwamori
机构
[1] Tokyo Institute of Technology,Department of Earth and Planetary Sciences
[2] Japan Agency for Marine-Earth Science and Technology,Department of Solid Earth Geochemistry
[3] Chiba Institute of Technology,R & D Center for Ocean Drilling Science
[4] ORCeNG,Institute of Geology and Geoinformation
[5] Institute of Volcanology and Seismology,undefined
[6] Far East Branch,undefined
[7] Russian Academy of Sciences,undefined
[8] 9 Piip Boulevard,undefined
[9] Institute of Experimental Mineralogy,undefined
[10] Russian Academy of Sciences,undefined
[11] 4 Academica Osypyana ul.,undefined
[12] Institute of Earthquake and Volcano Geology,undefined
[13] Geological Survey of Japan,undefined
[14] AIST,undefined
[15] Central 7,undefined
[16] Japan Agency for Marine-Earth Science and Technology,undefined
[17] 2-15 Natsushima-cho,undefined
[18] Earthquake Research Institute,undefined
[19] The University of Tokyo,undefined
[20] Geological Survey of Japan,undefined
[21] AIST,undefined
[22] Central 7,undefined
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摘要
The Kamchatka Peninsula is a prominent and wide volcanic arc located near the northern edge of the Pacific Plate. It has highly active volcanic chains and groups, and characteristic lavas that include adakitic rocks. In the north of the peninsula adjacent to the triple junction, some additional processes such as hot asthenospheric injection around the slab edge and seamount subduction operate, which might enhance local magmatism. In the forearc area of the northeastern part of the peninsula, monogenetic volcanic cones dated at <1 Ma were found. Despite their limited spatiotemporal occurrence, remarkable variations were observed, including primitive basalt and high-Mg andesite containing high-Ni (up to 6300 ppm) olivine. The melting and crystallization conditions of these lavas indicate a locally warm slab, facilitating dehydration beneath the forearc region, and a relatively cold overlying mantle wedge fluxed heterogeneously by slab-derived fluids. It is suggested that the collapse of a subducted seamount triggered the ascent of Si-rich fluids to vein the wedge peridotite and formed a peridotite–pyroxenite source, causing the temporal evolution of local magmatism with wide compositional range.
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