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

ABSTRACT: 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.

SUBMITTER: Nishizawa T

PROVIDER: S-EPMC5599635 | biostudies-literature | 2017 Sep

REPOSITORIES: biostudies-literature

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

Nishizawa Tatsuji T Nakamura Hitomi H Churikova Tatiana T Gordeychik Boris B Ishizuka Osamu O Haraguchi Satoru S Miyazaki Takashi T Vaglarov Bogdan Stefanov BS Chang Qing Q Hamada Morihisa M Kimura Jun-Ichi JI Ueki Kenta K Toyama Chiaki C Nakao Atsushi A Iwamori Hikaru H

Scientific reports 20170914 1

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, mon ...[more]

PMID: 28912418

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Project description:We report the results of experiments designed to separate the effects of temperature and pressure from liquid composition on the partitioning of Ni between olivine and liquid, [Formula: see text]. Experiments were performed from 1300 to 1600 °C and 1 atm to 3.0 GPa, using mid-ocean ridge basalt (MORB) glass surrounded by powdered olivine in graphite-Pt double capsules at high pressure and powdered MORB in crucibles fabricated from single crystals of San Carlos olivine at one atmosphere. In these experiments, pressure and temperature were varied in such a way that we produced a series of liquids, each with an approximately constant composition (~12, ~15, and ~21 wt% MgO). Previously, we used a similar approach to show that [Formula: see text] for a liquid with ~18 wt% MgO is a strong function of temperature. Combining the new data presented here with our previous results allows us to separate the effects of temperature from composition. We fit our data based on a Ni-Mg exchange reaction, which yields [Formula: see text] Each subset of constant composition experiments displays roughly the same temperature dependence of [Formula: see text] (i.e.,[Formula: see text]) as previously reported for liquids with ~18 wt% MgO. Fitting new data presented here (15 experiments) in conjunction with our 13 previously published experiments (those with ~18 wt% MgO in the silicate liquid) to the above expression gives [Formula: see text] = 3641 ± 396 (K) and [Formula: see text] = - 1.597 ± 0.229. Adding data from the literature yields [Formula: see text] = 4505 ± 196 (K) and [Formula: see text] = - 2.075 ± 0.120, a set of coefficients that leads to a predictive equation for [Formula: see text] applicable to a wide range of melt compositions. We use the results of our work to model the melting of peridotite beneath lithosphere of varying thickness and show that: (1) a positive correlation between NiO in magnesian olivine phenocrysts and lithospheric thickness is expected given a temperature-dependent [Formula: see text] and (2) the magnitude of the slope for natural samples is consistent with our experimentally determined temperature dependence. Alternative processes to generate the positive correlation between NiO in magnesian olivines and lithospheric thickness, such as the melting of olivine-free pyroxenite, are possible, but they are not required to explain the observed correlation of NiO concentration in initially crystallizing olivine with lithospheric thickness.

Dataset Information

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

Publications

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

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