Primary melt from Sannome-gata volcano, NE Japan arc: constraints on generation conditions of rear-arc magmas

The conditions under which rear-arc magmas are generated were estimated using primary basalts from the Sannome-gata volcano, located in the rear of the NE Japan arc. Scoriae from the volcano occur with abundant crustal and mantle xenoliths, suggesting that the magma ascended rapidly from the upper m...

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Veröffentlicht in:Contributions to mineralogy and petrology 2014-02, Vol.167 (2), p.1, Article 969
Hauptverfasser: Kuritani, Takeshi, Yoshida, Takeyoshi, Kimura, Jun-Ichi, Takahashi, Toshiro, Hirahara, Yuka, Miyazaki, Takashi, Senda, Ryoko, Chang, Qing, Ito, Yoshinori
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container_title Contributions to mineralogy and petrology
container_volume 167
creator Kuritani, Takeshi
Yoshida, Takeyoshi
Kimura, Jun-Ichi
Takahashi, Toshiro
Hirahara, Yuka
Miyazaki, Takashi
Senda, Ryoko
Chang, Qing
Ito, Yoshinori
description The conditions under which rear-arc magmas are generated were estimated using primary basalts from the Sannome-gata volcano, located in the rear of the NE Japan arc. Scoriae from the volcano occur with abundant crustal and mantle xenoliths, suggesting that the magma ascended rapidly from the upper mantle. The scoriae show significant variations in their whole-rock compositions (7.9–11.1 wt% MgO). High-MgO scoriae (MgO > ~9.5 wt%) have mostly homogeneous 87 Sr/ 86 Sr ratios (0.70318–0.70320), whereas low-MgO scoriae (MgO 0.70327); ratios tend to increase with decreasing MgO content. The high-MgO scoriae are aphyric, containing ~5 vol% olivine microphenocrysts with Mg# [100 × Mg/(Mg + Fe 2+ )] of up to 90. In contrast, the low-MgO scoriae have crustal xenocrysts of plagioclase, alkali feldspar, and quartz, and the mineralogic modes correlate negatively with whole-rock MgO content. On the basis of these observations, it is inferred that the high-MgO scoriae represent primary or near-primary melts, while the low-MgO scoriae underwent considerable interaction with the crust. Using thermodynamic analysis of the observed petrological features of the high-MgO scoriae, the eruption temperature of the magmas was constrained to 1,160–1,220 °C. Given that the source mantle was depleted MORB-source mantle, the primary magma was plausibly generated by ~7 % melting of a garnet-bearing spinel peridotite; taking this into consideration, and considering the constraints of multi-component thermodynamics, we estimated that the primary Sannome-gata magma was generated in the source mantle with 0.5–0.6 wt% H 2 O at 1,220–1,230 °C and at ~1.8 GPa, and that the H 2 O content of the primary magma was 6–7 wt%. The rear-arc Sannome-gata magma was generated by a lower degree of melting of the mantle at greater depths and lower temperatures than the frontal-arc magma from the Iwate volcano, which was also estimated to be generated by ~15 % melting of the source mantle with 0.6–0.7 wt% H 2 O at ~1,250 °C and at ~1.3 GPa.
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Scoriae from the volcano occur with abundant crustal and mantle xenoliths, suggesting that the magma ascended rapidly from the upper mantle. The scoriae show significant variations in their whole-rock compositions (7.9–11.1 wt% MgO). High-MgO scoriae (MgO &gt; ~9.5 wt%) have mostly homogeneous 87 Sr/ 86 Sr ratios (0.70318–0.70320), whereas low-MgO scoriae (MgO &lt; ~9 wt%) have higher 87 Sr/ 86 Sr ratios (&gt;0.70327); ratios tend to increase with decreasing MgO content. The high-MgO scoriae are aphyric, containing ~5 vol% olivine microphenocrysts with Mg# [100 × Mg/(Mg + Fe 2+ )] of up to 90. In contrast, the low-MgO scoriae have crustal xenocrysts of plagioclase, alkali feldspar, and quartz, and the mineralogic modes correlate negatively with whole-rock MgO content. On the basis of these observations, it is inferred that the high-MgO scoriae represent primary or near-primary melts, while the low-MgO scoriae underwent considerable interaction with the crust. Using thermodynamic analysis of the observed petrological features of the high-MgO scoriae, the eruption temperature of the magmas was constrained to 1,160–1,220 °C. Given that the source mantle was depleted MORB-source mantle, the primary magma was plausibly generated by ~7 % melting of a garnet-bearing spinel peridotite; taking this into consideration, and considering the constraints of multi-component thermodynamics, we estimated that the primary Sannome-gata magma was generated in the source mantle with 0.5–0.6 wt% H 2 O at 1,220–1,230 °C and at ~1.8 GPa, and that the H 2 O content of the primary magma was 6–7 wt%. The rear-arc Sannome-gata magma was generated by a lower degree of melting of the mantle at greater depths and lower temperatures than the frontal-arc magma from the Iwate volcano, which was also estimated to be generated by ~15 % melting of the source mantle with 0.6–0.7 wt% H 2 O at ~1,250 °C and at ~1.3 GPa.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/s00410-014-0969-7</doi></addata></record>
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source Springer Nature - Complete Springer Journals
subjects Analysis
Basalt
Earth
Earth and Environmental Science
Earth Sciences
Geology
Inclusions
Low temperature
Magma
Mantle
Melting
Mineral Resources
Mineralogy
Original Paper
Petrology
Rocks
Rocks, Igneous
Spinel group
Upper mantle
Volcanoes
title Primary melt from Sannome-gata volcano, NE Japan arc: constraints on generation conditions of rear-arc magmas
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