日本地球惑星科学連合2022年大会

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[J] 口頭発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG49] 地球惑星科学におけるレオロジーと破壊・摩擦の物理

2022年5月26日(木) 10:45 〜 12:15 304 (幕張メッセ国際会議場)

コンビーナ:東 真太郎(東京工業大学 理学院 地球惑星科学系)、コンビーナ:田阪 美樹(静岡大学 )、清水 以知子(京都大学大学院理学研究科地球惑星科学専攻)、コンビーナ:桑野 修(国立研究開発法人 海洋研究開発機構)、座長:東 真太郎(東京工業大学 理学院 地球惑星科学系)

10:45 〜 11:00

[SCG49-13] 西南日本川下かんらん岩捕獲岩から得られた日本海拡大時の変形の証拠

*田阪 美樹1、仲井 優河1 (1.静岡大学 )

キーワード:かんらん岩捕獲岩、かんらん石結晶方位定向配列、背弧拡大

In order to better understand plate dynamics, it is critical to know why and how back-arc spreading/rifting occurs near the convergent plate boundaries. In this presentation we focus on Japan Sea as an example of back arc. Two possible models have been proposed as the formation mechanism of the Japan Sea back-arc basins, which are “slab rollback model” and “plume model”. We investigated 12 spinel peridotite xenoliths in the Cenozoic Kawashimo alkali basalt, SW Japan. These peridotite xenoliths are dominantly harzburgite with minor lherzolite. Harzburgite and lherzolite showed coarse-grained or porphyroclastic texture, recording the variable degrees of deformation. Forsterite content of olivine and Cr# of spinel suggested that these samples are residual mantle peridotite with the various decree of partial melting. Olivine crystallographic preferred orientation in the peridotite xenoliths have orthorhombic pattern characterized by strong [010] axis point maxima normal to the foliation and [100] axis parallel to the lineation in both coarse-grained and porphyroclastic texture. This orthorhombic pattern implies that the peridotite xenoliths deformed under dislocation accommodated creep with (010)[100] slip system. Using a sub-grain size piezometer, the maximum differential stress varies from 5 to 15 MPa in the samples. Combining the olivine flow laws from previous deformation experiments with the obtained flow stress and grain size, we found that the peridotite xenoliths deformed under dislocation accommodated grain boundary sliding creep with relatively high strain rate such as 10-11 - 10-9 s-1. The range of high strain rate is comparable to that predicted from a thermomechanical model of back-arc spreading. Therefore, it is likely that the peridotite preserves deformation texture during the Japan Sea back-arc spreading. We also obtained the equilibrium temperature of 1239±18C based on two-pyroxene geothermometer, which is higher than those of any previously reported peridotite xenoliths in SW Japan. The obtained equilibrium P-T condition for the peridotite xenoliths implies that the hot mantle plume hypothesis is a more likely explanation as the formation mechanism of Japan Sea back-arc basins.