日本地球惑星科学連合2016年大会

講演情報

インターナショナルセッション(口頭発表)

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT11] Geodynamic evolution of northeast Asia and western Pacific

2016年5月24日(火) 13:45 〜 15:15 A05 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*木村 学(東京大学大学院理学系研究科地球惑星科学専攻)、Wu Jonny(Department of Geosciences, National Taiwan University)、Byrne Timothy(University of Connecticut)、沖野 郷子(東京大学大気海洋研究所)、座長:Wu Jonny(Department of Geosciences, National Taiwan University)、沖野 郷子(東京大学大気海洋研究所)

14:15 〜 14:30

[SIT11-03] Dynamic of the Japan subduction system

Claudio Faccenna1Hitoshi Kawakatsu2、*Thorsten W Becker3Francesca Funiciello1Adam Holt3 (1.Dip. Scienze Univrsità Roma TRE, Roma (Italy)、2.Earthquake Research Institute, Univ. of Tokyo, Tokyo (Japan)、3.Dept. Earth Science, Univ. Southern California Los Angeles (CA))

キーワード:subduction, Mariana-Izu-Bonin, geodynamic modeling

The geometry of the Mariana-Izu-Bonin (IBM)-Japan slab consists of a large cusp where the undulation of the trench is accompanied by a corresponding variation in slab dip, varying form sub-vertical beneath the Marianas to shallow dipping beneath Japan. The origin and the cause of these variations are still poorly understood.We reconstruct the backarc extensional system of the Philippine plate, showing that the triple junction between the IBM, Ryuku, and Japan migrated northward during the last 40 Ma reaching its present-day position. We balance back the subduction system on time, starting from recent tomographic models and using an absolute reference frame plate reconstruction model. Our kinematic model suggests that the evolution and the geometry of the Japan slab is controlled by the interaction with the surrounding slabs. We test this hypothesis with simple laboratory experiments. Our preliminary results suggest that the slab geometry is influenced by local and plate-scale mantle flow.