日本地球惑星科学連合2015年大会

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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-IT07] New constraints on the tectonic evolution of Northeast Asia

2015年5月25日(月) 11:00 〜 12:45 A03 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*Jonny Wu(Department of Geosciences, National Taiwan University)、Kyoko Okino(Ocean Research Institute, University of Tokyo)、Cedric Legendre(Institute of Earth Sciences, Academia Sinica, Taiwan)、Gaku Kimura(Department of Earth and Planetary Science of the Graduate School of Science, The University of Tokyo)、座長:谷 健一郎(国立科学博物館地学研究部)、Lee Yuan Hsi(Department of Earth and Environmental Sciences, National CHung-Cheng University)

11:45 〜 12:00

[SIT07-09] ダイナミックに発達する南海トラフ付加体

*辻 健1芦 寿一郎2木村 学2 (1.九州大学カーボンニュートラル・エネルギー国際研究所、2.東京大学)

キーワード:地震探査データ解析, 付加体, 南海トラフ, ダイナミックな変動, バックストップ

To evaluate evolution of accretionary prism as well as forearc basin, we analyzed seismic reflection data acquired in the Nankai Trough. On the seismic profiles, the volcanic layer can be identified as strong reflection at the surface of accretionary prism beneath landward edge of the Kumano forearc basin. The accretionary prism beneath the strong reflection was constructed before the deposition of volcanic layer (14-15Ma). The undeformed basin sediment above the volcanic layer indicates that the old accretionary prism has not been much deformed after construction of the forearc basin. The accretionary prism trench-ward of the old prism was constructed at ~6Ma. The age gap of accretionary prism indicates that plate subduction (or accretion process) was halted from 15Ma to 6Ma. Because the trench-ward younger accretionary prism is much deformed, the undeformed older accretionary prism beneath the volcanic layer could work as backstop. We further find a continuous ridge system beneath the Kumano forearc basin sediment and interpret that it was generated by activities of previous splay fault. The previous splay fault develops parallel to the backstop interface as well as the coastline of the Kii peninsula. These observations demonstrate that the evolution of accretion prism including backstop interface is not stable process, but it is strongly influenced by the plate convergence rate and direction.