日本地球惑星科学連合2022年大会

講演情報

[E] 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-CG44] Science of slow-to-fast earthquakes

2022年5月27日(金) 15:30 〜 17:00 103 (幕張メッセ国際会議場)

コンビーナ:加藤 愛太郎(東京大学地震研究所)、コンビーナ:田中 愛幸(東京大学理学系研究科)、山口 飛鳥(東京大学大気海洋研究所)、コンビーナ:波多野 恭弘(大阪大学理学研究科)、座長:山口 飛鳥(東京大学大気海洋研究所)、橋本 善孝(高知大学)

16:30 〜 16:45

[SCG44-34] 熊野沖南海トラフ付加体先端部の海山沈み込みに伴う海底下浅部の変形

*山口 飛鳥1大熊 祐一1福地 里菜2芦 寿一郎1木村 学3 (1.東京大学大気海洋研究所、2.鳴門教育大学、3.海洋研究開発機構)

Although the relationship between subducted seamount and seismicity has been discussed, the nature of structures formed by seamount subduction remains unclear. In this study, we focus on the structures of the toe of the accretionary prism, which might have been formed by a seamount subducting into the Nankai Trough off Kumano.
At the Kumano frontal prism, magnetic anomaly shows that a small seamount subducted into the west side of the NanTroSEIZE transect. The stratigraphy and ages of IODP Sites C0006, C0007, and C0024 constrain the structural development of the frontal thrust system. In the front prism, an out-of-sequence thrust (OOST) has been developed after the formation of the imbricate thrusts, and its activity was started after ~0.5 Ma based on the tephrochronology of Site C0024. This OOST activity would reflect the subduction of the seamount. On the west side of the OOST, indented topography and landslides are developed, indicating slope failures caused by seamount subduction. Okuma et al. (this meeting) proposed that the friction of the plate boundary fault affects the deformation processes of the accretionary prism rather than the topographic factor of the subducting seamount. Seismic profiles (Shiraishi et al., 2020) show that the plate boundary fault is located far above the seamount, therefore the friction of the decollement above the seamount should be the same as the surrounding area. To construct topographic and structural features around the seamount, pore fluid pressure of the decollement may be decreasing due to the development of faults. The landslide at the toe of off Kumano frontal prism will be investigated by the SHINSEI MARU KS-22-3 cruise, and the preliminary results will be also introduced in the presentation.