日本地球惑星科学連合2016年大会

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インターナショナルセッション(ポスター発表)

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-IT09] Hard-Rock Drilling: Oceanic Lithosphere to Continental Crust Formation

2016年5月23日(月) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*田村 芳彦(海洋研究開発機構 海洋掘削科学研究開発センター)、森下 知晃(金沢大学理工研究域自然システム学系)、Straub Susanne(コロンビア大学ラモント地球科学研究所)、佐野 貴司(国立科学博物館地学研究部)、海野 進(金沢大学理工研究域自然システム学系)、高澤 栄一(新潟大学理学部地質科学科)、道林 克禎(静岡大学学術院理学領域)

17:15 〜 18:30

[SIT09-P09] Evolutionary processes of submarine volcano in an incipient arc reference from the Oman Ophiolite

*草野 有紀1海野 進2北村 啓太朗3金山 恭子4 (1.産業技術総合研究所 地質調査総合センター、2.金沢大学理工研究域自然システム学系、3.アジア航測株式会社、4.鳥取県山陰海岸世界ジオパーク推進室)

キーワード:Subduction initiation, high-T subduction zone, Boninite, Oman Ophiolite, submarine volcano geology

The Oman ophiolite belonging to the Tethys ophiolite zone is one of the best places to investigate magmatic and volcanic developing processes of an infant arc. The Ophiolite had formed on a spreading axis and followed by subduction stage magmatism at approximately 100 Ma. The volcanostratigraphy is similar to that of the Izu-Bonin-Mariana Arc (e.g. Starn, 2004). However, the latest U-Pb age of zircon in plutonic bodies shows that there is only 0.5 m.y. time gap between the spreading and subduction stages (Riuox et al., 2014), therefore, it seems to record short-spanned island arc magmatism. Progressive geochemical change from island arc tholeiite (LV2) to boninite (UV2) in this period showed us the evolutionary process of the high-T and ephemeral subduction zone (Kusano et al., 2015). To reveal the stress history during the subduction stage, we reconstructed accretionary process of the arc magmas at the northern Oman ophiolite.
The subduction stage volcanic rocks (V2) extend >350 km along the Oman Ophiolite. In Wadi Salahi area, the V2 consist of the 600-970 m thick lower LV2 and 0-140 m thick upper UV2. Pahoehoe and sheet flows are dominate in the LV2, while 50 m thick pyroclastic rocks are partly distributed upward. Plural flow units and sporadically distributed plugs and dikes at 1-3 km spaces are recognized in the LV2. These plugs are 1.5-3 m in diameter with cylindrical layering of fine-grained and coarse-grained parts. The distribution of plugs and dikes look unbiased in the stratigraphic horizon. Because the LV2 was erupted through cone sheets (Alabaster et al., 1982), these plugs might be distributed along the “ring conduit”. Similar bulk rock compositions of the LV2 including lava flows and pyroclastic rocks suggest the share in the magma chamber. However, E-W concentration of strike of plugs and dikes would be resulted from the regional E-W compression (Umino et al., 1990).