日本地球惑星科学連合2015年大会

講演情報

口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS35] この星は、なぜ地球なのか? -水の役割-

2015年5月24日(日) 14:15 〜 16:00 201A (2F)

コンビーナ:*島 伸和(神戸大学大学院理学研究科惑星学専攻)、巽 好幸(海洋研究開発機構 地球内部ダイナミクス領域)、大槻 圭史(神戸大学大学院理学研究科)、中川 貴司(海洋研究開発機構数理科学・先端技術研究分野)、片山 郁夫(広島大学大学院理学研究科地球惑星システム学専攻)、藤江 剛(海洋研究開発機構)、中村 昭子(神戸大学大学院理学研究科地球惑星科学専攻)、座長:片山 郁夫(広島大学大学院理学研究科地球惑星システム学専攻)、島 伸和(神戸大学大学院理学研究科惑星学専攻)

14:30 〜 14:45

[MIS35-16] 沈み込み帯の水挙動とマグマの生成

*木村 純一1中島 淳一2 (1.(独)海洋研究開発機構、2.東北大学)

キーワード:沈み込み帯, 水, マグマ

Water at subduction zones is carried to mantle depths by the subducting oceanic plate and then released by dehydration. It then migrates upwards and contributes to melting of the mantle wedge to form primary arc magma. The magma thus captures and transfers water to the crust, or outgasses water to the atmosphere. Water, either in fluids or melts in both the slab and the mantle, promotes the dissolution and mobilization of elements and affects the physical properties of the sub-arc slab, mantle, and seismicity. In this paper, we present a coherent model to explain the geophysical and geochemical role of water beneath NE Japan. We first investigate the seismic structures of the downgoing slab and sub-arc mantle and examine the role of subducted water in forming these structures. We then use the Arc Basalt Simulator version 4, a petrological-geochemical model developed to describe the geochemical behaviours of water and elements in the slab, mantle, and arc basalt. Parameters governing these petrogenetic processes are also estimated by the model and compared to geophysical observations. The combined approach shows that (1) subducted sediment and igneous oceanic crust are almost fully hydrated, whereas only partial hydration occurs in the oceanic mantle; (2) this high slab water content leads to melting of the slab sediment and the uppermost basalt layer beneath the arc; (3) the released water via slab liquid promotes 3?25% melting of the mantle wedge at a depth of 50?30 km at a mantle temperature of 1250?1350 °C; (4) virtually 89% of slab water is released, 22% of the water returns to the forearc, and 38% enters the arc crust with the magma; and (5) 11% of the subducted water retained beyond a depth of 180 km is held in the slab, and 29% in nominally anhydrous minerals in the wedge mantle.