日本地球惑星科学連合2014年大会

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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-IT40_1PM1] 地殻流体:その分布と変動現象への役割

2014年5月1日(木) 14:15 〜 16:00 416 (4F)

コンビーナ:*中村 美千彦(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)、佐久間 博(東京工業大学大学院理工学研究科地球惑星科学専攻)、市來 雅啓(東北大学大学院理学研究科)、高橋 努(独立行政法人海洋研究開発機構 地球内部ダイナミクス領域)、座長:横山 哲也(東京工業大学大学院理工学研究科地球惑星科学専攻)、堀口 桂香(独立行政法人 産業技術総合研究所 地質情報研究部門 深部流体研究グループ)

15:00 〜 15:15

[SIT40-14] 東北日本のヘリウム同位体比分布;地質構造との比較

*堀口 桂香1風早 康平1塚本 斉1森川 徳敏1佐藤 努1大和田 道子1仲間 純子1 (1.産業技術総合研究所 地質情報研究部門)

キーワード:ヘリウム同位体比, 東北日本, 空間分布, 地質構造

The distribution of slab fluid defined by high Li/Cl ratios conforms the area of "hot fingers"(Tamura et al., 2002) in Northeast Japan (Kazahaya et al., submitted). Conversely, the high 3He/4He ratios distribute wider and do not match with slab-derived fluids indicating that some of the mantle-derived helium would not be transported with magmas or slab fluids but directly upwells as mantle-derived fluid. The 3He/4He ratios vary along the volcanic front showing an areal contrast; such as a low-ratio-area close to volcanoes are observed in the central part of Tohoku. We propose here an extended helium upwell model which can explain the spatial variation of 3He/4He ratios with the following concept; 1) The most important constraint for mantle helium upwelling is the crustal structure divided by tectonic lines; Hatagawa Tectonic Line (HTL) divides the Kitakami and Abukuma belts. Ryoke belt and north part of Abukuma belt is torn apart by number of faulting events. The rest of parts, Abukuma granitic province and Kitakami province form very large stable blocks which might prohibit helium to upwell from mantle. 2) A view from U-Th content in the crust is im-portant to understand the flat distribution of mantle helium in back-arc region; Low U-Th crust in the back-arc with less crustal 4He production is favora-ble to explain the flat and high 3He/4He signature, such as oceanic crust might have.Tanakura Tectonic Line (TTL) divides the thick crust of con-tinental margin (sedimentary prism and granite) with Ryoke belt.