日本地球惑星科学連合2016年大会

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セッション記号 S (固体地球科学) » S-GC 固体地球化学

[S-GC50] 固体地球化学・惑星化学

2016年5月22日(日) 13:45 〜 15:15 A07 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*下田 玄(産業技術総合研究所地質調査総合センター)、鈴木 勝彦(国立研究開発法人海洋研究開発機構・海底資源研究開発センター)、山下 勝行(岡山大学大学院自然科学研究科)、石川 晃(東京大学大学院総合文化研究科)、飯塚 毅(東京大学)、座長:石川 晃(東京大学大学院総合文化研究科)、飯塚 毅(東京大学)

15:00 〜 15:15

[SGC50-06] マントルリザボアの成因:沈み込み帯フィルターとマントル熱進化の役割

*木村 純一1Gill James2van Keken Peter3Skora Susanne4川畑 博5 (1.海洋研究開発機構・地球内部物質循環研究分野、2.カリフォルニア大学サンタクルツ・地球惑星科学科、3.カーネギー科学研究所・地球電磁気学科、4.ETH・地球化学-岩石学研究所、5.高知大学・研究教育学部)

キーワード:マントルリザボア、沈み込み帯フィルター、マントル熱史

Upwelling mantle melts at Mid-Ocean Ridges (MOR) to form basaltic igneous oceanic crust (IOC). IOC and overlying sediment (SED) descend into the mantle at subduction zones (SZ). The IOC, SED, and overriding mantle melt to form stable continental crust (CC) after crustal-level processing, whereas the residual slab is recycled into the lower mantle. We quantitatively explore the element re-distributions at MOR and SZ using numerical mass balance models, and we evaluate their roles in the Earth’s geochemical cycle. Our models of slab residues differ from previous ones by being internally consistent with geodynamic models of modern arcs and successful explanations of modern arc magma genesis, and by including element fluxes from the dehydration or melting of each underlying slab component. We find that the upper mantle potential temperature (Tp) was 1400–1650 °C from 3.5 to 1.7 Gyr before decreasing gradually to ~1300 °C today. Hot SZs with Tp ~1600 °C have a thermal structure like modern SW Japan where high-Mg andesite is formed that is like CC. Isotopically, residual IOC from hot SZ evolves to the HIMU OIB reservoir, residual SED to EMII, the residual base of the mantle wedge to EMI, and the residual top of the mantle wedge to the subcontinental lithosphere (SCLM) reservoir, after 1.7–2.5 Gyr of storage in the lower mantle. The Common (C) or Focal Zone (FOZO) reservoir is a stable mixture of the first three residues. Older recycled residues (~2.5 Gyr) form the DUPAL anomaly in the southern hemisphere, whereas younger ones (~1.7 Gyr) are in the northern hemisphere. These ages correspond to major CC forming events. We attribute the E-W heterogeneity of the depleted upper mantle (DMM) to involvement of sub-Gondwana SCLM except in the Pacific.