日本地球惑星科学連合2015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

2015年5月25日(月) 14:15 〜 16:00 102A (1F)

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(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)、山下 勝行(岡山大学大学院自然科学研究科)、座長:鈴木 勝彦(独立行政法人海洋研究開発機構・海底資源研究開発センター)、下田 玄(産業技術総合研究所地質調査総合センター)

14:15 〜 14:30

[SGC50-01] 海洋地殻の層状構造と2段階脱水:HIMU-FOZO-PREMAの成因に関する解釈

*下田 玄1小木曽 哲2 (1.産業技術総合研究所、2.京都大学人間・環境学研究科)

キーワード:HIMU, FOZO, PREMA, MORBs, OIBs

Isotopic composition of the ocean island basalts (OIBs) can be explained by mixing of isolated reservoirs in the Earth (White, 1985; Zindler and Hart, 1986; Hofmann, 1997; Stracke, 2012). In early research on the mantle reservoirs, the isotopic composition of OIBs was explained by the mixing of depleted MORB mantle (DMM) and three enriched reservoirs, those are HIMU (high-u: u = 238U/204Pb) EM1 (Enriched Mantle 1) and EM2 (Enriched mantle 2). In addition to these reservoirs, importance of reservoirs whose isotopic compositions are common and intermediate has been pointed out, such as, FOZO (Focal Zone, Hart et al., 1992) and PREMA (Prevalent Mantle, Zindler and Hart, 1986). Although these intermediate reservoirs have been used to describe the isotopic distribution of OIBs, existences of the intermediate reservoirs, themselves, are still in debate. Therefore, elucidating the origin of the intermediate reservoirs should be also important from the perspective of production of mantle heterogeneity (e.g., Hofmann, 1997; Stracke et al. 2005; Stracke, 2012).
To elucidate the origin of mantle reservoirs, geochemical modeling has been conducted, in which origin of HIMU, FOZO and PREMA is discussed. The results suggest that MORBs with high frequency (common MORBs) have chemical composition that is suitable for production of PREMA if chemical modification during subduction is negligible. It may suggest the importance of recycling of dry MORBs for the production of OIBs source. Dehydration of common MORBs beneath an arc can produce FOZO isotopic signatures if amount of dehydrated water is large (4 %) which may represent maximum amount of dehydrated aqueous fluid at sub-arc area. Thus, FOZO-PREMA isotopic array can be explained by recycling of common MORBs that release various amount of aqueous fluid during subduction. For the production of HIMU, additional dehydration (~2%) at high pressure is required. As high pressure dehydration release supercritical fluid, chemical fractionation during dehydration is different from the sub-arc process. This difference can explain isotopic difference between HIMU and FOZO.