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-GC 固体地球化学

[S-GC56_30PM2] 固体地球化学・惑星化学

2014年4月30日(水) 16:15 〜 17:45 415 (4F)

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:山下 勝行(岡山大学大学院自然科学研究科)、下田 玄(産業技術総合研究所地質調査総合センター)

17:15 〜 17:30

[SGC56-12] 南鳥島EEZ内におけるレアアース泥の構成鉱物の特徴およびその成因への示唆

*大田 隼一郎1高谷 雄太郎2藤永 公一郎2安川 和孝1中村 謙太郎1町田 嗣樹3原口 悟1加藤 泰浩2 (1.東京大学工学系研究科システム創成学専攻、2.東京大学工学系研究科エネルギー・資源フロンティアセンター、3.早稲田大学創造理工学部環境資源工学科)

キーワード:レアアース, レアアース泥, 深海底鉱物資源

The KR13-02 cruise was conducted in the southern part of the Minamitorishima to explore rare-earth elements and yttrium-rich mud (REY-rich mud) within Japanese Exclusive Economic Zone (EEZ) on January 2013. During the cruise, seven sediment cores were successfully collected. The results of bulk sediment analyses showed that one of the cores (PC05) has an extremely REY-concentrated layer with 6,596 ppm total REY (Kato et al., 2013; Suzuki et al., 2013) which is three times higher than the maximum concentration in the mud previously reported for the eastern South and central North Pacific Ocean (2,230 ppm; Kato et al., 2011). In addition to REY, P concentration in the layer is also noticeably high (Kato et al., 2013; Suzuki et al., 2013), suggesting that Ca phosphate (apatite) is mainly responsible for the REY-enrichment in the layer, as in the case for the mud presented in other areas (Kashiwabara et al., 2014). However, factors contributing the extreme enrichment of REY, which in turn might provide important insights into the genesis of REY-rich mud, are still uncertain. In the present contribution, we report mineralogical features of Minamitorishima REY-rich mud including the extremely REY-concentrated layer and discuss about its genesis.