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 M (領域外・複数領域) » M-IS ジョイント

[M-IS18] 海底マンガン鉱床の生成・環境・起源

2016年5月24日(火) 15:30 〜 17:00 304 (3F)

コンビーナ:*臼井 朗(高知大学自然科学系理学部門)、高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)、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)、座長:臼井 朗(高知大学自然科学系理学部門)、伊藤 孝(茨城大学教育学部)、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)

16:45 〜 17:00

[MIS18-06] 東北日本弧新第三系に産する層状マンガン鉱床についての最近の研究

*伊藤 孝1,2 (1.茨城大学教育学部、2.海洋研究開発機構海底資源開発資源センター)

キーワード:マンガン鉱床、東北日本弧、放散虫

In 1950s and 1960s, Neogene strata-bound manganese oxide deposits distributed in the Northeastern Japan Arc had studied vigorously in the viewpoint of the mineral exploration (e.g. Yoshimura. 1952, 1967). Based on the mineralogy, the major elements chemistry and the geological setting, it has been concluded that these deposits formed by submarine hydrothermal activities. Miura et al. (1992) carried out the geochemical studies including trace elements and rare earth elements (REE) compositions for the Neogene strata-bound manganese oxide deposits from southwestern Hokkaido and also concluded them to having hydrothermal origin. On the other hand, they also pointed out that these deposits showed the positive Ce anomalies, which are different characters from the hydrothermal manganese deposits occurred around the modern spreading centers. Recently, Sakai et al. (in prep.) showed radiolarian stratigraphy in the Fukaura district, one of the main occurrences of the Neogene strata-bound manganese oxide deposit in the Northeastern Japan Arc, and found the long term (ca. 6 to 7 m.y.) hiatus just above the manganese deposit horizon. The long-term exposure of the manganese oxide deposit to oxic seawater may be the cause of the REE pattern showing the positive Ce anomaly.