日本地球惑星科学連合2021年大会

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[J] 口頭発表

セッション記号 M (領域外・複数領域) » M-GI 地球科学一般・情報地球科学

[M-GI33] データ駆動地球惑星科学

2021年6月3日(木) 13:45 〜 15:15 Ch.18 (Zoom会場18)

コンビーナ:桑谷 立(国立研究開発法人 海洋研究開発機構)、長尾 大道(東京大学地震研究所)、上木 賢太(国立研究開発法人海洋研究開発機構)、伊藤 伸一(東京大学)、座長:上木 賢太(国立研究開発法人海洋研究開発機構)、桑谷 立(国立研究開発法人 海洋研究開発機構)

14:30 〜 14:45

[MGI33-03] 主要・微量元素組成データの独立成分分析に基づくレアアース泥の起源成分の空間分布

*平子 雅啓1、安川 和孝1,2、田中 えりか1、藤永 公一郎2,1、中村 謙太郎1、加藤 泰浩1,2 (1.東京大学大学院工学系研究科、2.千葉工業大学次世代海洋資源研究センター)


キーワード:深海堆積物、レアアース泥、独立成分分析、化学組成、多変量解析

Deep-sea sediments highly enriched in rare-earth elements and yttrium (termed REY-rich mud) are widely distributed in the Pacific and Indian Oceans [1, 2]. Because of the huge resource potential [3], REY-rich mud is expected as a new source for the industrially critical elements (i.e., REY). Toward future exploration and development, it is important to precisely understand the origin of REY-rich mud.

Independent Component Analysis (ICA), a method of multivariate analysis, was successfully applied to a chemical composition dataset of deep-sea sediments in the Pacific and Indian Oceans to elucidate the genesis of REY-rich mud [4]. However, in the previous study, only major-elements and REY were considered. In this study, ICA was performed on a higher-dimensional dataset consisting of major- and trace-elements to characterize source components of deep-sea sediments including REY-rich mud more comprehensively. Although the overall result was generally consistent with the previous work [4], some components were newly extracted and characterized mainly by trace elements. We also visualized the spatiotemporal distributions of the independent components containing information on 44 elements. In the presentation, we will present the results of the new and comprehensive analysis.



[1] Kato et al. (2011) Nat. Geosci. 4, 535-539.

[2] Yasukawa et al. (2014) J. Asian Earth Sci. 93, 25-36.

[3] Takaya et al. (2018) Sci. Rep. 8, 5763.

[4] Yasukawa et al. (2016) Sci. Rep. 6, 29603.