日本地球惑星科学連合2018年大会

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[JJ] ポスター発表

セッション記号 M (領域外・複数領域) » M-ZZ その他

[M-ZZ41] 海底マンガン鉱床の科学:基礎から応用まで

2018年5月23日(水) 13:45 〜 15:15 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:臼井 朗(高知大学海洋コア総合研究センター)、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、共同)、伊藤 孝(茨城大学教育学部)

[MZZ41-P06] Identification of oxide layer structures of ferromanganese nodules in the Minamitorishima EEZ using X-ray CT

*下村 遼1中村 謙太郎1町田 嗣樹2,3安川 和孝1,2藤永 公一郎2,1加藤 泰浩1,2,3 (1.東京大学大学院工学系研究科システム創成学専攻、2.千葉工業大学次世代海洋資源研究センター、3.海洋研究開発機構)

キーワード:マンガンノジュール、X線CT分析、南鳥島EEZ

In recent years, it has been discovered that ferromanganese nodules are densely distributed from the south to the east of the Japanese Exclusive Economic Zone (EEZ) around Minamitorishima [1]. Ferromanganese nodules in the Minamitorishima EEZ contain Co at the maximum of 0.65% and Ni at the maximum of 0.8% [2] and thus, expected as a future resource for the critical metals. To focus on the promising areas for the future development of the nodules, it is necessary to elucidate their origin. The internal structure of ferromanganese nodules is one of the most important keys to understanding the origin and growth history of the nodules.
In this study, we conducted X-ray CT analysis of the nodules from the Minamitorishima EEZ to nondestructively identify the internal structures of the nodules. As a result of the analysis, it was defined that the oxide layers of the nodules can be classified into 5 layers on the basis of the difference in X-ray absorption rate. We also found that the X-ray absorption rate corresponds to both the growth texture and chemical composition of the oxide layers. Moreover, several peaks were observed in the histograms of the total oxide layer thickness, and these peaks corresponded to number of oxide layers. This suggests that formations of ferromanganese nodules occur intensively during certain periods when each oxide layer starts growing.

References
[1] JAMSTEC (2016) press release, August 26, 2016.
[2] Machida et al. (2016) Geochemical Journal, 50, 539–555.