JpGU-AGU Joint Meeting 2020

講演情報

[J] 口頭発表

セッション記号 M (領域外・複数領域) » M-ZZ その他

[M-ZZ57] 海底マンガン鉱床の生成環境と探査・開発

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・海底資源センター)、伊藤 孝(茨城大学教育学部)

[MZZ57-03] Interlayer water structure in Na-, K- and Cs-birnessite

*Sujeong Park1Kideok D. Kwon1 (1.Kangwon National Univ.)

キーワード:Birnessite, Molecular dynamics simulation, Manganese, Interlayer, water content

Birnessite (Bi) is a major oxide mineral of manganese nodules found on the ocean floor. It is a layer-type mineral composed of Mn octahedral sheets with monovalent cations (Na+, K+ and Cs+) intercalated. However, the low crystallinity and fine-grained size of natural birnessite limit full characterization of the structure, particularly water structure in the interlayer which greatly impacts the mineral reactivity for metal sorption. In this study, we investigated the interlayer structures of Na-, K- and Cs-Bi using classical molecular dynamics (MD) simulations. While the d-spacing of Na-Bi was greater than that of K-Bi in experiments, our MD simulations calculated the d-spacing of K-Bi greater than that of Na-Bi. MD simulations with variations in the water content suggest that a much greater water content in Na-Bi is required to be consistent with experimental results, indicating large uncertainties in the interlayer water content. When the water content increased up to a buserite type mineral, MD simulations found an abrupt expansion of the d-spacing along with increased disorder in the orientations of the water molecules. We discuss the effects of the interlayer water structure on the d-spacing of birnessite.