JpGU-AGU Joint Meeting 2017

講演情報

[JJ] 口頭発表

セッション記号 S (固体地球科学) » S-GC 固体地球化学

[S-GC54] [JJ] 地球化学の最前線

2017年5月24日(水) 15:30 〜 17:00 101 (国際会議場 1F)

コンビーナ:鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、横山 祐典(東京大学 大気海洋研究所 高解像度環境解析研究センター)、橘 省吾(北海道大学大学院理学研究院自然史科学専攻地球惑星システム科学分野)、座長:鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、座長:橘 省吾(北海道大学大学院理学研究院自然史科学専攻地球惑星システム科学分野)

15:45 〜 16:00

[SGC54-08] イオン吸着型鉱床がレアアースの資源となる理由

*山口 瑛子1本多 翼高橋 嘉夫1 (1.東京大学)

キーワード:希土類元素、イオン吸着型鉱床、表面錯体、イオン半径、価数

Introduction
Rare earth element (REE) is a set of chemical elements essential for high technology industries. Ion-adsorption deposits of REE are appropriate for industries, since REE in the deposits can be easily extracted without treatment of radioactive elements, uranium and thorium. Ion-adsorption deposits are formed by adsorption of REE on weathered granite. However, it is not clear the relationship between the degree of weathering and potential of the weathered granite as REE ion-adsorption deposit. In this study, abundances and extraction ratios of REE were systematically examined for weathered granite samples with different degrees of weathering, which should be related to the variation of secondary minerals formed in the granite. In addition, the interaction of REE with potential secondary minerals was also studied to clarify the characteristics of ion-adsorption deposit, which is likely unique as a resource of REE.

Methods
Weathered granite samples were collected from Hiroshima, Shimane, and Tottori Prefectures in Japan and also from various climate zones in Sri Lanka. Mineral and major element compositions were examined by X-ray Diffraction (XRD) and X-ray fluorescence (XRF), respectively. CIA, which represents the degree of weathering, is calculated using the results of XRF. To reveal extraction ratio of REE, decomposed solutions of REE were prepared by two methods and their REE were measured by ICP-MS. One was prepared by acid digestion, which gives total REE concentration. The other was obtained by extraction by ammonium chloride solution, which corresponds to extractable concentration. To reveal the relationship between REE and other cations, adsorption experiment was performed, by which Kd was calculated. REE was absorbed to vermiculite and ferrihydrite in three solutions; 0.10 M NaNO3 aq., 1.0 M NaNO3 aq., and 1.0 M NH4Cl aq. To reveal the comparison between REE and other elements, K-edge EXAFS of lanthanum (La), strontium (Sr), barium (Ba), potassium (K), rubidium (Rb), and cesium (Cs) were also performed after their adsorption on the adsorbents to identify their adsorption species.

Results & Discussion
The result of XRF analysis revealed that the ability of adsorption depends on the degree of weathering and can be highest in mildly weathered granite, or in granite of which CIA (Chemical Index of Alteration) is 65~75. Coulpled with the XRD results, it was found that the relationship of REE and clay minerals is very important for Ion-absorption deposit. These results suggest that the potential of ion-adsorption deposit depends on the climate controlling the degree of weathering.
Kd, which is calculated using the results of adsorption experiment, revealed that extraction ratio of REE adsorbed to ferrihydrite is low and extraction ratio of REE adsorbed to clay minerals is high. In the REE pattern of Kd, REE adsorbed to ferrihydrite shows tetrad effect, which shows the formation of REE inner-sphere complex. REE adsorbed to vermiculite, on the other hand, do not show tetrad effect, or REE outer-sphere complex. Thus, when REE form outer-sphere complex, the extraction ratio of REE becomes high. Furthermore, Kd of REE and Sc are high. This is because they are trivalent and attracted electrostatically to a larger degree, which suggests that high charges of cations are important for ion-adsorption deposit. XAFS spectrum of the adsorbed mineral species similar to that of solution sample shows that the ion adsorbed to the mineral forms outer-sphere complex. The results revealed that the types of surface complex depend on the ionic size. Ions which are smaller than Ba2+ form outer-sphere complex, while ions larger than Ba2+ form inner-sphere complex. Thus, ions which can form ion-absorption deposit are smaller than Ba2+ and have high charges. Among the many hard ions, only REE meet the requirement to form the Ion-adsorption deposit.