日本地球惑星科学連合2019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-TT 計測技術・研究手法

[M-TT48] 地球化学の最前線

2019年5月26日(日) 15:30 〜 17:00 201A (2F)

コンビーナ:角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也(東京工業大学理学院地球惑星科学系)、小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)、座長:角野 浩史小畑 元(東京大学大気海洋研究所)、横山 哲也(東京工業大学)

16:45 〜 17:00

[MTT48-12] ニッケルラテライト鉱床におけるスカンジウムと他の希土類元素の化学種と分配挙動の違い

Haibo Qin1実松 健造2Arcilla Carlo3、*高橋 嘉夫1 (1.東京大学大学院理学系研究科地球惑星科学専攻、2.産業技術総合研究所地質調査総合センター、3.フィリピン大学)

キーワード:スカンジウム、希土類元素、ラテライト

Scandium (Sc) is a critical metal with wide applications in modern industrial applications. Consequently, the enrichment of Sc at earth surface has been of great interest in resource geology. It has been reported that laterite enriched with nickel (Ni laterite) contained significant amounts of Sc (about 80-100 ppm). The vertical profile of Ni laterite mainly consists of bed rock, saprolite, and limonite layers from bottom to the top. Generally speaking, Ni remobilized downward during weathering processes leads to the enrichment of Ni in the saprolite layer, while maximum Sc enrichment is found in the limonite layer mainly consisting of goethite. However, distribution and speciation of Sc in the limonite layer are not clear at present, which was examined by μ-XRF mapping and X-ray absorption fine structure (XAFS) spectroscopy in this study. In addition, similar information such as abundances and speciation was obtained also for other rare earth elements including yttrium (REY) to compare geochemical behaviors between Sc and REY.

Micro-XRF analysis revealed that Sc and Y are distributed to goethite in the limonite layer. Sequential extraction revealed that Sc remains in the residual phase which goethite is still present even after the treatments by reducing agents and aqua regia. XANES and EXAFS analyses for Sc in the limonite layer and its comparison with synthetic samples of Sc coprecipitated with goethite and Sc adsorbed on goethite revealed that Sc was incorporated within the goethite structure replacing Fe3+ site. This result is reasonable considering the similar ionic radii (6 coordination number) of Sc3+ (0.75 Å) and Fe3+ (0.65 Å). On the contrary, EXAFS for the Y samples synthesized similarly to Sc showed that Y cannot be incorporated within the goethite structure, possibly due to its large size (ionic radius of Y3+: 0.90 Å) compared with Fe3+. The sequential extraction showed that most of Y was present as ion-exchangeable species or Y in amorphous Fe and Mn oxides, which are consistent with the fact that Y is mainly present as adsorbed species on goethite. These results clearly explain fractionation of REY and Sc in limonite layer, with steep increase from Yb3+ to Sc3+ when we plot Sc at right of Lu in REY pattern.

The high concentration of Sc in Ni laterite is caused by (i) high concentration of Sc in the original rock (peridotite) and (ii) effective fixation of Sc3+ within goethite by substitution of Fe3+ site by Sc3+ during intense weathering to form laterite.