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Jingwenite-(Y) from the Yushui Cu deposit, South China: The first occurrence of a V-HREE-bearing silicate mineral

  • Peng Liu ORCID logo , Xiangping Gu , Wenlan Zhang , Huan Hu , Xiaodan Chen , Xiaolin Wang ORCID logo , Wenlei Song , Miao Yu and Nigel J. Cook ORCID logo
Published/Copyright: January 3, 2023
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Abstract

Jingwenite-(Y), Y2Al2V24+(SiO4)O4(OH)4, the first V-HREE-bearing silicate mineral discovered in nature, is an abundant component of a sediment-hosted stratiform Cu (SSC) deposit, Yushui, South China. The mineral occurs in bedded/massive sulfide-bearing ore and is associated with bornite, chalcopyrite, galena, xenotime-(Y), nolanite, thortveitite, roscoelite, barite, and quartz. Optically, jingwenite-(Y) is biaxial (+), with α = 1.92(4), β = 1.95(2), γ = 1.99(3) (white light), and 2V (calculated) = 83°. The dispersion is medium with r < v, and the pleochroism is with X = light brown, Y = brown, Z = dark brown. The color, streak, luster, and hardness (Mohs) are light brown, yellowish gray, vitreous, and 4½–5, respectively.

Jingwenite-(Y) is monoclinic, with space group I2/a, Z = 4, and unit-cell parameters a = 9.4821(2) Å, b = 5.8781(1) Å, c = 19.3987(4) Å, β = 90.165(2)°, and V = 1081.21(4) Å3. The structure of jingwenite-(Y) has chains of edge-sharing Al(V,Fe)-O octahedra and V(Ti)-O octahedra extending along the b-axis and linked by insular Si-O tetrahedra, leaving open channels occupied by HREEs. Jingwenite-(Y) is a new nesosilicate structural type.

Sm-Nd dating and Nd isotope signatures of jingwenite-(Y) reveal an epigenetic origin and suggest that HREEs and V were added to the SSC system via leaching of abundant heavy minerals in the footwall red sandstone by oxidized basinal brines. The abundance of jingwenite-(Y) at Yushui indicates that it could potentially be a valuable resource for HREE and V. Moreover, HREE and V mineralization can also occur in the same sediment-hosted Cu mineral system.

Acknowledgments and Funding

We thank Guoguang Wang, Xiaochun Li, Changhui Ke, Wei Jian, and Liang Li for their insightful discussion and technical assistance with EPMA and Sm-Nd isotope analysis. We appreciate the careful editing and constructive comments from Frank Hawthorne and one anonymous reviewer. This research was jointly funded by the National Natural Science Foundation of China (grants 42272070, 42130102, 42072054, and 41902072).

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Received: 2021-11-01
Accepted: 2022-02-01
Published Online: 2023-01-03
Published in Print: 2023-01-27

© 2023 Mineralogical Society of America

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