Geology, fluid inclusion and isotope geochemistry of the Hongyuan reworked sediment-hosted Zn–Pb deposit: Metallogenic implications for Zn–Pb deposits in the Eastern Tianshan, NW China

2018 ◽  
Vol 100 ◽  
pp. 504-533 ◽  
Author(s):  
Wan-Jian Lu ◽  
Li Zhang ◽  
Hua-Yong Chen ◽  
Jin-Sheng Han ◽  
Hong-Jun Jiang ◽  
...  
2014 ◽  
Vol 88 (s2) ◽  
pp. 1192-1193 ◽  
Author(s):  
Mingjie YU ◽  
Jingbin WANG ◽  
Qigui MAO ◽  
Lijuan WANG ◽  
Fang Tonghui

2014 ◽  
Vol 49 (6) ◽  
pp. 559-573 ◽  
Author(s):  
Yan-Shuang Wu ◽  
Pin Wang ◽  
Yong-fei Yang ◽  
Nan Xiang ◽  
Nuo Li ◽  
...  

2018 ◽  
Vol 100 ◽  
pp. 401-421 ◽  
Author(s):  
Weifeng Zhang ◽  
Huayong Chen ◽  
Lianhong Peng ◽  
Liandang Zhao ◽  
Wanjian Lu ◽  
...  

Minerals ◽  
2021 ◽  
Vol 11 (4) ◽  
pp. 348
Author(s):  
Minxin You ◽  
Wenyuan Li ◽  
Houmin Li ◽  
Zhaowei Zhang ◽  
Xin Li

The Baixintan mafic-ultramafic intrusion in the Dananhu-Tousuquan arc of the Eastern Tianshan orogenic belt is composed of lherzolite, olivine gabbro, and gabbro. Olivine gabbros contain zircon grains with a U-Pb age of 276.8 ± 1.1 Ma, similar to the ages of other Early Permian Ni-Cu ore-bearing intrusions in the region. The alkaline-silica diagrams, AFM diagram, together with the Ni/Cu-Pd/Ir diagram, indicate that the parental magmas for the Baixintan intrusion were likely high-Mg tholeiitic basaltic in composition. The Cu/Pd ratios, the relatively depleted PGEs and the correlations between them demonstrate that the parental magmas had already experienced sulfide segregation. The lower CaO content in pyroxenites compared with the Duke Island Alaskan-type intrusion and the composition of spinels imply that Baixintan is not an Alaskan-type intrusion. By comparing the Baixintan intrusion with other specific mafic-ultramafic intrusions, this paper considers that the mantle source of the Baixintan intrusion is metasomatized by subduction slab-derived fluids’ components, which gives rise to the negative anomalies of Nb, Ti, and Ta elements. Nb/Yb-Th/Yb, Nb/Yb-TiO2/Yb, and ThN-NbN plots show that the Baixintan intrusion was emplaced in a back-arc spreading environment and may be related to a mantle plume.


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