纳米比亚Cape Cross-Uis伟晶岩带稀有金属伟晶岩:地质、矿化、铷锶特征和岩石成因

M. Diehl
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引用次数: 20

摘要

Cape cross - us伟晶岩带(纳米比亚)的稀有金属伟晶岩含有亚经济到经济浓度的Sn, Nb, Ta, Li,出现在三个主要伟晶岩群中。未分带的稀有金属伟晶岩以浸染状锡石矿化和不同的Li、Ta和Nb浓度为特征,而分带和不分带的富Li稀有金属伟晶岩除了低品位锡石矿化外,还含有较高的Nb、Ta和Li浓度(500 ppm Nb;800 ppm Ta平均值)。这两种类型的产状都局限于半地堑构造张拉环境下泛非绿片岩相沉积的广泛剪切区。研究区带状和非带状伟晶岩中各矿物相的Rb/Sr同位素研究表明,伟晶岩熔体的侵位年龄为490 Ma,为泛非晚期。岩石学上,高87Sr/86Sr初始比值反映了地壳物质(基底岩)的部分熔融。研究区稀有金属伟晶岩起源于区域变质作用高峰期。向大西洋方向的变质等级较高,与Li、Nb和Ta浓度的增加相结合,表明了这一点。
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Rare metal pegmatites of the Cape Cross-Uis pegmatite belt, Namibia: geology, mineralisation, rubidium-strontium characteristics and petrogenesis

Rare metal pegmatites of the Cape Cross-Uis pegmatite belt (Namibia) containing sub-economic to economic concentrations of Sn, Nb, Ta, Li, occur in three main pegmatite swarms. Unzoned rare metal pegmatites are characterised by disseminated cassiterite mineralisation and varying Li, Ta and Nb concentrations, whereas zoned and poorly zoned pegmatites of the LI-rich rare metal type, beside low grade cassiterite mineralisation, contain higher Nb, Ta and Li concentrations (500 ppm Nb; 800 ppm Ta average). Occurrences of both types are confined to areas of extensive shearing in Pan-African greenschist facies metasediments within the tensional environment of a half-graben structure.

Rb/Sr isotope studies of various mineral phases in zoned and unzoned pegmatites in the study area indicate a late Pan-African emplacement age of 490 Ma for the pegmatitic melts. Petrogenetically, high 87Sr/86Sr initial ratios reflect partial melting of crustal material (basement rocks). Rare metal pegmatites in the study area are believed to have originated at the peak of regional metamorphism. This is indicated by higher metamorphic grades towards the Atlantic Ocean, which is combined with an increase in Li, Nb and Ta concentrations.

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