吉林大学学报(地球科学版) ›› 2016, Vol. 46 ›› Issue (6): 1711-1723.doi: 10.13278/j.cnki.jjuese.201606110
程文斌1,2, 尹力3, 陈翠华1,2, 宋玉坤4, 李关清5, 张兴国5, 夏抱本5, 达瓦次仁5
Cheng Wenbin1,2, Yin Li3, Chen Cuihua1,2, Song Yukun4, Li Guanqing5, Zhang Xingguo5, Xia Baoben5, Dawa Ciren5
摘要: 西藏柯月Pb-Zn-Sb-Ag多金属矿床位于雅鲁藏布江缝合带(IYS)与藏南拆离系(STDS)之间的北喜马拉雅成矿带。该矿床经详查验证,4 300 m以浅的矿体赋存于日当组钙质板岩夹薄层泥晶灰岩中,严格受北东向断裂控制,但深部延伸不明。本文通过该矿床I号矿体原生晕地球化学特征分析,对此问题进行初步探讨。研究表明,前缘晕元素为Hg、As、Tl,近矿晕元素为Pb、Zn、Sb、Ag、Au、Cd、Cu、Mn,尾晕元素为Sn、In、Bi;采用改良的格里戈良分带指数法计算分带序列为In-Mn-As-Cu-Zn-Cd-Bi-Pb-Sn-Hg-Tl-Ag-Au-Sb,重心法计算分带序列为In-Mn-As-Cu-Cd-Zn-Hg-Bi-Sn-Pb-Ag-Sb-Tl-Au;同时,讨论原生晕地球化学参数变化规律,并以各元素的几何平均值累乘比建立矿体的剥蚀参数模型及矿体原生晕叠加理想模型。综合以上分析,推测矿床有多次成矿作用叠加,上部存在剥蚀至尾部的矿体,而深部可能有矿体延伸。
中图分类号:
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