南京大学学报(自然科学版) ›› 2018, Vol. 54 ›› Issue (2): 398.
迟 哲1,倪 培1*,廖剑锋2,范明森1,刘 政1,张 鑫1
Chi Zhe1,Ni Pei1*,Liao Jianfeng2,Fan Mingsen1,Liu Zheng1,Zhang Xin1
摘要: 温屋矿区位于紫金山矿田的北部,区内发育良好的火山机构. 深部的温屋斑岩体具有钾化、青磐岩化等蚀变,并具有网脉状矿化特征,但目前没有发现富矿体. 尝试对比贫矿的温屋斑岩体和区内与之同期的富矿罗卜岭斑岩体的岩石地球化学特征,探究影响其成矿的相关因素. 研究显示温屋斑岩体与罗卜岭斑岩体主量元素成分相似,并均具有亏损Nb,Ta,Ti等高场强元素和Eu异常不明显的特征. 但是温屋斑岩体具有显著的Sr亏损和较大的MREE/HREE特征,而罗卜岭斑岩体基本无Sr异常,MREE与HREE配分较小. 地球化学特征的差异可能反映了两者经历了不同的分离结晶过程. 温屋斑岩以斜长石的分离结晶为主;罗卜岭斑岩体斜长石的分离结晶被抑制并可能经历了角闪石的分离结晶,相对富水. 温屋斑岩体的相对贫水导致成矿元素难以在热液中富集,可能制约了温屋地区的成矿潜力. 但是,在火山机构附近裂隙发育,有利于富矿流体的集中,因此火山机构附近可以成为有利的成矿物质富集区域.
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