ISSN 1009-6248CN 61-1149/P 双月刊

主管单位:中国地质调查局

主办单位:中国地质调查局西安地质调查中心
中国地质学会

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    金川超大型铜镍矿床Ⅳ矿区矿体成因及成矿过程

    Genesis and Ore-Forming Process of the No.Ⅳ Intrusion of Jinchuan Super-Large Ni-Cu Magmatic Sulfide Deposit

    • 摘要: 金川矿床Ⅳ矿区位于矿床最东段,一直未开展过矿体成因及成矿过程研究,很大程度上制约了对金川矿床成矿模式及找矿潜力的全面认识。笔者在系统岩心编录及宏观地质特征对比基础上,开展电子探针、全岩主量和稀土微量元素、铂族元素等分析。获取Ⅳ矿区含矿岩体中橄榄石Fo值及Ni含量分别为78.3%~83.9%和660×10−62593×10−6。岩石主量元素变化特征表明,Ⅳ矿区主要发生了橄榄石和辉石的分离结晶作用。赋矿岩体略富集轻稀土元素,明显富集LILE而亏损HFSE;Ⅳ-1号矿体铂族元素含量明显低于24号、1号和2号矿体,其母岩浆成分中较低的铂族元素含量是造成矿体铂族元素偏低的主要因素。综合矿床地质特征、橄榄石成分及铂族元素特征,认为Ⅳ矿区含矿岩浆是沿独立中心侵位的产物,已控制部分应为岩浆演化较充分的端元,其深部可能仍有一定的找矿潜力。

       

      Abstract: The No. Ⅳ mining area, situated at the easternmost of the Jinchuan magmatic sulfide deposit, has not been previously investigated for its genesis and mineralization processes. This gap limited the understanding of the deposit's overall mineralization model and exploration potential. In this study, it's conducted systematic core logging and compared macroscopic geological features, incorporating analyses of electron probe data, whole-rock major and trace elements, and platinum-group elements (PGEs). Our results indicate that the olivine Fo values and Ni contents in the ore-bearing rocks of the No.Ⅳ mining area range from 78.3% to 83.9% and 660×10−6 to 2593×10−6, respectively. Variations in major element chemistry suggest that the No. Ⅳ area primarily underwent fractional crystallization of olivine and pyroxene. The ore-bearing bodies are slightly enriched in light rare earth elements (LREE) and significantly enriched in large-ion lithophile elements (LILE), while being depleted in high-field-strength elements (HFSE). The PGE content of the IV-1 ore body is notably lower than that of the No. 24, No. 1, and No. 2 ore bodies, with the relatively low PGE content in its host magma identified as the main contributing factor. A synthesis of the macroscopic geological features, olivine composition, and PGE characteristics leads to the conclusion that the No. IV mining area was formed by an independent intrusion of ore-bearing magma. While part of the deposit is controlled by relatively evolved end-member magma, deeper regions may still hold significant exploration potential.

       

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