墨西哥杜兰戈Velardeña矿区始新世Santa María和Antares Zn-Pb(-Ag)矽卡岩矿床的成矿模式

IF 4.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Néstor Cano, Antoni Camprubí, Eduardo González-Partida, Ana K. González-Ambrocio, Pura Alfonso, Daniel P. Miggins, Edith Fuentes-Guzmán, Edith Cienfuegos-Alvarado, Alexander Iriondo
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引用次数: 0

摘要

Velardeña矿区的Santa María和Antares Zn-Pb(-Ag)矽卡岩矿床位于墨西哥中西部。它们沿着渐新世长英质侵入体和白垩纪石灰岩之间的接触面相距470米,在前进、后退、矿石后(Santa María)和晚期发育。首先,前进阶段是由 ~ 600°C和15wt%NaCl当量,由石榴石组成 + 硅灰石 ± 单斜辉石和黑云母 ± 钾长石组合。其次,逆行/成矿阶段是由300–500°C、盐度为20–30 wt%CaCl2(Santa María)和 >; 40wt%NaCl当量(Antares)。它包括绿泥石、角闪石、绿帘石、方解石、方星石、石英、绢云母、阿杜拉石、萤石和白云母的组合,与闪锌矿、黄铁矿、方铅矿、磁黄铁矿、毒砂、黄铜矿和Pb-Bi-Sb硫盐有关。第三,成矿后阶段是由 ~ 400°C和20–30 wt.%CaCl2,包括矿化不良的方解石脉。第四,晚期是由 <; 300°C和20-30 wt.%CaCl2(Santa María) ~ 15wt%NaCl当量(Antares),以及结晶的四面体矿物和黄铁矿 + marcasite。δ18之间的流体 ~ Santa María和之间的14‰和23‰ ~ 心宿二的12‰和17‰显示出对心宿二矿化流体的较少修改的岩浆亲和力;δ13在0‰和-6‰之间的流体记录了沉积C的再循环。此外,δ34SVCDT在-3‰和2‰之间的硫化物揭示了S的岩浆源。总之,这些数据表明,在Santa María,岩浆衍生的流体与围岩积极相互作用,而在Antares,流体-岩石相互作用较温和。在这两个矿床中,金属沉积是由含矿流体与碳酸盐岩的冷却和中和引发的。我们的阿杜拉纪40Ar/39Ar年龄约为37.5 Ma,矿床位于墨西哥中部-西北部的始新世-中新世早期成矿时代,在此期间,其他世界级的矽卡岩超热液系统被侵位(例如,Concepción del Oro和Mazapil Peñasquito)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Metallogenic model of the Eocene Santa María and Antares Zn-Pb(-Ag) skarn deposits, Velardeña Mining District, Durango, Mexico

The Santa María and Antares Zn-Pb(-Ag) skarn deposits in the Velardeña Mining District are located in central–NW Mexico. They lie 470 m apart along the contact between Oligocene felsic intrusions and Cretaceous limestones, and were developed during prograde, retrograde, post-ore (Santa María), and late stages. Firstly, the prograde stage was formed by fluids at ~ 600 °C and 15 wt% NaCl equiv., and consists of garnet + wollastonite ± clinopyroxene and biotite ± K-feldspar assemblages. Secondly, the retrograde/ore stage was formed by fluids at 300–500 °C with salinities of 20–30 wt% CaCl2 (Santa María) and > 40 wt% NaCl equiv. (Antares). It comprises assemblages of chlorite, amphibole, epidote, calcite, scapolite, quartz, sericite, adularia, fluorite, and muscovite associated with sphalerite, pyrite, galena, pyrrhotite, arsenopyrite, chalcopyrite, and Pb-Bi-Sb sulfosalts. Thirdly, the post-ore stage was formed by fluids at ~ 400 °C and 20–30 wt.% CaCl2 and comprises poorly mineralized calcite veins. Fourthly, the late stage was formed by fluids at < 300 °C and 20–30 wt.% CaCl2 (Santa María) and ~ 15 wt% NaCl equiv. (Antares), and crystallized tetrahedrite-group minerals and pyrite + marcasite. δ18Ofluid between ~ 14‰ and 23‰ at Santa María and between ~ 12‰ and 17‰ at Antares show a less-modified magmatic affinity for mineralizing fluids at Antares; δ13Cfluid between 0‰ and –6‰ register recycling of sedimentary C. Moreover, sulfides with δ34SVCDT between –3‰ and 2‰ reveal a magmatic source for S. Altogether, these data suggest that, at Santa María, magmatic-derived fluids actively interacted with the wall rocks, whereas at Antares the fluid-rock interaction was milder. In both deposits, metal deposition was triggered by the cooling and neutralization of ore-bearing fluids with carbonate rocks. Our 40Ar/39Ar dates for adularia of ca. 37.5 Ma place the deposits within the Eocene–early Miocene metallogenetic epoch of central–NW Mexico, during which other world-class skarn-epithermal systems were emplaced (e.g., Concepción del Oro and Mazapil-Peñasquito).

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来源期刊
Mineralium Deposita
Mineralium Deposita 地学-地球化学与地球物理
CiteScore
11.00
自引率
6.20%
发文量
61
审稿时长
6 months
期刊介绍: The journal Mineralium Deposita introduces new observations, principles, and interpretations from the field of economic geology, including nonmetallic mineral deposits, experimental and applied geochemistry, with emphasis on mineral deposits. It offers short and comprehensive articles, review papers, brief original papers, scientific discussions and news, as well as reports on meetings of importance to mineral research. The emphasis is on high-quality content and form for all articles and on international coverage of subject matter.
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