Late Variscan tectonic orogenic collapse as a trigger for Sn-W mineralizing systems. U-Pb ore geochronology across the Martinamor gneissic dome (Salamanca, Spain)

IF 3.2 2区 地球科学 Q1 GEOLOGY
Daniel Bermejo , Lorena Ortega , Santos Barrios Sánchez , Lorenzo Tavazzani , Pedro Castiñeiras , Cyril Chelle-Michou , Elena Crespo , Kelvin dos Santos Alves , Juan Gómez-Barreiro
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Abstract

Regional tectonothermal evolution is a primary factor for many mineral deposits formation. Late orogenic gravitational collapse has been widely recognized across different orogens, including the Variscan belt. The Martinamor gneissic dome is a well constrained structure related to the late-Variscan orogenic collapse in the Iberian Massif. We have investigated Sn-W mineralization spatially related to the Martinamor dome by LA-ICP-MS U-Pb dating of cassiterite and wolframite, revealing a wide mineralization timespan of 40 Myr. Our results show: a) an early (338.1 ± 5.8 Ma), minor mineralization phase, (W-dominated), potentially related to Variscan compressive phases; b) a second, major stage which lasted from 324.1 ± 5.9 to 300.7 ± 5.4 Ma, which includes Sn-bearing pegmatites and Sn-W veins formed under the syn-collisional extensional collapse. Structural evidence highlights the role of extensional detachments in channeling mineralizing fluids and creating suitable traps under ductile and ductile–brittle conditions; it also explains the temporal and spatial distribution of the Sn-W vein-type mineralizations in the zone.
Comparisons with other Variscan deposits in the Iberian Massif and European counterparts suggest a regional metallogenic cycle linked to late-Variscan extensional collapse, heat advection, and crustal partial melting processes. These findings underscore the Martinamor dome as a unique structure recording a protracted Variscan tectono-magmatic-metallogenic event, with implications for understanding Sn-W deposit formation in orogenic settings.

Abstract Image

晚期瓦里斯坎构造造山崩塌是锡-钨成矿系统的触发因素。西班牙萨拉曼卡Martinamor片麻岩圆顶U-Pb矿石地质年代学
区域构造热演化是许多矿床形成的主要因素。晚造山带的重力坍缩已在不同的造山带中得到了广泛的认识,包括瓦里斯坎带。马蒂纳莫片麻岩穹窿是伊比利亚地块中与晚瓦里西斯造山崩塌有关的约束良好的构造。通过对锡石和黑钨矿进行LA-ICP-MS U-Pb测年,研究了与Martinamor穹窿相关的Sn-W矿化空间特征,发现其成矿时间跨度为40 Myr。结果表明:a)早期(338.1±5.8 Ma)小矿化期,以w为主,可能与Variscan压缩期有关;b)第二主要阶段(324.1±5.9 ~ 300.7±5.4 Ma),主要发育含锡伟晶岩和Sn-W脉,形成于同碰撞伸展坍缩期。构造证据强调了伸展分离在延性和延性-脆性条件下引导矿化流体并形成合适圈闭的作用;解释了该区Sn-W脉型矿化的时空分布。与伊比利亚地块和欧洲同类Variscan矿床的比较表明,区域成矿旋回与晚期Variscan伸展塌陷、热平流和地壳部分熔融过程有关。这些发现强调了Martinamor穹窿是一个独特的构造,记录了一个漫长的Variscan构造-岩浆-成矿事件,对了解造山环境下的锡钨矿床形成具有重要意义。
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来源期刊
Ore Geology Reviews
Ore Geology Reviews 地学-地质学
CiteScore
6.50
自引率
27.30%
发文量
546
审稿时长
22.9 weeks
期刊介绍: Ore Geology Reviews aims to familiarize all earth scientists with recent advances in a number of interconnected disciplines related to the study of, and search for, ore deposits. The reviews range from brief to longer contributions, but the journal preferentially publishes manuscripts that fill the niche between the commonly shorter journal articles and the comprehensive book coverages, and thus has a special appeal to many authors and readers.
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