Polyphased rare-element magmatism during late orogenic evolution: geochronological constraints from NW Variscan Iberia

J. Melleton, E. Gloaguen, D. Frei, A. Lima, R. Vieira, T. Martins
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引用次数: 1

Abstract

Rare-element granites and pegmatites represent important sources of raw materials for “clean, green and high technologies”, such as lithium and tantalum, for example. However, mechanisms of rare-element granites and pegmatite’s origin are still far from being fully understood. Several rare-element pegmatite fields and a rare-element granite are known in the Variscan realms located in Iberia (Spain and Portugal), enhancing the interest of this area for studying the formation of these extremely fractionated melts. In situ U-Pb dating by LA-SF-ICP-MS of columbite-group minerals from rare-element granites and pegmatites of the Iberian Variscan belt provides new constraints on the generation of rare-element melts. Three events have been recognized: (i) Emplacement of the Argemela rare-element granite, in the Central Iberian Zone (CIZ), with an age of 326 ± 3 Ma; (ii) Emplacement of rare-element pegmatites from the Galicia-Trás-os-Montes Zone (GTOMZ), at an average age of 310 ± 5 Ma; (iii) Emplacement of rare-element pegmatites in the CIZ and in the southern GTOMZ at about 301 ± 3 Ma. These two last events are coeval with the two peaks of ages for the late orogenic magmatism at ca. 308 Ma and 299 Ma, and all dated rare-element pegmatites clearly emplaced during the late-orogenic evolution of the Variscan belt. Contemporaneous fields of rare-element pegmatites are arranged in belts following those formed by similar granitoid suites. Pegmatite fields from both the GTOMZ and the CIZ reveal a southward propagation of ages of emplacement, which matches the observed propagation of deformation, metamorphism and magmatism in the two different geotectonic zones. Existence of three successive rare-element events in the Iberian Massif argues against the involvement of lower crustal HP-HT metamorphism in the generation of rare-element melts. Possible sources of rare-element-enriched melts are more likely located in the middle to upper crust, as are the major components of granitic magmatism. Analyses of U and Pb isotopes from columbite-group minerals are very robust and reproducible, making them good candidates for dating ore deposits related to peraluminous magmatism as well as REE- and Nb-bearing deposits.
晚造山带演化中的多相稀有元素岩浆作用:来自伊比利亚西北部瓦里斯坎的地质年代学约束
稀有元素花岗岩和伟晶岩是“清洁、绿色和高科技”的重要原料来源,例如锂和钽。然而,稀土花岗岩和伟晶岩的成因机制还远未完全了解。在伊比利亚(西班牙和葡萄牙)的Variscan地区已知几个稀有元素伟晶岩田和一个稀有元素花岗岩,增强了该地区研究这些极端分异熔体形成的兴趣。利用LA-SF-ICP-MS对伊比利亚瓦里斯坎带稀有元素花岗岩和伟晶岩中的柱状岩群矿物进行原位U-Pb测年,为稀有元素熔体的生成提供了新的约束条件。已经确认了三个事件:(i)在中部伊比利亚地区(CIZ)发现了Argemela稀有元素花岗岩,年龄为326±3 Ma;(ii) Galicia-Trás-os-Montes带(GTOMZ)稀有元素伟晶岩就位,平均年龄为310±5 Ma;(iii)在约301±3 Ma时,稀有元素伟晶岩在离岛区和离岛区南部就位。这两个事件与晚造山岩浆活动的两个年龄高峰(约308 Ma和299 Ma)是同步的,所有的稀有元素伟晶岩的年代都明显是在晚造山演化时期形成的。同时期的稀有元素伟晶岩田呈带状排列,紧随着类似花岗岩系形成的田。GTOMZ和CIZ的伟晶岩场均显示侵位年龄向南扩展,这与两个不同大地构造带观测到的变形、变质和岩浆活动的扩展相吻合。伊比利亚地块连续三次稀有元素事件的存在,反驳了下地壳高温-高温变质作用参与了稀有元素熔体的形成。富稀有元素熔体的可能来源更可能位于地壳中上,这是花岗岩岩浆活动的主要组成部分。对柱状岩群矿物中U和Pb同位素的分析非常可靠且可重复,使其成为与过铝岩浆作用有关的矿床以及含REE和nb矿床定年的良好候选者。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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