Neoproterozoic juvenile continental crust formation in the Arabian Shield (Khamal intrusive complex, Western Arabia)

IF 2.5 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Lithos Pub Date : 2026-03-01 Epub Date: 2026-01-24 DOI:10.1016/j.lithos.2026.108420
Davide Berno , Alessio Sanfilippo , Mattia Bonazzi , Avanzinelli Riccardo , Jakub Fedorik , Abdulkader M. Afifi
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引用次数: 0

Abstract

The Arabian–Nubian Shield (ANS) is one of the largest Neoproterozoic juvenile crustal provinces on Earth, providing insights into crustal growth, mantle dynamics, and continental assembly. The Wadi Khamal Complex, in the northwestern Arabian Shield, is a mafic intrusive body comprising a central anorthositic core and marginal gabbronorites, with subordinate granites and younger felsic to basaltic dykes. This study integrates petrography, whole-rock and mineral geochemistry, Sr–Nd–Pb isotopes, zircon UPb geochronology, and equilibrium-melt modeling from minerals to reconstruct the origin, age, and conditions of emplacement of this anorthosite complex.
In the complex, the anorthosites are dominated by cumulate plagioclase (An₈₁–₃₆) with interstitial pyroxenes, whereas gabbronorites exhibit modal layering and magmatic foliation defined by plagioclase–pyroxene (± olivine). The granites are in primary contact with anorthosite. The anorthosite–gabbronorite–granite association is crosscut by multiple generations of felsic dykes; additional basaltic dykes are attributed, by field relations and chemistry, to Cenozoic alkaline magmatism coeval with Red Sea rifting. The complex intrudes older arc-related lithologies—including amphibolitized mélanges and a voluminous diorite–tonalite–granodiorite batholith—that are structurally important but not petrogenetically related to Wadi Khamal.
Bulk-rock and mineral systematics define trends consistent with assembly of cumulate anorthosite and gabbronorite from tholeiitic parental melts; because the data are cumulate-dominated, bulk trends need not follow liquid lines of descent. Equilibrium-melt proxies indicate LREE-enriched tholeiitic melts lacking arc-type NbTa troughs, consistent with small to moderate degrees of partial melting of a juvenile (depleted to slightly enriched) mantle. Nd–Sr–Pb isotope signatures (εNd(i) = +4.5 to +6.1; 87Sr/86Sr(i) = 0.70256–0.70277; 26Pb/24Pb(i) = 17.3–17.9; 27Pb/24Pb(i) = 15.4–15.5; 28Pb/24Pb(i) = 36.2–37.2) indicate juvenile, non-arc mantle with limited crustal input. New zircon UPb dating yields an emplacement age of 614 ± 3.4 Ma.
We conclude that the Wadi Khamal Complex represents a small-scale, late Ediacaran massif-type anorthosite assembled as a crystal-mush from juvenile tholeiitic melts during post-collisional extension. The isotopic contrast between the intrusion and later basaltic dykes underscores a long-term shift from juvenile asthenosphere-dominated sources to enriched, SCLM-influenced sources during Red Sea rifting.
阿拉伯西部Khamal侵入杂岩——阿拉伯盾新元古代幼年大陆地壳的形成
阿拉伯-努比亚地盾(ANS)是地球上最大的新元古代幼年地壳省之一,为地壳生长、地幔动力学和大陆组合提供了见解。位于阿拉伯盾西北部的Wadi Khamal杂岩体是一个基性侵入岩体,由中心斜长岩心和边缘长辉长岩组成,下部有花岗岩和较年轻的长英质至玄武岩岩脉。本研究结合岩石学、全岩和矿物地球化学、Sr-Nd-Pb同位素、锆石UPb年代学和矿物平衡熔融模拟,重建了该斜长杂岩的起源、年龄和侵位条件。杂岩中斜长岩以堆积斜长石(An₈₁-₃₆)为主,含间隙辉石,辉长岩则以斜长石-辉长石(±橄榄石)为特征的模态分层和岩浆叶理作用。花岗岩主要与斜长岩接触。斜长岩-辉长岩-花岗岩组合被多代长英质岩脉横切;根据野外关系和化学性质,附加的玄武岩岩脉归因于与红海裂陷同期的新生代碱性岩浆活动。该杂岩侵入了更古老的与弧相关的岩性,包括角闪岩和大量闪长岩-闪长岩-花岗闪长岩岩基,它们在结构上很重要,但在岩石学上与Wadi Khamal无关。大块岩石和矿物系统定义了与来自拉斑岩母熔体的堆积斜长岩和辉长岩组合相一致的趋势;因为数据是累积的,所以整体趋势不需要跟随液体下降线。平衡熔体指标表明,富lree的拉斑熔体缺乏弧型NbTa槽,与幼期(贫至微富)地幔小至中等程度的部分熔融相一致。Nd-Sr-Pb同位素特征(εNd(i) = +4.5 ~ +6.1;87Sr/86Sr(i) = 0.70256-0.70277;2⁰6Pb/2⁰4Pb(i) = 17.3-17.9;2⁰7Pb/2⁰4Pb(i) = 15.4-15.5;2⁰8Pb/2⁰4Pb(i) = 36.2-37.2)表明幼年、非弧地幔,地壳输入有限。新锆石UPb定年结果显示其就位年龄为614±3.4 Ma。我们的结论是,Wadi Khamal杂岩代表了一个小规模的,晚埃迪卡拉纪的块状斜长岩,它是由碰撞后伸展时期的幼期拉斑岩熔体形成的晶体糊状组合而成的。侵入岩与后来的玄武岩岩脉之间的同位素对比强调了红海裂谷期间从幼年软流圈主导的来源向富集的、受scm影响的来源的长期转变。
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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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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