Zircon inheritance, sources of Devonian granitic magmas and crustal structure in central Victoria

IF 1.2 4区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY Australian Journal of Earth Sciences Pub Date : 2022-11-16 DOI:10.1080/08120099.2023.2139757
J. Clemens, G. Stevens, L. Coetzer
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引用次数: 2

Abstract

Abstract In central Victoria, inherited zircon in Devonian igneous rocks and detrital zircon in metasedimentary country rocks and an amphibolite-facies xenolith show that Mesoproterozoic parts of the underlying Selwyn Block cannot be the source for all the silicic magmas. Zircon inheritance in S-type samples reveals significant thermal events at 525–425 Ma and 1200–1100 Ma. Both S- and I-type samples have prominent zircon age peaks at 420–410 Ma, which record high-grade metamorphism of the deep crust during the terminal phases of the Benambran and Bindian orogenies. All I-type rocks have 650–500 Ma peaks, suggesting derivation from an arc-related metavolcanic source in the upper Selwyn Block. Protoliths of the greenschist-facies Ordovician metasediments and the amphibolite-facies Cambrian metasedimentary xenolith were deposited in distal backarc settings. Most inherited zircon cores are metamorphic, and the strongest zircon inheritance occurs in hornblende-bearing I-type rocks, highlighting their largely crustal origin. Zircon populations at ca 1400 Ma, thought to signal sediment derivation from East Antarctica and Rodinia-Nuna, are mostly absent in I-type samples and some S-types. The ca 1400 Ma signal probably applies to the upper, metasedimentary Selwyn Block, so Devonian S-type magmas were sourced mainly in the deeper sections. Zircon inheritance in the Devonian igneous rocks was not influenced by the exposed metasedimentary country rocks. Two samples from one of the smaller plutons have contrasting patterns of zircon inheritance, suggesting relatively small-scale source heterogeneity. Many rounded and corroded cores in zircon crystals yield the same ages as the crystallisation dates for the rocks, and thus are antecrysts. Higher whole-rock Zr contents generally correlate with higher proportions of inherited zircon, and differentiation does not affect this relationship. The degree of partial melting of a magma source and the efficiency of crystal entrainment are critical in governing zircon inheritance. KEY POINTS Mesoproterozoic sections of the Selwyn Block cannot be the sources for all the Devonian silicic magmas in central Victoria. I-type rocks have 650–500 Ma zircon age peaks, suggesting derivation from arc-related metavolcanic rocks in the upper Selwyn Block. Hornblende-bearing I-type rocks have the strongest zircon inheritance patterns, indicating the largely crustal origins of I-type magmas. Exposed metasedimentary country rocks were not involved in magma genesis.
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维多利亚中部地区的锆石继承、泥盆纪花岗质岩浆来源及地壳结构
摘要在维多利亚州中部,泥盆纪火成岩中的继承锆石、变质沉积围岩中的碎屑锆石和角闪岩相捕虏体表明,下伏Selwyn地块的中元古代部分不可能是所有硅化岩浆的来源。S型样品中的锆石继承揭示了525–425年的重大热事件 Ma和1200–1100 Ma。S型和I型样品在420–410处都有显著的锆石年龄峰值 Ma,记录了本南布拉和宾甸造山运动末期深地壳的高级变质作用。所有I型岩石都有650–500 马峰,表明其来源于塞尔温地块上部与弧有关的变质火山源。绿片岩相奥陶世变质沉积的原岩和角闪岩相寒武纪变质沉积的捕虏体沉积在远弧后环境中。大多数继承的锆石岩芯是变质的,最强烈的锆石继承发生在含角闪石的I型岩石中,突出了它们主要的地壳起源。锆石数量约1400 Ma被认为是来自南极洲东部和Rodinia Nuna的沉积物来源的信号,在I型样品和一些S型样品中大多不存在。约1400 Ma信号可能适用于上部变质沉积的Selwyn地块,因此泥盆纪S型岩浆主要来源于较深的剖面。泥盆纪火成岩中锆石的继承不受裸露变质沉积围岩的影响。其中一个较小深成岩体的两个样本具有对比鲜明的锆石继承模式,表明相对小规模的来源非均质性。锆石晶体中许多圆形和腐蚀的岩芯产生的年龄与岩石的结晶日期相同,因此是前驱体。较高的全岩Zr含量通常与较高比例的继承锆石相关,而分异并不影响这种关系。岩浆源的部分熔融程度和晶体夹带效率是控制锆石继承的关键。要点Selwyn地块的中元古代部分不可能是维多利亚中部所有泥盆纪硅化岩浆的来源。I型岩石有650–500个 Ma锆石年龄达到峰值,表明其来源于塞尔温地块上部的弧相关变质火山岩。含角闪石的I型岩石具有最强的锆石继承模式,表明I型岩浆主要起源于地壳。裸露的变质沉积围岩不参与岩浆成因。
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来源期刊
Australian Journal of Earth Sciences
Australian Journal of Earth Sciences 地学-地球科学综合
CiteScore
2.80
自引率
8.30%
发文量
45
审稿时长
6-12 weeks
期刊介绍: Australian Journal of Earth Sciences publishes peer-reviewed research papers as well as significant review articles of general interest to geoscientists. The Journal covers the whole field of earth science including basin studies, regional geophysical studies and metallogeny. There is usually a thematic issue each year featuring a selection of papers on a particular area of earth science. Shorter papers are encouraged and are given priority in publication. Critical discussion of recently published papers is also encouraged.
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