Detrital zircon provenance of the Archean Moodies Group, Barberton Greenstone Belt, South Africa and Eswatini

IF 1.9 3区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY American Journal of Science Pub Date : 2022-02-01 DOI:10.2475/02.2022.01
C. Heubeck, N. Drabon, G. Byerly, Isabelle Leisgang, U. Linnemann, D. Lowe, R. Mertz‐Kraus, Alejandra Gonzalez-Pinzón, T. Thomsen, A. Zeh, Y. Rojas‐Agramonte, A. Kröner
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引用次数: 2

Abstract

Sandstones of the 3.22 Ga Archean Moodies Group represent one of the world's oldest quartz-rich sedimentary sequences. The provenance of this unit is unresolved because its quartz and common microcline can be sourced both from either now eroded or covered granitoid plutons outside the Barberton Greenstone Belt (BGB) or, alternatively and perhaps more controversially, (rhyo-)dacitic (sub-)volcanic rocks within the BGB. We compiled 31 detrital zircon data sets (n = 2588) from sandstones, reworked tuffs and conglomerate of the Moodies Group in order to constrain its age and provenance. After selection using quality criteria, the remaining zircons (n = 1621) in nearly all samples show a distribution corresponding to the four known major pulses of felsic magmatism in the BGB: 1) the ca. 3550 to 3530 Ma Theespruit and Sandspruit Formations at the base of the Onverwacht Group; 2) the ca. 3440 to 3410 Ma rhyo-dacites of the upper Hooggenoeg Formation, Onverwacht Group; 3) the ca. 3300 to 3280 Ma thin felsic tuffs in the Mendon Formation; and 4) the ca. 3260 to 3215 Ma felsic volcanic and shallow intrusive rocks of the Auber Villiers, Bien Venue and Schoongezicht Formations of the upper Fig Tree Group and the Moodies Group as well as their co-magmatic plutonic counterparts. Almost all data sets also contain near-concordant younger zircons as young as 2820 Ma, which can be attributed to one of six tectonic or magmatic events affecting the young Kaapvaal Craton in post-BGB time, causing the partial or complete resetting of the U-Pb system in some grains. The youngest (near-)concordant zircon clusters yield ages of ca. 3220 Ma in most locations, and the youngest discordant group of zircons from a reworked tuff near the top of the Moodies Group at 3212 ± 13 Ma agrees well with previous estimates of the maximum depositional age. With very few exceptions, the oldest zircons (ca. 3564 Ma) are only slightly older than the oldest rocks in the BGB stratigraphy (ca. 3550 Ma). Subtle regional and stratigraphic differences in age spectra may indicate localized or nearby sediment sources within a synorogenic setting. Preliminary age spectra along vertical stratigraphic profiles show little systematic variation, possibly indicating that intrabasinal recycling was dominant over considerable time periods of the basin's evolution. Extra-basinal plutonic sources of similar age and composition as the intra-BGB sources appear to be required to provide quartz and some feldspar to Moodies Group sandstones, although zircon age spectra, limited zircon Hf isotope data, sandstone petrography, facies analysis, and the high variability in Moodies conglomerate clast composition are consistent with uplift, deformation and erosion of several intra-BGB sources, but in particular from the region of the Onverwacht Anticline. Zircon populations, conglomerate clasts, and sandstone composition show no evidence that high-grade metamorphic rocks from the adjacent Ancient Gneiss Complex (AGC) contributed significantly to the Moodies Group.
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南非巴伯顿绿岩带、南非和斯瓦蒂尼太古宙穆迪群碎屑锆石物源
3.22 Ga太古宙穆迪群的砂岩代表了世界上最古老的富含石英的沉积序列之一。该单元的来源尚未确定,因为其石英和常见的微斜长石既可以来源于Barberton Greenstone Belt(BGB)外现已被侵蚀或覆盖的花岗质深成岩体,也可以来源于BGB内的(rhyo-)英安质(亚)火山岩。我们从穆迪组的砂岩、改造凝灰岩和砾岩中汇编了31个碎屑锆石数据集(n=2588),以限制其年龄和物源。在使用质量标准进行选择后,几乎所有样品中的剩余锆石(n=1621)显示出与BGB中长英质岩浆作用的四个已知主脉冲相对应的分布:1)Onverwacht群底部的约3550至3530 Ma Theespruit和Sandspruit组;2) Onverwacht群Hooggenoeg组上部的约3440至3410 Ma rhyo英安岩;3) Mendon组中约3300至3280 Ma的薄长英质凝灰岩;和4)上部无花果树群和穆迪群的Auber Villiers、Bien Venue和Schongezicht组的约3260至3215 Ma长英质火山岩和浅侵入岩,以及它们的同岩浆深成岩对应物。几乎所有的数据集都包含年龄为2820 Ma的近乎一致的年轻锆石,这可归因于后BGB时期影响年轻Kaapvaal火山口的六个构造或岩浆事件之一,导致一些颗粒中的U-Pb系统部分或完全重置。最年轻(接近)的一致锆石群在大多数位置产生的年龄约为3220 Ma,最年轻的不一致锆石群来自穆迪群顶部附近的改造凝灰岩,在3212±13 Ma,与之前对最大沉积年龄的估计非常一致。除了极少数例外,最古老的锆石(约3564 Ma)仅比BGB地层中最古老的岩石(约3550 Ma)略老。年龄谱中细微的区域和地层差异可能表明同造山带环境中的局部或附近沉积物来源。沿垂直地层剖面的初步年龄谱显示出很少的系统变化,这可能表明在盆地演化的相当长的一段时间内,盆地内的再循环占主导地位。尽管锆石年龄谱、有限的锆石Hf同位素数据、砂岩岩石学、相分析以及穆迪砾岩碎屑组成的高度变异性与隆起一致,但似乎需要与BGB内部来源具有相似年龄和成分的盆地外深成岩体来源来为穆迪群砂岩提供石英和一些长石,几个BGB内部源的变形和侵蚀,特别是来自Onverwacht背斜区域的。锆石种群、砾岩碎屑和砂岩成分没有证据表明邻近古片麻岩杂岩(AGC)的高级变质岩对穆迪群有重大贡献。
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来源期刊
American Journal of Science
American Journal of Science 地学-地球科学综合
CiteScore
5.80
自引率
3.40%
发文量
17
审稿时长
>12 weeks
期刊介绍: The American Journal of Science (AJS), founded in 1818 by Benjamin Silliman, is the oldest scientific journal in the United States that has been published continuously. The Journal is devoted to geology and related sciences and publishes articles from around the world presenting results of major research from all earth sciences. Readers are primarily earth scientists in academia and government institutions.
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