Petrogenesis of potassic granite suites along the southern margin of the Zimbabwe Craton

IF 1.2 4区 地球科学 Q2 GEOLOGY South African Journal of Geology Pub Date : 2023-03-01 DOI:10.25131/sajg.126.0004
G. Chagondah, A. Hofmann, M. Elburg, L. Iaccheri, J. Kramers, A. Wilson
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引用次数: 1

Abstract

An integrated approach embracing field studies, petrographic and geochemical investigations together with zircon U-Pb-Hf data was used to investigate the petrogenesis of potassic granite suites along the southern margin of the Zimbabwe Craton. Zircon U-Pb geochronology identifies age relationships, revealing coeval magmatism of the ca. 2 635 ± 5 to 2 625 ± 3 Ma Chilimanzi Suite, and the ca. 2 627 ± 7 Ma Razi Suite. Both suites represent syn- to late-tectonic, high-K, calc-alkaline, and metaluminous to weakly peraluminous granites and granodiorites with I-type affinity. The granite suites contain xenocrystic zircons, with the Chikwanda Pluton of the Chilimanzi Suite yielding a grain of up to 3 206 Ma old. Both granite suites exhibit eHf values of between -5.6 ± 1.3 and -7.3 ± 1.6 and TDM model ages of ca. 3.4 to 3.5 Ga which suggests a similar crustal source. The unradiogenic zircon Hf isotopic compositions are consistent with formation of the granite suites through partial melting of pre-existing crustal protoliths, including Palaeoarchaean tonalite-trondhjemite-granodiorites (TTGs) of the Zimbabwe proto-craton. Partial melting of lower crust gave rise to granitic melts that became emplaced over a relatively short time interval from 2 635 to 2 625 Ma and heralded the stabilisation of the Zimbabwe Craton. In addition to virtually identical ages, the Razi and Chilimanzi suites have similar geochemistry. Small geochemical differences between the Chilimanzi and the Razi suites are attributed to the crustal level at which they are preserved, the modal mineralogy and the extent to which the melts are evolved. The Razi Suite melts were generated from lower crust partial melting of thickened charnockite-enderbite source rocks rich in heat producing elements. The partial melting occurred under fluid-absent conditions and magmas were emplaced at lower to mid crustal levels. The Chilimanzi Suite magmas were similarly derived by the partial melting of TTG lower crust and were emplaced at upper crustal levels. Accordingly, the Chilimanzi Suite exhibits more evolved magmatic fractionation indices indicated by high Rb/Sr, as well as low K/Rb ratios relative to the Razi Suite. Both suites reveal varying degrees of enrichment in incompatible elements including Rb, Th, and U, as well simultaneous depletions in Ba, Sr, and Hf which underscores the role of fractional crystallisation in the evolution of the granitic magmas.
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津巴布韦克拉通南缘钾质花岗岩套的岩石成因
采用野外考察、岩石学和地球化学调查以及锆石U-Pb-Hf数据相结合的方法,研究了津巴布韦克拉通南缘钾质花岗岩套的岩石成因。锆石U-Pb年代学确定了时代关系,揭示了约2 635±5 ~ 2 625±3马赤里曼子组和约2 627±7马拉兹组的岩浆活动同期。这两套花岗岩和花岗闪长岩均为同构造-晚构造、高钾、钙碱性、铝质-弱过铝花岗岩和花岗闪长岩,具有i型亲和关系。花岗岩组含有异晶锆石,其中奇里曼兹组的奇克旺达岩体的锆石颗粒高达3 206 Ma。两个花岗岩组的eHf值均在-5.6±1.3 ~ -7.3±1.6之间,TDM模式年龄约为3.4 ~ 3.5 Ga,表明它们具有相似的地壳来源。非放射性成因的锆石Hf同位素组成与津巴布韦原克拉通古太古代闪长岩(TTGs)等原有地壳原岩部分熔融形成的花岗岩套相一致。下地壳的部分熔融产生了花岗岩熔体,这些花岗岩熔体在相对较短的时间间隔(2635 - 2625 Ma)内就位,预示着津巴布韦克拉通的稳定。除了年龄几乎相同之外,Razi组和Chilimanzi组具有相似的地球化学特征。Chilimanzi组和Razi组在地球化学上的微小差异归因于它们保存的地壳水平、矿物学模式和熔体演化的程度。拉孜套熔体是由富含产热元素的增厚绿绿岩-深黑岩烃源岩下地壳部分熔融形成的。部分熔融发生在无流体条件下,岩浆位于地壳中低水平。赤里曼子套岩浆同样是由TTG下地壳的部分熔融产生的,并位于地壳的上水平。因此,赤里曼子岩浆岩分选指标相对于拉子岩浆岩组表现为较高的Rb/Sr和较低的K/Rb。两套岩浆岩中Rb、Th、U等不相容元素均有不同程度的富集,Ba、Sr、Hf等元素也有不同程度的富集,说明了分馏结晶在花岗岩岩浆演化过程中的作用。
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来源期刊
CiteScore
3.60
自引率
5.60%
发文量
18
审稿时长
>12 weeks
期刊介绍: The South African Journal of Geology publishes scientific papers, notes, stratigraphic descriptions and discussions in the broadly defined fields of geoscience that are related directly or indirectly to the geology of Africa. Contributions relevant to former supercontinental entities such as Gondwana and Rodinia are also welcome as are topical studies on any geoscience-related discipline. Review papers are welcome as long as they represent original, new syntheses. Special issues are also encouraged but terms for these must be negotiated with the Editors.
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