Metasandstones of the Vilenga Formation of the Vetrenyi Belt: Composition, Isotopic–Geochronological Characteristic, and Provenances

IF 0.7 4区 地球科学 Q4 GEOSCIENCES, MULTIDISCIPLINARY
S. V. Mezhelovskaya, E. V. Asafov, A. N. Koshlyakova, D. P. Tobelko, A. D. Mezhelovsky, A. V. Sobolev
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Abstract

Two primary and two subordinate age groups of detrital zircons are distinguished as a result of isotopic–geochronological studies of metasandstones of the Vilenga Formation of the Vetrenyi Belt. A zircon group with an age of 2751 ± 7 Ma was potentially sourced from late granitoids (granodiorite–granite–leucogranites) abundant in the northern part of the Vodlozero domain. No source with an age of 2823 ± 5 Ma has been identified in the adjacent part of the Karelian granite–greenschist area. The zircons with the age of 2874 Ma were sourced from rocks of the BADR (basalt–andesite–dacite–rhyolite) series and adakites of the Sumozero–Kenozero greenschist belt. Previous study of detrital zircon from basal horizons of sections of the Vetrenyi Belt (Toksha Formation), as well as the underlying rocks for the metasandstones (Kozhozero Formation), showed the same main age peaks, which may indicate a stable tectonic setting at the beginning of the Paleoproterozoic and a common provenance of clastic material. Intermediate–felsic rocks with an age of 2940 Ma could also have made a small contribution in the formation of metasandstones.

Abstract Image

维特雷尼带维伦加地层的金属砂岩:成分、同位素地质年代特征和产地
摘要通过对 Vetrenyi 地带 Vilenga Formation 的元砂岩进行同位素-地质电子学研究,区分出了两个主要和两个次要的锆石碎片年龄组。年龄为 2751 ± 7 Ma 的锆石组可能来自 Vodlozero 地区北部丰富的晚期花岗岩(花岗闪长岩-花岗闪长岩-白花岗岩)。在卡累利阿花岗岩-片麻岩地区的邻近地区,没有发现年龄为 2823 ± 5 Ma 的锆石来源。年龄为 2874 Ma 的锆石来自苏莫泽罗-基诺泽罗绿斜岩带的 BADR(玄武岩-安山岩-黑云母-流纹岩)系列岩石和闪长岩。此前对维特伦伊带(托克沙构造)剖面基底地层以及玄武岩(科佐泽罗构造)底层岩石中的锆英石进行的研究显示出相同的主要年龄峰值,这可能表明在古近纪初有一个稳定的构造环境以及碎屑物质的共同来源。年龄为 2940 Ma 的中熔岩也可能在元砂岩的形成过程中起到了微小的作用。
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来源期刊
Doklady Earth Sciences
Doklady Earth Sciences 地学-地球科学综合
CiteScore
1.40
自引率
22.20%
发文量
138
审稿时长
3-6 weeks
期刊介绍: Doklady Earth Sciences is a journal that publishes new research in Earth science of great significance. Initially the journal was a forum of the Russian Academy of Science and published only best contributions from Russia. Now the journal welcomes submissions from any country in the English or Russian language. Every manuscript must be recommended by Russian or foreign members of the Russian Academy of Sciences.
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