TIME CONSTRAINTS ON THE FORMATION OF THE KANDALAKSHA AND KERETSK GRABENS OF THE WHITE SEA PALEO-RIFT SYSTEM FROM NEW ISOTOPIC GEOCHRONOLOGICAL DATA

Pub Date : 2021-09-17 DOI:10.5800/gt-2021-12-3-0540
N. Kuznetsov, A. Baluev, E. N. Terekhov, S. Kolodyazhnyi, E. S. Przhiyalgovskii, T. Romanyuk, A. S. Dubensky, V. Sheshukov, S. Lyapunov, T. Bayanova, P. Serov
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引用次数: 1

Abstract

Initially, the age and stratigraphic position of the Tersk formation were determined with respect to the fact that this formation overlaps the Early Proterozoic granitoids. Its top was marked by the rocks penetrated by the Late Devonian alkaline intrusions, including explosion pipes.This article presents the U-Pb isotopic dating of detrital zircon grains (dZr) from sandstones of the Tersk formation. It describes the geochemical compositions of the rocks and the Sm-Nd study results. In our study, the weighted average age of four youngest dZr grains from the sandstones of the Tersk formation is 1145±20 Ma, which suggests that the rocks above the studied rock layer (see the Tersk formation cross-section) are is not older than the end of the Middle Riphean. The U-Pb isotopic ages of dZr grains (provenance signals) from the sandstones of the Tersk formation were compared to the ages of other Upper Precambrian clastic strata in the northeastern East European platform (EEP) and adjacent areas. Our comparative analysis shows that these rocks significantly differ in age. This conclusion is in good agreement with the idea that at the end of the Middle and during the Late Riphean, several small (mainly closed) basins separated by uplifts dominated in the paleogeographic setting of the area wherein the White Sea rift system (WSRS) formed and developed. Temporal connections of these basins with the ocean were possible. Such paleogeographic setting does not favour the development of large rivers; this is why the grabens are mainly filled with local rock materials. The Keretsk and Kandalaksha grabens (WSRS) are filled with marine sediments eroded from the grabens walls. The local sediment sources include eclogite complexes (~1.9 Ga), which basic magmatism is dated at ~2.4–2.5 and ~2.7–2.9 Ga. Any potential primary sources for dZr grains are lacking in the area near the Keretsk graben. We suggest that such grains occurred due to recycling of the secondary sources of zircon, i.e. originated from ancient local sedimentary formations.
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新同位素年代学资料对白海古裂谷系坎达拉沙和克列茨克地堑形成的时间约束
最初,Tersk组的年龄和地层位置是根据该组与早元古代花岗岩类重叠的事实确定的。其顶部的标志是晚泥盆世碱性侵入物穿透的岩石,包括爆炸管。本文介绍了特尔斯克组砂岩碎屑锆石颗粒(dZr)的U-Pb同位素定年。介绍了岩石的地球化学组成和Sm-Nd的研究结果。在我们的研究中,Tersk组砂岩中4个最年轻的dZr颗粒的加权平均年龄为1145±20 Ma,这表明所研究的岩层(见Tersk组截面)上方的岩石年龄不超过中Riphean末期。将Tersk组砂岩中dZr颗粒(物源信号)的U-Pb同位素年龄与东欧地台东北部及邻近地区其他上前寒武纪碎屑地层的年龄进行了比较。我们的对比分析表明,这些岩石的年龄差别很大。这一结论与白海裂谷系形成和发育的古地理背景下,白海裂谷系中晚期以抬升分隔的几个小而封闭的盆地为主的观点是一致的。这些盆地与海洋的时间联系是可能的。这样的古地理环境不利于大河的发育;这就是为什么地堑主要由当地的岩石物质填充。克雷茨克地堑和坎大拉克沙地堑充满了从地堑壁上侵蚀而来的海相沉积物。局部沉积物来源为榴辉岩杂岩(~1.9 Ga),基性岩浆作用时间为~2.4 ~ 2.5 Ga和~2.7 ~ 2.9 Ga。克雷茨克地堑附近地区缺乏dZr颗粒的潜在主要来源。我们认为这些颗粒是由于锆石次生源的再循环作用而形成的,即起源于古老的当地沉积地层。
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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