Changing pattern of continental crust generation from late Mesoarchean to early Paleoproterozoic: Record from the southeastern Bastar Craton, central India

IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY
Samyayan Ghosal , Sukanta Dey , Jaganmoy Jodder , Manoj Kumar Sahoo , Marlina A. Elburg
{"title":"Changing pattern of continental crust generation from late Mesoarchean to early Paleoproterozoic: Record from the southeastern Bastar Craton, central India","authors":"Samyayan Ghosal ,&nbsp;Sukanta Dey ,&nbsp;Jaganmoy Jodder ,&nbsp;Manoj Kumar Sahoo ,&nbsp;Marlina A. Elburg","doi":"10.1016/j.precamres.2025.107835","DOIUrl":null,"url":null,"abstract":"<div><div>The Earth underwent significant changes during the late Mesoarchean to early Paleoproterozoic period, such as the advent of modern-style plate tectonics and widespread formation and emergence of continental crust. However, the details of temporal variations in mechanisms of continental crust formation during this critical period have been widely debated. The present work addresses such issue by providing comprehensive insights through field, petrographic, whole-rock elemental, and in-situ zircon LA-MC-ICP-MS U-Pb-Hf isotope data on granitoids from the previously unexplored southeastern part of the Bastar Craton, India. The study area records the formation of a ∼ 2.86 Ga high-HREE sodic granitoid, and is interpreted to be a product of shallow partial melting of a juvenile mafic crust in an intraplate setting. Detrital zircon ages from a paragneiss suggest subsequent crust generation around 2.75–2.65 Ga, with a shift from juvenile crust formation to reworking of older crust at ∼ 2.70 Ga. Thereafter, widespread high-temperature reworking of significantly older (Eo- to Paleoarchean) crust at ∼ 2.48–2.47 Ga produced voluminous ferroan, LILE- and HFSE-enriched potassic granitoids with A-type characteristics. By synthesizing craton-wide information, our results point towards the subduction and accretion of various arc-related terrains at ∼ 2.5 Ga within the Bastar Craton. It is argued that the ∼ 2.48 Ga high-temperature, ferroan potassic granitoids were formed in an extensional geodynamic setting during post-orogenic uplift. This marks the termination of the compressive forces of subduction, leading to final cratonization. Finally, granitoid exhumation shed immature clastic sediments, now preserved as paragneiss in nearby basins, likely formed by post-collisional extensional collapse. Comparison with other well-studied cratons suggests a common pattern − an initial late Mesoarchean to early Neoarchean period of juvenile magmatism associated with non-plate tectonic regime, followed possibly by the advent of modern-style plate tectonics, terrain accretion, and granitoid diversification in the late Neoarchean.</div></div>","PeriodicalId":49674,"journal":{"name":"Precambrian Research","volume":"427 ","pages":"Article 107835"},"PeriodicalIF":3.2000,"publicationDate":"2025-06-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Precambrian Research","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0301926825001615","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"GEOSCIENCES, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0

Abstract

The Earth underwent significant changes during the late Mesoarchean to early Paleoproterozoic period, such as the advent of modern-style plate tectonics and widespread formation and emergence of continental crust. However, the details of temporal variations in mechanisms of continental crust formation during this critical period have been widely debated. The present work addresses such issue by providing comprehensive insights through field, petrographic, whole-rock elemental, and in-situ zircon LA-MC-ICP-MS U-Pb-Hf isotope data on granitoids from the previously unexplored southeastern part of the Bastar Craton, India. The study area records the formation of a ∼ 2.86 Ga high-HREE sodic granitoid, and is interpreted to be a product of shallow partial melting of a juvenile mafic crust in an intraplate setting. Detrital zircon ages from a paragneiss suggest subsequent crust generation around 2.75–2.65 Ga, with a shift from juvenile crust formation to reworking of older crust at ∼ 2.70 Ga. Thereafter, widespread high-temperature reworking of significantly older (Eo- to Paleoarchean) crust at ∼ 2.48–2.47 Ga produced voluminous ferroan, LILE- and HFSE-enriched potassic granitoids with A-type characteristics. By synthesizing craton-wide information, our results point towards the subduction and accretion of various arc-related terrains at ∼ 2.5 Ga within the Bastar Craton. It is argued that the ∼ 2.48 Ga high-temperature, ferroan potassic granitoids were formed in an extensional geodynamic setting during post-orogenic uplift. This marks the termination of the compressive forces of subduction, leading to final cratonization. Finally, granitoid exhumation shed immature clastic sediments, now preserved as paragneiss in nearby basins, likely formed by post-collisional extensional collapse. Comparison with other well-studied cratons suggests a common pattern − an initial late Mesoarchean to early Neoarchean period of juvenile magmatism associated with non-plate tectonic regime, followed possibly by the advent of modern-style plate tectonics, terrain accretion, and granitoid diversification in the late Neoarchean.
中太古代晚期至古元古代早期大陆地壳生成变化模式:来自印度中部巴斯塔克拉通东南部的记录
中太古代晚期至古元古代早期,地球经历了现代板块构造的出现和大陆地壳的广泛形成和出现等重大变化。然而,在这一关键时期,大陆地壳形成机制的时间变化细节一直存在广泛的争论。本研究通过野外、岩石学、全岩元素和原位锆石LA-MC-ICP-MS U-Pb-Hf同位素数据对印度巴斯塔尔克拉通东南部未勘探的花岗岩类提供全面的见解,解决了这一问题。研究区记录了一个~ 2.86 Ga高三稀土钠质花岗岩的形成,并被解释为板内环境下幼小基性地壳浅部熔融的产物。副长岩的碎屑锆石年龄表明,在2.75-2.65 Ga前后地壳形成,在~ 2.70 Ga从幼年地壳形成向旧地壳改造转变。此后,在~ 2.48-2.47 Ga,对明显更古老(始古宙至古太古代)的地壳进行了广泛的高温改造,产生了大量具有a型特征的富含铁、LILE和hfse的钾质花岗岩。通过综合克拉通范围内的信息,我们的结果指向了巴斯塔克拉通内各种弧相关地形在~ 2.5 Ga的俯冲和增生。认为~ 2.48 Ga高温铁质钾质花岗岩形成于造山后隆升的伸展地球动力学背景。这标志着俯冲的压缩力的终止,导致最终的克拉通化。最后,花岗岩类发掘出未成熟的碎屑沉积物,现在以副长岩的形式保存在附近的盆地中,可能是由碰撞后的伸展崩塌形成的。与其他研究充分的克拉通相比,我们发现了一个共同的模式——中太古宙晚期至新太古宙早期与非板块构造制度相关的青少年岩浆活动,随后可能是新太古宙晚期现代板块构造、地形增生和花岗岩类多样化的出现。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
Precambrian Research
Precambrian Research 地学-地球科学综合
CiteScore
7.20
自引率
28.90%
发文量
325
审稿时长
12 months
期刊介绍: Precambrian Research publishes studies on all aspects of the early stages of the composition, structure and evolution of the Earth and its planetary neighbours. With a focus on process-oriented and comparative studies, it covers, but is not restricted to, subjects such as: (1) Chemical, biological, biochemical and cosmochemical evolution; the origin of life; the evolution of the oceans and atmosphere; the early fossil record; palaeobiology; (2) Geochronology and isotope and elemental geochemistry; (3) Precambrian mineral deposits; (4) Geophysical aspects of the early Earth and Precambrian terrains; (5) Nature, formation and evolution of the Precambrian lithosphere and mantle including magmatic, depositional, metamorphic and tectonic processes. In addition, the editors particularly welcome integrated process-oriented studies that involve a combination of the above fields and comparative studies that demonstrate the effect of Precambrian evolution on Phanerozoic earth system processes. Regional and localised studies of Precambrian phenomena are considered appropriate only when the detail and quality allow illustration of a wider process, or when significant gaps in basic knowledge of a particular area can be filled.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信