JANUÁRIA高地新太古代片麻岩和古元古代花岗岩的地球化学和U-Pb年代学:巴西SÃO FRANCISCO克拉通核的幼年和幼年地球记录

Q4 Earth and Planetary Sciences
Alexandre de Oliveira CHAVES, Christopher Rocha de REZENDE, Marco Antônio Leandro da SILVA, Ana Clara da Cruz PIRES
{"title":"JANUÁRIA高地新太古代片麻岩和古元古代花岗岩的地球化学和U-Pb年代学:巴西SÃO FRANCISCO克拉通核的幼年和幼年地球记录","authors":"Alexandre de Oliveira CHAVES, Christopher Rocha de REZENDE, Marco Antônio Leandro da SILVA, Ana Clara da Cruz PIRES","doi":"10.5016/geociencias.v42i2.17512","DOIUrl":null,"url":null,"abstract":"Within the proposal of secular evolution of the Earth system divided into seven phases: “Proto-Earth” (4.57–4.45 Ga); “Primordial Earth” (4.45–3.80 Ga); “Primitive Earth” (3.8–3.2 Ga); “Juvenile Earth” (3.2–2.5 Ga); “Youthful Earth” (2.5–1.8 Ga); “Middle Earth” (1.8–0.8 Ga); and “Contemporary Earth” (since 0.8 Ga), the 2.61-2.64 Ga High-K, meta- to peraluminous Januária High orthogneisses are inserted in the context of almost rigid behavior of the lithosphere, by the end of the Juvenile Earth. With protolith origin suggestive of intracrustal partial melting of local older TTG (tonalite-trondhjemite-granodiorite), these orthogneisses are the representatives in the São Francisco craton nucleus of the 2.8 Ga to 2.6 Ga potassic rocks found in archean cratons worldwide, and the occurrence of these rocks is a defining characteristic of the Juvenile Earth. Supported on evidence of the plate tectonic activity in Paleoproterozoic, the 2.14-2.19 Ga Januária High biotite granites are inserted in the context of Youthful Earth and they are the record of accretionary orogeny delineated by the edification of magmatic arc at that time. They are calc-alkaline, I-type rocks typical of subduction-related continental magmatic arcs. These biotite granites are probably derived from a High-K mafic source associated with tonalites.","PeriodicalId":35532,"journal":{"name":"Geociencias","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2023-09-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"GEOCHEMISTRY AND U-Pb GEOCHRONOLOGY OF THE NEOARCHEAN GNEISSES AND PALEOPROTEROZOIC GRANITES FROM JANUÁRIA HIGH: RECORDS OF JUVENILE AND YOUTHFUL EARTH IN THE SÃO FRANCISCO CRATON NUCLEUS (BRAZIL)\",\"authors\":\"Alexandre de Oliveira CHAVES, Christopher Rocha de REZENDE, Marco Antônio Leandro da SILVA, Ana Clara da Cruz PIRES\",\"doi\":\"10.5016/geociencias.v42i2.17512\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Within the proposal of secular evolution of the Earth system divided into seven phases: “Proto-Earth” (4.57–4.45 Ga); “Primordial Earth” (4.45–3.80 Ga); “Primitive Earth” (3.8–3.2 Ga); “Juvenile Earth” (3.2–2.5 Ga); “Youthful Earth” (2.5–1.8 Ga); “Middle Earth” (1.8–0.8 Ga); and “Contemporary Earth” (since 0.8 Ga), the 2.61-2.64 Ga High-K, meta- to peraluminous Januária High orthogneisses are inserted in the context of almost rigid behavior of the lithosphere, by the end of the Juvenile Earth. With protolith origin suggestive of intracrustal partial melting of local older TTG (tonalite-trondhjemite-granodiorite), these orthogneisses are the representatives in the São Francisco craton nucleus of the 2.8 Ga to 2.6 Ga potassic rocks found in archean cratons worldwide, and the occurrence of these rocks is a defining characteristic of the Juvenile Earth. Supported on evidence of the plate tectonic activity in Paleoproterozoic, the 2.14-2.19 Ga Januária High biotite granites are inserted in the context of Youthful Earth and they are the record of accretionary orogeny delineated by the edification of magmatic arc at that time. They are calc-alkaline, I-type rocks typical of subduction-related continental magmatic arcs. These biotite granites are probably derived from a High-K mafic source associated with tonalites.\",\"PeriodicalId\":35532,\"journal\":{\"name\":\"Geociencias\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-09-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Geociencias\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.5016/geociencias.v42i2.17512\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"Earth and Planetary Sciences\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geociencias","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.5016/geociencias.v42i2.17512","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Earth and Planetary Sciences","Score":null,"Total":0}
引用次数: 0

摘要

地球系统的长期演化分为七个阶段:“原地球”(4.57-4.45 Ga);“原始地球”(4.45-3.80 Ga);“原始地球”(3.8-3.2 Ga);“少年地球”(3.2-2.5 Ga);“青年地球”(2.5-1.8 Ga);“中土世界”(1.8-0.8 Ga);和“当代地球”(自0.8 Ga以来),2.61-2.64 Ga高钾,元至过铝Januária高正性是在岩石圈几乎刚性行为的背景下插入的,在幼年地球结束时。这些正长石的原岩起源暗示了局部更古老的TTG(闪长岩-闪长岩-花岗闪长岩)在壳内部分熔融,是世界范围内太古宙克拉通中发现的2.8 Ga ~ 2.6 Ga钾质岩石的 o Francisco克拉通核的代表,它们的出现是地球幼期的一个决定性特征。在古元古代板块构造活动证据的支持下,2.14-2.19 Ga Januária高黑云母花岗岩是在年轻地球背景下插入的,是当时岩浆弧的陶冶所描绘的增生造山作用的记录。它们是钙碱性的i型岩石,是与俯冲有关的大陆岩浆弧的典型特征。这些黑云母花岗岩可能来源于与调性岩有关的高钾基性花岗岩。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
GEOCHEMISTRY AND U-Pb GEOCHRONOLOGY OF THE NEOARCHEAN GNEISSES AND PALEOPROTEROZOIC GRANITES FROM JANUÁRIA HIGH: RECORDS OF JUVENILE AND YOUTHFUL EARTH IN THE SÃO FRANCISCO CRATON NUCLEUS (BRAZIL)
Within the proposal of secular evolution of the Earth system divided into seven phases: “Proto-Earth” (4.57–4.45 Ga); “Primordial Earth” (4.45–3.80 Ga); “Primitive Earth” (3.8–3.2 Ga); “Juvenile Earth” (3.2–2.5 Ga); “Youthful Earth” (2.5–1.8 Ga); “Middle Earth” (1.8–0.8 Ga); and “Contemporary Earth” (since 0.8 Ga), the 2.61-2.64 Ga High-K, meta- to peraluminous Januária High orthogneisses are inserted in the context of almost rigid behavior of the lithosphere, by the end of the Juvenile Earth. With protolith origin suggestive of intracrustal partial melting of local older TTG (tonalite-trondhjemite-granodiorite), these orthogneisses are the representatives in the São Francisco craton nucleus of the 2.8 Ga to 2.6 Ga potassic rocks found in archean cratons worldwide, and the occurrence of these rocks is a defining characteristic of the Juvenile Earth. Supported on evidence of the plate tectonic activity in Paleoproterozoic, the 2.14-2.19 Ga Januária High biotite granites are inserted in the context of Youthful Earth and they are the record of accretionary orogeny delineated by the edification of magmatic arc at that time. They are calc-alkaline, I-type rocks typical of subduction-related continental magmatic arcs. These biotite granites are probably derived from a High-K mafic source associated with tonalites.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Geociencias
Geociencias Earth and Planetary Sciences-Earth and Planetary Sciences (all)
CiteScore
0.70
自引率
0.00%
发文量
0
×
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:481959085
Book学术官方微信