Reviewing subduction initiation and the origin of plate tectonics: What do we learn from present-day Earth?

IF 2.9 3区 地球科学
Gang Lu, Liang Zhao, Ling Chen, Bo Wan, FuYuan Wu
{"title":"Reviewing subduction initiation and the origin of plate tectonics: What do we learn from present-day Earth?","authors":"Gang Lu,&nbsp;Liang Zhao,&nbsp;Ling Chen,&nbsp;Bo Wan,&nbsp;FuYuan Wu","doi":"10.26464/epp2021014","DOIUrl":null,"url":null,"abstract":"<p>The theory of plate tectonics came together in the 1960s, achieving wide acceptance after 1968. Since then it has been the most successful framework for investigations of Earth's evolution. Subduction of the oceanic lithosphere, as the engine that drives plate tectonics, has played a key role in the theory. However, one of the biggest unanswered questions in Earth science is how the first subduction was initiated, and hence how plate tectonics began. The main challenge is how the strong lithosphere could break and bend if plate tectonics-related weakness and slab-pull force were both absent. In this work we review state-of-the-art subduction initiation (SI) models with a focus on their prerequisites and related driving mechanisms. We note that the plume-lithosphere-interaction and mantle-convection models do not rely on the operation of existing plate tectonics and thus may be capable of explaining the first SI. Re-investigation of plate-driving mechanisms reveals that mantle drag may be the missing driving force for surface plates, capable of triggering initiation of the first subduction. We propose a composite driving mechanism, suggesting that plate tectonics may be driven by both subducting slabs and convection currents in the mantle. We also discuss and try to answer the following question: Why has plate tectonics been observed only on Earth?</p>","PeriodicalId":45246,"journal":{"name":"Earth and Planetary Physics","volume":"5 2","pages":"123-140"},"PeriodicalIF":2.9000,"publicationDate":"2021-04-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.26464/epp2021014","citationCount":"12","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Earth and Planetary Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.26464/epp2021014","RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 12

Abstract

The theory of plate tectonics came together in the 1960s, achieving wide acceptance after 1968. Since then it has been the most successful framework for investigations of Earth's evolution. Subduction of the oceanic lithosphere, as the engine that drives plate tectonics, has played a key role in the theory. However, one of the biggest unanswered questions in Earth science is how the first subduction was initiated, and hence how plate tectonics began. The main challenge is how the strong lithosphere could break and bend if plate tectonics-related weakness and slab-pull force were both absent. In this work we review state-of-the-art subduction initiation (SI) models with a focus on their prerequisites and related driving mechanisms. We note that the plume-lithosphere-interaction and mantle-convection models do not rely on the operation of existing plate tectonics and thus may be capable of explaining the first SI. Re-investigation of plate-driving mechanisms reveals that mantle drag may be the missing driving force for surface plates, capable of triggering initiation of the first subduction. We propose a composite driving mechanism, suggesting that plate tectonics may be driven by both subducting slabs and convection currents in the mantle. We also discuss and try to answer the following question: Why has plate tectonics been observed only on Earth?

Abstract Image

回顾俯冲起始和板块构造的起源:我们从现今的地球学到了什么?
板块构造理论形成于20世纪60年代,1968年后得到广泛接受。从那以后,它一直是研究地球演化的最成功的框架。海洋岩石圈的俯冲作用,作为驱动板块构造的引擎,在该理论中发挥了关键作用。然而,地球科学中最大的未解之谜之一是第一次俯冲是如何开始的,因此板块构造是如何开始的。主要的挑战是,如果没有板块构造相关的弱点和板块拉力,强大的岩石圈如何断裂和弯曲。在这项工作中,我们回顾了最新的俯冲起始(SI)模型,重点讨论了它们的先决条件和相关的驱动机制。我们注意到,羽流-岩石圈-相互作用和地幔-对流模式不依赖于现有板块构造的运作,因此可能能够解释第一次SI。对板块驱动机制的重新研究表明,地幔阻力可能是表面板块缺失的驱动力,能够触发第一次俯冲的起始。我们提出了一个复合驱动机制,表明板块构造可能同时受到俯冲板块和地幔对流的驱动。我们还讨论并试图回答以下问题:为什么板块构造只在地球上被观察到?
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
Earth and Planetary Physics
Earth and Planetary Physics GEOSCIENCES, MULTIDISCIPLINARY-
自引率
17.20%
发文量
174
×
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