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Growing primordial continental crust self-consistently in global mantle convection models

机译:在全球地幔对流模型中,生长原始的大陆地壳自始终如一

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The majority of continental crust formed during the hotter Archean was composed of Tonalite-Trondhjemite-Granodiorite (TTG) rocks. In contrast to the present-day loci of crust formation around subduction zones and intra-plate tectonic settings, ITGs are formed when hydrated basalt melts at garnet-amphibolite, granulite or eclogite facies conditions. Generating continental crust requires a two step differentiation process. Basaltic magma is extracted from the pyrolytic mantle, is hydrated, and then partially melts to form continental crust. Here, we parameterise the melt production and melt extraction processes and show self-consistent generation of primordial continental crust using evolutionary thermochemical mantle convection models. To study the growth of TTG and the geodynamic regime of early Earth, we systematically vary the ratio of intrusive (plutonic) and eruptive (volcanic) magmatism, initial core temperature, and internal friction coefficient. As the amount of TTG that can be extracted from the basalt (or basalt-to-TTG production efficiency) is not known, we also test two different values in our simulations, thereby limiting TTG mass to 10% or 50% of basalt mass. For simulations with lower basalt-to-TTG production efficiency, the volume of TTG crust produced is in agreement with net crustal growth models but overall crustal (basaltic and TTG) composition stays more mafic than expected from geochemical data. With higher production efficiency, abundant TTG crust is produced, with a production rate far exceeding typical net crustal growth models but the felsic to mafic crustal ratio follows the expected trend. These modelling results indicate that (i) early Earth exhibited a "plutonic squishy lid" or vertical-tectonics geodynamic regime, (ii) present-day slab-driven subduction was not necessary for the production of early continental crust, and (iii) the Archean Earth was dominated by intrusive magmatism as opposed to "heat-pipe" eruptive magmatism. (C) 2019
机译:在更热的Archean中形成的大多数大陆地壳由Tonalite-Trondhjemite-Granodiorite(TTG)岩石组成。与俯冲区域周围的地壳形成的现状基因座相反,当水合玄武岩在石榴石,粒细胞或eClogite面条条件下熔化时,形成ITG。生成大陆地壳需要两步分化过程。玄武岩岩浆从热解罩中提取,水合水合,然后部分熔化以形成大陆地壳。在这里,我们使用进化的热化学搭配对流模型参数化熔体生产和熔融提取过程,并显示自成的原始大陆地壳的原始陆地地壳。为了研究TTG的生长和早期地球的地球动力学制度,我们系统地改变了侵入式(Plutonic)和喷发(火山)岩浆,初始核心温度和内部摩擦系数的比例。作为可以从玄武岩(或玄武岩至TTG生产效率)中提取的TTG的量不知道,我们还在模拟中测试了两种不同的值,从而将TTG质量限制为玄武岩质量的10%或50%。对于具有较低玄武岩到TTG生产效率的仿真,产生的TTG地壳的体积与净地壳增长模型一致,但整体地壳(玄武岩和TTG)组成比地球化学数据从预期的预期保持更多的兆画。具有较高的生产效率,生产丰富的地壳,生产率远远超过典型的净地壳增长模型,但迈克斯地壳比率呈现出预期的趋势。这些建模结果表明,(i)早期地球表现出“升高的绒毛盖”或垂直构造地球动力学制度,(ii)当今的平板驱动的俯冲没有必要生产早期的欧洲地壳,(iii) Archean地球由侵入性岩浆广告主导,而不是“热管”爆发性岩浆广告。 (c)2019年

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