地球的早期演化,其地质历史的开端:花岗岩岩浆是如何以及何时出现的

Q4 Earth and Planetary Sciences
M. Kuzmin, V. Yarmolyuk, A. Kotov
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引用次数: 3

摘要

地球与太阳系和其他恒星-行星系统的行星有许多不同之处。这些差异是在其形成和地质历史过程中形成的。在混沌宙的早期,发生了地球的吸积,地球的主要物质分离成地幔和核,地球的卫星——月球出现了。4500万年前,地球的地质历史开始了。此时,地球上的内源性过程在很大程度上受到陨石小行星轰击的控制,造成了地球上层外壳的大规模融化和分化。在岩浆室中,分化一直持续到花岗岩类成分的熔体出现。盖迪纪的大陆地壳几乎完全被陨石轰击摧毁,最后一次猛烈的轰击发生在4000-3900年前的盖迪纪末期。盖迪时代的地质情况只能从该时代岩石中保存下来的锆石来判断。特别是,它们的地球化学特征表明地球有大气层。盖迪宙被太古宙所取代,自组织的过程开始在地球上占主导地位。这一时期,形成了由黑马岩—玄武岩和闪长岩—闪长岩—花岗闪长岩(TTG)系列岩石组成的地壳。在其形成过程中,地壳在上升地幔柱上的俯冲作用(地壳垂直生长)起了主导作用。与此同时,下玄武岩地壳在地幔中燃烧、榴辉化和熔融,导致TTG钠系岩石的出现。在3.1-3.0 Ga太古宙末期,决定太古宙地壳构造样式和发育的盖层构造(LID构造)被小板块构造所取代,后来被现代板块与地幔柱相结合的构造所取代。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The early evolution of the earth, the beginning of its geological history: how and when the granitoid magmas appeared
The Earth has a number of differences from the planets of the Solar System and other star-planetary systems. These differences were acquired during its formation and geological history. In the early Chaotic eon occurred the accretion of the Earth, the separation of the primary substance of the Earth into a mantle and a nucleus, a satellite of the Earth - the Moon appeared. 4500 Ma ago in the Gadey aeon the geological history of the Earth began. At this time, the endogenous processes on the Earth were controlled to a great extent by meteorite-asteroid bombardments, which caused large-scale melting and differentiation of the upper shells of the Earth. In the magmatic chambers differentiation proceeded until the appearance of melts of granitoid composition. The continental crust of Gadey time was almost completely destroyed by meteoric bombardments, the last heavy bombardment occurred at the end of the Gadey aeon 4000-3900 Ma ago. The geological situation of the Gadey time can be judged only from the preserved zircons from the rocks of that epoch. In particular, their geochemical features indicate that the Earth has an atmosphere. The Gadey eon was replaced by the Archean one, from which the processes of self-organization began to predominate on the Earth. At this time, a crust composed of komatiite-basalt and tonalite-trondhjemite-granodiorite (TTG) series of rocks was formed. In its formation, the processes of sagduction (vertical growth of the crust) over the rising mantle plumes was played the leading role. At the same time the lower basaltic crust was bured in the mantle, eclogitized and melted, which led to the appearance of the sodium series of TTG rocks. At the end of the Archean 3.1-3.0 Ga tectonics of the cover (LID tectonics), which determined the style of the structure and development of the Archean crust, is replaced by the tectonics of small plates, which was later replaced by modern tectonics - the tectonics of plates combined with mantle plumes.
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来源期刊
Litosfera
Litosfera Earth and Planetary Sciences-Geophysics
CiteScore
0.70
自引率
0.00%
发文量
39
审稿时长
12 weeks
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