通过迟缓俯冲生成阿新世熱帶地壳

Geology Pub Date : 2024-06-13 DOI:10.1130/g52196.1
Bradford J. Foley
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引用次数: 0

摘要

据认为,地球阿新世大陆上突出的闪长岩-黑云母-花岗闪长岩(TTG)是由水合玄武岩熔融形成的,但其形成的具体构造环境尚不清楚。TTG的成因模型包括在俯冲过程中下行的黑质地壳熔化到较热的地幔,以及在厚地壳高原底部熔化;虽然这两种模型都不能唯一地定义全球构造体系,但前者与移动盖构造相一致,后者则与停滞盖构造相一致。俯冲模型的一个主要问题是板坯在较热的地幔中下沉得太快、太陡,无法熔化下沉的地壳。然而,我的研究表明,岩石圈中粒度的减小导致了早期地球上相对较强的板块边界,从而减缓了板块下沉的速度。在这种 "迟缓俯冲 "过程中,当地幔温度为≳1600 °C时,下沉板块的温度足以熔化地壳。因此,通过迟缓俯冲的地壳熔化可以解释阿基坦时期由于地幔温度升高而形成的TTG,以及此后由于地幔冷却而产生的TTG。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Generation of Archean TTGs via sluggish subduction
The trondhjemite-tonalite-granodiorite (TTG) suite of rocks prominent in Earth’s Archean continents is thought to form by melting of hydrated basalt, but the specific tectonic settings of formation are unclear. Models for TTG genesis range from melting of downgoing mafic crust during subduction into a hotter mantle to melting at the base of a thick crustal plateau; while neither uniquely defines a global tectonic regime, the former is consistent with mobile lid tectonics and the latter a stagnant lid. One major problem for a subduction model is slabs sinking too quickly and steeply in a hotter mantle to melt downgoing crust. I show, however, that grain size reduction in the lithosphere leads to relatively strong plate boundaries on the early Earth, which slow slab sinking. During this “sluggish subduction,” sinking plates can heat up enough to melt when the mantle temperature is ≳1600 °C. Crustal melting via sluggish subduction can thus explain TTG formation during the Archean due to elevated mantle temperatures and the paucity of TTG production since due to mantle cooling.
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