Late Neoarchean sanukitoids in the North China Craton: A geodynamic perspective

Guozheng Sun , Shuwen Liu , Lintao Wang , Yang Yu , Shengyao Yu , Huahua Cao , Lei Gao , Yalu Hu , Jinghao Fu
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Abstract

The formation, evolution, and geodynamics of the Archean continent is a hot topic in solid earth science. Sanukitoids are the oldest Mg-Fe-K-rich granitoid magmas recognized so far on Earth, and their crust-mantle interaction process is a golden key to deciphering the formation and evolution of early continental crust. Sanukitoid suites consist of late Archean (3.0–2.5 Ga-old) plutonic rocks ranging from diorites, monzodiorites, and granodiorite, typically with abundant cognate mafic enclaves. Geochemically, they have a mantle signature (high content of Mg, Ni, Cr, and high Mg#) and enrichment in LILE (especially K, Ba, and Sr). It is generally believed that Archean sanukitoids originated from an enriched or metasomatized lithospheric mantle source, and its parental magmas are water-rich and highly oxidized, which is probably genetically related to gold mineralization. Here we compile the geochemical data for late Neoarchean (2.6–2.5 Ga) sanukitoids from the North China Craton and conduct a systematic petrogenetic classification. The less-differentiated sanukitoid magma (SiO2 < 62 wt%) was controlled by multiple factors such as metasomatic component, metasomatic degree, and melting P-T conditions, indicating that near-surface weathering had already existed in the late Archean. The differentiated sanukitoids (SiO2 > 62 wt%) were formed by extensive fractional crystallization of less-differentiated sanukitoid melts, accompanied by crust-mantle magmatic mixing. These late Neoarchean sanukitoids are distributed sporadically throughout the North China Craton without zonation. Combined with other evidence of magmatism, metamorphic deformation, and thermodynamic numerical modeling, we propose that the sanukitoids may develop under the microplate tectonic regime, characterized by small-scale and short-term warm subduction.

Abstract Image

华北克拉通新太古代晚期似岩浆岩:地球动力学视角
太古宙大陆的形成、演化及其地球动力学是固体地球科学研究的热点。Sanukitoids是迄今为止地球上发现的最古老的富镁铁钾花岗岩岩浆,其壳幔相互作用过程是破解早期大陆地壳形成演化的金钥匙。Sanukitoid套由晚太古代(3.0-2.5 ga)的闪长岩、二长岩和花岗闪长岩组成,通常具有丰富的同源基性包体。地球化学上,它们具有地幔特征(高Mg、Ni、Cr和高Mg#含量)和LILE富集(特别是K、Ba和Sr)。一般认为太古宙类岩浆岩起源于岩石圈地幔富集或交代源,其母岩浆为富水、高氧化岩浆,可能与金矿化有关。本文整理了华北克拉通新太古代晚期(2.6 ~ 2.5 Ga) sanukitoids的地球化学资料,并进行了系统的岩石成因分类。低分化sanukitoid岩浆(SiO2 <;62 wt%)受交代成分、交代程度、熔融P-T条件等多种因素控制,表明太古宙晚期已存在近地表风化作用。已分化的类sanukitae (SiO2 >;(62%)是由低分异的sanukitoid熔体广泛的分异结晶形成的,伴随着壳幔岩浆混合作用。这些新太古代晚期的类sanukita在华北克拉通中零星分布,无分带性。结合岩浆作用、变质变形和热力学数值模拟等证据,认为类sanukita可能发育在微板块构造体制下,具有小尺度、短期热俯冲的特征。
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