Potassium Isotope Evidence for Origin of Archean TTG Rocks From Seawater-Hydrothermally Altered Oceanic Crust

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
D.-Y. Xiong, X.-L. Wang, W. Li, Y.-F. Zheng, C. R. Anhaeusser, A. Hofmann, D. Wang, J.-Y. Li
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Abstract

Tonalite-trondhjemite-granodiorite (TTG) rocks constitute a crucial part of the Archean continental crust, yet their origins remain contentious. It is critical to decipher their source nature and hydration mechanism. This paper presents a study of whole-rock K stable isotopes in well-preserved ca. 3.51–3.42 Ga TTG rocks and associated mafic rocks from the Barberton granitoid-greenstone terrane (BGGT) in the Kaapvaal Craton, South Africa. The results show for the first time a substantial δ41K variation from −0.69 ± 0.07‰ to −0.32 ± 0.05‰ (2SD) for the Paleoarchean mafic rocks, exceeding the present mantle δ41K range from −0.6 to −0.3‰. This variation can be well explained by the seawater-hydrothermal alteration at different temperatures. Similarly, the Paleoarchean TTGs exhibit a wide δ41K range from −0.55 ± 0.04‰ to 0.07 ± 0.08‰ (2SD). In combination with available zircon δ18O values of 5.07–6.02‰, it is evident that Archean TTGs would be derived from partial melting of the seawater-hydrothermally altered oceanic crust (AOC). The distinct K-O isotope signatures demonstrate that the hydration of Archean mafic crust is caused by the hydrothermal alteration at mid-ocean ridges during seafloor spreading. The variable K-O isotope compositions in the Archean TTGs signify a series of processes that are dominated by the seawater-hydrothermally altered AOC in a Wilson cycle from divergence through convergence to rifting of Archean oceanic plates. This offers a viable mechanism for TTG petrogenesis and the growth of continental crust in the Archean.

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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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