Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/135085
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Type: Journal article
Title: Magmatic thickening of crust in non-plate tectonic settings initiated the subaerial rise of Earth's first continents 3.3 to 3.2 billion years ago
Author: Chowdhury, P.
Mulder, J.A.
Cawood, P.A.
Bhattacharjee, S.
Roy, S.
Wainwright, A.N.
Nebel, O.
Mukherjee, S.
Citation: Proceedings of the National Academy of Sciences of USA, 2021; 118(46):1-8
Publisher: Proceedings of the National Academy of Sciences
Issue Date: 2021
ISSN: 0027-8424
1091-6490
Statement of
Responsibility: 
Priyadarshi Chowdhurya, Jacob A. Muldera, b, Peter A. Cawooda, Surjyendu Bhattacharjeec, Subhajit Roya, Ashlea N. Wainwrightd, Oliver Nebela, and Subham Mukherjeee
Abstract: When and how Earth's earliest continents—the cratons—first emerged above the oceans (i.e., emersion) remain uncertain. Here, we analyze a craton-wide record of Paleo-to-Mesoarchean granitoid magmatism and terrestrial to shallow-marine sedimentation preserved in the Singhbhum Craton (India) and combine the results with isostatic modeling to examine the timing and mechanism of one of the earliest episodes of large-scale continental emersion on Earth. Detrital zircon U-Pb(-Hf) data constrain the timing of terrestrial to shallow-marine sedimentation on the Singhbhum Craton, which resolves the timing of craton-wide emersion. Time-integrated petrogenetic modeling of the granitoids quantifies the progressive changes in the cratonic crustal thickness and composition and the pressure–temperature conditions of granitoid magmatism, which elucidates the underlying mechanism and tectonic setting of emersion. The results show that the entire Singhbhum Craton became subaerial ∼3.3 to 3.2 billion years ago (Ga) due to progressive crustal maturation and thickening driven by voluminous granitoid magmatism within a plateau-like setting. A similar sedimentary–magmatic evolution also accompanied the early (>3 Ga) emersion of other cratons (e.g., Kaapvaal Craton). Therefore, we propose that the emersion of Earth’s earliest continents began during the late Paleoarchean to early Mesoarchean and was driven by the isostatic rise of their magmatically thickened (∼50 km thick), buoyant, silica-rich crust. The inferred plateau-like tectonic settings suggest that subduction collision–driven compressional orogenesis was not essential in driving continental emersion, at least before the Neoarchean. We further surmise that this early emersion of cratons could be responsible for the transient and localized episodes of atmospheric–oceanic oxygenation (O2-whiffs) and glaciation on Archean Earth.
Keywords: continental emersion
crustal thickness
Archean geodynamics
tonalite–trondhjemite–granodiorite
O2 whiffs and glaciation
Rights: © 2021. Published under the PNAS license
DOI: 10.1073/pnas.2105746118
Grant ID: http://purl.org/au-research/grants/arc/DP180100580
http://purl.org/au-research/grants/arc/FL160100168
Published version: http://dx.doi.org/10.1073/pnas.2105746118
Appears in Collections:Geology & Geophysics publications

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