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Published November 16, 2021 | Published + Supplemental Material
Journal Article Open

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

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.

Additional Information

© 2021 National Academy of Sciences. Published under the PNAS license. Edited by Roberta L. Rudnick, University of California, Santa Barbara, CA, and approved September 29, 2021 (received for review March 26, 2021). We thank the editor and three anonymous reviewers for their thorough and constructive reviews. We thank Rachelle Pierson (Monash University) and Graham Hutchinson (University of Melbourne) for assisting in sample processing and CL imaging of detrital zircons. Discussions with Pulak Sengupta, Jean-François Moyen, Oscar Laurent, and Fabio Capitanio are gratefully acknowledged. Data Availability: All data are given in the article and/or supporting information. This includes the previously published data that were used for this work (30, 31, 58-71). MATLAB codes and input files used in this study are available from GitHub (https://github.com/priyadarshi-geo/Continental-Emersion-2021). Author contributions: P.C. and J.A.M. designed research; P.C., J.A.M., S.B., S.R., A.N.W., and S.M. performed research; P.C., J.A.M., P.A.C., and O.N. analyzed data; and P.C., J.A.M., P.A.C., and O.N. wrote the paper. The authors declare no competing interest. This article is a PNAS Direct Submission. This article contains supporting information online at https://www.pnas.org/lookup/suppl/doi:10.1073/pnas.2105746118/-/DCSupplemental.

Attached Files

Published - e2105746118.full.pdf

Supplemental Material - pnas.2105746118.sapp.pdf

Supplemental Material - pnas.2105746118.sd01.xlsx

Supplemental Material - pnas.2105746118.sd02.xlsx

Supplemental Material - pnas.2105746118.sd03.xlsx

Supplemental Material - pnas.2105746118.sd04.xlsx

Supplemental Material - pnas.2105746118.sd05.xlsx

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Additional details

Created:
September 15, 2023
Modified:
October 23, 2023