Generation of Earth's Early Continents From a Relatively Cool Archean Mantle

Several lines of evidence suggest that the Archean (4.0–2.5 Ga) mantle was hotter than today's potential temperature (TP) of 1350 °C. However, the magnitude of such difference is poorly constrained, with TP estimation spanning from 1500 to 1600 °C during the Meso‐Archean (3.2–2.8 Ga). Such differences have major implications for the interpreted mechanisms of continental crust generation on the early Earth, as their efficacy is highly sensitive to the TP. Here we integrate petrological modeling with thermomechanical simulations to understand the dynamics of crust formation during Archean. Our results predict that partial melting of primitive oceanic crust produces felsic melts with geochemical signatures matching those observed in Archean cratons from a mantle TP as low as 1450 °C thanks to lithospheric‐scale RayleighTaylor‐type instabilities. These simulations also infer the occurrence of intraplate deformation events that allow an efficient transport of crustal material into the mantle, hydrating it. Plain Language Summary It has been believed that early Earth featured higher mantle temperature. The mantle temperature affects the geodynamic processes, and, therefore, the production of the continental crust, which has been a stable environment for the developing of life since Earth's infancy. However, our knowledge of the processes operating during the early Earth is still not definitive. The wide range of the mantle temperature estimation (from 1500 to 1600 °C) hampered our ability to understand early Earth's dynamic and geological data alone cannot provide a definitive answer. Therefore, it is necessary to integrate them with numerical modeling. Our contribution conjugates petrological modeling with thermal‐mechanical simulations to unveil the effect of continental crust production. Continental crust's extraction from partially melted hydrated basalts leaves behind dense rocks that sink into the mantle dragging part of surface hydrated rocks. These drips produce a major compositional change of the mantle and promote the production of new basaltic/continental crust. The combination of these processes cools the mantle, suggesting that it could not have been extremely hot for geological timescales. We show that such processes can be active even in a relatively cool mantle (1450–1500 °C), providing new constraints to understand the infancy of our planet. Key Points Geodynamic and thermodynamic modeling are applied to understand the production of continental