Due to the dearth of rock records during the Hadean, little is known about early crustal chemistry and geodynamics. Here, we present zircon trace and rare earth element and Lu-Hf measurements of zircons ∼ 3.3 Ga to ∼ 4.2 Ga from the Older Metamorphic Tonalitic Gneiss in the Singhbhum Craton to better understand geodynamic changes during the Hadean and Archean. We find decreasing, subchondritic zircon εHfT among zircons > 3.7 Ga and no indication of addition of new crustal material during the Hadean after initial formation of this protocrust. Trace and rare earth element analyses of > 3.7 Ga grains indicate derivation from a source heavily influenced by the enriched mantle with little evidence for flux melting, and no clear evidence for deep melting. At ∼ 3.7 Ga, we observe an average εHfT increase indicating new additions of juvenile felsic material. These zircons still show predominantly mantle-like trace elements, but with the appearance of some arc-like signatures and evidence for crustal thickening. This period of crustal reorganization speaks towards a shift in geodynamic regime characterized by the onset of communication between the mantle and the crust from which the zircons formed at this location. The presence of long-lived, mantle-derived protocrust in both India and South Africa appears to suggest the possibility of a local stagnant lid, albeit more data is necessary to confirm this. The presence of a transition of εHfT data globally may point towards an important, diachronous period of crustal reorganization 3.9 – 3.6 Ga ago.
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