Abstract
The continental crust growth/evolution processes and the tectonic regime through Eo-and Paleoarchean times are enigmatic due to the scarcity of preserved crust. The Gavia & SIM;o Block, Sa & SIM;o Francisco Craton (Brazil), contains exposed and well-preserved Eo-Paleoarchean crust remnants, providing a rare opportunity to investigate these issues. Here, we describe new U-Pb ages and Hf isotope data of 3.51-3.4 Ga tonalites and diorites from the Gavia & SIM;o Block and compare these with previously published Lu-Hf data from Hadean/Eo-Paleoarquean zircons from the Gavia & SIM;o Block and other primitive cratons. The Eo-to Paleoarchean evolution of the Gavia & SIM;o Block is registered by ca. 360 Myr of continuous magmatic events from ca. 3.66 Ga to 3.30 Ga. From the available Hf data, we interpret that each of the events younger than 3.6 Ga registers a new juvenile addition that assimilated older crust, whereas the rocks older than 3.6 Ga are exclusively formed through the reworking of a Hadean, and to a less extent early Eoarchean crust. The shift in the crust generation process with the input of juvenile material into the Gavia & SIM;o Block has been documented within the -3.8-3.5 Ga time in other primitive cratonic complexes including the Wyoming, Pilbara, Kaapvaal, Slave, Singhbhum, and Yilgarn. As documented in these other cratons, our data suggest that a shift in the Hf isotope record to rocks younger than 3.6 Ga reflects a transition from stagnant-lid to mobile-lid tectonics in the crust formation process of the Sa & SIM;o Francisco Craton. This change in the geodynamic regime appears to have been global at ca. -3.8-3.5 Ga and facilitated the extraction of juvenile melts, crustal reworking, evolved magmatism, and the production of stabilizing melt-depleted lithospheric mantle.
NSTL
Elsevier