Provenance of detrital zircons from the Ribeira and Dom Feliciano Belts, comparison with African equivalents and implications on Western Gondwana amalgamation

The geologic make-up of southern Brazil has been defined by processes related to the Brasiliano orogenic cycle and, in particular, to con tractional tectonic events that led to the amalgamation of different terranes, which culminated in the formation of Western Gondwana (Campos Neto and Figueiredo, 1995; Brito Neves and Cordani, 1991; Brito Neves et al, 1999, Campos Neto, 2000). Polycyclic deformation and metamorphism that masked the characteristics, including the age records, of the protoliths were associated with the juxtaposition of these different terranes. Ophiolitic remains and magmatic arc roots signal the existence of fossil subduction and collision zones, whereas intense post-tectonic to an orogenic granitic magmatism marks the end of the orogenic cycle towards the end of the Neoproterozoic Era. U-Pb dating of domains within single zircon grains has proven to be a very powerful tool for the unraveling of the complex tecto no-thermal evolution as well as in characterizing the provenance of the original sediments. This is due to the high resistance to weathering and to high closure temperatures with respect to the U-Pb isotope system in zircon. Over the past decade, the standard technique for this analytical approach has become the analyses of U-Pb isotope ratios by SHRIMP, preceded by cathodoluminescence analysis (McClaren et al 1994). In this study, a set of 11 new SHRIMP analyses on detrital zircon grains from the major metasedimentary units of the Ribeira and Dom Feliciano Belts of the southeastern portion of South America is presented and the data are compared with available analyses for the Gariep Belt (Basei et al. 2005) and a new analysis for the Damara Belt. Combined with available Sm-Nd bulk rock isotope data, the results will form the basis for a revised tectonic model for the formation of Western Gondwana