Ages and Hf isotopes of detrital zircons from Paleozoic strata in the Chagan Obo Temple area, Inner Mongolia: Implications for the evolution of the Central Asian Orogenic Belt

The Central Asian Orogenic Belt (CAOB), as one of the largest accretionary orogens in the world, was built up through protracted accretion and collision of a variety of terranes due to the subduction and closure of the Paleo-Asian Ocean in the Neoproterozoic to Early Mesozoic. Located in the Uliastai continental margin of the southeastern CAOB, the Chagan Obo Temple area is essential for understanding the tectonic evolution of the southeastern part of the CAOB and its relation with the "Hegenshan Ocean". In this study, detrital zircon U-Pb geochronology coupled with Hf isotopic analysis was performed on Paleozoic sedimentary strata in this area. Most detrital zircons from the studied samples possess oscillatory zoning and have Th/U ratios of 0.4-1.73, indicative of an igneous origin. Detrital zircons from the Ordovician to Devonian sedimentary strata yield a predominant age group at 511-490 Ma and subordinate age groups at 982-891 Ma, 834-790 Ma and similar to 574 Ma, and have a large spread of epsilon(Hf)(t) values (-20.77 to +16.94). Carboniferous and Early Permian samples yield zircon U-Pb ages peaking at similar to 410 Ma and similar to 336 Ma, and have dominantly positive epsilon(Hf)(t) values (+1.30 to +14.86). Such age populations and Hf isotopic signatures match those of magmatic rocks in the Northern Accretionary Orogen and the Mongolian arcs. A marked shift of provenance terranes from multiple sources to a single source and Hf isotope compositions from mixed to positive values occurred at some time in the Carboniferous. Such a shift implies that the Northern Accretionary Orogenwas no longer a contributor of detritus in the Carboniferous to Early Permian, due to the opening of the "Hegenshan Ocean" possibly induced by the slab rollback of the subducting Paleo-Asian Ocean. (C) 2016 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.