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Original Article |
1 1Research School of Earth Sciences, The Australian National University, Canberra A.C.T. 0200, Australia
2 2British Geological Survey, Keyworth, Nottingham NG12 5GG, UK
3 3Centro de Investigaciones Geológicas, Universidad Nacional de La Plata, La Plata, Argentina
4 4Departamento de Geología, Universidad Nacional de Córdoba, Córdoba, Argentina
5 5Departamento de Petrología y Geoquímica, Universidad Complutense, 28040 Madrid, Spain
New UPb radiometric dates for K-bentonite horizons within the Lower Cambrian to Middle Ordovician platform carbonates from the Precordillera terrane of NW Argentina provide further constraints on models for the allochthonous or parautochthonous accretion of this terrane. Two K-bentonite layers from the Talacasto section yield indistinguishable sensitive high-resolution ion microprobe (SHRIMP) UPb zircon dates of 469.5 ± 3.2 Ma and 470.1 ± 3.3 Ma respectively. These are within uncertainty of the UPb SHRIMP zircon date of 468.3 ± 3.4 Ma for a porphyritic rhyolite from the Famatinian magmatic arc, Sierra de las Planchadas, near Rio Chaschuil. Geochemical and isotope data also demonstrate the similarity of the K-bentonite and Chaschuil rhyolite parent magmas. Thus, it is highly probable that the Famatinian arc volcanoes provided the ash for the K-bentonite horizons, suggesting proximity to the Precordillera terrane during the deposition of the Lower Cambrian to Middle Ordovician platform carbonates. This implication supports a mid-Ordovician collision model, but could also be compatible with a parautochthonous model for docking of the Precordillera terrane, by movement along the Pacific margin of Gondwana, rather than across the Iapetus Ocean.
Keywords: UPb, SHRIMP, Ordovician, Gondwana, terranes.
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