The accretionary history of southern South America from the latest Proterozoic to the Late Palaeozoic: Some palaeomagnetic constraints
It is now accepted that southern South America was formed from several terranes of diverse origin and evolution. However, a detailed history of the accretionary processes has not been unravelled yet. Palaeomagnetism can play an important role in such an endeavour. Palaeomagnetic constraints on the t...
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2005
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| LEADER | 40019caa a22021737a 4500 | ||
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| 001 | PAPER-3983 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230607131849.0 | ||
| 008 | 190411s2005 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-23844497824 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Rapalini, A.E. | |
| 245 | 1 | 4 | |a The accretionary history of southern South America from the latest Proterozoic to the Late Palaeozoic: Some palaeomagnetic constraints |
| 260 | |c 2005 | ||
| 270 | 1 | 0 | |m Rapalini, A.E.; INGEODAV, Departamento de Cs. Geológicas, Fac. Cs. Exactas y Naturales, Pabellon 2, C1428EHA Buenos Aires, Argentina; email: rapalini@gl.fcen.uba.ar |
| 506 | |2 openaire |e Política editorial | ||
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| 504 | |a Ramos, V., Keppie, D., (1999) Laurentia - Gondwana Connections Before Pangea, 336. , (eds) Geological Society of America Special Paper | ||
| 504 | |a Ramos, V.A., Jordan, T.E., Allmendinger, R.W., Mpodozis, C., Kay, S.M., Cortés, J.M., Palma, M., Paleozoic terranes of the Central Argentine - Chilean Andes (1986) Tectonics, 5, pp. 855-880 | ||
| 504 | |a Ramos, V.A., Vujovich, G., Mahlburg Kay, S., McDonough, M., La orogénesis de Grenville en las Sierras Pampeanas Occidentales: La Sierra de Pie de Palo y su integración al supercontinente proterozoico (1993) 12th Congreso Geológico Argentino, 3, pp. 343-357. , Mendoza, Asociación Geológica Argentina, Buenos Aires | ||
| 504 | |a Ramos, V.A., Dallmeyer, R.D., Vujovich, G., Time constraints on the Early Paleozoic docking of the Precordillera, central Argentina (1998) The Proto-Andean Margin of Gondwana, 142, pp. 143-158. , Pankhurst, R.J. & Rapela, C.W. (eds) Geological Society, London, Special Publications | ||
| 504 | |a Ramos, V.A., Escayola, M., Mutti, D.I., Vujovich, G.I., Proterozoic - Early Paleozoic ophiolites of the Andean basement of southern South America (2000) Ophiolites and Oceanic Crust: New Insights from Field Studies and Ocean Drilling Program, 349, pp. 331-349. , Dilek, Y., Moores, E.M., Elthon, D., & Nicolas, A. (eds) Geological Society of America Special Paper | ||
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| 504 | |a Rapalini, A.E., Astini, R.A., Paleomagnetic confirmation of the Laurentian origin of the Argentine Precordillera (1998) Earth and Planetary Science Letters, 155, pp. 1-14 | ||
| 504 | |a Rapalini, A.E., Astini, R.A., La Remagnetización Sanrafaélica de la Precordillera: Nuevas Evidencias (2005) Revista De La Asociación Geológica Argentina, 60. , in press | ||
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| 504 | |a Rapalini, A.E., Tarling, D.H., Multiple magnetizations in the Cambrian - Ordovician carbonate platform of the Argentine Precordillera and their tectonic implications (1993) Tectonophysics, 227, pp. 49-62 | ||
| 504 | |a Rapalini, A.E., Vilas, J.F., Preliminary paleomagnetic data from the Sierra Grande Formation: Tectonic consequences of the first Middle Paleozoic paleopoles from Patagonia (1991) Journal of South American Earth Sciences, 4, pp. 25-41 | ||
| 504 | |a Rapalini, A.E., Vilas, J.F., Bobbio, M.L., Valencio, D.A., Geodynamic interpretations from paleomagnetic data of Late Paleozoic rocks in the Southern Andes (1989) Deep Structure and Past Kinematics of Accreted Terranes, 50, pp. 41-57. , Hillhouse, J.W. (ed.) American Geophysical Union, Geophysical Monograph Series | ||
| 504 | |a Rapalini, A.E., Tarling, D.H., Turner, P., Flint, S., Vilas, J.F., Palaeomagnetism of the Carboniferous Tepuel Group, central Patagonia, Argentina (1994) Tectonics, 13, pp. 1277-1294 | ||
| 504 | |a Rapalini, A.E., Astini, R.A., Conti, C.M., Paleomagnetic constraints on the tectonic evolution of Paleozoic suspect terranes from southern South America (1999) Laurentia - Gondwana Connections Before Pangea, 336, pp. 171-182. , Ramos, V. & Keppie, D. (eds) Geological Society of America Special Paper | ||
| 504 | |a Rapalini, A.E., Bordonaro, O., Berquo, T.S., Paleomagnetic study of Cambrian - Ordovician rocks in the Eastern Precordillera of Argentina: Some constraints on the Andean uplift of this block (2000) Tectonophysics, 326, pp. 173-184 | ||
| 504 | |a Rapalini, A.E., Velasco, M.S., Koukharsky, M., New paleomagnetic data from the Western Puna of Argentina: Some tectonic speculations on its Early Paleozoic evolution (2002) 5th International Symposium on Andean Geodynamics, pp. 505-508. , Toulouse, France, Extended Abstracts, Institut de recherche pour le développement, Paris | ||
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| 504 | |a Zimmermann, U., Bahlburg, H., The evolution of the Ordovician southern Puna retro-arc basin (NW Argentina): Provenance analysis and paleotectonic setting (1999) 4th International Symposium of Andean Geodynamics, pp. 830-831. , Göettingen (Germany), Abstracts, Institut de recherche pour le développement, Paris | ||
| 520 | 3 | |a It is now accepted that southern South America was formed from several terranes of diverse origin and evolution. However, a detailed history of the accretionary processes has not been unravelled yet. Palaeomagnetism can play an important role in such an endeavour. Palaeomagnetic constraints on the tectonic evolution of this region in the Proterozoic and Palaeozoic are reviewed and discussed. Data from the Rio de la Plata craton suggest that this block was already attached to most major Gondwana blocks by the end of the Proterozoic and may have formed a single continental mass with Congo-Sao Francisco, West Nile and Arabia throughout most of the Vendian. A large ocean separating these cratons from Amazonia and West Africa, prior to Gondwana assembly, is supported by available palaeomagnetic data. To the west of the Rio de la Plata craton is the Pampia terrane. Despite lack of palaeomagnetic data, geological evidence supports a model of Early Cambrian collision between these blocks. An Early Ordovician magmatic arc, the Famatina-Eastern Puna belt, which had developed on the western margin of the already accreted Pampia terrane, shows a systematic pattern of large clockwise rotation that has been interpreted as representative of the whole terrane. The favoured tectonic model portrays a continental magmatic arc with a back-arc basin to the east that was closed when the terrane rotated. There is little doubt of a Laurentian origin for the Cuyania (Precordillera) terrane, given the amount and diversity of evidence, including palaeomagnetism. The tectonic mechanism for accretion and its timing are still controversial. New palaeomagnetic data from Late Ordovician rocks of Cuyania support the 'Laurentian plateau' hypothesis, which suggests that Cuyania was still linked to Laurentia well into the Ordovician. Nevertheless, these new data do not rule out the more generally favoured 'microcontinent model'. To the west of Cuyania is the Chilenia terrane, separated by a belt of ophiolites of Late Ordovician age. Very little is known about this terrane, although some U-Pb ages and Nd model ages point to a Laurentian origin for its basement. Lack of palaeomagnetic data precludes determining its kinematic evolution. The Arequipa-Antofalla block may actually be a composite terrane. Palaeomagnetic data obtained so far come exclusively from the southern Antofalla block. Recently acquired data in the western Puna of Argentina confirm the originally proposed distribution of Early Palaeozoic palaeomagnetic poles, which, despite several uncertainties, delineate a pattern of significant counterclockwise rotations with a possible anomaly in palaeolatitude for the late Cambrian. The data suggest a major tectonic discontinuity between the Eastern and Western Puna of Argentina in the Early Palaeozoic. Four palaeomagnetic poles of Devonian to Permian age from the North Patagonian Massif are consistent in position and age with the Gondwana apparent polar wander path, suggesting that both continental masses have not experienced major relative displacement since the Devonian. The data do not, however, rule out a restricted separation of Patagonia orthogonal to its northern boundary in the Early or Middle Palaeozoic and subsequent collision in the Late Palaeozoic. © The Geological Society of London 2005. |l eng | |
| 593 | |a INGEODAV, Departamento de Cs. Geológicas, Fac. Cs. Exactas y Naturales, Pabellon 2, C1428EHA Buenos Aires, Argentina | ||
| 690 | 1 | 0 | |a ACCRETIONARY PRISM |
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| 651 | 4 | |a SOUTH AMERICA | |
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