Pampia: A large cratonic block missing in the Rodinia supercontinent

The large cratonic block of Pampia, at present in southern South America, is commonly missing in recent comprehensive reconstructions of Rodinia. This block was the conjugate margin of the Amazonia craton that corresponds to the W-NW-trending segment of the Sunsás orogen. This segment developed betw...

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Autor principal: Ramos, V.A
Otros Autores: Vujovich, G., Martino, R., Otamendi, J.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2010
Acceso en línea:Registro en Scopus
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100 1 |a Ramos, V.A. 
245 1 0 |a Pampia: A large cratonic block missing in the Rodinia supercontinent 
260 |c 2010 
270 1 0 |m Ramos, V.A.; Laboratorio de Tectónica Andina, FCEyN, Universidad de Buenos Aires, Buenos Aires, Argentina; email: andes@gl.fcen.uba.ar 
506 |2 openaire  |e Política editorial 
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520 3 |a The large cratonic block of Pampia, at present in southern South America, is commonly missing in recent comprehensive reconstructions of Rodinia. This block was the conjugate margin of the Amazonia craton that corresponds to the W-NW-trending segment of the Sunsás orogen. This segment developed between Sucre in Bolivia and Corumbá in Brazil as a result of a Mesoproterozoic collision. The western margin of Pampia partially coincides with the southern part of the Arequipa-Antofalla terrane that was also amalgamated during the Mesoproterozoic. The Cuyania terrane, a Laurentian rifted continental block, was accreted to the southern sector of this margin of Pampia in middle Ordovician times. The northern sector of the eastern margin of Pampia is the lower plate of the Brasiliano belt developed along the Paranapanema craton during the early Cambrian collision associated with the closure of the Clymene Ocean. The southern sector of the eastern margin partially coincides with the southern extension of the Transbrasiliano lineament, which juxtaposed the Rio de La Plata Craton with the Pampia cratonic block. Along this eastern margin the Pampean-Paraguay orogen was formed during the late Brasiliano cycle in latest Proterozoic-Early Cambrian time. The southern margin was generated by the collision of Patagonia during late Paleozoic times. This cratonic block of Pampia, so defined, has western and northern sectors formed by Mesoproterozoic orogens, while the eastern sector is partially formed by juvenile Neoproterozoic crust, although older rocks cannot be ruled out. The Pampia cratonic block was the locus of several magmatic belts associated with important metamorphism during the Paleozoic and preserved in the central part at lower crustal levels. © 2010 Elsevier Ltd.  |l eng 
536 |a Detalles de la financiación: x-182, PICTR 20298/4 
536 |a Detalles de la financiación: PIP 5437 
536 |a Detalles de la financiación: The present research was funded by the Ubacyt x-182 (V.A.R.); PICTR 20298/4 (J.O. and G.V.) and CONICET PIP 5437 (G.V.). The authors want to thank Drs. Umberto Cordani and Bley Brito Neves for their critical review of an early version of this manuscript. Llambías et al., 2003 E.J. Llambías D. Gregori M.A.S. Basei R. Varela C. Prozzi 
593 |a Laboratorio de Tectónica Andina, FCEyN, Universidad de Buenos Aires, Buenos Aires, Argentina 
593 |a Cátedra de Geología Tectónica, Universidad Nacional de Córdoba, Córdoba, Argentina 
593 |a Departamento de Geología, Universidad Nacional de Río Cuarto, Río Cuarto, Argentina 
593 |a CONICET(Consejo Nacional de Investigaciones Científicas y Técnicas), Argentina 
690 1 0 |a AMAZONIA 
690 1 0 |a ANDES 
690 1 0 |a CLYMENE 
690 1 0 |a GRENVILLE 
690 1 0 |a MESOPROTEROZOIC 
690 1 0 |a PARANAPANEMA 
690 1 0 |a CAMBRIAN 
690 1 0 |a COLLISION ZONE 
690 1 0 |a CRATON 
690 1 0 |a CRUSTAL STRUCTURE 
690 1 0 |a METAMORPHISM 
690 1 0 |a OROGENY 
690 1 0 |a PALEOZOIC 
690 1 0 |a PROTEROZOIC 
690 1 0 |a RECONSTRUCTION 
690 1 0 |a RODINIA 
690 1 0 |a SUPERCONTINENT 
690 1 0 |a AMAZONIA 
690 1 0 |a ANDES 
700 1 |a Vujovich, G. 
700 1 |a Martino, R. 
700 1 |a Otamendi, J. 
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