Mostrar el registro sencillo del ítem

dc.contributor.author
Weinberg, Roberto F.  
dc.contributor.author
Becchio, Raul Alberto  
dc.contributor.author
Farias, Pablo  
dc.contributor.author
Suzaño, Nestor Omar  
dc.contributor.author
Sola, Alfonso Manuel  
dc.date.available
2019-12-30T16:37:55Z  
dc.date.issued
2018-12  
dc.identifier.citation
Weinberg, Roberto F.; Becchio, Raul Alberto; Farias, Pablo; Suzaño, Nestor Omar; Sola, Alfonso Manuel; Early Paleozoic accretionary orogenies in NW Argentina: Growth of West Gondwana; Elsevier Science; Earth-science Reviews; 187; 12-2018; 219-247  
dc.identifier.issn
0012-8252  
dc.identifier.uri
http://hdl.handle.net/11336/93262  
dc.description.abstract
Two Early Paleozoic orogenic cycles in the Gondwana margin of NW Argentina were driven by subduction, and interrupted by collision of continental ribbons of Laurentian affinity. Subduction started at the passive margin of Gondwana, possibly in response to the end of amalgamation of the supercontinent. The passive margin was underlain by a hyper-extended continent-ocean transition, and low-angle subduction gave rise to a wide and hot fore-arc region during the Pampean orogenic cycle. The arrival of the first continent ribbon ended the Pampean cycle, steepened the subduction, further heating the fore-arc and restarting arc magmatism, after a magmatic lull, 250–300 km trenchwards, initiating the Famatinian orogenic cycle. This cycle started with a 30 Ma-long period of extension and marine sedimentation, followed by the arrival of the second continent ribbon and inversion the back-arc, initiating a ~20 Ma-long shortening event culminating with the shutting down of the arc. This event gave rise to a 300 km-wide, low-topography, hot orogeny. Thus, the many peculiarities of the two Paleozoic orogens of NW Argentina result from a subduction history that efficiently transferred heat to a 300–400 km-wide belt of turbidite-dominated sediments, that was first part of the Pampean fore-arc and then part of the Famatinian retroarc, developed at the extended continental margin of Gondwana. The two orogenies with continued high heat flux lasted ~110 Ma, giving rise to two calc-alkaline arcs separated by a 300 km belt of high-T – low-P migmatites and peraluminous granites formed by anatexis of sediments deposited on the passive margin as well as those deposited in the wide Pampean fore-arc. These turbidite-dominated sequences were metamorphosed and melted to form a continental crystalline basement and accreted to the cratonic margin, adding 500 km of crystalline rocks to the margin of Gondwana, at the same time that a similar process was happening in eastern Australia along the same continental margin. Interestingly this wide accretionary orogen has now become the region where the Andean system developed a wide orogeny above flat-slab subduction.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Elsevier Science  
dc.rights
info:eu-repo/semantics/restrictedAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/  
dc.subject
ACCRETIONARY OROGENY  
dc.subject
FAMATINIAN OROGEN  
dc.subject
PAMPEAN OROGEN  
dc.subject
PUNCOVISCANA SEQUENCE  
dc.subject
TECTONICS  
dc.subject.classification
Geología  
dc.subject.classification
Ciencias de la Tierra y relacionadas con el Medio Ambiente  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Early Paleozoic accretionary orogenies in NW Argentina: Growth of West Gondwana  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2019-10-18T18:26:51Z  
dc.journal.volume
187  
dc.journal.pagination
219-247  
dc.journal.pais
Países Bajos  
dc.journal.ciudad
Amsterdam  
dc.description.fil
Fil: Weinberg, Roberto F.. Monash University; Australia  
dc.description.fil
Fil: Becchio, Raul Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Investigaciones en Energía no Convencional. Universidad Nacional de Salta. Facultad de Ciencias Exactas. Departamento de Física. Instituto de Investigaciones en Energía no Convencional; Argentina  
dc.description.fil
Fil: Farias, Pablo. Monash University; Australia  
dc.description.fil
Fil: Suzaño, Nestor Omar. Universidad Nacional de Jujuy. Instituto de Geología Minera; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Investigaciones en Energía no Convencional. Universidad Nacional de Salta. Facultad de Ciencias Exactas. Departamento de Física. Instituto de Investigaciones en Energía no Convencional; Argentina  
dc.description.fil
Fil: Sola, Alfonso Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Salta. Facultad de Cs.naturales. Cátedra de Petrología Geonorte; Argentina  
dc.journal.title
Earth-science Reviews  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.earscirev.2018.10.001  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S001282521830309X