Evaluation of petrogenetic models for intermediate and silicic plutonic rocks from the Sierra de Valle Fertil-La Huerta, Argentina: Petrologic constraints on the origin of igneous rocks in the Ordovician Famatinian-Puna paleoarc


Autoria(s): OTAMENDI, J. E.; PINOTTI, L. P.; Basei, Miguel Angelo Stipp; TIBALDI, A. M.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

20/10/2012

20/10/2012

2010

Resumo

The whole Valle Fertil-La Huerta section appears as a calc-alkaline plutonic suite typical of a destructive plate margin. New Sr and Nd isotopic whole-rock data and published whole-rock geochemistry suggest that the less-evolved intermediate (dioritic) rocks can be derived by magmatic differentiation, mainly by hornblende + plagioclase +/- Fe-Ti oxide fractional crystallization, from mafic (gabbroic) igneous precursors. Closed-system differentiation, however, cannot produce the typical intermediate (tonalitic) and silicic (granodioritic) plutonic rocks, which requires a preponderant contribution of crustal components. Intermediate and silicic plutonic rocks from Valle Fertil-La Huerta section have formed in a plate subduction setting where the thermal and material input of mantle-derived magmas promoted fusion of fertile metasedimentary rocks and favored mixing of gabbroic or dioritic magmas with crustal granitic melts. Magma mixing is observable in the field and evident in variations of chemical elemental parameters and isotopic ratios, revealing that hybridization coupled with fractionation of magmas took place in the crust. Consideration of the whole-rock geochemical and isotopic data in the context of the Famatinian-Puna magmatic belt as a whole demonstrates that the petrologic model postulated for the Sierra Valle Fertil-La Huerta section has the potential to explain the generation of plutonic and volcanic rocks across the Early Ordovician paleoarc from central and northwestern Argentina. As the petrologic model does not require the intervention of old Precambrian continental crust, the nature of the basement on which thick accretionary turbiditic sequences were deposited remains a puzzling aspect. Discussion in this paper provides insights into the nature of magmatic source rocks and mechanisms of magma generation in Cordilleran-type volcano-plutonic arcs of destructive plate margins. (C) 2010 Elsevier Ltd. All rights reserved.

Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT)

ANPCYT-Argentina[PICTR 20298/04]

Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT)

ANPCYT-Argentina[PICT 01904/07]

CONICET[PIP 5211]

Consejo Nacional de Investigaciones Científicas y Técnicas de Argentina (CONICET)

SeCyT-UNRC

SeCyT-UNRC

Identificador

JOURNAL OF SOUTH AMERICAN EARTH SCIENCES, v.30, n.1, p.29-45, 2010

0895-9811

http://producao.usp.br/handle/BDPI/30229

10.1016/j.jsames.2010.07.004

http://dx.doi.org/10.1016/j.jsames.2010.07.004

Idioma(s)

eng

Publicador

PERGAMON-ELSEVIER SCIENCE LTD

Relação

Journal of South American Earth Sciences

Direitos

restrictedAccess

Copyright PERGAMON-ELSEVIER SCIENCE LTD

Palavras-Chave #Petrogenesis #Magmatic arc #Cordilleran granitoid #Famatinian #Puna #Sierras Pampeanas #PROTO-ANDEAN MARGIN #SUBDUCTION ZONE MAGMATISM #ISOTOPIC MIXING MODEL #LACHLAN FOLD BELT #U-PB #NW ARGENTINA #NORTHWESTERN ARGENTINA #S-TYPE #METASEDIMENTARY ROCKS #CRUSTAL EVOLUTION #Geosciences, Multidisciplinary
Tipo

article

original article

publishedVersion