Emplacement and temporal constraints of the Gondwanan intrusive complexes of northern Patagonia: La Esperanza plutono-volcanic case
dc.contributor.author | Martinez Dopico, Carmen I | |
dc.contributor.author | Lopez de Luchi, Mónica G | |
dc.contributor.author | Rapalini, A.E. | |
dc.contributor.author | Wemmer, Klaus | |
dc.contributor.author | Fanning, Christopher Mark | |
dc.contributor.author | Basei, Miguel Angelo Stipp | |
dc.date.accessioned | 2020-04-07T00:18:12Z | |
dc.date.issued | 2017-08-21 | |
dc.date.updated | 2019-11-25T07:50:41Z | |
dc.description.abstract | Two main lines of evidence disagree whether or not the Patagonian blocks collided with Gondwana. All models invoke the voluminous magmatism of the La Esperanza Complex as evidence for active subduction magmatic arc or to a postcollisional setting. The evolution of this bimodal igneous suite is reassessed with field, geochronological (SHRIMP U-Pb zircon and K-Ar mica) and petrophysical data. Emplacement of high-K calk-alkaline granitic magmas occurred at shallow crustal levels (2-8 +/- 2 km depth) related to the development and collapse of a caldera associated with a regional NW-SE structural trend. Magmatism involved intermediate hybrid pulses at 273 +/- 2 Ma and 255 +/- 2 Ma (Prieto Granodiorite) that shifted like a yo-yo to acidic magmas at 260 +/- 2 Ma and 250 +/- 2 Ma (Donosa and Calvo granites). Absence of solid-state deformation features and the low anisotropy degrees in the granites indicate that its fabric is magmatic in origin. Magnetic fabric in granodiorites displays a concentrical pattern with subhorizontal foliations and lineations. Parallel to the volcanic axis, magnetic foliations and moderately plunging lineations indicate a common feeder system for plutonics and volcanics. Donosa Granite shows a discordant pattern with WNW-ESE ENE-WSW trending low plunging lineations and foliations. The plutono-volcanic system construction (273-255 Ma) followed NW-SE and NE-SW diamond shape faults trends and supracrustal discontinuities. Magmatic Climax is bracketed at 260 Ma. The collapse of the edifice is evidenced by the intrusion of acid magma plugs and dike swarms between 250 and 246 Ma. A similar age range was identified in other areas of Patagonia related to syn and postcollisional tectonic events. No evidence of tectonic activity such as major uplift, metamorphism or thrusting was found excepting regional strike-slip faulting and extension. Therefore, La Esperanza Complex is a high crustal level episode, and as such may not have structurally recorded an active collision during its crystallization and cooling. | en_AU |
dc.description.sponsorship | This research has been supported by grants PIP CONICET 2009- 01502, 2012-112, and 2011-0100294, PICT 2006-1074, 2011-0956, 2011-100597 and UBACyT X183. | en_AU |
dc.format.extent | 21 pages | en_AU |
dc.format.mimetype | application/pdf | en_AU |
dc.identifier.issn | 0040-1951 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/202769 | |
dc.language.iso | en_AU | en_AU |
dc.publisher | Elsevier | en_AU |
dc.rights | © 2017 Elsevier B.V. | en_AU |
dc.source | Tectonophysics | en_AU |
dc.subject | Subvolcanic magmatic complexes, SHRIMP U-Pb dating, Anisotropy of magnetic susceptibility, Permian, Gondwana, Patagonia | en_AU |
dc.title | Emplacement and temporal constraints of the Gondwanan intrusive complexes of northern Patagonia: La Esperanza plutono-volcanic case | en_AU |
dc.type | Journal article | en_AU |
dcterms.dateAccepted | 2017-05-19 | |
local.bibliographicCitation.lastpage | 269 | en_AU |
local.bibliographicCitation.startpage | 249 | en_AU |
local.contributor.affiliation | Martinez Dopico, Carmen I, Universidad de Buenos Aires | en_AU |
local.contributor.affiliation | Lopez de Luchi, Mónica G, Ciudad Universitaria | en_AU |
local.contributor.affiliation | Rapalini, A.E., Universidad de Buenos Aires | en_AU |
local.contributor.affiliation | Wemmer, Klaus, University of Göttingen | en_AU |
local.contributor.affiliation | Fanning, Christopher, College of Science, The Australian National University | en_AU |
local.contributor.affiliation | Basei, Miguel Angelo Stipp, Universidade de Sao Paulo | en_AU |
local.contributor.authoremail | mark.fanning@anu.edu.au | en_AU |
local.contributor.authoruid | Fanning, Christopher, u4029993 | en_AU |
local.description.embargo | 2037-12-31 | |
local.description.notes | Imported from ARIES | en_AU |
local.identifier.absfor | 040304 - Igneous and Metamorphic Petrology | en_AU |
local.identifier.absfor | 040303 - Geochronology | en_AU |
local.identifier.absfor | 040203 - Isotope Geochemistry | en_AU |
local.identifier.absseo | 970104 - Expanding Knowledge in the Earth Sciences | en_AU |
local.identifier.ariespublication | u4485658xPUB1154 | en_AU |
local.identifier.citationvolume | 712-713 | en_AU |
local.identifier.doi | 10.1016/j.tecto.2017.05.015 | en_AU |
local.identifier.essn | 1879-3266 | en_AU |
local.identifier.scopusID | 2-s2.0-85020315900 | |
local.identifier.thomsonID | 000409284500021 | |
local.identifier.uidSubmittedBy | u4485658 | en_AU |
local.publisher.url | https://www.elsevier.com/ | en_AU |
local.type.status | Published Version | en_AU |
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