The Estancia Glencross Area EGA volcanic rocks form a series of five isolated buttes located at the southern end ca. 52°S of the discontinuous belt of Cenozoic basaltic lava formations occurring in the extra-Andean Patagonia. EGA volcanics are subalkaline basalts and basaltic andesites erupted at 8.0-8.5 Ma in a region closely behind the Andean Cordillera. EGA volcanism predated by about 4-5 My the onset of the volcanism in the nearby Pali Aike Volcanic Field, which produced highly primitive, alkaline lavas. Incompatible trace-element distributions and Sr-Nd isotope compositions of EGA rocks are those typical of within-plate OIB-type basalts and are indicative of minimal interaction of sub-lithospheric magmas with enriched reservoirs. The geochemical characteristics of EGA volcanics, as well as their age and location are consistent with a model of slab window opening beneath this region. The high silica content and the garnet signature of the estimated EGA primary magma are explained by a two-stage process involving the initial production of melts from a garnet lherzolite source followed by the reaction of these melts with harzburgite country rocks during their ascent through the mantle lithosphere. The melt/harzburgite reaction, favoured by a slow melt ascent rate, as well as the low magma production at EGA, are likely related to the dominantly compressive stress regime operating in this area during Late Miocene.

Slab window-related magmatism from southernmost South America: the Late Miocene mafic volcanics from the Estancia Glencross Area (ca. 52°S, Argentina?Chile)

Agostini S;
2001

Abstract

The Estancia Glencross Area EGA volcanic rocks form a series of five isolated buttes located at the southern end ca. 52°S of the discontinuous belt of Cenozoic basaltic lava formations occurring in the extra-Andean Patagonia. EGA volcanics are subalkaline basalts and basaltic andesites erupted at 8.0-8.5 Ma in a region closely behind the Andean Cordillera. EGA volcanism predated by about 4-5 My the onset of the volcanism in the nearby Pali Aike Volcanic Field, which produced highly primitive, alkaline lavas. Incompatible trace-element distributions and Sr-Nd isotope compositions of EGA rocks are those typical of within-plate OIB-type basalts and are indicative of minimal interaction of sub-lithospheric magmas with enriched reservoirs. The geochemical characteristics of EGA volcanics, as well as their age and location are consistent with a model of slab window opening beneath this region. The high silica content and the garnet signature of the estimated EGA primary magma are explained by a two-stage process involving the initial production of melts from a garnet lherzolite source followed by the reaction of these melts with harzburgite country rocks during their ascent through the mantle lithosphere. The melt/harzburgite reaction, favoured by a slow melt ascent rate, as well as the low magma production at EGA, are likely related to the dominantly compressive stress regime operating in this area during Late Miocene.
2001
Istituto di Geoscienze e Georisorse - IGG - Sede Pisa
57
67
89
Slab windows
Mafic rocks
Patagonia
Petrology
Geodynamics
Field works carried out in collaboration with colleagues of Patagonia University have evidenced for the first time the presence of an Upper Miocene magmatism in the southern part of Argentina. Such a magmatism along with that previously investigated has allowed to propose a geodynamical model that justifies this back-arc alkaline magmatism of the Andean Arc. The astenoshperic upwelling is related to slab-window forming as the result of an oblique collision of the north-trending Pacific Chilean Ridge. Lithos is an international journal mainly devoted to the petrologic significance of magmatic and metamorphic rocks in their geodynamical context. In the last few years, Lithos has improved the quality of the published papers and has achieved a high impact factor
0
info:eu-repo/semantics/article
262
D'Orazio M. ; Agostini S. ; Innocenti F. ; Haller M.J. ; Manetti P. ; Mazzarini F.
01 Contributo su Rivista::01.01 Articolo in rivista
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/24355
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