Age and composition of granulite xenoliths from Paso de Indios, Chubut province, Argentina

被引:15
作者
Castro, Antonio [1 ]
Aragon, Eugenio [2 ]
Diaz-Alvarado, Juan [3 ]
Blanco, Idael [4 ]
Garcia-Casco, Antonio [4 ]
Vogt, Katharina [5 ]
Liu, D-Y. [6 ]
机构
[1] Univ Huelva, Dept Geol, Campus Carmen, Huelva 21071, Spain
[2] Fac Ciencias Nat & Museo UNLP La Plata, Ctr Invest Geol UNLP CONICET, Buenos Aires, DF, Argentina
[3] Univ Huelva, Dept Geodinam & Paleontol, Huelva 21071, Spain
[4] Univ Granada, Dept Mineral Petrol, E-18071 Granada, Spain
[5] ETH, Inst Geophys, Zurich, Switzerland
[6] Chinese Acad Geol Sci, Beijing SHRIMP Ctr, Beijing, Peoples R China
关键词
Granulite xenoliths; Lower crust; Jurassic magmatism; South America; BREAK-UP; MANTLE; PATAGONIA; MAGMATISM; CONSTRAINTS; EVOLUTION; GARNET; CRUST; ARCS;
D O I
10.1016/j.jsames.2011.06.001
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Granulite xenoliths enclosed in Paleogene alkali basalts from the locality of Paso de Indios in The Argentinean Patagonia, have been studied for petrology, geochemistry and U-Pb SHRIMP zircon geochronology. These are lower crust xenoliths composed of pyroxene and plagioclase dominantly. Symplectitic overgrowths with olivine and new pyroxene-plagioclase formation around the large pyroxene crystals are common. The study of phase equilibrium yields a decompression path from pressure 0.9 GPa at temperatures of about 1000 degrees C. The major element composition does not correspond with any known basaltic or andesitic magmas. They have SiO2 < 50 wt% and MgO = 6 wt% and lower, very close in composition to the bulk lower continental crust composition. They are extremely depleted in incompatible elements with values as low as Rb = 15.3 to 4.1 ppm; Y = 6.2 to 2.5 ppm; Th = 0.92 to 0.13 ppm; U = 0.51 to 0.22 ppm; Sigma REE = 53 ppm. This depletion is attributed to a residual origin of the granulites. In situ age determination with SHRIMP yields a Concordia age of 175.9 +/- 4.9 Ma with MSWD = 1.4. This age represent the time of complex lithosphere evolution in relation with the formation of this residual crust. (C) 2011 Elsevier Ltd. All rights reserved.
引用
收藏
页码:567 / 574
页数:8
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