The late Cretaceous lithospheric mantle beneath the Central Andes: Evidence from phase equilibria and composition of mantle xenoliths

被引:35
作者
Lucassen, F
Franz, G
Viramonte, J
Romer, RL
Dulski, P
Lang, A
机构
[1] Free Univ Berlin, FB Geowissensch, D-12249 Berlin, Germany
[2] Geoforschungszentrum Potsdam, D-14473 Potsdam, Germany
[3] TU Berlin, Petrol EB15, D-10623 Berlin, Germany
[4] Univ Nacl Salta, RA-4400 Salta, Argentina
[5] GEONORTE, RA-4400 Salta, Argentina
[6] Consejo Nacl Invest Cient & Tecn, RA-4400 Salta, Argentina
[7] WWU Munster, Zent Lab Geochronol, D-48149 Munster, Germany
关键词
Central Andes; peridotite xenoliths; thermobarometry; chemical composition; isotopic composition; mantle metasomatism;
D O I
10.1016/j.lithos.2004.08.002
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Temperature estimates and chemical composition of mantle xenoliths from the Cretaceous rift system of NW Argentina (26 degrees S) constrain the rift evolution and chemical and physical properties of the lithospheric mantle at the eastern edge of the Cenozoic Andean plateau. The xenolith suite comprises mainly spinel lherzolite and subordinate pyroxenite and carbonatized lherzolite. The spinel lherzolite xenoliths equilibrated at high-T (most samples >1000 degrees C) and P below garnet-in. The Sm-Nd systematics of compositionally unzoned clino- and orthopyroxene indicate a Cretaceous minimum age for the high-T regime, i.e., the asthenosphere/lithosphere thermal boundary was at ca. 70 km depth in the Cretaceous rift. Major elements and Cr, Ni, Co and V contents of the xenoliths range between values of primitive and depleted mantle. Calculated densities based on the bulk composition of the xenoliths are <3280 kg/m(3) for the estimated P-T conditions and indicate a buoyant, stable upper mantle lithosphere. The well-equilibrated metamorphic fabric and mineral paragenesis with the general lack of high-T hydrous phases did not preserve traces of metasomatism in the mantle xenoliths. Late Mesozoic metasomatism, however, is obvious in the gradual enrichment of Sr, U, Th and light to medium REE and changes in the radiogenic isotope composition of an originally depleted mantle. These changes are independent of the degree of depletion evidenced by major element composition. Nd-143/Nd-144(i) ratios of clinopyroxene from the main group of xenoliths decrease with increasing Nd content from >0.5130 (depleted samples) to ca. 0.5127 (enriched samples). Sr-87/Sr-86(i) ratios (0.7127-0.7131, depleted samples; 0.7130-0.7134, enriched samples) show no variation with variable Sr contents. Pb-i isotope ratios of the enriched samples are rather radiogenic (Pb-206/Pb-204(i) 18.8-20.6, Pb-207/Pb-204(i) 15.6-15.7, Pb-208/Pb-204(i) 38.6-47) compared with the Pb isotope signature of the depleted samples. The large scatter and high values of 208Pb/204Pbi ratios of many xenoliths indicates at least two Pb sources that are characterized by similar U/Pb but by different Th/Pb ratios. The dominant mantle type in the investigated system is depleted mantle according to its Sr and Nd isotopic composition with relatively radiogenic Pb isotope ratios. This mantle is different from the Pacific MORB source and old subcontinental mantle from the adjacent Brazilian Shield. Its composition probably reflects material influx into the mantle wedge during various episodes of subduction that commenced in early Paleozoic or even earlier. Old subcontinental mantle was already replaced in the Paleozoic, but some inheritance from old mantle lithosphere is represented by rare xenoliths with isotope signatures indicating a Proterozoic origin. (C) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:379 / 406
页数:28
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