Geochemistry of eclogite xenoliths from the Udachnaya Kimberlite Pipe: Section of ancient oceanic crust sampled

被引:29
|
作者
Agashev, A. M. [1 ]
Pokhilenko, L. N. [1 ]
Pokhilenko, N. P. [1 ,2 ]
Shchukina, E. V. [1 ,2 ]
机构
[1] Russian Acad Sci, Siberian Branch, VS Sobolev Inst Geol & Mineral, Koptyuga Pr 3, Novosibirsk 630090, Russia
[2] Novosibirsk State Univ, Pirogova St 2, Novosibirsk 630090, Russia
基金
俄罗斯科学基金会; 俄罗斯基础研究基金会;
关键词
Eclogite; Xenolith; Lithospheric mantle; Geochemistry; Oceanic crust; Subduction; DIAMOND-BEARING ECLOGITE; LITHOSPHERIC MANTLE; SUBDUCTION ZONES; TRACE-ELEMENTS; MGO ECLOGITES; SOUTH-AFRICA; WEST-AFRICA; WHOLE-ROCK; CONSTRAINTS; SIBERIA;
D O I
10.1016/j.lithos.2018.05.027
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
A suite of seventeen unique, large, and fresh eclogite xenoliths from the Udachnaya pipe have been studied for their whole-rock and mineral major- and trace-element compositions. Based on their major-element compositions, the Udachnaya edogites can be subdivided in two groups: high magnesian (Mg#68.8-81.9) and low magnesian (Mg#56.8-59). The two eclogite groups are clearly different in the style of correlation between major elements. Positive correlations of FeO and CaO with MgO are observed in the low-magnesian group, whereas these correlations are negative in the high-magnesian group. In terms of trace element composition, the Udachnaya eclogites are enriched over Primitive Mantle, but comparable to mid-ocean-ridge basalt composition, except for significant enrichment in large-ion lithophile elements (LILE; Rb, Ba, K, Sr). Most of the samples show a positive Eu anomaly, irrespective of group. Reconstructed whole-rock composition from clinopyroxene and garnet modal abundances contains much less incompatible elements (LILE, light rare earth elements, high field strength elements) than measured composition. Approximately 60 to 100% of the middle rare earth elements, Zr, and Hf, and nearly 100% of the heavy rare earth elements, Co, V, and Sc of the whole-rock budget are concentrated in Gar and Cpx. Variations in major element compositions cover a full section of the modern and Archaean oceanic crust, from troctolite, through gabbroic rocks, to basalts. The low-Mg# eclogites could have formed from upper oceanic crust protoliths, being a mixture of basalts and gabbro, whereas the high-Mg# eclogites are originated from gabbro-troctolite section of the lower oceanic crust. Concordant variations of Eu anomaly with the Lu/Sr ratio and the V and Ni contents in the eclogite compositions are in agreement with the fractionation of plagioclase, clinopyroxene, and olivine in their low-pressure precursor rocks. Negative correlations of SiO2 and MgO, and a low Nd/Yb-NMORB ratio, in the low-Mg# eclogites are in agreement with partial melt loss, but the presence of accessory quartz limits the degree of melting to 13%. Major and trace element compositions suggest that the high-Mg# eclogites, and, consequently, the lower oceanic crust, could not have experienced significant melt loss, and subduction in the Archaean may have been essentially dry, compared to the present day. (C) 2018 Elsevier B.V. All rights reserved.
引用
收藏
页码:187 / 200
页数:14
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