Oxygen isotope systematics of South African olivine melilitites and implications for HIMU mantle reservoirs

被引:36
作者
Day, James M. D. [1 ]
Peters, Bradley J. [1 ]
Janney, Philip E. [2 ]
机构
[1] Univ Calif San Diego, Scripps Inst Oceanog, Geosci Res Div, La Jolla, CA 92093 USA
[2] Univ Cape Town, Dept Geol Sci, ZA-7701 Rondebosch, South Africa
基金
美国国家科学基金会;
关键词
Oxygen isotopes; Trace elements; Olivine; Melilitite; HIMU; Mantle; RECYCLED OCEANIC LITHOSPHERE; TRACE-ELEMENTS; ORIGIN; CRUST; KIMBERLITE; BASALTS; EVOLUTION; XENOLITHS; COMPLEX; ROCKS;
D O I
10.1016/j.lithos.2014.05.009
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
Oxygen isotopes are useful tracers of silicate melt generation processes because of the relatively constant abundance of oxygen in silicate reservoirs and the large isotopic fractionation that can occur between O-18 and O-16 during low (<350 degrees C) and high (>350 degrees C) temperature alteration processes at Earth's surface. Studies of oceanic island basalts (OIB) have demonstrated the important role of assimilation of hydrothermal altered crust on O-18/O-16 ratios, as well as evidence that some OIB mantle sources contain recycled oceanic or continental crust and lithosphere based on correlations between oxygen and radiogenic isotopes. To further investigate how oxygen isotope signatures may be used as tracers in intraplate volcanic rocks, we report olivine compositions from South African olivine melilitites. Olivine melilitites are considered to be related to Group 1 kimberlites and form from asthenospheric melting beneath mature oceanic islands or under off-craton continental lithosphere. South African olivine melilitites also exhibit radiogenic isotopic signatures similar to high-mu (HIMU; high-U-238/Pb-204) OIB, suggesting sources containing subducted oceanic lithosphere. Olivine from South African melilitites has trace element compositions that are consistent with a magmatic origin from a HIMU-type mantle melt and have a remarkably restricted range in primary O-18/O-16 ratios (delta O-18 = 4.99-5.26%o; Average = 5.14 +/- 0.17%o, 2 sigma) that are within the mantle olivine range (delta O-18 = 5.2 +/- 0.3%o). These compositions indicate that South African olivine melilitites require a HIMU mantle source with the oxygen isotope characteristics of ambient peridotite mantle and can be explain through either: (1) intra-mantle differentiation processes that fractionate U(and Th) from Pb, but not O-18/O-16 ratios, or (2) a dominantly peridotitic source with HIMU-like trace-element and radiogenic isotope characteristics inherited from equilibration and remixing of ancient recycled oceanic lithosphere. In contrast, some HIMU ocean island basalts require mantle sources with low-delta O-18, indicating that they originate from distinct recycled mantle lithologies (e.g., pyroxenite/eclogite). (C) 2014 Elsevier B.V. All rights reserved.
引用
收藏
页码:76 / 84
页数:9
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