In situ perovskite Sr–Nd isotopic constraints on the petrogenesis of the Ordovician
Mengyin kimberlites in the North China Craton
Yue-Heng Yang
a
, Fu-Yuan Wu
a,
⁎, Simon A. Wilde
b
, Xiao-Ming Liu
c
, Yan-Bin Zhang
a
,
Lie-Wen Xie
a
, Jin-Hui Yang
a
a
State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, P. O. Box 9825, Beijing 100029, China
b
Department of Applied Geology, Curtin University of Technology, P. O. Box U1987, Perth, Western Australia 6845, Australia
c
State Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Xi'an 750069, China
abstract article info
Article history:
Received 5 October 2008
Received in revised form 17 February 2009
Accepted 18 February 2009
Editor: R.L. Rudnick
Keywords:
Laser ablation analyses
Sr–Nd–Hf isotopes
Perovskite
Mengyin kimberlite
North China Craton
Precise Sr, Nd and Hf isotopic data are important indicators in deciphering the evolution of magmatic rocks
and their source. However, such data are difficult to obtain for kimberlite, since these rocks are commonly
contaminated by both crustal and mantle materials and also show extensive alteration and weathering
following emplacement. In this study, numerous kimberlitic samples from Mengyin in northeast China were
selected for U–Pb dating and Sr–Nd–Hf isotopic analysis of perovskite. In situ U–Pb analyses of fresh
perovskite yield an age of 470±4 Ma, which is considered the emplacement age of the Mengyin kimberlite.
However, the altered perovskite shows Pb loss and yields Paleozoic-Mesozoic ages, indicating that perovskite
is not as strongly resistant to isotopic modification as previously thought. In situ Sr–Nd isotopic analyses by
laser ablation of perovskite grains collected from the main Mengyin kimberlite record uniform Sr and Nd
isotopic compositions with an average initial
87
Sr/
86
Sr ratio of 0.70371±12 and ε
Nd
(t) value of 0.13±0.22,
which are identical, within uncertainties, to the values obtained by solution analyses. However, they are
significantly different from comparable data obtained from whole rock samples, indicating that initial Sr–Nd
isotopic ratios calculated from whole rock measurements on kimberlites are likely to record mixed isotopic
signatures, due to crustal contamination and/or subsequent alteration. This conclusion is also supported by
the Hf isotopic data for perovskite. Meaningful isotopic ratios for kimberlite can therefore only be obtained
from single minerals such as pervoskite. The Mengyin samples investigated in this study have isotopic
compositions similar to the Group I kimberlite, as defined in Southern Africa, and are interpreted to reflect
derivation from a primitive mantle source. Combined with the fact that the Mengyin kimberlites were
emplaced coevally with regional lithospheric uplift in the Ordovician at ∼ 470 Ma, it is proposed that a mantle
plume triggered kimberlite magmatism in this part of the North China Craton.
© 2009 Elsevier B.V. All rights reserved.
1. Introduction
Kimberlite is a unique ultramafic rock derived from either the
lithosphere or sub-lithospheric mantle (Mitchell, 1986, 1995; Woolley
et al., 1996) and can provide invaluable information about the
composition and structure of that lithosphere (Mitchell, 1986).
Based on mineralogical and petrological characteristics and Sr–Nd
isotopic data, kimberlites can be divided into two main types; Group I
(non-micaceous, with low initial Sr and high initial Nd isotope
signatures) and Group II (phlogopite-bearing, with high initial Sr and
low initial Nd isotope signatures) (Smith, 1983); a transitional type
has also been reported (Becker and Le Roex, 2006). However, two
important problems hamper the determination of kimberlite genesis.
Firstly, kimberlite, by definition, contains abundant, variably-sized
crustal and mantle xenoliths (Mitchell, 1986), which makes it difficult
to determine the initial isotopic composition of the kimberlitic
magma. Secondly, kimberlite is highly susceptible to alteration during
both emplacement and by later weathering, due to its high content of
volatiles and mantle minerals. Therefore, the combined effects of
contamination and post-emplacement alteration limit the reliability
of whole-rock isotopic analyses (Mitchell, 1986), and make these
largely ineffective when trying to determine mantle sources (Heaman,
1989).
Fortunately, perovskite (CaTiO
3
) can be used to circumvent many
of the problems outlined above since it occurs mainly in the kimberlite
groundmass and crystallized early in the magmatic history, along with
ilmenite, rutile and magnesian chromite, and prior to crystallization
of monticellite, phlogopite, serpentine and calcite (Mitchell, 1972,
1986; Thy et al., 1987). Therefore, perovskite has the potential to
record the primary geochemical and isotopic signature of the magma,
prior to any contamination and/or weathering. Furthermore, although
perovskite is unstable in residual magmatic fluids (H
2
O and CO
2
)
and is commonly resorbed and/or mantled by thin rims of rutile, it is
Chemical Geology 264 (2009) 24–42
⁎ Corresponding author. Tel.: +86 10 82998217; fax: +86 10 62010846.
E-mail address: wufuyuan@mail.igcas.ac.cn (F.-Y. Wu).
0009-2541/$ – see front matter © 2009 Elsevier B.V. All rights reserved.
doi:10.1016/j.chemgeo.2009.02.011
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