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Accepted Manuscript
Geochronology and geochemistry of late Paleozoic magmatic rocks in the Yin-
waxia area, Beishan: Implications for rift magmatism in the southern Central
Asian Orogenic Belt
Rongguo Zheng, Tairan Wu, Wen Zhang, Qingpeng Meng, Zhaoyu Zhang
PII: S1367-9120(14)00189-8
DOI: http://dx.doi.org/10.1016/j.jseaes.2014.04.022
Reference: JAES 1938
To appear in: Journal of Asian Earth Sciences
Received Date: 2 December 2013
Revised Date: 21 April 2014
Accepted Date: 23 April 2014
Please cite this article as: Zheng, R., Wu, T., Zhang, W., Meng, Q., Zhang, Z., Geochronology and geochemistry
of late Paleozoic magmatic rocks in the Yinwaxia area, Beishan: Implications for rift magmatism in the southern
Central Asian Orogenic Belt, Journal of Asian Earth Sciences (2014), doi: http://dx.doi.org/10.1016/j.jseaes.
2014.04.022
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1
Geochronology and geochemistry of late Paleozoic magmatic rocks in the Yinwaxia area,
Beishan: Implications for rift magmatism in the southern Central Asian Orogenic Belt
Rongguo Zheng a, Tairan Wu a, Wen Zhang b, Qingpeng Meng a, Zhaoyu Zhang a
a MOE Key Laboratory of Orogenic Belts and Crustal Evolution, School of Earth and Space
Sciences, Peking University, Beijing 100871, China
b Institute of Geology, Chinese Academy of Geological Sciences,
Beijing 100037, China
Corresponding author:
Tairan Wu
MOE Key Laboratory of Orogenic Belts and Crustal Evolution
School of Earth and Space Sciences
Peking University
Beijing 100871
China
Tel. +86 10 62765534
Email: [email protected]
2
Abstract: Mafic-ultramafic rocks are distributed widely in the Beishan rift, which is located
in the southern Beishan, central southern Central Asian Orogenic Belt. The Yinwaxia study
area is located in eastern Beishan rift, where mafic-ultramafic rocks occur along major faults.
The zircon SHRIMP U-Pb age obtained of a gabbro is 281±11 Ma, and the age of the basalt is
constrained by the youngest xenocrystal with an age of 265 Ma, which substantiate that these
mafic rocks formed in Permian. Basalts and gabbros exhibit similar geochemical
characteristics including: high SiO2, total Fe2O3 and TiO2 contents; low MgO contents and
Mg# values; and tholeiitic characteristics. Yinwaxia mafic rocks have relatively high total
rare earth element contents, enrichment in light rare earth elements, enrichments in the high
field strength elements, and obvious negative Nb-Ta-Ti anomalies. Basalts exhibit low
(87Sr/86Sr)i and high εNd(t) values, while gabbros exhibit relatively high (87Sr/86Sr)i and low
εNd(t) values. Isotopic compositions of these mafic rocks display a mixed trend between
depleted and enriched mantles. Meanwhile, differing εNd(t) values show that basalts were
intensively contaminated by juvenile crustal materials, but gabbros were contaminated by
older continental crust. We conclude that Yinwaxia mafic rocks were derived from
lithospheric mantle metasomatized by fluids and/or melts from subducted slab; parental
magmas underwent AFC processes, then emplaced along faults in a continental rift. We
collected geochemical and geochronological data in the study area, and collated
geochronological data from previous workers in the Beishan orogenic belt to develop a
geochronological frequency diagram. From these data and analyses we deduced a model of
tectonic evolution for the Beishan orogenic belt. Considering the geochemistry,
sedimentological evidence for rifting, and the geochronological frequency diagram, we
3
propose that the Beishan rift had entered a post-collision stage since Early Devonian, and
then changed into a continental rift stage around late Carboniferous-early Permian.
Key words: Beishan, mafic rocks, SHRIMP, Sr-Nd isotope, continental rift, Central Asian
Orogenic Belt
4
1. Introduction
The Central Asian Orogenic Belt (CAOB) is the largest area of Phanerozoic continental
accretion and crustal growth in the world (Sengör et al., 1993; Jahn et al., 2000; Kovalenko et
al., 2004; Windley et al., 2007). The CAOB extends from Kazakhstan in the west to eastern
Siberia in the east (Fig. 1), and separates the Siberian craton in the north from the Tarim and
north China (or Sino-Korean) cratons in the south (Zonenshain et al., 1990; Mossakovsky et
al., 1994; Jahn et al., 2000; Badarch et al., 2002). There is a general consensus that the CAOB
grew by successive lateral accretions of arcs, accretionary complexes and a few continental
blocks southward from Siberia and southern Mongolia during the evolution of the
Paleo-Asian Ocean (Windley et al., 2007; Kröner et al., 2008; Xiao et al., 2009, 2013;
Safonova and Santosh, 2014.). Although the timing of the final closure of the Paleo-Asian
ocean is still a matter of debate, accumulating evidence suggests a diachronous closing
process which resulted in many and diverse tectonic regimes in the late Paleozoic within this
immense accretionary orogenic belt. After the amalgamation, the CAOB was affected by
continental magmatic activities and modified by intracontinental orogenic reactivations
(Windley et al., 1990; Wartes et al., 2002; Khain et al., 2003; Kröner et al., 2007, 2010).
The late Paleozoic was an important period of tectonic transition and crustal growth of
the CAOB; the crustal growth is represented by large volumes of juvenile granitoids with
positive εNd and low initial (87Sr/86Sr)i values (Han et al., 1997; Jahn et al., 2000; Chen and
Jahn, 2004). However, this period was also characterized by emplacements of many coeval
mafic-ultramafic complexes having controversial origins (Hong et al., 2003; Han et al.,
2004; Zhou et al., 2004; Zhao et al., 2006; Windley et al., 2007; Mao et al., 2008; Pan et al.,
5
2008; Pirajno et al., 2008). One group of these late Paleozoic mafic-ultramafic complexes
occurs in the the Beishan orogenic belt, located in the middle region of the southernmost
CAOB (Fig.1a). The Beishan orogenic belt has many Cu-Ni-bearing mafic-ultramafic
complexes, especially in the southern portion of the belt (Mao et al., 2008; Pirajno et al.,
2008; Zhang et al., 2008). Most of these mafic-ultramafic rocks crop out along regional
large-scale faults or sutures, such as mafic rocks in the Pobei and Liuyuan areas. Chemical
and isotopic compositions of continental mafic rocks provide the best proxy record for the
chemical and physical evolution of the deep continental lithosphere and underlying mantle
(Farmer, 2003). Mafic–ultramafic rocks can also provide valuable information for
unraveling the geological history of orogenic belts. Although many researches have
focused on mafic-ultramafic rocks in the southern Beishan as noted above, there are still
controversies regarding their tectonic implications of these rocks.
Mafic-ultramafic complexes in the southern Beishan are usually described as the
products of within-plate magmatic activity (Jiang et al., 2006; Mao et al., 2008; Pirajno et al.,
2008; Zhang et al., 2008), formed as a result of post-orogenic extension or plume related
magmatic process (Qin et al., 2011; Su et al., 2011a, 2011b, 2012b). Conversely, it has also
been suggested that these mafic-ultramafic complexes are Alaskan-type intrusions, generated
in the early Permian subduction-related environment (Xiao et al., 2004a; Mao et al., 2006; Ao
et al., 2010). Alternatively, some workers have argued that mafic complexes in the southern
Beishan were associated with a mantle plume that resulted in Permian flood basalts in the
western part of the Tarim block (Qin et al., 2011; Su et al., 2011a, 2011b, 2012b). This work
certainly will provide crucial insights into the mechanism of orogenesis and tectonic history
6
of the southern Beishan.
In light of these conflicting theories, we present new geochronological, and major and
trace element data, as well as whole rock Sr-Nd isotopic compositions, for the mafic rocks in
the Yinwaxia area, in the eastern sector of southern Beishan. To provide further insight into
the mechanism of orogenesis and tectonic history of the southern Beishan orogenic belt, we
also complied the geochronological data previously reported in the literature to describe
magmatic sequences of the Beishan rift. From this large data set, we endeavored to define
tectonic settings of mafic rocks in the Yinwaxia area, discuss the formation mechanism, and
develop a reasonable tectonic evolution model.
2. Geological background
The Beishan orogenic belt, situated in the southernmost CAOB, is a conjunction
region of the CAOB and North China and Tarim cratons (Fig. 1a). It is separated from the
Tianshan orogenic belt to the west by the Ruoqiang-Xingxingxia fault, and from the
Mongolia-Xing’anling orogen to the east by the Altyn Tagh-Alxa fault. The Dunhuang
block, part of the Tarim craton (Zhang et al., 2013), is located to the south of the Beishan
orogenic belt (Zhou and Graham, 1996; Wu et al., 1998; Zhang et al., 2011a). Tectonically,
the Beishan orogenic belt is often regarded as the eastern extension of the Chinese Tian
Shan (Li, 1980; Liu and Wang, 1995; Xiao et al., 2010), and it comprises an assemblage of
blocks, magmatic arcs and ophiolitic mélanges formed by subduction-accretion processes
of the Paleo Asian Ocean. The Beishan area exhibits well-preserved Neoproterozoic to late
Paleozoic sequences with intervening ophiolitic zones, and most workers usually divided
the orogenic belt into three sub-belts (southern, middle, and northern) by Xiaohuangshan
7
and Niujuanzi-Yueyashan ophiolitic belts, which are southern, middle and northern Beishan
(Zuo and He, 1990). The southern Beishan belt is composed of Precambrian strata,
Paleozoic volcanic-sedimentary formations, and magmatic intrusions. The upper Paleozoic
strata in the southern Beishan are all terrestrial (GSBGMR, 1966), in contrast to the other
two belts. The southern Beishan belt is separated from the middle Beishan belt by the
Niujuanzi-Yueyashan ophiolite zone. The middle Beishan belt is characterized by early
Paleozoic volcanic-sedimentary formations and magmatic intrusions, usually regarded as
having resulted from early Paleozoic subduction events (Zuo and He, 1990; Dai et al., 2003;
Ao et al., 2010). The middle Beishan belt is separated from the northern Beishan belt by the
Xiaohuangshan ophiolitic zone. The northern Beishan belt is relatively complex, and is
further subdivided into two zones by Hongshishan ophiolitic belt. The northern zone is
mainly composed of lower Paleozoic and magmatic intrusions, however, the southern zone
of the northern belt is characterized by Carboniferous strata and late Paleozoic granitoids.
The Beishan rift is located in the southern Beishan belt, bordering on the Dunhuang
block to the south. The Huaniushan arc is located to the north of the Beishan rift, and
bounded by the Gubaoquan-Hongliuyuan shear zone (Fig. 1b; BGMRXUAR, 1993; Xu et
al., 2009). The Beishan rift is mainly composed of Carboniferous-Permian strata and
magmatic intrusions. Fault-related uplifts and sags are well developed in the rift, and the
contact between each pair of strata from Precambrian to Permian is separated by faults (Xu
et al., 2009; Su et al., 2012b). The Beishan rift is characterized by exposures of numerous
mafic-ultramafic complexes, most of which host Ni-Cu sulfide ore deposits.
Mafic-ultramafic complexes such as Poshi, Hongshishan, Bijiashan and Liuyuan
8
complexes, are mainly distributed in the western and central part of the Beishan rift, and
intrude the Proterozoic and Carboniferous strata, (Jiang et al., 2006; Qin et al., 2011; Su et
al., 2011 a, 2011b; Zhang et al., 2011a).
The Yinwaxia area, in which we collected new data, is located in the eastern part of the
Beishan rift (Fig. 1b). Strata exposed in the Yinwaxia area are mainly Paleozoic, including
upper Silurian, Devonian, Carboniferous and Permian, and the Permian strata are
distributed most widely (Fig. 2). The upper Silurian strata in the Yinwaxia area are
composed of massive volcanic rocks: basic volcanic rocks dominate the lowest sequence,
though the topmost sequence comprises bimodal volcanic rocks, including amygdaloidal
basalts and rhyolites (GSBGMR, 1966; Liu et al., 1999). These Silurian basic and acidic
volcanic rocks display interbeds, similar to rift-related rock associations. The Permian
strata distributed across the southern Beishan include the Shuangbaotang group, the Jinta
group (the lower Permian) and the Fangshankou group (the upper Permian). The
Shuangbaotang group mainly consists of clastic rocks, including sandstones, pebbly
sandstones, limestones, bioclastic limestones. The Jinta group mainly consists of basalts,
andesitic basalts, and andesites with siliceous slate and phyllite interlayers. Permian strata
in the Yinwaxia area are domanited by the Fangshankou group, which consists
predominantly of felsic volcanic and pyroclastic rocks with eruption-explosion facies,
including rhyolites, dacites, rhyolite breccia lavas, rhyodacites and homogeneous volcanic
tuff. Mafic rocks occur rarely in the Fangshankou group. Additionally, there exist terrestrial
plant fossils and other terrestrial materials in the Fangshankou group. Geochemical studies
of volcanic rocks in the Fangshankou group demonstrate that they are bimodal volcanic
9
rocks, and formed in a continental rift setting (Liu et al., 1999), and features of Permian
sedimentary strata also support the existence of a Permian continental rift. Late Paleozoic
granitoids are distributed widely in the Yinwaxia area, and typical examples are biotite
granites in the southern Yinwaxia pluton and monzonitic granites in the Xijianquanzi
pluton. Previous studies prove that these late Paleozoic granitoids exhibit positive εNd(t)
and εHf(t) values, implying additions of depleted mantle (or a juvenile component) in their
evolution. These granitoids were mixed products of crustal and mantle derived magmas,
and formed in an extensional tectonic setting (Zhang et al., 2010, 2011b, 2012).
3. Field occurrence and petrography
Mafic-ultramafic rocks exposed in the Yinwaxia area include basalts, gabbros, and
ultramafic rocks (Fig. 2; GSBGMR, 1966). Basalts comprise the upper part of the Permian
strata, and the remaining mafic-ultramafic rocks were emplaced into Paleo-Proterozoic
strata.
The Yinwaxia area ultramafic rocks intruded into the Paleo-Proterozoic strata as an
apophysis, including serpentinites and pyroxenites. The mineral assemblages of the
serpentinites are mainly serpentine (75–80%), calcite (10–15%), spinel (5–10%) and
magnetite (1–5%); they display microscopic crystalloblastic texture and scales
crystalloblastic texture microscopically. Mafic rocks in the Yinwaxia area include basalts
and gabbros. Yinwaxia area gabbros also intruded into the Paleo-Proterozoic strata. They
are dark–light green, and exhibit medium-grained gabbroic texture. The main mineral
assemblages of the gabbros are clinopyroxenes and plagioclase, and they also contain
minor amphibole, chlorite, magnetite and ilmenite. Many clinopyroxenes underwent
10
intensive amphibolitizations, and plagioclases were usually altered to chlorites. Basalts are
a main component of Permian strata in the Yinwaxia area, and display massive structures.
These basalts also show porphyritic textures with phenocrysts of plagioclase and pyroxene
(0.1–0.2 mm in size) set in a groundmass of plagioclase microlites, granules of pyroxene,
and glass.
4. Analytical methods
4.1 SHRIMP zircon analyses
Separations of zircon crystals were accomplished by conventional heavy liquid and
magnetic techniques. The individual crystals were mounted in epoxy together with the
TEMORA standard zircons, and then polished to approximately half thickness. Then the
zircons were photographed in reflected and transmitted light as well as SEM
cathodoluminescence (CL) images which were all taken at Peking University to study the
internal structures in order to identify the suitable target for spot analysis.
U-Pb isotopic ratios of zircon crystals were measured using the SHRIMP II in the
Beijing SHRIMP Centre, Institute of Geology, Chinese Academy of Geological Sciences,
Beijing, China. Instrumental conditions and measurement procedures are the same as those
described by Compston et al. (1992). Spots of approximately 20μm-diameter were
analyzed. Data for each spot were collected in sets of five scans. The 206Pb/238U ratios of
the samples were corrected using reference zircon of TEMORA (206Pb/238U = 0.06683; 417
Ma). The data were corrected for common Pb on the basis of the measured 204Pb. The
decay constants and present-day 238U/235U value given by Steiger and Jager (1977) were
used. Uncertainties given for individual analyses (ratios and ages) are at 1σ level whereas
11
the uncertainties in calculated weighted mean ages are reported as the 95% confidence
level. Concordia plots and weighted mean age calculations were carried out using
ISOPLOT/Ex 3.23 (Ludwig, 2003). The SHRIMP U-Pb data are reported in Table 1.
4.2 Whole-rock geochemical analyses
The major, trace and rare earth elements (REEs) were analyzed at the Laboratory of
Orogenic Belts and Crustal Evolution, Peking University. Rock samples for whole rock
analyses were crushed and then pulverized in an agate mill. Whole rock major elements
were analyzed by X-ray fluorescence (XRF) on fused glass beads, following the analytical
procedures of Li et al. (2006) and the analytical precision is within 0.1%. Trace elements
were analyzed using Inductively Coupled Plasma Mass Spectrometer (ICP-MS), following
the technique of Li (1997). About 50 mg of powder from each sample was dissolved in
high-pressure Teflon bombs using a HF+HNO3 mixture. The analytical precision for the
common trace elements was superior to 5%, while that of Nb and Ta was superior to 10%.
Analytical results are listed in Table 2.
Analyses for Sr and Nd isotopes and Sm, Nd, Rb, and Sr concentrations were
performed at the Institute of Geology, Chinese Academy of Geological Sciences (IGCAGS),
using the Solid Isotope Mass Spectrometer MAT-262 from German Finnigan Corporation.
Analytical procedures are described in detail by Yang et al. (2010). During analysis, the
NBS-987 standard yielded an average value of 87Sr/86Sr=0.710274±11 (2σ) and the JMC
standard yielded an average value of 143Nd/144Nd=0.512096±12 (2σ). Mass fractionation of
Sr and Nd isotopes were corrected by 86Sr/88Sr =0.1194 and 146Nd/144Nd = 0.7219. During
analyses, the backgrounds of Rb-Sr and Sm-Nd were 100-300 pg and 50-100 pg,
12
respectively. Analytical results are listed in Table 3.
4.3 Mineral composition analyses
Clinopyroxenes were analyzed using a JEOL JXA-8100 wavelength dispersive
electron microprobe at Peking University. The operating conditions were 15 kV
acceleration voltages with 10 nA beam current and a beam diameter of 1 μm. Analytical
results are listed in Table 4.
5. Analytical results
5.1 Geochronology
Zircons from the basalt sample (Y-14) have wide ranges of U (79-500 ppm), Th
(24-198 ppm) contents and high Th/U ratios (0.23-1.04), which are characteristics of
magmatic zircons (Belousova et al., 2002;Wu and Zheng, 2004). Two older 206Pb/238U age
(1693.7Ma and 2181.9Ma) were obtained, and the other eight analyses yield 206Pb/238U
apparent ages of 267.4~314.3Ma. In the CL images (Fig. 3), zircon grains from the basaltic
sample display high variable characteristics. Some of them are similar to those in gabbro
(i.e. 8.1), and some resemble the magmatic zircon in felsic rocks (i.e. 5.1, 6.1 and 7.1).
Different zircon morphologies indicate that most of them (if not none of them) were not
formed during basaltic magmatism, but are xenocrystals captured by basaltic magma
during its eruption. Thus, the age of the basalt should be constrained by the youngest
xenocrystal (~265 Ma, i.e. late Permian), and this is in agreement with the field occurrence.
Zircons from the gabbro sample (Y-5) are mostly euhedral and short columnar. Their
CL images (Fig. 3) show that they display light color, and parallel banded patterns,
composed of light and dark bands, which are typical characteristics of zircons from gabbros
13
(Jian et al., 2003). They have wide ranges of U (63-511 ppm), Th (43-213ppm) contents
and high Th/U ratios (0.14-0.86), which are characteristics of magmatic zircons (Belousova
et al., 2002;Wu and Zheng, 2004). Two older 206Pb/238U age (1729.7Ma and 1902.6Ma)
were obtained, and the other seven analyses yield 206Pb/238U apparent ages of
264.9-297.3Ma, with a weighted mean age of 281±11 Ma (MSWD=3.4, n=7) (Fig.3).
5.2 Whole-rock geochemistry
5.2.1 Basalts
The Yinwaxia basalt samples have high SiO2 contents ranging from 46.38 to 54.15
wt. %, and plot in the andesitic basalts and andesite fields on the Nb/Y-Zr/TiO2 diagram
(Fig. 4a). The MgO contents and magnesium number (Mg#) values are low (3.14—4.29
wt. % and 36.13—47.59, respectively), suggesting evolving magma. These samples also
have relatively low total alkali contents (Na2O+K2O=2.66—6.71 wt. %), and higher Na2O
contents (mostly K2O/Na2O=0.30—0.95). They also have relatively low Al2O3 contents
(13.03—14.74 wt. %), similar to that of tholeiitic basalts. In addition, they have relatively
high total Fe2O3 (10.40—14.11 wt. %, mostly>12 wt. %), TiO2 (2.01—2.88 wt. %) and
P2O5 (0.68—1.10 wt. %) abundances, which accord with characteristics of high Fe-Ti basic
rocks around the world (FeOt >12 wt. % and TiO2> 2 wt. %; Clague and Bunch, 1976;
Clague et al., 1981; Perfit and Fornari, 1983) around the world. In the AFM ternary
diagram (Fig. 4b), these basalts exhibit tholeiitic characteristics.
These basalts exhibit consistent rare earth elements (REEs) characteristics. They have
high total REEs contents (177.89–195.03ppm), and display enrichments in the light REEs
(LREEs) relative to middle REEs (MREEs) [(La/Sm)N=1.92–2.38] and heavy REEs
14
(HREEs) [(La/Yb)N=3.63–3.97]. There are essentially no Eu anomalies (δEu=0.93–0.99),
indicating rare affections of plagioclase fractional crystallizations. In the
Chondrite-normalized REE diagram (Fig. 5a), these basalt samples have similar LREEs
contents to that of the ocean island basalt (OIB), but higher MREEs and HREEs contents.
Overall, the Yinwaxia basalts have relatively flat REE patterns compare with OIB.
In the Primitive mantle-normalized multi-element diagram (Fig. 6a), basalt samples
display obvious depletions in the Nb-Ta-Sr-Ti-La-Ce suite. In addition, they have high field
strength element (HFSE) contents which are similar to those of OIB, but higher than those
of mafic rocks from the Tarim Large Igneous Province (TLIP), the Columbia River basalts
and average continental arc rocks (Farmer, 2003; Kelemen et al., 2004; Tian et al., 2010).
The Yinwaxia basalts also have higher HREE contents than those of the TLIP, Columbia
River, and average continental arc rocks. Relative to HFSEs, there are no obvious
enrichments in the large ion lithophile elements (LILEs, e.g., Cs, Rb, Ba, Pb, and Sr).
5.2.2 Gabbros
Compared with the basalts, Yinwaxia gabbro samples have higher SiO2 contents
(50.37–55.62 wt. %), MgO contents (5.13–6.32wt. %) and Mg# values (50.41–61.49). They
also have low total alkali (Na2O+K2O=1.94–5.73 wt. %), CaO (5.60–9.36 wt. %) and Al2O3
contents (13.63–16.06 wt. %). However, the gabbros have relatively low TFe2O3
(8.72–11.08 wt. %), TiO2 (1.32–2.16 wt. %) and P2O5 (0.21–0.36 wt. %) contents. In the
Nb/Y-Zr/TiO2 diagram (Fig. 4a), Yinwaxia gabbro samples plot in the andesite field, and
display tholeiitic characteristics (Fig. 4b) in the AFM diagram.
The Yinwaxia gabbro samples have lower total REE contents (94.69–122.76 ppm)
15
than the basalts. Similarly, they also display enrichments in the LREEs relative to MREEs
[(La/Sm)N=2.03–2.72] and HREEs [(La/Yb)N=2.99–3.75]. These gabbro samples display
slight negative Eu anomalies, δEu=0.77–0.91, indicating a slight effect of plagioclase
fractional crystallization. Compared with OIB, these gabbros have higher HREE contents,
and display flatter REE patterns in the Chondrite-normalized REE diagram (Fig. 5b).
In the Primitive mantle-normalized multi-element diagram (Fig. 6b), Yinwaxia
gabbros display depletions in Nb, Ta, Ti, La and Ce and enrichments in Cs, Rb, U, Pb and
Th. They have lower HFSE content than that of basalts, which is a similar pattern to that of
mafic rocks from the Tarim Large Igneous province (TLIP) and Columbia River basalts.
Relative to HFSEs, there are also no obvious enrichments in LILEs.
5.3 Whole-rock Sr-Nd isotopic composition
Whole-rock Rb-Sr and Sm-Nd isotopic compositions for mafic rocks in the Yinwaxia
area are listed in Table 3, and plotted in Fig. 7. Initial 87Sr/86Sr and 143Nd/144Nd ratios were
calculated using 280 Ma for gabbros, and 260 Ma for basalts. The gabbros have initial
87Sr/86Sr ratios ranging from 0.706739 to 0.707990, and εNd(t) ranging from −3.42 to −0.68.
The basalts have lower initial Sr isotopic [(87Sr/86Sr)i=0.703774–0.705322], but higher εNd(t)
values (4.69–7.28). In Fig.7, samples plot in the ocean island basalts (OIB) field, indicating
a mixing trend between depleted mantle and EM2 (enriched mantle type II).
5.4 Clinopyroxenes mineral chemistry
Major element analyses of clinopyroxenes from the YInwaxia gabbros are reported in
Table 4. Plots of Alz (percentage of tetrahedral sites occupied by Al) vs. TiO2 in augite from
gabbroic and ultramafic cumulates show that augite data arrays for arc-related cumulates
16
have a trend of substantially higher Al/Ti in clinopyroxene than that of rift-related tholeiitic
rocks (Loucks, 1990). All clinopyroxenes in gabbros from the Yinwaxia study area plot
along the rift-related trend (Fig. 8a). In the discrimination diagram (Fig. 8b), all the
analyzed clinopyroxenes fall in the compositional fields for the plume-influenced basalts
from Iceland and within oceanic plate basalts, distinct from subduction-related settings.
6. Discussion
All the rocks in this study underwent strong alteration, consistent with high loss on
ignition (LOI) values (1.60-4.92 wt. %). Therefore, the major and trace element
geochemistry described here is based on immobile elements during low-temperature
alteration and metamorphism up to the greenschist facies (Beccaluva et al., 1979; Pearce
and Norry, 1979; Shervais, 1982). Generally, those immobile elements include Al, Ca, Mg,
high field strength elements (e.g. Th, Zr, Hf, Nb, Ta, Ti,Y) and REE including Sm-Nd
isotopic system.
6.1 Fractional crystallization and crustal contamination
No systematic variation trend within the different rock types can be observed in
covariations of some selected major elements and their ratios against MgO. In contrast, the
good correlation of most of the elements with MgO suggests that common processes
controlled the compositions of the different rock types. In particular, positive correlations
between CaO, CaO/Al2O3 and MgO support the fractionation of clinopyroxene. TFe2O3
and TiO2 are generally negatively correlated with MgO in all the rocks, suggesting that
Fe-Ti oxides played an important role in their evolutions. The presence of phenocrystic
plagioclase in most samples also supports significant early crystallization of this mineral,
17
which would account for the coherent negative Sr anomalies observed (Fig. 6), although
this seems nominally inconsistent with the absence of obvious negative Eu anomaly in the
REE patterns (Fig. 5). Frey et al. (1993) and Xu et al. (2001) have interpreted this
phenomenon to result from high Eu3+/Eu2+ ratios in magmas because Eu2+ is compatible
with plagioclase, whereas Eu3+ is not. It follows that relatively little Eu may be lost during
fractional crystallization of plagioclase in a system with a high oxygen fugacity.
Element covariations suggest that clinopyroxene and plagioclase should be the
principal fractionating phases in these mafic rocks. Some fractionations of Fe-Ti oxides
also occurred.
Crustal contaminations could potentially increase SiO2, K2O, Zr, Hf, Th, Cs, Rb and
Ba abundances and La/Nb and Zr/Nb ratios, but decrease Ti/Yb and Ce/Pb ratios in mafic
magmas (Campbell and Griffiths, 1993; Barker et al., 1997; MacDonald et al., 2001). It is
possible to use ratios of highly incompatible elements in mafic rocks to determine these
ratios in their mantle source regions, given that elements having similar Kds produce
incompatible element ratios that are independent of the degree of partial melting of the
mantle source or the amount of subsequent magmatic differentiation (Hanson, 1989;
Hofmann, 1997). In addition, Nb is one of the high field strength elements (HFSEs), and
generally has low concentrations in the crust. Though La is typically enriched in the crust,
Th is commonly enriched in sediments. Therefore, the high (Th/Nb)N ratio (>1) and low
Nb/La ratio (<1) are two reliable indicators for crustal contamination (Saunders et al., 1992;
Xia et al., 2007). (Th/Nb)N ratios of Yinwaxia mafic rocks range from 1.51 to 3.90, larger
than 1, and their Nb/La ratios range from 0.0029 to 0.084, far away less than 1. In addition,
18
Ti/Y ratios vary from 168 to 307, slightly higher than those of bulk continental crust and
Archean bulk crust (160 and 187, respectively; Taylor and McLennan, 1985). Yinwaxia
mafic rocks also exhibit low Nb/U (7.43–15.42) ratios, similar to that of continental crust
(8.45, Sun and McDonough, 1989). All these ratios indicate that Yinwaxia magmas might
have experienced some degree of crustal material contamination. Trends of crustal
contamination also appear on the basis of the correlation between εNd(t), Nb/La and Mg
number. It is concluded that Yinwaxia mafic rocks experienced some degree of crustal
assimilations.
6.2 Characteristics of magma sources
Sr and Nd isotopic ratios are usually used for discrimination of mantle sources.
Mixing between Depleted Mantle (DM) and Enriched Mantle I (EM1) or Enriched Mantle
II (EM2) will produce a negative trend and OIB-like components in a plot of (87Sr/86Sr)i
versus εNd(t) (Zinder and Hart, 1986). Sr-Nd isotopic compositions of all the Yinwaxia
rocks have typical OIB-like signatures, and clearly show a mixing trend between DM and
EM2 components in the genesis of the magmas (Fig. 7). In addition, several previous
studies have attributed the mantle heterogeneity, especially the formation of an EM2
reservoir, to subduction-related modification (e.g., Zindler and Hart, 1986; Rollinson, 1993;
Turner et al., 1997; Zhou et al., 2004; Su et al., 2012b). Because the EM2 mantle
component is considered to be a mantle contaminated by subduction-related modifications
(Weaver, 1991; Greeough at al., 2005), it appears that mantle sources of mafic rocks in the
Yinwaxia area were intensively depleted and variably enriched by subduction slab-derived
components. In fact, previous studies have proved the existence of Paleozoic subduction
19
events. Previous studies (Mao et al., 2012; Su et al., 2012a; Zheng et al., 2012) discovered
numerous Paleozoic subduction-related indicators, such as late Ordovician Nb-enriched
basalts (451 Ma) in the Liuyuan area (Mao et al., 2012). Therefore, there might be an early
Paleozoic arc (Fig. 1b; Xiao et al., 2010) and the early Paleozoic subduction process could
have variably modified mantle sources beneath the Beishan rift.
Though both basalts and gabbros were significantly contaminated by crustal
materials, they exhibit very different εNd(t) values (Fig 7), which could be ascribed to the
different crustal materials incorporated into the primitive magmas of mafic rocks (Zhang
and Zou, 2012). Contamination by old crust could quickly decrease εNd values of the mafic
rocks, while contamination by juvenile crustal materials would have a weak influence on
the εNd values (Zhang and Zou, 2012). Therefore, we suggest that Yinwaxia basalts were
intensively contaminated by juvenile crustal materials, while Yinwaxia gabbros were
contaminated by the old continental crust further, supported by the fact that gabbros intrude
into the Paleo-Proterozoic, which comprises of migmatite, metavolcanic rock, and gneiss.
Previous studies (Zhang et al., 2010, 2011b, 2012) show that post-collisional and A-type
granitoids with ages of 280–250Ma are widely exposed in this region (Fig. 1b). Sr-Nd
isotopic compositions of Yinwaxia basalts display a mixing trend of magma derived from
depleted mantle with magma forming coeval A-type granites (Fig. 7). Therefore, we
speculate that these basalts were contaminated by parental magmas of coeval A-type
granites.
We conclude that Yinwaxia mafic rocks were derived from lithospheric mantle
metasomatized by fluids and/or melts derived from subducted slab materials. Parental
20
magmas underwent clinopyroxene, plagioclase and Fe-Ti oxide fractionations. In addition,
basalts were contaminated by parental magmas of coeval A-type granites, while gabbros
were contaminated by the older continental crust, and these different contaminants led to
different Sr-Nd isotopic characteristics.
6.3 Tectonic setting
In the Primitive mantle-normalized multi-element diagram (Fig. 6), Yinwaxia mafic
rocks display obvious negative Nb-Ta-Ti anomalies, similar to those of magmatic rocks
formed in a subduction zone. Compared to compositions of average continental arc rocks, it
is clear that LILEs of the Yinwaxia mafic rocks are lower, while their HFSEs are obviously
higher (Fig. 6), indicating that their mantle sources are totally different from those of
arc-derived magmatic rocks. However, the Yinwaxia mafic rocks exhibit trace element
characteristics similar to those of continental flood basalts having crustal contamination.
Because of crustal contamination, continental flood basalts generally exhibit negative
Nb-Ta-Ti anomalies, and positive Pb-Rb-Ba-Th-U anomalies, similar to basalts derived
from subduction settings (Kelemen et al., 2004). As discussed above, Yinwaxia mafic rocks
experienced crustal assimilation, which caused negative Nb-Ta anomalies. In addition,
because oxidation-reduction and aqueous solutions of melting sources in the
subduction-related setting are different from those of other tectonic settings, we can use
some trace elements ratios and covariant relationship diagrams between related elements to
distinguish within plate basalts and subduction-related basalts (Pearce and Norry, 1973;
Shervais, 1982; Rollinson, 1993). In the tectonic setting discrimination diagrams (Fig. 9),
21
Yinwaxia mafic rocks exhibit different characteristics than basalts in the arc setting, and are
instead similar to that of basalts generated within-plate.
Granitoids are distributed widely in the southern Beishan, especially in the Yinwaxia
area, most notably including the Yinwaxia and Xijianquanzi granites. The Yinwaxia pluton
has a LA-ICP-MS U-Pb age of 281.7±2.9Ma, similar to that of the Yinwaxia mafic rocks.
The pluton mainly consists of biotite granites which belong to the middle-K, calc-alkaline
series with metaluminous-peraluminous characteristics and high SiO2 and (Na2O + K2O)
contents; samples invariably exhibit relatively small Chondrite-normalized light rare earth
element (LREE) enrichments with flat heavy rare earth elements (HREE), weak negative
Eu anomalies, with depletion of Nb, Ba, P, and Ti and enrichment of Rb, Pb, and K in their
primitive mantle-normalized trace elements patterns (Zhang et al., 2010, 2011b). Yinwaxia
pluton rocks exhibit positive εHf(t) (4.4–7.8) and εNd(t) (0–1.3), and their isotopic data
emphasizes the importance of the depleted mantle (or juvenile component) in its genesis.
The Yinwaxia granites are the mixed products of crustal and mantle derived magmas and
formed under an extensional tectonic setting in the Early Permian. The LA-ICP-MS zircon
U-Pb age of the Xijianquanzi granite is 266.1±2.2 Ma, and εHf(t) values are positive,
1.3–4.7. The Xijianquanzi granitoid mainly consists of monzonitic, alkali-rich, high
potassium granites with some “A-type like” granite characteristics, e.g., high 10000×Ga/Al
values and weakly V-shaped Chondrite-normalized REE patterns. Chemical characteristics
of the Xijianquanzi granitoids indicate that they were mixed products of crustal and mantle
derived magmas, and were formed in a rift setting in an extensional period. Studies of these
granitiods in the Yinwaxia area suggest an extensional setting, and that these granitiods
22
with positive εHf(t) or εNd(t) values formed with strong crust-mantle interactions, similar to
other voluminous CAOB granites with positive εHf(t) or εNd(t) values (Han et al., 1997; Wu
et al., 2000, 2002; Chen and Jahn, 2004; Hong et al., 2004; Jahn et al., 2004).
The Permian strata distributed extensively in the southern Beishan developed
numerous faults with NE strike orientation. As noted in section 2, volcanic rocks in the
Fangshankou group are bimodal and formed in a continental rift setting (Liu et al., 1999).
Sedimentary formations of the Permian strata also support the existence of a Permian
continental rift in the Yinwaxia area. In addition, cherts occur along the regional faults (Fig.
1b), suggesting a relatively extensive Permian continental rift.
Considering the geochemical data of the Yinwaxia mafic rocks and the coeval
granitoids, and the characteristics of the Permian sedimentary formations, we conclude that
the Yinwaxia mafic rocks were formed in a continental rift, rather than a subduction setting.
6.4 Tectonic implications
The Beishan orogenic belt is considered to be a typical and key area for understanding
the formation and tectonic evolution of the central southern Altaids (the CAOB) between
the Tianshan and Inner Mongolia (Ao et al., 2010; Xiao et al., 2010; Guo et al., 2012). The
CAOB underwent a complex Paleozoic evolution including amalgamation of many
disparate tectonic terranes, and some fundamental tectonic problems have remained
unsolved, especially for the Beishan rift (Ao et al., 2010; Liu et al., 2011; Su et al., 2011a, b,
2012b; Zhang et al., 2011). To better understand the tectonic evolution of the Beishan rift,
we made a geochronological frequency diagram (Fig. 10) using published zircon ages, and
23
from this developed a tectonic evolution model of the Beishan rift (Fig. 11). The age data in
the frequency diagram (Fig. 10) were collected from mean and concordant ages of
magmatic (mostly) and metamorphic rocks in the Beishan rift and its adjacent region. Only
zircon ages measured by more precise analytical methods were compiled for Fig. 10 (Table
5), such as LA-ICP-MS, SHRIMP and SIMS zircon U-Pb ages. Rock types included in the
Fig. 10 are ultramafic rocks, mafic-ultramafic rocks, granitoids, dacites, rhyolites and
eclogites. In constructing the plots of Fig. 10, we quote the 206Pb/238U age for zircons,
instead of their mean or concordant ages, and filters were applied to screen out results with
unacceptably large analytical errors and unacceptable discordance. Based on these age data
quoted, we developed the relative probability plot of magmatic zircons from Paleozoic
rocks of the Beishan rift (Fig. 10), and from this plot, we obtained four peak ages,
including 534Ma, 450Ma, 415Ma and 282Ma.
The peak age of 534 Ma mainly reflects ages of ophiolitic mélanges. Dating results of
cumulate gabbros in the Hongliuhe ophiolite suggest it formed 516 ± 7 Ma (Zhang and Guo,
2008). In the eastern part of the same ophiolitic belt, the Yueyashan ophiolite was formed
in the early Cambrian, with a SHRIMP U-Pb age of 533±1.7 Ma (Ao et al., 2012). This
ophiolitic belt is the oldest one in the Beishan orogenic belt, and their geochemical
characteristics of these ophiolites suggest affinities with SSZ-type ophiolites (Ao et al.,
2012; Zheng et al., 2012). From these data we conclude that the major ocean, as a branch of
the Paleoasian Ocean represented in the Beishan orogenic belt, was formed in the
Precambrian (Fig. 11a), and that some micro-continental blocks might have been
distributed in this ocean, such as the Mazongshan and Hanshan blocks. Subduction of
24
intra-oceanic lithosphere generated the Hongliuhe-Yueyashan ophiolite in the period
533–516Ma.
Subduction between the Mazongshan and Dunhuang blocks continued and generated
various magmatic and metamorphic rocks (Fig.11b) with peak ages of 450Ma (Fig. 10).
Previous studies reported that U-Pb isotope analyses of zircons from the Liuyuan
Nb-enriched basalts and dacites yielded concordant ages of 450.5±3.9 Ma and 441.8±3.1
Ma, respectively. Petrogenetic studies show that the Nb-enriched basalts resulted from
partial melting of mantle wedge peridotites, which were previously metasomatized by
adakites (Mao et al., 2012). A narrow eclogite zone was reported along the boundary
between granitic gneisses and paragneisses in the Gubaoquan-Liuyuan area (Liu et al.,
2002), and the U-Pb dating of the Gubaoquan eclogites indicates an Ordovician age of c.
465 Ma for the eclogite facies metamorphism. Petrologic studies proved that eclogites
started as oceanic crust in the Palaeoasian Ocean, which was subducted to eclogite depths
in the Ordovician (Qu et al., 2011). Occurrences of early Paleozoic eclogites, Nb-enriched
basalts and arc-related dacites prove progressive subduction in the southern Beishan area
during the early Paleozoic (Liu et al., 2011; Zhang et al., 2011; Mao et al., 2012).
In the Beishan rift, there developed a series of Silurian-Devonian post-collisional
granitoids whose ages form a peak age of 415Ma in the geochronological frequency
diagram (Fig. 10), including the Shuangfengshan A-type granite (415±3Ma, Li et al., 2009),
the Huitongshan A-type granite (397±3Ma, Li et al., 2011) and high potassium
calc-alkaline granitoids (396-436 Ma, Zhao et al., 2007) in the Liuyuan area. The
Shuangfengshan A-type granite is the oldest A-type granite in the Beishan rift yet
25
discovered (Li et al., 2009). Previous studies suggest that these granitoids were formed in a
post-collisional setting, and resulted from partial melting of continental crust owing to the
under-plating of the mantle-derived magma related to slab break-off (Zhao et al., 2007; Li
et al., 2009, 2011). In addition, a molasse sedimentary sequence was found in the upper
Devonian strata around the Dundunshan area, also indicating a post-collisional setting in
the late Devonian (He et al., 2004). Thrust-nappe structures were reported in the
Precambrian to Ordovician strata, which displayed N-S compressions, W-E strike-slips and
were formed in the Late Silurian to Early Devonian (Liu et al., 2002). Characteristics of the
granitoids and strata in the Beishan rift all confirm a large-scale collisional event in the late
stage of early Paleozoic, then Beishan rift came into post-collisional stage (Fig. 11c).
The statistical results of the geochronological analysis (Fig. 10) show that magmatic
activities were rare in the Beishan rift, and no magmatic rocks have yet been reported with
an age of 340–380Ma (Table 5). Rock types of Upper Devonian and Lower Carboniferous
units in the area also correspond to the statistical results of the geochronological analysis.
The Upper Devonian is composed of keratophyre, breccia, tuff and sandstone, in
unconformable contact with the Middle Devonian. The Upper and Middle Devonian units
are continental sediments, and constitute the molasse formation in the Beishan rift (He et
al., 2004). There are also rare magmatic rocks in the Lower Carboniferous section, which is
mainly composed of phyllite, limestone, sandstone and conglomerate and characterized by
shallow-marine to nonmarine sedimentary rocks (GSBGMR, 1966). We speculate that this
period (340–380Ma) included continued orogenesis (the late Devonian) and marine
regression (the early Carboniferous) processes, with rare magmatic activities.
26
In recent studies, Zhang et al. (2008) collected age data of 18 mafic and 21 granitic
rocks from Tarim and its marginal areas, and obtained an age span of 260–320 Ma with a
peak age of 275 Ma. In addition, Qin et al. (2011) collected zircon U-Pb age data from
basalts and mafic dykes in the Beishan rift, eastern Tianshan and Tarim basin, and obtained
a peak age of 280 Ma. In the current study, we collected zircon U-Pb ages of magmatic
rocks including mafic-ultramafic rocks, diorites, granitoids and rhyolites in the Beishan rift,
and obtained a similar peak age of 282 Ma (Fig. 10). It is obvious that an important
magmatic event took place near 280Ma in the Beishan rift, even in the NW China. Most
studies suggest that magmatic rocks of this period formed in the within-plate setting (Mao
et al., 2006, 2008; Qin et al., 2011; Su et al., 2011a, 2011b, 2012b; Zhang et al., 2011a),
though there are still controversies concerning the geodynamics models, including
plume-related magmatisms (Qin et al., 2011; Su et al., 2012b) and lithospheric
delamination (Zhang et al., 2011a). As discussed above, Yinwaxia mafic rocks exhibit
obvious geochemical differences from mafic rocks in the Tarim Large Igneous Province
(TLIP). Specifically, Yinwaxia mafic rocks have obvious negative Nb-Ta-Ti anomalies, and
have higher HFSE and HREE abundances, which indicate that they derived from partial
melting of spinel lherzolites with relatively low melting degrees, unlikely typical mafic
rocks associated with plume. In addition, Yinwaxia mafic rocks also display different Sr-Nd
isotopic compositions (Fig. 7). It is notable that distributions of mafic-ultramafic rocks in
the Beishan area are linear along faults, rather than having the planar distribution expected
of a mantle plume (Fig. 1b). For example, the Poyi, Poshi and Luodong intrusions occur
along the Baidiwa fault (Mao et al., 2008; Pirajno et al., 2008), and the Liuyuan and
27
Yinwaxia mafic rocks occur along the Hongliuyuan fault (Zhang et al., 2011a; Cai et al.,
2012). It is also totally different from magmatic activities associated with a mantle plume,
which are always planar distributions (Campbell and Griffiths, 1990; Renne and Basu,
1991; Coffin and Eldholm, 1994). According to discussions above, it is hard to attribute
formations of Yinwaxia mafic rocks to magmatic activities associated with a mantle plume.
On the basis of the geochemical characteristics of Yinwaxia mafic rocks and a regional
tectonic evolutionary model using regional geochronological data, we propose that the
Yinwaxia mafic-ultramafic rocks resulted from magmatism associated with lithospheric
delamination and asthenosphere upwelling in a continental rift setting. In this scenario, the
Mazongshan and Dunhuang blocks collided in the late stage of the early Paleozoic,
thickening the lithosphere of the Beishan area, leading to a gravitational instability, which
provides the driving force for the lithosphere delamination. Afterwards the asthenosphere
upwelled and provided heat leading to partial melting of the lithopheric mantle, which had
been metasomatized by fluids or melts derived from subducted slab. In the course of rifting
in the late Carboniferous-Permian, the partial melting continued regionally, and parental
magmas of mafic and ultramafic rocks were produced owing to decompression.
Consequently, undergoing fractional crystallization (AFC) processes, parental magmas
were emplaced along faults and formed mafic and ultramafic rocks in the Beishan rift (Fig.
11d).
7. Conclusion
The Yinwaxia mafic rocks formed in the Permian (265 Ma and 281 Ma). The overall
28
isotopic compositions of these mafic rocks imply an OIB-like mantle source, display
DM-EM2 mixed trends, and indicate derivation from lithospheric mantle metasomatized by
fluids and/or melts derived from subducted slab. Parental magmas underwent fractionations
of clinopyroxene, plagioclase and Fe-Ti oxides. Yinwaxia basalts were contaminated by
parental magmas of coeval A-type granites, while gabbros were contaminated by the older
continental crust, causing different Sr-Nd isotopic characteristics for these rock types.
Taking into account the geochemistry of the Yinwaxia mafic rocks and coeval granitoids,
and characteristics of the Permian sedimentary formations, we conclude that Yinwaxia
mafic rocks were formed in a continental rift, and derived from magmatism associated with
lithospheric delamination and asthenosphere upwelling in a continental rift setting.
Acknowledgement
This study was financially supported by the National Natural Science Foundation of
China (Grant no. 41372225). We sincerely thank Wenjiao Xiao, Keda Cai and one
anonymous reviewer for their constructive comments that greatly helped to improve the
manuscript. We also appreciate the assistances of Libing Gu, Fang Ma, Hangqiang Xie,
Jinrong Li and Qiannan Li for geochronological and geochemical analyses.
29
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List of Figures
Fig. 1 (a) Geological sketch map of the Central Asian Orogenic Belt (modified after Şengör
et al., 1993; Jahn et al., 2000). (b) The geological map of the Beishan rift and its
adjacent region (modified after Wang et al., 2007; age data are from Zhao et al., 2007;
Li et al., 2009, 2011, 2013; Su et al., 2011 and references therein; Zhang et al., 2011a;
Mao et al., 2012; Jiang et al., 2013).
Fig. 2 The geological map of the Yinwaxia area (modified after GSBGMR, 1966).
Fig.3 Cathodoluminescence (CL) images and SHRIMP dating results of zircons from the
basalt and the gabbro in the Yinwaxia area.
Fig. 4 (a) The Zr/TiO2 versus Nb/Y chemical classification diagram for mafic rocks from
the Yinwaxia (after Winchester and Floyd, 1977); (b) AFM diagram (A=Na2O+K2O,
F=FeO, M=MgO) for mafic rocks from the Yinwaxia area. The boundary line between
tholeiitic and calc-alkaline rock types is from Miyashiro (1974).
Fig. 5 The Chondrite-normalized REE pattern of basalts (a) and gabbros (b) from the
Yinwaxia area (normalized data and N-MORB values are from Sun and McDonough,
1989). Mafic rocks in the Tarim large igneous province are basalts from boreholes at
depths between 5,166 and 6,333 m in the northern Tarim uplift (Tian et al., 2010).
48
Fig.6 The N-MORB-normalized trace elements spiderdiagram of basalts (a) and gabbros(b)
from the Yinwaxia area (normalized data and E-MORB values are from Sun and
McDonough, 1989).Mafic rocks in the Tarim large igneous province are basalts from
boreholes at depths between 5,166 and 6,333 m in the northern Tarim uplift (Tian et
al., 2010). Data of basalts in the East African Rift, average continental arc and OIB are
collected from Shinjo et al. (2011), Kelemen et al. (2004) and Sun and McDonough
(1989).
Fig. 7 εNd(t) vs. (87Sr/86Sr)i diagram for mafic rocks from the Yinwaxia area (Zindler and
Hart,1986). Data for mafic rocks in the western part of Beishan rift are from Su et al.,
(2012). Data for mafic rocks in the Liuyuan area are from Zhang et al. (2011a). Data
for granites in the Yinwaxia area are from Zhang et al. (2011b) and Feng et al. (2012).
DMM, depleted mantle-derived melt; EM1, enriched mantle1; EM2, enriched mantle2;
εNd(280Ma)=10.96 and (87Sr/86Sr)i=0.7022 are values of DMM.
Fig. 8 (a) Plots of Alz (percentage of tetrahedral sites occupied by Al) vs. TiO2 in
clinopyroxenes from gabbros of the Yinwaxia area (after Loucks, 1990).
(b) The TiO2-Na2O-SiO2/100 diagram, using compositions of clinopyroxenes for
discriminating different tectonic settings (after Beccaluva et al., 1989). Abbreviations,
E-MORB: enriched mid-ocean ridge basalt; N-MORB: normal mid-ocean ridge basalt;
WOPB: within oceanic plate basalts; ICB: Iceland basalts; SSZ: supra-subduction
49
zone basalts.
Fig. 9 Tectonic setting discrimination diagrams for Yinwaxia mafic rocks. (a) Zr/Y-Zr
diagram (after Pearce and Norry, 1979); (b) Ti–Zr diagram (after Pearce, 1982).
Fig. 10 Relative probability plots of zircon 206Pb/238U ages from magmatic and
metamorphic rocks in the Beishan rift and its adjacent area.
Fig. 11 The tectonic evolution model for the Beishan rift. See text for detailed discussions.
List of tables
Table 1 SHRIMP U-Pb data of the basalt (Y-14) and the gabbro (Y-5) in the Yinwaxia area.
Notes: Errors are 1-sigma; Pbc and Pb* indicate the common and radiogenic lead,
respectively. Common Pb corrected using measured 204Pb.
Table 2 Major and trace elements compositions of basalts and gabbros in the Yinwaxia
area.
Table 3 Whole rock isotopic compositions of basalts and gabbros in the Yinwaxia area.
Table 4 Major element analyses of clinopyroxenes from gabbros of the Yinwaxia area.
Table 5 Compiled ages of magmatic and metamorphic rocks in the Beishan rift and its
adjacent area.
50
Table 1
Notes: Common Pb corrected using the measured 204Pb. Pb* indicate the radiogenic lead, Pbc indicate the common lead.
Spots U
(ppm)
Th
(ppm) Th/U
206Pb*
(ppm)
206Pbc
(%)
207Pb* 206Pb*
±%
207Pb* 235U
±%
206Pb* 238U
±%
Age(Ma) 206Pb 238U
1σ 207Pb 206Pb
1σ
The gabbro sample ( Y-5) 1.1 216 174 0.84 8.9 1.25 0.0557 9.9 0.36 10.2 0.0472 2.5 297.3 7.3 441 220
2.1 63 52 0.86 2.6 5.69 0.0576 49.7 0.35 50.0 0.0445 6.0 280.9 16.4 516 1091
3.1 303 42 0.14 11.5 1.57 0.0471 8.8 0.28 9.1 0.0437 2.1 275.8 5.7 54 210
4.1 263 55 0.22 77.9 0.24 0.1139 1.7 5.39 2.6 0.3433 2.0 1902.6 32.2 1862 30
5.1 398 213 0.55 14.4 0.56 0.0530 6.1 0.31 6.5 0.0420 2.0 264.9 5.3 328 139
6.1 511 196 0.40 19.8 1.54 0.0542 5.2 0.33 5.8 0.0445 2.6 280.5 7.0 380 118
7.1 133 58 0.45 5.2 1.02 0.0470 3.7 0.29 4.3 0.0454 2.2 286.2 6.1 50 87
8.1 117 64 0.56 4.7 0.79 0.0470 7.5 0.30 7.8 0.0468 2.2 295.0 6.4 49 179
9.1 162 81 0.52 43.0 0.06 0.1032 0.8 4.38 2.2 0.3078 2.0 1729.7 30.5 1683 15
The basalt sample ( Y-14)
1.1 79 24 0.31 27.6 0.67 .1437 2.1 7.98 3.0 .4028 2.2 2181.9 41.3 2273 36
2.1 201 183 0.94 7.2 2.44 .0510 16.0 0.29 16.2 .0406 2.4 256.7 6.0 242 369
3.1 500 112 0.23 21.6 0.66 .0516 2.9 0.36 3.5 .0500 1.9 314.3 5.8 268 66
4.1 233 139 0.62 9.3 1.37 .0487 9.5 0.31 9.7 .0456 2.1 287.3 5.9 136 222
5.1 241 152 0.65 8.9 1.88 .0479 6.9 0.28 7.2 .0423 2.1 267.4 5.5 92 163
6.1 133 58 0.45 5.2 1.02 .0470 3.7 0.29 4.3 .0454 2.2 286.2 6.1 50 87
7.1 117 64 0.56 4.7 0.79 .0470 7.5 0.30 7.8 .0468 2.2 295.0 6.4 49 179
8.1 197 198 1.04 7.8 1.81 .0466 24.1 0.29 24.2 .0454 2.5 286.2 7.1 27 577
9.1 200 117 0.60 8.2 4.55 .0318 32.9 0.20 33.0 .0454 2.5 286.1 6.9 -983 972
10.1 142 63 0.46 36.6 0.00 .1133 1.2 4.69 2.4 .3005 2.1 1693.7 31.1 1852 22
51
Table 2
No. Y-1 Y-2 Y-3 Y-4 Y-5 Y-6 Y-7 Y-8 Y-9
Rocks Gabbro Gabbro Gabbro Gabbro Gabbro Gabbro Gabbro Basalt Basalt
SiO2 55.62 52.81 52.96 53.33 51.70 53.27 50.37 53.29 54.15 TiO2 1.59 1.38 2.06 2.16 1.36 1.32 1.335 2.56 2.56 Al2O3 15.48 16.06 15.31 15.25 15.27 15.27 13.63 14.74 14.53
TFe2O3 9.54 9.28 11.04 11.08 9.20 8.96 8.72 12.89 11.98 MnO 0.16 0.15 0.20 0.16 0.15 0.12 0.164 0.24 0.22 MgO 5.46 6.22 5.36 5.13 6.26 6.16 6.32 3.72 3.14 CaO 5.60 9.36 6.70 6.45 8.96 7.49 8.46 6.35 6.59Na2O 2.79 1.00 1.80 1.87 2.33 2.22 4.97 1.64 1.51 K2O 0.52 0.93 0.88 0.90 0.91 1.19 0.76 1.35 1.69 P2O5 0.27 0.21 0.34 0.36 0.23 0.23 0.237 0.78 0.80LOI 2.83 2.47 3.21 3.20 3.52 3.64 4.92 2.29 2.72Total 99.85 99.88 99.88 99.89 99.88 99.87 99.89 99.86 99.89 Mg# 55.75 59.59 51.66 50.49 59.99 60.21 61.49 38.81 36.59
Sc 31.0 30.9 36.3 34.0 33.8 26.5 36.1 26.3 25.8 V 183 165 230 225 178 152 220 174 177 Co 33.8 35.8 30.6 31.4 35.3 32.8 34.2 21.8 18.1 Ga 17.9 17.2 18.0 18.7 17.4 17.1 19.0 22.9 21.4 Li 13.9 14.5 15.7 16.5 14.5 14.7 10.7 8.05 7.37Be 1.29 1.03 1.05 1.33 1.03 1.32 1.129 1.66 1.41 Cs 0.38 0.41 0.58 0.68 0.90 0.73 0.8182 0.89 0.80 Rb 3.71 72.3 15.6 13.8 11.6 43.4 20.7 14.7 17.5 Sr 232 341 197 187 406 347 588 220 331 Ba 222 107 164 118 102 125 175 226 254 Th 3.54 2.55 2.49 3.00 2.65 3.97 2.48 2.77 2.52 U 1.30 0.825 0.741 0.934 0.813 1.15 0.855 1.07 1.13Ta 0.593 0.462 0.581 0.591 0.434 0.573 0.417 0.923 0.864 Nb 8.84 7.02 8.77 9.30 7.19 8.55 7.38 14.6 13.5 Hf 6.34 4.84 5.48 6.31 5.02 6.39 6.74 8.53 7.96 Zr 299 228 262 299 229 303 248 406 377 Y 40.1 33.1 40.8 42.0 34.3 37.4 40.9 63.3 61.7 Pb 11.8 11.7 15.9 4.86 7.77 9.55 10.7 7.84 6.46 La 15.5 12.4 12.2 15.8 12.5 15.3 14.4 24.7 23.5 Ce 39.5 31.5 33.4 40.5 32.3 38.4 37.2 61.2 58.8Pr 5.09 4.02 4.52 5.25 4.16 4.86 5.10 8.23 7.97 Nd 23.5 18.6 22.1 24.6 19.5 22.1 22.9 39.8 38.9 Sm 5.96 4.80 5.99 6.37 5.08 5.61 5.85 10.2 10.1Eu 1.74 1.52 1.95 1.89 1.62 1.51 1.79 3.47 3.37 Gd 7.04 5.62 7.11 7.43 6.02 6.49 6.84 11.9 11.7 Tb 1.16 0.943 1.18 1.24 1.01 1.08 1.14 1.92 1.89 Dy 7.42 5.99 7.51 7.79 6.39 6.99 7.21 12.0 11.7
52
Table 2 continued
No. Y-10 Y-11 Y-12 Y-13 Y-14 Y-15 Y-16 Y-17
Rocks Basalt Basalt Basalt Basalt Basalt Basalt Basalt Basalt
SiO2 51.46 51.73 53.90 52.82 51.77 53.18 53.33 47.38 TiO2 2.77 2.69 2.57 2.88 1.99 2.10 2.05 2.62 Al2O3 14.00 14.16 14.66 14.65 14.55 13.74 13.03 13.73
TFe2O3 13.61 13.72 12.94 13.23 11.00 11.61 10.40 14.11 MnO 0.24 0.28 0.25 0.23 0.21 0.21 0.21 0.20 MgO 4.03 4.08 3.33 3.55 3.90 3.93 4.29 3.99 CaO 6.56 6.43 5.84 5.26 6.43 6.10 6.84 6.59 Na2O 2.50 1.59 1.61 2.05 4.40 4.45 3.81 4.14 K2O 1.04 1.07 1.54 1.72 1.30 2.26 1.96 1.36 P2O5 0.82 0.86 0.80 0.88 0.75 0.69 0.68 1.10 LOI 2.87 3.28 2.43 2.41 3.59 1.60 3.30 4.69 Total 99.89 99.88 99.87 99.68 99.90 99.89 99.9. 99.91 Mg# 39.44 39.53 36.13 37.13 43.84 42.70 47.59 38.39
Sc 27.5 26.0 26.2 27.4 28.0 28.6 27.7 35.1 V 209 176 170 179 174 197 188 336 Co 24.5 23.4 19.3 22.9 18.0 20.8 17.8 37.5 Ga 21.2 21.2 22.7 22.8 24.7 25.5 23.6 23.1 Li 8.89 9.64 8.72 10.1 9.11 5.27 6.64 22.2 Be 1.56 1.41 1.54 1.45 1.40 1.64 1.46 1.07 Cs 0.462 0.361 1.00 0.794 1.31 0.711 0.911 3.43 Rb 11.0 10.8 16.8 16.9 13.0 21.7 23.1 31.4 Sr 239 290 220 299 317 332 266 346 Ba 150 131 265 250 442 379 247 179 Th 2.32 2.47 2.82 2.63 2.82 2.99 2.70 1.56 U 0.872 0.903 0.921 1.13 1.31 1.17 0.878 0.561Ta 0.813 0.851 0.872 0.864 0.749 0.813 0.427 0.554 Nb 12.8 13.6 14.2 13.9 13.8 14.2 10.9 8.64 Hf 7.44 7.59 8.71 8.24 10.4 11.2 10.0 7.27 Zr 353 363 418 388 388 421 377 238 Y 59.8 59.9 64.6 63.9 70.9 72.1 66.1 55.7 Pb 6.18 8.29 11.3 11.2 10.7 9.45 10.7 16.9 La 22.0 22.6 24.5 24.5 25.0 25.9 24.5 19.1
Ho 1.52 1.23 1.54 1.59 1.31 1.43 1.47 2.43 2.37Er 4.50 3.65 4.45 4.64 3.87 4.26 4.30 7.02 6.83 Tm 0.642 0.513 0.622 0.662 0.551 0.622 0.612 0.994 0.953 Yb 4.25 3.41 4.08 4.34 3.64 4.08 3.97 6.51 6.19 Lu 0.621 0.494 0.591 0.632 0.533 0.592 0.584 0.972 0.914
∑REE 118.45 94.69 107.25 122.76 98.49 113.33 113.33 191.35 185.19
(La/Nb)N 3.65 3.64 2.99 3.64 3.43 3.75 3.62 3.79 3.79
δEu 0.82 0.89 0.91 0.84 0.86 0.77 0.87 0.97 0.95
53
Ce 55.8 56.8 61.9 62.1 65.6 65.9 61.7 50.2 Pr 7.63 7.72 8.32 8.39 9.06 9.01 8.35 7.18 Nd 37.6 37.6 40.2 41.0 45.4 43.9 41.3 37.1 Sm 9.84 9.76 10.3 10.7 11.4 11.2 10.5 9.91 Eu 3.25 3.25 3.45 3.58 3.69 3.74 3.59 3.45 Gd 11.6 11.5 12.1 12.4 12.9 12.9 12.0 11.4 Tb 1.86 1.85 1.96 1.99 2.12 2.13 1.95 1.79 Dy 11.6 11.5 12.2 12.3 13.0 13.1 12.1 10.7 Ho 2.32 2.32 2.48 2.49 2.61 2.65 2.44 2.09 Er 6.61 6.69 7.25 7.14 7.56 7.69 7.05 5.78 Tm 0.924 0.933 1.02 0.992 1.05 1.09 0.992 0.774 Yb 5.99 6.09 6.67 6.47 6.90 7.06 6.47 4.81 Lu 0.872 0.891 0.983 0.952 1.03 1.05 0.961 0.692
∑REE 177.89 179.50 193.33 195.03 207.43 207.24 193.86 164.90
(La/Nb)N 3.67 3.71 3.67 3.78 3.63 3.67 3.79 3.97
δEu 0.93 0.94 0.95 0.95 0.93 0.95 0.98 0.99 Note: Major elements are analyzed using XRF (in wt %), trace elements using ICP-MS (in ppm)
54
Table 3
Sample No.
Rb [ppm]
Sr [ppm]
87Rb/86Sr 87Sr/86Sr Error (2σ)
(87Sr/86Sr)i Sm [ppm]
Nd [ppm]
147Sm/144Nd 143Nd/144Nd Error (2σ)
(143Nd/144Nd)i εNd(t)
Y-8 13.4 204.3 0.1895 0.704475 0.000012 0.703774 10.4 39.6 0.1598 0.512938 0.000011 0.512644 7.09
Y-9 17.2 265.6 0.1874 0.706015 0.000013 0.705322 10.5 39.2 0.1617 0.512945 0.000010 0.512648 7.16
Y-10 9.75 189.8 0.1487 0.704405 0.000015 0.703854 9.20 34.7 0.1608 0.512950 0.000012 0.512654 7.28
Y-11 10.4 198.4 0.1516 0.704556 0.000014 0.703996 9.52 35.9 0.1605 0.512949 0.000011 0.512654 7.27
Y-12 16.4 196.5 0.2422 0.704718 0.000013 0.703822 10.3 38.8 0.1605 0.512817 0.000013 0.512521 4.69
Y-6 41.4 345.8 0.3612 0.709434 0.000011 0.707990 5.61 22.10 0.1359 0.512351 0.000015 0.512101 -3.41
Y-7 20.5 568.0 0.1018 0.707188 0.000015 0.706781 5.71 22.4 0.1276 0.512410 0.000014 0.512175 -1.97
Y-5 11.4 407.3 0.0824 0.708110 0.000015 0.707781 5.18 19.71 0.1405 0.512500 0.000010 0.512241 -0.68
Y-2 71.3 336.1 0.6137 0.709193 0.000012 0.706739 4.60 18.53 0.1283 0.512463 0.000011 0.512227 -0.96
Y-1 3.51 231.2 0.0462 0.707304 0.000011 0.707119 5.76 23.13 0.1385 0.512497 0.000012 0.512242 -0.66
55
Table 4
Continued
Sample 4.3 5.1 5.2 6.1 6.2 6.3 7.1 7.2
SiO2 52.03 52.15 52.24 52.41 51.63 51.07 50.92 51.67
TiO2 0.85 0.71 0.72 0.73 0.84 1.05 0.85 0.81
Al2O3 2.23 2.45 2.14 2.04 2.01 2.04 2.2 2.51
Cr2O3 0.21 0.41 0.26 0.44 0.01 0 0.05 0.57
Fe2O3 1.53 1.19 0.05 0.94 2.43 1.11 2.69 2.6
FeO 5.44 5.1 6.44 5.46 5.54 7.72 5.27 3.98
Sample 1.1 2.1 2.2 3.1 3.2 4.1 4.2 9.2
SiO2 51.13 51.58 52.16 50.83 50.9 51.17 51.37 51.39
TiO2 0.93 0.88 0.87 0.79 0.8 0.94 0.99 0.86
Al2O3 3.15 2.28 2.42 3.17 2.3 1.93 2.17 2.46
Cr2O3 0.62 0.03 0.12 0.76 0.45 0.02 0 0.27
Fe2O3 2.31 1.66 1.87 2.05 2.57 2.05 1.78 2.42
FeO 4.5 5.85 5.46 4.35 4.22 6.42 6.3 4.45
MnO 0.13 0.23 0.21 0.19 0.2 0.24 0.23 0.14
MgO 16.25 15.93 16.38 16.33 16.17 15.55 15.8 15.72
CaO 20.67 20.73 20.84 20.35 20.81 20.26 20.21 21.7
Na2O 0.41 0.31 0.33 0.37 0.35 0.36 0.36 0.39
K2O 0 0 0.02 0.02 0.02 0.01 0.02 0
Totals 100.1 99.48 100.68 99.21 98.79 98.94 99.23 99.8
Cations normalized to 6 oxygens
Si 1.88 1.913 1.909 1.883 1.897 1.915 1.913 1.899
Ti 0.026 0.025 0.024 0.022 0.022 0.026 0.028 0.024
Al 0.137 0.1 0.104 0.138 0.101 0.085 0.095 0.107
Cr 0.018 0.001 0.003 0.022 0.013 0.001 0 0.008
Fe3+ 0.064 0.046 0.051 0.057 0.072 0.058 0.05 0.067
Fe2+ 0.138 0.181 0.167 0.135 0.131 0.201 0.196 0.138
Mn 0.004 0.007 0.007 0.006 0.006 0.008 0.007 0.004
Mg 0.89 0.881 0.893 0.901 0.898 0.867 0.877 0.866
Ca 0.814 0.824 0.817 0.808 0.831 0.813 0.807 0.859
Na 0.029 0.022 0.023 0.027 0.025 0.026 0.026 0.028
K 0 0 0.001 0.001 0.001 0 0.001 0
Sum 4 4 4 4 4 4 4 4
Wo 42.69 42.63 42.35 42.48 42.99 41.91 41.79 44.52
En 46.7 45.58 46.32 47.43 46.48 44.75 45.46 44.87
Fs 10.61 11.79 11.33 10.09 10.53 13.34 12.75 10.61
56
MnO 0.21 0.17 0.14 0.18 0.25 0.25 0.15 0.17
MgO 16.49 16.4 16.23 16.67 15.96 15.11 15.77 16.42
CaO 20.55 20.92 20.53 20.57 20.53 19.82 20.72 20.97
Na2O 0.34 0.36 0.28 0.35 0.42 0.37 0.34 0.48
K2O 0.01 0.01 0 0 0 0 0 0
Totals 99.89 99.87 99.04 99.78 99.62 98.54 98.96 100.18
Cations normalized to 6 oxygens
Si 1.916 1.918 1.939 1.929 1.914 1.923 1.902 1.896
Ti 0.024 0.02 0.02 0.02 0.023 0.03 0.024 0.022
Al 0.097 0.106 0.094 0.089 0.088 0.091 0.097 0.109
Cr 0.006 0.012 0.008 0.013 0 0 0.001 0.017
Fe3+ 0.042 0.033 0.001 0.026 0.068 0.031 0.075 0.072
Fe2+ 0.168 0.157 0.2 0.168 0.172 0.243 0.165 0.122
Mn 0.007 0.005 0.004 0.006 0.008 0.008 0.005 0.005
Mg 0.905 0.899 0.898 0.914 0.882 0.848 0.878 0.898
Ca 0.811 0.824 0.816 0.811 0.815 0.8 0.829 0.825
Na 0.024 0.026 0.02 0.025 0.03 0.027 0.025 0.034
K 0 0 0 0 0 0 0 0
Sum 4 4 4 4 4 4 4 4
Wo 42.1 43.08 42.62 42.25 42.1 41.6 42.58 43.02
En 47 47 46.88 47.64 45.54 44.12 45.09 46.87
Fs 10.9 9.92 10.51 10.11 12.37 14.28 12.33 10.12 Continued
Sample 7.3 8.1 8.2 9.1
SiO2 51.46 50.85 51.32 51.73
TiO2 0.74 0.96 0.96 0.91
Al2O3 2.3 3.17 2.34 2.2
Cr2O3 0.56 0.46 0.03 0.07
Fe2O3 2.32 1.41 2.22 1.36
FeO 3.96 5.03 5.6 6.13
MnO 0.21 0.14 0.22 0.18
MgO 16.9 15.94 15.67 15.95
CaO 20.48 20.43 20.82 20.57
Na2O 0.36 0.4 0.39 0.34
K2O 0 0.02 0 0
Totals 99.29 98.81 99.56 99.45
Cations normalized to 6 oxygens
Si 1.902 1.892 1.905 1.919
Ti 0.021 0.027 0.027 0.025
57
Al 0.1 0.139 0.102 0.096
Cr 0.016 0.014 0.001 0.002
Fe3+ 0.065 0.04 0.062 0.038
Fe2+ 0.122 0.156 0.174 0.19
Mn 0.007 0.004 0.007 0.006
Mg 0.931 0.884 0.867 0.882
Ca 0.811 0.814 0.828 0.818
Na 0.026 0.029 0.028 0.024
K 0 0.001 0 0
Sum 4 4 4 4
Wo 42.04 42.99 42.88 42.41
En 48.27 46.67 44.91 45.76
Fs 9.69 10.34 12.21 11.83
58
Table 5
Location Rock type Age (Ma) Analytical method Data source
Xuanwoling Gabbro 260.7±2.0 SIMS Su et al., 2010a
Poshi Olivine gabbro 275.5±1.2 SIMS Ao, 2010
Poshi Olivine gabbro 284±2.2 SIMS Qin et al., 2011
Poyi Alkaline granite vein 251.4±1.4 SIMS Su et al., 2010b
Poyi Gabbro 271±6.2 SIMS Ao, 2010
Luodong Gabbro 284.0±2.3 SIMS Su et al., 2010b
Luodong Gabbro 283.8±1.1 LA-ICP-MS Ao, 2010
Hongshishan Olivine gabbro 281.8±2.6 LA-ICP-MS Ao et al., 2010
Hongshishan Troctolite 286.4±2.8 SIMS Su et al., 2010c
Hongshishan Diorite 279.7±4.8 SIMS Qin et al., 2011
Hongshishan Dacite 279.1±2.9 SIMS Qin et al., 2011
Hongshishan Ryholite 321.7±3.4 SIMS Su et al., 2011
Bijiashan Gabbro 279.2±2.3 SIMS Qin et al., 2011
Liuyuan Nb-enriched basalts 451.6±4.4 SIMS Mao et al., 2012
Liuyuan Dacites 442.23±3.1 SIMS Mao et al., 2012
Liuyuan Diorite 272.7±4.4 SHRIMP Zhang et al., 2011
Liuyuan Diorite 291.4±4.9 SHRIMP Zhang et al., 2011
Liuyuan Ultramafic rocks 250.4±9.0 SHRIMP Zhang et al., 2011
Liuyuan Granodiorite 423±8 SHRIMP Zhao et al., 2007
Liuyuan Monzonitic granite 396±15 SHRIMP Zhao et al., 2007
Liuyuan K-feldspar granite 436±9 SHRIMP Zhao et al., 2007
Shuangfengshan A-type granite 415±3 LA-ICP-MS Li et al., 2009
Huitongshan A-type granite 397±3 LA-ICP-MS Li et al., 2011
Gubaoquan Eclogite 465±10 LA-ICP-MS Liu et al., 2011
Hongliuhe ophiolite Cumulate gabbro 516.2±7.1 SHRIMP Zhang and Guo, 2008
Hongliuhe ophiolite Biotite granite 404.8±5.2 SHRIMP Zhang and Guo, 2008
Qiaowan Granodiorite 303.7±2.4 LA-ICP-MS Feng et al., 2012
59
Yinwaxia Biotite granite 281. 7 ± 2. 9 LA-ICP-MS Zhang et al., 2011
Xijianquanzi Monzonitic granite 266.1±2.2 LA-ICP-MS Zhang et al., 2010
Yueyashan ophiolite Plagiogranite 533±1.7 SIMS Ao et al., 2011
Yueyashan ophiolite Plagiogranite 536±7 SHRIMP Hou et al., 2012
60
61
62
63
64
65
66
67
68
69
70
71
Highlights
� Yinwaxia mafic rocks were formed in Permian (265 Ma and 281 Ma).
� They derived from lithospheric mantle metasomatized by fluids and/or melts.
� Yinwaxia mafic rocks formed in a continental rift.