draft · 2020-03-24 · draft 21 granitoids were derived from common sources of melting from the...
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Early–Middle Permian postcollisional granitoids in the northern Beishan orogen, NW China: Evidence from U–Pb
ages and Sr–Nd–Hf isotopes
Journal: Canadian Journal of Earth Sciences
Manuscript ID cjes-2019-0088.R2
Manuscript Type: Article
Date Submitted by the Author: 01-Oct-2019
Complete List of Authors: Min, Li; China Geological Survey, Tianjin Center,China Geological Survey; China Geological Survey, North China Center for Geoscience InnovationHoutian, Xin; China Geological Survey, Tianjin Center, China Geological Survey; China Geological Survey, North China Center for Geoscience InnovationBangfang, Ren; China Geological Survey, Tianjin Center, China Geological Survey; China Geological Survey, North China Center for Geoscience InnovationYunwei, Ren; China Geological Survey, Tianjin Center, China Geological Survey; China Geological Survey, North China Center for Geoscience InnovationWengang, Liu; China Geological Survey, Tianjin Center, China Geological Survey; China Geological Survey, North China Center for Geoscience Innovation
Keyword: northern Beishan orogen, Early–Middle Permian, tectonic setting, zircon U–Pb dating, Sr–Nd isotopes, zircon Hf isotopes
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1 Early–Middle Permian postcollisional granitoids in the northern
2 Beishan orogen, NW China: Evidence from U–Pb ages and Sr–Nd–
3 Hf isotopes
4 Min Li1,2,*, Houtian Xin1,2, Bangfang Ren1,2, Yunwei Ren1,2, and Wengang Liu1,2
5 1Tianjin Center, China Geological Survey, Tianjian, 300170, China
6 2North China Center for Geoscience Innovation, Tianjian, 300170, China
7 Abstract: The geochemistry and Sr–Nd isotope, zircon U–Pb, and zircon Hf isotope
8 compositions are reported for monzogranites and granodiorites from the Hazhu area in
9 the northern Beishan orogen, NW China. Zircon U–Pb dating yields two ages of 270.1
10 ± 1.1 and 277.4 ± 1.2 Ma for the monzogranites and 263.6 ± 1.2 and 262.2 ± 1.1 Ma
11 for the granodiorites. These monzogranites and granodiorites are metaluminous to
12 weakly peraluminous I-type and belong to mid-K calc-alkaline and high-K
13 calc-alkaline series. They exhibit high Mg# values and middle degrees of
14 differentiation (D.I. = 70.7–88.1). They are enriched in large-ion lithophile elements
15 and light rare-earth elements and depleted in high field strength elements. They
16 display high (87Sr/86Sr)i ratios of 0.6995 to 0.7070 and high εNd(t) values of 4.37–5.70
17 with Nd model ages (TDM) of 522–789 Ma, suggesting a juvenile crustal origin.
18 Furthermore, their εHf(t) values are all positive, and Hf isotopic crustal model ages
19 (TC DM = 394–1097 Ma) also indicate a juvenile crustal origin. According to the data
20 obtained in this study and other regional geological data acquired recently, the Hazhu
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21 granitoids were derived from common sources of melting from the Neoproterozoic to
22 Late Paleozoic juvenile crusts. The younger intrusions (granidiorites) are more basic,
23 probably as a result of more juvenile lower crust being melted along with
24 asthenospheric upwelling, which led to the addition of more basic components. These
25 granitoids formed in a postcollisional setting. The tectonic regime transformed from
26 an arc-related compressional setting to postcollisional extension, probably as a result
27 of lithospheric extension and thinning in response to oceanic lithospheric
28 delamination. These granitoids in the northern Beishan orogen were probably
29 emplaced in a postcollisional extensional setting and suggest vertical continental
30 crustal growth in the southern Central Asian Orogenic Belt.
31 Key words:northern Beishan orogen; Early–Middle Permian; tectonic setting;
32 zircon U–Pb dating; Sr–Nd isotopes; zircon Hf isotopes
33 1. Introduction
34 The Central Asian Orogenic Belt (CAOB), located among the Eastern Europe,
35 Siberia, Tarim, and North China plates (Fig. 1a), which evolved from the Late
36 Mesoproterozoic (Kröner et al., 2014), is one of the world’s most significant areas in
37 terms of continental crust growth and transformation in the Phanerozoic (Sengör et
38 al., 1993; Khain et al., 2002; Jahn et al., 2009; Windley et al., 2007; Sun et al., 2008;
39 Xiao et al., 2009,2010; Lei et al., 2011; Wilhem et al., 2012; He et al., 2014; Tian et
40 al., 2015; Zhu et al., 2016). The orogenesis of the CAOB was long-lived, lasting
41 for >800 million years, involving multiple subduction phases and long, continuous
42 accretion and featuring complex accretionary orogenesis and continental growth (Xiao
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43 and Santosh, 2014). The CAOB significantly grew laterally during multiple growth
44 periods in the Paleozoic (Xiao et al., 2008; Xu et al., 2013). The Beishan orogen,
45 situated at the southern margin of the CAOB (Fig. 1b), is a conjunction region of the
46 Kazakhstan plate and North China (Alxa block) and Tarim (Dunhuang block) cratons
47 (Liu et al., 2011; Zhao et al., 2012; Zhang et al., 2012a; Guo et al., 2014; Xu et al.,
48 2014; Zhao et al., 2015). The Beishan orogen is considered to be the eastern extension
49 of the Tianshan orogeny tectonically (Liu and Wang, 1995; Xiao et al., 2010), and it is
50 connected to Tianshan suture zone to the west and to the Soren suture zone to the east
51 (Guo et al., 2012). The Beishan orogen comprises an assemblage of blocks (Su et al.,
52 2012), magmatic arcs, and ophiolitic m é langes formed by subduction–accretion
53 processes of the Paleo-Asian Ocean (Zheng et al., 2014; Cleven, et al., 2015a; Ao et
54 al., 2016).
55 As an important part of the southern margin of the CAOB, granitoids widely
56 developed during the formation of the Beishan orogen in the Paleozoic (Jiang et al.,
57 2006; Su et al., 2011; Zhang et al., 2012b; Li et al., 2013; Jia et al., 2016). Two phases
58 of subduction and collision orogeny occurred in the Beishan area in the Paleozoic.
59 The first phase occurred in the Early Paleozoic from the Middle Cambrian to the Late
60 Silurian (Dai et al., 2003; He et al., 2005). The weighted mean 206Pb–238U age of 533
61 ± 1.7 Ma obtained from a plagiogranite in the Yueyashan–Xichangjing ophiolite
62 indicates that the ocean floor formed during the Early Cambrian (Ao et al., 2012). The
63 Hongliuhe–Niujuanzi–Xichangjing Ocean underwent northward subduction beneath
64 the Mazongshan microcontinent from the Late Ordovician to the Late Silurian (He et
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65 al., 2005; Yang et al., 2013; Cleven et al., 2015b; Song et al., 2016). The ocean closed
66 at the end of the Silurian (He et al., 2005). The second phase occurred in the Late
67 Paleozoic with development of the Hongshishan–Baiheshan Ocean in the Early
68 Carboniferous (He et al., 2005; Wang et al., 2014). After that, the tectonic magmatic
69 evolution is controversial. Considerable research has focused on the southern Beishan
70 orogen in the Late Paleozoic. The Beishan orogen was in a postorogenic stage of the
71 extensional environment in the Late Carboniferous (Feng et al., 2012). From the
72 beginning of the late Early Permian, it progressed to a rift stage during a
73 postcollisional extensional period (Zhang et al., 2011). However, little research has
74 addressed the northern Beishan orogen in the Late Paleozoic, especially in the
75 Permian.
76 In this contribution, we present new geochronological and major and trace
77 element data, as well as Sr–Nd isotopic compositions and zircon Hf isotopic
78 compositions, for the granitoids in the Hazhu area in the northern Beishan orogen.
79 Our aim is to provide further insight into the mechanism of
80 petrogenesis, properties of the magma sources, and tectonic history of the northern
81 Beishan orogen.
82 2. Regional geologic background
83 The tectonic units of the Beishan area are divided into the Tarim plate in the south
84 side and the Kazakhstan plate in the north side (Ao et al., 2012; Yang et al., 2012;
85 Zheng et al., 2012;Tian et al., 2014). A secondary tectonic unit is in the Kazakhstan
86 plate; in order from north to south, this unit comprises the Queershan–Hulishan Early
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87 Paleozoic active continental margin zone, the Hongshishan–Heiyingshan Late
88 Paleozoic active continental margin zone, the Xingxingxia–Mingshui–Hanshan block
89 (Ding et al., 2017), and the Gongpoquan–Dongqiyishan Early Paleozoic active
90 continental margin zone (Yang et al., 2012; Song et al., 2013; Guo et al., 2014; Yu et
91 al., 2016; Wang et al., 2018) (Fig. 1b).
92 The study area, located south of the Hongshishan–Baiheshan–Pengboshan fault,
93 belongs to the Hongshishan–Heiyingshan Late Paleozoic active continental margin
94 zone (Fig. 1b). It mainly comprises Paleozoic strata, including Middle Devonian and
95 Carboniferous strata, and the Carboniferous strata are distributed most widely. The
96 Carboniferous strata include the Lvtiaoshan Formation and the Baishan Formation.
97 The Lvtiaoshan Formation mainly consists of clastic rocks, including sandstones,
98 pebbly sandstones, limestones, and bioclastic limestones. The Baishan Formation
99 mainly consists of felsic volcanic and pyroclastic rocks with eruption–explosion
100 facies, including rhyolite and rhyolitic welded tuff. Additionally, there exist
101 Precambrian overlying sedimentary rocks—the Beishan Rock Group in the
102 southwestern part of the study area.
103 Permian granitoids are situated in the eastern part the study area; these include
104 granodiorites and monzogranites, which form an elliptic complex (Fig. 2). This
105 subrounded pluton, with an outcrop area of 100 km2, invaded the Carboniferous
106 granite and sandstone of the Lvtiaoshan Formation. This resulted in small
107 compressional deformation folds (Fig. 3a) in the sandstone, the fold hinges of which
108 are perpendicular to the compression direction formed by the pluton emplacement.
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109 The monzogranites are located at the edge of the elliptic complex rock, and the
110 granodiorites, which intrude into the monzogranites (Fig. 3b), are located in the center
111 of the elliptic complex rock.
112 And there are many magic microgranular enclaves (MMEs) in the complex; these
113 are spherical (Figs. 3c–3e), with the larger ones being >100 cm in diameter (Fig. 3c).
114 Some of them have fine-grained rims and a chilled border (Fig. 3f). The MMEs have
115 the same plagioclase phenocryst and amphibole phenocryst as the host rock (Figs. 3d–
116 3f), and there are many plagioclase phenocrysts and amphibole phenocrysts in the
117 MMEs (Fig. 3f).
118 The monzogranites are characterized by rapakivi-like texture (Fig. 3g) with
119 massive structure. They are composed of phenocrysts (10%–15%) and matrix (85%–
120 90%), the former consisting of k-feldspar and plagioclase (Fig. 3h) and the latter
121 consisting of k-feldspar, quartz, plagioclase, biotite, and hornblende (Fig. 3h). The
122 rock contains k-feldspar (35%–40%), plagioclase (30%–35%), quartz (20%–25%),
123 biotite (3%–4%), and hornblende (1%–2%).
124 The granodiorites (Fig. 3i) are composed of phenocrysts (10%) and matrix
125 (90%), the former consisting of plagioclase and quartz and the latter consisting of
126 plagioclase, k-feldspar, quartz, biotite, and hornblende. The rock contains plagioclase
127 (50%–55%), k-feldspar (15%–20%), quartz (20%–25%), biotite (1%–2%), and
128 hornblende (3%–4%).
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129 3. Sample analysis method
130 3.1. Zircon U–Pb and Hf isotope analysis
131 Zircons for laser ablation multicollector inductively coupled plasma mass
132 spectrometry (LA-ICP-MS) U–Pb dating were separated from two samples of the
133 monzogranites (02TW19 and 02TW24) and two samples of the granodiorites
134 (02TW31 and 02TW32). Zircon sorting was completed by the Langfang Geological
135 Survey Institute of Hebei Province. The samples were crushed and washed in
136 accordance with the conventional method and separated by magnetic and gravity
137 liquid separation, and then zircon with purity of >99% was selected under a binocular
138 lens. Zircon target making and transmission, reflection, and cathodoluminescence
139 (CL) images were completed with a JXA-8800R electron microprobe at the Tianjin
140 Institute of Geology and Mineral Resources (TIGMR). Zircon U–Pb analyses were
141 conducted by LA-MC-ICP-MS. The laser used was a NEWWAVE 193 nm FX and
142 the mass spectrometer used was Thermo Fisher's NEPTUNE (Geng et al., 2011). The
143 laser spot diameter was 35 m, and helium was used as the carrier gas of the
144 denudation material. The analysis process is described in Yuan et al. (2004) and Liu et
145 al. (2008). The software ICPMSDataCal (Liu et al., 2010) was used to process the
146 final test data offline. Common Pb was corrected by 208Pb following the procedure of
147 Andersen (2002). ISOPLOT 3.0 was used to plot U–Pb age harmonics and calculate
148 the average age weight (Ludwig, 2003).
149 Zircon Hf isotope analysis was conducted in the Isotope Laboratory of TIGMR,
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150 using a NEPTUNE (MC-ICPMS) system at the same oscillation band as but at
151 different location from the U–Pb dating analysis. The measured laser beam diameter
152 was 35 m and the laser pulse frequency was 8–10 Hz. For analysis conditions and
153 processes we refer to Geng et al. (2011). In the analysis process, the value of epsilon
154 Hf(t) is calculated on the basis of the zircon U–Pb age. The decay constant of 176Lu is
155 1.867 × 10−11 year−1 (Soderlund et al., 2004), the ratio of 176Hf/177Hf of chondrite is
156 0.282785, and the ratio of 176Lu/177Hf is 0.0336 (Bouvier et al., 2008). The calculation
157 of deficit mantle model age (TDM) refers to the current deficit mantle 176Hf/177Hf ratio
158 of 0.28325 and 176Lu/177Hf ratio of 0.0384 (Griffin et al., 2000). By assuming that the
159 parent magma of each zircon comes from the average continental crust, the crustal
160 model age (TC DM) of zircon Hf isotopes can be calculated by using the 176Lu/177Hf
161 ratio of 0.015 (Griffin et al., 2002).
162 3.2. Whole-rock geochemistry
163 The whole-rock geochemistry was analyzed at TIGMR. First, the weathering
164 crust was removed from fresh samples and then crushed by a crusher. The crushed
165 samples were ground into powder (>200 mesh) by a ball mill for analysis of major
166 and trace elements. The main elements were determined by X-ray fluorescence
167 spectrometry (XRF). FeO was determined by the volumetric method of hydrofluoric
168 acid–sulfuric acid solution and potassium dichromate titration. The analytical
169 accuracy was better than 2%. The trace elements were measured by ICP-MS, and the
170 analytical accuracy was better than 5%. The detailed analytical procedure followed
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171 that of Gao et al. (2003).
172 3.3. Whole-rock Sr–Nd isotopes
173 Sr–Nd isotope analyses were conducted at TIGMR using a Triton thermal
174 ionizer. The spectral analysis accuracy was better than 0.002%. Sample dissolution
175 was performed using acid digestion (HF + HClO4 + HNO3). Separation of Rb and Sr
176 was done through AG50W × 12 strongly acidic cation exchange resins. Nd was
177 separated and purified by HEHEHP resin (P507) technology. Isotope measurement of
178 the background was conducted within the error range. The results of international
179 standard sample BCR-2 were as follows: 143Nd/144Nd = 0.512630 ± 4 (2σ) and
180 87Sr/86Sr = 0.704985 ± 7 (2σ).
181 4. Results
182 4.1. Zircon U–Pb geochronology
183 The granitoid samples yielded adequate zircons for LA-ICPMS U–Pb dating.
184 The analytical results are listed in Table 1.
185 The zircon grains used for LA-ICP-MS U–Pb analyses of the monzogranite
186 (02TW19 and 02TW24) were mostly euhedral, transparent to translucent, and
187 colorless; they exhibited clear oscillatory zoning with smooth surfaces, were generally
188 120–170 μm in length, and had length/width ratios between 1:1 and 2.5:1. Most
189 zircon grains showed fine prismatic shape with abraded pyramids (Fig. 4). Samples
190 02TW19 and 02TW24 had uranium concentrations ranging from 320 to 1607 and
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191 from 429 to 1958 ppm, respectively, and the Th/U ratio was variable between 0.32
192 and 0.90 and between 0.39 and 0.58, respectively. Zircons of this study are
193 characteristic of magmatic origin and have magmatogenic oscillatory zones.
194 The zircon grains used for LA-ICP-MS U–Pb analyses of the granodiorite
195 (02TW31 and 02TW32) were also mostly euhedral, transparent to translucent, and
196 colorless; they exhibited clear oscillatory zoning with smooth surfaces, were generally
197 100–180 μm in length, and had length/width ratios between 1:1 and 2.5:1. Most
198 zircon grains show fine prismatic shape with abraded pyramids. Compared with
199 zircon grains of the monzogranites, some zircon grains of the granodiorite were
200 subcircular (Fig. 4). Samples 02TW31 and 02TW32 had uranium concentrations
201 ranging from 239 to 1428 ppm and from 267 to 842 ppm, respectively, and their Th/U
202 ratios were variable between 0.44 and 1.52 and between 0.44 and 1.05, respectively.
203 Zircons of this study are characteristic of magmatic origin and have magmatogenic
204 oscillatory zones.
205 Most zircon grain ages of the monzogranite (02TW19) plot on the concordia
206 curve uniformly and are considered to be concordant within error, except for
207 measuring point 19, which falls below the concordia curve in the U–Pb concordia
208 diagram, and its 206Pb/238U value is small, probably resulting from radiogenic Pb loss.
209 Analyses of the data table and concordia plots are reported at the 1σ level and
210 uncertainties in weighted mean ages are quoted at the 95% confidence level. The
211 weighted average 206Pb/238U age of the 23 zircon grains with a confidence of 95% is
212 270.1 ± 1.1 Ma (MSWD = 0.61, n = 23) (Fig. 5).
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213 The 206Pb/238U ages of the zircon grains in the monzogranite (02TW24) exhibit
214 ages mainly of 271–283 Ma. All ages plot on the concordia curve uniformly, and the
215 weighted average 206Pb/238U age of the 24 zircon grains with a confidence of 95% is
216 277.4 ± 1.2 Ma (MSWD = 0.85, n = 24) (Fig. 5).
217 Most zircon grain ages in the granodiorite (02TW31) plot on the concordia curve
218 uniformly. The 206Pb/238U ages of mainly 260–269 Ma are considered to be
219 concordant within error, except for measuring point 18, which falls below the
220 concordia curve in the U–Pb concordia diagram, probably as a result of radiogenic Pb
221 loss. The weighted average 206Pb/238U age of the 23 zircon grains with a confidence of
222 95% is 263.6 ± 1.2 Ma (MSWD = 0.64, n = 23) (Fig. 5).
223 The 206Pb/238U ages of the zircon grains in the granodiorite (02TW32) exhibit
224 ages mainly of 260–265 Ma. All ages plot on the concordia curve uniformly, and the
225 weighted average 206Pb/238U age of the 24 zircon grains with a confidence of 95% is
226 262.2 ± 1.1 Ma (MSWD = 0.31, n = 24) (Fig. 5).
227 In conclusion, zircon ages of 270.1 ± 1.1 and 277.4 ± 1.2 Ma in the late Early
228 Permian can be interpreted as representing the crystallization age of the monzogranite,
229 and zircon ages of 263.6 ± 1.2 and 262.2 ± 1.1 Ma in the late Middle Permian can be
230 interpreted as representing the crystallization age of the granodiorites.
231 4.2. Geochemistry
232 Major and trace element data for 12 representative samples of the monzogranites
233 and granodiorites are presented in Table 2.
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234 Based on the total alkali-silica diagram of Middlemost (1989) (Fig. 6a), these
235 samples plot in the field of granodiorite and granite. Based on the standard ore
236 diagram of Streckeisen (1979), these samples plot in the field of granodiorite and
237 monzogranite (Fig. 6b). These geochemical classification results are confirmed by
238 petrographic studies.
239 The monzogranite and granodiorite (host rock) samples belong to a low-Fe
240 calc-alkaline series (Fig. 6c). The characteristics of major elements can be
241 summarized as follows: (1) SiO2 contents is high (66.12%–73.94%), with
242 differentiation index ranging from 70.70 to 88.07. (2) The A/NK–A/CNK diagram
243 shows that monzogranites and granodiorites range from metaluminous to weakly
244 peraluminous with A/CNK ratios from 0.94 to 1.02 (Fig. 6d). (3) The monzogranites
245 and granodiorites have moderate ALK (Na2O+K2O) contents (6.42%–7.82%) and
246 Na2O contents (3.66%–4.33%). (4) The granodiorite samples exhibit medium-K
247 calc-alkaline properties, while the monzogranites exhibit high-K calc-alkaline
248 properties (Fig. 6e). (5) All samples plot within the magnesian granitoid fields (Fig.
249 6f), and the monzogranite and granodiorite plot within the calc-alkalic field (Fig. 6g)
250 in the classification diagrams of Frost et al. (2001).
251 In the chondrite-normalized rare earth element (REE) diagram (Fig. 7a), the
252 monzogranites and granodiorites have moderately fractionated REE patterns
253 ((La/Yb)N = 5.1–8.9), moderately fractionated light REEs ((La/Sm)N = 3.3–5.0), and
254 weakly fractionated heavy REEs ((Gd/Lu)N = 1.0–1.4). They have low total REE
255 contents (ΣREE = 83.6–129.0 ppm). The granodiorites have slight Eu anomalies
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256 (Eu/Eu* = 0.67–0.92), whereas the monzogranites of this pluton have weaker negative
257 Eu anomalies (Eu/Eu* = 0.44–0.68).
258 In the primitive-mantle-normalized spidergram (Fig. 7b), the monzogranites and
259 granodiorites are all enriched in Rb, Th, U, and light REE and depleted in high field
260 strength elements, such as Ta, Nb, P, and Ti. The monzogranites have low Sr contents
261 (134 × 10−6 to 367 × 10−6) but high Yb contents (1.83–2.31), while the granodiorites
262 contain higher Sr and lower Yb contents than the monzogranites.
263 4.3. Sr–Nd isotopes
264 Sr–Nd isotopic data of the eight granitoids samples are given in Table 3 and are
265 displayed in Fig. 8. All data and parameters are within the normal range and there are
266 no abnormal values. For example, 87Rb/86Sr is not high (<3), so there is no abnormally
267 low Isr value (<0.700), which indicates that the test results have geological
268 significance. In addition, the average fSm/Nd is between −0.6 and −0.2 (Fig. 8a),
269 indicating that the differentiation of the granitoids is not obvious. It can be concluded
270 that Sm–Nd isotopes in the rocks well record the characteristics of their protoliths,
271 which also shows that the model age TDM is effective (Jahn et al., 2000).
272 The four granodiorites samples have positive εNd(t) values (4.37–5.70) and
273 relatively low initial 87Sr/86Sr ratios (0.7021–0.7033), whereas the four monzogranites
274 have positive εNd(t) values (4.52–4.81) and relatively high initial 87Sr/86Sr ratios
275 (0.6995–0.7070). In the diagram of εNd(t) versus (87Sr/86Sr)i, all samples plot in the
276 first and second quadrants (Fig. 8b).
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277 4.4. Zircon Hf isotopes
278 Representative zircons from the paragneiss samples 02TW19.2 and 02TW32.2
279 were chosen for in situ MC-ICP-MS Hf isotope analysis (Table 4). They were taken
280 from the same zircons but different sites as a result of the large size of the
281 laser-ablation pits (Fig. 4). Sixteen zircon grains from the monzogranite (sample
282 02TW19.2) with a weighted mean 206Pb/238U age of 270.1 ± 1.1 Ma have similar Hf
283 isotopic compositions with 176Hf/177Hf ratios of 0.282855–0.283008 (Fig. 9a), εHf(t)
284 values of +8.2 to +14.1 (Fig. 9b), and Hf isotopic crustal model ages (TC DM) of
285 394–772 Ma. Zircon #10 (02TW19.2.10) with a 206Pb/238U age of ~267 Ma has a high
286 176Hf/177Hf ratio of 0.283110, a positive high εHf(t) value of 17.5, and young Hf
287 isotopic crustal model ages (TC DM) of 182 Ma. Sixteen zircon grains from the
288 granodiorite (sample 02TW32.2) with a weighted mean 206Pb/238U age of 262.2 ± 1.1
289 Ma were analyzed: They have variable Hf isotopic compositions, with 176Hf/177Hf
290 ratios of 0.282704–0.283004 (Fig. 9a), εHf(t) values of +3.0 to +13.7 (Fig. 9b), and TC
291 DM of 413–1097 Ma.
292 5. Discussion
293 5.1. Timing of Permian granitic magmatism in the northern Beishan orogen
294 Zircon grains in this study are euhedral and colorless, with typical magmatic
295 oscillatory zoning and high Th/U ratios of 0.32 and 1.11, indicating magmatic origin.
296 Therefore, these ages represent the emplacement ages of the Hazhu Permian
297 granitoids. The results of LA-ICP MS zircon U–Pb dating show that the
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298 monzogranites and granodiorites were crystallized at 262–277 Ma, thus constraining
299 their emplacement age as the Early–Middle Permian. Generally, these results combine
300 with other regional geological data acquired recently indicate that the Permian was an
301 important period of granitic magmatism in the northern Beishan orogen.
302 Numerous research findings have revealed that many Permian granitoids were
303 emplaced in a postorogenic or postcollisional tectonic setting from the eastern
304 Tianshan orogen to the Beishan orogen in NW China (Yuan et al., 2007; Chen et al.,
305 2011; Liu et al., 2012; Zhang et al., 2012; Li et al., 2013). Besides, the emplacement
306 age of the alkaline mafic and felsic magmatism is 280–240 Ma in this regional
307 extensional setting (Pirajno et al., 2010; Song et al., 2011). This age is basically
308 consistent with the zircon U–Pb age (262–277 Ma) of the monzogranites and
309 granodiorites in this study. Generally, research studies on Permian granitoids in the
310 study area have been relatively sparse compared with those on the east Tian orogen
311 and the southern Beishan orogen. Thus, the Permian magmatism, recognized from the
312 northern Beishan orogen in this study, provides further information on Permian
313 magmatism in the northern Beishan orogen and even the CAOB.
314 5.2. Granite types and origin
315 The degree of differentiation of monzogranites and granodiorites are,
316 respectively, medium (D.I. = 82.6–88.1) and low (D.I. = 70.7–79.3). All samples
317 generally plot in I-and S-type granite areas on the FeOT/MgO versus SiO2 diagram
318 (Fig. 6h); however, there are no S-type granite minerals such as muscovite, cordierite,
319 and garnet in the granitoids of this study. On the Ce versus SiO2 diagram, all samples
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320 plot in the I-type granite area. The experimental results show that, in quasi-aluminous
321 and weak peraluminous magma, the solubility of apatite is very low, and it is
322 inversely correlated with SiO2 during magmatic evolution, whereas, in strong
323 peraluminous magma, the solubility of apatite is higher, and the trend is opposite (Zhu
324 et al., 2009). These different behaviors of apatite in I-type and S-type granitoids can
325 be used to distinguish between I-type and S-type granitoids (Li et al., 2007). The data
326 in this study show that all samples exhibit quasi-aluminous characteristics (A/CNK <
327 1.1), and the content of P2O5 is low, decreasing with the increase of SiO2 content,
328 which is consistent with the evolution trend of I-type granite. Therefore, the granitoids
329 of this study exclude the possibility of S-type granites.
330 The zircon saturation temperature (Tzr) of granitoids in this study range from
331 745°C to 782°C (Table 5), which is obviously lower than that of A-type granite,
332 which is >800°C (Liu et al., 2003). Whalen et al. (1987) proposed that AKI
333 ((Na2O+K2O)/Al2O3, molecular number ratio) = 0.85 and ALK (Na2O+K2O) = 8.5%
334 should be the lower limit of A-type granite. The AKI and ALK values of monzonite
335 and granodiorite samples collected in this study do not reach the lower limit of A-type
336 granite, and they are less than the lower limit of AKI (AKI = 1) of alkaline granite.
337 Whalen et al. (1987) also found that A-type granite has the characteristics of low
338 Al and high Ga and Zr. If we take 10000 × Ga/Al = 2.6 as the lower limit value of
339 A-type granite, we find that the 10000 × Ga/Al value of granodiorite and monzonite
340 samples are lower than this value.
341 The contents of Zr, Nb, Ce, and Zr+Nb+Ce+Y are lower than the lower limit
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342 values of A-type granites (Zr = 250×10−6, Nb = 35×10−6, Ce = 148×10−6, and
343 Zr+Nb+Ce+Y = 350×10−6; Whalen, 1987), exhibiting the characteristics of I-type
344 granites (Fig. 6i).
345 5.3. Petrogenesis of the Permian granitoids
346 Geochemical characteristics are primarily controlled by source compositions,
347 physical conditions, partial melting, and fractional crystallization.
348 The Permian granitoids yield similar crystallization ages, uniform zircon Hf
349 isotope compositions, similar Sr–Nd isotope compositions, and coherent
350 major-element composition variations. Thus, the protoliths of the monzogranites and
351 granodiorites most likely share the same genetic origin. Negative correlations of
352 Fe2O3T, MgO, and CaO with respect to SiO2 suggest fractional crystallization of mafic
353 minerals, such as biotite and hornblende. Negative correlations of Fe2O3T, TiO2, and
354 P2O5 with respect to SiO2 suggest fractional crystallization of apatite and ilmenite.
355 K-feldspar phenocrysts formed in the early stage were melted into round spheres
356 by high-temperature mafic magma; afterward, some K-feldspar phenocrysts were
357 surrounded by plagioclase to form rapakivi texture (Fig. 3g). The MMEs exhibit
358 chilled contacts against the host rock. Ellipsoidal, rounded, and lenticular plastic flow
359 patterns show that the MMEs have morphological characteristics of quenched
360 inclusions, which can be distinguished from homologous inclusions and xenoliths,
361 indicating that local magma emplacement is liquid or semisolid. The MMEs in this
362 study are similar to those of the quenched enclaves, which are products of
363 crystallization basic magma with host magma in a plastic state at the same time
364 (Zhang et al., 2012; Shu et al., 2018). This finding provides evidence of the
365 interaction between ferromagnesian magma and felsic magma.
366 Permian granitoids in this study are characterized with positive zircon epsilon Hf
367 values of 3.0 to 14.1 and high 176Hf/177Hf ratios of 0.282855 to 0.283008, which
368 places them between chondrites and depleted-mantle evolution lines (Fig. 9). The
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369 zircon Hf isotopic composition of the granodiorites exhibits obvious heterogeneity
370 with the range of epsilon Hf varying to 10.7 epsilon units. The corresponding Hf
371 isotopic crustal model age (TC DM) is mainly concentrated from 1012 to 394 Ma,
372 which is from the Neoproterozoic to the Devonian. Nd model ages (TDM) are young
373 (0.52–0.79 Ga) for Permian granitoids in this study (Fig. 8c), being similar to
374 Phanerozoic granites in the Central Asia orogen (Kovalenko et al., 1996) and younger
375 than those intruded in microcontinents (Kovalenko et al., 1996; Hong et al., 2000). In
376 the diagram of εNd(t) versus 206Pb/238U age (Fig. 8d), all samples plot between
377 chondrite and depleted mantle, indicating that no Precambrian basement was involved
378 in the formation of granitoids in the study area.
379 By comparison, zircon grains from the Permian granite in the southern Beishan
380 orogen, with a weighted mean 206Pb/238U age of 285 ± 4 Ma, have variable εHf(t)
381 values from weakly negative to weakly positive (−2.7 to +3.2) and TC DM of 0.82–
382 1.04 Ga (Zhang et al., 2012). Moreover, zircon grains from the Silurian granite in the
383 study area, with a weighted mean 206Pb/238U age of 422 ± 2 Ma, have variable εHf(t)
384 values from negative to weakly positive (−5.6 to +3.6) and TC DM of 1.19–1.76 Ga
385 (unpublished). Overall, the Permian granitoids exhibit zircon 176Hf/177Hf and εHf(t)
386 values that are similar to those of the Carboniferous granitoids in this belt, but these
387 values are different from those of Permian and Triassic granitoids in the southern
388 Beishan orogen (Fig. 9). The Permian granitoids exhibit higher εHf(t) values than the
389 Silurian granite in the same area (Fig. 9b). They have positive εHf(t) values between
390 chondrite and primitive mantle, being as high as +14.1, and TC DM of 394–1097 Ma,
391 suggesting source rocks of the Permian granitoids with a characteristic of
392 juvenile crust from the Neoproterozoic to the Late Paleozoic.
393 A great deal of research has shown that the CAOB began to grow and evolve in
394 the Late Mesoproterozoic (Kröner et al., 2014) and is one of the most prominent areas
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395 for the growth and transformation of the Phanerozoic continental crust in the world
396 (Windley et al., 2007; Sun et al., 2008; Xiao et al., 2009, 2010; Wilhem et al., 2012;
397 Li et al., 2018; Li et al., 2019). During the multistage oceanic lithosphere subduction
398 and accretion from the Proterozoic to the Late Paleozoic, large-scale mantle-derived
399 material formed new crust by underplating. Like other parts of the CAOB, the
400 Beishan region underwent large-scale Phanerozoic crustal growth (Jiang and Nie,
401 2006; Mao et al., 2012). At the same time, the Neoproterozoic orogeny extensively
402 existed in the Beishan area, which formed the Neoproterozoic continental crust (Yu et
403 al., 2015; Zong et al., 2017). Besides, isotope studies in the Beishan area indicate
404 significant juvenile input during the Neoproterozoic to Late Paleozoic according to
405 the high epsilon Nd values, zircon epsilon Hf values, young Nd model age, and Hf
406 isotopic crustal model age. Therefore, the Permian granites in the Hazhu area may
407 have been formed by partial melting of the juvenile crust from the Neoproterozoic to
408 Late Carboniferous.
409 In this study, the crust and depleted mantle in the Beishan area are used as
410 mixing endmembers; mantle material involvement ratios during magma formation of
411 Hazhu Permian granodiorites and monzogranites are calculated as 92.0% to 95.3% by
412 simple binary mixing simulation (Table 3). It is further confirmed that the Permian
413 granitoids in the study area were formed by partial melting of juvenile crust
414 containing a numerous mantle-derived components. In the two-component mixing
415 model, the mantle material involvement ratios of the granidiorites (92.8%–95.3%,
416 with an average value of 94.1%) are higher than those of the monzogranites (93.1%–
417 93.7%, with an average value of 93.5%). Meanwhile, the zircon Hf isotopic
418 composition of the granodiorites exhibit obvious heterogeneity with the range of
419 epsilon Hf varying to 10.7 epsilon units, but the range of epsilon Hf of the
420 monzogranites just varies to 5.9 epsilon units. The εNd(t) values of the granidiorites
421 are higher than those of the monzogranites, indicating additional mantle components
422 and juvenile crust. It should be noted that the granidiorites are 10 Ma younger than
423 the monzogranites. Furthermore, the younger intrusion has basic and less evolved
424 composition than the older monzogranite intrusion. Initial 87Sr/86Sr ratios exhibit a
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425 decreasing trend with decreasing SiO2, also indicating additional mantle components
426 and juvenile crust. Although the composite granitoid body has a common source, the
427 variable degree of partial melting during different times means that the monzogranite
428 and granodiorite melts were formed by juvenile crusts of different periods from the
429 Neoproterozoic to the Late Paleozoic. The differences above between the
430 granodiorites and monzogranites demonstrate greater additions of basic components
431 as time progressed, suggesting that more mantle-derived components were added to
432 the magma chamber. Furthermore, the saturation temperature (Tzr) of granitoids in
433 this study was <800°C, suggesting that they emplaced in environments of crustal
434 thickening (Miller et al., 2003) and that during the Early–Middle Permian the tectonic
435 regime probably transformed from compression to extension. In the extensional
436 environment, more and more juvenile lower crust melted and asthenospheric
437 upwelling occurred, which led to the younger intrusion becoming more basic.
438 5.4. Tectonic settings of the Permian granitoids
439 The Permian intrusive rock assemblages are monzogranite, granodiorite, and
440 alkali feldspar granite in the study area. Large-scale crystal caves are developed in the
441 Permian granitoids, indicating an extensional environment. The emplacement age of
442 alkaline mafic felsic magmatism in the regional extensional environment is 280–240
443 Ma (Pirajno et al., 2010; Song et al., 2011; Ma et al., 2016; Zhang et al., 2015; Zhang
444 et al., 2015; Xue et al., 2016), which is basically consistent with the zircon U–Pb age
445 of monzonite and granodiorite (262–277 Ma). Moreover, the Early–Middle Permian
446 olivine gabbro and gabbro diorite are newly defined in the northern Dahongshan area,
447 northwest of the study area. Their geochemical characteristics reflect the
448 characteristics of mantle-derived magma without obvious contamination of crustal
449 materials. This indicates that they formed in the stage of oceanic lithospheric
450 delamination after arc–continent collision. Based on the above facts, it can be
451 concluded that the Permian granitoids formed in the postcollision stage may be
452 closely related to crust–mantle detachment and lithospheric thinning. Although the
453 strong depletion of Nb, Ta, Zr, P, and Ti in the studied granitoids is a typical feature
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454 of subduction-related magmatic rocks, the content of high field strength elements in
455 typical crustal melts is low. This indicates that the depletion of high field strength
456 elements such as Nb, Ta, and Ti inherited the characteristics of source rocks and
457 cannot be used as a sign of subduction-related magmatic rocks.
458 Regionally, the Paleo-Asian Ocean subducted southward during the Early
459 Carboniferous, forming a limited oceanic basin of the Hongshishan–Baiheshan with
460 back-arc cracking origin (Xie et al., 2009; Wang at al., 2014; Li et al., 2018). The Late
461 Carboniferous magmatic arc age on the southern side of the Hongshishan–Baiheshan
462 ophiolite belt is 320 to 300 Ma and its geochemical characteristics exhibit the polarity
463 of the oceanic crust subducting southward. With the southward subduction of the
464 Hongshishan Ocean, a large number of intermediate-acid calc-alkaline magmatic
465 rocks formed in the study area in the Late Carboniferous (Li et al., 2018; Ren et al.,
466 2019); meanwhile, the Paleo-Asian Ocean continued to subduct southward in the Late
467 Carboniferous, forming the Queershan inherited island arc.
468 The Middle–Upper Permian Shuangbaotang Formation strata overlay the
469 Carboniferous Baishan Formation at an unconformity angle in the Shenluotan area.
470 The bottom conglomerates there symbolize the discontinuity of sedimentation at the
471 bottom of the Shuangbaotang Formation strata. The regional arc magmatic events all
472 ended before the Early–Middle Permian, as represented by the sedimentary events of
473 the Shuangbaotang Formation. The isotopic ages of regional alkaline felsic mafic
474 magmatism are 280–240 Ma, which is consistent with the postcollision granitoids
475 under the Permian extensional system in this study. It is presumed that the regional
476 arc–continent collision occurred in the Early Permian, and then the lithospheric
477 extension and thinning caused by oceanic lithospheric delamination resulted in
478 melting of different-period juvenile crusts from the Neoproterozoic to the Late
479 Paleozoic, forming the monzogranites (Fig. 10). As time progressed, more and more
480 juvenile lower crust melted and asthenospheric upwelling occurred, which led to the
481 younger intrusion becoming more basic and to the formation of the granodiorites.
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482 6. Conclusions
483 (1) Zircon U–Pb dating revealed that Early–Middle Permian granitic magmatism
484 occurred at 277–262 Ma in the northern Beishan orogen, NW China. The granitoids
485 exhibit calc-alkaline and high-K calc-alkaline series and are metaluminous to weakly
486 peraluminous I-type.
487 (2) The monzogranites and granodiorites are enriched in large-ion lithophile
488 elements and light REEs and evolved Sr–Nd isotopic compositions, suggesting a
489 juvenile crustal origin. They also exhibit positive εHf(t) values of 3.0 to 14.1 and
490 single-stage Hf model ages of 394 to 797 Ma. Therefore, their source contains
491 juvenile crust from the Neoproterozoic to Late Paleozoic that had positive εHf(t)
492 values at the Early–Middle Permian time.
493 (3) Petrological characteristics and geochemical and isotopic tracing suggest that
494 these granitoids derived from common sources, being melting of Neoproterozoic to
495 Late Paleozoic juvenile crusts. Moreover, the younger intrusions (granidiorites) are
496 more basic, probably the result of more juvenile lower crust being melted along with
497 asthenospheric upwelling, which led to the addition of more basic components.
498 (4) These granitoids formed in a postcollisional setting. The tectonic regime
499 transformed from an arc-related compressional setting to postcollisional extension,
500 probably caused by lithospheric extension and thinning in response to oceanic
501 lithospheric delamination.
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502 Acknowledgments
503 This work was funded by the Geological Survey Project of China (Grant Nos.
504 DD20190371 and DD20190038) and the National Science Foundation of China
505 (Grant No. 41872068).
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829 Zhang, W., Pease, V., Wu, T., Zheng, R.G., Feng, J., He, Y.K., Luo, H.L., Xu, C.,
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A list of figure captions Fig. 1. Simplified tectonic location map for the Beishan orogeny (modified after Yang et al., 2012;
Li et al., 2013)
Fig. 2. Geological sketch map of Hazhu area in Ejina banner
Fig. 3. Field potos and photomicrographs of the granitoids in Hazhu area
Fig. 4. CL image and dating of zircons for the monzogranite and granodiorite(yellow circle
represent U-Pb measure point and blue circle represent Hf isotope measure point)
Fig. 5. Zircon LA-MC-ICP-MS U-Pb concordia diagram of the monzogranite and granodiorite
Fig. 6. Major element diagrams
Fig. 7. (a) Chondrite-normalized rare earth element patterns and (b) primitive mantle-normalized
trace element spider diagrams.
Fig. 8 . (a) fSm/Nd vs. TDM diagram for the granitoids, (b) εNd(t) vs. (87Sr/86Sr)i diagram,
(c) εNd(t) vs. TDM diagram, (d) εNd(t) vs. intrusive U–Pb Age diagram
Fig. 9 . (a) 176Hf/177Hf vs. intrusive U–Pb age diagram and (b) εHf(t) vs. intrusive U–Pb age
diagram
Fig. 10. Schematic diagram showing the petrogenetic model for the Permian granitoids in northern
Beishan orogen
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C A O B
Siberia
Craton
Eas
tE
uope
anC
rato
n
a
Tianshan solonker
NorthChinaTarim
TETHYSIDES
Fig.1b
Queershan arc
Baiyushan-Huaniushan arc
Aqishan-Zhangfangshan rift zone
Heiyingshan arc Gongpoquan arcXingxingxia-Hanshan Block
National border Fault
b
Dunhuang Blcok
Dunhuang Blcok
NiujuanziShibanjin
Heiyingshan
Aqishan
Hanshan
Xichangjin
0 40 80 120 160kmMongolia
40°
40°
41°
42°
42°
00′
40′
20′
00′
40′
93° 94° 95° 96° 97° 98° 99° 100°
Hongliuyuan
Hongliuhe
Huaniushan
Fig.2
N
Fig. 1. Simplified tectonic location map for the Beishan orogeny (modified after Yang et al., 2012; Li et al., 2013)
Beishan Rock Group
Carboniferous granite
Devonian
Permian granodiorite
Carboniferous
Permian monzogranite
Carboniferous andersite
Cretaceous Quaternary sample location
Carboniferous rhyolite
0 1 2 km
N
42°15′
98°30′
42°00′
99°00′
42°00′
98°30′
Fig. 2. Geological sketch map of Hazhu area in Ejina banner
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Draft g
200μm
1i
Qtz
Hbl
Bt
Pl
200μm
h
QtzPl
Hbl
Bt
Kfs
Pl
Hbl
porphyritic granodiorite
porphyritic monzogranite
b
mafic enclave
porphyritic monzogranite
e
plagioclase phanerocryst
d
plagioclase phanerocryst
a
folds in country rock
f
plagioclase phanerocryst
amphibole phanerocryst
rapakivi-like texture
c
Fig. 3. Field potos and photomicrographs of the granitoids in Hazhu areaa Folds in country rock; b Intrusion relationship; c MME in monzogranite; d – Plageioclase phanerocryst in monzogranite; e
Plageioclase phanerocryst in granodiorite; f Plageioclase and amphibole phanerocryst in granodiorite and MME; g Rapakivi-like texture; h Photomicrographs of monzogranite; i Photomicrographs of granodiorite. Mineral abbreviation: Qtz, quartz; Pl,
plagioclase; Bt, biotite; Hbl, hornblende; Kfs, K-feldspar.
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275±3 275±3278±3
278±3277±3
277±3
278±3
277±3277±3
279±3
279±3279±3
276±3
278±3242322
1916
1413
121098631
271±3
270±3
271±3
270±3
269±3271±3
269±3266±3
271±3
21
4
36
4
7
596
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148 1711
271±3
2113
269±3
20
14
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16
265±3 264±3262±3
262±3
262±3
263±3 265±3
264±3263±4
263±3
264±3
265±3 263±3
264±3
1 3 45 6 7 10
13 14 15
17 2223 24
261±3
261±3 260±3261±3Ma 265±3
262±3264±3
261±3
263±3
263±3262±3
263±3
263±3 261±3
31 4
2 7 3 8410
5 12 613 7
148
159
1610 18 12 2214
23 1524 16
275±3
02TW19
02TW24
02TW31
02TW32
100μm
Fig. 4. CL image and dating of zircons for the monzogranite and granodiorite(yellow circle represent U-Pb measure point and blue circle represent Hf isotope measure point)
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254
258
262
266
270
274
278
0.0395
0.0405
0.0415
0.0425
0.0435
0.0445
0.25 0.27 0.29 0.31 0.33 0.35207
Pb/235
U
254258
262
266
270
274
250
254
258
262
266
270
274
0.0395
0.0405
0.0415
0.0425
0.0435
0.26 0.28 0.30 0.32
254
258
262
266
270
258
262
266
270
274
278
282
286
0.0405
0.0415
0.0425
0.0435
0.0445
0.0455
0.28 0.29 0.30 0.31 0.32 0.33
20
6 Pb
/23
8 U
260
268
276
284
(a)02TW19
270.1±1.1MaMSWD=0.61,n=23
260
264
268
272
276
280
284
288
292
296
0.041
0.042
0.043
0.044
0.045
0.046
0.047
0.28 0.29 0.30 0.31 0.32 0.33 0.34
264
272
280
288
(b)02TW24
277.4±1.2MaMSWD=0.85,n=24
(c)02TW31 263.6±1.2MaMSWD=0.64,n=23
20
6 Pb
/23
8 U
20
6 Pb
/23
8 U
(d)02TW32
262.2±1.1MaMSWD=0.31,n=24
20
6 Pb
/23
8 U
207Pb/
235U
Fig. 5. Zircon LA-MC-ICP-MS U-Pb concordia diagram of the monzogranite and granodiorite
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( )
0
1
2
3
4
5
6
7
45 50 55 60 65 70 75 80
TF
eO
/Mg
O
SiO2
strong CA series
CA
LF-CA
TH
0
1
2
3
0.5 0.7 0.9 1.1 1.3 1.5 1.7 1.9
A/N
K
A/CNK
CCG
CAG
IAG
RAG
POG
I-Stype( )d
Peraluminous
Peralkaline
Metaluminous
0.4
0.5
0.6
0.7
0.8
0.9
1.0
1.1
50 55 60 65 70 75 80
TT
FeO
/(F
eO+
Mg
O)
SiO2
Caledonian post- collisiona plutons (Frost et al.,2001)
( )f
Ferroan
Magnesian
-6
-4
-2
0
2
4
6
8
10
12
50 55 60 65 70 75 80
Na
O+
KO
22
-CaO
SiO2
(g)
Caledonian post- collisiona plutons (Frost et al.,2001)
alkalic
alkali-calcic
calc-alkalic
calcic
0
1
2
3
4
5
6
7
40 50 60 70 80K
O2
SiO2
Low-K
Calc-alkaline
High-K
Shoshonitic
(e)
5
15
25
35
45
0 10 20 30 40 50 60 70 80
Q'
ANOR
(b)
monzogranite
granodiorite
0
3
6
9
12
15
18
30 40 50 60 70 80 90
Na
O+
KO
22
SiO2
Ir
(a)
granite
granodiorite
SiO2
0.1
1
10
100
65 70 75 80
TF
eO
/Mg
O A
I&S
(h)
Zr+Nb+Ce+Y10 100 1000 10000
1
10
100
(Na
O+
KO
)/C
aO2
2
(i)
A
FG
OGT
cmonzogranitegranodiorite
Fig. 6. Major element diagrams. (a) Total alkalis vs. SiO2 (TAS) diagram (after Middlemost, 1989), (b)Q’ vs. ANOR standard ore diagram (modified after Streckeisen, 1979), (c) total FeO /MgO vs. SiO2 (after
Deng et al., 2010), (d) A/NK vs. A/CNK diagram (after Maniar and Piccoli, 1989), (e)K2O vs. SiO2 diagram (after Peccerillo and Taylor, 1976), (f) total FeO/(total FeO + MgO) vs. SiO2
diagram (after Frost et al., 2001), (g) Na2O + K2O–CaO vs. SiO2 diagram (after Frost et al., 2001), (h) total FeO/MgO vs. SiO2 diagram, (i) (Na2O + K2O)/CaO vs. (Zr + Nb + Ce + Y) diagram (Whalen et al., 1987).
Total FeO (FeOT) = FeO + 0.9 Fe2O3, A/CNK = mol Al2O3/(Na2O + K2O + CaO), A/NK = mol Al2O3/(Na2O + K2O), FG: fractionated granites; OGT: unfractionated M-, I- and S-type granites
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0.1
1
10
100
1000
Ro
ck/C
ho
nd
rite
0.1
1
10
100
1000
Ro
ck/P
rim
itiv
e M
antl
emonzogranitegranodiorite
(a) (b)
La Ce Pr Nd Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Rb BaTh U Nb Ta K La Ce Sr P Nd Zr Hf SmEu Ti Tb Y Yb Lu
Fig. 7. (a) Chondrite-normalized rare earth element patterns and (b) primitive mantle-normalized trace element spider diagrams.The values of chondrite and primitive mantle are from Sun and Mcdonough (1989).
-0.8
-0.6
-0.4
-0.2
0.0
0.2
0.0 0.2 0.4 0.6 0.8
f Sm
/Nd
T (Ga)DM
(a)
(87Sr/86Sr) I
0.690 0.700 0.710 0.720 0.730 0.740
ε Nd
15
10
5
0
-5
-10
-15
-20
(b)
Eastern Tian shan andSouthern Beishan intrusions
East Tianpost orogenic granites
mantle array
granodiorites
monzogranitesEMⅠ
EMⅡ
-20
-15
-10
-5
0
5
10
15
0.0 0.1 0.2 0.3 0.4 0.5
Age (Ga)
ε Nd
-20
-15
-10
-5
0
5
10
0.0 0.5 1.0 1.5 2.0 2.5 3.0
ε Nd
T (Ga)DM
Hercyniangranites(France)
Himalayagranite
CHUR
Archaean Crust
Early-Middle Proterozoic Crust
CHUR
Depleted Mantle
c( ) (d)
granodiorite
monzogranite
Central Asia granitesmicrocontinents
Data: Kovalenko et al.(1996)
granodiorite
monzogranite
Fig. 8 . (a) fSm/Nd vs. TDM diagram for the granitoids, (b) εNd(t) vs. (87Sr/86Sr)i diagram, (c) εNd(t) vs. TDM diagram, (d) εNd(t) vs. intrusive U–Pb Age diagram. Fields dapted from Naderi
et al. (2018), and reference compositions dapted from Wang et al. (2008)
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-20
-15
-10
-5
0
5
10
15
20
200 250 300 350 400 450 500
ε(t
)H
f
Age
Depleted mantle
CHUR
(b)
Triassicgranitoids
Pemian granitoids in southern Beishan
Carboniferous-Pemian granitoids in northern Beishan
Silurian granitoidsin northern Beishan
0.2820
0.2825
0.2830
0.2835
200 250 300 350 400 450 500
17
61
77
Hf/
Hf
Age
Depleted mantle
CHUR
Lower crust
(a)
Silurian granitoidsin northern Beishan
Carboniferous-Pemian granitoids in northern Beishan
granodiorite
monzogranite
Fig. 9 . (a) 176Hf/177Hf vs. intrusive U–Pb age diagram and (b) εHf(t) vs. intrusive U–Pb age diagram. Data for Siluriangranitoids and Triassic granitoids in the centralmassif and Permian granitoids in the southernmassif are from Li et al. (2009, 2011,
2012), Mao et al. (2009) and Zhang et al. (2012).
Lithosp
heric
man
tle
Lithospheric mantle
breakoff slab
Baiheshan accretio
nary complex
Baishan arc
Continen
tal c
rust
junenile crustal MASH zone
Carboniferousgranitoids Permian granitoids
Extension
Upwelling asthenosphere
Continental crust
CarboniferousBaishan Formation
Permian Shuangbaotang Formation
unconformity
N S
W
E
Permian (277-262Ma)
Oceanic crust Asth
enosp
here m
antle
Asthenosphere mantle
Fig. 10. Schematic diagram showing the petrogenetic model for the Permian granitoids in northern Beishan orogen
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Table 1
Table 1 Zircon LA-MC-ICP-MS U-Pb dating result of the monzogranites (02TW19.2 and 02TW24.1) and granodiorites (02TW31.1 and 02TW32.2)Spot No. 含量(×10-6) Isotopic ratios Apparent age (Ma)
02TW19.2 Pb U 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ 208Pb/232Th 1σ 232Th/238U 1σ 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ
1 36 839 0.0428 0.0004 0.3099 0.0044 0.0525 0.0006 0.0144 0.0001 0.3476 0.0006 270 3 274 4 308 28
2 51 1150 0.0429 0.0004 0.3088 0.0053 0.0522 0.0007 0.0158 0.0002 0.3849 0.0010 271 3 273 5 294 31
3 30 565 0.0438 0.0004 0.3111 0.0047 0.0516 0.0007 0.0305 0.0001 0.5041 0.0013 276 3 275 4 266 30
4 46 1043 0.0428 0.0004 0.3068 0.0044 0.0520 0.0006 0.0156 0.0001 0.3939 0.0005 270 3 272 4 286 27
5 31 656 0.0425 0.0004 0.3074 0.0043 0.0524 0.0007 0.0208 0.0001 0.4426 0.0006 268 3 272 4 304 28
6 50 1132 0.0429 0.0005 0.3091 0.0043 0.0523 0.0006 0.0151 0.0001 0.3974 0.0009 271 3 273 4 296 27
7 51 1173 0.0427 0.0004 0.3088 0.0041 0.0524 0.0006 0.0156 0.0000 0.3219 0.0013 270 3 273 4 303 27
8 28 627 0.0428 0.0004 0.3066 0.0044 0.0519 0.0007 0.0160 0.0001 0.3818 0.0011 270 3 272 4 283 31
9 43 937 0.0426 0.0004 0.3070 0.0046 0.0523 0.0007 0.0160 0.0001 0.4803 0.0006 269 3 272 4 298 29
10 48 1065 0.0429 0.0004 0.3074 0.0041 0.0520 0.0006 0.0141 0.0000 0.4647 0.0010 271 3 272 4 285 27
11 27 613 0.0427 0.0004 0.3084 0.0046 0.0524 0.0007 0.0142 0.0001 0.4432 0.0032 270 3 273 4 302 30
12 30 669 0.0429 0.0004 0.3079 0.0060 0.0521 0.0009 0.0134 0.0002 0.4666 0.0008 271 3 273 5 288 41
13 27 613 0.0429 0.0004 0.3084 0.0044 0.0522 0.0007 0.0126 0.0000 0.4713 0.0015 270 3 273 4 294 30
14 40 826 0.0436 0.0004 0.3125 0.0050 0.0520 0.0008 0.0114 0.0000 0.9016 0.0010 275 3 276 4 284 34
15 14 320 0.0427 0.0004 0.3035 0.0079 0.0516 0.0014 0.0094 0.0001 0.7555 0.0090 269 3 269 7 268 63
16 30 699 0.0423 0.0004 0.3038 0.0050 0.0521 0.0008 0.0118 0.0001 0.4785 0.0015 267 3 269 4 288 35
17 23 527 0.0425 0.0004 0.3051 0.0062 0.0520 0.0010 0.0104 0.0001 0.5838 0.0012 269 3 270 5 287 43
18 26 607 0.0427 0.0004 0.3051 0.0071 0.0518 0.0011 0.0133 0.0002 0.4081 0.0010 269 3 270 6 278 49
19 32 805 0.0372 0.0004 0.3725 0.0052 0.0726 0.0009 0.0141 0.0001 0.4049 0.0008 235 2 322 5 1004 25
20 28 643 0.0427 0.0004 0.3088 0.0048 0.0525 0.0007 0.0126 0.0001 0.4182 0.0011 269 3 273 4 306 32
21 25 566 0.0429 0.0004 0.3053 0.0045 0.0516 0.0007 0.0124 0.0001 0.3971 0.0003 271 3 271 4 267 31
22 30 695 0.0429 0.0004 0.3042 0.0051 0.0515 0.0008 0.0123 0.0001 0.4183 0.0006 270 3 270 5 263 36
23 22 507 0.0421 0.0004 0.3039 0.0069 0.0523 0.0011 0.0136 0.0001 0.4228 0.0003 266 3 269 6 300 49
24 77 1607 0.0429 0.0004 0.3077 0.0042 0.0521 0.0006 0.0136 0.0001 0.7649 0.0030 271 3 272 4 288 27
Spot No. 含量(×10-6) Isotopic ratios Apparent age (Ma)
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02TW24.1 Pb U 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ 208Pb/232Th 1σ 232Th/238U 1σ 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ
1 45 964 0.0436 0.0004 0.3134 0.0048 0.0521 0.0007 0.0172 0.0001 0.4716 0.0002 275 3 277 4 290 29
2 28 590 0.0443 0.0004 0.3178 0.0055 0.0520 0.0008 0.0160 0.0001 0.4637 0.0015 280 3 280 5 286 37
3 29 629 0.0437 0.0004 0.3129 0.0046 0.0520 0.0007 0.0156 0.0000 0.4769 0.0015 275 3 276 4 285 30
4 40 848 0.0434 0.0004 0.3084 0.0043 0.0515 0.0006 0.0160 0.0000 0.5315 0.0009 274 3 273 4 263 29
5 20 429 0.0429 0.0004 0.3101 0.0095 0.0524 0.0015 0.0169 0.0002 0.4675 0.0005 271 3 274 8 304 67
6 35 751 0.0441 0.0004 0.3141 0.0044 0.0517 0.0006 0.0168 0.0000 0.4563 0.0020 278 3 277 4 273 29
7 57 1175 0.0434 0.0004 0.3094 0.0041 0.0517 0.0006 0.0182 0.0001 0.5764 0.0019 274 3 274 4 272 27
8 93 1958 0.0440 0.0004 0.3119 0.0040 0.0514 0.0006 0.0168 0.0000 0.5005 0.0013 278 3 276 4 258 26
9 32 684 0.0439 0.0005 0.3164 0.0047 0.0523 0.0007 0.0178 0.0001 0.4435 0.0016 277 3 279 4 298 29
10 46 953 0.0439 0.0004 0.3148 0.0043 0.0520 0.0006 0.0173 0.0000 0.5473 0.0012 277 3 278 4 284 28
11 34 734 0.0436 0.0004 0.3119 0.0070 0.0519 0.0010 0.0192 0.0003 0.4173 0.0022 275 3 276 6 279 44
12 37 787 0.0441 0.0005 0.3158 0.0046 0.0519 0.0007 0.0172 0.0001 0.4669 0.0023 278 3 279 4 282 29
13 33 698 0.0439 0.0005 0.3126 0.0060 0.0516 0.0008 0.0183 0.0003 0.4248 0.0021 277 3 276 5 267 37
14 28 616 0.0439 0.0005 0.3135 0.0047 0.0518 0.0007 0.0167 0.0001 0.4013 0.0020 277 3 277 4 278 30
15 28 606 0.0446 0.0005 0.3173 0.0054 0.0516 0.0008 0.0166 0.0001 0.4441 0.0020 281 3 280 5 269 35
16 39 843 0.0442 0.0005 0.3167 0.0044 0.0519 0.0006 0.0163 0.0002 0.3852 0.0028 279 3 279 4 283 28
17 30 651 0.0443 0.0005 0.3187 0.0048 0.0521 0.0007 0.0178 0.0002 0.4172 0.0023 280 3 281 4 291 30
18 33 697 0.0446 0.0005 0.3207 0.0051 0.0522 0.0008 0.0151 0.0001 0.4839 0.0011 281 3 282 4 292 34
19 42 905 0.0442 0.0005 0.3128 0.0044 0.0514 0.0006 0.0140 0.0001 0.4860 0.0038 279 3 276 4 257 28
20 36 776 0.0443 0.0005 0.3167 0.0050 0.0518 0.0007 0.0146 0.0002 0.4479 0.0037 280 3 279 4 277 30
21 32 693 0.0449 0.0005 0.3212 0.0050 0.0519 0.0007 0.0142 0.0002 0.3977 0.0031 283 3 283 4 279 30
22 28 610 0.0442 0.0005 0.3206 0.0050 0.0526 0.0007 0.0132 0.0002 0.4562 0.0027 279 3 282 4 313 31
23 34 761 0.0438 0.0005 0.3179 0.0046 0.0527 0.0007 0.0132 0.0001 0.4129 0.0029 276 3 280 4 315 29
24 29 635 0.0441 0.0005 0.3156 0.0052 0.0519 0.0008 0.0134 0.0001 0.4435 0.0015 278 3 278 5 280 35
Spot No. 含量(×10-6) Isotopic ratios Apparent age (Ma)
02TW31.1 Pb U 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ 208Pb/232Th 1σ 232Th/238U 1σ 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ
1 11 239 0.0420 0.0005 0.2978 0.0166 0.0515 0.0029 0.0138 0.0002 0.4826 0.0023 265 3 265 15 262 128
2 18 408 0.0412 0.0005 0.2948 0.0064 0.0519 0.0011 0.0128 0.0001 0.6818 0.0005 260 3 262 6 280 49
3 14 312 0.0418 0.0005 0.2978 0.0108 0.0516 0.0019 0.0137 0.0001 0.4468 0.0011 264 3 265 10 268 83
4 30 675 0.0415 0.0004 0.2969 0.0058 0.0519 0.0010 0.0129 0.0001 0.6395 0.0063 262 3 264 5 283 44
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5 23 532 0.0415 0.0004 0.2952 0.0052 0.0516 0.0008 0.0128 0.0001 0.4905 0.0010 262 3 263 5 268 38
6 21 464 0.0415 0.0005 0.3010 0.0051 0.0526 0.0008 0.0111 0.0001 0.6609 0.0021 262 3 267 4 312 35
7 26 588 0.0417 0.0005 0.2984 0.0052 0.0519 0.0008 0.0135 0.0001 0.4806 0.0022 263 3 265 5 283 34
8 20 459 0.0415 0.0005 0.2966 0.0076 0.0518 0.0011 0.0141 0.0002 0.5004 0.0014 262 3 264 7 278 50
9 23 527 0.0421 0.0005 0.2996 0.0062 0.0517 0.0010 0.0128 0.0001 0.4358 0.0012 266 3 266 6 270 43
10 42 935 0.0419 0.0005 0.2985 0.0046 0.0516 0.0007 0.0134 0.0001 0.5587 0.0008 265 3 265 4 268 31
11 18 415 0.0412 0.0004 0.2925 0.0053 0.0515 0.0009 0.0123 0.0001 0.6425 0.0074 260 3 260 5 265 39
12 27 599 0.0423 0.0005 0.3036 0.0050 0.0520 0.0007 0.0130 0.0001 0.6031 0.0023 267 3 269 4 288 33
13 28 642 0.0418 0.0005 0.2975 0.0047 0.0516 0.0007 0.0133 0.0001 0.4959 0.0012 264 3 264 4 269 31
14 37 745 0.0416 0.0005 0.2984 0.0046 0.0520 0.0007 0.0125 0.0000 1.0352 0.0042 263 3 265 4 286 31
15 23 514 0.0416 0.0005 0.2984 0.0050 0.0521 0.0008 0.0129 0.0001 0.6098 0.0027 263 3 265 4 289 34
16 27 592 0.0414 0.0004 0.2967 0.0047 0.0520 0.0007 0.0125 0.0000 0.7074 0.0047 262 3 264 4 284 33
17 31 706 0.0418 0.0004 0.2960 0.0044 0.0514 0.0007 0.0130 0.0000 0.5737 0.0016 264 3 263 4 258 31
18 108 1428 0.0452 0.0005 1.6798 0.0278 0.2694 0.0039 0.0197 0.0002 1.5219 0.0220 285 3 1001 17 3303 23
19 19 388 0.0426 0.0004 0.3008 0.0067 0.0512 0.0011 0.0104 0.0000 1.1140 0.0051 269 3 267 6 250 49
20 27 536 0.0425 0.0005 0.3016 0.0089 0.0515 0.0014 0.0221 0.0005 0.6176 0.0039 268 3 268 8 263 62
21 31 713 0.0414 0.0005 0.2953 0.0044 0.0517 0.0007 0.0098 0.0002 0.6149 0.0089 262 3 263 4 272 32
22 24 529 0.0419 0.0005 0.2984 0.0050 0.0516 0.0008 0.0113 0.0001 0.7657 0.0025 265 3 265 4 268 35
23 18 416 0.0417 0.0004 0.2965 0.0054 0.0516 0.0009 0.0118 0.0001 0.5575 0.0018 263 3 264 5 267 39
24 20 466 0.0418 0.0004 0.2975 0.0051 0.0516 0.0008 0.0119 0.0001 0.5079 0.0017 264 3 264 5 268 37
Spot No. 含量(×10-6) Isotopic ratios Apparent age (Ma)
02TW32.2 Pb U 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ 208Pb/232Th 1σ 232Th/238U 1σ 206Pb/238U 1σ 207Pb/235U 1σ 207Pb/206Pb 1σ
1 24 500 0.0413 0.0005 0.2957 0.0056 0.0519 0.0009 0.0123 0.0001 0.8938 0.0118 261 3 263 5 280 39
2 21 461 0.0414 0.0004 0.2925 0.0063 0.0512 0.0010 0.0126 0.0001 0.8040 0.0037 261 3 261 6 252 45
3 14 329 0.0413 0.0004 0.2955 0.0065 0.0519 0.0011 0.0122 0.0001 0.4746 0.0021 261 3 263 6 282 48
4 23 475 0.0413 0.0004 0.2949 0.0051 0.0518 0.0008 0.0124 0.0001 0.9015 0.0060 261 3 262 5 276 36
5 19 405 0.0414 0.0004 0.2984 0.0062 0.0523 0.0010 0.0124 0.0001 0.8530 0.0137 261 3 265 6 300 45
6 19 421 0.0415 0.0004 0.2972 0.0061 0.0519 0.0010 0.0122 0.0001 0.6998 0.0043 262 3 264 5 282 44
7 27 596 0.0412 0.0004 0.2951 0.0054 0.0520 0.0009 0.0124 0.0000 0.6589 0.0016 260 3 263 5 284 40
8 12 267 0.0413 0.0004 0.2938 0.0083 0.0516 0.0014 0.0122 0.0001 0.6957 0.0037 261 3 262 7 269 64
9 14 317 0.0417 0.0005 0.2962 0.0072 0.0516 0.0012 0.0124 0.0001 0.6513 0.0027 263 3 263 6 266 54
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10 14 309 0.0420 0.0004 0.2991 0.0073 0.0517 0.0012 0.0123 0.0001 0.6782 0.0045 265 3 266 6 272 53
11 15 322 0.0420 0.0005 0.2971 0.0087 0.0513 0.0014 0.0126 0.0001 0.6412 0.0012 265 3 264 8 255 64
12 23 524 0.0415 0.0004 0.2948 0.0052 0.0516 0.0008 0.0125 0.0001 0.5283 0.0018 262 3 262 5 267 38
13 16 346 0.0418 0.0004 0.2995 0.0108 0.0520 0.0018 0.0114 0.0001 0.7738 0.0013 264 3 266 10 286 80
14 13 303 0.0414 0.0004 0.2908 0.0065 0.0510 0.0011 0.0125 0.0001 0.5510 0.0021 261 3 259 6 239 49
15 25 556 0.0417 0.0004 0.2970 0.0050 0.0517 0.0008 0.0127 0.0001 0.6414 0.0030 263 3 264 4 273 35
16 14 315 0.0416 0.0004 0.2993 0.0070 0.0521 0.0012 0.0125 0.0001 0.4988 0.0007 263 3 266 6 291 51
17 28 555 0.0420 0.0004 0.3001 0.0050 0.0518 0.0008 0.0218 0.0001 0.6253 0.0044 265 3 267 4 278 35
18 51 842 0.0415 0.0004 0.2979 0.0046 0.0521 0.0007 0.0254 0.0001 1.0516 0.0065 262 3 265 4 289 32
19 26 477 0.0418 0.0005 0.2968 0.0053 0.0515 0.0008 0.0295 0.0003 0.6059 0.0013 264 3 264 5 264 38
20 24 447 0.0414 0.0004 0.2937 0.0056 0.0514 0.0009 0.0361 0.0002 0.4842 0.0018 262 3 261 5 259 42
21 37 665 0.0411 0.0004 0.2927 0.0064 0.0516 0.0011 0.0210 0.0001 0.9764 0.0019 260 3 261 6 268 48
22 17 299 0.0417 0.0004 0.2961 0.0087 0.0515 0.0015 0.0422 0.0003 0.4992 0.0017 263 3 263 8 265 66
23 35 620 0.0416 0.0004 0.2980 0.0054 0.0519 0.0009 0.0495 0.0002 0.4407 0.0019 263 3 265 5 282 39
24 33 585 0.0413 0.0004 0.2962 0.0047 0.0520 0.0008 0.0460 0.0003 0.4666 0.0056 261 3 263 4 287 34
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Table 2
Table 2 Major(%)and trace elements(×10-6)compositions of the monzogranites and granodiorites
Sample No. 02.19.2 02.24.1 02.39.1 02.40.2 02.25.2 02.31.1 02.32.1 02.32.2 02.33.2 02.38.1 7965.2 7907.1
Lithology monzogranite granodiorite
SiO2 73.94 71.42 71.32 72.91 69.61 69.03 67.76 67.7 68.02 68.9 66.12 66.61
Al2O3 13.11 14.42 14.44 14.28 14.78 15.09 15.32 15.86 15.78 15.48 15.93 16.01
Fe2O3 0.67 0.58 1.2 0.9 1.06 1.51 1.53 1.5 1.48 1.47 1.93 1.75
FeO 1.54 1.71 1.34 1 1.67 1.57 1.76 1.77 1.66 1.55 1.98 1.94
CaO 1.32 2.12 2.35 1.9 3.15 3.23 3.59 3.54 3.5 3.26 3.99 3.9
MgO 0.73 0.82 0.99 0.63 1.04 1.32 1.48 1.48 1.49 1.21 1.98 1.85
K2O 4.15 3.67 3.4 3.53 3.02 2.84 2.75 2.62 2.73 2.67 2.33 2.37
Na2O 3.64 4.06 3.96 4.07 4.12 4.03 4.07 4.31 4.18 4.22 4.03 4.06
TiO2 0.33 0.36 0.38 0.29 0.42 0.47 0.51 0.5 0.46 0.46 0.57 0.53
P2O5 0.081 0.088 0.098 0.076 0.12 0.12 0.13 0.12 0.12 0.13 0.14 0.14
MnO 0.056 0.059 0.061 0.052 0.072 0.063 0.067 0.067 0.064 0.069 0.072 0.07
L.O.I 0.27 0.51 0.31 0.25 0.76 0.55 0.83 0.34 0.33 0.42 0.7 0.56
Total 99.84 99.82 99.85 99.89 99.82 99.82 99.80 99.81 99.81 99.84 99.77 99.79
FeOT 2.14 2.23 2.42 1.81 2.62 2.93 3.14 3.12 2.99 2.87 3.72 3.52
Fe2O3T 2.38 2.48 2.69 2.01 2.92 3.25 3.49 3.47 3.33 3.19 4.13 3.91
Mg# 41.67 43.52 46.18 42.19 45.39 48.59 49.73 49.87 51.08 46.90 52.77 52.47
A/CNK 1.02 0.99 1.00 1.02 0.94 0.97 0.95 0.97 0.97 0.98 0.97 0.98
ALK 7.82 7.78 7.39 7.63 7.21 6.92 6.89 6.97 6.95 6.93 6.42 6.48
D.I. 88.07 83.88 82.58 86.22 79.25 77.29 75.26 75.03 75.30 77.20 70.70 71.49
Cr 4.29 4.51 5.62 4.35 4.42 7.74 9.4 8.55 9.62 7.68 17.5 19.7
Ni 3.17 3.27 4.34 3.13 4.41 6.5 7.12 7 7.92 4.76 13.8 14.4
Co 3.67 4.25 5.11 3.14 5.64 7.21 7.8 7.92 7.69 6.25 10.6 9.61
Rb 135 114 96.9 87.4 91.5 76 79.8 71.5 85.4 74.2 59.6 63.1
Cs 6.2 4.3 3.03 2.36 5.08 3.85 3.23 2.64 6.27 3.23 2.1 3.18
Sr 134 204 246 211 288 327 337 358 362 341 407 406
Ba 535 574 532 553 517 470 494 490 591 504 475 461
V 31.2 33.4 39.8 27.8 44.6 55.2 56.3 56.5 55 47.6 73.2 70
Sc 6.5 6.99 7.9 7.49 8.74 7.63 7.53 8.06 9.56 8.18 10.7 10.3
Nb 7.47 6.63 7.33 6.58 6.52 5.36 6.14 5.79 5.62 6.2 5.08 4.93
Ta 0.7 0.6 0.82 0.68 0.58 0.49 0.55 0.53 0.48 0.53 0.41 0.38
Zr 141 101 126 141 148 170 125 163 116 160 138 142
Hf 4.32 3 3.81 4.06 4.36 4.55 3.44 4.25 3.04 4.42 3.53 3.61
Ga 14.3 14.9 14.9 15 15.2 14.8 15.5 15.5 15.2 15.9 15.5 15.8
U 1.82 1.5 1.48 1.19 1.24 1.22 1.33 1.24 1.08 1.47 1.11 1.01
Th 10.5 9.28 11 7.38 8.03 6.62 6.67 6.23 5.26 8.74 5.12 5.35
La 19.6 14.4 26.5 18.1 17.4 21.7 14.4 16.6 13.7 15.5 17.8 16.3
Ce 36 26 41.2 30.8 29.6 34.6 25.2 27.8 25 27.4 29.1 27.8
Pr 4.42 3.33 5.34 3.78 4.06 4.6 3.33 3.7 3.32 3.76 3.98 3.61
Nd 15.7 12.3 18.2 12.7 15 16 12.5 13.9 12.8 14.1 15 13.7
Sm 3.11 2.49 3.4 2.41 3.04 2.8 2.57 2.74 2.72 2.81 2.9 2.66
Eu 0.45 0.58 0.64 0.52 0.66 0.72 0.71 0.77 0.77 0.74 0.85 0.82
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Gd 3.21 2.75 3.37 2.47 3.02 2.95 2.58 2.78 2.84 2.96 2.79 2.81
Tb 0.52 0.44 0.54 0.4 0.5 0.45 0.41 0.44 0.46 0.46 0.44 0.43
Dy 3.19 2.75 3.16 2.52 3 2.57 2.5 2.69 2.69 2.81 2.67 2.48
Ho 0.66 0.58 0.67 0.51 0.64 0.52 0.5 0.54 0.52 0.58 0.52 0.48
Er 1.96 1.62 1.91 1.51 1.91 1.49 1.43 1.55 1.5 1.7 1.43 1.37
Tm 0.32 0.27 0.31 0.26 0.3 0.24 0.22 0.25 0.24 0.27 0.23 0.21
Yb 2.27 2.02 2.31 1.83 2.15 1.74 1.56 1.71 1.64 1.91 1.52 1.48
Lu 0.37 0.31 0.38 0.31 0.34 0.29 0.26 0.28 0.26 0.31 0.24 0.25
Y 20 17.6 21.1 15.9 19.6 16.2 15.4 16.3 16.8 18.2 16 15.4
ΣREE 111.8 87.4 129.0 94.0 101.2 106.9 83.6 92.1 85.3 93.5 95.5 89.8
LREE/HREE 6.34 5.50 7.53 6.96 5.88 7.85 6.21 6.40 5.74 5.85 7.08 6.82
(La/Yb)N 6.19 5.11 8.23 7.09 5.81 8.95 6.62 6.96 5.99 5.82 8.40 7.90
(La/Sm)N 4.07 3.73 5.03 4.85 3.70 5.00 3.62 3.91 3.25 3.56 3.96 3.96
(Gd/Lu)N 1.07 1.10 1.10 0.98 1.10 1.26 1.23 1.23 1.35 1.18 1.44 1.39
δEu 0.44 0.68 0.58 0.65 0.67 0.77 0.84 0.85 0.85 0.79 0.92 0.92
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Table 3
Table 3 Sm-Nd and Rb-Sr isotopic compositions of the monzogranites and granodiorites
Sample Age (Ga) Rb Sr 87Sr/86Sr (87Sr/86Sr)i Sm Nd 143Nd/144Nd (143Nd/144Nd)i TDM(Ga) T2 DM(Ga) εNd fSm/Nd f(%)
02.19.2 0.27 135 134 0.710659 0.699458 3.11 15.7 0.512758 0.512536601 0.678807 0.648 4.81 -0.36 0.937
02.24.1 0.27 114 204 0.71135 0.705137 2.49 12.3 0.512748 0.51252174 0.718361 0.671 4.52 -0.35 0.931
02.39.1 0.27 96.9 246 0.711324 0.706944 3.4 18.2 0.512743 0.512534204 0.65213 0.652 4.76 -0.40 0.936monzogranite
02.40.2 0.27 87.4 211 0.711654 0.707048 2.41 12.7 0.512742 0.512529906 0.66673 0.658 4.68 -0.39 0.934
02.31.1 0.26 76 288 0.704934 0.702111 2.8 15 0.512775 0.512574102 0.600501 0.600 5.29 -0.40 0.946
02.32.1 0.26 79.8 327 0.705054 0.702443 2.57 16 0.512768 0.512595129 0.52189 0.567 5.70 -0.48 0.953
02.32.2 0.26 71.5 337 0.705594 0.703324 2.74 12.5 0.512763 0.512527088 0.789213 0.675 4.37 -0.30 0.928granodiorite
02.33.2 0.26 85.4 358 0.705537 0.702985 2.72 13.9 0.512758 0.512547397 0.667338 0.643 4.77 -0.37 0.936Note: f(%) is the proportion of mantle-derived components in the crust-mantle binary mixtures calculated by DePaolo et al. (1991) method. f=(Ndc/Ndm)/[(Ndc/Ndm)+( εm-εs)/ ( εs-εc), Ndc and Ndm represent abundance of Nd in crustal and mantle endmember respectively. εs, εc and εm represent εNd(t) values of sample, crust and mantle, Ndc=43.4×10-6, Ndm=15×10-6, εc=-14.24, εm=8.54.
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Table 4
Table 4 Zircon Hf isotopic data of the monzogranite (02TW19) and granodiorite (01TW32)
02TW19 Age (Ma) 176Yb/177Hf 176Lu/177Hf 176Hf/177Hf 176Hf/177Hfi εHf(0) εHf(t) TDM (Ma) TC DM (Ma)
1 271 0.0587 0.0017 0.282963 0.282954 6.7 12.4 417 5022 276 0.0820 0.0023 0.282996 0.282984 7.9 13.6 376 4303 270 0.0561 0.0016 0.282957 0.282949 6.5 12.2 425 5154 271 0.0797 0.0022 0.282935 0.282925 5.8 11.4 463 5695 270 0.0837 0.0024 0.282997 0.282985 8.0 13.5 374 4316 269 0.0729 0.0021 0.282982 0.282972 7.4 13.0 393 4637 271 0.1456 0.0040 0.282855 0.282835 2.9 8.2 610 7728 275 0.0612 0.0018 0.282968 0.282959 6.9 12.7 411 4889 270 0.0847 0.0026 0.282910 0.282897 4.9 10.4 506 63310 267 0.0988 0.0029 0.283110 0.283095 11.9 17.3 211 18211 269 0.0613 0.0017 0.282903 0.282894 4.6 10.2 504 63912 269 0.0637 0.0018 0.282968 0.282959 6.9 12.5 412 49313 271 0.0460 0.0014 0.282986 0.282979 7.6 13.3 381 44514 269 0.0577 0.0016 0.282990 0.282982 7.7 13.4 376 43915 266 0.0535 0.0015 0.282947 0.28294 6.2 11.8 437 53716 271 0.0495 0.0013 0.283008 0.283002 8.4 14.1 348 394
02TW32 Age (Ma) 176Yb/177Hf 176Lu/177Hf 176Hf/177Hf 176Hf/177Hfi εHf(0) εHf(t) TDM (Ma) TC DM (Ma)
1 261 0.0715 0.0020 0.282704 0.282694 -2.4 3.0 797 1097 2 261 0.0740 0.0021 0.282858 0.282848 3.0 8.4 576 751 3 260 0.0589 0.0017 0.282898 0.282890 4.5 9.9 510 654 4 261 0.0614 0.0018 0.282905 0.282896 4.7 10.1 503 641 5 265 0.0562 0.0017 0.282838 0.282830 2.3 7.9 597 788 6 262 0.0466 0.0013 0.282907 0.282900 4.8 10.3 493 630 7 264 0.1420 0.0031 0.282921 0.282905 5.3 10.5 498 618 8 261 0.0284 0.0008 0.282928 0.282924 5.5 11.1 456 576 9 263 0.0926 0.0023 0.282896 0.282884 4.4 9.8 524 666 10 263 0.0599 0.0015 0.282958 0.282950 6.6 12.1 423 516 11 265 0.0770 0.0021 0.282898 0.282887 4.5 9.9 517 657 12 262 0.0724 0.0018 0.282901 0.282892 4.6 10.0 509 649 13 264 0.0801 0.0019 0.282896 0.282886 4.4 9.8 517 661 14 263 0.0616 0.0015 0.282981 0.282973 7.4 12.9 389 463 15 263 0.0707 0.0017 0.283004 0.282995 8.2 13.7 358 413 16 261 0.0846 0.0019 0.282916 0.282907 5.1 10.5 487 615
Table 5
Table 5 Result from saturated Zr thermometer of the monzogranites and granodioritessample Zr(10-6) M Tzr(0C)
02.19.2 141 1.4 779 02.24.1 101 1.5 745 02.39.1 126 1.5 764 monzogranite
02.40.2 141 1.4 778 02.25.2 148 1.6 768 02.31.1 170 1.6 782 02.32.1 125 1.7 752 02.32.2 163 1.6 776 02.33.2 116 1.6 749 02.38.1 160 1.6 778 7965.2 138 1.7 760
granodiorite
7907.1 142 1.6 764
Note: TZr = 129000 /[2.95 + 0.85M + ln( 469000 /Zrsamle) ],M is some cationic ratios in rock, M = ( Na + K + 2Ca) /( Al × Si).
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DraftLith
ospher
ic m
antle
Lithospheric mantle
breakoff slab
Baiheshan accretio
nary complex
Baishan arc
Continen
tal c
rust
junenile crustal MASH zone
Carboniferousgranitoids Permian granitoids
Upwelling asthenosphere
Continental crust
CarboniferousBaishan Formation
Permian Shuangbaotang Formation
unconformity
N S
W
E
Permian (277-262Ma)
Extension
Oceanic crust Asth
enosp
here m
antle
Asthenosphere mantle
Schematic diagram showing the petrogenetic model for the Permian granitoids in northern Beishan orogen
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