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Article

Archean Crustal Evolution of the Alxa Block, Western North China Craton: Constraints from Zircon U-Pb Ages and the Hf Isotopic Composition

1
Chengdu Exploration and Development Research Institute of PetroChina Daqing Oilfield Co., Ltd., Chengdu 610000, China
2
Institute of Geology, Chinese Academy of Geological Sciences, Beijing 100044, China
*
Author to whom correspondence should be addressed.
Minerals 2023, 13(5), 685; https://doi.org/10.3390/min13050685
Submission received: 24 March 2023 / Revised: 4 May 2023 / Accepted: 15 May 2023 / Published: 17 May 2023

Abstract

:
The Alxa Block is an important component of the North China Craton, but its metamorphic basement has been poorly studied, which hampers the understanding of the Alxa Block and the North China Craton. In this study, we conducted geochronological and geochemical studies on three TTG (tonalite–trondhjemite–granodiorite) gneisses and one granitic gneiss exposed in the Langshan area of the eastern Alxa Block to investigate their crustal evolution. The zircon U-Pb dating results revealed that the protoliths of the TTG and granitic gneisses were formed at 2836 ± 20 Ma, 2491 ± 18 Ma, 2540 ± 38 Ma, and 2763 ± 42 Ma, respectively, and were overprinted by middle–late Paleoproterozoic metamorphism (1962–1721 Ma). All gneiss samples had high Sr/Y ratios (41–274) and intermediate Mg# values (44.97–55.78), with negative Nb, Ta, and Ti anomalies and moderately to strongly fractionated REE patterns ((La/Yb)N = 10.6–107.1), slight Sr enrichment, and positive Eu anomalies, displaying features of typical high-SiO2 adakites and Archean TTGs. The magmatic zircons from the 2.84 Ga and 2.49 Ga TTG rocks had low εHf(t) values of −1.9–1.7, and −3.83–2.12 with two-stage model ages (TDMC) of 3.24–3.11 Ga and 3.10–3.01 Ga, respectively, whereas those from the 2.54 Ga TTG rock exhibited εHf(t) values ranging from −1.1 to 3.46 and TDMC from 3.0 Ga to 2.83 Ga, suggesting that the crustal materials of the basement rocks in the eastern Alxa Block were initially extracted from the depleted mantle during the late Paleoarchean to Mesoarchean era and were reworked in the late Mesoarchean and late Neoarchean era. By contrast, the Alxa Block probably had a relative younger crustal evolutionary history (<3.24 Ga) than the main North China (<3.88 Ga), Tarim (<3.9 Ga), and Yangtze (<3.8 Ga) Cratons and likely had a unique crustal evolutionary history before the early Paleoproterozoic era.

1. Introduction

Tonalite–trondhjemite–granodiorite (TTG) rocks constitute a major part of Archean continental crust and provide information about the composition, tectonic environment, and evolution of the early continental crust [1,2]. Studies have shown that the early Precambrian era was an important period of crustal growth, the continental crust formed between 3.0 Ga and 2.5 Ga accounted for 36% of the present continental crust, and the continental crust formed during 2.15–1.65 Ga accounted for 39% [3]. There are two views stating that Precambrian crustal growth was concentrated in three main stages: either 3.6 Ga, 2.7 Ga, and 1.8 Ga or 2.7 Ga, 1.9 Ga, and 1.2 Ga [3,4].
The China continent mainly consists of three early Precambrian nuclei, including the Yangtze Craton (YC), Tarim Craton (TC), and North China Craton (NCC) (Figure 1) [5,6,7,8,9,10]. In recent decades, major progress has been made in the reconstruction of the crustal growth history of the YC and TC [11,12,13,14,15,16]. Paleoarchean (3437–3262 Ma) TTG rocks have been found in the YC with two-stage Hf model ages from Hadean to Eoarchean [17,18,19,20,21]. Recently, Eoarchean (ca. 3.7 Ga) TTG rocks have been identified from the TC [22]. Additionally, the oldest detrital zircons from the basement rocks of the two cratons were dated 3.8–3.2 Ga with Eoarchean to Paleoarchean two-stage Hf model ages from the Eoarchean to Paleoarchean era [23,24,25], which suggest that the crustal evolution of the two cratons had already begun before the Paleoarchean era.
As one of the oldest cratons in China, the North China Craton (NCC) experienced a long and complicated geological history [29,30,31,32]. Most present models divide the NCC into the Eastern Block, Western Block, and Trans North China Orogen (TNCO) [27,33] (Figure 1). The early Precambrian tectonic pattern of the NCC remains controversial. Some scholars have believed that cratonization was completed ca. 2.5 Ga, marked by the “Wutai Movement” [34,35], followed by regional extension at the end of the Paleoproterozoic era that resulted in the destruction of the NCC (called activation) [36], while others have believed that the basement of the NCC had not been completely consolidated until ca. 1.9 Ga [37,38,39,40], and the “Lvliang Movement” ca. 1.8 Ga caused the Eastern Block and Western Block of the NCC to join together along the TNCO [7,41].
The Alxa Block is located in the westernmost part of the NCC. Compared with the main NCC and the YC and TC, the Precambrian basement of the Alxa Block is relatively less studied, which restricts a better understanding of the evolution of the NCC. In this paper, we report new geochronological and geochemical results for Meso-Neoarchean rocks from the Langshan area, which confirm the existence of the Archean basement in the Alxa Block and reveal evidence for the crustal evolution of the NCC.

2. Geological Background and Sample Descriptions

The Alxa Block, as the westernmost part of the NCC, is adjacent to the Central Asian Orogenic Belt in the north, the TC in the west, and the North Qilian Orogenic Belt in the south. The Precambrian basement of the Alxa Block is mainly exposed in the Longshoushan, Beidashan, Yabulaishan, Bayanwulashan, and Langshan areas (Figure 2), and the Bayanwula–Langshan Fault in the east is considered the eastern boundary of the Alxa Block [42,43]. The wide distribution of deserts and limited basement outcrops in the Alxa Block hamper the understanding of its tectonic pattern. The NE-oriented Langshan Mountains, located on the northeastern margin of the Alxa Block (Figure 2), are key areas in unravelling the early Precambrian geological evolution between the NCC and Alxa Block.
As the oldest basement in the Langshan area, the Diebusige Complex is mainly composed of banded biotite plagioclase gneiss, amphibolite gneiss, magnetite quartzite, marble, intrusive k-feldspar granite, and amphibolite. Some chronological studies have been conducted on the Diebusige Complex, but the formation age of the Diebusige Complex remains uncertain. Yang et al. (1988) [44] determined that the Rb-Sr isochron age of amphibolite was 3219 Ma, while Li et al. (2006) [45] obtained a Sm-Nd isochron age of 3081 ± 49 Ma, suggesting that the Diebusige Complex was formed in the Paleo-Mesoarchean era. The 2.75–3.5 Ga ages of detrital zircons and 2.5–2.69 Ga, 1.9–1.95 Ga, and 1.8–1.85 Ga ages of metamorphic zircons that Geng et al. (2006, 2007, 2010) [46,47,48,49] obtained from the Diebusige gneisses indicated that they were formed in the Neoarchean and underwent tectono-thermal events in the late Neoarchean and late Paleoproterozoic era. Dan et al. (2012) [50] suggested that the supracrustal rocks of the Diebusige Complex were deposited at 2.0–2.45 Ga and experienced metamorphism at 1.89 Ga and 1.79 Ga. Based on the chronology of the metamorphic basement, they believed that there was no Archean rock exposed in the eastern Alxa Block. However, Gong et al. (2012) [51] and Zhang et al. (2013) [52] found ca. 2.5 Ga TTG rock in the Beidashan area, providing evidence for the existence of exposed Archean rocks in the Alxa Block.
Figure 2. Geological map of the Alxa Block, westernmost North China Craton, and basement distribution of the Alxa Block. The ca. 2.5 Ga TTG rocks exposed in Beidashan area are from references [51,52].
Figure 2. Geological map of the Alxa Block, westernmost North China Craton, and basement distribution of the Alxa Block. The ca. 2.5 Ga TTG rocks exposed in Beidashan area are from references [51,52].
Minerals 13 00685 g002
Three TTG gneiss samples and one granitic gneiss sample were selected from the Diebusige Complex for this study; their detailed locations are shown in Table 1. All samples are gray–white, fine-to-medium grained, and generally show gneissic fabrics. Mineral grains are subhedral to anhedral, and some show serrated boundaries (Figure 3). The tonalitic gneiss (1810-1) mainly consists of plagioclase, quartz, hornblende, and minor biotite. Hornblende grains show recrystallization fronts, and quartz grains show irregular and crenulated margins, which suggests dynamic recrystallization. The trondhjemitic gneiss (1814-3) is mainly composed of plagioclase, quartz, hornblende, minor biotite, and K-feldspar. It was strongly affected by later deformation, and plagioclase and hornblende showed different degrees of fragmentation and alteration. Another tonalitic gneiss (1816-1) is characterized by a typical mineral assemblage of plagioclase, quartz, hornblende and biotite. Plagioclase grains show polysynthetic twinning, and quartz occurs as fine-grained and anhedral grains. Hornblende is the major dark mineral, and recrystallization is apparent in the surrounding area. The granitic gneiss (D798) is mainly composed of quartz, plagioclase, and biotite with minor accessory minerals of apatite, and mylonitization occurs under the superposition of later tectonic events.

3. Analytical Methods

3.1. Geochemistry

Whole-rock major and trace element analyses were completed at Wuhan Sample Solution Analytical Technology Co., Ltd. (Wuhan, China), and external standards and repeated samples were used to comprehensively control the analytical quality. Whole-rock major elements were measured using XRF, and five standards, BHVO-2, GSP-2, W-2A, GBW07103 and GBW07316, were determined in parallel. Trace elements were analyzed by inductively coupled plasma–mass spectrometry (ICP–MS) on an Agilent 7700e instrument with a shielded torch, and four standards, AGV-2, BHVO-2, BCR-2 and RGM-2, were used to monitor the analytical quality. The relative standard deviations for the whole-rock major and trace elements are within ±5%.

3.2. Zircon U-Pb Dating and Hf Isotopic Composition

SHRIMP zircon U-Pb dating was performed using a sensitive high-resolution ion microprobe (SHRIMP-II) at the Beijing SHRIMP Center, Institute of Geology, Chinese Academy of Geological Sciences, Beijing. The analytical procedure was the same as that of Williams. (1998) [53]. The primary flow intensity was 4.5 nA, and the spot size was 25–30 μm. Standard zircon TEM (417 Ma) was used for the age corrections [54]. Data processing was carried out using the ISOPLOT program [55], and uncertainties for individual analyses were quoted at 1σ, whereas those for weighted mean ages were quoted at a 2σ and 95% confidence level.
Zircon in situ Lu-Hf analyses were carried out using an NU plasma II MC-ICP–MS at the School of Earth and Space Sciences, Peking University. An ArF-excimer laser ablation system of Geolas HD (193 nm) was used with a 44 μm spot size. The analytical procedure was the same as that of Zhang et al. (2016) [56]. Data reduction was conducted using the IOLITE program [57]. Zircon 91,500 was used as an internal standard with a reference value of 176Hf/177Hf = 0.282307 ± 31 (2SD) [58], zircon Plešovice was used as the monitoring standard, and the value of 176Hf/177Hf = 0.282483 (2SD) was obtained, which was consistent with the suggested value of 0.282482 ± 13 (2SD) [59].

4. Results

4.1. Whole-Rock Major and Trace Elements

Whole-rock major and trace element analyses were performed on four samples, including three TTG gneisses (1810-1, 1814-3, and 1816-1) and one granitic gneiss (D798). The analytical results are given in Table 2.

4.1.1. Major Element Geochemistry

The TTG gneisses from the Diebusige Complex in the Langshan area had SiO2 contents of 60.55–77.80 wt.%, Al2O3 contents of 10.90–19.11 wt.%, and Na2O/K2O ratios of 0.93–6.38. In the normative An-Ab-Or diagram (Figure 4a), the samples 1810-1 (2.84 Ga) and 1816-1 (2.54 Ga) plotted in the tonalite field, except for sample 1814-3 (2.49 Ga), which plotted in the trondhjemite field. According to the A/NK vs. A/CNK classification (Figure 4b), the two tonalitic gneisses were weakly metaluminous, while the trondhjemitic gneiss was weakly peraluminous, which was in line with the TTG rocks with corresponding ages in the NCC. All TTG gneisses showed features of subalkaline series in the TAS diagram (Figure 4c). They mainly plotted in the medium-to-low K fields of the calc-alkaline and tholeiitic series in the K2O vs. SiO2 diagram (Figure 4d). In addition, they had Mg# values ranging between 44.97 and 52.23, with an average of 49.96 (Table 2), slightly higher than those of Archean high-Al TTGs (42 on average).
The 2.76 Ga granitic gneiss (D798) had SiO2 contents of 64.18–72.30 wt.% (69.63 wt.% on average), Al2O3 contents of 12.11–16.18 wt.% (14.37 wt.% on average), and Na2O/K2O ratios of 0.59–2.97 (1.15 on average). It displayed high-K calc-alkaline features in the K2O vs. SiO2 diagram (Figure 4d) and showed similar characteristics to the 2.5 Ga trondhjemitic gneiss (1814-3) in the TAS diagram and the A/NK vs. A/CNK diagram (Figure 4b,c). This rock had Mg# values of 45.89–55.78 (49.87 on average), which are in accordance with the TTG gneisses (Table 2).

4.1.2. Trace Element Geochemistry

In the chondrite-normalized REE diagrams (Figure 5a,c), the TTG gneisses show similar characteristics to the TTG rocks in the NCC. Three TTG gneisses exhibit broadly similar REE distribution patterns and different LREE and HREE fractionation degrees. They all have positive Eu anomalies with EuN/EuN* > 1.29. The 2.84 Ga tonalitic gneiss (LaN/YbN = 45.41) and the 2.54 Ga trondhjemitic gneiss (LaN/YbN = 19.21–50.58, 32.06 on average) show high fractionation between LREEs and HREEs, while the 2.49 Ga tonalitic gneiss shows relatively lower fractionations (LaN/YbN = 10.59–14.31, 12.64 on average).
In the primitive-normalized trace element diagrams (Figure 5b,d), three TTG gneisses show similar features in enrichment of LILEs (e.g., Rb, Ba, and Sr) and depletion of HFSEs (e.g., Nb, Ta, and Ti). They have variable contents of Cr and Ni. The 2.49 Ga tonalitic gneiss shows much higher Cr (118.5 ppm on average) and Ni (38.3 ppm on average) contents than the 2.54 Ga trondhjemitic gneiss (30.2 ppm and 7.8 ppm on average, respectively) and 2.84 Ga tonalitic gneiss (8.9 ppm and 9.4 ppm, respectively). The TTG gneisses and granitic gneisses are characterized by high Sr and low Y contents with high Sr/Y ratios (>41), analogous to average high-SiO2 adakites and Archean TTG [60].
The 2.76 Ga granitic gneiss exhibits characteristics similar to those of TTG gneisses in REE and trace element patterns (Figure 5c,d) and shows high REE fractionation (LaN/YbN = 12.82–107.07, 45.99 on average) and distinctly positive Eu anomalies (EuN/EuN* = 1.43–10.97, 3.49 on average). It also shows concentrations of Rb, Ba, and Sr contents and depletions of Nb, Ta, and Ti contents and has low contents of Cr (16.1 ppm on average) and Ni (11.8 ppm on average) that are similar to 2.84 Ga tonalitic gneiss.

4.2. Zircon U-Pb Dating and Hf Isotopic Results

The zircon U-Pb dating results of the TTG and granitic gneiss samples (1810-1, 1814-3, 1816-1, and D798) are presented in Table 3, and representative zircon features are presented in Figure 6. All tested samples contain subhedral–euhedral zircon grains with near oval shapes and arc-shaped terminations. The diameter of zircons from samples 1810-1, 1814-3, 1816-1, and D798 are between 200 μm and 400 μm. Cathodoluminescence (CL) imaging of most zircons reveals core–mantle–rim textures of oscillatory zoned cores overprinted by broad (<80 μm) or thin mantle (<50 μm) and rim (<15 μm) domains (Figure 6). The oscillatory zoned zircon cores are characterized by lower CL brightness values than the rims. Overgrowth mantles and rims are commonly narrow in all samples, with rare grains that are bright gray, homogeneous, and internally structureless. We interpret the zircon cores to have a magmatic origin, with mantles and rims resulting from metamorphic recrystallization [61]. In situ zircon Hf isotope analyses were conducted on the representative zircons of the three TTG gneisses (Figure 6), and the results are listed in Table 3. For the 2.54 Ga tonalitic gneiss (1816-1), the Hf isotopic compositions of the six inherited zircon cores were calculated based on the weighted mean age of 2616 ± 11 Ma, while the other nineteen magmatic zircon cores were calculated based on the crystallization age of 2540 ± 38 Ma. Similarly, the Hf isotopic compositions of ten magmatic zircon cores from the 2.49 Ga trondhjemitic gneiss (1814-3) were calculated based on the crystallization age of 2491 ± 18 Ma.

4.2.1. Tonalitic Gneiss Sample 1810-1

Twenty-four analyses were obtained from the tonalitic gneiss sample (1810-1), and three analyses were discordant (spots 1.1, 7.1 and 11.1; Table 3). Two concordant analyses from zircon cores with (spots 6.1 and 15.3) well-preserved oscillatory zoning yield 207Pb/206Pb ages of 2826 ± 16 Ma and 2842 ± 13 Ma, respectively, with a weighted mean 207Pb/206Pb age of 2836 ± 20 Ma (MSWD = 0.63), which was proposed to be the crystallization age of the protolith (Figure 7a). In addition, there were two 207Pb/206Pb age groups from the inherited zircon cores that yielded mean 207Pb/206Pb ages of 2880 ± 17 Ma (MSWD = 0.04) and 2918 ± 8 Ma (MSWD = 0.80). The weighted mean 207Pb/206Pb ages of the two Paleoproterozoic age groups obtained from the unzoned rim domains were 1951 ± 12 Ma (MSWD = 0.95; 1962–1935 Ma) and 1867 ± 12 Ma (MSWD = 1.3; 1915–1843 Ma) (Figure 7a). We considered these two age groups, ca. 1.87 Ga and ca. 1.95 Ga, to represent the ages of metamorphic events [61].
Eight magmatic zircon cores from the 2.84 Ga tonalitic gneiss (1810-1) had 176Hf/177Hf ratios between 0.280948 and 0.281053 (Table 4), age-corrected εHf(t) values ranging from 1.89 to 1.71, with two-stage Hf model ages (TDMC) of 3111–3242 Ma, respectively. Ten metamorphic zircon mantles or rims had relatively higher 176Hf/177Hf ratios between 0.281086 and 0.281181 and lower εHf(t) values from -18.90 to -13.49, with two-stage Hf model ages (TDMC) of 3143–3336 Ma.

4.2.2. Trondhjemitic Gneiss Sample 1814-3

Of the twenty-seven analyses of zircons from the trondhjemitic gneiss sample (1814-3), fourteen from the oscillatory zoned cores yield 207Pb/206Pb ages ranging between 2191 ± 24 Ma and 2577 ± 21 Ma. Ten analyses (2443–2555 Ma) yield a weighted mean 207Pb/206Pb age of 2491 ± 18 Ma (MSWD = 0.99; Table 3; Figure 7b). Eleven analyses were obtained from the oscillatory unzoned rims and yield 207Pb/206Pb ages ranging between 1702 Ma and 1943 Ma, with a weighted mean 207Pb/206Pb age of 1834 ± 45 Ma (MSWD = 0.58; Figure 7b). Together with the intercept ages of 1819 ± 120 Ma and 2422 ± 59 Ma (MSWD = 0.66) (Figure 7b), we consider the mean 207Pb/206Pb age of 2491 ± 18 Ma obtained from the oscillatory zoned cores to represent the crystallization age of the trondhjemitic gneiss and the mean 207Pb/206Pb age of 1834 ± 45 Ma obtained from the unzoned rims to represent the age of metamorphism overprinted on the trondhjemitic gneiss [61].
Ten magmatic zircons from the 2.49 Ga trondhjemitic gneiss (1814-3) have 176Hf/177Hf ratios between 0.281112 and 0.281170 (Table 4), corresponding to age-corrected εHf(t) values between −3.38 and −2.12, slightly lower than those of magmatic zircons from sample 1810-1. The two-stage Hf model ages (TDMC) range from 3011 Ma to 3096 Ma. Three analyses from the metamorphic zircon grains or rims present 176Hf/177Hf ratios varying from 0.281137 to 0.281235, and their age-corrected εHf(t) values are between −18.83 and −13.45. The corresponding two-stage Hf model ages (TDMC) range from 3070 to 3269 Ma.

4.2.3. Tonalitic Gneiss Sample 1816-1

Thirty-two analyses were obtained from the tonalitic gneiss sample (1816-1) (Table 3; Figure 7c). Six analyses from the inherited cores yield 207Pb/206Pb ages of 2588–2667 Ma, with a weighted mean age of 2616 ± 11 Ma (MSWD = 0.98; Figure 7c). Eighteen analyses from magmatic zircon cores show variable degrees of Pb loss with 207Pb/206Pb ages of 2042–2555 Ma, and seven analyses from metamorphic zircons or rims yield 207Pb/206Pb ages of 1748–1866 Ma. All analyses except for those from inherited zircons define a discordia line with an upper concordia intercept age of 2540 ± 38 Ma and a lower concordia intercept age of 1764 ± 42 Ma (MSWD = 0.90; Figure 7c). Six concordant analyses from unzoned rim domains (spots 10.1, 16.1, 19.1, 22.1, 27.1, and 29.1) that yield 207Pb/206Pb ages between 1820 ± 32 Ma and 1748 ± 39 Ma have a weighted mean age of 1784 ± 24 Ma (MSWD = 0.63), which is identical to the intercept ages within errors. Therefore, ages of 2540 ± 38 Ma and 1784 ± 24 Ma are proposed to reflect the crystallization and metamorphic ages of the tonalitic gneiss, respectively.
Nineteen magmatic zircon cores from the 2.54 Ga tonalitic gneiss have 176Hf/177Hf ratios ranging from 0.281159 to 0.281252 (Table 4), age-corrected εHf(t) values from −1.10 to 1.52, with two-stage Hf model ages (TDMC) ranging from 2868 Ma to 2999 Ma, respectively. Seven metamorphic zircon grains exhibit 176Hf/177Hf ratios between 0.281215 and 0.281517 and relatively lower εHf(t) values between −15.70 and −4.20. The corresponding two-stage Hf model ages (TDMC) are 2574–3110 Ma, which are mainly concentrated in the ranges of 2697–2799 Ma, respectively. In addition, six inherited zircon cores show a similar 176Hf/177Hf ratio range of 0.281162–0.281223, with εHf(t) values of 0.80–3.46 and corresponding two-stage Hf model ages (TDMC) of 2832–2965 Ma.

4.2.4. Granitic Gneiss Sample D798

Twenty-eight analyses were obtained from the granitic gneiss sample (D798) (Table 3; Figure 7d). Twelve analyses show a large error (≥87 Ma), which is useless for age determination, and two analyses are discordant (spots 3.1 and 18.1). Nine analyses show variable degrees of Pb loss with 207Pb/206Pb ages of 2380–2801 Ma and define a discordia line with an upper concordia intercept age of 2763 ± 42 Ma (MSWD = 0.88; Figure 7d). The only analysis (spot 20.1) close to the concordia line that yields a 207Pb/206Pb age of 2760 ± 10 Ma responds well to the upper intercept age, reflecting the protolith emplacement age of the granitic gneiss. Four analyses from unzoned rims yield 207Pb/206Pb ages of 1852–1721 Ma and are interpreted as the metamorphic ages of the granitic gneiss [61].

5. Discussion

5.1. Petrogenesis of the TTG Rocks and Granitic Gneiss

The TTG gneisses from the Diebusige Complex are characterized by high SiO2 contents (>62 wt.%), Sr/Y ratios (41–191) and intermediate Mg# values (44.97–52.23) (Table 2), with negative Nb, Ta, and Ti anomalies and enrichment in Sr (Figure 5b,d). These characteristics are similar to those of Archean TTGs and high-SiO2 adakites, which are consistent with the results in the Sr vs. (CaO + Na2O) diagram (Figure 8a). The low εHf(t) values (-3.83 to 3.46) and the presence of old xenocrystic zircons (2.84 Ga and 2.54 Ga tonalitic gneiss samples) suggest a crustal origin for the protoliths. The moderately to strongly fractionated REE patterns ((La/Yb)N = 10.59–50.58), low Sr contents (373.38–677.51 ppm) and positive Eu anomalies (EuN/EuN* = 1.29–3.73)) suggest partial melting in the garnet stability field and the absence of plagioclase in the residue. Generally, rutile has a lower Nb/Ta ratio than chondrite, and its residue in the source or separation and differentiation during magmatic crystallization led to a higher Nb/Ta ratio of the melts [62]. Element Nb has a higher distribution coefficient than Ta in hornblende [63,64], and the presence of hornblende in the residue led to lower Nb/Ta and Dy/Yb ratios and higher Zr/Sm ratios for the corresponding melts [65]. The 2.49 Ga trondhjemitic gneiss and 2.54 Ga tonalitic gneiss in the Langshan area have Nb/Ta ratios lower than those of chondrite (17.6 [66]; 19.9 [67]), indicating that the negative Nb, Ta, and Ti anomalies were not caused by residual rutile in the source but were more likely related to the residues of hornblende in the source. The 2.84 Ga tonalitic gneiss has high Nb/Ta ratios; thus, its negative Nb, Ta, and Ti anomalies may have been controlled by rutile residues in the source. Together with the classification proposed by Moyen (2011) [68], the 2.49 Ga trondhjemitic gneiss and 2.54 Ga tonalitic gneiss were derived from partial melting of garnet-bearing amphibolite under high-to-medium pressure conditions, while the 2.84 Ga tonalitic gneiss was derived from partial melting of rutile-bearing eclogite under high-pressure conditions (Figure 8b,c).
The 2.76 Ga granitic gneiss from the Diebusige Complex has SiO2 contents (66.43–74.49 wt.%), Sr/Y ratios (47–274, 117 on average), and intermediate Mg# values (45.89–55.78, 49.87 on average) (Table 2 and Figure 8d), with significantly negative Nb and Ta anomalies and slight Ti anomalies (Figure 5d), which are similar to ca. 2.5 Ga TTG gneisses discussed above and show the features of high-SiO2 adakites (Figure 8a). High Sr/Y ratios, moderate to strong REE fractionations and positive Eu anomalies (EuN/EuN* = 1.43–10.97) suggest that the granitic gneiss was probably derived from partial melting of a subducted basaltic slab with garnet in the residue. The granitic gneiss shows low Nb/Ta (7.25–14.96, 10.81 on average) and Zr/Sm ratios (10.13–192.51, 67.30 on average), indicating that it was derived from partial melting of garnet-bearing amphibolite (Figure 8c).
Previous studies have suggested that the potential source of Archean TTGs and modern adakites may have been the melting of subducting oceanic crust [2,60,72,73], thickened lower crust [74,75,76], or delaminated lower crust [74,77]. Generally, TTG or adakitic melts with low Mg# values and Cr and Ni concentrations can be generated by the partial melting of mafic rocks underplating the lower crust [69,78], while those generated from the partial melting of a subducting slab and delaminated thickened lower crust would have higher Mg# values and MgO, Cr, and Ni contents on account of the interaction with the overlying mantle wedge during ascent [60,74,79,80]. Additionally, TTG melts produced by the partial melting of the delaminated lower crust would have higher contents of MgO (>3 wt.%), TiO2 (>0.9 wt.%) and compatible elements [81,82,83]. The low MgO (<3.21 wt.%) and TiO2 (<0.81 wt.%) contents of TTG gneisses from the Langshan area can rule out the origin of partial melting of the delaminated lower crust. The Mg# value can be used as a marker to reflect whether the mafic rock was contaminated by the mantle during the melting process; generally, the Mg# value of a typical mid-oceanic ridge basalt is <60 (51 on average), and the Mg# value of the melt formed by its partial melting is <45 [69,76]. All TTG gneisses and the granitic gneiss in this study show similar Mg# values (approximately 50) (Figure 8d), indicating that a certain degree of mantle contamination may have occurred during the ascent of the TTG melts. However, they have different compatible element compositions: the 2.84 Ga tonalitic gneiss and 2.76 Ga granitic gneiss have low Cr and Ni contents, and the 2.49 Ga trondhjemitic and 2.54 Ga tonalitic gneisses have relatively high contents of Cr and Ni. Therefore, the 2.84 Ga tonalitic gneiss and 2.76 Ga granitic gneiss might have formed by the partial melting of the thickened lower crust, whereas the 2.49 Ga trondhjemitic and the 2.54 Ga tonalitic gneisses are probably related to the partial melting of the subducted oceanic slab.

5.2. Archean to Late Paleoproterozoic Crustal Evolution in the Alxa Block

The Diebusige Complex is one of the oldest metamorphic series in the eastern Alxa Block. The results show that the 2.84 Ga and 2.54 Ga tonalitic gneisses, the 2.49 Ga trondhjemitic gneiss, and the 2.76 Ga granitic gneiss are components of the Diebusige Complex. The magmatic zircon age populations at ca. 2.8 Ga and ca. 2.5 Ga indicate that the eastern Alxa Block experienced at least two magmatic events in the late Mesoarchean to late Neoarchean era. Zircon Hf isotope analysis shows that all magmatic zircons from the TTG rocks have εHf(t) values ranging from −3.83 to 3.46, which suggest a crustal origin for the protoliths. Previous studies have suggested that the two-stage zircon Hf model age (TDMC) can accurately reflect the extraction time of source materials from depleted mantle [84]. Magmatic zircons from the 2.84 Ga tonalitic gneiss have TDMC values between 3.24 Ga and 3.11 Ga, while those from the 2.54 Ga tonalitic gneiss and 2.49 Ga trondhjemitic gneiss have TDMC values of 3.0–2.83 Ga and 3.10–3.01 Ga, respectively, indicating that the Langshan TTG gneisses were derived from reworking of Paleo-Mesoarchean crust and mixed with mantle materials to different degrees during migration. The 2.84 Ga tonalitic gneiss is the oldest rock currently exposed in the Alxa Block. Recently, Gong et al. (2012) and Zhang et al. (2013b) [51,52] recognized 2.5 Ga TTG rocks from the Beidashan Complex in the western Alxa Block. Zircon Hf isotopic features suggested that the western Alxa Block experienced a mostly 2.8–2.7 Ga crustal growth and a ca. 2.5 Ga magmatic–metamorphic event. The TDMC values of 3.59–3.02 Ga obtained from the ca. 2.8 Ga-inherited zircons also implied the existence of Paleo-Mesoarchean crustal materials in the western Alxa Block [52]. Combined datasets show that the eastern and western Alxa Block probably had the same Paleo-Mesoarchean crust, and the Alxa Block experienced Paleo-Mesoarchean crustal growth, a ca. 2.8 Ga magmatic event, and a ca. 2.5 Ga magmatic–metamorphic event.
The Langshan TTG gneisses and granitic gneiss recorded continuous metamorphic ages of 1962–1721 Ma with peaks at ca. 1.95 Ga and ca. 1.85 Ga. Paleoproterozoic metamorphic events were widely developed in every Precambrian basement in the Alxa Block, such as the Bayanwulashan Complex in the eastern Alxa Block and the Beidashan Complex and Longshoushan Complex in the western Alxa Block [50,52,85,86]. The remaining NCC also recorded these two metamorphic events, and previous studies have suggested that ca. 1.95 Ga and ca. 1.85 Ga corresponded to the formation ages of the Khondalite Belt and the TNCO [27,87,88,89,90], respectively. However, whether the formation of the TNCO could have affected the Alxa Block located in the westernmost part of the NCC is still uncertain. A few models suggested the ca. 1.95 Ga and ca. 1.85 Ga events were related to the assembly and breakup of the Paleoproterozoic Columbia supercontinent since they have been identified globally (e.g., Laurentia, Baltica, Amazonia, and India [91,92,93,94,95,96]).

5.3. Early Geological History of the Alxa Block in Comparison with the YC, TC, and Main NCC

The NCC, YC, and TC are three old cratons in China that constitute the main nucleus of the Chinese continent [5,6,27,97]. Despite considerable progress over recent decades in understanding the Precambrian evolution of these three cratons, limited work has been conducted on comparing their early geological histories [7,8,98,99,100,101,102].
As an important component of the Archean crust, TTG rocks play an important role in the study of Precambrian crustal evolution. In terms of the YC, previous studies show that Paleo-Neoarchean TTG rocks were well developed in the YC [11,13,103,104,105,106,107]. The oldest TTG rocks were formed during 3437–3262 Ma, and zircon Hf isotope studies have suggested that these rocks with εHf(t) values of −4.7–1.2 were sourced from the Hadean to Eoarchean crust [17,18,19,20,21,103,104] (Figure 9). Additionally, detrital zircons with ages of 3.8–3.2 Ga have been identified in the YC [24,25], indicating that the beginning of crustal evolution of the YC was as early as the Eoarchean to Paleoarchean era (Figure 9 and Figure 10d). Mesoarchean TTG rocks from the YC have εHf(t) values of −10-3, which yield TDMC values ranging between ca. 3.8 Ga and ca. 3.0 Ga [20,105] (Figure 10f). This suggests that Eoarchean to Paleoarchean crustal materials in the YC were reworked in the Mesoarchean. The Neoarchean rocks were also recognized from the YC [15], and their zircon Hf isotopic features suggest a derivation from Mesoarchean reworked components (Figure 10f).
The discovery of ca. 3.7 Ga tonalitic gneisses with a mean εHf(t) value of −0.7 ± 2.6 suggests that the crustal evolution of the TC began before the Eoarchean era [22] (Figure 9 and Figure 10c). Detrital zircons from metasedimentary rocks in the northern TC were dated ca. 2.5 Ga to ca. 3.5 Ga with TDMC values from ca. 3.9 Ga to ca. 3.7 Ga [23], similarly indicating that the crustal components in the TC may have been generated as early as ca. 3.9 Ga. Neoarchean orthogneisses and mafic–ultramafic rocks are widely exposed in the TC [12,16,95,98,99]. Previous studies have shown that continuous magmatic events occurred in the Neoarchean era, and zircon Hf isotopes yield a large range of εHf(t) values (ca. −8–10) with two-stage model ages from the Paleoarchean to Neoarchean era (ca. 3.4–2.8 Ga) [16,23,98,116,117] (Figure 9 and Figure 10c). This suggests that basement rocks in the TC involved synchronous crustal growth and reworking during the Paleo-Neoarchean era.
Numerous detrital and inherited zircons from a variety of metasedimentary rocks in the eastern NCC have been dated 3.88–3.6 Ga, suggesting that the beginning of crustal evolution of the NCC was as early as before the Eoarchean era [30,121,122,123,124] (Figure 10d). Recently, ca. 3.8 Ga TTG rocks and granulite enclaves were also identified in the NCC [125,126], further confirming the existence of Eoarchean continental materials and the initial time of crustal evolution of the NCC. Paleoarchean zircons from the eastern NCC have εHf(t) values ranging from −5 to 3 and give Eo-Paleoarchean two-stage model ages varying from 3.9 Ga to 3.4 Ga (Figure 9 and Figure 10b). Zircons from the Mesoarchean and Neoarchean TTG rocks have variable εHf(t) values of −5.5–10.2 (3.6 on average) and −7.8–12.6 (4.1 on average) with two-stage model ages of 4.2–2.8 Ga and 3.9–2.5 Ga, respectively (Figure 9 and Figure 10b). These results indicate that basement rocks in the main NCC involved synchronous crustal growth and reworking, similar to the TC during the Paleo-Neoarchean era.
The Alxa Block is the westernmost component of the NCC. The existence of Archean rocks has long been controversial until ca. 2.5 Ga TTG rocks were identified from the western Alxa Block [51,52]. Mesoarchean to early Paleoproterozoic granitic gneisses (2.76 Ga) and TTG gneisses (2.84 Ga, 2.54 Ga, and 2.49 Ga) from the Langshan area in the eastern Alxa Block are reported in this study. As mentioned above, magmatic zircons from the Langshan TTG gneisses have εHf(t) values ranging from −3.83 to 3.46 and two-stage model ages ranging from 3.3 Ga to 2.9 Ga with peaks at ca. 3.2 Ga and ca. 3.0 Ga. Magmatic zircons from the ca. 2.5 Ga TTG rocks in the western Alxa Block have εHf(t) values varying from -5.54 to 8.98, and two-stage model ages mainly vary from 3.0 Ga to 2.6 Ga, with a peak at ca. 2.8 Ga [51,52]. By contrast (Figure 9 and Figure 10), the eastern Alxa Block recorded a 3.3–2.9 Ga crustal growth and 2.8–2.7 Ga and ca. 2.5 Ga crustal reworking, which have been extensively recorded in most ancient cratons worldwide [31,75,126,127], whereas the western Alxa Block recorded a 2.8–2.7 Ga crustal growth and ca. 2.5 Ga crustal growth and reworking. This indicates that the eastern Alxa Block has older crustal materials than the western Alxa Block, and crustal growth and reworking simultaneously occurred 2.8–2.7 Ga in the Alxa Block (Figure 10a,b). The combination of available datasets suggests that the oldest basement exposed in the Alxa Block formed in the Paleo-Mesoarchean era and that crustal evolution began in the Paleoarchean era, which was younger than those of the main NCC, TC, and YC (Figure 9 and Figure 10). Therefore, we suggest that the Alxa Block probably has its unique crustal evolutionary history before the early Paleoproterozoic.

6. Conclusions

Based on geological, geochronological, geochemical, and zircon Lu-Hf isotope data from the Langshan area in the eastern Alxa Block, we reach the following conclusions:
(1).
The granitic gneiss and three TTG gneisses from the Langshan area were mainly emplaced 2.76 Ga, 2.84 Ga, 2.54 Ga, and 2.49 Ga, respectively, supporting the existence of Archean rocks in the eastern Alxa Block.
(2).
Zircon Lu-Hf isotope data indicated that the Langshan TTG gneisses were derived from partial melting of crustal materials extracted from depleted mantle during the Paleoarchean to Mesoarchean era (3.24–2.83 Ga).
(3).
The eastern Alxa Block experienced an important period of crustal growth during ca. 3.24–2.83 Ga, followed by crustal reworking of ca. 2.8 Ga and ca. 2.5 Ga, and the Alxa Block probably had its unique crustal evolution history from before the early Paleoproterozoic era, which was younger than that of the main NCC, TC, and YC.

Author Contributions

Conceptualization, J.Q. and J.Z.; methodology, B.Z.; software, H.Z.; investigation, P.N., J.Q. and J.Z.; resources, J.Q.; data curation, P.N., B.Z. and H.Z.; writing—original draft preparation, P.N.; writing—review and editing, J.Q. and J.Z.; visualization, P.N., B.Z. and H.Z.; supervision, J.Q.; funding acquisition, J.Q. and J.Z. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by: Basic Scientific Research Fund of the Institute of Geology, Chinese Academy of Geological Sciences, grant number J2103; China Geological Survey, grant number DD20230217; National Natural Science Foundation of China, grant number 41972224.

Data Availability Statement

The data presented in this study are available on reasonable request from the corresponding authors.

Acknowledgments

We would like to thank the Key Laboratory of Mineral Resources Evaluation in Northeast Asia, Ministry of Land and Resources of China, the Wuhan Sample Solution Analytical Technology Co., Ltd., and the Beijing SHRIMP Center, Institute of Geology, Chinese Academy of Geological Sciences, Beijing, for their support and assistance on sample processing, zircon U–Pb dating, Hf isotope and major and trace element analyses. The authors are grateful for the critical comments from the anonymous reviewers, which profoundly enhanced the quality of this manuscript.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. Distribution of Precambrian basement and subdivision of the North China Craton [26,27,28]. Additionally, shown are the locations of Archean TTGs with rock ages.
Figure 1. Distribution of Precambrian basement and subdivision of the North China Craton [26,27,28]. Additionally, shown are the locations of Archean TTGs with rock ages.
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Figure 3. Field photos and representative photomicrographs of the TTG rocks and granitic samples from the Diebusige Complex, eastern Alxa Block. (a,b) Tonalitic gneiss sample 1810-1; (c,d) trondhjemitic gneiss sample 1814-3; (e,f) tonalitic gneiss sample 1816-1; and (g,h) granitic gneiss sample D798. Qtz: quartz; Pl: plagioclase; Bt: biotite; Kfs: K-feldspar; Amp: amphibole; and Ca: calcite.
Figure 3. Field photos and representative photomicrographs of the TTG rocks and granitic samples from the Diebusige Complex, eastern Alxa Block. (a,b) Tonalitic gneiss sample 1810-1; (c,d) trondhjemitic gneiss sample 1814-3; (e,f) tonalitic gneiss sample 1816-1; and (g,h) granitic gneiss sample D798. Qtz: quartz; Pl: plagioclase; Bt: biotite; Kfs: K-feldspar; Amp: amphibole; and Ca: calcite.
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Figure 4. Geochemical discrimination diagrams for the TTG and granitic gneisses from the Diebusige Complex, eastern Alxa Block. (a) An-Ab-Or diagram of the gneiss samples after O’Conner (1965) and Barker (1979); (b) ANK vs. ACNK diagram; (c) SiO2 vs. total alkali (Na2O + K2O) content diagram (Middlemost, 1994); and (d) SiO2 vs. K2O diagram.
Figure 4. Geochemical discrimination diagrams for the TTG and granitic gneisses from the Diebusige Complex, eastern Alxa Block. (a) An-Ab-Or diagram of the gneiss samples after O’Conner (1965) and Barker (1979); (b) ANK vs. ACNK diagram; (c) SiO2 vs. total alkali (Na2O + K2O) content diagram (Middlemost, 1994); and (d) SiO2 vs. K2O diagram.
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Figure 5. Chondrite-normalized REE patterns (a) and (c) and primitive mantle-normalized spider diagrams (b) and (d) for the TTG and granitic gneisses in the eastern Alxa Block.
Figure 5. Chondrite-normalized REE patterns (a) and (c) and primitive mantle-normalized spider diagrams (b) and (d) for the TTG and granitic gneisses in the eastern Alxa Block.
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Figure 6. Representative cathodoluminescence images of dated zircons. The white solid-line circle and white number represent the analytical spot of U-Pb dating and dating result, respectively. The yellow dashed-line circle and yellow number represent the the analytical spot of Hf isotope and its corrected 176Hf/177Hf value, respectively.
Figure 6. Representative cathodoluminescence images of dated zircons. The white solid-line circle and white number represent the analytical spot of U-Pb dating and dating result, respectively. The yellow dashed-line circle and yellow number represent the the analytical spot of Hf isotope and its corrected 176Hf/177Hf value, respectively.
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Figure 7. U–Pb concordia diagrams for zircons from the TTG rocks (ac) and granitic gneiss (d) in the eastern Alxa Block. The purple and black ellipses represent analyses for inherited or xenocrystic zircons; The gray ellipses represent discordant analyses; The blue ellipses represent analyses for magmatic zircons, while the red and green ellipses represent analyses for metamorphic zircons.
Figure 7. U–Pb concordia diagrams for zircons from the TTG rocks (ac) and granitic gneiss (d) in the eastern Alxa Block. The purple and black ellipses represent analyses for inherited or xenocrystic zircons; The gray ellipses represent discordant analyses; The blue ellipses represent analyses for magmatic zircons, while the red and green ellipses represent analyses for metamorphic zircons.
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Figure 8. Geochemical modeling results for the TTG and granitic gneisses in the eastern Alxa Block. (a) Sr vs. (CaO + Na2O) diagram after references [60,64,69]; (b) Ce/Sr vs. Y diagram after reference [68]; and (c) Nb/Ta vs. Zr/Sm diagram and melting curves after reference [70]; (d) Mg# vs. SiO2 diagram after reference [71].
Figure 8. Geochemical modeling results for the TTG and granitic gneisses in the eastern Alxa Block. (a) Sr vs. (CaO + Na2O) diagram after references [60,64,69]; (b) Ce/Sr vs. Y diagram after reference [68]; and (c) Nb/Ta vs. Zr/Sm diagram and melting curves after reference [70]; (d) Mg# vs. SiO2 diagram after reference [71].
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Figure 9. Diagram of εHf(t) values vs. 207Pb/206Pb ages for zircons from the basement rocks in the Alxa Block and the main North China, Tarim, and Yangtze cratons. Data for the Alxa Block are from references [51,52] and this study; (2) data for the main North China Craton are from references [30,65,106,108,109,110,111,112,113,114,115]; (3) data for the Tarim Craton are from references [22,23,98,99,116,117]; and (4) data for the Yangtze Craton are from references [11,14,17,19,21,24,102,103,107,118,119,120].
Figure 9. Diagram of εHf(t) values vs. 207Pb/206Pb ages for zircons from the basement rocks in the Alxa Block and the main North China, Tarim, and Yangtze cratons. Data for the Alxa Block are from references [51,52] and this study; (2) data for the main North China Craton are from references [30,65,106,108,109,110,111,112,113,114,115]; (3) data for the Tarim Craton are from references [22,23,98,99,116,117]; and (4) data for the Yangtze Craton are from references [11,14,17,19,21,24,102,103,107,118,119,120].
Minerals 13 00685 g009
Figure 10. Zircon Hf isotope model age (TDMC) histogram for basement rocks of the eastern Alxa Block (a), western Alxa Block (b), whole Alxa Block (c), and the main North China (d), Tarim (e), and Yangtze (f) cratons. Data sources are the same as those in Figure 9.
Figure 10. Zircon Hf isotope model age (TDMC) histogram for basement rocks of the eastern Alxa Block (a), western Alxa Block (b), whole Alxa Block (c), and the main North China (d), Tarim (e), and Yangtze (f) cratons. Data sources are the same as those in Figure 9.
Minerals 13 00685 g010
Table 1. GPS locations and lithology of the representative samples.
Table 1. GPS locations and lithology of the representative samples.
SampleGPS LocationLithologyMineral Assemblage
1810-140°35′55.15″ N
106°16′42.56″ E
Tonalitic gneissQtz (25%) + Pl (65%) + Hb (5%) + Bt (5%)
1814-340°35′53.69″ N
106°16′53.29″ E
Trondhjemitic gneissQtz (35%) + Pl (45%) + Hb (10%) + Bt (5%) + Kfs (5%)
1816-143°34′20.01″ N
106°12′29.44″ E
Tonalitic gneissQtz (20%) + Pl (60%) + Hb (15%) + Bt (5%)
D79840°35′19.14″ N
106°15′38.23″ E
Granitic gneissQtz (30%) + Pl (55%) + Bt (15%)
Table 2. Analytical results of major (.wt%) and trace (ppm) elements for TTG and granitic gneisses in the eastern Alxa Block.
Table 2. Analytical results of major (.wt%) and trace (ppm) elements for TTG and granitic gneisses in the eastern Alxa Block.
SampleD7981810-11814-31816-1
Rock TypeGranitic GneissTonalitic GneissTrondhjemitic GneissTonalitic Gneiss
SiO269.84 71.54 72.30 71.67 64.1866.78 68.8671.88 77.80 69.41 60.55 66.49 66.14 62.04 68.71
TiO20.23 0.18 0.21 0.36 0.300.41 0.300.20 0.05 0.42 0.08 0.18 0.64 0.81 0.41
Al2O315.10 13.68 12.11 12.58 15.9915.64 16.1 13.71 10.90 12.17 19.11 14.64 14.86 14.32 13.13
TFe2O31.71 1.48 1.60 2.61 2.903.28 2.06 1.72 1.39 4.66 4.06 4.80 5.26 7.73 4.32
MnO0.03 0.03 0.03 0.04 0.050.05 0.03 0.02 0.02 0.07 0.06 0.07 0.09 0.11 0.07
MgO1.09 0.71 0.76 1.26 1.55 1.64 0.88 0.88 0.76 2.54 2.24 2.56 2.17 3.21 2.37
CaO1.30 1.87 2.33 2.13 2.61 1.96 2.99 1.12 3.73 1.79 1.50 1.73 4.19 5.00 4.94
Na2O3.89 3.05 2.85 4.14 3.68 4.13 5.35 3.28 2.81 4.03 6.77 4.46 3.66 3.44 3.61
K2O4.07 4.62 4.81 2.75 5.08 3.48 1.80 5.14 1.33 2.02 2.94 1.90 1.20 0.84 0.57
P2O50.02 0.01 0.07 0.08 0.28 0.10 0.13 0.01 0.06 0.07 0.13 0.08 0.14 0.11 0.14
LOI2.56 2.66 2.74 2.22 3.03 2.32 1.17 1.77 1.47 2.60 2.30 2.90 1.46 2.19 1.61
total99.84 99.83 99.80 99.84 99.64 99.77 99.74 99.72 100.32 99.77 99.73 99.81 99.81 99.80 99.87
Li8.38 6.49 5.89 17.09 15.10 10.34 7.04 8.92 3.86 19.48 16.84 19.23 17.20 22.83 14.37
Be0.84 0.72 0.50 1.28 0.93 1.08 1.18 0.75 3.66 19.48 16.84 19.23 1.06 1.07 14.37
V20.76 21.38 22.70 48.02 33.44 40.58 30.73 19.20 14.24 40.84 25.75 36.85 79.20 147.61 66.26
Cr10.99 15.67 9.71 25.59 26.64 18.78 11.87 9.86 8.93 34.20 55.55 29.44 111.93 201.04 42.63
Co3.44 3.81 3.75 6.80 5.59 7.18 4.99 3.68 3.29 10.89 7.79 7.77 14.03 37.06 13.86
Ni5.23 9.68 8.25 16.56 27.86 17.08 5.13 4.33 9.45 12.14 8.13 5.94 20.84 82.17 12.01
Cu3.02 5.04 19.99 5.27 7.77 3.55 11.61 3.05 11.95 32.24 3.33 2.06 13.22 101.59 4.38
Zn36.91 29.61 28.43 51.61 47.10 60.55 51.85 40.81 36.47 68.66 61.95 81.60 71.27 128.54 70.22
Ga19.03 16.48 13.63 19.91 19.15 18.89 22.54 15.49 13.52 15.19 20.46 15.60 18.19 19.69 17.97
Rb93.85 111.34 111.73 54.82 115.10 79.24 22.07 110.95 44.49 39.21 70.00 44.53 14.48 14.39 5.93
Sr278.77 222.19 205.53 330.25 428.20 449.88 869.58 377.05 373.38 456.51 677.51 442.67 474.87 415.79 474.31
Zr113.94 136.68 56.92 57.47 50.75 40.80 24.83 33.28 70.93 248.84 26.99 253.78 81.80 30.48 21.72
Nb4.32 2.75 5.05 4.39 5.72 3.51 3.75 5.18 1.30 5.62 1.86 11.25 13.10 9.78 4.27
Sn0.65 0.82 0.62 0.45 0.53 0.41 0.87 0.46 0.31 0.61 0.46 0.47 0.87 0.77 0.77
Cs0.62 1.03 0.53 0.63 0.60 0.75 0.18 0.75 0.37 0.62 0.59 0.65 1.30 1.48 1.01
Ba842.77 988.31 1338.22 856.66 2428.99 1319.21 1248.15 1951.79 320.81 1152.90 1509.41 768.83 772.23 579.27 371.54
La18.41 14.32 19.41 14.81 34.00 19.66 25.73 11.03 14.10 19.33 26.71 16.84 27.88 18.44 16.61
Ce27.52 21.03 26.58 21.87 57.76 27.93 45.31 14.38 23.64 28.00 42.47 27.73 47.66 30.38 27.16
Pr2.61 1.88 2.64 2.21 6.03 2.65 4.90 1.10 2.03 2.64 4.04 2.70 5.19 3.57 3.35
Nd8.45 5.89 8.95 7.79 21.12 8.71 17.59 3.01 5.50 8.58 13.57 9.39 18.77 13.46 12.59
Sm1.23 0.71 1.40 1.24 3.19 1.26 2.45 0.31 0.59 1.02 1.75 1.29 2.88 2.00 2.12
Eu0.75 0.84 0.89 0.92 1.79 1.20 0.98 1.00 0.22 1.15 1.62 1.19 1.18 1.36 1.04
Gd0.89 0.54 1.19 1.04 2.41 1.02 1.56 0.23 0.41 0.82 1.29 1.04 2.55 1.85 1.90
Tb0.12 0.07 0.17 0.15 0.33 0.14 0.18 0.04 0.07 0.11 0.17 0.14 0.38 0.27 0.28
Dy0.48 0.43 0.75 0.76 1.48 0.70 0.60 0.16 0.32 0.49 0.72 0.68 2.03 1.51 1.50
Ho0.10 0.11 0.14 0.16 0.27 0.14 0.09 0.03 0.06 0.11 0.14 0.15 0.42 0.33 0.31
Er0.25 0.45 0.36 0.44 0.74 0.35 0.25 0.12 0.20 0.31 0.37 0.45 1.25 1.02 0.87
Tm0.04 0.09 0.05 0.07 0.09 0.05 0.03 0.02 0.03 0.06 0.05 0.08 0.20 0.17 0.13
Yb0.27 0.75 0.29 0.44 0.54 0.32 0.16 0.15 0.21 0.42 0.36 0.59 1.31 1.17 0.86
Lu0.05 0.14 0.04 0.07 0.08 0.05 0.03 0.03 0.04 0.07 0.06 0.11 0.21 0.19 0.13
Y2.95 3.46 4.35 4.68 7.84 3.84 3.18 1.75 2.09 3.23 3.54 4.05 11.57 8.70 8.33
Sc2.47 3.73 1.63 6.32 3.36 5.26 2.69 2.68 2.23 4.77 4.41 4.95 11.37 17.85 9.83
Hf3.99 4.34 1.70 1.67 1.68 1.24 0.74 1.13 1.89 7.30 0.84 6.55 2.34 1.62 0.67
Ta0.45 0.38 0.44 0.60 0.49 0.29 0.31 0.35 0.04 0.75 0.79 2.94 2.74 0.80 0.68
Tl0.53 0.58 0.55 0.36 0.55 0.39 0.14 0.51 0.29 0.26 0.34 0.25 0.13 0.11 0.07
Pb23.65 21.86 20.55 17.63 22.81 18.43 19.37 20.22 15.96 7.48 15.20 5.78 9.76 10.42 7.81
Th5.43 0.27 2.68 0.42 1.36 0.31 0.14 0.18 4.59 0.40 0.43 5.01 0.51 0.22 0.10
U0.53 0.37 0.19 0.17 0.50 0.14 0.07 0.09 0.65 0.31 0.09 0.51 0.26 0.26 0.06
Mg#55.78 48.5548.4548.8551.4349.7345.8950.2552.0451.8752.2351.3944.9745.1352.05
EuN/EuN*2.08 3.99 2.05 2.41 1.89 3.13 1.43 10.97 1.29 3.73 3.15 3.03 1.30 2.13 1.55
Sr/Y94.66 64.29 47.27 70.51 54.65 117.03 273.54 215.45 178.30 141.29 191.28 109.33 41.03 47.80 56.91
La/Yb68.20 19.02 66.24 33.57 62.62 61.23 158.81 76.08 67.36 46.47 75.03 28.49 21.23 15.70 19.32
Nb/Ta9.55 7.25 11.56 7.33 11.58 12.05 12.17 14.96 30.37 7.52 2.36 3.83 4.78 12.20 6.25
Zr/Sm92.33 192.51 40.72 46.46 15.89 32.33 10.13 108.04 119.91 243.96 15.44 196.73 28.40 15.21 10.24
Gd/Yb3.31 0.71 4.06 2.35 4.44 3.18 9.62 1.61 1.98 1.96 3.62 1.76 1.94 1.58 2.21
Ce/Sr0.10 0.09 0.13 0.07 0.13 0.06 0.05 0.04 0.06 0.06 0.06 0.06 0.10 0.07 0.06
(La/Yb)N45.98 12.82 44.66 22.63 42.22 41.28 107.07 51.29 45.41 31.33 50.58 19.21 14.31 10.59 13.02
Mg# = 100 × Mg/(Mg + Fe2+); TFeO = TFe2O3 × 0.8998; EuN/EuN* = 2 × EuN/(SmN + GdN); N: chondrite normalized; LOI: loss on ignition.
Table 3. Zircon U-Pb isotopic data obtained by SHRIMP for TTG and granitic gneisses in the eastern Alxa Block.
Table 3. Zircon U-Pb isotopic data obtained by SHRIMP for TTG and granitic gneisses in the eastern Alxa Block.
Spot No206Pbc (%)UThTh/U206Pb*207Pb/206PbError in %207Pb/235UError in %206Pb/238PbError in %Error corr207Pb/206Pb206Pb/238UDiscordant (%)
ppmppmppmAge (Ma)Age (Ma)
D798: Granitic gneiss
1.10.94 56 24 0.44 24.10.1831 2.712.56 3.20.4977 1.70.533 2681 452604 373
2.10.37 470 112 0.25 1680.1600 0.519.14 1.20.4145 1.10.911 2456 8.62236 219
2.225.34 51 30 0.61 22.90.1610 147.70 150.3520 4.10.274 2446 2401943 6721
3.10.31 92 77 0.86 35.60.1609 1.39.98 1.90.4499 1.40.753 2465 212395 293
4.10.65 69 77 1.16 29.70.1848 1.712.69 2.30.4983 1.60.671 2696 282607 333
5.12.29 36 24 0.68 9.640.1087 6.54.52 6.90.3018 2.10.307 1777 1201700 314
6.11.36 37 19 0.53 12.50.1381 57.41 6.40.3890 3.90.616 2202 872119 704
7.10.52 140 110 0.81 500.1599 1.29.10 1.80.4130 1.40.765 2454 202229 269
8.114.76 52 38 0.74 16.30.1010 174.19 170.3009 2.60.149 1643 3201696 38−3
9.10.69 74 31 0.43 27.40.1567 1.79.24 2.30.4278 1.60.695 2420 292296 315
10.13.97 31 15 0.51 120.1180 7.26.94 7.70.4270 2.40.317 1924 1302293 46−19
11.12.33 18 12 0.69 5.710.1160 5.95.68 6.50.3549 2.50.389 1895 1101958 42−3
11.210.14 53 14 0.27 10.90.1350 313.90 330.2108 4.50.139 2159 5601233 4443
12.11.16 55 45 0.84 15.30.1064 34.63 3.40.3159 1.70.497 1738 541769 26−2
13.11.48 45 29 0.65 13.50.1133 3.55.34 40.3417 1.80.464 1852 641895 30−2
14.118.37 31 17 0.56 8.150.0810 362.80 360.2480 3.60.098 1211 7101428 44−18
15.18.97 165 105 0.66 45.30.0990 133.91 130.2873 1.70.133 1597 2301628 24−2
16.12.34 46 20 0.45 14.70.1090 125.45 120.3616 2.50.201 1788 2201990 40−11
17.10.23 210 203 1.00 63.40.1234 1.25.97 1.90.3512 1.40.768 2005 211940 243
18.10.19 121 91 0.78 45.10.1730 0.8110.31 1.60.4323 1.40.867 2587 142316 2810
19.10.52 147 103 0.72 40.40.1073 1.44.70 1.90.3180 1.30.692 1753 251780 21–2
20.10.11 177 146 0.85 81.20.1921 0.6114.11 1.40.5326 1.30.900 2760 102752 280
21.10.16 224 222 1.03 90.90.1753 0.611.39 1.40.4712 1.20.900 2609 102489 255
22.10.26 170 1 0.00 81.40.1970 0.6115.09 1.40.5557 1.30.902 2801 102849 29–2
23.12.51 39 26 0.69 11.60.0956 4.74.41 5.10.3345 1.90.372 1539 891860 30–21
24.10.67 140 102 0.75 39.80.1054 1.54.78 20.3286 1.30.669 1721 271832 21–6
25.11.23 61 27 0.46 21.30.1531 2.88.40 3.30.3981 1.60.499 2380 492160 309
26.16.87 72 22 0.31 180.1220 114.47 120.2661 2.20.192 1985 2001521 2823
1810–1: Tonalitic gneiss
1.10.07 99 39 0.41 42.40.1849 0.7812.68 1.80.4974 1.60.902 2697 132603354
2.10.01 453 107 0.24 1380.1186 0.855.80 1.40.3549 1.20.809 1935 15195820−1
3.10.01 47 102 2.23 13.50.1172 1.75.35 2.30.3310 1.60.702 1915 301843264
3.20.03 307 176 0.59 88.80.1133 0.695.26 1.40.3368 1.20.872 1853 12187120−1
3.30.12 164 141 0.89 480.1158 0.945.43 1.60.3403 1.30.810 1892 171888210
4.10.02 184 56 0.31 83.70.1935 0.5714.09 1.40.5280 1.30.912 2772 9.32733281
4.20.01 1102 3 0.00 3370.1204 0.875.90 1.60.3557 1.40.846 1962 161962230
5.10.10 52 49 0.98 14.80.1157 25.28 2.60.3312 1.70.640 1890 361844272
6.10.01 338 168 0.51 1600.2000 0.9815.22 1.50.5521 1.20.773 2826 162834270
7.10.01 771 548 0.74 3700.2120 0.2816.32 1.20.5584 1.10.970 2921 4.52860262
7.20.09 76 28 0.38 39.70.2073 1.417.42 2.40.6090 1.90.803 2885 23306847−6
8.10.06 80 56 0.72 21.50.1156 1.34.95 1.90.3104 1.40.756 1890 231742228
9.10.00 594 127 0.22 1650.1141 0.565.08 1.30.3230 1.20.900 1866 101804183
10.10.00 1373 743 0.56 5310.1901 0.4811.80 1.30.4503 1.20.925 2743 7.823972313
11.10.07 91 36 0.41 40.50.2098 1.914.99 3.70.5180 3.20.854 2904 312691707
12.10.04 123 48 0.40 62.20.2185 0.817.80 1.70.5908 1.50.875 2970 13299335−1
13.10.02 204 77 0.39 97.90.2101 0.6916.17 1.60.5581 1.40.900 2906 112859332
13.20.01 480 205 0.44 2380.2067 0.5616.45 1.60.5772 1.50.938 2880 9.1293736−2
14.10.03 224 112 0.52 62.80.1127 0.955.07 1.70.3263 1.40.818 1843 171820221
14.20.09 274 94 0.35 83.10.1187 0.865.78 1.60.3529 1.30.835 1937 15194922−1
15.10.09 94 36 0.40 26.80.1130 1.35.15 20.3304 1.50.760 1849 231840240
15.20.02 775 11 0.01 2390.1200 0.465.94 1.30.3588 1.20.931 1957 8.2197620−1
15.30.02 718 185 0.27 3380.2020 0.7815.25 2.50.5480 2.40.949 2842 132816541
16.10.43 26 27 1.07 7.650.1148 2.55.42 3.20.3423 20.620 1876 46189833−1
1814–3: Trondhjemitic gneiss
1.10.19 31 31 1.05 12.80.1588 1.510.682.40.4879 1.80.773 2443 25256138−5
2.10.12 25 6 0.24 10.60.1661 1.711.432.60.4994 20.761 2518 28261142−4
3.10.02 84 86 1.06 34.70.1646 0.9310.871.70.4788 1.40.837 2504 16252230−1
3.21.15 5 3 0.62 1.560.1172 6.35.297.40.3270 40.533 1914 1101825635
3.30.20 20 12 0.62 8.420.1698 2.811.443.60.4890 2.30.629 2555 472564480
4.10.09 26 29 1.13 10.30.1557 1.79.752.60.4540 20.755 2410 292413390
5.10.00 6 2 0.35 1.880.1101 4.55.3960.3550 40.662 1802 82195967−9
6.10.17 32 18 0.58 13.30.1637 1.510.972.40.4861 1.80.767 2495 26255439−2
6.20.28 12 9 0.75 3.440.1171 3.55.224.40.3232 2.70.611 1913 631805426
7.10.36 14 3 0.26 3.910.1103 3.35.054.20.3318 2.60.611 1805 60184741−2
8.10.36 10 4 0.49 2.770.1081 4.25.035.10.3374 2.90.574 1768 76187447−6
9.10.00 2 1 0.60 0.5630.1191 7.85.93100.3610 6.30.631 1943 1401987110−2
9.20.33 15 13 0.89 6.520.1645 2.211.333.50.5000 2.70.769 2503 37261258−4
10.10.02 54 41 0.79 18.50.1371 1.47.522.10.3981 1.60.753 2191 242160291
10.2−0.23 16 4 0.25 4.660.1095 2.85.073.70.3360 2.40.657 1791 51186739−4
11.10.00 33 32 0.98 13.10.1593 3.710.074.20.4587 1.90.458 2448 632434391
12.10.12 40 28 0.73 18.80.1811 2.513.7130.5493 1.60.552 2663 41282237−6
13.10.09 37 26 0.72 16.10.1720 1.312.072.10.5089 1.70.803 2577 21265237−3
16.10.08 103 87 0.87 390.1517 0.939.21.80.4397 1.50.851 2365 162349301
16.20.28 15 10 0.72 4.230.1136 3.65.224.50.3332 2.70.607 1858 641854440
17.11.12 8 3 0.39 2.350.1043 7.94.89.50.3340 5.30.556 1702 150185685−9
18.13.93 7 3 0.40 1.850.1150 114.89120.3070 5.20.423 1886 2001727798
19.10.47 39 20 0.53 15.70.1632 2.210.573.20.4700 2.30.722 2489 382483480
20.10.15 31 22 0.73 140.1732 1.512.512.40.5240 1.90.795 2588 24271642−5
21.10.00 22 24 1.15 9.070.1601 1.810.6130.4800 2.40.802 2457 30252950−3
22.10.00 15 3 0.21 4.150.1136 3.25.044.20.3217 2.70.646 1857 571798423
23.10.27 24 18 0.78 10.20.1627 2.810.923.50.4870 2.10.613 2484 47255745−3
1816–1: Tonalitic gneiss
1.10.05 80 44 0.56 25.40.1365 26.962.50.3699 1.60.615 2029 272183 357
2.10.02 158 131 0.86 47.60.1259 1.86.112.80.3516 2.10.762 1942 362042 325
3.10.01 149 116 0.80 520.1481 2.28.32.60.4066 1.40.523 2200 252324 385
4.10.03 154 113 0.76 66.80.1754 1.112.191.80.5038 1.40.776 2630 302610 18−1
4.20.13 140 71 0.53 59.90.1740 0.7211.941.50.4975 1.30.879 2603 292597 120
5.10.09 85 56 0.69 32.70.1593 19.861.90.4488 1.60.839 2390 312448 172
6.10.04 108 54 0.52 440.1651 0.8710.82.20.4746 20.918 2504 422508 150
7.10.01 355 342 1.00 1380.1630 0.9210.171.50.4523 1.20.791 2406 242487 163
8.10.00 153 88 0.59 67.10.1771 0.6812.471.50.5105 1.30.889 2659 292626 11−1
9.10.02 322 272 0.87 1180.1524 0.888.931.80.4248 1.60.873 2282 302373 154
10.10.12 110 71 0.67 30.30.1080 1.24.7561.90.3194 1.40.758 1787 221766 22−1
11.10.04 88 50 0.58 340.1598 19.881.80.4483 1.50.824 2388 292454 173
12.10.04 134 107 0.83 55.20.1762 0.7911.671.60.4804 1.30.863 2529 282618 133
13.10.28 82 35 0.44 23.40.1141 1.55.182.10.3295 1.50.712 1836 241866 272
14.10.04 268 186 0.72 82.60.1264 0.886.2541.60.3588 1.30.826 1977 222049 164
15.10.03 155 123 0.82 63.90.1634 1.410.81.90.4794 1.30.698 2525 282491 23−1
16.10.00 44 27 0.64 120.1101 1.94.82.60.3163 1.80.691 1772 281801 342
17.10.04 79 50 0.66 35.70.1815 0.913.21.70.5275 1.50.853 2731 332667 15−2
18.10.06 159 120 0.78 49.40.1365 1.16.81.70.3615 1.30.776 1989 222183 199
18.2−0.03 110 61 0.57 46.70.1697 111.581.80.4949 1.50.822 2592 322555 17−1
19.10.00 54 53 1.02 14.80.1091 1.74.812.40.3199 1.70.700 1789 261784 310
20.10.08 82 42 0.53 340.1731 2.211.542.70.4837 1.50.552 2543 312588 372
21.10.02 267 208 0.81 92.80.1420 2.37.922.70.4047 1.40.511 2191 262251 403
22.10.13 65 28 0.44 180.1096 1.54.852.20.3210 1.60.719 1794 251793 280
23.10.00 159 80 0.52 60.40.1578 0.749.641.60.4430 1.40.882 2364 272432 123
24.10.11 120 98 0.84 48.50.1630 0.8510.511.60.4679 1.40.851 2474 282487 140
25.10.03 94 67 0.74 34.70.1579 1.89.332.30.4286 1.40.634 2299 282434 306
26.10.04 199 151 0.78 74.50.1590 1.99.542.50.4354 1.70.671 2330 332445 325
27.10.39 62 28 0.47 16.90.1069 2.14.682.70.3177 1.60.613 1778 251748 39−2
28.10.04 131 75 0.59 56.50.1773 0.7512.281.60.5024 1.40.888 2624 312628 120
29.10.35 67 33 0.50 18.20.1112 1.84.82.40.3132 1.60.672 1756 241820 323
30.10.66 265 187 0.73 860.1366 1.37.082.60.3757 2.30.875 2056 402185 226
Errors are 1-sigma; Pbc and Pb* indicate the common and radiogenic portions, respectively. Error in Standard calibration was 0.22% (not included in above errors but required when comparing data from different mounts). Common Pb corrected using measured 204Pb.
Table 4. Lu-Hf isotopic data for zircons from TTG rocks in the eastern Alxa Block.
Table 4. Lu-Hf isotopic data for zircons from TTG rocks in the eastern Alxa Block.
No.Measured Age (Ma)Used Age (Ma)176Yb/177Hf176Lu/177Hf176Hf/177Hf (corr)εHf(0)εHf(t)TDMTDMCfLu/Hf
1810–1: Tonalitic gneiss
2.11935 1935 0.008069 0.000277 0.281181 0.000013 −56.27 −13.49 0.46 2831 3134−0.99
3.11915 1915 0.011251 0.000387 0.281154 0.000014 −57.22 −15.05 0.50 2875 3196−0.99
3.31892 1892 0.009593 0.000331 0.281128 0.000012 −58.13 −16.41 0.44 2905 3246−0.99
4.12772 2772 0.015876 0.000621 0.281053 0.000014 −60.78 0.42 0.48 3027 3111−0.98
4.21962 1962 0.010297 0.000390 0.281165 0.000013 −56.84 −13.62 0.47 2861 3162−0.99
5.11890 1890 0.005287 0.000177 0.281153 0.000013 −57.26 −15.37 0.44 2861 3192−0.99
6.12826 2826 0.029679 0.001094 0.281031 0.000017 −61.55 −0.04 0.61 3094 3178−0.97
8.11890 1890 0.007648 0.000272 0.281133 0.000013 −57.98 −16.23 0.45 2895 3235–0.99
9.11866 1866 0.014119 0.000632 0.281168 0.000014 −56.73 −15.96 0.49 2874 3203−0.98
10.12743 2743 0.032849 0.001155 0.281035 0.000015 −61.42 −1.89 0.54 3094 3203−0.97
11.12904 2904 0.011499 0.000435 0.280979 0.000018 −63.42 1.15 0.64 3112 3182−0.99
12.12970 2970 0.009732 0.000366 0.280948 0.000015 −64.51 1.71 0.53 3148 3208−0.99
13.12906 2906 0.029166 0.001132 0.281010 0.000018 −62.32 0.92 0.63 3127 3195–0.97
13.22880 2880 0.016740 0.000676 0.280963 0.000021 −63.98 −0.45 0.77 3153 3242−0.98
14.21937 1937 0.008957 0.000322 0.281169 0.000014 −56.69 −13.93 0.49 2850 3158−0.99
15.11849 1849 0.008050 0.000352 0.281086 0.000014 −59.61 −18.90 0.50 2962 3336−0.99
15.32842 2842 0.041481 0.001464 0.281023 0.000014 −61.84 −0.68 0.49 3136 3223−0.96
16.11876 1876 0.008185 0.000293 0.281169 0.000015 −56.69 −15.28 0.52 2848 3176−0.99
1814–3: Trondhjemitic gneiss
1.12443 2491 0.023648 0.000801 0.281170 0.000014 −56.65 −2.12 0.49 2884 3011−0.98
2.12518 2491 0.012920 0.000479 0.281123 0.000015 −58.32 −3.25 0.54 2923 3068−0.99
3.12504 2491 0.010837 0.000401 0.281112 0.000016 −58.69 −3.49 0.55 2931 3079−0.99
3.32555 2491 0.023738 0.000807 0.281152 0.000016 −57.29 −2.77 0.55 2909 3043−0.98
6.12495 2491 0.016543 0.000587 0.281137 0.000016 −57.82 −2.93 0.58 2912 3051−0.98
6.21913 1913 0.010601 0.000413 0.281192 0.000018 −55.89 −13.79 0.64 2826 3131−0.99
8.11768 1768 0.008023 0.000293 0.281137 0.000015 −57.81 −18.83 0.54 2890 3269−0.99
9.22503 2491 0.017259 0.000587 0.281112 0.000016 −58.71 −3.83 0.56 2946 3096−0.98
11.12448 2491 0.020314 0.000703 0.281152 0.000015 −57.28 −2.59 0.53 2901 3034−0.98
19.12489 2491 0.011975 0.000419 0.281135 0.000017 −57.90 −2.73 0.61 2903 3041−0.99
21.12457 2491 0.021810 0.000711 0.281134 0.000017 −57.93 −3.26 0.62 2926 3068−0.98
22.11857 1857 0.009303 0.000381 0.281235 0.000019 −54.35 −13.45 0.67 2766 3070−0.99
23.12484 2491 0.017408 0.000619 0.281132 0.000017 −57.99 −3.15 0.62 2921 3062−0.98
1816–1: Tonalitic gneiss
1.12183 2540 0.008120 0.000341 0.281196 0.000014 −55.73 0.71 0.51 2815 2909−0.99
2.12042 2540 0.018306 0.000719 0.281205 0.000015 −55.40 0.39 0.52 2830 2925−0.98
3.12324 2540 0.019608 0.000785 0.281240 0.000017 −54.16 1.52 0.61 2788 2868−0.98
4.12610 2616 0.019010 0.000764 0.281190 0.000017 −55.94 1.48 0.59 2854 2931−0.98
4.22597 2616 0.007257 0.000312 0.281223 0.000015 −54.77 3.46 0.54 2777 2832−0.99
5.12448 2540 0.008014 0.000324 0.281208 0.000016 −55.30 1.17 0.58 2798 2885−0.99
6.12508 2540 0.007759 0.000320 0.281183 0.000014 −56.18 0.29 0.51 2831 2929−0.99
7.12487 2540 0.037669 0.001519 0.281252 0.000019 −53.76 0.65 0.67 2826 2911−0.95
8.12626 2616 0.008833 0.000360 0.281186 0.000015 −56.09 2.05 0.52 2830 2903−0.99
9.12373 2540 0.025353 0.001020 0.281249 0.000017 −53.86 1.41 0.62 2793 2873−0.97
10.11766 1766 0.008814 0.000354 0.281229 0.000017 −54.58 −15.70 0.59 2773 3110−0.99
11.12454 2540 0.010133 0.000398 0.281209 0.000017 −55.29 1.05 0.61 2803 2891−0.99
12.12618 2616 0.024690 0.000973 0.281204 0.000018 −55.44 1.61 0.63 2851 2925−0.97
13.11866 1866 0.007226 0.000292 0.281215 0.000017 −55.07 −13.87 0.60 2787 3098−0.99
14.12049 2540 0.029831 0.001212 0.281251 0.000017 −53.79 1.15 0.61 2805 2886−0.96
15.12491 2540 0.013793 0.000541 0.281188 0.000017 −56.02 0.07 0.60 2841 2941−0.98
16.11801 1801 0.002951 0.000119 0.281388 0.000015 −48.93 −8.96 0.52 2544 2799−1.00
17.12667 2616 0.010778 0.000429 0.281184 0.000018 −56.16 1.86 0.64 2838 2912−0.99
18.12183 2540 0.017517 0.000689 0.281208 0.000018 −55.30 0.54 0.65 2824 2917−0.98
18.22555 2540 0.011776 0.000483 0.281162 0.000015 −56.95 −0.76 0.55 2872 2982−0.99
19.11784 1784 0.004382 0.000165 0.281405 0.000018 −48.35 −8.82 0.65 2525 2779−1.00
20.12588 2540 0.014708 0.000577 0.281166 0.000015 −56.81 −0.78 0.54 2873 2983−0.98
21.12251 2540 0.023336 0.000939 0.281174 0.000017 −56.49 −1.10 0.62 2888 2999−0.97
22.11793 1793 0.006664 0.000281 0.281417 0.000018 −47.92 −8.32 0.65 2516 2761−0.99
23.12432 2540 0.007641 0.000319 0.281159 0.000016 −57.04 −0.57 0.59 2863 2973−0.99
24.12487 2540 0.017488 0.000671 0.281209 0.000019 −55.26 0.61 0.67 2821 2913−0.98
25.12434 2540 0.011524 0.000450 0.281171 0.000017 −56.63 −0.39 0.60 2857 2964−0.99
26.12445 2540 0.031465 0.001271 0.281214 0.000019 −55.09 −0.26 0.68 2859 2957−0.96
27.11748 1748 0.004465 0.000183 0.281458 0.000022 −46.48 −7.78 0.77 2455 2697−0.99
28.12628 2616 0.014402 0.000576 0.281162 0.000017 −56.95 0.80 0.62 2879 2965−0.98
29.11820 1820 0.007359 0.000304 0.281517 0.000020 −44.39 −4.20 0.71 2383 2574−0.99
30.12185 2540 0.012065 0.000470 0.281174 0.000017 −56.52 −0.31 0.60 2855 2960−0.99
Note: measured age (Ma) represents the measured age of SHRIMP U-Pb dating for the analyses, and the used age (Ma) represents the ages that are used during the calculation of εHf(t) and model age. The crustal model ages (TDMC) were calculated by assuming 176Lu/177Hf ratio of 0.010 for the upper crust.
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Niu, P.; Qu, J.; Zhang, J.; Zhang, B.; Zhao, H. Archean Crustal Evolution of the Alxa Block, Western North China Craton: Constraints from Zircon U-Pb Ages and the Hf Isotopic Composition. Minerals 2023, 13, 685. https://doi.org/10.3390/min13050685

AMA Style

Niu P, Qu J, Zhang J, Zhang B, Zhao H. Archean Crustal Evolution of the Alxa Block, Western North China Craton: Constraints from Zircon U-Pb Ages and the Hf Isotopic Composition. Minerals. 2023; 13(5):685. https://doi.org/10.3390/min13050685

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Niu, Pengfei, Junfeng Qu, Jin Zhang, Beihang Zhang, and Heng Zhao. 2023. "Archean Crustal Evolution of the Alxa Block, Western North China Craton: Constraints from Zircon U-Pb Ages and the Hf Isotopic Composition" Minerals 13, no. 5: 685. https://doi.org/10.3390/min13050685

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