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.
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.
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].
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.
Table 1.
GPS locations and lithology of the representative samples.
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.
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.
Table 2.
Analytical results of major (.wt%) and trace (ppm) elements for TTG and granitic gneisses in the eastern Alxa Block.
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).
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.
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).
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.
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.
Table 3.
Zircon U-Pb isotopic data obtained by SHRIMP for TTG and granitic gneisses in the eastern Alxa Block.
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.
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].
Figure 7.
U–Pb concordia diagrams for zircons from the TTG rocks (a–c) 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.
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.
Table 4.
Lu-Hf isotopic data for zircons from TTG rocks in the eastern Alxa Block.
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).
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].
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).
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 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.
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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