6.1.1. Evaluation of Post-Magmatic Alteration
The loss on ignition (LOI) values of hornblende gabbro samples are generally low, ranging from 1.46 to 3.13 wt%, indicating that these rocks have only experienced weak low-temperature alteration. These rocks are dominated by plagioclase, clinopyroxene, and hornblende, with their alteration mainly consisting of chloritization and sericitization. Such alterations consume only small amounts of mafic minerals and plagioclase, incorporate limited structural water, and thus contribute weakly to LOI. Although a few samples (e.g., YQ-11, YQ-20) show slightly higher LOI values, possibly related to locally enhanced alteration of hornblende, the overall degree of alteration has not significantly affected the geochemical signals of immobile elements.
In contrast, the LOI values of olivine websterite samples are notably higher, ranging from 4.22 to 5.4 wt%, reflecting intense low-temperature alteration. As ultramafic cumulates, these rocks are mainly composed of olivine, orthopyroxene, and clinopyroxene. Their high MgO contents (18.57–28.19 wt%) provide sufficient material basis for serpentinization. During the reaction of olivine with aqueous fluids to form serpentine, large amounts of structural water are incorporated, which are released during LOI analysis and directly increase the LOI values. The widespread serpentinization observed in the petrographic thin sections provides direct evidence for this process.
6.1.2. Magmatic Source
The whole-rock trace elements of the Chengxuanbei intrusion exhibit typical geochemical signatures of subduction zone magmas: the large-ion lithophile elements (LILEs, e.g., Rb, Ba, Th, U) are significantly enriched, whereas the high-field-strength elements (HFSEs, e.g., Nb, Ta, Zr, Hf) are markedly depleted (
Figure 9a). This geochemical fingerprint is highly consistent with mantle wedge metasomatism triggered by fluids released from dehydrated subducting slab [
40].
In the La/Nb versus La/Ba diagram (
Figure 12a), both the hornblende gabbro and olivine websterite samples from the Chengxuanbei intrusions are concentrated in the field of subduction-metasomatized lithospheric mantle, far from the ocean island basalt (OIB) and depleted mantle (DM) end-members. The La/Nb ratios are mostly concentrated in the range of 1–5, with the La/Ba ratios varying between 0.05 and 0.3. These features are distinct from the typical low La/Nb and high La/Ba characteristics of OIB, as well as the high La/Nb and low La/Ba composition of primitive depleted mantle, clearly indicating that the magma source was not primitive depleted mantle, but rather a lithospheric mantle wedge that had undergone intense fluid metasomatism [
41].
In the Th/Yb versus Ba/La diagram (
Figure 12b), all the sample points plot along the “fluid metasomatism” trend, characterized by significantly elevated Ba/La ratios (5–30) and relatively low Th/Yb ratios (<2). This trend is in sharp contrast to the remarkably increased Th/Yb ratios caused by “sediment input”, further confirming that fluid metasomatism, rather than direct sediment mixing, was the dominant mechanism of source modification [
41]. Subduction fluids not only enriched the large-ion lithophile elements (LILEs), but also selectively extracted elements such as Ba and Th, thus shaping the unique trace element distribution pattern of the Chengxuanbei intrusions.
The Sr-Nd-Hf isotopes provide quantitative constraints on the mantle source affinity. The intrusion has initial
87Sr/
86Sr ratios of 0.7042–0.7057, higher than the typical values of depleted mantle (0.702–0.703); the
εNd(
t) values range from 0.14 to 1.43, lying between those of depleted mantle (
εNd(
t) ≈ +5 to +10) and continental crust (
εNd(
t) ≈ −10 to 0) [
42]. The zircon
εHf(
t) values vary from 2.47 to 3.56, displaying overall weakly depleted mantle signatures.
The isotopic compositions show no strong enrichment signals derived from the ancient enriched lithospheric mantle or melting of subducted sediments [
14,
26], thus ruling out these potential source candidates. Collectively, the parental magma of the Chengxuanbei intrusions originated from a depleted mantle wedge metasomatized by subduction fluids of the Paleo-Asian Ocean. These subduction fluids carried large-ion lithophile elements and fluid-mobile elements into the mantle wedge, lowering the mantle solidus and triggering partial melting, and finally generating mafic–ultramafic magmas with island arc geochemical affinities [
2,
10].
The melting pressure and residual mineral phases of the mantle source can be effectively distinguished via rare earth element (REE) partitioning diagrams. Melting within the garnet stability field (>70–80 km) results in significant enrichment of heavy rare earth elements (HREEs, e.g., Yb, Tb), whereas melting in the spinel stability field (<70–80 km) preserves relatively flat HREE patterns [
43].
In the (La/Sm) versus (Sm/Yb) diagram (
Figure 13a), all the samples from the Chengxuanbei intrusion plot within the field of spinel lherzolite, with the (Sm/Yb) ratios concentrated between one and three. They are far from the garnet lherzolite field ((Sm/Yb) > 5) and show a clear contrast with the garnet field samples from the Tarim Large Igneous Province. This feature clearly indicates that the residual phase during mantle melting was dominated by spinel, corresponding to a shallow melting depth.
In the (La/Sm) versus (Tb/Yb) diagram (
Figure 13b), all the samples fall within the spinel stability field, with the (Tb/Yb) ratios ranging from one to two, far below the threshold of (Tb/Yb) > 2 for the garnet stability field (equivalent to depths >70–80 km). This further confirms that mantle melting occurred in the spinel stability field rather than the deeper garnet stability field.
The partition coefficient of Ca in olivine is extremely sensitive to the water content of magmas: low Ca concentrations generally indicate high initial water contents in mantle-derived magmas, because H
2O significantly reduces the partition coefficient of Ca between olivine and melt, thereby retaining more Ca in the melt [
44]. In the Fo vs. Ca diagram (
Figure 14), the olivine grains from the olivine websterite of the Chengxuanbei intrusion exhibit two key characteristics: (1) their Fo values are tightly clustered between 79.8 and 81.0, indicating crystallization from a magnesian basaltic primary magma without extreme differentiation; and (2) their Ca contents are extremely low (<300 ppm), markedly lower than those of mantle olivine (Fo > 90, Ca > 1000 ppm). These features are nearly identical to those of the neighboring Chengxuan mafic–ultramafic intrusion [
45]. Together with the samples from the Luotuoshan and Xinandong intrusions in the region, they plot within the island arc basalt field, in marked contrast to the high-Ca signature of the ~280 Ma Tarim ultramafic rocks.
6.1.3. Magmatic Evolution
The Chengxuanbei intrusion underwent magmatic evolution dominated by fractional crystallization and cumulus processes. The major element covariations, mineral chemistry, and petrographic evidence collectively constrain a clear evolutionary path.
The major element covariations show that SiO
2, Al
2O
3, and CaO exhibited strong negative correlations with MgO, whereas FeOᵀ displayed a positive correlation with MgO (
Figure 8). These trends are consistent with the early fractional crystallization of olivine and clinopyroxene from mantle-derived mafic magmas [
48,
49]. As a relatively primitive lithology, the olivine websterite contains high MgO contents (18.57%–28.86%), accompanied by elevated Cr and Ni abundances. In contrast, the hornblende gabbro and gabbro show markedly decreased MgO and increased SiO
2 and Al
2O
3, reflecting prolonged fractional crystallization and magmatic evolution toward Si- and Al-enriched compositions.
The mineral chemistry reveals the comprehensive crystallization sequence. The olivine exhibits homogeneous compositions, with Fo values clustered at 79.8–81.0 and Ni contents of 573 ppm–1320 ppm. The absence of coupled decreases in Fo and Ni caused by extreme differentiation indicates a moderate fractional crystallization intensity [
27,
28]. The clinopyroxene is predominantly diopside, characterized by a restricted compositional range (Mg
# = 86–88; Wo = 3.2–3.5; En = 80.4–81.6) and tight clustering in the Wo-En-Fs classification diagram (
Figure 7). This suggests stable physicochemical conditions during crystallization and high magma–mineral equilibrium [
30,
50]. The petrographic observations reveal that the intrusions are dominated by massive structures with gradational contacts between lithologies, lacking typical layered cumulate textures. This indicates that major differentiation occurred in a deep magma chamber, followed by rapid emplacement.
The high-field-strength element tectonic discrimination diagrams show that the samples strictly fall within the island arc calc-alkaline basalt field (
Figure 15), further indicating that the magma preserved geochemical fingerprints of a subduction-metasomatized source during fractional crystallization without significant intraplate overprinting [
40,
51]. Combined with the whole-rock rare earth and trace element patterns, magmatic evolution was dominated by the crystallization sequence olivine → clinopyroxene → plagioclase → hornblende, accompanied by weak-to-moderate alterations, such as chloritization, serpentinization, and uralitization, which did not modify the major evolutionary trend. Overall, the Chengxuanbei intrusions are characterized by moderate fractional crystallization and rapid emplacement, representing a typical evolutionary model for mantle-derived mafic magmas in orogenic belts [
9,
12].
6.1.4. Crustal Contamination
Crustal contamination is a key mechanism controlling sulfide saturation and Cu-Ni mineralization in magmatic systems [
53,
54]. The Chengxuanbei intrusion exhibits significant crustal contamination characteristics in terms of major elements, trace elements, Sr-Nd-Hf isotopes, and sulfur isotopic compositions.
In terms of major elements, from the olivine websterite to the hornblende gabbro, the MgO content decreases rapidly, while SiO
2 and Al
2O
3 increase synchronously (
Figure 8a,b), which is consistent with the typical geochemical trends of silicic crustal contamination. Regarding the trace elements, the clear negative anomalies of Nb-Ta and Zr-Hf cannot be explained solely by their source characteristics; the contents of crustal-enriched elements, such as Rb, Ba, and Th, are significantly higher than those of primitive mantle-derived magmas. The sensitive element ratios, such as Ce/Nb versus Th/Nb, Th/Yb versus Ta/Yb, and Th/Zr versus La/Yb, exhibit clear linear correlations (
Figure 16), unequivocally indicating assimilation of crustal material during magma ascent [
54,
55],This is similar to the characteristics of the Qixin Cu-Ni deposit in Beishan, Xinjiang (
Figure 16).
To further quantitatively constrain the intensity of crustal contamination, a two-component binary mixing model was established using a diagram of (
143Nd/
144Nd)
i versus La/Sm (
Figure 16f). This mixing model employed two geochemically constrained end-members, following the classical mass balance binary mixing theory [
56]: a primary mantle-derived magma end-member and a Beishan continental crust end-member. The primary magma end-member was defined based on the least-contaminated olivine websterite samples from the Chengxuanbei intrusion, characterized by an initial
143Nd/
144Nd ratio of ~0.51259 and a low La/Sm ratio. The continental crust end-member adopted the average composition of Paleozoic continental crust in the southern Beishan orogen, featuring a low initial
143Nd/
144Nd ratio (~0.5095–0.5105) and a relatively high La/Sm ratio [
57]. In the modeling, the rare earth elements La and Sm were assumed to behave as typical incompatible elements with stable bulk partition coefficients during the mixing process, without significant geochemical fractionation induced by fractional crystallization [
58]. The theoretical mixing curve was calculated using the standard binary mixing equation, and a least squares optimization was applied to fit the curve to the geochemical data points, achieving an optimal match between the theoretical trend and the measured samples [
59]. All the sample points fell along the theoretical mixing trend, indicating that the Chengxuanbei magma experienced limited crustal contamination.
Figure 16.
Crustal contamination discrimination diagrams for the Chengxuanbei mafic–ultramafic intrusion ((
f) modified after [
42], Qixin data are from [
60]). (
a) Th/Nb vs. Ce/Nb; (
b) Ta/Yb vs. Th/Yb; (
c) Nb vs. Th; (
d) Th/Zr vs. La/Yb; (
e) La/Yb vs. Ce/Yb; (
f) (
143Nd/
144Nd)i vs. La/Sm isotopic variation diagram, where the black squares represent the crustal contamination trend with contamination percentages labeled.
Figure 16.
Crustal contamination discrimination diagrams for the Chengxuanbei mafic–ultramafic intrusion ((
f) modified after [
42], Qixin data are from [
60]). (
a) Th/Nb vs. Ce/Nb; (
b) Ta/Yb vs. Th/Yb; (
c) Nb vs. Th; (
d) Th/Zr vs. La/Yb; (
e) La/Yb vs. Ce/Yb; (
f) (
143Nd/
144Nd)i vs. La/Sm isotopic variation diagram, where the black squares represent the crustal contamination trend with contamination percentages labeled.
The Sr-Nd-Hf isotopes provide robust constraints on crustal contamination. The increase in the initial
87Sr/
86Sr ratios and decrease in the
εNd(
t) values show a negative correlation (
Figure 10), representing a typical crust–mantle mixing trend. The zircon ε
Hf(
t) values are lower than those of weakly contaminated mantle-derived intrusions and show a weak coupling with the whole-rock Nd isotopes, indicating that contamination persisted throughout magma evolution [
24,
25]. The Sr-Nd isotopic modeling based on La/Sm versus the initial
143Nd/
144Nd indicates that the Chengxuanbei intrusion was contaminated by crustal material, a feature consistent with those of known mineralized intrusions in the southern Beishan belt [
5,
61].
The sulfur isotopes provide direct evidence for the addition of crustal sulfur. The whole-rock δ
34S values of the intrusion range from 3.7‰ to 6.5‰ (average 5.1‰), which are higher than those of primitive mantle sulfur (0‰ ± 3‰) and MORB sulfur (−1.28 ± 0.33‰). These values overlap with the δ
34S range of Paleozoic crustal sulfides in the Beishan area (0‰ to +6‰) [
62], suggesting that the magma assimilated sulfur-bearing crustal strata [
37,
53]. No significant variation in sulfur isotopes is observed among the different lithofacies, implying that the addition of crustal sulfur likely occurred early in the magma evolution, broadly contemporaneous with crustal contamination, thus providing a material prerequisite for subsequent sulfide saturation. However, the average δ
34S value of the Chenxuanbei intrusion (5.1‰) appears slightly higher than the δ
34S values reported for other Beishan areas (as illustrated in
Figure 11b, where the values mostly fall between −3‰ and 2‰). This may indicate that the Chenxuanbei mafic–ultramafic intrusion experienced a relatively higher degree of crustal contamination. Although crustal contamination is the most plausible explanation, the δ
34S values (3.7–6.5‰) are higher than typical crustal sulfur values in the Beishan Paleozoic strata (0 to +2‰, [
63]). This may indicate assimilation of marine sulfate-bearing sediments (e.g., evaporites or carbonate-hosted sulfates), which are known to occur in the Devonian–Carboniferous sequences of the Beishan region. Alternatively, fractional degassing of SO
2 from a moderately oxidized magma could have also produced heavy δ
34S in residual sulfide melts. Further in situ S isotope analyses of individual sulfide minerals are needed to resolve this.