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Article

Cogenetic Origin of Magmatic Enclaves in Peralkaline Felsic Volcanic Rocks from the Sanshui Basin, South China

1
School of Civil and Hydraulic Engineering, Xichang University, Xichang 615013, China
2
School of Ocean Science, China University of Geosciences, Beijing 100083, China
*
Authors to whom correspondence should be addressed.
Minerals 2023, 13(5), 590; https://doi.org/10.3390/min13050590
Submission received: 22 March 2023 / Revised: 21 April 2023 / Accepted: 21 April 2023 / Published: 24 April 2023
(This article belongs to the Section Mineral Geochemistry and Geochronology)

Abstract

:
Centimeter-scale magmatic enclaves are abundant in peralkaline felsic volcanic rocks in the Sanshui Basin. Their lithology is mainly syenite and syenitic porphyry, and they mainly comprise alkali feldspar and amphibole, which is similar to the mineral assemblage of the host trachyte and comendite. The SiO2 content in the syenitic enclaves is ~63 wt%, which is similar to that of the host trachyte but lower than that of the comendite. Thermobarometric calculations showed that the syenitic enclaves crystallized at similar temperature and pressure conditions as their host trachyte. The results of mass-balance modeling and MCS modeling indicate that the syenitic enclaves likely experienced an approximately 74% fractional crystallization from the basaltic parental magma. Combined with the similar mineral assemblages and geochemical characteristics of the host trachyte, we think that the enclaves resulted from the in situ crystallization of trachytic magma in the shallow crust and that they had a cogenetic origin with their host volcanic rocks, which means that they were likely to derived from the identical magma chamber which was formed from different batches of magma mixing/mingling. The recharge and mixing of basaltic magma triggered the eruption of trachytic magma eruption. The syenitic crust may have been disaggregated by the ascending trachytic magma and brought to the surface as syenitic enclaves. The syenitic enclaves in volcanic rocks provide unique information on the magmatism of the shallow crust as evidence of magma mixing/mingling.

1. Introduction

Magmatic enclaves are widely recognized in both the plutonic and volcanic rocks [1]. Magmatic enclaves commonly found in calc-alkaline granites have been generically referred to as mafic microgranular enclaves (MMEs) to constrain the origin and evolution of the magma and crust-mantle interaction [2,3]. Although magmatic enclaves have been frequently studied, their origin is debated [2,4,5]. Their main sources include: (1) more mafic magma blobs mixed with felsic magma [1,2,6,7], (2) restitic enclaves formed by crustal remelting [8,9,10], (3) cumulated crystals of early minerals in the magma chamber [11,12,13], (4) rapidly cooling crystalline phases at the margins of magma conduits, and (5) trapped xenoliths [14,15]. The magma mixing/mingling model is the best model and indicates a crust–mantle interaction [4,6,16]. Fewer magma enclaves are present in volcanic rocks than in plutonic rocks; however, magmatic inclusions are also prevalent in some volcanic rocks [17,18,19,20,21,22,23,24,25,26], especially alkaline volcanic rocks [27,28,29,30,31,32,33,34,35,36,37,38]. Volcanic eruptions triggered by magmatism brought plutonic and subvolcanic samples to the surface, and these enclaves provide rich geological information and can study the deep earth [29,33,37]. The petrological, geochemical, and mineralogical characteristics of these enclaves provide unique information that can reveal the magmatic process of the shallow magma chamber.
For this study, the whole rock major, trace elements, and mineral chemistry of the syenitic enclaves commonly found in trachyte and comendite in the Sanshui Basin were investigated, whereby we conducted thermobarometric calculations and a thermodynamic model to explore the origin and petrogenesis of the syenitic enclaves, relationship with host trachyte and comendite, and constrained the magmatic process in the Sanshui Basin.

2. Geological Background

The Sanshui Basin is located at the margin of the South China Block (Figure 1a) and is constrained by the NE-trending Sihui–Wuchuan Fault, NW-trending Gangyao–Shawan Fault, and Xijiang Fault, and is shaped like a rhombus extending north-south with an area of approximately 3300 km2 [39]. The basin is underlain by the Hercynian-Indosinian folded zone [40]. Because the area is influenced by the far-field effect of the subduction of the Paleo–Pacific and the Neo–Tethys plates [41], this region has been in an extensional setting and has formed the rift basin since the Late Cretaceous [42], and, ultimately, the continental lithosphere ruptured under the Sanshui Basin in the Cenozoic [43].
From the Late Cretaceous to the Eocene (64–38 Ma), there were a total of 13 volcanic cycles and 123 eruptions occurred in the Sanshui Basin, and the thickness of the volcanic stratigraphy exceeded 2700 m [39]. These volcanic rocks are distributed in the center of the basin, with a north–south distribution of approximately 45 km and a bimodal volcanic assemblage dominated by trachyte and comendite in volume (whose total eruption thickness exceeds 1000 m and surface exposure area exceeds 14 km2), followed by basaltic rocks. Based on the spatial distribution of trachyte and comendite, the Sanshui basin is divided into the Shiling cluster and the Xiqiao cluster (Figure 1b). The Cenozoic volcanic eruptions recorded in the Sanshui Basin occurred from 64 Ma to 38 Ma, but the main eruption period occurred from 53 Ma to 56 Ma [41]. The trachyte and comendite formed via protracted fractional crystallization (with insignificant crustal contamination) during the ascend of the basaltic magma into the crust [39,44].

3. Materials and Methods

We analyzed five syenitic enclaves collected from the Sanshui Basin, and our analysis included a major element and trace element analysis of the whole-rock and mineral chemical analysis.
The syenitic enclaves were crushed into approximately 200 mesh powders in an agate mill. The whole-rock major and trace element concentrations were obtained by using X−ray fluorescence (XRF) and inductively coupled plasma mass spectrometry (ICP−MS) at the ALS laboratory, Guangzhou. The major elements analyzed had analytical uncertainties of <5%. The trace elements were separated using cation-exchange techniques before running the ICP−MS analysis. The analytical uncertainties were estimated at 10% for the elements with abundances <10 ppm, and ~5% for those with abundance >10 ppm.
The mineral compositions in the syenitic enclaves were measured with a FE-EPMA (JEOL JXA-8530F Plus, Tokyo, Japan) equipped with five wavelength-dispersive spectrometers and an energy-dispersive spectrometer (EDS, OXFORD INSTRUMENTS X-MAX 20, Abingdon, UK) at the State Key Laboratory of Nuclear Resources and Environment, East China University of Technology, China. The accelerating voltage, beam current, and beam size were operated at 15 kV, 20 nA, and 1 μm, respectively. The peaks and backgrounds for P, Ti, Nb, Ta, Zr, Hf, U, Th, REEs, and Y were measured with counting times of 20 s and 10, and those for Si, Al, Mg, Ca, Mn, Fe, Na, and F were measured with counting times of 10 s and 5 s. All the data were corrected by using standard ZAF correction procedures. The analytical uncertainties were <1% for the major elements.

4. Results

4.1. Petrography

Syenitic enclaves are mainly found at Zoumaying, Libian (Figure 2b), and Zizhugang in the Shiling cluster and are generally between 1–5 cm in size. These enclaves are usually dark gray in color and thus have clear boundaries with a blue–green and purplish–red host rock. The magmatic enclaves exhibit a typical igneous texture and can be divided into medium-fine-grained syenite and syenite porphyry according to the texture; additionally, the main mineral assemblage is alkali feldspar and amphibole with minor clinopyroxene. alkali feldspar is the predominant mineral, up to 5 mm in size, with a transparent (fresh) –white color (altered), while amphibole is fine–grained and dark–green color.
The medium-fine-grained syenite has a granular texture and consists of a large amount of alkali feldspar (>85 vol%) followed by minor amounts of sodium amphibole (4–8 vol%), clinopyroxene (<3 vol%), quartz (<3 vol%), and accessory minerals including Ti-Fe oxides, apatite, monazite, haleniusite, and zircon (Figure 3). The alkali feldspars phenocrysts are euhedral–subhedral with a slight alteration. The clinopyroxenes are subhedral–anhedral and are up to 7 mm in the 20ss022-1, whereas the sodium amphibole, quartz, and other accessory minerals are anhedral and filled in the alkali feldspar crystal framework.
The syenite porphyry has a porphyroid texture, and the phenocryst mineral is dominated by alkali feldspar, which is generally 3–7 mm in size and about 12 vol% in content. The groundmass minerals are dominated by microcrystalline alkali feldspar, Ti-Fe oxides, and sodium amphibole, with small amounts of apatite and zircon as accessory minerals.
The magmatic enclave host rocks are trachyte and comendite, both of the fresh host rocks are gray–green with a porphyritic structure, the phenocryst minerals are dominated by alkali feldspar, and the trachytes have 6–24 vol% phenocryst, whereas the comendites have 1–7 vol% phenocryst and are generally brick-red due to oxidation.

4.2. Whole-Rock Geochemistry

The whole-rock geochemical composition of the syenitic enclaves are shown in Table 1 and Table 2. The syenitic enclaves had a high loss on ignition (LOI, 1.03–1.71 wt%), and the high LOI may have been caused by the later alteration that resulted in low Na2O content [45] which was also observed in the host rocks [41]. Therefore, the Na2O concentration of syenitic enclaves was corrected using the method recommended by White [45]. A plot of FK/A vs. P.I. (FK/A = (Fe + K)/Al, mol, with all Fe calculated as Fe2+, P.I. = (Na + K)/Al, mol) was presented in Figure 4a, enclaves from 19ss036-1 and 19ss037-1 lied below the 95% confidence interval and demonstrated the Na2O loss. The Na2O-corrected syenitic enclaves showed weakly peralkaline affinity with peralkaline index (P.I.) = 1.00–1.08.
The major elements of the syenitic enclaves were similar to those of the trachyte exposed in the Sanshui Basin; they had high alkali content (Na2O*+K2O = 11.93–12.27 wt%), low MgO content (0.14–0.32 wt%), and low CaO (0.62–0.86 wt%), but the SiO2 content was restricted (<1 wt% variation). All of the syenitic enclaves fell in the field of alkaline feldspar syenite field based on petrographic observation (Figure 4b) and plotted in the syenite field according to the classification (Figure 4c). The syenitic enclaves were ferroan with a Fe/Fe+Mg value ranging 0.92 to 0.95, and alkaline with a MALI index (Na2O+K2O-CaO) range 11.40 to 11.61, corresponds to the A-type granite [48].
Compared with the host rocks or other peralkaline felsic volcanic rocks in the Sanshui Basin, the variation of in the trace elements in the syenitic enclaves was restricted. The primitive mantle normalized pattern (Figure 5a) showed that all syenitic enclaves had enriched in high field strength elements (HFSE, such as Zr, Hf, Nb, and Ta) and were depleted in Ba, Sr, P, Eu, and Ti, which indicated the fractional crystallization of plagioclase, alkali feldspar, apatite, and Fe–Ti oxides during the magmatic evolution process, which was similar to what occurred with the host rocks. The chondrite normalized rare earth element pattern (Figure 5b) showed that the syenitic enclaves in the Sanshui Basin were characterized by moderate LREE enrichment relative to HREE, with (La/Yb)N ratios of 12.3–19.8, negative Eu anomalies (Eu/Eu* = 0.16–0.21) and various Ce anomalies (Ce/Ce* = 0.37–1.30), which was considered to be the result of hydrothermal alteration [41,49].
Table 2. Trace elements composition of the syenitic enclaves of the Sanshui Basin.
Table 2. Trace elements composition of the syenitic enclaves of the Sanshui Basin.
Sample19ss036-119ss037-2a19ss037-2b20ss020-120ss022-119ss036-120ss020-120ss022-1Kilombe,
Kenya
Azores,
Portugal
Rock TypeSyeniteSyeniteSyeniteSyeniteSyeniteTrachyteComenditeTrachyteSyenite,
n = 20
Syenite,
n = 17
GroupEnclaveEnclaveEnclaveEnclaveEnclaveHostHostHostEnclaveEnclave
Ba98.0065.2075.6088.1072.3040.9061.1019.7048.7061.00
Be4.514.193.974.114.626.227.697.91 4.11
Co0.601.001.000.800.9021.400.300.60 4.16
Cr111111.332
Cs0.582.602.350.521.670.812.982.560.911.44
Ga40.7041.9040.6039.1039.8046.9050.7045.3035.5529.57
Hf21.2023.1020.8020.1020.4042.5052.1025.0014.4025.36
Nb188177166179176272336164195217
Ni0.50.30.30.50.40.81.21.8
Pb10.009.2012.409.3010.8019.5013.6010.40
Rb166219193160188229306176137186
Sr22.8016.2016.0019.8021.109.0314.507.2011.8579.15
Ta9.5011.609.509.109.9017.4020.909.4011.5713.67
Th19.3522.3021.4018.2023.3036.9049.5019.4518.3125.64
U3.252.742.333.012.455.165.203.545.037.97
V17561481.332.01.0 35.75
Zr9729978839039131834236011905581119
Y96948592901652051714456
La245183155215204227439416145157
Ce313130398301170267167723175292
Pr54373350394782912430
Nd19112811617312816729731581103
Sm32.5020.8019.1029.3020.1032.3057.3059.0011.9116.04
Eu1.791.051.171.661.291.183.105.461.341.62
Gd24.7018.0016.1022.9015.9727.7049.3045.4010.0413.27
Tb3.623.002.693.352.635.467.236.971.422.04
Dy20.1018.2015.9518.8015.8729.2038.3035.308.1911.21
Ho3.533.473.103.283.035.717.016.391.592.11
Er9.6610.058.988.918.7716.5019.0016.804.826.21
Tm1.351.481.341.281.372.922.722.380.890.94
Yb8.889.999.028.218.9417.8017.6014.656.156.27
Lu1.281.471.311.181.302.422.522.201.020.93
LaN/YbN19.7913.1012.3318.7816.379.1517.8920.3716.8917.99
Ce/Ce*0.640.371.300.690.440.600.200.870.660.97
Eu/Eu*0.190.160.200.190.210.120.170.310.360.33
Nb/U5864715972536546
Ce/Ce* = 2CeN/(LaN + PrN), Eu/Eu* = 2EuN/(SmN + GdN), normalized from [50].

4.3. Mineral Geochemistry

We performed a mineral chemical analysis on the syenitic enclaves and the results are listed in the Table 3, Table 4 and Table 5.
Alkali feldspars were mainly classified as sanidine and anorthoclase (Figure 6a) with An0–6Ab53–74Or22–44. The absence of an obvious zoned texture and the relatively stable composition of the alkali feldspars (Or variation < 5) indicated that they were in equilibrium with the host melt. The An content of alkali feldspars exhibited low (An = 0–6), and the Or values of the alkali feldspars in the syenitic enclaves hosted in the comendite varied more than in the trachyte (Table 3).
Figure 6. Mineral compositions of the syenitic enclaves. (a) Feldspar composition plotted into the ternary An-Ab-Or system, isotherm lines are from [51]; (b) clinopyroxene composition plotted into the Wo-En-Fs system after [52]; (c) sodium-calcium amphibole composition plotted in scheme diagram; (d) sodium amphibole composition plotted in scheme diagram after [53], B(Ca+Σ2+): Sum of Ca2+, Fe2+, and Mg2+ cations at B site in amphibole, ΣB: Sum of total cations at B site in amphibole.
Figure 6. Mineral compositions of the syenitic enclaves. (a) Feldspar composition plotted into the ternary An-Ab-Or system, isotherm lines are from [51]; (b) clinopyroxene composition plotted into the Wo-En-Fs system after [52]; (c) sodium-calcium amphibole composition plotted in scheme diagram; (d) sodium amphibole composition plotted in scheme diagram after [53], B(Ca+Σ2+): Sum of Ca2+, Fe2+, and Mg2+ cations at B site in amphibole, ΣB: Sum of total cations at B site in amphibole.
Minerals 13 00590 g006
Table 3. Electron microprobe analyses of alkaline feldspar for the syenetic enclaves in the Sanshui Basin.
Table 3. Electron microprobe analyses of alkaline feldspar for the syenetic enclaves in the Sanshui Basin.
Point036-2-1036-2-2036-2-3036-2-4036-2-5022-2-1022-2-2022-2-3022-2-4020-2-1020-2-2020-2-3020-2-4020-2-5020-2-6
SiO266.7767.4966.9565.8766.6067.7667.2768.4065.3666.8366.4666.8367.8167.6966.95
TiO20.050.020.020.050.030.060.040.020.070.040.110.000.050.130.06
Al2O318.4718.5718.8218.8719.3218.4918.7417.7018.8419.6018.7017.8418.1618.4917.84
FeOt0.180.420.260.200.230.370.150.270.420.320.140.920.260.230.26
MnO0.010.010.030.000.00-0.030.000.000.000.020.000.020.000.01
CaO1.190.180.120.760.440.340.700.250.560.860.680.000.270.710.66
Na2O6.896.856.937.597.967.466.938.188.458.906.966.448.328.266.32
K2O5.495.677.275.825.605.895.165.455.554.136.807.845.424.817.88
Total99.0499.21100.4199.16100.17100.3999.01100.2799.25100.6899.8799.86100.31100.3199.97
Formulae on basis of 8 oxygens
Si3.0033.0222.9932.9732.9713.0123.0133.0392.9572.9562.9853.0173.0163.0043.015
Ti0.0020.0010.0010.0020.0010.0020.0010.0010.0020.0010.0040.0000.0020.0040.002
Al0.9790.9840.9921.0041.0160.9690.9890.9271.0041.0220.9900.9490.9520.9670.947
Fe3+0.0070.0160.0100.0080.0090.0140.0060.0100.0160.0120.0050.0350.0100.0090.010
Mn0.0010.0000.0010.0000.0000.0000.0010.0000.0000.0000.0010.0000.0010.0000.000
Ca0.0570.0080.0060.0370.0210.0160.0340.0120.0270.0410.0330.0000.0130.0340.032
Na0.6000.5980.6000.6650.6880.6430.6020.7050.7410.7640.6060.5630.7180.7110.552
K0.3150.3250.4140.3350.3190.3340.2950.3090.3200.2330.3890.4510.3070.2720.453
total4.9644.9555.0175.0225.0244.9904.9405.0035.0685.0285.0145.0155.0185.0005.011
An611422413430133
Ab626459646765656968745956697053
Or323541323134323029223844302744
T872877866877883891890899898871841834862864828
An = Ca/(Ca+Na+K) × 100, Ab = Na/(Ca+Na+K) × 100, Or = K/(Ca+Na+K) × 100. T = thermometeric calculations based on [54], T is in °C.
Table 4. Electron microprobe analyses of clinopyroxenes and thermobarometric calculations for the syenetic enclaves in the Sanshui Basin.
Table 4. Electron microprobe analyses of clinopyroxenes and thermobarometric calculations for the syenetic enclaves in the Sanshui Basin.
Piont022-1022-2022-3022-4022-5022-6036-1036-2036-3036-4036-5036-6036-1
SiO248.9149.3849.1548.1449.4549.6549.5849.8849.8748.9749.7749.8851.03
TiO20.590.510.490.560.600.480.340.330.440.520.390.290.03
Al2O30.390.330.320.320.510.420.310.350.320.320.390.360.16
FeO20.9721.4921.8922.5519.7822.1520.6721.1521.3522.5722.1920.8733.64
MnO0.840.910.980.890.820.920.870.940.920.900.980.832.04
MgO6.976.416.845.777.125.467.056.426.335.635.616.760.01
CaO21.0020.0119.9820.9520.4719.8320.1520.3819.7820.3019.5320.451.01
Na2O0.390.410.430.380.370.620.460.580.440.430.500.5411.39
Total100.0599.45100.0899.5699.1499.5299.44100.0399.4499.6499.3699.9799.31
Formulae on basis of 6 oxygens
Si1.9451.9721.9561.9421.9671.9851.9731.9771.9861.9651.9911.9762.121
Ti0.0180.0150.0150.0170.0180.0140.0100.0100.0130.0160.0120.0090.001
Al0.0180.0160.0150.0150.0240.0200.0150.0160.0150.0150.0190.0170.008
Fe3+0.1290.0630.1150.1430.0520.0430.0810.0790.0300.0830.0220.0840.922
Fe2+0.5610.6510.6070.6090.6030.6950.6020.6180.6800.6690.7200.6020.157
Mn0.0280.0300.0330.0310.0280.0310.0290.0310.0310.0310.0330.0280.072
Mg0.4130.3800.4060.3470.4220.3250.4180.3800.3760.3370.3350.3990.000
Ca0.8950.8530.8520.9050.8720.8490.8590.8660.8440.8730.8370.8680.045
Na0.0300.0320.0330.0300.0290.0480.0360.0440.0340.0330.0380.0420.917
Total4.0364.0124.0324.0394.0154.0124.0234.0224.0084.0234.0064.0234.243
Wo4544434545444445444444444
En2120201722172120191717200
Fs35373638343935363738393596
T1-----880--898-880--
P10.610.720.670.890.531.140.320.230.290.360.580.20-
T2867869867867888867869867875867870883-
P21.281.501.501.501.501.131.331.031.171.251.251.07-
T3936938935925940925877875875867869876-
P3222222222222-
Wo = Ca/(Ca + Mg + Fe) × 100, En = Mg/(Ca + Mg + Fe) × 100, Fs = Fe/(Ca + Mg + Fe) × 100. T1 and P1= thermobarometric calculations based on cpx-melt model [55], T2 and P2 = thermobarometric calculations based on cpx-only model [56], T3 and P3 = thermobarometric calculations based on cpx-melt model [56], T is in °C and P is in kbar.
Table 5. Electron microprobe analyses of amphibole for the syenetic enclaves in the Sanshui Basin.
Table 5. Electron microprobe analyses of amphibole for the syenetic enclaves in the Sanshui Basin.
Point022-1-1022-1-2022-1-3022-1-4036-1-1036-1-2036-1-3036-1-4037-1-1037-1-2037-1-3037-1-4037-1-5
SiO249.7550.3848.9349.6349.9649.2548.2749.7248.6748.8849.5050.1449.08
TiO20.300.941.010.670.781.130.600.700.470.650.740.640.76
Al2O30.190.390.490.560.330.490.370.530.540.620.450.460.59
FeOt34.5035.5633.9834.1534.1333.5735.8334.2435.2135.9934.6934.4534.11
MnO1.291.061.201.171.371.171.070.901.080.880.921.161.19
MgO0.130.110.210.250.270.290.190.270.310.270.290.300.28
CaO1.722.952.732.692.192.322.352.672.662.651.892.082.68
Na2O6.336.145.826.576.287.376.166.656.336.007.146.777.39
K2O1.321.301.341.371.331.371.331.341.331.301.351.361.36
F2.051.331.431.391.671.210.982.151.901.691.591.761.92
Cl0.030.050.030.090.060.050.020.050.040.070.060.050.07
Total96.7399.6696.5797.9497.6497.7196.7698.3097.7398.2697.9398.4298.60
Formulae on basis of 23 oxygens
Si7.8267.7917.7237.7517.8067.7077.6427.7707.6647.6777.7477.8007.673
Al0.1370.1500.2370.1970.1470.2350.3250.1760.2990.2830.1990.1460.274
Ti0.0110.0450.0230.0380.0270.0480.0160.0370.0150.0220.0410.0360.037
T.sum7.9747.9867.9837.9867.9807.9917.9837.9837.9787.9817.9877.9827.984
Al0.0000.0000.0000.0000.0000.0000.0000.0000.0000.0000.0000.0000.000
Ti0.0240.0640.0970.0410.0650.0850.0560.0450.0410.0550.0460.0390.052
Fe3+1.2041.0711.1211.0871.1671.0831.2330.9991.1751.1281.0791.1141.109
Mn2+0.1440.1240.1360.1370.1530.1400.1220.1070.1240.1010.1110.1340.141
Mg0.0290.0260.0500.0580.0640.0690.0440.0640.0730.0630.0680.0700.065
Fe2+3.3403.5403.3603.4343.3213.3973.4223.5293.4383.5143.4743.4083.448
C.sum4.7414.8264.7644.7584.7694.7744.8774.7434.8524.8614.7784.7644.816
Mn2+0.0280.0150.0250.0180.0270.0150.0210.0120.0210.0160.0120.0190.016
Fe2+0.0000.0000.0050.0000.0000.0000.0880.0000.0240.0840.0000.0000.000
Ca0.4440.6000.6030.5790.5010.5240.5510.5790.5890.5820.4610.4780.578
Na1.5681.4261.4331.5331.5321.6441.4091.5271.4271.3521.5991.5781.597
B.sum2.0402.0412.0652.1302.0602.1832.0692.1182.0602.0342.0722.0742.192
Na0.3640.4140.3480.4550.3710.5920.4820.4880.5050.4740.5660.4620.642
K0.2750.2630.2780.2790.2750.2780.2760.2730.2750.2680.2750.2770.278
A.sum0.6390.6780.6260.7350.6460.8710.7580.7610.7800.7420.8410.7390.919
F0.9120.5870.6360.6180.7390.5430.4340.9720.8550.7580.7140.7820.869
Cl0.0070.0130.0070.0210.0160.0120.0050.0130.0100.0170.0140.0130.018
NameArfKtpKtpKtpKtpArfKtpKtpKtpKtpArfArfKtp
T.sum, C.sum, B.sum, A.sum are the sum of cation at T site, C site, B site, and A site, respectively. Arf = Arfvedsonite, Ktp = Katophorite.
Clinopyroxene was only observed in the enclaves (20ss022-1, 19ss036-1), and the clinopyroxenes were characterized by Mg# (Mg/Mg + Fe × 100) = 30–39 and a compositional range of Wo43-45En17-21Fs34-39 with low Na contents (<0.45 apfu, atoms per formula unit), which was similar to the equilibrium clinopyroxenes in the host trachyte [57]. Aegirine observed in the alkaline feldspar framework (Figure 3h) had a composition of Q18Jd0Aeg82, and Na apfu = 0.95.
According to the nomenclature of Hawthorne [53], amphiboles in the syenitic enclaves are classified as sodium-calcium and sodium amphiboles (Figure 6c,d) by using the machine learning method [58]. The amphiboles exhibited higher F concentrations (0.43–0.91 apfu) than the Cl concentrations (<0.021 apfu), and high Fe2+/(Fe2+ + Mg2+) ratios (0.97 to 0.99), which was similar to that of the amphiboles in A-type granite [59].

4.4. Thermobarometeric Calculation

To estimate the syenitic enclaves’ crystallization condition and magmatic evolution, we performed a series of thermobarometric calculations on the syenitic enclaves to determine the magma crystallization condition.
The crystallization temperature of the syenitic enclaves was estimated by using clinopyroxene (cpx)-melt [55,56], cpx-only [56], and alkaline feldspar-melt [54] thermometers. When calculating the values obtained from the cpx-melt thermometer, we used an initial H2O content of 4.5 wt% and pressure of 1.5 kbar, and the calculation results showed that the crystallization temperature ranged from 880 °C to 897 °C. The cpx-melt and cpx-only thermometers, which were based on random-forest machine learning, did not need additional conditions in the calculation [56]; the cpx-only thermometer provided a consistent estimate of 867–888 °C, and cpx-melt thermometer results showed crystallization temperatures ranging 867 °C to 877 °C for 19ss036-1 and exceeding 925 °C for 20ss022-1, which may have been related to the variations of melt composition. Similar results were calculated when using the alkaline feldspar-melt thermometer, with temperatures ranging 872 °C to 883 °C in 19ss036-1, 891 °C to 898 °C in 20ss022-1, and 828 °C to 871 °C in 20ss020-1.
The pressure of the syenitic enclaves were estimated by using cpx-melt [55,56] and cpx-only [56] barometer; the cpx-melt barometric calculations showed crystallization pressures ranged 0.17 to 1.14 kbar, the cpx-only barometric calculations showed a higher pressure of 1.07–1.50 kbar, and the cpx-melt barometer provided an estimate of 2 kbar. The thermobarometric results showed that, assuming a pressure to depth conversion of 2.8 km/kbar, syenitic enclaves crystallized in the shallow crust which were similar to the results of the volcanic rock calculations [57].

5. Discussion

5.1. Geochemical Characterization of the Syenitic Enclaves

The syenitic enclaves in the peralkaline volcanic rocks were ferroan and alkaline, corresponded to the A-type granite [48]; these rocks mainly formed in an extensional tectonic setting [60]. On the Th/Ta vs. Yb diagrams [61], the syenitic enclaves fell in the intraplate volcanic rock field (Figure 7a), which is consistent with the tectonic context of the bimodal volcanic rocks [39,43]. The Rb vs. Ta + Yb [62], (Th/Ta)N vs. (Y/Nb)N [63], and Zr vs. 10,000 Ga/Al [60] diagrams indicated that they formed in an intraplate setting similar to the host trachyte and comendite. The Nb/Y vs. Nb + Y diagram [64] and the Nb-Y-3Ga ternary diagram [60] were clustered in the A1-type rhyolite field, which indicated that they developed in a continental rift tectonic setting. The high FeO and low Al2O3 content in the amphibole also indicated that they formed in anorogenic tectonic setting [65].

5.2. Petrogenesis of the Syenitic Enclaves

The syenitic enclaves had a high Nb/U ratio (Table 2) and Nb-Ta enrichment, which was similar to the characteristics of the basaltic rocks in the Sanshui Basin [39,43]; this indicated that the syenitic enclaves had a genetic relationship with the basaltic rocks. The Pb anomaly was not obvious, which indicated insignificant contamination by the crustal materials [66]. The Ba, Sr, P, Eu, and Ti depletion reflected the fractional crystallization of plagioclase, alkaline feldspar, apatite, and Fe-Ti oxides during the magmatic evolution. In addition, the low concentrations of transition metal elements (Ni, Co, Cr, Sc) also indicated the crystallization of mafic minerals (olivine, clinopyroxene). Therefore, mass-balance and thermodynamic modeling were applied to investigate whether the syenitic composition could be created from the basaltic parental magma via fractional crystallization.
The basalt sample 14ss012-1 [67], which had a higher MgO content (7.35 wt%), was selected as the parental composition for the mass-balance calculation. The mass-balance calculation results showed that the sum of the squared residuals was 0.85 (Table 6), which indicated that syenite can be produced via fractional crystallization. The calculated results indicated that the evolution from 14ss012-1 to 19ss036-1 could be calculated via 74% fractional crystallization of a phase assemblage including olivine (11%), clinopyroxene (14%), plagioclase (39%), apatite (2%), magnetite (5%), and ilmenite (3%). The calculated trace element concentrations were broadly compatible with the results of 74% fractional crystallization of the syenitic enclaves, the diversity in the various trace elements may have been caused by the presence of accessory minerals or alterations (Table 6 and Figure 8).
The parental composition of 14ss012-1 and mineral geochemical composition are from [67], Ol = olivine, Cpx = clinopyroxene, Pl = plagioclase, Ap = apatite, Ilm = ilmenite, Mag = magnetite. Odiff = observed different, Cdiff = calculated different, SSR = the sum of the squared residuals, and Wt% = the weight % of removed phase. Trace element calculation based on the Rayleigh fractionation model, and the mineral partition coefficients were cited from the GERM Database (https://kdd.earthref.org/KdD/ accessed on 20 April 2023) and showed in Table S1.
The thermodynamic magma chamber simulator (MCS) [68] was applied to model the fractional crystallization from the basaltic to syenitic magma. Basalt (17ss060-1, [69]) was selected as the starting composition. The basalt was not primitive [70] due the low Ni (less than 130 ppm), Cr (less than 247 ppm), and Mg# (42–61) [67] content, which indicated that basaltic magma underwent fractional crystallization of olivine and clinopyroxene. The oxygen fugacity of the starting composition was set under the fayalite–magnetite–quartz (FMQ) buffer, the oxygen fugacity of cogenetic trachyte calculated by Chen [41], and the pressure and initial water content were 1 kbar and 0.5–2 wt%, respectively. The liquidus temperature was 1130 °C when the olivine crystallized, followed by plagioclase, clinopyroxene, magnetite, apatite, and ilmenite. The approximate composition range of the syenitic enclave was 880 °C to 930 °C (Figure 9), which corresponded to 64–69 wt% of the total crystalline phase, including olivine (~5 wt%), clinopyroxene (~20 wt%), plagioclase (34–38 wt%), apatite (~0.5 wt%), magnetite (~11 wt%), and ilmenite (~0.5 wt%), which was similar to the major elements mass-balance result, which again indicated the genesis of the fractional crystallization of the syenitic enclaves.

5.3. Origin of the Syenitic Enclaves

The geochemical characteristics of the syenitic enclaves host rocks in the Sanshui Basin suggested that they were produced via prolonging fractional crystallization from the basaltic magma in the shallow crust [39,44]. Many similarities in the geochemical characteristics of the syenitic enclaves and their host rocks existed, this combined with their similar mineral assemblages and mineralogical characteristics demonstrated that the syenitic enclaves were crystallized from the same magma chamber with the peralkaline felsic volcanic rocks, and thus were “cogenetic”. Three models of the magmatic enclaves crystallized from the cogenetic magma are advocated: (1) the cumulated crystals of early minerals [11,13], (2) the injection of cogenetic magma [32], and (3) the fragment of marginal crystalline phases [29,30,37]. The distinctive boundaries, alkali feldspar grain size plunges, fibrous alkaline feldspar, and acicular amphibole were observed at the boundary of the host trachyte/comendite and syenitic enclaves. We think that the syenitic enclaves likely originated from the crystallization of the cogenetic trachytic magma, and the main evidence for this is as follows:
Petrographically, no cumulated and compacted crystal textures of tabular alkali feldspar were observed in the thin sections (Figure 3). Additionally, no glass component was observed in the alkali feldspar framework, but rather anhedral sodium hornblende and aegirine, which indicated that the syenite formed via crystallization or nearly crystallization. Syenitic enclaves are mainly found in trachyte, followed by comendite. Due to the similar crystallization temperature and pressure conditions of syenite and trachyte were estimated [57], if the two types of magmas mix, rocks with different crystallinity are unlikely to form. Thus, the undercooling texture of syenitic enclaves hosted in trachyte (Figure 3c,d) may indicate an earlier interaction with the cold wall-rock rather a trachytic magma injection. Therefore, the syenite enclaves hosted in the trachyte were more likely originated from earlier crystallization prior to the trachytic magma [29,37], the granular and porphyritic structures were probably represented the various temperatures within the magma chamber, and the alkali feldspar in the syenite coursing in a relatively stable temperature and pressure condition compared with the syenite porphyry. If the syenitic magma mixed with the comenditic magma, the hotter syenitic magma injected into the colder comenditic magma, a high degree of undercooling would have led to the undercooling textures in the syenitic enclaves, and this would have led to the buildup of volatiles and second boiling in the comenditic melt [32,71]. As a result, many vesicles and undercooling textures would have been formed in syenitic enclaves as in Pantelleria [32]. However, the magmatic enclaves hosted in both trachyte and comendite in the Sanshui Basin had few vesicles, and the enclaves with an undercooling texture only were observed in the enclaves hosted in trachyte (19ss036, Figure 3c,d). Therefore, we think that the syenitic enclaves may resulted from the in situ crystallization of earlier trachytic magma batches.
Geochemically, the major element and trace element characteristics of the syenitic enclaves were similar to those of the host trachyte; namely, they had a similar SiO2 content as well as trace element and rare earth element normalized patterns. More than 85% alkaline feldspar was in syenitic enclaves, and the negative Eu anomaly would have been insignificant or even positive if these syenitic enclaves had cumulated genesis, the accumulation of alkaline feldspaer would have buffered the negative Eu anomaly [29] owing the higher Eu partition coefficient (KdEuafs/liq = 0.37), compared with Sm (KdSmafs/liq = 0.03) and Gd (KdGdafs/liq = 0.03) [72].However, Eu anomalies of the syenitic enclaves were not significantly correlated with their host rock; the syenitic enclaves exhibited equal and lower Eu anomalies than those of the trachytes in the Sanshui Basin. Therefore, the syenitic enclaves were unlikely to be the cumulated crystal genesis.
Earlier researchers have suggested that syenitic enclaves in alkaline volcanic systems are caused by in situ crystallization [29,30,34,37]. Some researchers describe these cogenetic enclaves as “autoliths” (auto = self, lith = stone) [13,29], whereby the name represents the fact that they have the same origin as the host rock.

5.4. Implications for the Alkaline Volcanic System

The bimodal volcanic rocks in the Sanshui Basin provide a unique opportunity to study the magma plumbing system of alkaline volcanic systems in continental rifts, and studying syenitic enclaves is essential to refine the magma plumbing system.
The clinopyroxene in the basalt suggested the presence of a basaltic magma reservoir that continues from the lower crust to the shallow crust [57]. Both the geochemical and thermometer results indicated that the felsic volcanic rocks and syenitic enclaves were products of the basaltic magma that underwent protracted fractional crystallization in the magma reservoir of the upper crust depths. They had similar mineral assemblages: both were dominated by alkali feldspar, followed by sodium amphibole and clinopyroxene, and minor Ti-Fe oxides. In the deep magma reservoir, the basaltic magma continuously underwent fractional crystallization and evolved to trachytic magma; when a batch of trachytic magma is produced, this trachytic magma is first in situ crystallized on the roof and walls of the magma reservoir as a crust [37], and it simultaneously forms a barrier against the exchange of energy and material between trachytic magma and wall-rocks (Figure 10). The underplated basaltic magma maintained near crystallization and provided materials for the upper magma reservoirs, which allowed the trachytic melt to remain in the shallow crustal reservoir longer and thereby eventually forming the bimodal volcanic rocks [29,37]. Thus, the cogenetic syenitic enclaves and trachyte were formed under different crystallization conditions within the magma reservoir, syenitic enclaves were formed via in situ crystallization on the roof and walls of the magma reservoir where heat and energy were most easily lost, and trachyte and comendite resulted from surface eruptions, which is similar to how the enclaves in the volcanic rocks of the Pantelleria, Azores, and East African rift valleys are formed [30,32,34,35,37] The high Mg# clinopyroxene in host trachyte and the embayed alkali feldspar phenocryst in trachyte and comendite suggest magma recharge [57] and mixing, whereby the injection of basaltic magma triggered local heating and eventually induced a trachytic and comenditic magma eruption, and the ascending trachytic and comenditic magma disaggregated the in situ syenitic crystallized crust, which was brought to the surface as syenitic enclaves.

6. Conclusions

  • The peralkaline felsic volcanic rocks in the Sanshui Basin commonly contain syenite and syenite porphyry enclaves. The petrological, geochemical, and mineralogical characteristics of the syenite and syenite porphyry enclaves indicated that they were cogenetic with the host trachyte and comendite and were formed by the fractional crystallization of the basaltic magma.
  • The syenitic enclaves are the results of in situ crystallization of the trachytic magma in the shallow crust according to the thermobarometric calculation and petrological texture. The recharge of the basaltic magma triggered a trachytic and comenditic eruption, and the ascending trachytic and comenditic magma disaggregated the in situ syenitic crystallized crust which was brought to the surface as syenitic enclaves.

Supplementary Materials

The following supporting information can be downloaded at: https://www.mdpi.com/article/10.3390/min13050590/s1, Table S1: Partition coefficients used for trace element modeling [73,74,75,76,77,78,79,80].

Author Contributions

Conceptualization, P.C. and N.F.; methodology, P.C. and Z.Z.; investigation, P.C. and Z.Z.; resources, N.F.; writing—original draft preparation, P.C.; writing—review and editing, N.F. and B.Q.; visualization, B.Q.; supervision, B.Q.; project administration, N.F.; funding acquisition, N.F. All authors have read and agreed to the published version of the manuscript.

Funding

This research was funded by National Natural Science Foundation of China (No. 41572207) and Fundamental Research Funds for National Universities, Xichang University (No. YBZ202264).

Data Availability Statement

The original contributions presented in the study are included in the article.

Acknowledgments

We are grateful to Yu Zhang, and Yang Liu for their help in the field works. We thank Hui Zhang and Jianbing Duan for help in EPMA analyze at ECUT.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. (a) Distribution map of volcanic basins in the northern continental margin of the South China Sea; (b) geological map of the Sanshui Basin.
Figure 1. (a) Distribution map of volcanic basins in the northern continental margin of the South China Sea; (b) geological map of the Sanshui Basin.
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Figure 2. (a) Simplified geological map of the Shiling cluster; (b) oxidized comendite outcrop in Libian, Western Shiling; (ce) hand specimen photographs of magmatic enclaves. Individual enclaves exhibit distinctive boundaries with host trachyte and comendite.
Figure 2. (a) Simplified geological map of the Shiling cluster; (b) oxidized comendite outcrop in Libian, Western Shiling; (ce) hand specimen photographs of magmatic enclaves. Individual enclaves exhibit distinctive boundaries with host trachyte and comendite.
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Figure 3. Representative photomicrographs of syenitic enclaves, individual enclaves exhibit distinctive boundaries with host trachyte and comendite. (a) the syenite porphyry and host trachyte, 19ss037-1, PPL; (b) the syenite porphyry and host comendite, the dark schlieren is mainly acicular amphibole, 20ss022-1, PPL; (c) the fibrous alkaline feldspar in syenite porphyry indicating high undercooling, 19ss036-1, PPL; (d) same field as (c), CPL; (e) the clinopyroxene in the syenite, the fine-grained alkali feldspar and amphibole indicating a rapid crystallization, 19ss022-1, PPL; (f) same field as (e), CPL; (g) anhedral amphibole fill in the alkali feldspar crystal framework in the sytnite, 14ss003-3, PPL, (h) anhedral aegirine fill in the alkali feldspar crystal framework in the sytnite, 19ss035-1, PPL. Afs, alkali feldspar; Cpx, clinopyroxene; Aeg, aegirine; Arf, arfvedsonite; Ap, apatite; Ti-Fe Oxi, Ti-Fe oxide. PPL = plane polarized light, CPL = crossed-polars light. The red line represents the boundary between the syenitic enclaves and the host rock.
Figure 3. Representative photomicrographs of syenitic enclaves, individual enclaves exhibit distinctive boundaries with host trachyte and comendite. (a) the syenite porphyry and host trachyte, 19ss037-1, PPL; (b) the syenite porphyry and host comendite, the dark schlieren is mainly acicular amphibole, 20ss022-1, PPL; (c) the fibrous alkaline feldspar in syenite porphyry indicating high undercooling, 19ss036-1, PPL; (d) same field as (c), CPL; (e) the clinopyroxene in the syenite, the fine-grained alkali feldspar and amphibole indicating a rapid crystallization, 19ss022-1, PPL; (f) same field as (e), CPL; (g) anhedral amphibole fill in the alkali feldspar crystal framework in the sytnite, 14ss003-3, PPL, (h) anhedral aegirine fill in the alkali feldspar crystal framework in the sytnite, 19ss035-1, PPL. Afs, alkali feldspar; Cpx, clinopyroxene; Aeg, aegirine; Arf, arfvedsonite; Ap, apatite; Ti-Fe Oxi, Ti-Fe oxide. PPL = plane polarized light, CPL = crossed-polars light. The red line represents the boundary between the syenitic enclaves and the host rock.
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Figure 4. (a) FK/A vs. P.I diagram, after [45]. (b) QAPF diagram after [46]: 1, quartz alkaline feldspar syenite; 2, alkaline feldspar syenite, 3, quartz diorite; 4, diorite. (c) R1 vs. R2 classification diagram after [47]: 1, alkaline gabbro; 2, monzo-gabbro; 3, monzonite; 4, monzo−diorite; 5, quartz−monzonite. (d) SiO2 vs. Fe/(FeO+MgO) diagram, after [48].
Figure 4. (a) FK/A vs. P.I diagram, after [45]. (b) QAPF diagram after [46]: 1, quartz alkaline feldspar syenite; 2, alkaline feldspar syenite, 3, quartz diorite; 4, diorite. (c) R1 vs. R2 classification diagram after [47]: 1, alkaline gabbro; 2, monzo-gabbro; 3, monzonite; 4, monzo−diorite; 5, quartz−monzonite. (d) SiO2 vs. Fe/(FeO+MgO) diagram, after [48].
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Figure 5. Primitive mantle normalized trace element distribution patterns (a) and chondrite normalized REE distribution patterns (b) for the syenitic enclaves in the Sanshui Basin. Syenitic enclaves of Kilombe are from [34], and syenitic enclaves of Azores are from [29,30]. Normalized values are from [50].
Figure 5. Primitive mantle normalized trace element distribution patterns (a) and chondrite normalized REE distribution patterns (b) for the syenitic enclaves in the Sanshui Basin. Syenitic enclaves of Kilombe are from [34], and syenitic enclaves of Azores are from [29,30]. Normalized values are from [50].
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Figure 7. Trace element distribution diagrams for syenitic enclaves from the Sanshui Basin. (a) Th/Ta vs. Yb diagram after [61]. (b) Rb vs. Ta + Yb diagram after [62], where WPG = within plate granite, VAG = volcanic arc granite, ORG = ocean ridge granite, and syn-COLG = syn-collision granite. (c) (Th/Ta)N vs. (Y/Nb)N diagram after [63]. (d) Zr vs. 10,000 Ga/Al diagram after [60]. (e) Nb/Y vs. Nb + Y diagram after [64]. (f) Nb-Y-Ce diagram after [60]. A1 field represents mantle-derived granites, A2 field represents crustal-derived granites.
Figure 7. Trace element distribution diagrams for syenitic enclaves from the Sanshui Basin. (a) Th/Ta vs. Yb diagram after [61]. (b) Rb vs. Ta + Yb diagram after [62], where WPG = within plate granite, VAG = volcanic arc granite, ORG = ocean ridge granite, and syn-COLG = syn-collision granite. (c) (Th/Ta)N vs. (Y/Nb)N diagram after [63]. (d) Zr vs. 10,000 Ga/Al diagram after [60]. (e) Nb/Y vs. Nb + Y diagram after [64]. (f) Nb-Y-Ce diagram after [60]. A1 field represents mantle-derived granites, A2 field represents crustal-derived granites.
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Figure 8. Trace elements variation diagrams with fractional crystallization model for the syenetic enclaves from the Sanshui Basin. (a) Nb vs. Sr, (b) Y vs. Th. Circled intervals represent 10% fractionation. Partition coefficients were calculated from Table 6.
Figure 8. Trace elements variation diagrams with fractional crystallization model for the syenetic enclaves from the Sanshui Basin. (a) Nb vs. Sr, (b) Y vs. Th. Circled intervals represent 10% fractionation. Partition coefficients were calculated from Table 6.
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Figure 9. MCS fractional crystallization modeling of basaltic parental composition (17ss060-1) from the Sanshui Basin showing the major oxide element evolution curves under the set condition. The models show the liquid compositions at 10°C intervals at 0.5 wt% H2O (grey triangle), 1 wt% H2O (green circle), and 2 wt% H2O (purple square).
Figure 9. MCS fractional crystallization modeling of basaltic parental composition (17ss060-1) from the Sanshui Basin showing the major oxide element evolution curves under the set condition. The models show the liquid compositions at 10°C intervals at 0.5 wt% H2O (grey triangle), 1 wt% H2O (green circle), and 2 wt% H2O (purple square).
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Figure 10. Schematic model of the magma plumbing system associated with bimodal volcanic rocks in the Sanshui Basin.
Figure 10. Schematic model of the magma plumbing system associated with bimodal volcanic rocks in the Sanshui Basin.
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Table 1. Major elements composition of the syenitic enclaves of the Sanshui Basin.
Table 1. Major elements composition of the syenitic enclaves of the Sanshui Basin.
Sample19ss036-119ss037-2a19ss037-2b20ss020-120ss022-119ss036-120ss020-120ss022-1Kilombe,
Kenya
Azores,
Portugal
Lat.(N)23°8′43″23°8′47″23°8′47″23°9′45″23°9′10″23°8′43″23°9′45″23°9′10″
Lon.(E)112°55′22″112°55′47″112°55′47″112°55′41″112°57′15″112°55′22″112°55′41″112°57′15″
rock typesyenitesyenitesyenitesyenitesyenitetrachytecomenditetrachytesyenite, n = 20syenite, n = 17
groupenclaveenclaveenclaveenclaveenclavehosthosthostenclaveenclave
SiO263.8463.5863.1963.7763.2664.5171.7465.4762.1062.77
TiO20.490.460.470.440.510.360.420.310.640.62
Al2O317.0315.7716.1116.5616.1015.6612.5115.5515.7216.89
FeOt5.096.646.605.216.464.583.814.476.123.99
MnO0.060.120.120.080.090.050.010.090.240.22
MgO0.140.280.270.170.320.100.210.090.200.57
CaO0.860.690.730.620.770.170.110.520.591.10
Na2O5.995.895.946.196.225.443.666.686.997.09
Na2O*7.067.137.236.927.15
K2O4.944.874.915.025.135.375.165.415.325.29
P2O50.050.020.030.030.040.040.020.040.040.09
LOI1.421.341.531.711.032.741.440.441.140.61
Total99.9199.6699.9099.8099.9399.0299.0999.0799.1199.23
P.I.1.001.081.070.940.98
The whole-rock chemical compositions of host rocks are from [41], Syenitic enclaves of Kilombe are from [34], and syenitic enclaves of Azores are from [29,30]. LOI: Loss on ignition. P.I. (Peralkaline Index) = Na+K/Al, mol.
Table 6. Mass-balance modeling input parameters and results.
Table 6. Mass-balance modeling input parameters and results.
Model14ss012-119ss036-1CpxOlPlApIlmMagOdiffCdiffRES
SiO247.4164.1248.5638.2551.390.210.280.2716.7216.500.22
TiO22.790.491.400.130.0951.8926.65−2.30−2.420.12
Al2O317.0717.116.870.0330.320.020.110.940.040.000.03
FeOt10.005.117.2222.860.610.845.2570.58−4.89−5.010.11
MnO0.150.060.130.350.010.10.741.45−0.09−0.110.02
MgO7.310.1414.7838.150.080.361.510.05−7.17−7.180.01
CaO8.760.8620.440.2412.7552.240.140.03−7.90−7.87−0.03
Na2O3.507.090.580.064.040.090.030.033.593.62−0.03
K2O2.264.960.020.050.650.030.0602.703.43−0.73
P2O50.740.05000.0346.0700−0.69−0.970.28
Total100.00100.00100100100100100100
SSR 0.59
Wt% 11.4414.4639.302.142.574.53 74.45
Nb89.7188 188302114
ZrS150972 972539−433
Sr87422.8 22.83−19.8
Rb45.8165 165164−1
Y26.196 96960
Ni900.5 0.50−0.5
Th3.819.4 19.414−5.4
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Chen, P.; Qian, B.; Zhou, Z.; Fang, N. Cogenetic Origin of Magmatic Enclaves in Peralkaline Felsic Volcanic Rocks from the Sanshui Basin, South China. Minerals 2023, 13, 590. https://doi.org/10.3390/min13050590

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Chen P, Qian B, Zhou Z, Fang N. Cogenetic Origin of Magmatic Enclaves in Peralkaline Felsic Volcanic Rocks from the Sanshui Basin, South China. Minerals. 2023; 13(5):590. https://doi.org/10.3390/min13050590

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Chen, Peijia, Bo Qian, Zhiwei Zhou, and Nianqiao Fang. 2023. "Cogenetic Origin of Magmatic Enclaves in Peralkaline Felsic Volcanic Rocks from the Sanshui Basin, South China" Minerals 13, no. 5: 590. https://doi.org/10.3390/min13050590

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