Zhen
Zeng
ab and
Fei
Wu
*a
aSchool of Earth Sciences, State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Wuhan, 430074, China. E-mail: wufei@cug.edu.cn
bState Key Laboratory of Soil and Sustainable Agriculture, Institute of Soil Science, Chinese Academy of Sciences, Nanjing, 210008, China
First published on 9th November 2023
Vanadium (V) isotopes are a powerful tool for fingerprinting the redox-state variations in geological processes, but their widespread application is hindered by the complicated processes of separation of V from matrix elements. In this study, we established a two-stage chromatography technique using cation and anion exchange resins for V purification from natural samples. This method can quantitatively and efficiently separate V from matrix elements, especially Ti and Cr, which introduce spectral interferences. The V isotopic composition was analysed using multi-collector inductively coupled plasma-mass spectrometry. The instrumental mass fractionation of V isotopic ratios was corrected by the sample-standard-bracketing method. The δ51V values of two in-house standard solutions, CUG-V and BDH-V, were 0.04 ± 0.08‰ (2 SD, n = 121) and −1.23 ± 0.08‰ (2 SD, n = 91), respectively. The V isotope compositions of 13 reference materials, including igneous rock, manganese nodules, carbonaceous siliceous shale, sediment and soil, were measured in this study. Based on the repeated measurements of pure solution and reference materials, the long-term reproducibility was better than ± 0.10‰ (2 SD) for δ51V values. The new approach to V isotope analysis presented in this work is both economical and time-efficient, improving the ability for further investigation of V isotope geochemistry in various geological and environmental systems.
Vanadium has two long-lived isotopes (50V and 51V) with abundances of 0.24% and 99.76%,9 respectively. With the development of analytical methods using multi-collector inductively coupled plasma-mass spectrometry (MC-ICP-MS), high-precision measurements of V isotopes have recently been developed.10–21 Vanadium isotope compositions are generally reported as δ51V values, which are the deviations of V isotope ratios relative to AA-V solution:10 δ51V = [(51V/50Vsample)/(51V/50VAA) − 1] × 1000‰. Large V isotope fractionations have been predicted by theoretical and experimental studies,22–24 and observed in natural samples, which implies their wide application to study geological processes. The distinct δ51V in chondritic meteorite,25,26 Martian,27 lunar,28 and terrestrial materials29,30 were proposed to reflect V isotope fractionation during planetary differentiation in the Solar System and the formation of the Moon. Vanadium isotope variations observed in mantle-derived magmas are thought to indicate variable isotope fractionation during mantle partial melting, which are likely controlled by the degree of partial melting and fO2 variations in the mantle.29,31–33 The δ51V values of igneous rocks show apparently increasing with the degree of magma differentiation, indicating remarkable V isotope fractionation during magmatic evolution.31,34,35 In addition, different magmatic differentiation trends of V isotopes are observed in different magmatic systems, which is thought to be controlled by variable crystallized minerals with different isotope fractionation factors. Thus, V isotopes could also be used to distinguish between different fractionating assemblages and thus contribute to our understanding of differentiation processes during magma evolution.35
Limited isotope fractionation was observed during rock weathering,36 which is consistent with the observation that the δ51V of average river waters was similar to that of average upper continental crust.20 For comparison, the δ51V of the seawater were significantly heavier than those of river waters due to the fact that the main sinks of V in the ocean, i.e., oxic sediment, anoxic sediment, euxinic sediment and hydrothermal sediment, preferentially captured light V isotopes from seawater.21,37–39 The strong correlation between δ51V in marine authigenic sediments and the overlying redox conditions suggests that vanadium isotopes in sediments have the potential to trace variations in the marine palaeo-redox state, particularly to trace subtle redox variations in local oxygen-deficient to low oxygen environments.40–44 Moreover, the variations in V isotopes in terrestrial materials could be used to trace the sources of vanadium in crude oils, soils, lake sediments and aquatic food chains.15,18,19,45
Despite the promising application of V isotopes, the dataset and investigation of V isotopes are still limited due to the complicated and inefficient chemical purification procedure of V isotopes. There are several reasons for this problem. First, the sample-standard-bracketing (SSB) method is the only applicable method for V isotope measurement, which requires a nearly 100% recovery rate of V to avoid isotopic fractionation during chemical purification. Second, V is a trace element, and the low tolerance of the matrix effect during instrumental measurement requires the quantitative removal of matrices during chemical purification. Last, both 50Ti and 50Cr exhibit isobaric interferences on the minor 50V, which significantly affects the determination of V isotopes. Therefore, the quantitative separation of V from matrix elements, especially Cr and Ti, is crucial to obtain high-precision and accurate V isotope ratios. To overcome the above difficulties, chemical purification of V from matrix elements typically involved multiple sequential ion exchange chromatography columns in previous works. For instance, Nielsen, et al.10 used anion and TRU SPEC resin to separate the majority of matrix elements, followed by quantitative removal of the remaining matrix elements, especially Cr and Ti, via two or more anion exchange columns. In an effort to improve time-efficiency, Wu, et al.13 utilized cation exchange resin to remove the majority of matrix elements. In summary, previous methods required at least four stage ion exchange columns, consuming considerable time and reagents. In this study, we established a simplified purification procedure, consisting of a two-step ion exchange process using one cation exchange column and one anion exchange column to effectively separate V from matrices.
The reference materials used in this study included four igneous rock standards from the United States Geological Survey (USGS), one manganese nodule standard from the USGS, one carbonaceous siliceous shale standard from the Institute of Geophysical and Geochemical Exploration (IGGE) of the Chinese Academy of Geological Sciences and seven soil and sediment standards from the National Institute of Standards and Technology (NIST) and IGGE.
The sample digestion and chemical purification procedures were carried out in an ultraclean laboratory of the State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Wuhan. Samples (10–100 mg) containing 2–20 μg V were weighed into 7 mL Teflon PFA screw cap vials (Savillex) and digested with concentrated HF and HNO3 (3:1, v/v) at 120–140 °C for 24 h to decompose silicates. The soil and sediment samples were pretreated with HClO4–HNO3–HF mixture acids (1:1:2, v/v/v) at 160 °C for 8 h to digest organic matter before decomposing the silicates. Then, the samples were dried and treated with aqua regia first at room temperature for 12 h and then heated to 100 °C for 4 h to ensure that all V in the solution were oxidized to pentavalent V (V5+). After subsequent evaporation to dryness, samples were treated with 2 mL of 3 mol L−1 (M) HCl to convert all anions to chloride. Finally, the sample was dried and re-dissolved in 1 mL of 1 M HCl at 120 °C for 4 h, and then 1 mL ultrapure H2O was used to dilute the sample solution which was ready for ion-exchange purification in the first column.
Resin | Eluent | Vol. (mL) | Comment |
---|---|---|---|
Column 1 2 mL AG50W-X12 (200–400 mesh) | 4 M HNO3 + 0.5 M HF | 20 | Clean resin |
H2O | 5 | Clean resin | |
0.5 M HCl | 5 | Condition resin | |
Load sample in 0.5 M HCl | 2 | — | |
0.1 M HCl + 0.05 M HF | 5 | Elute Ti, Al and Cr | |
0.1 M HCl | 13 | Elute Ti, Al and Cr | |
0.1 M HNO3 + 2% H2O2 | 6 | Collect V | |
4 M HNO3 | 20 | Elute matrix elements | |
Column 2 1 mL AG1-X8 (200–400 mesh) | 1 M HNO3 | 10 | Clean resin |
H2O | 5 | Clean resin | |
0.1 M HCl + 1% H2O2 | 5 | Condition resin | |
Load sample in 0.1 M HCl + 1% H2O2 | 1 | — | |
0.1 M HCl + 1% H2O2 | 15 | Elute matrix elements | |
1 M HNO3 | 10 | Collect V |
Since V is a trace element, even a small proportion of matrix elements (especially Ti and Cr) remaining in the solution after the first step of purification would significantly influence the V isotope measurement.10,13 With the aim of quantitatively removing the remaining matrix elements, a second purification step was carried out using an anion exchange resin column. One milliliter of anion exchange resins (AG1-X8, 200–400 mesh, Bio-Rad, USA) was loaded into the pipette tip with quartz wool inserted as a porous barrier to retain the resins. Fig. 1b illustrates the typical elution curves for V purification procedures in the second column. After cleaning with 10 mL 1 M HNO3 and 3 mL H2O, the anion exchange resins were conditioned with 3 mL 0.1 M HCl + 1% H2O2. Sample dissolved in 1 mL 0.1 M HCl + 1% H2O2 was loaded onto the resin. Matrix elements were eluted with 15 mL of 0.1 M HCl + 1% H2O2, and V was collected using 10 mL 1 M HNO3 afterwards. After evaporation of the collected V cut, 1 mL of 1:1 (v/v) concentrated HNO3 and 30% H2O2 were added to the beaker, which was closed and heated on a hot plate at 80 °C for four hours to decompose organic matter eluted from resins. Finally, the sample was dried and dissolved in 2% HNO3 (m/m) for instrumental analysis. The total procedure blank was below 2 ng, which is negligible compared to a total of 2–20 μg V in the samples.
MC-ICP-MS | Thermo Fisher Scientific, Neptune Plus | |||||
Cooling Ar | ∼16 L min−1 | |||||
Auxiliary Ar | ∼0.70 L min−1 | |||||
Nebulizer Ar | ∼1.05 L min−1 | |||||
Mass resolution | High resolution | |||||
Typical sensitivity | ∼120 V per μg mL−1 for 51V | |||||
Cones | Ni jet cone, X-skimmer cone | |||||
Desolvator | Aridus II | |||||
Ar sweep | ∼3 L min−1 | |||||
Solution uptake rate | ∼50 μL min−1 | |||||
Faraday cup | L4 | L2 | C | H1 | H3 | H4 |
Resistor | 1011 Ω | 1011 Ω | 1011 Ω | 1010 Ω | 1011 Ω | 1011 Ω |
Mass | 47Ti | 49Ti | 50V | 51V | 52Cr | 53Cr |
To overcome the above obstacles, we proposed a novel chromatography strategy with a cation exchange resin (Table 1). As shown in the elution curve (Fig. 1a), after loading sample solution, Ti and Al were first eluted using 0.1 M HCl + 0.05 M HF and 0.1 M HCl, as they form anionic fluorides that have low affinity with cation resin, in the presence of trace HF.49,50 Then, V was eluted from the cation resin with 0.1 M HNO3 + 2% H2O2 (v/v) in the form of a V-peroxide anionic complex, which does not bind with the cation resin. For comparison, other cationic matrix elements were still retained on the cation exchange resin,30 because they have high equilibrium distribution coefficients under low acidity conditions.51 Thus, V could be separated from almost all the matrix elements with this column procedure. After this step of purification, all sample solutions exhibited 49Ti/51V and 52Cr/51V ratios lower than 10−4 and 10−3, respectively, representing a decrease of three to five orders of magnitude (Table 3).
Isotopic ratio | Sample | Before separation | After first column | After second column |
---|---|---|---|---|
49Ti/51V | GSP-2 | 4.3 | 6.5 × 10−5 | 0.4 × 10−5 |
SRM2711a | 6.7 | 3.8 × 10−5 | 0.4 × 10−5 | |
BHVO-2 | 2.8 | 3.2 × 10−5 | 0.3 × 10−5 | |
BCR-2 | 1.8 | 1.1 × 10−5 | 0.3 × 10−5 | |
52Cr/51V | GSP-2 | 0.32 | 2.0 × 10−4 | 0.4 × 10−4 |
SRM2711a | 0.54 | 1.5 × 10−4 | 0.5 × 10−4 | |
BHVO-2 | 0.76 | 1.3 × 10−4 | 0.4 × 10−4 | |
BCR-2 | 0.04 | 0.5 × 10−4 | 0.3 × 10−4 |
The elution curves of cations, such as Mg,52 V,13 and Rb,53 might drift with different amounts of these elements loaded into the cation resin columns. Therefore, to ensure quantitative collection of V during the purification procedure, we conducted experiments to determine the elution curves of different types of samples containing variable amounts of V, ranging from 2 μg to 20 μg. The samples used in this experiment included GSP-2, SRM2711a, BHVO-2 and BCR-2, which represent granodiorite, soil and basalt, respectively. The V concentration of these reference materials ranged from 52 to 420 μg g−1. The results showed that regardless of the variable loading amount of V and matrix elements onto the column, the elution curves of V overlapped perfectly with each other (Fig. 2). Thus, the recovery rates of V with this purification procedure were consistently higher than 99%. This is because previous methods generally used diluted HNO3 (0.2–1.2 M) to gradually elute V from the column,13,15 depending on the distribution coefficient of V in the cation exchange resins. Instead, hydrogen peroxide was used in this procedure to form V-peroxide anion complexes that could not bind to cation exchange resins, allowing V to be directly eluted. It is notable that there were a few small bubbles generated in the column when using 0.1 M HNO3 + 2% H2O2 to elute V, as hydrogen peroxide was partly catalyzed to decomposition by Fe retained in the resin. Despite this issue, the consistently high recovery rates of V for different types of samples with variable Fe/V ratios demonstrate that H2O2 was sufficient to completely form the V-peroxide anion complex. Furthermore, we conducted three repetitions of the purification using the same cation exchange resin and found that the elution curve of V could be well replicated, regardless of the number of usages.
In order to quantitatively separate the remaining Ti, Cr and other matrix elements to meet the requirements of instrumental measurement, an anion resin column procedure using peroxide and weak acid was necessary.10,13 Since our method has already separated the majority of matrix elements after the first column, and with 49Ti/51V and 52Cr/51V below 10−4 and 10−3 respectively (Table 3), we only need to perform one round of anion exchange resin purification (Table 1).
In summary, our purification scheme offers several advantages over previous studies: (1) the purification process requires only two separation steps, greatly reducing the time and reagents required for the whole procedure; (2) the method relies on the desorption of V-peroxide complex anions from cation exchange resin under dilute acid conditions, demonstrating excellent reproducibility and operational feasibility; (3) the elution curves of V in the first column will not shift when increasing the amount of V from 2 μg to 20 μg, obtaining a broader range of applicability; (4) the cation or anion exchange resin used in the method can be repeatedly used, effectively reducing costs. Therefore, our V isotope analysis method is both economical and time-efficient.
50Vcorrected = 50Vmeasured − 49Timeasured × (50Ti/49Ti)IMF − 52Crmeasured × (50Cr/52Cr)IMF | (1) |
RT = RIMF × (m1/m2)β | (2) |
Nielsen, et al.10 observed significant V isotope drift in the correction of isobaric interferences from 50Ti or 50Cr when the instrumental mass fractionation factor varied from −1.8 to −2.2. To address this issue, Wu, et al.13 obtained the real-time instrument mass fractionation factor of Ti and Cr isotopes by measuring the pure standard Ti and Cr solution with natural abundance before each measurement sequence began. For comparison, Schuth, et al.16 introduced Fe solution as external standard, and used the instrumental mass fractionation factor of Fe to correct Cr–Ti interferences. Both approaches assumed that the Ti and Cr isotope ratios of residual Cr and Ti in the samples were consistent with those in the Ti and Cr standard solutions, respectively.13,16 However, the Ti and Cr isotopic ratios of natural samples exhibited significant variation.54,55 In addition, isotope fractionation could occur during the removal of Cr and Ti in the column. Thus, the trace Cr and Ti remaining after purification probably have different isotopic compositions from standard Ti and Cr solutions. This could cause V isotopic offsets of the measured δ51V value from the true δ51V value (Δ51V = δ51Vmeasured − δ51Vtrue) after isobaric calibration of Cr and Ti.
In this study, we conducted doping experiments to assess the effect of Cr and Ti isotope differences on the accuracy of V isotope measurements. Variable amounts of GSB-Ti (GSB 04-1757-2004, 1000 μg mL−1) were added to a 1 μg mL−1 AA-V solution to evaluate the extent to which the Ti remaining in the solution could be effectively corrected. First, we used the correction method from Wu, et al.13 to assess the V isotopic offset generated by correcting the isobaric interference when using Ti isotopic ratios of GSB-Ti. We determined the 50Ti/49Ti ratio of 50 ppb GSB-Ti after instrumental fractionation and used this ratio as (50Ti/49Ti)IMF for isobaric correction. The results demonstrated that Δ51V values were close to 0 within uncertainty when the sample had 49Ti/51V < 4 × 10−4 (Fig. 3a). However, when we assumed a ±5‰ difference in Ti isotopes between the remaining Ti in the solution and GSB-Ti, i.e., (50Ti/49Ti)remain/(50Ti/49Ti)GSB-Ti = 0.995 and (50Ti/49Ti)remain/(50Ti/49Ti)GSB-Ti = 1.005, the results showed that Δ51V values deviated obviously from 0 within uncertainty when 49Ti/51V > 4 × 10−5 (Fig. 3a). A similar correction was also applied for the interference of 50Cr. First, we measured the 50Cr/52Cr ratio of 50 ppb GSB-Cr (GSB 04-1723-2004, 1000 μg mL−1) after instrumental fractionation and used this ratio as (50Cr/52Cr)IMF to correct the interference of 50Cr. The results revealed that when the sample had 52Cr/51V < 4 × 10−3, the Δ51V values were close to 0 within uncertainty (Fig. 3b). We also assumed a ±5‰ difference in Cr isotopes between Cr remaining in the solution and GSB-Cr, i.e., (50Cr/52Cr)remain/(50Cr/52Cr)GSB-Cr = 0.995 and (50Cr/52Cr)remain/(50Cr/52Cr)GSB-Cr = 1.005. The Δ51V values shifted distinctly from 0 within uncertainty with 52Cr/51V > 8 × 10−4, when using Cr isotopic ratios different from GSB-Cr for correction (Fig. 3b). Due to the unknown Ti or Cr isotopic composition of natural samples, Δ51V values may also shift significantly from 0 when the sample solution has 49Ti/51V > 4 × 10−5 or 52Cr/51V > 8 × 10−4. In this study, all sample solutions from different types of reference materials after two-step purification procedures had 49Ti/51V < 1 × 10−5 and 52Cr/51V < 1 × 10−4 (Table 3), thereby not affecting our measurement accuracy. This also demonstrates that our chemical purification process is reliable and universally applicable.
The long-term analysis of the BDH-V solution produced an average δ51V value of −1.23 ± 0.08‰ (2 SD, n = 91), which was consistent with the literature values.10,12,13 The repeated determination of the CUG-V solution gave an average δ51V value of 0.04 ± 0.08‰ (2 SD, n = 121). For the reference materials, V isotope analyses were repeatedly conducted with independent digestion and purification through different columns. The δ51V values of these reference materials (BHVO-2, BCR-2, AGV-2, GSP-2 and NOD-A) were −0.87 ± 0.08‰, −0.81 ± 0.09‰, −0.72 ± 0.05‰, −0.61 ± 0.10‰ and −1.02 ± 0.07‰, respectively. These δ51V values are consistent with the literature values.11,13,26 In summary, our V isotopic analytical method has been shown to accurately and precisely measure V isotopes, with a long-term reproducibility of δ51V values better than ±0.10‰ (2 SD) as demonstrated through the analysis of these reference materials.
Name | δ 51V (‰) | 2 SD (‰) | n |
---|---|---|---|
BHVO-2 | −0.88 | 0.08 | 3 |
BHVO-2 | −0.85 | 0.07 | 3 |
BHVO-2 | −0.85 | 0.03 | 3 |
BHVO-2 | −0.91 | 0.06 | 3 |
Average | −0.87 | 0.08 | 12 |
Prytulak, et al.11 | −0.89 | 0.08 | 9 |
Wu, et al.13 | −0.83 | 0.09 | 22 |
BCR-2 | −0.83 | 0.05 | 3 |
BCR-2 | −0.75 | 0.10 | 3 |
BCR-2 | −0.82 | 0.05 | 3 |
BCR-2 | −0.82 | 0.10 | 3 |
BCR-2 | −0.83 | 0.05 | 3 |
Average | −0.81 | 0.09 | 15 |
Prytulak, et al.11 | −0.95 | 0.16 | 27 |
Wu, et al.13 | −0.78 | 0.08 | 36 |
Nielsen, et al.26 (WHOI) | −0.79 | 0.15 | 24 |
Nielsen, et al.26 (ICL) | −0.80 | 0.14 | 3 |
AGV-2 | −0.71 | 0.04 | 3 |
AGV-2 | −0.74 | 0.05 | 3 |
AGV-2 | −0.70 | 0.03 | 3 |
Average | −0.72 | 0.05 | 9 |
Prytulak, et al.11 | −0.50 | 0.19 | 4 |
Wu, et al.13 | −0.70 | 0.10 | 37 |
Nielsen, et al.26 | −0.73 | 0.17 | 16 |
GSP-2 | −0.57 | 0.10 | 3 |
GSP-2 | −0.63 | 0.07 | 3 |
GSP-2 | −0.64 | 0.08 | 3 |
Average | −0.61 | 0.10 | 9 |
Prytulak, et al.11 | −0.63 | 0.10 | 6 |
Wu, et al.13 | −0.62 | 0.07 | 26 |
Nielsen, et al.26 | −0.76 | 0.15 | 4 |
NOD-A | −0.97 | 0.10 | 3 |
NOD-A | −1.05 | 0.06 | 3 |
NOD-A | −1.06 | 0.04 | 3 |
NOD-A | −1.02 | 0.02 | 3 |
NOD-A | −1.02 | 0.05 | 3 |
NOD-A | −1.02 | 0.03 | 3 |
Average | −1.02 | 0.07 | 18 |
Wu, et al.13 | −0.99 | 0.10 | 19 |
GSR-20 | −0.27 | 0.06 | 3 |
GSR-20 | −0.32 | 0.06 | 3 |
GSR-20 | −0.30 | 0.05 | 3 |
GSR-20 | −0.32 | 0.02 | 3 |
Average | −0.30 | 0.06 | 12 |
GSD-28 | −0.79 | 0.10 | 3 |
GSD-28 | −0.73 | 0.01 | 3 |
GSD-28 | −0.76 | 0.07 | 3 |
Average | −0.76 | 0.08 | 9 |
GSD-32 | −0.76 | 0.06 | 3 |
GSD-32 | −0.77 | 0.04 | 3 |
GSD-32 | −0.77 | 0.05 | 3 |
Average | −0.76 | 0.04 | 9 |
GSS-24 | −0.74 | 0.03 | 3 |
GSS-24 | −0.77 | 0.04 | 3 |
GSS-24 | −0.78 | 0.01 | 3 |
GSS-24 | −0.81 | 0.04 | 3 |
GSS-24 | −0.76 | 0.06 | 3 |
Average | −0.77 | 0.06 | 15 |
GSS-25 | −0.79 | 0.02 | 3 |
GSS-25 | −0.75 | 0.02 | 3 |
GSS-25 | −0.70 | 0.08 | 3 |
GSS-25 | −0.72 | 0.03 | 3 |
Average | −0.74 | 0.08 | 12 |
SRM2709a | −0.76 | 0.03 | 3 |
SRM2709a | −0.69 | 0.05 | 3 |
SRM2709a | −0.81 | 0.05 | 3 |
SRM2709a | −0.77 | 0.06 | 3 |
Average | −0.76 | 0.10 | 12 |
SRM2710a | −0.75 | 0.06 | 3 |
SRM2710a | −0.78 | 0.05 | 3 |
SRM2710a | −0.69 | 0.10 | 3 |
Average | −0.74 | 0.10 | 9 |
SRM2711a | −0.75 | 0.03 | 3 |
SRM2711a | −0.70 | 0.05 | 3 |
SRM2711a | −0.75 | 0.08 | 3 |
Average | −0.73 | 0.07 | 9 |
Fig. 5 The δ51V values of reference materials. Error bars reflect two standard deviations. Data are from Table 3. The range of δ51V values of the upper continental crust (UCC) is from Tian, et al.56 |
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