Lana
Abou-Zeid
*a,
Martin
Wiech
b and
Frank
Vanhaecke
a
aAtomic & Mass Spectrometry – A&MS Research Unit, Department of Chemistry, Ghent University, Campus Sterre, Krijgslaan 281 – S12, 9000 Ghent, Belgium. E-mail: lana.abouzeid@ugent.be
bInstitute of Marine Research, PO Box 1870, Nordnes, 5817 Bergen, Norway
First published on 25th June 2025
This study presents a comprehensive methodological investigation aimed at optimizing selenium (Se) isotopic analysis using MC-ICP-MS. Fundamental aspects of the plasma were revisited through spatial profiling, enabling detailed characterization of the distribution of Se+ and ArAr+/ArArH+ species within the plasma. Increasing the sampling depth (sampling further upstream in the plasma) proved more effective than the commonly employed methane addition, offering a more effective suppression of the Ar-based species, although at the cost of some loss in the sensitivity for Se. Under these conditions, precision values (expressed as 2SD) of 0.03‰ and 0.17‰ were obtained for δ82/78Se and of 0.08‰ and 0.38‰ for δ82/76Se, at 100 and 25 μg L−1, respectively. Moreover, the method proved robust, with a long-term reproducibility of 0.07‰ (2SD, n = 120) and high accuracy, even at up to 30% sample-standard concentration mismatch. However, the method's relatively high hydride formation rate (∼7 × 10−3) limits its applicability to samples with As/Se post-isolation ratios ≤0.05, beyond which mathematical corrections lead to biased results. Finally, the method was validated using the SELM-1 reference material, for which the δ82/78Se and δ82/76Se values were in excellent agreement with published data, and was subsequently applied to a set of tuna fish organs (liver, spleen, kidney, and intestine). This study demonstrates that the method that was developed, optimized and validated forms a solid basis for further investigating Se metabolic pathways in marine fish and for elucidating its role in Hg detoxification.
Selenium has six stable isotopes with masses ranging from 74 to 82 amu and occurs in multiple redox states, i.e. Se(0), Se(−II), Se(IV) and Se(VI), which are involved in several environmental and biogeochemical processes.9–11 Due to their mass difference, Se isotopes participate with slight differences in the reaction rate (kinetically governed isotope fractionation) and/or in the equilibrium state (thermodynamically governed isotope fractionation) in chemical reactions, leading to isotopic fractionation.12 This makes Se isotopic analysis highly valuable for tracing Se sources in the environment and understanding its redox cycling and metabolic transformations in natural systems.13–16 Selenium isotopic analysis is typically performed using multi-collector inductively coupled plasma-mass spectrometry (MC-ICP-MS) due to the high sample throughput and high precision typically offered by this technique.17,18 However, MC-ICP-MS isotopic analysis of Se is associated with numerous challenges. First, Se has a high ionization potential (9.75 eV), resulting in a relatively poor ionization yield in the ICP source (30%)19 and therefore, a lower sensitivity compared to other elements. This poses the first challenge for precise isotope ratio measurements, as a reduced ion beam intensity can lead to higher uncertainty (counting statistics), while in most sample types, Se is present at very low concentrations only. To mitigate this lower sensitivity, Se is commonly introduced into the MC-ICP-MS unit under “dry plasma conditions” using a hydride generation (HG) system.20–23 The latter involves the reduction of Se(IV) by sodium borohydride (NaBH4), resulting in the formation of gaseous Se-hydride. This introduction system increases the Se introduction efficiency in comparison to the standard wet plasma approach using a pneumatic nebulizer and spray chamber and therefore results in an enhanced Se signal intensity. Unfortunately, HG is not Se-selective and other hydride-forming elements such as Ge and As are also converted into gaseous hydrides by NaBH4 and further introduced into the MC-ICP-MS unit, causing spectral interferences affecting the signals of the Se isotopes (overlap of the signals of 74Ge+ and 74Se+, 75AsH+ and 76Ge+ and 76Se+, and 76GeH+ and 77Se+). Moreover, the HG process is susceptible to interferences from transition metal ions from elements such as cobalt (Co), copper (Cu), nickel (Ni), and iron (Fe) if present in the sample. These elements are reported to inhibit the conversion of Se(IV) into Se-hydride form, leading to a reduction in Se ion signal intensity.24 Therefore, a chemical purification prior to HG-MC-ICP-MS measurement is necessary to separate Se from these interfering elements. This is typically accomplished using the well-established thiol cellulose powder (TCP) method, as it ensures quantitative Se recovery and provides optimal separation efficiency from these interfering elements.24 However, any Se loss during chromatographic isolation may induce isotopic fractionation, thereby compromising the accuracy of isotope ratio measurements. To address this limitation, the double-spike approach is often used, which involves adding a known mixture of enriched Se isotopes to the sample, allowing one to correct for these losses and for instrumental mass discrimination occurring at the level of the MC-ICP-MS. Despite the advantages offered by this approach, it is costly, labor-intensive and requires meticulous sample preparation, while the analysis of samples with an isotopic composition that deviates substantially from the natural one can require longer rinsing to avoid cross-over contamination due to memory effects.
Another significant challenge in Se isotope ratio measurement using MC-ICP-MS is the occurrence of spectral interferences, primarily arising from argon-based polyatomic ions, the signals of which overlap with those of most of the Se isotopes. The most important ones are argon (Ar) dimers, formed by the combination of different Ar isotopes, i.e.40Ar36Ar+ and 38Ar38Ar+ (both to a lesser extent), 40Ar38Ar+ and especially 40Ar40Ar+, the signals of which overlap with those of 76Se, 78Se and 80Se, respectively, in addition to 40Ar37Cl+, which interferes with the monitoring of 77Se. These interferences are impossible to resolve using a “traditional” MC-ICP-MS not equipped with a collision/reaction cell, as the mass resolution required exceeds the capabilities of the commercially available instrumentation.17 One of the most effective strategies reported to mitigate this problem is the introduction of methane gas (CH4) into the plasma,25,26 which has been adopted by many researchers for Se isotope ratio measurement and is typically accomplished by introducing CH4 through the hydride generation unit.21,22,27 Already an amount as low as 1–3 mL min−1 of 2% CH4 in Ar was shown to successfully decrease the signal intensity of ArAr+ and ArArH+ ions by nearly a factor of 2 and at the same time increase the Se signal intensity by approximately a factor of 1.5, resulting in an improved Se/interference ratio, and therefore, in more accurate Se isotope ratio measurements.26 However, while this solution significantly reduced the formation of Ar-based interferences, it did not eliminate them entirely, further restricting accurate Se isotope ratio measurements at low concentration levels.
Using an MC-ICP-MS equipped with a collision/reaction cell (CRC) nowadays is probably the most effective solution for eliminating Ar-based interferences affecting the Se+ signals. However, this type of instrumentation was introduced relatively recently only, such that the large majority of all MC-ICP-MS instrumentation used worldwide is not equipped with a CRC. Moreover, the MC-ICP-MS units equipped with a CRC are also substantially more expensive. Therefore, in this work, we present an alternative approach for reducing the spectral overlap of the Ar-based interferences hampering Se isotopic analysis through revisiting some fundamental aspects of the plasma using a “traditional” MC-ICP-MS unit. For this aim, radial and axial profiling of the plasma was conducted in order to elucidate the distribution of ArAr+, ArArH+ and Se+ ions. These profiles enabled the selection of an optimal torch position such that plasma regions with reduced formation of the interfering ions are extracted via the sampling cone orifice, thereby enhancing the Se/interference signal ratio. In addition, the effect of the torch position on the accuracy and precision of Se isotope ratio data was also evaluated. The results obtained under these optimized instrument settings were compared to those achieved using the widely adopted CH4 addition approach. Moreover, TCP was used for separating Se from matrix elements, ensuring quantitative Se recovery, thereby eliminating the requirement for a double-spike approach. Finally, the method was validated using the selenium-enriched yeast (SELM-1) reference material, previously characterized for its Se isotopic composition by several groups and was applied to a set of tuna fish organs as a proof-of-concept application. This method paves the way to more routine studies of the Se isotopic signature as an additional source of information for revealing the metabolic pathways of Se in fish and further elucidating its role in Hg detoxification.
3NaBH4 + 3H2O + 3HCl + 2H2SeO3 → 3NaCl + 2H2Se + 3H3BO3 + 6H2 | (1) |
In the hydride generation (HG) unit, the sample is first acidified with 2 M HCl solution in a mixing tee (Mixing Tee 1 in Fig. S1†). Subsequently, it is mixed with NaBH4 (0.4% w/v in 0.1 M NaOH) in a second mixing tee (Mixing Tee 2), and is allowed to react with NaBH4 in a mixing loop, resulting in the reduction of Se(IV) to Se(−II), in the form of H2Se.
Selenium is then introduced into the MC-ICP-MS unit under dry conditions. For the experiments involving CH4 addition, a CH4/Ar (2/98 mol%) gas mixture (Air liquid, Belgium) was introduced in the additional gas port (Fig. S1†).
The instrument settings of the HG unit and MC-ICP-MS instrument are summarized in Table 1.
Hydride generation unit | ||
---|---|---|
Solution | Composition | Uptake rate |
HCl | 2 M | 0.182 mL min−1 |
NaBH4 | 0.4% w/v in 0.1 M NaOH | 0.182 mL min−1 |
Sample | 2 M HCl | 0.364 mL min−1 |
MC-ICP-MS cup configuration | |||||||||
---|---|---|---|---|---|---|---|---|---|
Cup | L4 | L3 | L2 | L1 | C | H1 | H2 | H3 | H4 |
Mass | 73 | 75 | 76 | 77 | 78 | 80 | 81 | 82 | 83 |
MC-ICP-MS | |||
---|---|---|---|
Instrument settings | Data acquisition parameters | ||
Sampling cone | Ni; Jet-type; 1.1 mm Ø orifice | Integration time | 4.194 s |
Skimmer | Ni; X-type; 0.8 mm Ø orifice | Uptake time | 240 s |
Plasma gas flow rate | 15 L min−1 | Measurement | 1 block, 60 cycles |
Auxiliary gas flow rate | 0.7 L min−1 | Mass resolution | Low |
Carrier gas flow rate (HG) | 1.2 L min−1 | ||
Additional gas flow rate (HG) | 0 L min−1 | ||
RF power (W) | 1200 |
The signal intensity was monitored at all m/z using Faraday cups connected to amplifiers equipped with 1011 Ω resistors, except at m/z = 80, at which the signal intensity was monitored using a Faraday cup connected to an amplifier equipped with a 1010 Ω resistor, which can tolerate higher currents without saturation.
Se isotope ratios were reported in the delta notation, as per mil deviation (‰), relative to the NIST SRM-3149 standard:
![]() | (2) |
The bias induced by instrumental mass discrimination was corrected for using the sample-standard bracketing approach (SSB), by measuring the NIST SRM 3149 standard before and after each sample. Interference correction will be further detailed in Section 2.4.
Plasma conditions | |
---|---|
Plasma gas flow rate (L min−1) | 15 |
Auxiliary gas flow rate (L min−1) | 0.9 |
RF power (W) | 1550 |
Nebulizer gas flow rate (L min−1) | 1.0 |
Optional gas | NA |
Reaction gas flow rate – O2 (mL min−1) | 0.45 (30%) |
Ions monitored | 80Se16O+, Co(NH3)2+, Ni(NH3)2+, Fe(NH3)2+, Cu(NH3)2+, AsO+, Te+ (IS) and Ga+ (IS) |
Integration time (s) | 1 |
Replicates | 10 |
Sweeps | 100 |
For obtaining the net signal for 80Se, the following calculations were performed:
After correcting for the 82Kr interference by means of OPZ subtraction, 82Se(corr) can be used to calculate the signal of 80Se using the natural abundances of the Se isotopes (eqn (3)).
![]() | (3) |
Subsequently, the signal for 40Ar40Ar+ can be calculated using eqn (4).
40Ar40Ar(calc)+ = I(80) − 80Secalc+ | (4) |
Using the natural abundances of the Ar isotopes, the contribution from ArAr+ ions at m/z = 76 and 78 can be calculated as described in eqn (5) and (6).
![]() | (5) |
![]() | (6) |
These calculated ArAr+ signals were only used to evaluate the contribution from these interferences to the signals at m/z = 76 and 78. The contribution (%) was calculated by dividing the calculated signal intensity for 76ArAr(calc)+ and 78ArAr(calc)+ by the total signal intensity at mass 76 and 78, respectively. As the occurrence of ArAr+ ions was minimized to the maximum extent (see the Results and discussion section), an OPZ subtraction was sufficient to correct for this contribution. The additional correction using these estimated signals only added errors to the final results.
![]() | (7) |
The HG rate is typically very stable throughout a measurement session and is assumed to be the same for all Se isotopes. Therefore, the HG rate was used to correct the signal obtained at m/z = 78 for the contribution from 77SeH+ as shown in eqn (8) and (9):
77SeH+ = 77Se+ × HG rate | (8) |
78Secorr+ = I(78) − 77SeH+ | (9) |
In the case of As, it is assumed that the AsH+/As+ ratio is identical to 82SeH+/82Se+. Therefore, the HG rate was also used to correct the signal at m/z = 76 for the contribution from 75AsH+ as shown in eqn (10) and (11):
75AsH+ = 75Ascorr+ × HG rate | (10) |
76Secorr+ = I(76) − 75AsH+ | (11) |
![]() | ||
Fig. 1 Radial (x, y) and axial (z) spatial profiling of 80ArAr+, 81ArArH+ and 80Se+ with a fixed carrier gas flow rate of 1.2 L min−1. For radial profiling, the z position was fixed at −4.0 mm. |
As can be seen in Fig. 1, the profiles obtained with and without Se in solution are nearly identical, with Ar-based interference intensities remaining consistent, even when experiments were conducted on different days. This observation aligns with the findings of Pogge von Strandmann et al.,29 who used HG coupled to a sector field ICP-MS unit operated in high resolution mode to monitor the stability of Ar-based interfering signals. The authors showed that the intensity obtained for ArAr+ was identical with and without Se present in solution, and stable throughout the measurement session.29
Furthermore, as shown in Fig. 1(a-1) and (b-1), the radial profiles of ArAr+ and ArArH+ exhibit a distinct double or bimodal peak shape, in accordance with the observations of Fraser and Beauchemin.30 The profiles reveal two maxima at distinct positions: −3.23 mm and −1.5 mm on the y-axis, and −1.5 mm and 0.3 mm on the x-axis, with maximum signal intensities of approximately 25 V for 80ArAr+ and 10 V for ArArH+. At the central position between the two peaks (2.33 mm on the y-axis and −0.6 mm on the x-axis), a minimum intensity is observed for the interfering species with 0.05 V for 80ArAr+ and 2.22 V for ArArH+, being respectively 500- and 4.5-fold lower than those observed at the maxima of each peak. Moreover, a maximum contribution from the 80Se+ signal at m/z = 80 is observed at this position with an intensity of 5.70 V, making these x and y values optimal for a high Se/interference ratio. Following this observation, the y and x positions were fixed at −0.6 mm and 2.33 mm, respectively, and the z position of the torch (sampling depth or distance between the tip of the torch and the sampling cone aperture) was changed from 2.5 mm (torch at the furthest position from the sampler cone, thus sampling further downstream in the ICP), to 0 mm as the central position (medium position), and finally to −4 mm (torch at the closest position to the sampler cone, thus sampling more upstream in the ICP), as reported in Fig. 1(c-1) and (c-2). The axial profile reveals a different behavior of the Se+ and interfering ion species, respectively. For 80ArAr+, the signal exhibits a maximum of 62 V at 2.5 mm and decreases when bringing the torch closer to the sampling cone, reaching 0.27 V at −4 mm. For 80Se+, the signal displays a slight increase first, reaching a maximum of 23.83 V at 1.5 mm, before slowly decreasing to 5.47 V at −4 mm. This observation is in accordance with previous observations from Holliday and Beauchemin who stated that sampling more upstream in the plasma results in reduced signal intensity due to the short residence time of the analyte in the plasma.28 Finally, for ArArH+, an increase is first observed, reaching a maximum of 4.82 V at −2 mm after which the signal decreases to a minimum of 2.48 V at −4 mm. Based on these results, it can be concluded that a torch position of −4 mm (sampling more upstream in the ICP), seems to be the most suitable for drastically reducing the contribution from ArAr+ to the Se+ signals, with signal intensities of 0.27 V for 80ArAr+ and of 5.47 V for 80Se+. It is important to mention that the tuning parameters were shown to be very robust, with signal intensities for Se-ions and Ar-based interferences being consistent across multiple days. Only minor adjustments to the torch position (always within the predefined range) were occasionally necessary.
Although the ArAr+ signal intensity has been drastically reduced under these conditions, the signal for ArArH+ remains relatively high (2.48 V), compromising the accuracy of the signal obtained for the 77Se+ signal if not properly accounted for. According to the literature, introducing CH4 into the plasma has proven effective in reducing the occurrence of ArAr+ and, more notably, ArArH+ while also enhancing the Se signal by a factor of 1.5 due to the carbon effect.22,26,31,32 Therefore, to further suppress the contribution from ArArH+ under the optimized conditions, the impact of CH4 addition was assessed, as discussed in the following section.
![]() | ||
Fig. 2 Effect of CH4 addition on 80Se+, 80ArAr+ and 81ArArH+ signal intensities, at different carrier gas flow rates. |
Under the optimized conditions (carrier gas 1.2 L min−1, sampling depth of −4 mm and y and x positions of −0.6 mm and 2.33 mm), increasing the CH4 flow rate led to a nearly 2-fold decrease in the signal intensities for both Se and Ar-based interfering ions upon addition of 1 mL min−1 of CH4 gas only. Consequently, no further CH4 flow rate testing was performed under these conditions. When the carrier gas flow rate was slightly reduced to 1.1 L min−1 (Fig. 2(b)), a similar trend of signal suppression was observed. However, at 1.0 L min−1 (Fig. 2(c)), a different trend was observed. The Se signal intensity increased by a factor of 2 when the CH4 flow rate was increased to approximately 0.8–1.0 mL min−1, while the ArAr+ signal intensity decreased by a similar factor. This behavior aligns with the observation previously reported in the literature.26 Surprisingly, the ArArH+ signal intensity increased with the addition of CH4, reaching a maximum of 0.9 V at a flow rate of 1.0 mL min−1. This result contrasts with findings in the literature, where CH4 addition is reported to significantly decrease the ArArH+ intensity. This discrepancy is likely due to differences in the plasma parameters used in our study as compared to those in previously reported work. Despite this increase, the ArArH+ intensity remains approximately 2.5-fold lower than that observed under our optimized conditions without CH4 addition (Section 3.1). Beyond 1.0 mL min−1 of CH4, the signal intensities for both Se+ and the Ar-based interfering ions begin to decline, mirroring the trend observed in Fig. 2(a) and (b). In addition, the signal intensities for ArAr+ and ArArH+ observed when introducing a 2 M HCl blank solution were compared under optimized conditions (i) without CH4 addition (Fig. 3(a)) and (ii) with CH4 addition (Fig. 3(b)).
![]() | ||
Fig. 3 Comparison of the signal intensities for ArAr+ and ArArH+ (a) without CH4 addition, under optimized plasma conditions and (b) with CH4 addition. |
The results show that optimizing the plasma settings and sampling at higher sampling depth significantly reduces the contribution from ArAr+ to the signal monitored, with only 0.27 V observed at m/z 80 for the blank. However, although CH4 addition does reduce the intensity of the signal at mass 80 as reported in the literature, the remaining contribution from the blank under optimized conditions (signal intensity of 10 V) remains relatively high – approximately 40-fold higher than the value obtained without CH4 addition. In contrast, the ArArH+ signal is significantly lower (about 3-fold lower) when CH4 is added to the plasma, compared to the conditions without CH4. Based on these observations, we prioritized the substantial reduction in the contribution from ArAr+ achieved by optimizing the instrument settings without the addition of CH4, as ArAr+ represents a major interferent affecting two of the Se isotopes, 76Se and 78Se. Consequently, these optimized conditions were selected for all subsequent analyses. Given the relatively high contribution from ArArH+ observed under these conditions, we focused on δ82/78Se and δ82/76Se and omitted δ82/77Se due to the potentially high contribution from ArArH+ at an m/z = 77. The contribution was too prominent for accurate correction using the OPZ correction only.
In order to evaluate the impact of the sampling depth on the accuracy of Se isotope ratio measurements, a Se Merck solution (LOT HC44697996), previously characterized for its Se isotopic composition,22 was measured at the three above-mentioned sampling depths and at three concentrations (25, 50, and 100 μg L−1). The bias introduced by instrumental mass discrimination was corrected for using external correction with a standard measured in a SSB approach following the application of the OPZ and hydride corrections described in the Experimental section. The final results for δ82/78Se and δ82/76Se are shown in Fig. 4.
![]() | ||
Fig. 4 Effect of the sampling depth (z position of the torch) on the accuracy and precision of δ82/78Se (a) and δ82/76Se (b) at 25, 50 and 100 μg L−1 of Se. The full red line represents the value of the Se Merck solution obtained by Chang et al.22 and the dotted red lines represent the corresponding ±2SD range. The dots represent the mean value of n ≥ 3 measurements and the error bars represent the 2SD. |
At 1.5 mm sampling depth, the accuracy and precision of the Se isotope ratio measurement is compromised, especially at the lowest concentration levels of 25 μg L−1, with −0.48 ± 0.28‰ and +0.98 ± 2.37‰ for δ82/78Se and δ82/76Se, respectively (reference value −0.72 ± 0.07 and −1.07 ± 0.16, as reported by Chang et al. 201722). This can be explained by the low signal intensity for the Se isotopes monitored at such a low concentration (0.689 V for 82Se) and therefore, the high contribution of the interference to the signal intensity (1.1% contribution from 78ArAr+ at m/z = 78 and 13% contribution from 76ArAr+ at m/z = 78, see the ESI†). Such a contribution is too significant to be accurately accounted for using the OPZ correction. At 0 mm sampling depth, with nearly equal contributions from the Se+ and interference signals, the values were accurate and precise for δ82/78Se with −0.72 ± 0.13‰ and −0.69 ± 0.06‰ at 50 and 100 μg L−1, respectively (less than 0.5% contribution from 78ArAr+), except at 25 μg L−1 where δ82/78Se showed high 2SD values −0.78 ± 0.32‰ (0.8% contribution from 78ArAr+). In contrast, the values are inaccurate and imprecise for δ82/76Se, with −3.04 ± 0.90‰, −2.10 ± 0.24‰ and −0.92 ± 0.37 for 25, 50 and 100 μg L−1 of Se, respectively, due to the significant contribution from ArAr+ at m/z = 76 (2.7–9% contribution). Finally, at −4 mm sampling depth, the values are accurate and precise for both ratios (e.g., −0.72 ± 0.05‰ and −1.08 ± 0.04‰ for δ82/78Se and δ82/76Se, respectively, at 50 μg L−1 of Se), except at 25 μg L−1 for which the precision was degraded (ex. −0.70 ± 0.17‰ and −1.15 ± 0.38‰ for δ82/78Se and δ82/76Se, respectively) due to the low signal intensity obtained for the Se+ signals (0.157 V for 76Se, 0.4105 V for 78Se and 0.1637 V for 82Se). At this position, the contribution from 78ArAr+ to the signal at m/z = 78 ranged between 0.03% and 0.1%, only, and the contribution from 76ArAr+ to the signal at m/z = 76 ranged between 0.4 and 1.4% at 100 and 25 μg L−1 of Se, respectively. These values highlight the effective reduction of Ar-based interferences under the plasma conditions selected, resulting in improved accuracy and precision of the Se isotope ratio measurements.
The values obtained for δ82/78Se and δ82/76Se are accurate, even at −25% and +30% concentration mismatch between the sample and the bracketing standard. It is important to emphasize that while the amplitude of the mass bias is influenced by the analyte concentration and matrix composition, it is also systematically influenced by instrumental conditions.33 Andrén et al. (2004) showed that the torch position (sampling depth) has a significant impact on the magnitude and stability of the mass bias. They reported that when the torch is moved closer to the sampler cone, the intensity of the ion beam dropped by almost 20% and the amplitude of the mass bias increased; however, the mass bias was more stable and the precision of the isotope ratio measurement was improved.33 These findings may help explain the results presented in Fig. 5, where the mass bias appears largely unaffected by concentration mismatch. This could be attributed to the stable operating conditions and the stable mass bias achieved at a torch position of −4 mm, as similarly reported by Andrén et al. (2004). Despite this wide tolerable range of sample-standard mismatch, a maximum of 10% mismatch was adopted throughout the remainder of this study as this is the standard range used for most isotope systems in our laboratory.
The δ82/78Se values remain accurate regardless of the As/Se ratios, since 78Se is not affected by spectral interferences from this element. In contrast, δ82/76Se is significantly impacted, even at As/Se ratios as low as 0.1. As mentioned previously, significant spectral interference affecting the monitoring of 76Se is caused by the formation of 75AsH+. Under the conditions used, this interference can be reliably corrected for up to an As/Se ratio of 0.05, yielding a δ82/76Se value of −0.97‰ (compared to −1.87‰ without correction). However, at higher ratios, the correction is no longer fit-for-purpose. For example, for an As/Se ratio of 0.1, the uncorrected value of −2.55‰ is adjusted to −0.72‰ after correction. This trend of over-correction continues with increasing As/Se ratios, resulting in increasingly heavier values – for example, at a ratio of 0.5, the corrected δ82/76Se shifts to +0.55‰, whereas the uncorrected value is at −8‰. This contrasts with the results reported in the literature, where As/Se ratios up to 0.6 were reliably corrected for using the same mathematical correction, combined with a double-spike correction approach.23,29 This inconsistency with the results reported in the literature can be explained by the high hydride formation rate of ∼7 × 10−3 (calculated for 82SeH+/82Se+ according to eqn (7)) obtained under our experimental conditions, which is higher than the values reported in the literature (∼10−3–10−4).29 When it is assumed that the AsH+/As+ ratio is identical to 82SeH+/82Se+ (eqn (10)), the AsH+ formation under the conditions used is significant even at low As/Se ratios. This constitutes a limitation for the method, making it only suitable for samples showing an As/Se content ≤0.05 post TCP chemistry, or for samples without As. For samples with high As concentrations, a further optimization of the TCP separation conditions will be necessary to achieve lower residual As/Se ratios.
The average of all δ82/78Se values obtained for the Se Merck solution is −0.71 ± 0.07 (2SD, n = 120), in accordance with the values previously reported by Chang et al.22 for the same solution (reference value −0.72 ± 0.07). This further demonstrates the method's robustness and suitability for accurate and precise Se isotope ratio measurements.
Finally, the validated method was applied to a set of tuna fish organs (liver, spleen, kidney, and intestine), previously characterized for their Hg concentration, speciation and isotopic composition. The aim of this kind of work is to study the role of Se in the Hg detoxification process through monitoring its concentration and isotopic composition. The different fish organs have been subjected to acid digestion and to Se isolation using the TCP method in triplicate. The Se recovery (%) and information on the elemental composition of these samples before and after isolation (represented as the X/Se ratio, with X being the element of interest) are summarized in Table 3.
Fe/Se | Co/Se | Ni/Se | Cu/Se | As/Se | Se recovery (%) | ||
---|---|---|---|---|---|---|---|
Liver | Before isolation | 5.78 | 0.01 | 0.04 | 5.07 | 0.29 | 101 ± 3% |
After isolation | 0.05 | 0.00 | 0.00 | 0.01 | 0.05 | ||
Spleen | Before isolation | 18.25 | 0.00 | 0.00 | 0.01 | 0.02 | 97 ± 3% |
After isolation | 0.02 | 0.00 | 0.00 | 0.00 | 0.01 | ||
Kidney | Before isolation | 18.26 | 0.01 | 0.01 | 3.08 | 0.12 | 96 ± 2% |
After isolation | 0.03 | 0.00 | 0.00 | 0.01 | 0.02 | ||
Intestine | Before isolation | 4.90 | 0.00 | 0.02 | 0.42 | 0.57 | 98 ± 3% |
After isolation | 0.16 | 0.00 | 0.02 | 0.02 | 0.08 |
For all organs analyzed in triplicate, Se was quantitatively eluted from the column, with recovery factors ≥96% ± 2%. Moreover, critical elements known to interfere with the hydride generation process (Fe, Co, Ni, and Cu) and those causing spectral interference affecting the signals of the Se isotopes of interest (As), were efficiently removed from the matrix, with an X/Se ratio post TCP chemistry of 0 ≤ X/Se ≤ 0.16. The As/Se ratio in the sample prior to TCP was already low (≤0.57) and was further reduced following the TCP purification, now ranging between 0.01 and 0.05 (except for the intestine for which it was slightly higher). These residual As/Se ratios fall within the acceptable range for accurate mathematical correction, as previously demonstrated in Section 3.5.
Subsequently, the purified Se fractions were subjected to MC-ICP-MS measurement using the previously developed method at a Se concentration of 100 μg L−1. Throughout the sequence, the Se Merck solution was measured as a quality control solution at the beginning and at the end of the sequence and in-between every 6 samples for monitoring the accuracy of the isotope ratio measurements (δ82/78Se = −0.70 ± 0.09‰ and δ82/76Se = −1.07 ± 0.14‰, Mean ± 2SD, n = 7). Furthermore, the δ82/78Se value, obtained for the samples and the Se Merck solution, was plotted as a function of the corresponding δ82/76Se values. The three-isotope plot obtained is provided as Fig. 8.
![]() | ||
Fig. 8 Three-isotope plot of δ82/78Se vs. δ82/76Se of all data points for the tuna fish organs and for the different measurements of the Se Merck solution throughout the sequence. |
The δ82/78Se vs. δ82/76Se three-isotope plot of Fig. 8 shows a linear trend (R2 = 0.9871), with a slope of 0.6871, which closely matches the slope of the theoretical mass-dependent fractionation of 0.6497, calculated according to Young et al. (2002), assuming thermodynamically governed fractionation.38 This confirms that our results are accurate and not affected by spectral interference. For a further interpretation of the Se isotopic composition in tuna fish organs, the δ82/78Se results were plotted together with the Se concentration found in each organ. The results are shown in Fig. 9.
As shown in Fig. 9, δ82/78Se values for all tuna fish organs display a Se isotopic composition that is heavier than that of the standard (positive δ82/78Se values). The spleen had the highest Se content and displayed the lightest Se isotopic composition +0.17 ± 0.05‰ (n = 3, 1SD), whereas the liver showed the heaviest δ82/78Se value of all organs measured: +0.57 ± 0.07‰ (n = 6, 1SD). This is consistent with the previous observations of Marchán-Moreno et al. (2024)37 and Clark & Johnson et al. (2010)39 who also reported that the liver of fish (catfish, sunfish and carp) and seabirds (giant petrels) exhibited the heaviest Se isotopic composition of all organs analysed. This was attributed to the liver being the primary site for Se intake from the diet, from which Se is redistributed to other organs for various metabolic functions. The unutilized Se tends to accumulate in the liver and becomes enriched in heavier isotopes, as lighter isotopes are preferentially involved in the metabolic processes.37 The depletion in the heavier Se isotopes in the other organs (lighter isotopic composition) shown in Fig. 9 supports the hypothesis of lighter Se isotopes being more efficiently distributed from the liver to the other tissues.
When comparing the Se isotopic composition obtained in this work with that of Hg measured in the same organs by Wiech et al. (2024),6 a similar trend is observed. The authors showed that the liver exhibited the heaviest Hg isotopic composition, followed by the intestine and the kidney, while the spleen showed the lightest δ202Hg values. This pattern was attributed to differences in Hg speciation, particularly the methylmercury (MeHg) content, which was the highest in the liver and lowest in the spleen. Since during methylation, there is a slight preference for the heavier Hg isotopes being incorporated, MeHg is enriched in the heavier isotopes compared to inorganic Hg (iHg). Moreover, Wiech et al. (2024)6 reported that the masses of both Hg and Se present in the particulate form were the highest in the spleen and kidney, suggesting that HgSe nanoparticle formation predominantly occurs in these organs. This supports the idea that the spleen and kidney might play a key role in the Hg detoxification process by Se. Although coming from one individual fish only, the Se concentration and isotopic data obtained in this study support this view: in addition to the lowest content of MeHg, the spleen and kidney exhibited the highest Se concentration and the lightest Se isotopic composition. These initial results suggest that isotopic analysis can be an additional tool for investigating whether Se is actively involved in the demethylation of MeHg. It is important to highlight that, to the best of the authors' knowledge, this work is the first reporting data on the Se isotopic composition in marine fish organs and in tuna fish particularly. As such, data interpretation remains tentative due to the very limited availability of Se isotope ratio data in biological systems, particularly in marine organisms. In fact, the only data reported for biological samples are limited to fish and plants from a Se-contaminated lake,39,40 plankton from the Pacific Ocean,41 and more recently tissues (liver, kidney, muscle and brain) of a marine top-predator seabird.37 Therefore, based on these promising initial results, Se isotopic analysis of a wider collection of tuna fish organs (higher number of individuals) can aid in better understanding of the role of Se in Hg detoxification processes in marine fish.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5ja00196j |
This journal is © The Royal Society of Chemistry 2025 |