M.
Wälle
* and
C. A.
Heinrich
ETH Zurich, Institute of Geochemistry and Petrology, Department of Earth Sciences, Clausiusstrasse 25, 8092 Zurich, Switzerland. E-mail: waelle@erdw.ethz.ch; Fax: +41 44 632 18 27; Tel: +41 44 632 77 94
First published on 7th March 2014
A state-of-the-art, highly sensitive sector-field inductively coupled plasma mass spectrometer (SF-ICP-MS) was evaluated for analyzing fluid inclusions in combination with a 193 nm excimer laser ablation, with the aim of expanding the technique to smaller inclusions and/or lower element concentrations. A well-defined assemblage of numerous co-genetic fluid inclusions and thin layers (50 nm) of chromium and copper containing traces of gold were studied regarding reproducibility and detection limits. For comparison, aliquots were analyzed with a quadrupole (Elan 6100 DRC) and the SF-ICP-MS instrument (Element XR). While using an element menu of 21 elements covering the mass range from lithium (7 amu) to lead (208 amu), approximately ten times lower detection limits were found for the SF-ICP-MS, whereby the cycle time increased by only 20% compared with the quadrupole instrument. An absolute detection limit for e.g. gold of 1 femtogram (10−15 g) was found for fluid inclusions analysis. Detection efficiencies of 2.6 × 10−5 counts per ablated atom for copper and 3.1 × 10−5 for chromium were determined by ablating the thin layers. The detection efficiency for sodium in the fluid inclusions was 2 × 10−7, about five times lower than that expected from the sensitivity obtained on NIST SRM 610 glass.
The small size of natural as well as synthetic fluid inclusions, typically ranging from a few microns up to a few tens of microns in most samples, remains an ongoing challenge in many applications. The smaller inclusion size affects LA-ICP-MS in two ways: it reduces the absolute mass of any element to be detected, but it also leads to shorter signals that are more difficult to quantify in a representative manner.
Absolute detection limits, largely determined by inclusion mass and the concentration of the elements of interest contained in an inclusion, are the first-order limitations in applying fluid inclusion microanalysis to resolve important geochemical questions in hydrothermal ore formation as well as metamorphic and magmatic petrology. Small inclusions of dilute fluids forming in low-temperature geological environments have been largely inaccessible to microanalytical studies, which is regrettable because smaller fluid inclusions occur in far greater numbers and may commonly be better preserved than larger ones. However, going to smaller inclusions means lowering the total mass available for an analysis. This is particularly critical for economically interesting trace elements such as gold, which is commonly present in concentrations below 1 μg g−1 and therefore close to or below the detection limit in a wide range of inclusions. Reducing the absolute amount in an inclusion by going down to the smallest possible size in LA-ICP-MS primarily requires maximizing the sensitivity of the ICP-MS,31 although for some elements the background intensity is the limiting factor (e.g., anion components like S, Cl, and Br (ref. 32)).
The duration of small and highly transient signals, typically showing an almost instantaneous rise in intensity after the inclusion is breached and a more gradual decline depending on ablation progress, is the second limiting factor in LA-ICP-MS microanalysis of fluid inclusions. Representative signal quantification of multiple elements across a wide range of atomic masses requires an adequate definition of this time-dependent signal. Simultaneous detection using a multi-collector ICP-MS is limited by the small mass range of these magnetic-field based spectrometers and the need to include Na as an internal standard for quantifying natural fluid inclusion compositions.21 The recently introduced Mattauch-Herzog ICP-MS33 using a detector plane and a time of flight ICP-MS34 both allow simultaneous detection across the entire mass range. Although, recent applications show a similar sensitivity to Q-ICP-MS instruments,34 their dynamic range, from major (e.g. percents of Na) to trace elements (e.g., ng g−1 Au) present in single inclusions, so far precludes useful applications to this type of microanalysis.
With sequential detection of elements, a compromise must be achieved between shortening the signal (leading to a greater chance of detection of a given total mass of an element above the instrumental background) and a representative sampling of all elements of interest (requiring an adequate number of significant readings of all elements that are counted successively during each acquisition cycle). The use of short peaks in a single collector ICP-MS using a sequential acquisition method raises the risk of spectral skew.35 Such non-representative sampling may lead to systematic errors in individual inclusion analyses and can only be corrected by analyzing and averaging numerous inclusions considered to have identical compositions. Thanks to its rapid element scanning through the entire mass range, quadrupole mass spectrometry (Q-ICP-MS) has been the detection method of choice for many years of fluid inclusion research. Today, state-of-the-art single-collector sector-field ICP-MSs have comparably fast-scanning magnets, but considerably higher sensitivities compared to Q-ICP-MS, especially with sample introduction by liquid nebulization but also in combination with laser ablation36,37 and electrothermal vaporization (ETV).38 ETV signals have a similar duration to LA signals from fluid inclusions, so that ETV experiments38 also show the suitability of the Element XR to record fast changing transient signals. According to Resano et al.38 about 20 different masses can be reliably measured in a few second long ETV signal using a SF-ICP-MS. However, spectral skew is less of an issue in these analyses because measurements are easy to replicate, in contrast to fluid inclusions where each microsample has a finite mass.
In this study, we explore the suitability of a state-of-the-art SF-ICP-MS for quantifying low short transient signals of multiple elements across a wide mass range, by the ablation of thin layers of known analyte density and of a well-defined assemblage of numerous compositionally identical fluid inclusions. A Q-ICP-MS (Elan 6100 DRC) was used for direct comparison using the same ablation optics and aerosol transport system, using He as the sample-chamber gas merged with Ar (± minor H2) downstream from the sample cell.
(1) |
Elan 6100 DRC | Element XR | |
---|---|---|
Carrier gas | 1.1 L min−1 He + 5 mL min−1 H2 | 1.0 L min−1 He |
Nebulizer gas flow | 0.8–0.82 L min−1 Ar | 0.946–0.950 L min−1 Ar |
Auxiliary gas flow | 0.85 L min−1 Ar | 0.95 L min−1 Ar |
Cooling gas flow | 15.5 L min−1 Ar | 15 L min−1 Ar |
Plasma power | 1550 W | 1350 W |
Dwell times | 10 ms (Au: 80 ms) | 10 ms (Au: 80 ms) 5 samples per peak |
Cycle time | 343 ms | 418 ms |
Isotopes (for fluid inclusions): | 7Li, 11B, 23Na, 24Mg, 27Al, 29Si, 39K, 44Ca, 55Mn, 57Fe, 65Cu, 66Zn, 75As, 85Rb, 88Sr, 107Ag, 121Sb, 133Cs, 137Ba, 197Au, 208Pb | |
Oxide ratio (ThO+/Th+) | ∼0.5% | ∼0.3% |
Thin layers (50 nm) of chromium and copper on a glass slide were produced by physical vapor deposition. A microscope cover glass (thickness ∼ 0.2 mm) was glued on top of these layers to allow controlled ablation and to avoid erratic flaking off the crater rim. These sandwiched layers were ablated with a 90 μm spot which (due to the high numerical aperture of the imaging objective and the resulting conical ablation pit20) sampled a 80 μm circle of the layer, as determined by optical microscopy after ablation. Trace concentrations of ∼2 ppm Au in chromium and ∼40 ppm Au in gold were found by LA-ICP-MS measurements. These transient gold signals are close to the detection limit of the Elan 6100 DRC instrument. They resemble transient signals from fluid inclusion but are more reproducible in terms of absolute gold mass, thus allowing a direct comparison of the sensitivities of both instruments.
The ablation rate on NIST SRM 610 was determined by ablating three craters (40 μm) for 30 s with a repetition rate of 10 Hz, i.e. 300 laser shots each. We ablated the side of a thin slice of doubly polished NIST SRM 610, using the same fluence (5.5 J cm−2) as for the standard measurements for fluid inclusion analysis. Afterwards the depth of the crater was measured with a microscope placed perpendicular to the craters. The measured depth of the flat-bottomed craters was 48 μm resulting in an ablation rate of 0.16 μm per laser pulse.
We used an assemblage of numerous fluid inclusions on a single healed microfracture in a quartz crystal from an Alpine fissure vein found near Thusis, Switzerland,41 ranging in size from a few microns to ∼200 μm. All fluid inclusions have an identical salinity of 4.0 ± 0.1 wt% NaCl equivalent and contain an aqueous liquid and a small vapor bubble homogenizing at 130 ± 5 °C, but no daughter crystals.41 The average diameter of each inclusion was measured in a microscope before ablation and a spherical symmetry was assumed to estimate the inclusion volume.
Sample | Isotope | Elan 6100 DRC [counts per ablated atom] | Element XR [counts per ablated atom] |
---|---|---|---|
Copper layer (50 nm) | 65Cu | 3.7 × 10−6 | 2.6 × 10−5 |
197Au | 1.3 × 10−5 | 1.1 × 10−4 | |
Chromium layer (50 nm) | 53Cr | 2.7 × 10−6 | 3.1 × 10−5 |
197Au | 9.8 × 10−6 | 1.0 × 10−4 | |
Fluid inclusions | 23Na | 8 × 10−9 | 2 × 10−7 |
The higher sensitivity and suitable time resolution of the transient signal of the Element XR is demonstrated in Fig. 1. Two otherwise identical fluid inclusions of ∼55 μm and ∼25 μm in diameter were analyzed with the Elan 6100 DRC and the Element XR respectively; the first inclusion is about ∼10 times larger by volume and contained mass. Backgrounds are generally higher on the Element XR than on the Elan 6100 DRC. This is especially pronounced for sodium and to a smaller extent for lithium backgrounds. The potassium background is similar due to the 38ArH+ interference on the Elan 6100 DRC, caused by the hydrogen addition to the carrier gas. Strontium, cesium and boron were consistently detected as major signals by both instruments and in all inclusions, besides Na. Their average concentrations (± one standard deviation) determined with the Element XR and the Elan 6100 DRC, respectively, were 39 ± 16 and 35 ± 22 μg g−1 (Sr), 46 ± 17 and 50 ± 36 μg g−1 (Cs), and 670 ± 155 and 720 ± 295 μg g−1 (B). This indicates no significant difference between the measurements from the two instruments. The distribution of the obtained strontium concentrations in relation to the inclusion size is shown in Fig. 2. Other elements like antimony, barium, lead and rubidium (Fig. 3) also show consistent concentrations or limits of detection in the smaller inclusions. The measurements of those elements clearly demonstrate the advantage of the Element XR for quantifying trace element concentrations in smaller inclusions. Detection limits for gold concentrations as a function of inclusion size are shown in Fig. 4 and indicate that the detection limit is about one order of magnitude lower for the Element XR compared to the Elan 6100 DRC. The trend lines indicate the expected correlation of a homogenous assemblage with the volume of near-spherical inclusions, indicating an absolute limit of detection of 1 fg (10−15 g) gold for the Element XR and about 10 fg (10−14 g) gold for the Elan 6100 DRC under optimized conditions. These trend lines are calculated from the LOD and the inclusions size, assuming a bulk density of 0.95 g cm−3 of the inclusions corresponding to 5 volume% vapor bubbles. Both datasets of individual inclusions follow such a trend, except for inclusions with diameters greater than 100 μm, which have only been measured with the Elan 6100 DRC and may not have been completely ablated at the maximum available crater size of 90 μm. Also, minimum detected concentrations (LOD) for very large inclusions do not further improve, because signals become longer and are increasingly affected by background intensities on minor elements, as already discussed by Günther et al.21
Our data further allow an estimate of detection efficiency for Na in fluid inclusions compared to solid standard materials. Knowing the size of an inclusion allows estimating the amount of liquid it contains. With the estimated density and the salinity determined by microthermometry, the absolute amount of sodium in each inclusion can be calculated. Relating the calculated masses of Na to the integrated signal intensities gives a detection efficiency (see Table 2), which is considerably lower than the ones reported earlier using NIST SRM 610, 612 and 614 based on determining the ablated volume by profilometry.31 Calculating the expected sodium intensities from the ablation rate of NIST SRM 610, its sodium concentration and the crater volume, the inclusion size and sodium content lead to higher sodium intensities than the actual measured ones as shown in Fig. 5. The measured integrated sodium intensities represent just 14% (Elan 6100 DRC) and 22% (Element XR), on average for medium sized inclusions (25 to 90 μm), of the intensities expected from NIST glass ablation. A minor offset in the calculated values may originate from the different sensitivities obtained on different days, which were not resolvable by the tuning procedure. The scatter in the measured sodium counts in the smaller inclusions is likely related to asymmetric inclusions shapes and a resulting spherical asymmetry. Nevertheless, the detection efficiency from fluid inclusions is significantly lower than that obtained by ablating homogeneous solids. This signal deficiency may either be due to a less efficient transport of the ablated liquid from the inclusion, compared to the aerosol ablated from a solid material, a less efficient ionization in the ICP or a less efficient ion extraction from the ICP.
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