Laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) U–Pb carbonate geochronology: strategies, progress, and limitations
Laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) U–Pb geochronology of carbonate minerals, calcite in particular, is rapidly gaining popularity as an absolute dating method. The high spatial resolution of LA-ICP-MS U–Pb carbonate geochronology has benefits over traditional isotope dilution methods, particularly for diagenetic and hydrothermal calcite, because uranium and lead are heterogeneously distributed on the sub-millimetre scale. At the same time, this can provide limitations to the method, as locating zones of radiogenic lead can be time-consuming and “hit or miss”. Here, we present strategies for dating carbonates with in situ techniques, through imaging and petrographic techniques to data interpretation; our examples are drawn from the dating of fracture-filling calcite, but our discussion is relevant to all carbonate applications. We review several limitations to the method, including open-system behaviour, variable initial-lead compositions, and U–daughter disequilibrium. We also discuss two approaches to data collection: traditional spot analyses guided by petrographic and elemental imaging and image-based dating that utilises LA-ICP-MS elemental and isotopic map data.
Calcite (CaCO3), along with other carbonate minerals (e.g. aragonite, dolomite, magnesite), forms in a wide variety of geological environments as both a primary and secondary mineral phase, including diagenetic, biogenic, igneous, metamorphic, and hydrothermal environments. Calcite can incorporate uranium upon its formation, making it a potentially suitable chronometer for U–Pb and U–Th geochronology. Calcite geochronology therefore has the potential to provide direct timing constraints to a broad suite of geoscience applications. Calcite has been dated in the past by chemical dissolution and isotope dilution (ID) with measurement by either Thermal ionisation mass spectrometry (TIMS) or inductively coupled plasma mass spectrometry (ICP-MS) (e.g. Smith and Farquhar, 1989; DeWolf and Halliday, 1991; Brannon et al., 1996; Rasbury et al., 1997; Richards et al., 1998; Woodhead et al., 2006; Pickering et al., 2010), collectively referred to here simply as ID. More recently, there has been a proliferation in the use of laser ablation (LA-) ICP-MS applied to calcite geochronology (Li et al., 2014; Coogan et al., 2016; Roberts and Walker, 2016; Ring and Gerdes, 2016; Methner et al., 2016; Goodfellow et al., 2017; Burisch et al., 2017, 2018; Drake et al., 2017, 2019, 2020; Hansman et al., 2018; Hellwig et al., 2018; Godeau et al., 2018; Beaudoin et al., 2018; Bertok et al., 2019; Drost et al., 2018; Mangenot et al., 2018; Nicholson et al., 2020; Nuriel et al., 2017, 2019; Parrish et al., 2018; Walter et al., 2018; Yokoyama et al., 2018; Smeraglia et al., 2019; Holdsworth et al., 2019; MacDonald et al., 2019; Scardia et al., 2019). Presently, we are not aware of successful secondary ion mass spectrometry (SIMS) U–Pb dating of carbonate mineralisation, but this presents an alternative microbeam method to laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS).
The first review of the possibilities for carbonate geochronology was published by Jahn and Cuvellier (1994), and this was substantially updated by Rasbury and Cole (2009). The latter provided up-to-date discussion on U–Pb isotope systematics in carbonates, particularly regarding Pb–Pb and U–Pb isochron methods, as well as a review of the applications to date. At that time, both marine- (e.g. limestone, dolomite) and meteoric-water-sourced carbonates (e.g. speleothems and tufas) had received the most attention, due to their often favourable uranium contents, and studies of hydrothermal carbonate were scarce (e.g. Brannon et al., 1996; Grandia et al., 2000). U–Pb dating of speleothems has been further reviewed by Woodhead et al. (2006, 2012), focussing on data generated by ID, and more recently Woodhead and Petrus (2019) have discussed the use of LA-ICP-MS for speleothem dating.
Now that microbeam (i.e. LA-ICP-MS and SIMS) U–Pb geochronology is proving to be a useful method for a range of geoscience applications, it is pertinent to address what can be achieved with the method, what the current limitations are, and where improvements can be made in the future. We refer to LA-ICP-MS through the rest of this paper, but acknowledge that nearly all of the points we cover are equally relevant to SIMS methods. The key benefit to LA-ICP-MS dating is that its high spatial resolution can be used to relate U–Pb and other geochemical analyses to imaged textures. This is critical for providing context to the obtained dates. Carbonate materials are heterogeneous in composition elementally, isotopically, and texturally. These factors can all lead to scatter in U–Pb data and will often hinder the ability to generate high-precision (i.e. <1 % 2σ) U–Pb dates. In fact, after propagation of all relevant uncertainties, final LA-ICP-MS U–Pb dates typically exceed 3 % precision (2σ). For this reason, LA-ICP-MS carbonate U–Pb geochronology is particularly suited for applications in tectonics and crustal fluid flow but commonly less suited for applications in stratigraphy and palaeoclimate.
Here we present a review of LA-ICP-MS U–Pb carbonate geochronology, focusing on its benefits, application, and limitations. We pay particular attention to hydrothermal and diagenetic carbonates; these can constrain the ages of mineral systems, crustal deformation, and fluid flow and represent a significant growth area for this method. Using several case studies, we highlight the utility of image-guided analysis, where various imaging techniques provide critical context for interpreting U–Pb data. We also provide case studies for an age-mapping technique that is an alternative to traditional static spot ablation and can be used in combination with sample imagery to generate U–Pb age data. Finally, we highlight issues surrounding initial-lead compositions, initial disequilibrium in the U–Pb system, and open-system behaviour.
Geochronology by ID provides the most accurate assessment of the U–Pb age of a sample, through the use of calibrated isotopic tracer solutions, but it is time-consuming and requires a clean laboratory facility for sample dissolution and column chemistry. The spatial resolution of ID is typically much lower than that offered by microbeam techniques, although resolution can be increased by using a high-precision micro-drill for direct sampling. A major limiting factor is that carbonate materials typically have very low U concentrations (ca. 10 ppb to 10 ppm U) compared with traditional U-bearing accessory minerals (e.g. often >100 ppm U in zircon). This means that samples with low Pb concentrations yield higher blank∕sample ratios, hindering the accuracy and precision of the resulting data, and secondly that the comparatively large volumes of material needed for ID analyses result in an “averaging” effect and a reduction in spread in U∕Pb space.
LA-ICP-MS is a much quicker technique than ID and therefore less expensive per analysis. Several samples can be run in a single day, meaning the technique is ideal for screening of large sample sets to find the most suitable material. The effect of blanks sourced from dissolution and chemical purification is negated, and very low (<100 ppb) Pb contents can be analysed. However, LA-ICP-MS is generally less precise analytically compared to ID approaches. Another major limitation is the need to normalise to a matrix-matched reference material. This means that the uncertainty of the reference material becomes a limiting uncertainty, and matrix effects between materials of different composition will generate scatter and/or bias in the U–Pb dates that are difficult to correct for.
The biggest benefit of LA-ICP-MS comes from the spatial resolution (less than ca. 100 µm) at which data can be obtained, particularly given the length scales of uranium concentration heterogeneity in carbonate. We find that for hydrothermal and diagenetic calcite in particular, uranium is heterogeneously distributed across veins and vein phases and within individual crystals (see Fig. 1). Uranium concentration heterogeneity typically spans 1 to 3 orders of magnitude, with the length scale of this variation being commonly much less than 1 mm. Targeting of high-U domains is therefore difficult without a high spatial-resolution sampling method. Intracrystalline uranium distributions within calcite define several patterns (see Fig. 1): concentrated along cleavage planes (a), growth-zone controlled (c, d, and f), concentrated towards grain rims (areas of b and e), and with apparent disorder (areas of b and e). Laser ablation has the spatial resolution capable of targeting such elemental (and isotopic) zonation, making it easier to avoid distinguishable alteration zones and inclusions at the 10–100 µm scale.
For common-lead-bearing minerals such as calcite, the extreme range in parent∕daughter ratios encountered (quoted here as 238U divided by initial lead as 204Pb; a ratio known as μ) means that ID does not always lead to an improvement in precision on the regressed age. This is demonstrated by the schematic model in Fig. 2. Sampling for ID provides an average of elemental and isotopic zonation within the analytical volume, perhaps >1 mm3, depending on the concentration of U and Pb within the crystal(s). The resulting data should be precise (depending on the sample∕blank ratios), but may potentially have a small spread in parent∕daughter ratios (i.e. 238U∕206Pb) due to the averaging effect during sampling. In contrast, LA sampling has the potential to target and utilise such zonation, better resolving endmember μ compositions, and resulting in analyses with a greater spread in 238U∕206Pb ratios. This potentially improves the resolving power of a regression of the measured isotopic ratios allowing the definition of, ideally, the high-μ (radiogenic lead) and low-μ (initial lead) endmember compositions of the data array (see Fig. 2). Along with the generally high-n datasets generated by the LA-ICP-MS approach, these well-constrained regressions can result in a similar precision for 206Pb∕238U ages than those using ID data alone.
When calculating an age and uncertainty from a regression or isochron, it is assumed that (1) the dataset describes a single age population whose variability or scatter is derived solely from the analytical process, (2) each analysis represents a closed system, and (3) all analyses share the same initial Pb isotope composition. When these assumptions are satisfied, the MSWD should be about 1 (mean squared weighted deviation; Wendt and Carl, 1991). LA-ICP-MS data points generally have a lower precision than those derived by ID. These lower-precision data points can mask scatter that exists within the level of the data-point uncertainties. This caveat must be considered when interpreting regressed data (or weighted means). In other words, age interpretations rely on isochron assumptions that can only be resolved at the level of the data-point uncertainties. More precise ID data, therefore, have better resolution of scatter and better constrain the likelihood that a sample does not comprise a single population. However, sampling for ID can also contribute to this scatter by analysing larger amounts of material, with a greater chance of including altered zones or zones from different generations. For applications where the best possible precision is needed (e.g. for stratigraphic constraints or characterisation of potential U–Pb carbonate reference materials), a workflow involving both LA-ICP-MS dating followed by ID on the most favourable material is likely to be the most effective. For applications where the required precision is on the order of several percent, image-guided LA-ICP-MS without ID is suitable.
3.1 μ (238U∕204Pb) in carbonate
An “ideal” U–Pb chronometer requires the incorporation of U (the parent isotopes 238U and 235U, which decay to 206Pb and 207Pb, respectively) and zero or low concentrations of initial (or “common”) Pb during its formation; this is typically expressed as the ratio of parent uranium to initial Pb – 238U∕204Pb or μ. In addition, both the parent and daughter isotopes ideally remain a closed system from formation until the present day. Many chronometers lack these ideal criteria but still provide successful materials for dating: the subset of “common-lead-bearing chronometers” comprise small to large initial-lead concentrations that are of uniform composition (e.g. titanite, apatite). The ideal criteria are generally rare in carbonates, but many carbonate materials from a range of different geological environments are successful common-lead-bearing chronometers. Rasbury and Cole (2009) showed that carbonates of meteoric origin have the highest μ values and hydrothermal varieties the lowest, with marine varieties in the middle (see Supplement Fig. S1). However, the recent literature on calcite dating demonstrates that with careful characterisation and sampling, high-μ domains can be found in a range of hydrothermal and diagenetic calcite.
The amount of U needed to generate an age is dependent on two factors: (1) the age of the material and (2) the initial μ ratio of the material. The younger a sample is, the less time there is for the growth of radiogenic daughter Pb from parent U. With a higher μ, the ratio of measured radiogenic Pb to common (initial) Pb will be higher, giving greater confidence and (in general) precision and accuracy to the resulting age determination. The effect of these factors is shown in Fig. 3. Two Tera–Wasserburg plots are shown, with isochrons for samples of different ages (100 to 10 Ma in panel a; 1000 to 100 Ma in panel b). The most accurate and precise age determinations, i.e. those that can be interpreted with most confidence, are generated when the sample comprises abundant radiogenic lead, i.e. gets close to the lower part of the concordia curve where the regression intercepts. Each plot shows regressions for individual samples between a common-lead composition (∼0.8) and a radiogenic endmember (with the age labelled). The colour-coded points along each regression reflect the amount of radiogenic lead that will be created by decay of 238U, based upon the given μ value. For example, utilising the plot in panel a, a sample of 15 Ma, with a μ of 10 000, will have a measured 207Pb∕206Pb of ∼0.4, equalling about a 50:50 ratio between radiogenic and initial lead. To get a near-concordant measurement of this sample would require a μ value of over 200 000. These plots demonstrate that when simply regarding the abundance of radiogenic lead, older samples are more amenable to dating than those young in age. The preservation of a closed isotopic system over long time periods is what makes dating old samples (i.e. Precambrian materials) potentially difficult.
In the absence of concordant analyses, both high μ and a significant spread in initial μ values are required to generate the most robust ages, as these will pin the isochron at the radiogenic endmember with greater confidence. Some calcite exhibits sufficiently high μ to generate concordant data (e.g. Richards et al., 1998; Roberts and Walker, 2016; Nuriel et al., 2017); these ages do not heavily rely on the composition of the common-lead endmember, but such ages are rare with a material that so commonly exhibits high initial-lead abundances. Ages can be derived from isochrons with low amounts of radiogenic lead, i.e. those with low μ . Such isochrons can be regressed to provide lower-intercept ages, but the confidence in these ages is subject to having well-behaved data conforming to a single population, requiring precise data-point uncertainties (e.g. Fig. 4g). Such low μ isochrons can potentially give imprecise and even inaccurate lower-intercept ages, and thus confirmation through multiple samples and/or alternative age constraints is favoured.
In Fig. 4, we present a selection of “real-world” data to highlight the potential complexity of carbonate U–Pb data. These data from natural samples broadly range from undesirable to most desirable from a to i, with the following notable characteristics.
Dominated by common lead with large data-point uncertainties (due to low count rates) that hamper the distinction between open-system behaviour and radiogenic ingrowth of lead.
All analyses are ca. 100 % common lead, with high count rates providing a precise measurement of the composition of this common lead.
Mixed and scattered data that do not fall on a single linear isochron. This is likely caused by open-system behaviour, potentially involving both addition and subtraction of parent 238U.
Majority of data define a linear array with a large spread in U∕Pb ratios. Some other analyses fall on a horizontal array, suggesting they experienced open-system behaviour (e.g. local 238U mobility).
Data form an apparent single linear array, but large uncertainties (due to low count rates) may obscure mixed ages or minor open-system behaviour.
Dominated by relatively radiogenic isotopic compositions, but with large data point uncertainties due to low count rates. The narrow range in μ leads to a large age uncertainty from extrapolating to the lower concordia intercept. The age uncertainty would be improved with a common-lead composition estimated from contemporaneous low-μ samples of the same suite.
A short isochron, termed a “small-scale isochron” by Ring and Gerdes (2016). There are no radiogenic isotopic compositions to anchor the extrapolation to a lower-intercept concordia date, but a tight data array yields a realistic intercept age.
Dominated by radiogenic isotopic compositions, and the spread in the array provides a precise lower-intercept date; small data-point uncertainties improve the ability to identify potential outliers.
A precise regression due to well-behaved closed system behaviour, high count rates giving small uncertainties, and a large spread in U∕Pb ratios providing a precise estimate of both the age and the common-lead isotopic composition.
3.2 U and Pb contents in carbonate
At present, there is a lack of predictive criteria that can be used in the field or in the laboratory to screen samples prior to analysis for high-μ domains. Radionuclide incorporation in calcite is not well understood despite several decades of interest, primarily driven by the field of nuclear waste storage and characterisation (e.g. Langmuir, 1978; Milton and Brown, 1987; Sturchio et al., 1998; Reeder et al., 2000, 2001; Kelly et al., 2003; Weremeichik et al., 2017; Drake et al., 2018). This is because trace element incorporation in calcite does not rely on thermodynamically determined partition coefficients but on a large number of phenomenological variables, including trace element availability, calcite growth rate, temperature, pH, Eh, pCO2, and the ratio in solution, ionic size, and U complexation. Furthermore, different trace elements can be preferentially incorporated into structurally different growth steps and faces of growing calcite crystals (Paquette and Reeder, 1995; Reeder, 1996).
Rasbury and Cole (2009) provided a geochronology-focused review of U and Pb in calcite, and we note the following salient features: (1) Pb is both particle reactive and relatively insoluble; (2) Pb is found at very low levels in most fluids (ppt–ppb), providing high Ca∕Pb ratios; (3) Pb can be substituted for Ca in the crystal lattice, although the Pb cation is larger – ionic radii of Ca2+ and Pb2+ in 6-fold coordination are 114 and 133 pm, respectively; (4) U exists in multiple oxidation states, and its solubility is strongly affected by Eh and pH; and (5) both U(VI) and U(IV) states have been found in calcite, but not with both states together in the same sample.
Points 4 and 5 above are important for understanding why and when uranium is incorporated into calcite and whether remobilisation is likely. Sturchio et al. (1998), using a combination of X-ray absorption spectroscopy and X-ray microprobe fluorescence, demonstrated that the uranium in a sample of spar calcite was in the form of U(IV) and that U(VI) was less likely based on size and ionic structure (ionic radii of U(IV) and U(VI) in 6-fold coordination are 103 and 93 pm, respectively). Given that U(IV) is less mobile than U(VI), this study provided important support for U–daughter geochronology. Kelly et al. (2003), however, found that U(VI) as uranyl () was the dominant species in a natural sample of vein calcite, which they considered to be more representative of typical low-U material than the Sturchio sample. Drake et al. (2018) found much higher concentrations of uranium in calcite precipitated from deep anoxic groundwater than experimental determinations that were performed in oxic conditions, and they interpreted this high uranium uptake as being due to the incorporation of U(IV) and thus that the partition coefficient for U(IV) in these environmental conditions is orders of magnitude larger than for U(VI). It is evident that more data from natural carbonates in different settings are needed to more fully understand the controls on U and Pb incorporation.
We have compiled uranium and lead concentration data from carbonates analysed in the British Geological Survey (BGS) laboratory over several years (Fig. 5). From our data, we see that median U and Pbtotal concentrations are 1.9 and 0.003 ppm, respectively. Diagenetic carbonate has the second-highest median uranium content (0.4 ppm), but also has a high Pb content (0.35 ppm). Veins in both terrestrial and mid-ocean ridge settings have low U and Pb contents, with median values well below 100 ppb for both. Biogenic samples, although a smaller dataset, have low contents of U and Pb, generally lower than diagenetic material. Note that this compilation presents total Pb contents, and includes radiogenic Pb as well as initial Pb. The samples in Fig. 5 are mostly younger than 200 Ma or <4 Ma for the speleothems. The concentration data and U∕Pb ratios demonstrate that speleothems in general are much more amenable to U–Pb geochronology, which is why they have been the main focus for this method until the last few years. Dating diagenetic and vein-fill calcite, with more variable and lower contents of U and higher contents of Pb, has a lower chance of success than speleothems (although it should be noted that the speleothems in general have already been visually pre-screened during sampling).
Ideally, a predictive framework could be constructed to aid field sampling and laboratory-based sub-sampling of carbonate material for geochronological analyses. However, given the large number of variables controlling U and Pb in carbonate, it is unlikely that such a tool can be developed without measuring a large number of parameters in the mineralising or diagenetic system. Relevant information might include the redox history of the system. For example, oxidising fluids may mobilise U as U(VI), which is soluble in hydrous fluids, leading to U loss during fluid–mineral interaction. Conversely, U may undergo much higher precipitation into the mineral phase at redox fronts representing reducing conditions, since reduced U(IV) has lower solubility. Other pertinent information for predicting success includes the nature of the host rock and the source of the fluids. For example, if the mineralising fluids transmit through Pb-rich units, then an undesirable enrichment in the fluid Pb∕Ca may potentially take place, leading to lower initial 238U∕204Pb.
The complex nature of trace element uptake, including Pb and U, in carbonate mineralisation is exemplified by recent studies in hydrothermal settings. Fracture mineralisation in the crystalline basement of southern Sweden has been investigated extensively to evaluate potential geological nuclear waste repository facilities. Several studies have shown that most trace element concentrations vary over an order of magnitude within calcite samples (at the thin section scale), and up to several orders of magnitude across individual fractures (Drake et al., 2012, 2014; Maskenskaya et al., 2014; Milodowski et al., 2018). These authors suggest that (1) trace element chemistry does not trace the source rock of the metals; (2) the co-variation in most trace elements implies changing metal ∕ Ca ratios in the fracture waters; and (3) in situ factors affect trace element incorporation, such as microbial activity, metal speciation, crystal habit, water type, and co-precipitation of other phases such as barite and pyrite. Our own experience of vein-filling fractures matches these previous studies, as shown for example by the basalt-hosted calcite in the Faroe Islands (see Fig. 7).
As discussed above, it is difficult to predict which carbonate samples are most suitable for U–Pb geochronology. We therefore utilise several methods to screen material, with the aim of limiting the time wasted on unsuitable samples, improving the quality of data that are collected, and enhancing the overall efficacy of LA-ICP-MS U–Pb carbonate geochronology. The purpose of sample imaging is two-fold: it provides important spatial characterisation of U and Pb within the sample and also provides the petrographic and compositional context to assess mineral growth mechanisms and alteration textures that are critical for linking dates to processes.
4.1 Non-destructive techniques
A range of non-destructive imaging techniques are available for sample imaging (see Fig. 6), including optical microscopy, cathodoluminescence (CL), back-scattered electron imaging (BSE), charge-contrast imaging (CCI), and etch-track or digital autoradiography techniques. Both reflected light and transmitted light are excellent tools for characterising carbonate minerals; the latter being the mainstay of all petrographic analysis. Features which are usefully distinguished in transmitted light include twinning planes, fluid inclusions, and grain boundaries (see Fig. 6e). Reflected light is a particularly useful technique for characterising carbonates in polished blocks, when thin sections are not available, and it also highlights crystal boundaries and contrasts between different mineral faces (see Fig. 6a and b).
In carbonate minerals, CL intensity is related to trace element contents but not specifically U concentration. CL brightness is generally ascribed to a number of emitters, with Mn2+ being the most dominant luminescence activator and Fe2+ being the dominant luminescence quencher in calcite and dolomite (e.g. Machel, 1985, 2000; Savard et al., 1995), although rare earth elements (REEs) such as Eu2+, Eu3+, Dy3+, Sm3+, and Tb3+ along with Pb2+ may also activate luminescence in some cases (Richter et al., 2003). Despite not being directly related to U, the very high spatial resolution of CL is useful for identifying micrometre-scale calcite crystal growth zonation and alteration (Fig. 7a and b) and for characterising different mineral generations formed from different fluids (e.g. Barnaby and Rimstidt, 1989; Tullborg et al., 2008; Milodowski et al., 2018).
BSE imaging (see Fig. 6c and d) also does not correlate directly with trace concentrations of uranium but with the mean atomic number of the mineral. It is useful as an imaging tool for characterising zonation, alteration, and growth patterns, although we note that the contrast in zonation largely reflects variations in major element composition, and as such it is typically less sensitive than CL. Ukar and Laubach (2016) provide a recent review of high spatial-resolution scanning electron microscope (SEM)-based imaging of vein-filling calcite mineralisation.
CCI under the SEM directly images differences in dielectric properties, which produce charge or conductivity contrasts in the near surface of the sample that are detected by the secondary electron emission and may reflect compositional variations or strain induced by deformation (Watt et al., 2000; Robertson et al., 2005). Although the exact origin of charge contrast is poorly understood, it can provide useful information on crystal growth, compositional zoning, and microstructural features (see Fig. 6a). It is an underutilised method for geological materials and has been previously applied to garnet (Cuthbert and Buckman, 2005), feldspar (Flude et al., 2012), limestone (Buckman et al., 2016), and biogenic calcite (Lee et al., 2008). The technique requires very clean and carefully prepared and polished sample surfaces because it is sensitive to surface contamination and mechanical defects, and imaging needs to be undertaken on uncoated samples under low-vacuum conditions.
In addition to the microscopy-based methods listed above, a lower-resolution but potentially useful technique is provided by storage-phosphor imaging-plate (IP) autoradiography using a plastic support film coated with a photostimulated phosphor () (Hareyama et al., 2000). This technique records an image of the spatial distribution and intensity of total radioactivity (from alpha, beta, and gamma emitters) from a flat sample surface. In natural geological materials, IP radiography records radioactivity from U, Th (and their radioactive daughters), 87Rb, and 40K (Hareyama et al., 2000; Cole et al., 2003). Although U is not specifically discriminated, it has been shown to be a useful screening tool for finding U-bearing domains in carbonate materials (Cole et al., 2005; see Fig. 6f). The method has been particularly applied to speleothem studies where its large sample-size capabilities (up to at least 40 cm) are beneficial. Spatial resolution is a few tens of micrometres, depending on the pixel size of the laser scanner. However, the detection limit depends on the exposure time of the IP in direct contact with the sample surface: routinely this is around 14–28 d, giving a detection limit of a few parts per million U, which is typically higher than many carbonate samples. Whilst this may be suitable for speleothems, which typically have higher uranium concentrations, we do not regularly adopt the method for very low U contents in vein-filling or diagenetic carbonates.
Fluorescence imaging has long been used in defining and characterising growth fabrics in speleothems, although it does not specifically identify U-rich regions. This usually involves irradiating a sliced sample with UV light and observing the excited fluorescence emission at a longer (visible light) wavelength, using either a standard UV microscope or digital scanning with a UV laser system (e.g. Shopov et al., 1994; Baker et al., 1995, 2008; Perrette et al., 2005). Fine growth detail with spatial resolutions of between 50 to 100 µm are achievable. Speleothem fluorescence under UV at excitation wavelengths of 300–420 nm is dominated by the intrinsic fluorescence of natural high molecular weight and aromatic organic (“humic” and “fulvic”) compounds, with emission between 400–480 nm (Baker et al., 2008). However, we have also successfully imaged speleothems (see Fig. 6f) and other geological materials (Field et al., 2019) by direct laser-stimulated scanning fluorescence imaging (LSSFI) using 635 nm (red) and 450 nm (blue) wavelength excitation with 650 and 520 nm low-pass wavelength filters, respectively. Although, such equipment is principally applied to the imaging of biological materials labelled with organic fluorescent dyes (fluorochromes) (e.g. fluorescein), it is able to image variations in fluorescence originating from organic laminae and subtle differences between carbonate minerals (calcite, aragonite), revealing microtextural details with a resolution of about 100 µm.
4.2 Destructive techniques
Several approaches for destructive sample screening using LA-ICP-MS are available. These can include either systematic or non-systematic (random) spot traverses across carbonate samples and can include full analyses (i.e. a 30 s ablation following a pre-ablation) or a much shorter analysis time (with or without pre-ablation). We commonly adopt systematic traverses across samples utilising shorter ablation times but including a pre-ablation, so as to avoid common Pb from the surface. This is a quick way to determine with reasonable precision and accuracy whether a sample is a single age population that represents a closed isotopic system with a suitable range in μ. For some samples, this provides potentially useable age information that does not require any further refinement (e.g. Fig. 4h–i). Conversely, this may provide a population of data that exhibits no potential, i.e. dominated by common lead (e.g. Fig. 5a–b), open-system behaviour (e.g. Fig. 4d), or mixed analyses (e.g. Fig. 4c). Screening in this way allows us to analyse several samples or sample aliquots in a single LA-ICP-MS session and thus identify the material most likely to provide an accurate and precise age.
Either as an alternative to spot traverses or subsequent to spot traverses, we use LA-ICP-MS mapping to determine both the location and nature of U and Pb zonation in the carbonate material. Whereas spot traverses provide rapid screening of multiple samples or aliquots, mapping provides fairly rapid (5×5 mm in <2 h) screening across complexly zoned samples. Different approaches can be adopted, a suite of major and trace elements can be analysed alone, a suite of elements for age determination (i.e. Pb to U ± Hg) can be measured, or, depending on ICP-MS instrumentation, these can be combined, i.e. using a quadrupole ICP-MS (Drost et al., 2018) or a split-stream set-up utilising two ICP-MS instruments (e.g. Kylander-Clark et al., 2013). As will be shown by the examples in the subsequent sections, trace element maps are useful for directly comparing U and Pb zonation with other trace and major elements. We have found that in primary vein-filling calcite, U typically correlates with other trace elements; this varies between samples but can include V, Mn, Y, and the REEs. We can use this information to distinguish primary zones of calcite from those that have been altered (see Sect. 6). Elements, or elemental ratios such as Ba∕Ca, can be used to distinguish alteration zones or secondary material (e.g. a detrital component). For example, in meteoric carbonates, high Th is commonly attributed to detrital matter. The production of trace element maps rapidly produces extra information that can be related to any later age determination, facilitating the relating of the age to a specific growth event, i.e. the petrochronological approach (i.e. Kylander-Clark et al., 2013; Engi et al., 2017).
An alternative approach is to produce maps that generate U–Pb data directly (see Sect. 6.2). These have obvious utility in determining suitable domains of calcite; however, for common-lead-bearing minerals they can be difficult to interpret by visual inspection. Pb–Pb or Pb–U isotope maps can be created with ease; however, because of the inherent inclusion of common lead, a map of common-lead-corrected 206Pb∕238U ages or ratios is more useful. Common-lead-corrected age maps require (1) precise knowledge of the initial-lead composition (or upper intercept in Tera–Wasserburg space) and (2) knowledge that the initial Pb composition is homogeneous across the mapped region, something that is not always the case (see Sect. 7.2). However, with the recent advent of more advanced data processing software, such as the Monocle plug-in for iolite (Petrus et al., 2017), complex age determination from maps is becoming more achievable (see Sect. 6.2). The caveat with such data processing packages is that non-related domains defining a single age with a good precision can potentially be selected with subjectivity and without relation to actual geological or mineralogical process. For this reason, we suggest that it is imperative that users relate domains they have selected for U–Pb age determination to specific mineralogical domains that can be identified independently with other means, whether these be entire crystals, domains of crystals, growth bands, or specific veinlets. As suggested by Drost et al. (2018), who demonstrate the method for carbonate sediments, it is also useful to compare conventional spot ablation analyses with the map-generated dates to verify the accuracy of the latter.
The LA-ICP-MS method for carbonate follows a typical sample-standard bracketing approach using a matrix-matched reference material, i.e. as for other silicate or phosphate minerals (e.g. zircon, monazite, titanite, rutile, apatite, allanite), with only minor modifications. Similarly, uncertainty propagation and data reporting should follow the community-based guidelines for zircon of Horstwood et al. (2016). Details on the LA-ICP-MS method for carbonate adopted by three major laboratories taking a similar approach are provided in Roberts and Walker (2016) and Drake et al. (2017) for the British Geological Survey laboratory (Nottingham, UK); Ring and Gerdes (2016) and Methner et al. (2016) for Goethe Universität (Frankfurt, Germany); and Nuriel et al. (2017, 2019) for the University of California Santa Barbara (Santa Barbara, USA). Ablation spot sizes are typically larger than for silicate or phosphate minerals – generally >40 µm and often >100 µm – and fluences are also often high (>4 J cm−2). As with all U–(Th)–Pb LA-ICP-MS geochronology, we advocate the use of consistent ablation parameters between samples and reference materials.
There are two key points of the method we feel are worth highlighting that differ from “standard” methods based on silicate minerals such as zircon. Firstly, the heterogeneous nature of the Pb isotope composition of matrix-matched, i.e. calcite or dolomite, minerals (due to variable common-Pb incorporation) means that normalisation of the Pb–Pb isotope ratios is currently achieved using a synthetic glass rather than a carbonate, typically NIST612 or NIST614. At present, there is no evidence to suggest that the Pb–Pb mass bias is variable across different matrices. Secondly, calculation of the reproducibility of the primary and secondary matrix-matched reference materials, which is for uncertainty propagation (Horstwood et al., 2016) and determination of the true method accuracy and precision, is hindered by the fact that the carbonate reference materials currently employed have U∕Pb heterogeneity that is equal to or much larger than the analytical uncertainties (Roberts et al., 2017). This means there will typically be a significant excess variance of the reference material U∕Pb isotope measurements in any one session (including after correction for common lead), which does not describe the reproducibility of the analytical system but instead reflects the natural variation in the reference material. If propagated onto the sample data-point uncertainties as a within-session excess variance as recommended for zircon in Horstwood et al. (2016), these data point uncertainties will be overestimated, masking any smaller-scale real geological scatter in the sample isochron and resulting in ages with erroneously high precision. For this reason, it is suggested that calculation of the session-based reproducibility is best estimated using a more homogeneous material such as NIST glass or zircon. However, it should be noted that through this practice results can only be compared in a relative sense within session or between sessions if validation materials are compiled and used. To compare data in an absolute sense, i.e. to assign an age and total uncertainty to a material for comparison between laboratories and/or with other methods, the uncertainty from the primary reference material must be included to reflect the accuracy with which the matrix-matched normalisation is known. In this way, the uncertainty of the primary reference material constitutes a limiting uncertainty in any sample age. Improved reference materials with less scatter around the U∕Pb isochron are therefore a prerequisite for improving this method.
Generating ages and relating these to geological processes requires the marriage of spatially resolved variations in composition (elemental and isotopic) and U–Pb isotopic concentrations. In this section, we present several case studies to highlight how the integration of compositional image-based data with U–Pb data can be used to interpret and refine age data. First we present the standard approach, which used independent imagery and analysis to target, refine, and interpret the U–Pb analyses that are based on static spot ablations; this is the same concept as using CL imagery to help interpret zircon dates. A second approach (age mapping) is to use mapping tools not just to image the sample and its composition but to extract age data from the map itself (Petrus et al., 2017; Drost et al., 2018).
6.1 Image-guided dating
The aim of most dating studies is to constrain the timing of primary calcite formation rather than subsequent secondary alteration. Trace element mapping using LA-ICP-MS is a particularly useful tool to assist with the identification of growth zoning, particularly on the scale of millimetre- to centimetre-sized chips. Figure 7a and b show examples of vein-fill calcite where uranium zonation can be compared to other major and trace elements. The trace element mapping reveals large variation in trace element contents across the directions of growth, interpretable as changing metal∕Ca ratios in the mineralising fluids (e.g. Drake et al., 2014). The trace element zonation in both of these samples can be traced with the optically visible growth zonation, indicating its primary nature. Sample TJN-0-1 (Fig. 7a) was presented in Roberts and Walker (2016), and we have re-dated it here locating spots in three separate areas with different uranium concentration. The dates all overlap (Fig. 7a), but the precision of the dates is controlled by the amount of radiogenic to common lead, which broadly correlates with the U concentration of the sample and where the traverse was located. For this sample, the trace elements are low, including the Mn content, meaning the entire sample appears dark in cold-stage CL. Therefore, elemental mapping with LA-ICP-MS is one of the few techniques that can be used to characterise the elemental zonation in such samples.
Sample TJN-6-1 (Fig. 7b) is a single large crystal, with a rim of zeolite. Trace element mapping reveals a strong correlation between most elements, again, representing the primary growth zonation. High Mn and V “fingers” intersect the growth zonation and are visible optically. We interpret these as pathways of secondary alteration. Given that the vein exhibits vuggy textures, it is possible that fluids have precipitated or altered the original calcite much later than the original period of calcite precipitation. Trace element mapping allows us to visualise and fingerprint these alteration zones and avoid or remove them from analyses used for dating. A benefit to this approach is that the maps can then be used to estimate the trace metal contents of the mineralising fluids, which in turn provides information about rock–water interaction and the redox conditions, for example. These maps also demonstrate that no measurable diffusion of trace elements across the calcite crystals has occurred over a significant time span, as the distribution is interpreted as a primary feature.
Alteration zones can sometimes be observed visually, without the need for imaging techniques, as demonstrated by the vein sample in Fig. 7c. In this particular sample, the CL emission was rather dark, limiting its use for distinguishing the altered and non-altered parts of the vein. Trace element mapping, however, clearly distinguishes a region of alteration running across the vein that is characterised by enrichment and depletion on trace and major elements (e.g. low Mg, high La, Mn, and Pb). Screening data from this sample, comprising randomly located spot traverses across the vein, are presented in Fig. 7c. The data have a large array of common to radiogenic Pb compositions, with significant scatter including several data with low U∕Pb and Pb∕Pb ratios. The U–Pb data are compatible with open-system behaviour and/or mixed age domains. Placing spots away from the altered region, and within a region with high uranium, yields a more robust regression that we interpret as a primary date of calcite formation.
In the final example (Fig. 7d), the only mapped elements were U and Pb, but the sample was also imaged using CCI. Both the elemental maps and CCI image show laminations that are interpreted as growth zonation and a reflection of the primary distribution of trace elements (U and Pb in this case). Faintly visible on the CCI are thin veinlets that cross-cut the growth bands. On the elemental maps, these are clearly distinguished as regions of Pb enrichment and U depletion, suggesting that Pb-rich fluids have percolated through this fracture-fill calcite. Since the spots that lie on the alteration pathways have high Pb counts, the age data were culled based on Pb concentration (>300 ppb Pb removed). This approach reduced the scatter in the regression, providing a more precise age, presumably through the removal of data that reflect variable common-lead compositions.
6.2 Age mapping of vein-fill carbonates
An alternative approach to using elemental maps to “manually” locate spots or refine spot data is to generate a combined elemental and U–Pb isotopic 2D dataset (i.e. map); the benefit of this method is that software tools can be used to both discriminate between specific isotopic data based upon chosen criteria and also to show regions within these pooled datasets that have similar compositional characteristics. Iolite (Paton et al., 2011) is one of the most commonly used data reduction tools for both U–Pb isotopic data (Paton et al., 2010) and for the generation of elemental 2D maps. Monocle is a software plug-in for iolite that allows the user to generate maps of isotopic and elemental data (Petrus et al., 2017) and to define and extract regions of pooled compositional data, including those used for age calculations. Drost et al. (2018) demonstrated the efficacy of the software for dating carbonate sediments, whereby features such as bioclasts and detrital components are removed. For a detailed explanation of the protocol, see Drost et al. (2018). In brief, each pixel of the elemental and isotope ratio maps corresponds to one duty cycle of the ICP-MS. First, pixels are removed, using user-defined selection criteria that are believed to be related to alteration, secondary material, or a younger or older carbonate generation. This is usually conducted after an initial inspection of the mapping data combined with prior imaging and petrography; however, the screening can also employ an iterative approach after the generation of initial U–Pb isochrons. After this screening or filtering, the remaining data are pooled into a number of pseudo-analyses (each corresponding to the same number of pixels) based on a suitable isotope ratio, such as 238U∕208Pb or 235U∕207Pb. The pooling is achieved using an empirical cumulative distribution function (ECDF) to maximise the spread in U∕Pb ratios and an appropriate number of pixels to produce a reasonable population of data, for example 20 to 40 data points. Here, we present examples of this approach applied to vein-filling calcite.
Figure 8 shows an example of a vein cross-cutting a sedimentary host rock, with clear zonation within the vein. Since it is a syntaxial vein (crystals growing from the wall rock to the centre), this zonation probably represents changing fluid chemistry as the calcite crystals were precipitating. However, it could represent multiple generations of calcite precipitation. Criteria were selected for filtering of the data to highlight the outer regions of the vein; Rb <0.05 ppm, Th <0.01 ppm, and Sr <400 ppm. The U–Pb data were then filtered to remove data with low U and Pb signals, since no initial rejection of data based on detection limit was conducted using this data reduction method; criteria for acceptance were 238U >500 cps and 207Pb∕206Pb <1.5. The remaining data produce a robust isochron with a lower-intercept date of 61.0±1.7 Ma (MSWD =1.12; 21 pooled analyses). This date overlaps that previously obtained using spot analyses that were derived from the entire width of the vein (59.5±1.7 Ma; Beaudoin et al., 2018).
To demonstrate image-based dating on another complex sample, we re-dated the vein presented in Fig. 7c (NR1511). This vein features visible textures and chemistry associated with alteration. The mapped region (see Fig. 9) is entirely within the vein (no host rock). High concentrations in several elements (e.g. Cu, Rb, Sr, Ba, and Pb) reflect veinlets that can be seen optically as a yellow altered region. The remaining portion of the vein varies in U content, which likely represents chemical zonation across the coarse sparry calcite growth. A fairly robust isochron (MSWD =2.0) was obtained after filtering of the data for the clearly altered regions, cleaning up the U–Pb data to remove low U and Pb signals and pooling the data based on 207Pb∕235U. The criteria for acceptance were Cu <0.2 ppm, Ba <10 ppm, Rb <0.01 ppm, and 238U <10 000 cps (for removal of alteration) and 238U >500 cps, 207Pb∕206Pb , and 206Pb∕208Pb (for “cleaning up” the U–Pb data). These data yielded a date of 283.1±9.4 Ma, which overlaps that obtained from spot analyses and manual location of the spot data based on prior LA-ICP-MS mapping (286±12 Ma; see Fig. 7c).
7.1 Isotopic composition of common lead
Carbonates nearly always take up some amount of lead during their formation, referred to as common or initial lead. Contamination during handling (i.e. during cutting and polishing) or from recent exposure to the environment will have a modern isotopic composition of common lead, i.e. approximating the Stacey and Kramers (1975) model for terrestrial lead composition in the present day, roughly 207Pb∕206Pb =0.84. Distinguishing between such contamination and the common lead incorporated during formation can be difficult. Well-behaved U–Pb isotopic systematics in a carbonate sample should yield a single mixing line between the common and radiogenic endmembers and ideally will have enough spread in U∕Pb ratios to yield a precise regression with low uncertainties at both the lower (radiogenic lead) and upper (common lead) intercepts. However, many samples will exhibit a lack of spread in U∕Pb ratios or will be dominated by radiogenic compositions (e.g. Fig. 4f). Although a best-fit line may be calculated for such data, the slope, and thus age may be inaccurate. Thus, it is useful for such samples to have an estimation of the common-lead composition through other means, such as from nearby cogenetic samples formed at the same age or from different minerals also believed to have been formed at the same age.
For some mineral chronometers, such as the phosphate mineral monazite, it is common to use an estimate of the common-lead composition based on the Stacey and Kramers (1975) model (e.g. Palin et al., 2013; Regis et al., 2016). In our experience, this is an acceptable approach because from a number of different studies, we find that the common-lead composition determined from other minerals (i.e. feldspar, biotite, apatite) overlaps the Stacey and Kramers (1975) composition (e.g. Stübner et al., 2014; Warren et al., 2014). For carbonate, however, we find this is not always such a suitable approach. Our experience, particularly from fracture fill but also evident in diagenetic and sedimentary carbonates, is that common-lead compositions are often more radiogenic (lower 207Pb∕206Pb ratios) than those predicted by the terrestrial lead model (Stacey and Kramers, 1975) for the age of carbonate crystallisation. This situation can occur if the carbonate has incorporated unsupported radiogenic lead during its formation. This most readily occurs by the incorporation of radiogenic lead that is derived from an ancient source, i.e. lead produced by uranium decay in a closed system for a long time, but which is decoupled from its parent uranium before being incorporated into the measured carbonate.
We have compiled sample data with robust U–Pb regressions from the BGS laboratory (both published and unpublished) and presented these as a compilation of common-lead intercepts (207Pb∕206Pb). The data are split into fracture-fill and diagenetic samples and represent different host lithologies, different ages (dominated by Cretaceous to Miocene), and different geological regions. It is clear that for many samples in this compilation, anchoring at a value close to the terrestrial lead model composition for Phanerozoic ages, i.e. 207Pb∕206Pb ∼0.84, will lead to calculated ages older than the true age due to steepening of the regression. The importance of the common-lead composition in providing constraints on a calculated age will depend on the amount of measured radiogenic lead in a given sample; samples dominated by common lead and lacking in radiogenic lead will need a well-defined array to produce a confident lower intercept. We find that within individual vein samples, the apparent composition of the common-lead endmember can vary, limiting the precision of the regression and derived age. For speleothems, Woodhead et al. (2012) demonstrate that most samples analysed in their lab yield common-lead compositions overlapping Stacey and Kramers (1975), and thus their ages are largely insensitive to the common-lead compositions. This likely reflects the fact that they are precipitated from meteoric water that incorporates modern lead derived from a regional upper-crustal lead composition.
The highly radiogenic initial-lead values (207Pb∕206Pb ) recorded in our compilation are mostly from two settings: young fractures in Proterozoic crystalline crust of Sweden (n=10) and young fractures in the Bighorn Basin that overlies Archaean basement (n=24). In both cases, lead leached from the bulk rock, although ancient, is not radiogenic enough to produce the measured values. Instead, leaching of unsupported radiogenic lead from uriniferous minerals (i.e. high μ) is required (e.g. titanite, allanite, monazite, xenotime, and zircon) as a causative mechanism. Radiogenic lead is in fact a well-known, widespread feature found in ore deposits across Sweden (e.g. Johansson and Rickard, 1984; Romer and Wright, 1993).
An additional complexity in interpreting carbonate U–Pb data is that fine-scale variability in initial-lead compositions may exist. This is because the fluids involved in carbonate precipitation may vary on very short timescales, with varying fluid–rock interaction leading to different Pb components being leached into the fluids. The timescale of varying fluid involvement may be much shorter than the resolution of the U–Pb data, such that data with variable initial-lead compositions may not be resolvably different in age and, hence, will merely lead to increased scatter on the U–Pb isochron. Heterogeneous initial-lead compositions can be seen in an example of sandstone-hosted vein material from the Moab Fault, southeast Utah (Fig. 11). U–Pb data were obtained from different sections of the vein material formed along different orientations. The data exhibit a high level of common or initial lead, with limited spread in radiogenic-lead contents, but still forming a scattered regression to a lower-intercept value. Using different colours to discriminate between different sections of vein, it is clear that they have subtly different initial-lead compositions, as indicated by the upper intercept (207Pb∕206Pb value) of the data arrays. These lead compositions are more radiogenic than that predicted by the Stacey and Kramers (1975) terrestrial composition. The existence of variable Pb compositions on small length scales (<1 mm) means that careful attention is required to interpret complex data. However, the spatial resolution of LA-ICP-MS means that these details can potentially be teased out.
In summary, vein-filling, diagenetic, and hydrothermal carbonates often do not exhibit Stacey and Kramers (1975) model Pb compositions for their assumed age but typically yield more radiogenic compositions. This means that regressions anchored with assumed common-lead compositions are susceptible to inaccuracy. Mixed common-lead compositions in samples hamper the derivation of single age regressions, implying multiple fluid sources. Mixed ages and atypical lead compositions can also make age mapping problematic.
7.2 Dating young material – dealing with disequilibria
As described in Sect. 3, the younger the age of the sample analysed, the lower the potential for precise and accurate age determination due to the lack of radiogenic ingrowth of lead. However, young carbonates are a high priority in many applications because they can date events more relevant to the earth system at present and because U–Pb can extend the age range of sample suites or study areas where U–Th age dating is also feasible. For example, records of environmental change in deep time require the dating of speleothems that are older than 500 ka (see Woodhead et al., 2012, 2019), and the dating of veins that record seismic cycles extending beyond 500 ka (see Uysal et al., 2011; Williams et al., 2017) can provide constraints on earthquakes and other hazards associated with subsurface fractures. These particular applications are likely to require high levels of precision, i.e. for the Quaternary, of much less than ±100 kyr, and potentially even less than ±10 kyr or <1000 years for the Holocene. Achieving such precision requires very high U to achieve abundant radiogenic lead and higher μ values (see Fig. 3).
A major issue for accurate dating of young samples (i.e. <10 Ma) is the potential effect of initial daughter isotope disequilibrium within the uranium decay chains. The simplest form of the U–Pb and Pb–Pb age equations, often used for older samples, assumes that all long-lived daughter isotopes in the U decay chain are initially present in secular equilibrium. Both the U decay series contain long-lived daughter isotopes, including 234U ( ka), 230Th ( ka), and 226Ra ( ka) in the 238U decay chain, and 231Pa ( ka) in the 235U decay chain. Of these, 234U has the longest half-life and therefore the largest potential effect on U–Pb dates. The excess initial 234U often observed in natural waters will lead to the generation of unsupported 206Pb. If uncorrected, excess initial 234U produces overestimated 206Pb∕238U and lower-intercept dates. An excess of the other intermediate daughter products, like 230Th, relative to secular equilibrium will bias the age with a smaller magnitude but in the same direction, whereas a deficit will result in dates that are too young.
Carbonates are commonly precipitated from fluids containing 234U∕238U out of secular equilibrium. Thus, this initial disequilibrium must be considered in any age determination. Age corrections for initial U daughter deficits are at maximum ∼1.44 times the half-life of the daughter isotope for zero initial abundance. But for initial excesses, the age difference can be many times larger. For most older samples dated by U–Pb, the effect of disequilibrium is deemed to be insignificant compared to larger measurement uncertainties. For this reason, initial disequilibrium has thus far not been mentioned in any publication concerning LA-ICP-MS U–Pb dating except for those dealing with young speleothems (e.g. Hopley et al., 2019). However, here we demonstrate that initial disequilibrium may be a very significant cause of uncertainty for carbonates precipitated from groundwater and other crustal fluids and not just for very young (<1 Ma) samples.
In young samples, particularly those within the range of U–Th geochronology (<600 ka), the initial 234U∕238U ratio (234U∕238U0) can be estimated based on the combination of the present-day measured 234U∕238U (234U∕238Unow), and either the measured 230Th∕238U or the estimated date of formation. The robustness of this estimate is highly dependent on the precision and accuracy at which the isotope ratio(s) can be measured (the atom ratio is very small, making high-precision measurement >1 ‰ difficult). In addition, if the offset between 234U∕238Unow and secular equilibrium is small, then the measurement may overlap secular equilibrium within uncertainty. For this reason, the highest precision possible is a necessary target for any disequilibrium correction measurement.
For older samples (i.e. those older than about 4 times the half-life of 234U) and/or those with only a small degree of initial disequilibrium, 234U∕238Unow is likely to have reached secular equilibrium. This means that 234U∕238U0 cannot be estimated from the measured data alone. One approach to alleviate this problem is to take known initial ratios from younger samples (<600 ka) formed in approximately the same geologic setting and apply these corrections to the older samples from the same setting (e.g. Woodhead et al., 2006, 2019). This approach is only applicable if the geological environment is well known and the hydrological system believed to be relatively stable.
There are various causes of 234U excess in fluid–mineral systems, which have been studied at length (e.g. Osmond and Cowart, 1992, 2000; Porcelli and Swarzenski, 2003; Suksi et al., 2006). In summary, 234U is generated from α decay of 238U and may preferentially be increased in the fluid state during mineral–fluid interaction due to oxidation state and valence differences between the U species (e.g. Suksi et al., 2006). Uranium activity ratios record information on the redox state of fluids, the source of uranium in the fluids, and potentially the timing of uranium residence in the fluid; therefore, they have long been a focus of groundwater studies (e.g. Osmond et al., 1968; Osmond and Cowart, 2000; Porcelli and Swarzenski, 2003). Of general interest here is whether carbonates precipitated from different geological settings are likely to have significant 234U excess such that any measured 238U∕206Pb dates will be inaccurate.
Cave drip water that generates speleothem deposits typically has excess 234U relative to secular equilibrium, although sometimes 234U is depleted. Overall, most cave systems have initial activity ratios that are not grossly offset from secular equilibrium. This means that an uncertainty limit can be placed on such carbonates with reasonable confidence. Disequilbrium corrections will significantly affect age estimates with high precision but not the low-precision estimates that typically characterise LA-ICP-MS dates. For example, Woodhead et al. (2019) used an estimate of 1.0±0.3 for 234U∕238U0 in their study of speleothems from the Nullarbor plain, Australia, and this had negligible impact on the resultant compilation of U–Pb dates. Hopley et al. (2019) estimated a range of 234U∕238U0 =1.26 to 2.99 for the “cradle of humankind” in South Africa, with a mean of 1.9 and discussed a resulting potential age range of 5.8 to 4.8 Ma. A known excursion from “typical” activity ratios is the Transvaal Dolomite Aquifer, also in South Africa. Speleothem deposits in cave systems that interacted with water from this aquifer have anomalously high U activity ratios ranging from ca. 2 to 12 (Kronfeld et al., 1994). This well-known occurrence highlights that speleothem deposits could arise from fluids with variable and anomalous activity ratios and thus that attention must be given to accurately estimating the 234U∕238U0 when dating such deposits.
Unfortunately, activity ratio data that are relevant to hydrothermal and other vein-filling carbonates are sparse and potentially more variable. Carbonates precipitated in the shallow crust may arise from percolating groundwater, seawater, deep brines, formation waters, or a mixture of these sources. We can use existing data on these fluid sources to make an initial estimate of what range may exist in terrestrial carbonates. Groundwater is well known to have highly variable and significant 234U excess (e.g. Osmond and Cowart, 1976). Figure 12 shows a compilation of 234U∕238U activity ratios taken from a range of literature sources (see Supplement for sources). The population of data for groundwater (Fig. 12a), mostly shallow but including some saline and deeper samples, has a median activity ratio of 2.25 and is skewed towards higher values, with a significant tail up to ∼11. Data from hydrothermal fluids and deep brines are less abundant in the literature but can be estimated from young carbonates precipitated in travertines and hydrothermal veins. The compilation shown in Fig. 12b is dominated by samples from Turkey and the surrounding regions. It has a median of 1.41 and is right-skewed with a tail ranging up to ∼8 and only a few higher values.
The compilations in Fig. 12 are somewhat alarming, as they suggest that vein-filling carbonates have a high likelihood of having activity ratios out of secular equilibrium (where 234U∕238U ). The compilations shown are biased by sampling, so uncertainties in the range of activity ratios should not be based on these compilations. However, a very conservative view would be that shallow-groundwater 234U∕238U activity ratios average closer to ∼2 than they do to ∼1; hydrothermal waters average closer to ∼1.5; and permissible values may be extremely out of secular equilibrium at >10. The data reveal that precise age estimates of young carbonates derived from crustal fluids are going to be severely hampered by a lack of knowledge of the U activity ratios.
To demonstrate the effect of initial activity ratios out of secular equilibrium, we have modelled synthetic data in Fig. 13. This figure shows curves representing samples of 10 different ages, which would range from 500 ka to 9 Ma if 234U∕238U0 was in secular equilibrium (∼1) during formation. The true age of the samples get younger as 234U∕238U0 increases. The effect does not decrease in significance as we look at older ages, i.e. the age offset on a sample with a measured age of 8 Ma is similar to that on a sample of 4 Ma. The curves are shown on a log scale because in many systems, the variation in activity ratio is going to vary a small amount, close to secular equilibrium (∼1). For example, in the Nullarbor plain cave systems, the variation is likely to be within 30 % of 1 (Woodhead et al., 2019). Systems with large variations in initial activity ratios, for example some hydrothermal systems, would lead to a large uncertainty in the obtained dates. Ignoring the effect of the likely 234U excess in vein-filling carbonates is likely to lead to significant inaccuracy of dates by tens of percent, in general by overestimating the age. Considering the impact that unconstrained initial 234U∕238U ratios have on young dates leads to significant (>10 %) uncertainties.
So far, the discussion has involved the uncertainties surrounding excess or deficient 234U during calcite growth. However, there are several other intermediate daughter products in the uranium decay chains that can pose problems for the accuracy of measured ages; see Richards et al. (1998) and Woodhead et al. (2006) for previous discussion of these. The isotope 230Th is a potential consideration in the accuracy of 238U–206Pb ages. In general, most speleothem-dating studies assume no initial 230Th in the system, as Th is very insoluble in water compared to U. Any excess initial 230Th during formation would also result in artificially old measured ages. 231Pa is another daughter product in the decay chain, which, again, is considered very insoluble and does not form part of the disequilibrium corrections at present. 226Ra, another intermediate product, may co-precipitate with U, but its short half-life of 1.6 kyr means it is likely to have little impact on U–Pb ages (Richards et al., 1998). A final concern is the gas 222Rn, as this may be lost from the system by diffusive processes. A study into the effect of this showed negligible impact on the 238U–206Pb ages of a Quaternary speleothem (Richards et al., 1998).
Although the effects of disequilibrium in these shorter-lived intermediate daughter products are considered to be minor and likely within the uncertainty of measured LA-ICP-MS U–Pb dates, it is worth noting that hydrological systems outside of those concerning speleothems and meteoric water have not been explored. Most of the issues presented here, particularly the excess 234U problem, are part of the 238U decay chain and thus have implications for 238U∕206Pb and lower-intercept ages. The 235U decay chain has different intermediate daughter products, and thus measured 235U∕207Pb and lower-intercept ages will be affected by a different set of processes. The problem of excess 234U is alleviated if 235U–207Pb ages can be used instead of 238U–206Pb ages. However, there have been few attempts to utilise 235U–207Pb dates (e.g. Hopley et al., 2019) because the low abundances of these isotopes in comparison to 238U and 206Pb are major limitations on the uncertainty of the measurements. Engel et al. (2019) have provided a solution that will potentially increase the accuracy of age estimates for speleothems, utilising the 235U decay chain as well as using 208Pb in place of 204Pb as the initial-lead composition. This approach is based on ID, and it is unclear how effective it will be for LA-ICP-MS dating, given that 204Pb is difficult to measure at high precision.
In summary, initial disequilibrium is clearly a major issue for the accuracy of U–Pb dating of carbonates. The effect is significant for material of any age, but as we get to older carbonates, the analytical uncertainty contributions will begin to swamp the uncertainties surrounding disequilibrium. For the dating of Neogene–Quaternary carbonates, prior knowledge of likely activity ratios (e.g. by measuring younger or present-day values of the precipitating fluid and inferring no change back in time) is critical for precise and accurate dates. The variation in hydrothermal systems that mix meteoric water with older brines is likely to be large in terms of the degree of 234U excess. More information is needed to further understand what sort of values can be expected in different systems and different settings. From our preliminary compilation, it is apparent that 234U excess is the norm rather than the exception. For now, the absolute values and uncertainties in young dates (late Neogene to Quaternary) with no estimation of the initial disequilibria should be treated with caution.
7.3 Dating old material – dealing with a potentially open system
Many early carbonate dating studies were attempted on very old material, i.e. Proterozoic and Archaean (e.g. Moorbath et al., 1987; Jahn, 1998; Taylor and Kalsbeek, 1990; Whitehouse and Russell, 1997); these mostly utilised Pb–Pb dating. A major issue of the Pb–Pb method is that Pb contents of crustal fluids are much higher than that of the primary carbonates, and, therefore, even small amounts of fluid-related alteration can dominate the measured Pb–Pb composition and lead to an age that is not representative of primary carbonate precipitation (e.g. Sumner and Bowring, 1996). Although there have been a handful of studies dating old carbonate material since the 1990s (e.g. Ray et al., 2003; Sarangi et al., 2004; Babinski et al., 2007; Fairey et al., 2013), Pb–Pb and U–Pb dating of Precambrian material has become a rarely used technique. This is presumably due to the difficulty in obtaining meaningful primary ages of old material. The dominant reason for this difficulty can generally be distilled down to open-system behaviour; i.e. dating material that has remained a closed isotopic system since its formation is increasingly difficult with increasingly older material. This is simply because thermal- and/or fluid-induced mobility of parent and daughter isotopes becomes increasingly likely if the material has been exposed to multiple deformation-, burial-, uplift-, glaciation-, weathering- or fracture-related events. Early studies documented various transformative processes and their impact on Pb–Pb∕U–Pb isotope systematics, e.g. fluid infiltration in limestone (Smith et al., 1991), diagenetic change from aragonite to calcite (Jones et al., 1995), and resetting of Pb isotope signatures during metamorphism (Russell et al., 1996; Whitehouse and Russell, 1997; Babinski et al., 1999). In general, the existence of some form of open-system behaviour within a given dataset has only been recognised through the isotopic data themselves, not through an independent dataset. This is simply achieved by assessing the robustness of the Pb–Pb or U–Pb data array with mathematical means, e.g. using the MSWD value, and explaining analytical scatter outside of a robust array as due to open-system behaviour. With in situ methods, the approaches that we have described in Sect. 5 may allow for some independent removal of data that pertains to open-system behaviour, leaving a dataset that corresponds to a closed system.
A method that has been utilised to screen for altered samples in whole-rock geochemistry is to test for effects of modern weathering using 234U∕238U ratios (Albut et al., 2019). Ancient samples should have measured 234U∕238U activity ratios in secular equilibrium, and departure from this in a measured sample would imply a more recent addition or subtraction of 234U through weathering processes, indicating some modern fluid–rock interaction. This method of sample screening has not been applied to U–Pb dating, but we suggest is worthy of investigation.
In Fig. 4 we documented various U–Pb datasets to demonstrate the range of behaviour that is seen with natural carbonates. Here we provide some additional comments regarding open-system behaviour, first in terms of U mobility, followed by that of Pb mobility. Uranium is mobile in oxidising fluids, so U enrichment and depletion relative to Pb are assumed to be the most common cause of open-system behaviour that will occur in natural carbonates. In Tera–Wasserburg space (238U∕206Pb vs. 207Pb∕206Pb), U mobility will be apparent as sub-horizontal trends in the data, with movement to the right reflecting gain of 238U and movement to the left reflecting loss of 238U (see Fig. 14). During a period of mobility, uranium may move into a fluid phase, such that the remaining carbonate solid remains variably depleted in 238U, or uranium may partially move from its original location to another within the measured sample volume. In the former, this can sometimes be detected from the isotopic data if a distinct departure from a robust regression is defined by a sub-horizontal array (see Fig. 4d). In the latter case of uranium mobility, some domains will be depleted, whereas others will be enriched. This may be difficult to ascertain from the isotopic data alone if the mobility is pervasive through the material because the induced scatter in the U–Pb regression (from both positive and negative movement in 238U∕206Pb) cannot be resolved from other causes of scatter, such as mixing between different age domains.
Lead can be substituted for Ca in the calcite lattice and is also insoluble in most upper-crustal fluids; for these reasons, U mobility is generally considered in favour of Pb mobility. Fluid-assisted mobility of U is certainly the most likely cause of open-system behaviour because of the solubility of some U species. However, at high temperatures, solid-state diffusion is also a factor for consideration. Based on experimental data, Pb diffusion in calcite is essentially slow enough to be non-existent below 300 ∘C (when considering the composition of a grain 1 mm in diameter; Cherniak, 1997); however, at higher temperatures (>400 ∘C), diffusion of lead is possible if encountered for long periods (>20 Myr). Empirical observations of Pb (or U) diffusion in calcite are lacking. Diffusion is unlikely in the low-temperature calcites that have formed the basis of most modern LA-ICP-MS dating studies; however, carbonates form in a range of higher-temperature environments as well, such as alteration veins within deeply subducted crust. Understanding how the calcite U–Pb system works at medium- to high-metamorphic grades may therefore become very relevant information, allowing this chronometer to be used to understand dates and rates in deep-crustal environments.
7.4 Analytical limitations
At present, there is only one reference material in circulation that has been widely used and documented for the purpose of U–Pb normalisation (WC-1; Roberts et al., 2017). WC-1 has an uncertainty in its U∕Pb ratio of 2.5 % 2σ. Using this material for normalisation of U∕Pb ratios or for validation of the method accuracy limits the final age uncertainty of any particular sample to ∼2.5 %. To improve beyond this range requires the characterisation of natural (or production and characterisation of U and Pb doped synthetic) materials, with a final U∕Pb precision better than 2.5 %. There is also a requirement for additional well-characterised materials (i.e. those with robust U–Pb systematics and well documented ID U–Pb datasets) that can be used as secondary reference materials (i.e. those run as unknowns), for the assessment of accuracy and long-term reproducibility.
Another major limitation is the nature of carbonate matrices and the lack of quantified data on the matrix effect between different carbonate minerals and structures. Inter-element fractionation (i.e. U∕Pb in this case) is one of the major limitations on the reproducibility and accuracy of laser ablation U–Pb dating. For this reason, matching matrices of the reference material with that of the sample has been standard practise in U-bearing accessory mineral geochronology. Several groups have tried to limit the effect of this issue by utilising normalisation and data reduction procedures that reduce the effect (e.g. Burn et al., 2017; Neymark et al., 2018), but regardless of the matrix used for normalisation, validation of the method should still utilise a similar matrix to the sample. Carbonates clearly have a large range of structures, even with calcite, for example, sparry to micritic, with wide-ranging crystal or grain sizes and porosity. Nuriel et al. (2019) noted differences between the use of coarse-grained sparry reference materials and to fine-grained polycrystalline reference materials, with the latter being skewed towards older ages by several percent. To move towards better precision and accuracy of the LA-ICP-MS U–Pb method, it will be necessary to have a range of well-characterised reference materials that cover variable carbonate mineralogy (e.g. aragonite, dolomite, calcite), as well as internal morphology and texture.
To date, LA-ICP-MS U–Pb carbonate geochronology has been utilised for a wide range of applications. These include the dating of speleothem deposition (Hopley et al., 2019; Scardia et al., 2019; Nicholson et al., 2020), brittle deformation (Roberts and Walker, 2016; Ring and Gerdes, 2016; Goodfellow et al., 2017; Hansman et al., 2018; Parrish et al., 2018; Beaudoin et al., 2018; Nuriel et al., 2017, 2019; Smeraglia et al., 2019), hydrocarbon migration (Holdsworth et al., 2019, 2020), hydrothermal ore mineralisation (Burisch et al., 2017, 2019; Kreissl et al., 2018), hydrothermal and deep-crustal fluid flow (Drake et al., 2017, 2019, 2020; Mazurek et al., 2018; Walter et al., 2018; Incerpi et al., 2020; MacDonald et al., 2019), pedogenesis (Methner et al., 2016; Liivamägi et al., 2019), ocean crust alteration (Coogan et al., 2016), diagenesis in sedimentary deposits (Li et al., 2014; Pagel et al., 2018; Mangenot et al., 2018; Godeau et al., 2018; Lawson et al., 2018), and sedimentary deposition (Drost et al., 2018). Published dates range in age from 0.6 to 548 Ma (see Fig. 15), MSWDs range from 0.2 to 89 (Fig. 15a), and quoted uncertainties range from 0.6 % to 143 % (2 s; Fig. 15b). The majority of dated samples so far range from the Neogene to Jurassic, with ∼50 % being Oligocene or younger. Across this age range, the uncertainty is variable and uncorrelated to age or MSWD, demonstrating that the age uncertainty reflects an interplay of factors and includes the heterogeneous nature of carbonate materials. It should be noted, however, that many dates with large uncertainties or mixed results are likely unpublished, biasing this compilation towards successful samples. For example, it is possible that many unreported and failed attempts at dating samples that are Palaeozoic and older have been made. We also note that many samples have reported age uncertainties better than the WC-1 reference material, indicating that the systematic uncertainties have not been fully incorporated for these dates.
A major benefit of carbonate geochronology is that carbonate minerals provide an archive of data that can be linked to the age of formation. Fluid inclusions, stable isotopes (carbon and oxygen), radiogenic isotopes (strontium), and elemental compositions all reveal insight into the fluid composition that precipitated the mineral. This combination has long been an approach within the field of palaeohydrology; however, the timing of mineralisation and hence fluid flow has generally involved only relative estimates with large uncertainties or the dating of phases associated with higher-temperature activity (e.g. Re–Os dating of molybdenite). The addition of absolute chronological information is a critical step to understand the timing of fluid flow through the crust in a range of settings, for example, within hydrocarbon-bearing basins, within ore-forming mineral systems, and within upper-crustal bedrock that may be used to host anthropogenic waste or outputs (e.g. radioactive waste, storage, and sequestration of CO2).
A benefit of utilising LA-ICP-MS as a method of dating is that the same crystals that have been dated can be measured for various other chemical proxies and signatures. Several previous studies have combined fluid inclusions and/or stable carbon and oxygen isotope analysis with LA-ICP-MS dating (e.g. Mangenot et al., 2018; Pagel et al., 2018; Goodfellow et al., 2016; Walter et al., 2018), but for most of these, it is not clear if the same volume of material or simply the same genetic domain has been sub-sampled for both the dating as well the additional isotope analyses. The use of petrography and imaging allows for the same genetic domain to be analysed for several methods; however, there are also several approaches that allow for an overlapping analytical volume to be analysed. Dated material can be micro-drilled or micro-milled following laser ablation, with the powder being analysed for additional chemical information (e.g. Sr, C, O isotopes). Alternatively, thin sections or polished blocks can be analysed using a combination of in situ techniques, for example, ion microprobe measurement of stable isotope and/or elemental compositions and laser ablation measurement of Sr isotopes, elemental compositions, and U–Pb dating. Drake et al. (2017, 2019, 2020) demonstrate the utility of combining ion microprobe stable carbon and oxygen isotope analysis with U–Pb dating to study palaeohydrology and ancient microbial activity.
In addition to traditional carbon and oxygen isotope measurements (δ13C and δ18O), clumped isotopes (Δ47) can provide the temperature of mineral formation (e.g. Eiler, 2007). Several studies have demonstrated the combination of clumped isotope thermometry with dating (e.g. Quade et al., 2017; Mangenot et al., 2018; Lawson et al., 2017; MacDonald et al., 2019). These apply the technique to the dating of palaeosol for climatic records, diagenetic mineralisation for basin histories, and hydrothermal veins to understand crustal fluid flow. This combination of techniques is a clear growth area with a range of applications across earth and environmental science.
Finally, carbonates also comprise a host of major and trace metals that offer further isotopic information that has yet to be fully explored, for example, stable isotopes of Ca, Zn, Fe, and Cu. Linking these with U–Pb dates from the same material could provide high-resolution records of natural fractionation processes in subsurface environments.
LA-ICP-MS U–Pb carbonate geochronology has been demonstrated by this and previous studies to offer a potentially robust technique to date the timing of carbonate mineral formation. Limitations on the technique arise from several challenges. These include the typically low U content of carbonates in many settings, the propensity for carbonate to include significant concentrations of Pb upon formation, and the ease with which fluids can alter or reprecipitate mineral growth. LA-ICP-MS being an in situ technique, with high spatial resolution compared to physical sampling for bulk dissolution studies, enables many of the hurdles in carbonate geochronology to be overcome.
Accurate and informative U–Pb carbonate geochronology demands careful imaging and petrographic analysis to establish a link between date and process. Various imaging techniques can be utilised prior to or after dating to aid with mineral characterisation and with the refinement and interpretation of the resulting age data. We refer to this as image-guided analysis. An alternative technique involves directly determining age data from image-based data itself, which we refer to as image-based analysis. Both techniques have their different benefits and applicability, and their efficacy depends on the instrumentation used and the type of material; for example, quadrupole ICP-MS is suited to image-based analysis, as a large element suite can be measured. Limitations on using quadrupole instrumentation are the detection limits for U and Pb when counting a large suite of elements. In contrast, multi-collector instruments can be used for image-based analysis and have a very low detection limit, but the mass range is restricted between Hg and U, meaning that additional elements useful for understanding the U and Pb distribution cannot be measured simultaneously. Overall, image-based analysis is only nascent in geochronology and as such has not been fully explored. Limitations on the accuracy of ages and their interpretation comes from several sources. Variability in initial-lead composition needs to be acknowledged when interpreting complex U–Pb data, and carbonates commonly have initial compositions that are different to that predicted by model estimates, e.g. Stacey and Kramers (1975). Disequilibrium in the U–Pb decay chains is typically only explored in very young samples (<1 Ma) but can have a potentially significant effect on the accuracy of ages throughout the Quaternary to Neogene. The variability in U isotope ratios in natural waters is a cause for concern in dating young material and indicates that more work to understand the natural variability that can be expected in carbonate precipitates is required.
The applications of carbonate U–Pb geochronology are vast, with a key benefit to the laser ablation approach being that specific volumes of material can be analysed for several isotopic and elemental proxies and signatures, whilst also providing absolute chronological information. The LA-ICP-MS method is limited by factors that include the uncertainties in reference material isotope ratios, matrix effects, and long-term reproducibility; taking these into consideration, the method is best applied to applications where age uncertainties of greater than 3 %–4 % are of benefit. For applications where high precision (i.e. <1 %) is required, such as calibration of palaeoclimate records or of evolutionary change and then follow-up analysis with ID is the only method that can potentially achieve the necessary precision. The future of the method in terms of accuracy and precision requires well-characterised (by isotope dilution methods) reference materials covering a range of carbonate matrices. The range of studies published over the last 5 years (2014 to 2019) has revealed a wide array of geoscience applications that are both amenable to, and benefit from, LA-ICP-MS U–Pb carbonate geochronology.
The focus of this paper is not on the meaning of the age data presented or its implications for faulting or fluid flow; however, we provide brief information for interested readers.
A1 Figure 7a and b – Faroe Island brittle faults
The significance of the Eocene ages has been discussed by Roberts and Walker (2016). This paper was the first to demonstrate the applicability of LA-ICP-MS U–Pb carbonate geochronology to dating brittle structures in the upper crust.
A2 Figures 7c and 9 – Variscan-related vein in the Northumberland Basin
The age of ca. 287 Ma for the dated calcite crystal can be linked to deformation of the host rock based on the vein structure. The calcite is taken from a planar fracture forming on the axial plane of a small fold that has accommodated bedding-plane sliding (Fig. 8). The fracture is filled with calcite mineralisation of the stretched vein type (Bons et al., 2012), and that is interpreted to have formed soon after the opening of the vein and synchronous with deformation. The age of ca. 287 Ma broadly overlaps with the intrusion of the Whin Sill (ca. 297 Ma; Larry Heaman, personal communication within De Paola et al., 2005) and is therefore compatible with the model of partitioned transpression of De Paola et al. (2005), who suggest that deformation was synchronous with the Whin Sill intrusion.
A3 Figure 7d – Sellafield fracture mineralisation
Sample 877 was collected from the modern-day saline transition zone between the upper fresh groundwater system and the deeper saline basinal-basement groundwater system, at a depth of −635 m within the St Bees Sandstone Group (Triassic) in Sellafield borehole BH10A (equivalent to samples B697 and D750: Appendix Table S2 of Milodowski et al., 2018). Externally, this calcite exhibits a “nailhead” (i.e. c-axis-flattened) crystal habit (Fig. 10). However, detailed petrographic analysis reveals it has a complex growth history: comprising cores of c-axis-elongated calcite characteristic of the deeper saline groundwater that are syntaxially overgrown by later equant and c-axis-flattened calcite characteristic of the overlying fresh groundwater zone (Milodowski et al., 2018). The U–Pb analyses all come from within the saline groundwater-zone-type calcite core region (rather than the later freshwater-type overgrowth that has extremely low U). Late-stage (generation “ME9”) calcite is a characteristic feature of the present-day fracture-controlled deep groundwater system in the Sellafield area of the west Cumbrian coastal plain (Milodowski et al., 2018). The resulting age suggests that ME9 calcite growth in the sampled fracture was initiated in the late Miocene and has been preserved (or at least partially preserved until the present day). The implication is that the modern groundwater system was developed following regional Miocene uplift, and younger groundwater recharge relating to glaciations and/or uplift of the region have not led to complete re-precipitation of fracture-filling calcite, with calcite precipitation continuing to the present day. Taken together with other petrographic, stable isotope, strontium isotope, fluid inclusion, microchemical analyses, and whole-crystal U–Th age dating, the age data support the interpretation that despite evidence for glacial recharge, the geochemical conditions (e.g. pH, Eh) have remained stable over this period at potential repository depths (cf. Milodowski et al., 2018).
A4 Figure 8 – vein set of the Bighorn Basin, Wyoming
This sample is from a vein set in the sedimentary cover of the Bighorn Basin and is part of a larger study that analysed the timing of deformation in the foreland of the Sevier and Laramide orogenies and how this deformation propagated in time and space (Beaudoin et al., 2018).
A5 Figure 11 – Moab Fault
This sample comprises multiple thin (1 to 5 mm wide) veins collected from the footwall damage zone of the Moab Fault in southeast Utah. Regional deformation is primarily driven by salt tectonics (Gutiérrez, 2004), and salt dissolution has produced up to 1 km of offset within the sedimentary rocks along the Moab Fault (Foxford et al., 1996). Fault zone deformation was closely associated with fluid flow and carbonate cementation (Eichhubl et al., 2009; Hodson et al., 2016). Ar–Ar ages from clay fault gauge range from 63 to 43 Ma and are interpreted to record the final episodes of faulting and fracture generation (Pevear et al., 1997; Solum et al., 2005). Our new lower-intercept age of 22 Ma is imprecise but clearly younger than the early Tertiary ages. This suggests that circulating fluids continued to move along the fault zone long after the cessation of fault-related deformation.
U–Pb data presented in Sect. 6 are provided in the Supplement Table (Carbonate Strategies Supplement S1), along with the corresponding methods and analytical details in the Supplement text (Carbonate Strategies Supplement S2).
The supplement related to this article is available online at: https://doi.org/10.5194/gchron-2-33-2020-supplement.
NMWR, KD, DC, and AS collected the analytical data. MSAH and DJC provided oversight to data collection and interpretation. AEM, HD, and JL assisted with sample petrography. RJW, RH, and JI assisted with sample collection. KD, NB, JKL, and RJW contributed samples. NMM assisted with data analysis. NMWR collated literature data. All authors contributed to writing the paper.
The authors declare that they have no conflict of interest.
This article is part of the special issue “In situ carbonate U–Pb geochronology”. It is a result of the Goldschmidt conference, Barcelona, Spain, 18–23 August 2019.
David Chew and Kerstin Drost acknowledge a Science Foundation Ireland grant (15/IA/3024) that is partly funded by the Geological Survey of Ireland and the Environmental Protection Agency, Ireland. Henrik Drake acknowledges a Swedish Research Council grant (2017-05186) and a Formas grant (2017-00766). Nick M. W. Roberts thanks Jeremy Rushton for continued support and interest in sample petrography, Joe Emmings for help with R, and Troy Rasbury, Randy Parrish, and Chris Smith for discussion and encouragement during the “early years' of carbonate dating at the BGS.
This research has been supported by the UK Natural Environment Research Council (grant no. NE/S011587/1).
This paper was edited by Catherine Mottram and reviewed by Andrew R. Kylander-Clark and Troy Rasbury.
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