Laura
Hendriks‡
*ab,
Stefan
Kradolfer‡
*b,
Tiziana
Lombardo
c,
Vera
Hubert
c,
Markus
Küffner
d,
Narayan
Khandekar
e,
Irka
Hajdas
a,
Hans-Arno
Synal
a,
Bodo
Hattendorf
b and
Detlef
Günther
b
aLaboratory of Ion Beam Physics, ETH Zurich, Otto-Stern-Weg 5, 8093 Zurich, Switzerland. E-mail: laurah@phys.ethz.ch
bLaboratory of Inorganic Chemistry, ETH Zurich, Vladimir-Prelog-Weg 1, 8093 Zurich, Switzerland. E-mail: krastefa@inorg.chem.ethz.ch
cLaboratory for Conservation Research, Collection Centre, Swiss National Museum, Lindenmoosstrasse 1, 8910 Affoltern am Albis, Switzerland
dSwiss Institute for Art Research (SIK-ISEA), Zollikerstrasse 32, 8008 Zürich, Switzerland
eStraus Center for Conservation and Technical Studies, Harvard Art Museums, 32 Quincy, Cambridge, MA 02138, USA
First published on 14th January 2020
Isotopic studies are gaining much interest in heritage science, as they can provide insight into a material's age and provenance. Radiocarbon (14C) dating affords a time frame for the materials being studied, thus providing a historical context, whereas the specific pattern of lead isotope ratios may be used to set geographical constraints on the source of the original materials. Both methods require invasive sampling from the object, and henceforth limits their respective application. With the focus on lead white paint (2PbCO3·Pb(OH)2), in this study we extract the time of production of the pigment from the carbonate anion by radiocarbon dating while its origin is traced by lead isotope analysis on the cation. The methodology was applied to 12 British and 8 Swiss paintings from the 18th to 20th century, with known dates and provenance. The 14C analysis of the lead white in combination with the organic binder and canvas alone places all objects between the 17th and 20th centuries, which is in agreement with their signed date, wheras the lead isotope analysis of all samples are consistent with lead ores from European deposits. In most of the cases the combined results are consistent with the art historical data and prove that isotope analysis is intrinsic to the object. This feasibility study conducted on paintings of known age demonstrates the possibility to maximize the information output from lead white paint, thus increasing the benefits of a single sampling.
The source of the lead ores used in the production of the lead white pigment can be traced and narrowed to locations by lead isotope analysis, which can then serve as proxy for the provenance of the object.6–9 The variability between the different lead isotopes and different ores is a result of them being at the end of the decay chain of uranium and thorium. The primary ratios change by an increase in the amount of the radiogenic 208/207/206Pb, whereas the 204Pb is not a decay product. A particular example which benefitted from this analysis was the authentication of Vermeer's Saint Praxedis,10 where the lead isotope analysis provided indisputable evidence that the painting was made in Holland and upon comparison with lead white from another Vermeer's picture suggest that both paintings were rendered from the same batch of pigment. During the Middle-Ages, Venice was the major production location for lead white, producing a high quality pigment, “Venetian white”. By the 17th century, it was delocalized to Holland which became the leader in lead white production in the 18th century, where the traditional Stack process was implemented into large scale production and become known as the Dutch process.11 By the end of the 18th century, the Netherlands was home to over 35 lead white factories, from which large exports to other European countries took place.12 In England, following the embargo policies of Elizabeth I, the British lead white industry took off some years after that in Holland, which is extensively reviewed in the work of Rowe (2017).13
The radiocarbon age gained from the carbonate delivers insight regarding the time or method of production of the white pigment. Indeed, depending on the manufacturing process, the carbonate anion will carry a defined 14C signature. In the case of the traditional Stack process, which involves the oxidation of metallic lead over fermenting organic material, the atmospheric 14C signature is trapped in the carbonate and thus can readily be dated. Prior work made use of this property to date ancient cosmetics from the Greeks and Egyptians,14 whereas 21th century Stack produced lead white was dated to the year of production with the help of the “bomb peak” calibration curve.15 By the beginning of the 19th century, new patents replaced the atmospheric source of carbon dioxide with burned coal or other petrochemical feedstock and salt dissolution, which causes a drastic impact on the 14C signature. These geological sources are devoid of 14C, and upon 14C dating translate to ages which are several thousand years. Therefore, the abundance of 14C in lead carbonate can provide information regarding its manufacturing process, as well as the time of production.
The data from such an isotopic analyses can place an object into its historical context. Thus, when focusing on the lead white pigment specifically, analysis provides insights into its production over time emphasizing when the global lead market extended beyond local ores and became a European-wide market. However, to access this information invasive sampling of a work of art is necessary. Pb isotope ratios can be measured from as little as 50–200 μg paint,7 whereas 14C analysis of the lead white carbonate requires more material, between 1 mg15 to 20–25 mg.16
Each technique focusses on a specific ion only, either the carbonate anion for 14C or the Pb-cation, meaning that in both cases the information potential of the sample is not fully accessed. Consequently, there is a need to improve micro-analysis in order to maximise the research output by combining both techniques. The goal of this work is to combine the two isotope systems to gain more insights from a single painting sample that requires minimal sampling.
The mass discrimination correction was performed using the empirically determined value for thallium by applying an exponential model.34,35 Periodic measurements of a certified Pb isotope reference material (NIST SRM981, NIST, USA) were made to monitor the stability of the analyses. All ratios can be traced to reference values of SRM981 published values.36,37 Correction of mercury overlap to 204Pb was carried out in a similar fashion by measuring 202Hg and using the mass discrimination value obtained for 205,203Tl to estimate and subtract the ion signal of 204Hg. The data were evaluated and plotted by the open software R (version 3.4.3, https://www.r-project.org). More detailed information concerning the measurements, the data treatment and all the corresponding parameters/data are given in the ESI (pages S14–17†).
From the collected data, it is clear that the lead white samples, which range from the 18th to 20th century, were produced following the Stack manufacturing process as the measured 14C is present at atmospheric levels. The calibration of the 14C ages to real calendar ages was conducted with the IntCal13 atmospheric calibration curve38 as all objects are pre-1950. Some samples show close to modern 14C concentration (F14C > 1), thus one may infer the use of the post-atmospheric bomb NH1 calibration,39 which results in the same probability distribution as with Intcal13 with the additional extension of the 1950s time window. The resulting broad time intervals are a direct consequence of the numerous wiggles and the plateau shape of the calibration curve between 1700–1950, also known as “Stradivarius gap”.40 This nickname was given following the unsuccessful attempt in using 14C measurements to date the most famous violins of Antonio Stradivari, which were built in the period from 1700 to 1725 AD. This behaviour of the calibration is linked to variations of atmospheric 14C as a consequence of solar activity fluctuations as well as to the increased burning of fossil fuels which dilutes the natural 14C signal, also known as the Suess effect.41–43 An example of this unfortunate situation is depicted in Fig. 1, which illustrates the lead carbonate age distribution resulting from the 14C measurement. A precise dating is impossible and multiple time windows are possible, ranging from 16th to mid-20th century. The same is observed for the dating of the binder and canvas material as displayed in Fig. 2 (sample code LM-161897). Although a more precise dating was not possible, the additional dating of the canvas and the organic binder is of help to constrain the possible time windows, as their respective date ranges agree among each other and the respective calibration is consistent with the signed date of 1813.
From Fig. 2 a similar conclusion can be drawn for half of the investigated paintings, where an overlap of the dating of different materials is observed. Clear examples of such overlaps are Marco Ricci and Sir Arthur Stockdale Cope. Such a statement is however only possible as the attributed dates are known. In the case of unknown aged paintings, a precise dating with micro amounts of lead white is for this period impossible and a larger time window must be considered. A smaller measurement uncertainty would be beneficial, but would require more material and multiple measurements. Therefore, it becomes interesting to date, not only the support material or pictorial layer but all together: the pigment, binder and canvas, and then to observe if their respective 14C ages are consistent with one another.
The 14C signature of the carbonate anion is an archive of the lead white industry, as the varying source of CO2 is recorded in the carbonate. What is interesting in the collected data (see ESI: Tables S3 and S4†) is the widespread of 14C age indicating an atmospheric 14C source, i.e. produced following the Stack process. Surprisingly, few samples show a fossil fuel signature (>1000 years), which is an indication of a 19th century alternative to the traditional lead white production process. In particular, two objects from the beginning of the 20th century, namely from a Swiss artist dated 1907 (LM-158151) as well as British artist 1901 (Sir Arthur Stockdale Cope) still show the signal of a Stack processed lead white pigment. This observation can be explained by the fact that although alternative processes were numerous, the well-known Dutch lead white industry remained the most robust means of lead white production. Artists favoured Stack/Dutch processed lead white owing to its superior quality.44 Thus, although the 19th century was rich in innovations, industries which implemented modern scientific technologies suffered from the competition with the Dutch industry. Homburg and De Vlieger (1996) describe the dominance of the Dutch manufacturing process as “a victory of practice over science”, which is corroborated by Pulsifer (1888) who states that the major factories in France and England mostly reverted to the Dutch process during the 19th century.12,45
Nonetheless, two objects carried a depleted 14C signal, which is characteristic of a fossil source and indicative of alternative production methods to the Stack process. The lead white pigment present in the green paint on the reverse of Margrit's portrait (SIK-98511) was determined to be >5000 years old.¶ The second sample from this study showing a depleted 14CO2 source, belongs to the painting from the British artist Samuel Alken. The 14C data corresponds to an age of >4000 years. Two reasons may be plausible for this result, which could not be verified in the frame of this project. Either the high chalk content present in the sample interacted with the oil matrix and biased the thermal extraction of the lead carbonate, or lead white with a depleted 14C signal maybe produced in the Chamber process following James Creed's patent was available to him while working at the Royal Academy School of London.
With the aim of maximising information output from a unique sample, the possibility of radiocarbon dating the organic binder following the extraction of the carbonate age was also pursued. Unfortunately, Raman analysis very often revealed the presence of carbon black (see Tables S1 and S2 in ESI† regarding material characterisation), which is problematic as it introduces a second source of carbon other than the organic binder. When comparing the 14C ages of the canvas, carbonate and organic binder, paint samples where carbon black is identified, are systematically older than the other two components (ESI: Tables S3 and S4†). The age of carbon black can substantially vary as it is produced from burning organic matter, which is not necessarily from the artist's lifetime. With the aim of dating the lead white isotope when carbon black was identified, the binder age is not considered in the further discussion. When samples were collected from tacking margins, the dating of the canvas was also pursued. From Fig. 2, the additional dating of either the canvas or binder reinforces the lead white dating, and supports the idea that artists used material from their time of activity as the 14C ages correlate with the signed date. In some cases, an offset between the lead white's age and the canvas is observed, which can be explained by different usages of the different materials, such as canvas, pigment and organic binder. It is commonly observed that the canvas support predates the signed date by 2–5 years, although some samples show longer “in-built” ages due to recycling.46 In contrast, the paint materials, namely the pigment and binding media, may have much longer shelf life's varying from years to decades.
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Fig. 3 Lead isotope ratios (± standard deviation) for the sample collection of this project (206Pb/204Pb vs.207Pb/204Pb). The paintings from British artist are labelled blue (points), the ones form Swiss Artists are red (triangles). The three different plots are separated based on the century of the signed date to the corresponding painting. The empty data points represent samples where the CaCO3-load can bias the lead isotope ratios. A representation of all the individually labelled results is given in the ESI (Fig. S7†). The number of data points is corresponding to the amount of different measurements (several replicates per paintings). |
Additionally, the influence of mercury was considered. By visually sampling pure white zones, one can theoretically avoid this contamination but vermilion (HgS) can still occur as it was used as additives in the Stack process to counteract the yellowing of the white pigment.44 The samples “Joshua Reynolds”, “Ricci”, “LM-40076”, “LM-7723”, “LM-52427”, showed a substantial mercury content and were accordingly corrected, resulting in relative changes of between 0.1% and 0.4% to the uncorrected 206Pb/204Pb and 207Pb/204Pb isotope ratios, which were <0.07% for all other samples. The presence of vermilion was confirmed by Raman measurements for “Joshua Reynolds” only. Interestingly, Raman analysis for some samples showed specific vermilion bands but no interfering signal was observed in the ICPMS measurements. The reason is that paint samples may be inhomogeneous in particle distribution, thus although vermilion was not identified in some specific samples, it could still be present as seen in the ICPMS data and vice versa.
The interpretation of the lead isotope ratios is in general a non-trivial task and requires some assumptions regarding the lead ore origin and its processing. Indeed, inhomogeneous lead ore bodies from the same site, different ore bodies with the same isotopic signature, (un-)intentionally mixing of two or more ore sources (blending/recycling), fraction effects during metallurgical handling, etc. are all aspects to be considered in the data interpretation as discussed by Baron et al. (2009).48
The Pb-isotope ratio results for all samples are shown in Fig. 3, grouped by century and itemized for the different origins (British artists in blue and Swiss ones in red). The individual measurement results are listed in the ESI (Table S10†). The whole isotope data set is in the range of 18.37–18.48 for the isotope abundance ratio 206Pb/204Pb and from 15.61–15.67 for 207Pb/204Pb. These values are in general agreement with prior literature concerning the age range (17th–20th century) and may constrain the geographical origin of the lead ore sources.6 All replicates show an expected grouping and a characteristic linearity in the 206Pb/204Pb vs.207Pb/204Pb plot, a feature often reported in Pb-isotopes determination given by the uncertainty on the 204Pb-signal.
A provenance distinction between samples collected from objects from Great Britain and Switzerland is not visually observed in Fig. 3, indeed one observes a rather clear overlap of the isotopic ratios.
In his pioneer work to archaeometric isotope ratio analysis, Keisch et al. (1976) introduced the “Lead Isotope Ratio Index” (LIRI), which combines the measured isotope ratios and plots it against the sample age (see Figure S8†).6 The results obtained in this study are in general agreement with their findings and can be integrated into the framework of lead isotope analysis concerning lead white pigments. We find a narrow distribution of the LIRI before 1850, which points to the signature of British ores (18.2–18.4). This observation correlates with the work of van Loon (2019)49 and fits our expectation as the largest lead white producers of the time were the British and Dutch, which imported British lead, thus resulting in a narrow isotopic spread. Later in the 19th, more European ores (i.e. Germany/Austria)6,45 as well as influence from beyond Europe are to be expected but the calculated LIRI index for the set of studied samples stays fairly constant and does not indicate any apparent influence from globalization concerning the used lead source for lead white in our samples.
Nonetheless, when classifying the data per century, the direct comparison of the ratios 206Pb/204Pb vs.207Pb/204Pb, becomes clearer. In Fig. 3 the analyzed paintings are separated into 18th, 19th and 20th century, which provides a better distinction of the lead isotopes’ variations. Paintings originating in the 18th century show a close grouping around 15.62 and 18.45 for 207Pb/204Pb and 208Pb/204Pb respectively. In the 19th century, a transition phase is noticeable as the clustering gets larger: in particular, two sub-cluster can be identified, one overlapping with those from the 18th century paintings while the second group has lower 206Pb/204Pb ratios of 18.38. These latter ones relate to artworks dated after 1860 (LM-114651, Wells (duplicate)). The isotope ratios for the later work (20th century), on the other hand show substantially higher 207Pb/204Pb which was also observed in the work by Stevenson (2016).9 When plotting the isotope ratios 207Pb/206Pb vs.208Pb/206Pb, (ESI: Figure S9†) a similar grouping for the individual periods is becoming apparent. The older paintings are characterized by lower values and both increase with the dated age. The transition phase for the 19th century is again present. Most 19th century belonging objects show a similar grouping with the data of the 18th century. In particular, sample LM 161897 (1813) shows a very close overlaps and as already discussed, two exceptions dated after 1860 (LM-114651, Wells) show a distinct separation.
The isotope composition for lead ores all over Europe is given as a complicated, not always distinct distribution and some ore sources show some overlap.7,8 The presented data agree with reference data from several lead ore sites, in particular those from Great Britain (all), Germany (all), Poland (17th/18th), Spain (20th) and Netherlands (19th/20th). Solely there is no overlap with the data from Italian ores sites and it seems very unlikely that lead white from non-European lead ores are present in the listed sample set.||
Among the objects of study, the tacking margins of the British paintings (see Figure S3, ESI†) which were removed upon lining the original canvases, were ideal in the sense that enough material was present (10–100 mg) and were collected in a passive manner, i.e. the lining process is a common practice, and the removal of tacking margins was an accepted part of the treatment at that time. After separation from the textile threads 3 to 30 mg lead white bearing paint was collected, which resulted in 20–100 μg C from the lead white pigment. Sample LM-161897 depicted in Fig. 1 was collected from the canvas corner edge below the frame, hereby providing 25 mg material comprising textile and paint material. However not all artworks are framed and could be sampled below the frame nor are they painted over the edges, thus reducing the possibilities for discrete sampling. Figure S1/2 from the ESI† illustrates the sampling of the Swiss artist's objects, where paint material was scratched off the edges of the work and amounted to 0.7 to 3 mg material. Overall all collected samples provided sufficient material to conduct both 14C analysis followed by lead isotope ratio analysis. Only sample LM-161803, which weighed 0.7 mg, represented not enough material for the analysis (<10 μg C from the carbonate, <10 μg remaining material for Pb-analysis).
The results obtained in this study showcase the benefit of combining multiple (isotope-) techniques and use them as proxy to place an artwork in an historical context. The interpretation of the individual results coming from the two methods relies on additional information provided by historical context such as production process, raw material source involved and trading, etc. Overall, the data collected in the frame of this feasibility study delivers a consistent pattern between signed dates, their radiocarbon ages (see Fig. 2), their spread of the lead isotopes based on their age (see Fig. 3) and the comparisons with possible raw material sources.
However, this paper does not claim it can solve authentication cases alone. Indeed, the data set of this study was limited to about 20 paintings, a larger number of samples would be more representative. Furthermore, the aim of the presented work was not to present an in-depth art historical interpretation and discussion regarding the trade/production/use of lead or lead white pigment but rather to demonstrate the successful approach in extracting supplementary information by combining isotopic analysis from a single lead white bearing paint sample.
The gathered data on the chosen examples from both Swiss and British artists covering the 18th to 20th centuries, show trends directly related to the lead white industry. Pb-isotopes give insight into the trading of the raw material i.e. up until 1860s a single cluster is observed, which points to a single source of lead (likely British ores), while after 1860 a larger spread in Pb-isotope ratio is noticeable. The later points to increased mining activities in different ores sites across Europe, which correlates with industrial development. In order to successfully apply the methodology for authentication issues, a broader Pb isotope ratio database would help to support statements about geographical classifications, which has already been launched by other groups. Such broader campaigns are ongoing, namely a large project funded by the Netherlands Institute for Conservation, Art and Science (NICAS) entitled Multi-isotopic analysis of early modern art (MITEEMA). Unfortunately, at the time of this study, their results were not yet published.51
With respect to 14C dating, the calibration of the 14C ages will define the ambiguity of the data. In the frame of this validation study, the results were coherent with the signed date, hence demonstrating the proof of principle of the method. In real case applications, 14C analysis is only considered in a last instance, as the method is both invasive and destructive. Moreover, when sampling is granted, the results are expected to be meaningful, i.e. provide a precise dating. When targeting a likely attribution between 1700–1950, however, no decisive evidence is possible using micro-sampling. In contrast, for objects belonging to other time periods, such as the 13th century or created following the bomb peak (post-1950) a microscale approach is feasible. Hence, when considering uncertified objects, incoherencies between the different 14C ages can be considered as red flags. For instance, if an attributed 16th century painting displays a depleted 14C lead white signal, synonym of 19th century production, or an enriched signal typical for bomb peak material, it is an obvious chronological inconsistency. Unfortunately, today's rate of fossil fuel consumption and respective CO2 emission is reducing the relative content of the atmospheric 14C content, which in turn no longer allows the conversion of 14C ages to definite dates. In particular, if lead white is prepared within the next decade following the traditional method, its 14C signal will show a similar 14C signature to Roman or medieval periods, meaning that radiocarbon dating will be useless for objects with insufficient context.
The present discussion has been limited to the lead white pigment but did not extend to the paint matrix, which also carries information. The investigation of (ultra-)trace element composition of different pigments may be a further direction of research, to identify specific fingerprints related to origin, production or historic events, such as the nuclear weapon testing.
Footnotes |
† Electronic supplementary information (ESI) available: General sample description and sampling location Fig. S1, 2, 3 and Tables S1, 2. Radio carbon data measurements Tables S3, 4. Digestion protocol Table S5. ICP-MS parameters Tables S6, 7. Lead isotope data and quality control Tables S8, 9, 10 and Fig. S4, 5, 6, 7, 8, 9. See DOI: 10.1039/c9an02346a |
‡ These authors contributed equally. |
§ Historically Accurate Oil Painting Reconstruction Techniques, in short the HART project was part of the De Mayerne Programme led by Professor Dr Jaap Boon and funded by the Netherlands Organisation for Scientific Research (NWO) between 2002 to 2005, where Dr Carlyle was Principle Investigator (Carlyle, HART Project Report, 2005). |
¶ In comparison to previously published value of 25![]() |
|| Lead white literature mentions significant difference in product quality and it is commonly agreed that the lead white denoted as Venetian white as well as Kremeserweiss are of superior class, rendering the purest white but are also the most expensive.52,54 Both products are locally produced and henceforth carry a defined Pb isotope fingerprint. Kremserweiss played an essential role on the continent since the late 18th century and may explain the observed spreading in lead isotopic ratios. |
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