For each painting analyzed, several small areas were chosen to examine based on pigment hue, apparent homogeneity of the paint, and the thickness of the paint. Data was obtained with a Bruker Tracer III-SD pXRF detector, and analyzed in Bruker’s S1pXRF software. The spectra for the different points were compared to one another in order to attempt to isolate the constituent elemental building blocks responsible for a particular hue. In some cases, a distinct pigment color was determined, and in others, the colors were clearly a blend of two or more colors. Though some of the pigments analyzed remain ambiguous, for the most part this method of analysis was successful.
There are two major drawbacks to using pXRF to analyze pigments. The first is that the Bruker pXRF instrument is unable to detect organic elements due to the low fluorescence energy levels of low Z-number elements. This means that the analyses presented here are likely incomplete. A number of organic based pigments exist and are frequently used, but given the inability of the instrument to detect them, they were necessarily ignored for this study. In some cases, it is noted that due to a lack of otherwise compelling data, organic pigments are the most likely source of a color, but this is inference based on a lack of evidence.
The second drawback is that fundamentally, XRF analysis is unable to detect chemical structure. The elemental composition is read, but the chemical bonds between the elements are not (Cesareo et al 2008, 206, McGlinchey 2012, 131). Many elements are present in a wide variety of pigments. Iron (Fe) for example can be found in hematite red, orange and yellow ochre, and even Prussian blue (Eastaugh et. al. 2004, 112, 144). When each pigment point is analyzed, the hue of the point must be taken into account when attempting to find the best chemical fit for the elements present. Below is a table summarizing the pigments identified in this study with their chemical formula and earliest known use.
Pigment name
|
Chemical Formula
|
Date
|
Barium white
|
BaSO4
|
Used in Antiquity, manufactured from 1830CE in France
|
Titanium white
|
TiO2
|
First produced in 1821CE, but not available to artists until the late 1920s CE
|
Lead white
|
Pb3(CO3)2(OH)2
|
At least as old as 1500BCE in Egypt and Greece
|
Zinc white
|
ZnO
|
First produced as early as 1782CE, mass produced by 1835CE
|
Realgar red
|
As4S4
|
Used in antiquity
|
Hematite (or ochre)
|
Fe2O3
|
Used since prehistoric times
|
Red lead (minium)
|
Pb3O4
|
Used since the Roman empire
|
Vermillion red
|
HgS
|
Used in antiquity
|
Lemon yellow
|
BaCrO4 or SrCrO4
|
Discovered in 1809CE
|
Cadmium yellow
|
CdS
|
Discovered in 1817CE
|
Chrome yellow
|
PbCrO4
|
Discovered in 1809CE
|
Zinc yellow
|
ZnCrO4
|
Discovered in 1809CE
|
Chromium oxide green
|
Cr2O3
|
Discovered in 1809CE
|
Cobalt green
|
Co – doped zinc oxide
|
Discovered in 1809CE
|
Verdigris green
|
Cu(C2H3O2)2 • 2Cu(OH)2
|
Used in antiquity
|
Azurite blue
|
Cu3(CO3)2(OH)2
|
Known since the 15th century, manufactured artificially since the 18th century
|
Cerulean blue
|
CoO • SnO2
|
Introduced in 1821, reintroduced in 1860
|
Cobalt blue
|
Co – doped alumina
|
Discovered in 1775, manufactured from 1804 for artists
|
Egyptian blue
|
CaCuSi4O10
|
Used in antiquity
|
Han blue
|
BaCuSi2O6
|
Discovered in 1859
|
Prussian blue
|
(Fe4[Fe(CN)6]3)
|
Known since 1704, manufactured from 1870 for artists
|
Smalt
|
Co – doped Si glass
|
Known since mid-16th century
|
Cobalt Violet
|
Co3(PO4)2 or Co3(AsO4)2
|
Discovered in 1859
|
Table 1: Pigment names and chemical formulas (From Artioli 2010, Roy 1986, and Wehlte 1975).
2.1 Sample Painting Analysis
Elemental data points were collected across all 33 paintings, then collated and compared. An example of how the analysis was carried out across the assemblage can be seen here with the 1922 painting Dawn in the Hills (Figure 1). Apart from being a particularly beautiful painting in its own right, Dawn in the Hills is highly treasured due to the fact that it is the last painting that Onderdonk ever painted (Rudolph 2008, 40).
A total of seven points were analyzed for this painting. Points 1 and 2 are the whites of the sky, points 3 and 4 are blues, point 5 is the green of the tree to the left of the painting, point 6 is the reddish background in the lower left-hand corner, and point 7 is the signature. This painting was framed and unable to be removed from the frame, but for those that were unframed or able to be removed from a frame, a portion of non-painted canvas was analyzed to determine the elements present in the primer. After each point was tested, they were analyzed by color grouping.
2.1.1 White
The elemental composition of the white of the clouds in points 1 and 2 are predominantly zinc and lead, and therefore are most likely to be a zinc white and a lead white. Both zinc and lead peaks are consistent across all peaks, and so it stands to reason that the painting was primed with both.
2.1.2 Blue
Both blues of points 3 and 4 are clearly cobalt based when compared to the white spectrum of point 1. As with the rest of Onderdonk’s paintings in the 1920s, this cobalt based blue does not have the indicative tin or aluminum peaks that would point toward cerulean blue or cobalt blue. Nonetheless, this cobalt signature is consistent with the other blues in Onderdonk’s late period work.
2.1.3 Green
The green of point 5 is a chromium based green, almost certainly chromium oxide (emerald green).
2.1.4 Red and Signature
The area behind the signature is a reddish orange, which appears to be iron based, indicating hematite. In point 6, there is also a trace of mercury, indicating that the red highlights are vermillion (HgS) instead of iron. Point 7, the signature, has a slightly higher peak for chromium, likely indicating that the red and green were mixed to make a darker color.
For Dawn in the Hills, as the spectra were analyzed, the results were added to a spreadsheet for comparison across the collection. As the results continued to build, patterns and trends started to become clear.