In 1954 archaeologists excavated a shrine to an unknown deity at the Greek settlement of Paestum in southern Italy, which was dated to the sixth century BC. Within this shrine they found six bronze hydriai (storage jars) and two amphorae, arranged around a large iron bed. The jars contained a pasty residue with a wax-like aroma. Traces of this substance were also found on the outside of the jars, which were originally sealed with cork, leading the archaeologists to conclude that it was originally a liquid, although possibly a fairly viscous one. It was interpreted that the bed was intended to be the residing place of the unknown deity, with the contents of the hydriai and amphorae were intended as offerings.
Honey, in the Greek and Roman worlds, was a substance of some significance. As the only practical way to sweeten food and drinks, it was economically important, but it also had spiritual significance, being associated with wisdom and immortality, and therefore a suitable offering to the gods. With this in mind, it seemed highly likely that the original contents of the Paestum hydriai was honey.
With this in mind, the Bee Research Association in London arranged for an analysis of the residue to be carried out. The substance was found to be insoluble in water, but soluble in organic solvents, and to contain trace amounts of Plant and Insect remains, Fungi, and pollen, which led the scientists carrying out the analysis to conclude that it was probably a remnant of the wax which had originally sealed the jars.
In 1970 scientist at the Istituto Centrale del Restauro in Rome carried out an analysis on residues found around the neck and in the bottom of one of the amphorae from Paestum. This was found to comprise a saponifiable substance (substance which will react with an alkali to form a soap), such as a wax, fat, or resin, but contain no detectable sugar or protein (the major components of honey).
The residue was tested again in 1983 by the Laboratory of the Rome Chamber of Commerce, who again found that it was a saponifiable substance insoluble in water but soluble in organic solvents, and did not contain any sugary or starchy substances. On this occasion gas chromatography was also used to analyse the residue, concluding that it was 77.4% palmitic acid, 6.1% oleic acid, 5.2% stearic acid, 1.0% heptadecanoic acid, 1.0% linoleic acid + arachidic acid, 0.4% linoleic acid, and 6.5% unidentified substance. Since triglycerides of palmitic acid are extremely common in nature, the researchers concluded that the container had held animal fat or a vegetable oil.
In 2019, the residue from the Paestum hydriai was loaned to the Ashmolean Museum in Oxford, for an exhibition, 'Last Supper in Pompeii', and permission was obtained to carry out a new analysis of the biomolecular composition of the substance, using modern equipment not available when the previous tests were carried out.
In a paper published in the Journal of the American Chemical Society on 30 July 2025, Luciana da Costa Carvalho and Elisabete Pires of the Mass Spectrometry Research Facility at the University of Oxford, Kelly Domoney of the Ashmolean Museum, Gabriel Zuchtriegel of the Parco Archeologico di Pompei, and James McCullagh, also of the Mass Spectrometry Research Facility at the University of Oxford, present the results of this new analysis, and confidently identify the original material within the Paestum hydriai.
The residue arrived at the Ashmolean Museum in a non-hermetically sealed Perspex box, in which it had apparently been displayed at the Paestum Museum. In order to reduce the chances of modern contamination affecting their results, Carvalho et al. took samples from 40 mm below the surface for analysis, as well as from each distinct colour zones observed on the exterior of the material; black, orange, and green, colours which suggest some sort of interaction with the bronze vessel itself over the past 2500 years. Carvalho et al. also obtained modern beeswax, honey, and honeycombs from locations in Italy and Greece in order to compare these to the residue sample.
Carvalho et al. first used Fourier Transform Infrared Spectroscopy to obtain an overview of the chemical substances present within the sample. This yielded a spectrum almost identical to that of modern beeswax for the interior sample, strongly supporting the idea that this was the original substance. They also compared the spectra of new and artificially aged honeycombs from both Greece and Italy, establishing that there was little difference in these, and that these structures appear to be chemically stable at least
Next, Carvalho et al. carried out a Gas Chromatography coupled to Quadrupole Time-Of-Flight Mass Spectrometry analysis of the sample, along with samples of honey, beeswax, and fresh and artificially aged honeycomb. This produced almost no results for the beeswax, suggesting that the bulk components of this material were broken down by the high temperature at which this method operates (over 300°C), but did produce results from the sample, as well as from the honey and honeycomb controls, suggesting that the sample was never pure beeswax.
Anion exchange Ion-Chromatography coupled to Mass Spectrometry identified seven hexose sugars, hexadecanoic acid, heneicosane, octadecanoic acid, pentacosane, heptacosane, nonacosane, and hentriacontane within the sample at levels higher than would be expected in beeswax, but lower than would be expected in honey. It also found significant levels of the sulphur amino acid taurine, which was not present in any of the control samples.
These hexose sugars were also recovered from aqueous extracts of honeycomb (i.e. the liquid obtained by soaking honeycomb in water)along with gluconolactone (a derivative of glucose) and galacturonic acid, and low levels of succinic, malic, and citric acids. All of these compounds were yielded at higher levels by the fresh honeycombs than by the artificially aged honeycombs.
Finally Carvalho et al. used a proteomic approach to try to identify specific proteins within the sample, as well as the beeswax and honeycomb controls, which were compared to the UniProt All Proteins database. The reesidue sample produced matches for three proteins derived from the royal jelly produced by the Western Honeybee, Apis mellifera, several Bacteria-derived proteins, and a number of common contaminant proteins, including keratins, caseins, lysyl endopeptidase, and trypsin. Encouraged by this, they then compared the sample to the Bee-specific UniProt Honey database, a search which yielded eight matches, including some associated with the Eastern Honeybee, Apis cerana cerana,
Proteins were also recovered from the modern honeycomb samples, but not the beeswax, indicating that they were derived from the honey portion of the comb. Notably, the royal jelly protein signature from the Greek and Italian honeycombs was quite different, although this was not completely unexpected as the two looked different. Carvalho et al. note that factors such as climate and the floral sources from which nectar is obtained can affect protein expression in Bee products, so this difference does not necessarily mean the Bees were particularly different.
Finally, a sample of the surface residue showing orange, black, and green colouration was subjected to X-ray photoelectron spectroscopy. This determined that the green areas of this residue were composed of 74.98% carbon, 20.78% oxygen, and 4.24% copper, with the copper portion largely dominated by Cu²⁺ ions, while the black areas were composed of 77.96% carbon, 20.12% oxygen, and 1.92% copper, with the copper dominated by Cu⁺ ions, and the orange areas were comprised of 86.50% carbon and 13.50% oxygen. The discoloration in these areas is, therefore, presumed to be derived by interactions between the original substance and the copper portion of the bronze vessel.
Honey is comprised primarily of sugars (typically 79% of the total mass, including 39% fructose), along with water (typically 18% of total mass), acids (0.17-1.17% of total mass) and trace amounts of other substances, such as vitamins, enzymes, flavonoids, and phenolic compounds. Over time this mixture undergoes Maillard reactions ('browning') as the amino acids of the proteins react with the sugars. This will occur more rapidly if the honey is stored at a warmer temperature. Eventually, the honey will take on a dark hue, as the sugars break down into furans and the acid content rises.
Previous studies of the Paestum hydriai residues concluded that this was a wax, most likely used to seal the vessels. The most commonly use wax in the ancient world was beeswax, a substance with quite different properties to honey. Beeswax is typically comprised of about 64% esters, 14% odd medium chain alkanes, 12% free acids, 2% acid polyesters, 1% acid monoesters, 1% free alcohols, and 6% other materials. Beeswax is much more stable than honey, but over time the acid and alcohol contents will increase as the was esters hydrolyse and the shorter chain alkanes are eliminated.
The Fourier Transform Infrared Spectrum obtained by Carvalho et al. yielded results very similar to beeswax, suggesting that this may have formed a significant portion of the material from which the residue was derived. However, the Gas Chromatography coupled to Quadrupole Time-Of-Flight Mass Spectrometry analysis carried out suggested that the substance could not be pure beeswax. A study of the proteins present within the sample found several associated with honey production in the Western Honeybee, Apis mellifera, with a subsequent search of the Bee-specific UniProt Honey database yielded proteins associated with the Eastern Honeybee, Apis cerana cerana. Also produced were proteins associated with the wood-decay Fungus Armillaria gallica, and the parasitic Mite Tropilaelaps mercedesae, which targets Honeybees.
Eastern and Western Honeybees are closely related, and even where divergence has occurred, their proteins tend to be very similar. Furthermore, there is ample evidence for the cultivation of the Western Honeybee in ancient Italy, but none for the Eastern Honeybee. For these reasons, Carvalho et al. conclude that the readings suggesting the Eastern Honeybee as a source of proteins are probably erroneous, caused by the software trying to 'best fit' ancient degraded proteins.
The presence of proteins associated with the Mite Tropilaelaps mercedesae is also interesting. This Mite originated in Asia, and has a long historic connection with the Eastern Honeybee, but is generally thought only to have begun to infect Western Honeybees in the past few centuries. Carvalho et al. observe that it would be tempting to interpret this as evidence that the material at Paestum originated in Central Asia, but that a more likely scenario is that the proteins in question are common to a range of Acarid Mites.
Carvalho et al, conclude that a bulk composition similar to beeswax combined with the presence of proteins and other molecules found in honey make it likely that the material within the Paestum hydriai was almost certainly a honeycomb. This matches well with ancient literature, which frequently cites honey and other Bee-products as being suitable offerings for the gods, but contradicts earlier studies which were unable to obtain this result. Carvalho et al. emphasise that this underlines the importance of revisiting samples which have previously been analysed with less modern techniques, thus allowing our imptoving technology to improve our understanding of the past.
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