Archaeological glass contains information about the movement of goods and ancient economies, yet our understanding of critical aspects of the ancient glass industry is fragmentary. During Roman times, distinct glass types produced in coastal regions of Egypt and the Levant used evaporitic soda (natron) mixed with Nile-derived sands. In the Levant, furnaces for producing colourless Roman glass by addition of manganese have been uncovered, whereas the source of the desirable antimony-decolourised Roman glass remains an enigma. In the Edict of Diocletian, this colourless glass is listed as “Alexandrian” referring to Egypt, but its origin has been ambiguous. Previous studies have found overlapping strontium and neodymium isotope ratios for Levantine and Egyptian glass. Here, we confirm these findings and show for the first time, based on glasses from the ancient city of Gerasa, that hafnium (Hf) isotopes are different in Egyptian and Levantine natron glasses, and that Sb Roman glass is Egyptian. Our work illustrates the value of Hf isotopes in provenancing archaeological glass. We attribute the striking difference in Hf isotopes of Egyptian versus Levantine glasses to sorting of zircons in Nile sediments during longshore drift and aeolian transport along the south-eastern Mediterranean coast leaving behind a less juvenile fraction.
The Roman glass industry underwent a massive expansion over the first century CE. At its peak it supplied not only tablewares for households across the Empire but also furnished major public buildings with many tonnes of glass for windows and mosaics1,2. The raw glass was made by fusing Egyptian evaporitic soda (natron) and sand to produce large glass slabs in tank furnaces with capacities of 8–20 tonnes3,4. These were broken up and distributed to glass workshops where the glass was remelted and shaped into objects for use5,6. This division of production continued until at least the ninth century, when a change from a mineral soda flux over to plant ash occurred bringing about the end of the Roman glassmaking tradition7,8.
The technological achievements of the Roman glass industry were precocious and not surpassed until the rise of the European industries in the eighteenth century. In particular, the Romans produced large quantities of an expensive and highly valued glass, described by Pliny9 as “colourless or transparent, as closely as possible resembling rock crystal” (Fig. 1), where the iron from the sand was oxidised from blue Fe2+ to very pale Fe3+ by the addition of antimony oxide, Sb2O310,11. In the Price Edict of Diocletian, this colourless glass is listed as “Alexandrian” thereby referring to Egypt12. Despite this, the production site for this so-called Sb Roman glass is unknown but several authors have suggested, on the basis of circumstantial evidence, that it was in Egypt13,14 (see Supplementary Information for details).
Strong evidence that the primary glassmaking factories melting sand and natron to glass were predominantly located along the coast of the eastern Mediterranean is provided by isotopic measurements. Strontium (Sr) isotope compositions for the majority of natron glass groups are close to that of modern seawater, indicating the incorporation of marine shell in the batch and suggesting the use of beach sand as a silica source15,16,17. With regards to neodymium (Nd) isotopes, nearly all natron glass types show a characteristic Nile-related signature reflecting the use of coastal sands along the south-eastern Mediterranean that comprise largely Nile-derived sediments transported here by longshore drift18,19. Hafnium (Hf) isotopes have not previously been applied to man-made archaeological material (see Supplementary Information). Here, we present Sr, Nd and Hf results on natron glass types and show that, unlike the Sr and Nd systems, hafnium isotopes distinguish between natron glass made in Egypt and those made in the Levant, and, in particular, place the production of Sb Roman glass in Egypt.
The modern town of Jerash, located about 50 km from modern Jordan's capital Amman (ancient Philadelphia), is the location of the ancient city of Gerasa, which belonged to the Decapolis, a group of semi-autonomous Greco-Roman city states operating under Roman protection20 (Fig. 2). The city prospered during the first millennium CE until an earthquake in 749 CE led to its demise and abandonment21,22. Samples for this study come from excavations undertaken by the Danish-German Jerash Northwest Quarter Project in highest area within the ancient walled city where our previous elemental and Sr isotope analyses of 25 glass vessel sherds showed a dominance of Apollonia-type glass from the Syro-Palestinian Coast dating to the Byzantine period along with a small early Roman glass assemblage23,24.
Our screening of a further 160 glass fragments shows the presence of a larger number of previously-established compositional groups: Mn Roman and Levantine-I glass types from Syro-Palestine as well as high TiO2 Egypt-Ib, Egypt-Ic and Foy 2.1 types from Egypt. Two additional identified types, Sb Roman and Sb-Mn Roman glass, cannot be unambiguously attributed to either Syro-Palestine or Egypt. The latter glass type, Sb-Mn Roman glass, shows characteristics of both Roman glass types because it is the result of mixing Sb Roman and Mn Roman type glasses during recycling25. On the basis of our screening, a subset of 37 sherds from Gerasa that includes representatives of all identified natron glass types was chosen for Sr, Nd and Hf isotopic analysis.
Dissolution and ion exchange chromatography were performed for 20 mg fresh glass collected from the centre of the vessels to avoid exposed surface contamination. Strontium, neodymium and hafnium isotope analyses were done by Multicollector-ICPMS at AGiR platform using a DSN nebulizer. Hafnium fractions were run in 2% HNO3–1% HF, mass fractionation corrected for by normalising to 179Hf/177Hf of 0.7325 and the results normalised to our in-house Ames Hf standard that was adjusted to the low Hf intensity of the glass solutions (down to 20 ppb total Hf). Neodymium and strontium analyses were corrected by normalisation to 146Nd/144Nd = 0.7219 and 86Sr/88Sr = 0.1194 and to the JNdi and NBS 987 standards, respectively. Well-characterized glass and basalt standards were processed and run with the samples to characterise reproducibility and accuracy. For major and trace elements, 1mmx1mm fresh glass fragments were mounted in epoxy, polished and analysed by electron microprobe and Laser Ablation ICPMS. See Supplementary Information for detailed description of our methods and SI Table S2 for analytical data.
Results and discussion
Sr, Nd and Hf isotope compositions of the Gerasa glasses are presented in Fig. 3 as Egyptian groups (panel 1), Levant groups (panel 2) and recycled Roman glass (panel 3). We include Sb Roman glass with the Egyptian glass groups on the basis of our new Hf isotope data (see discussion below). Nd and Hf isotope compositions are reported using the conventional εNd(0) and εHf(0) notations that show part per 10,000 deviations from the present-day chondritic uniform reservoir (CHUR) values26 (see Fig. 3 caption and Supplementary Information for details). The 87Sr/86Sr ratios for all glass types fall within a narrow range (0.7085–0.7091) close to modern-day seawater27 (Fig. 3a). The only exceptions are Egypt Ib glasses with markedly lower 87Sr/86Sr ratios (≈ 0.7075). Likewise, εNd(0) values for all glass types overlap within analytical uncertainty (Fig. 3b), while εHf(0) for Egyptian and Levant glasses are clearly distinct with the former below and the latter above − 12.2 (grey dotted line in Fig. 3c). The εHf(0) values around − 13.9 for Sb Roman glasses place this type with Egyptian products and are indistinguishable from Egypt I and Foy 2.1 glasses. A critical observation from Fig. 3c is that the εHf(0) values observed for Sb-Mn Roman glass encompass the entire Egypt and Levant range (panel 3 in Fig. 3c) as would be expected for mixtures of glass from Egypt (Sb Roman) and the Levant (Mn Roman). Hf isotopes in natron glass of unknown provenance therefore fingerprint whether the glassmaking sands were from Egypt or the Levant, and place Sb Roman glass production in Egypt.
To illustrate the underlying processes responsible for the difference in the Hf isotope signatures of Egyptian and Levant glasses, we begin by considering how trace elements, 87Sr/86Sr and εNd(0) compositions of our Egyptian and the Levant type glasses from Gerasa cannot be utilise to unambiguously distinguish sand sources on the coasts of Egypt and Syro-Palestine.
The locations of the raw glass furnaces so far discovered occur mainly on the coastal strip of Syro-Palestine (e.g. Apollonia and Jalame in Fig. 2). Published evidence for primary glass furnaces in Egypt is limited, apart from those close to the ancient soda sources around the Wadi el Natrun, some 50 km northwest of Cairo4 (Fig. 2). Because of this paucity of known Egyptian production sites, and restrictions on the availability of Egyptian cultural material for analysis, attribution of glass types to Egypt is generally inferred from (1) a failure to match the elemental compositions of the well-characterised products of the Palestinian furnaces and (2) the elevated TiO2 concentrations, which are characteristic of the limited data on Egyptian sands as well as of well-provenanced Egyptian glass dating to the Islamic period28,29. However, this approach does not exclude potential sand sources in other areas of the Mediterranean where Nd isotopic compositions and Ti concentrations are broadly consistent with the inferred Egyptian glass compositions19,30. It would also fail for any glass made in Egypt using high quality sands, which had been intentionally selected to be low in iron oxides (and thus unlikely to have elevated TiO2) such as the sands used in the renowned antimony-decolourised glass.
The 87Sr/86Sr ratios just below the value for Holocene seawater observed for the Gerasa glasses conform to previous observations for natron glass and reflect the presence of present-day marine carbonates in the glassmaking recipe16,17,18 (Fig. 3a, SI Fig. S1). Slightly low radiogenic 87Sr/86Sr ratios of 0.7085 for one Mn Roman and one Sb-Mn sample are likely due to minor contamination by strontium from the Mn-ore added to decolourise the glass16,31,32,33 (Fig. 3a). Even lower 87Sr/86Sr ratios around 0.7075 for the Egypt Ib samples can be explained by relative high contributions of strontium from minor minerals in the glassmaking sands due to a low carbonate component in the glasses (as reflected by their low CaO concentrations; SI Table S1). Irrespective of these minor variations, the homogeneous 87Sr/86Sr ratios in glass types from the two regions exclude strontium isotopes as a discriminant between glass from Egypt and the Levant.
Hafnium and neodymium in natron glass are controlled by minerals in the sands used for glass production. A complication in distinguishing sands along the south-eastern Mediterranean coast is their common origin from the Nile Delta. The Nile drains large and widely different terranes producing sediments that accumulate in the Delta and from here are transported due to the Nile littoral cell by longshore drift around the south-eastern Mediterranean and, to a smaller degree, via aeolian transport to the coasts of Sinai and modern-day Israel34,35 (Fig. 2). The two major Nile tributaries, the Blue Nile and Atbara, carry mafic minerals (in particular pyroxene) high in neodymium from Tertiary basalts in the Ethiopian highlands36 (Fig. 2). The result is the slightly negative εNd(0) values observed for Nile delta and coastal sands as well as in Egyptian and Levantine glass14,16,18,19 (Fig. 3b; SI Fig. S1). Slightly higher concentrations of Nd in Egyptian natron glass (8–11 ppm) versus Levantine glass (5–8 ppm) indicate the partial loss of these mafic minerals during longshore transport37, while the εNd(0) values remain constant (SI Table S2).
Hafnium in Nile sands and thus natron glass originates from the mineral zircon that traces the detrital quartz component38. The Nile, Sinai and Red Sea follow a collision zone (the northern end of the East African orogeny) that marked the closure of east and west Gondwana and consisted of oceanic island arc volcanics with back-arc sedimentary basins, in some periods mixed with older crustal materials36. Extensive work has shown that zircons and quartz in Nile sands derive from detrital rocks that formed from the breakdown of these collision-zone terranes. The source rocks have been suggested to be the Cambrian-Ordovician sandstone covering much of North Africa35 or the Um Had Conglomerate although the latter is mainly made up of material eroded only from the Arabian-Nubian Shield39 (Fig. 2). As observed for the minerals controlling neodymium, zircon drops out of the sediments during longshore transport34, which is reflected in the Hf concentrations of 2–4 ppm for the Egyptian natron glass versus below 2 ppm in the Levantine glass from Gerasa (SI Table S2). An important implication of our study is therefore that the longshore transport of the Nile sediments not only leads to lower Hf concentrations in the sediments (and thus glass) along the Levantine coast, but also to changes in the Hf isotope composition. This could be due to (1) the addition of zircons of different compositions delivered by rivers which drain inland Israel or (2) a preferential deposition of larger, non-juvenile zircons during longshore transport. The first possibility can be excluded since the inland lithologies from modern Israel are dominated by carbonates, while siliciclastic sediments of Jordan drain eastwards rather than towards the Mediterranean coast40. Therefore, it appears that there is a progressive change in the Hf isotopic composition of eastern Mediterranean coastal sand due to hydraulic sorting of zircons of different ages and size. Unfortunately, Hf isotope data for bulk sands to confirm this have not been reported from the Nile Delta and Sinai-Israeli coasts. Fieldings et al.41 report values of − 15 to − 22 (average of − 18) for 5 bulk aeolian sands from the Western Desert (WD-C samples in their Fig. 1), which match well the εHf(0) of − 16 to − 13 observed for Egyptian glass groups but their εNd(0) values and location suggest that they are unlikely to have supplied abundant material to the sands of the eastern Mediterranean coast.
While Hf isotope studies of bulk sands are limited, numerous studies have utilised combined U–Pb dating and Hf isotopes of the detrital zircon populations in Nile sands from the Egyptian and Israeli coasts to constrain the sediment source(s). These show identical εHf(0) overall systematics with a dominance of 0.56–1.15 Ga zircons with εHf(0) of + 12 to − 70 representing a mixture of juvenile and non-juvenile late Mesoproterozoic to Neoproterozoic sources, as well as small populations of Archaean–Palaeoproterozoic and Palaeozoic zircons35,39,41. However, these studies target cores and only sometimes include analysis of rims from single, often zoned zircon grains39,41,42,43 and cannot be directly related to bulk sand compositions. Thus, analysis of bulk Nilotic sands would be required to evaluate the fractionation mechanism proposed here. For the present, we conclude that natron glass groups reflect the sorting of zircons during the longshore transport of glassmaking sands leading to a change in Hf isotope compositions along the Mediterranean coast. This feature of the coastal sands has enabled us to confirm suspicions that the famous colourless glass of ancient Rome was indeed produced in Egypt despite its low TiO2, Zr and Hf concentrations. The reason for the latter characteristics is most likely that iron-poor sands were targeted for their production and that these sands had zircons that were not yet sorted due to longshore transport (and thus were located in Egypt). Hafnium isotopes are likely to become increasingly important in tracing the products of the early glass industries, not only in Roman empire, but also elsewhere.
All data are supplied in this article, Supplementary Information and Supplementary Data Tables.
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The work was supported by Carlsberg Foundation, the Danish National Research Foundation under Grant DNRF119 (Centre of Excellence for Urban Network Evolutions-UrbNet), the Danish National Research Foundation under Grant 26-123/8 (Niels Bohr Professorship in Geoscience), the Deutsche Forschungsgemeinschaft; Deutscher Palästina-Verein; the EliteForsk initiative of the Danish Ministry of Higher Education and Science, and H. P. Hjerl Hansens Mindefondet for Dansk Palæstina-forskning. We thank O. Neill (GeoAnalytical Lab, Washington State University) for performing the EMP analyses, and R. Andreasen and I. Søgaard for assistance during MC-ICPMS analyses and cleanlab processes.
The authors declare no competing interests.
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Barfod, G.H., Freestone, I.C., Lesher, C.E. et al. ‘Alexandrian’ glass confirmed by hafnium isotopes. Sci Rep 10, 11322 (2020). https://doi.org/10.1038/s41598-020-68089-w
Journal of Archaeological Science: Reports (2021)