MERCURY AND SMALL-SCALE GOLD MINING AT ANCIENT SARDIS, TURKEY
Modern uses for cinnabar and mercury are numerous; however, in the Byzantine world, cinnabar was used as a pigment (vermillion) and to produce mercury that was used for gilding or amalgamation of fine-grained alluvial gold. At Sardis, alluvial gold mining dates to ~700 aC and continues today, and, as recently as 1984, sluice concentrates at Sardis were amalgamated. Geology and availability of mercury, a mercury retort, regional Roman use of mercury for amalgamation, and the very fine-grained (~0.03 mm) alluvial gold at Sardis all indicate that amalgamation must be reconsidered as the ages-old mining technology that supplied alluvial gold to ancient Sardis’ refineries.
Inductively Coupled Plasma (ICP) geochemical studies in Colombia and Perú indicate that gold from alluvial sources may contain ~5000 ppm Hg sourced from cinnabar/mercury outcrops, underground coal fires, alluvial gold mining, or volcanic eruptions. However, modern amalgam (Hg+Au) in the gold pan contains >300,000 ppm Hg—this amalgam must be burned (refogado), as would have been done in the past, to volatilize the mercury, leaving end-product gold with only trace amounts of mercury. Prehispanic gold artifacts from museums in Bogotá and Lima typically contain <20 ppm Hg—consistent with a reduction in the mercury content during amalgam burning. Therefore, we are similarly using ICP to determine the metal content, particularly Pt and Hg, of end-product Byzantine gold to interpret the mining technology used at ancient Sardis.