Natural Science in Archaeology
Natural Science in Archaeology
Natural Science in Archaeology
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194 8 Ceramic Raw Materials<br />
Ch<strong>in</strong>ese prov<strong>in</strong>ces (Guo 1987). In north Ch<strong>in</strong>a, a different, high-alum<strong>in</strong>a, raw material<br />
was used <strong>in</strong> the development of porcela<strong>in</strong>. The basic constituents were kaol<strong>in</strong><br />
with admixed quartz, mica, and carbonates. Both raw materials transformed <strong>in</strong>to the<br />
dense porcela<strong>in</strong> at between 1200 and 1300°C.<br />
Rich deposits of what is termed porcela<strong>in</strong> stone were discovered <strong>in</strong> the southern<br />
prov<strong>in</strong>ces of Ch<strong>in</strong>a <strong>in</strong> late Shang times. Ch<strong>in</strong>ese porcela<strong>in</strong> stone is a rock composed<br />
ma<strong>in</strong>ly of quartz and sericite (f<strong>in</strong>e-gra<strong>in</strong>ed hydromica). Porcela<strong>in</strong> stone sometimes<br />
also conta<strong>in</strong>ed small amounts of feldspar and/or kaol<strong>in</strong>ite. Throughout the long<br />
development of Ch<strong>in</strong>ese porcela<strong>in</strong>, the potters experimented with a variety of raw<br />
materials to achieve special effects. Without any knowledge of the chemical elements,<br />
potters learned which manganese and iron oxides would color porcela<strong>in</strong><br />
glazes and that high phosphate raw materials encouraged bubbles <strong>in</strong> the glaze (see<br />
Scott and Kerr 1993).<br />
Protoporcela<strong>in</strong> was produced as early as the Shang Dynasty (seventeenth to eleventh<br />
centuries BCE) <strong>in</strong> Ch<strong>in</strong>a. The earliest protoporcela<strong>in</strong> has a lead-free glaze and<br />
a fairly vitrified body, suggest<strong>in</strong>g the use of high fir<strong>in</strong>g techniques. Protoporcela<strong>in</strong><br />
requires suitable raw material as well as a high fir<strong>in</strong>g temperature. A recent paper by<br />
Chen et al. (1999) explores the potential of chemical composition <strong>in</strong> characteriz<strong>in</strong>g<br />
protoporcela<strong>in</strong> sources. Their results suggest a centralized source of production of<br />
protoporcela<strong>in</strong> dur<strong>in</strong>g the Shang Dynasty, perhaps at Wucheng. No dramatic change<br />
occurred <strong>in</strong> mak<strong>in</strong>g proto-porcela<strong>in</strong> dur<strong>in</strong>g the follow<strong>in</strong>g Zhou Dynasty (eleventh<br />
century to 221 BCE) (Medley 1976). Europeans did not develop a true form of porcela<strong>in</strong><br />
until early <strong>in</strong> the eighteenth century (K<strong>in</strong>gery 1986b).<br />
8.7 Glass<br />
Glasses are solid, noncrystall<strong>in</strong>e silicate bodies. The rapid solidification of a silicate<br />
melt forms glass. To understand the raw material requirements for glass, it is<br />
necessary to review the chemicals needed to make glass. Consider<strong>in</strong>g only ancient<br />
glass, the most important constituent is silica (SiO 2 ). Pure silica will make a glass,<br />
but only at exceed<strong>in</strong>gly high temperatures. One of the most efficient and easily<br />
obta<strong>in</strong>able additives to reduce the temperature of fusion is Na 2 O. A second compound<br />
that serves well as a flux is lead oxide (PbO). Potassium oxide (K 2 O) and<br />
calcium oxide (CaO) also serve to reduce temperatures of fusion. Ancient glass<br />
found on archaeological sites may appear varicolored, because the <strong>in</strong>clusion of<br />
manganese imparts a lavender hue after long exposure to the sun. Over very long<br />
periods, glasses may crystallize, because they are unstable compared with an<br />
assemblage of crystall<strong>in</strong>e m<strong>in</strong>erals of the same total composition. This process is<br />
called devitrification. A good <strong>in</strong>troduction to glass and other vitreous materials,<br />
especially colorants, is given by Biek and Bayley (1979). The compositions of<br />
ancient Egyptian, Roman, European, and Syrian glass are presented and discussed<br />
by Freestone (1991). Analysis of w<strong>in</strong>dow glass found at Pompeii <strong>in</strong>dicates it was<br />
composed of 69% silica, 17% soda, 7% lime, 3% alum<strong>in</strong>a, and 1% iron oxide with