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Glaze crystallization is a key surface decoration technique in black-glazed ceramics, reflecting the advanced craftsmanship of ancient ceramic production. In this study, a black-glazed ceramic sherd from the Song Dynasty (960–1279 C.E.), excavated in Nanjing, China, was systematically analyzed using optical microscopy, macro-X-ray fluorescence (Macro-XRF) imaging, and field-emission scanning electron microscopy coupled with energy-dispersive X-ray spectroscopy (FESEM-EDS) and Raman spectroscopy. The results reveal well-shaped stellate crystals within the cover glaze, which are comprised of oval crystals, brown prismatic crystals, fibrous crystals, and reddish-brown spherical crystals. These crystals are identified as α-cristobalite, rich-Ca and low-Mg hedenbergite [Ca(Mg 0.09 Fe 0.89 Mn 0.02 )Si 2 O 6 ] and rich-Ca spinel ferrite [(Ca 0 . 6 Mg 0 . 4 )Fe 2 O 4 ], respectively. A potential growth mechanism for these structures is proposed. The α-cristobalite nuclei serve as a structurally compatible, low-energy substrate for hedenbergite nucleation. Local enrichment of Ca and Fe, combined with liberated SiO 4 units, supplies the components for hedenbergite growth, which proceeds radially as prismatic and fibrous aggregates around the cristobalite core. As crystallization advances, localized Fe enrichment and micro-oxidizing conditions at the hedenbergite–glass interface promote the precipitation of Ca-rich spinel ferrite as submicron spheres intergrown with hedenbergite. Prolonged cooling further enhances this intergrowth, ultimately producing the well-ordered, multilevel stellate structures observed.
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Long et al. (2025) studied this question.
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