Direct evidence for metallic mercury causing photo-induced darkening of red cinnabar tempera paints

December 16, 2021

Title

Direct evidence for metallic mercury causing photo-induced darkening of red cinnabar tempera paints

Author

Kerstin Elert, Manuel Perez Mendoza & Carolina Cardell

Year

2021

Journal

Communications Chemistry

Abstract

Photo-induced darkening of red cinnabar (HgS) has attracted the interest of many researchers as it drastically impacts the visual perception of artworks. Darkening has commonly been related to metallic mercury (Hg0) formation in the presence of chlorides. Based on the study of UV-aged cinnabar pigment and tempera paint we propose an alternative pathway for the blackening reaction of cinnabar, considering its semiconductor properties and pigment-binder interactions. We demonstrate that darkening is caused by the oxidation of cinnabar to mercury sulfates and subsequent reduction to Hg0 via photo-induced electron transfer without the involvement of chlorides, and provide direct evidence for the presence of Hg0 on UV-aged tempera paint. Photooxidation also affects the organic binder, causing a competing depletion of photo-generated holes and consequently limiting but not impeding mercury sulfate formation and subsequent reduction to Hg0. In addition, organics provide active sites for Hg0 sorption, which is ultimately responsible for the darkening of cinnabar-based paint.

Instrument

FT/IR-6200

Keywords

HgS, pigment, photooxidation