It is widely known
that the vivid hue of red cinnabar can darken
or turn black. Many authors have studied this transformation, but
only a few in the context of the archeological site of Pompeii. In
this work, the co-occurrence of different degradation patterns associated
with Pompeian cinnabar-containing fresco paintings (alone or in combination
with red/yellow ocher pigments) exposed to different types of environments
(pre- and post-79 AD atmosphere) is reported. Results obtained from
the in situ and laboratory multianalytical methodology revealed the
existence of diverse transformation products in the Pompeian cinnabar,
consistent with the impact of the environment. The effect of hydrogen
sulfide and sulfur dioxide emitted during the 79 AD eruption on the
cinnabar transformation was also evaluated by comparing the experimental
evidence found on paintings exposed and not exposed to the post-79
AD atmosphere. Our results highlight that not all the darkened areas
on the Pompeian cinnabar paintings are related to the transformation
of the pigment itself, as clear evidence of darkening associated with
the presence of manganese and iron oxide formation (rock varnish)
on fragments buried before the 79 AD eruption has also been found.