Oxygenated
derivatives of polycyclic aromatic hydrocarbons (PAHs), or oxyPAHs,
recently captured the interest of the scientific community for their
photochemical reactivity in a water–ice matrix mimicking the
interstellar medium. Furthermore, oxyPAHs are interesting molecules
for the study of the origin of life for their prebiotic potential.
However, their stability and transformation pathways under astrophysically
relevant conditions have remained largely unexplored. Herein we report
the photochemical behavior of 1-naphthol (1-HN) and 1,6- and 1,8-dihydroxynaphthalene
(DHN) either as pure powdered solids or adsorbed on forsterite or
anatase surface. All the compounds showed an extensive decrease of
main vibrational bands, accompanied in the case of DHNs by the formation
of new molecular species. Irradiation of 1,8-DHN at 80 K resulted
in the IR-detectable generation of CO2 (2340 cm–1), a process reported by other authors following irradiation of PAHs
in water–ice analogues at 14 K. These results, when compared
to model autoxidation experiments, indicated a high susceptibility
of hydroxylated naphthalene derivatives to UV radiation leading to
free radical and carbonyl-containing extended quinone intermediates
(preliminary DFT calculations) with partial degradation and decarboxylation.
On the basis of these results, oxyPAH formation and photoprocessing
on minerals is proposed as a plausible pathway of PAHs transformation
under astrochemical conditions of prebiotic relevance.