Although
hexagonal ice (ice Ih) is the most common and
highly studied crystalline form of ice, its nucleation from clathrate
hydrates is poorly understood. Here, we report the formation of ice
Ih through the dissociation of formaldehyde hydrate, prepared
under ultrahigh vacuum (UHV) in the temperature window of 130–135
K. This unique route for crystallization is highly facile, and it
occurs below the usual crystallization temperature of ice Ih of 155 K in UHV; the associated activation energy is also lower.
Time-dependent reflection absorption infrared spectroscopy was used
to detect the formaldehyde hydrate and to determine the crystallization
kinetics of ice Ih. The dissociation of formaldehyde hydrate
is found to be a diffusion-controlled process, which reduces the activation
barrier of crystallization. This study provides evidence that formaldehyde
hydrate can exist in extremely low (P, T) conditions without forming
the geminal diol or its polymer in the presence of water. This new
and facile route of crystallization in the context of interstellar
environments may have implications for cometary and prebiotic science.