Amorphous Mixtures of Ice and C60 Fullerene
Carbon and ice make up a substantial proportion of our Universe. Recent space exploration has shown that these two chemical species often coexist including on comets, asteroids and in the interstellar medium. Here we prepare mixtures of C<sub>60</sub> fullerene and H<sub>2</sub>O by vapor co-deposition at 90 K with molar C<sub>60</sub>:H<sub>2</sub>O ratios ranging from 1:1254 to 1:5. The C<sub>60</sub> percolation threshold is found between the 1:132 and 1:48 samples, corresponding to a transition from matrix-isolated C<sub>60</sub> molecules to percolating C<sub>60</sub> domains that confine the H<sub>2</sub>O. Below this threshold, the crystallization and thermal desorption properties of H<sub>2</sub>O are not significantly affected by the C<sub>60</sub>, whereas the crystallization temperature of H<sub>2</sub>O is shifted towards higher temperatures for the C<sub>60</sub>-rich samples. These C<sub>60</sub>-rich samples also display exotherms corresponding to the crystallization of C<sub>60</sub> as the two components undergo phase separation. More than 60 volume percent C<sub>60</sub> is required to significantly affect the desorption properties of H<sub>2</sub>O. A thick blanket of C<sub>60</sub> on top of pure amorphous ice is found to display large cracks due to water desorption. These findings may help understand the recently observed unusual surface features and the H<sub>2</sub>O weather cycle on the 67P/Churyumov–Gerasimenko comet.