Shock and post-shock temperatures in an ice–quartz mixture: implications for melting during planetary impact events

a r t i c l e i n f o Keywords: shock temperature impact cratering melting water ice equation of state Melting of H 2 O ice during planetary impact events is a widespread phenomenon. On planetary surfaces, ice is often mixed with other materials; yet, at present, the partitioning of energy between the components of a shocked mixture is still an open question in the shock physics community. Knowledge of how much energy is partitioned into the ice component is necessary to predict and interpret a wide range of processes, including shock-induced melting and chemistry. In this work, we construct a conceptual framework for the thermodynamic pathways of the components in a shocked hydrodynamic mixture by defining three broad regimes based on the characteristic length scale of the mixture compared to the thickness of the shock front: (1) small length scale mixtures where pressure and temperature equilibrate immediately behind the shock front; (2) intermediate length scales where pressure but not thermal equilibration is achieved behind the shock front; and (3) long length scales where pressure equilibration requires multiple shock wave reflections. We conduct shock wave experiments, reaching pressures from 8 to 23 GPa, in an H 2 O ice–SiO 2 quartz mixture in the intermediate length scale regime. In each experiment, all the parameters required to address the question of energy partitioning were determined: the shock velocity in the mixture, the shock front thickness, and the shock and post-shock temperatures of the H 2 O component. The measured pressure is in agreement with the bulk compressibility of the mixture. The shock and post-shock temperatures of the H 2 O component indicate that the ice was shocked close to the principal Hugoniot. Therefore, in the intermediate length scale regime, the partitioning of shock energy is defined initially by the Hugoniots of the components at the equilibrated pressure. We discuss energy partitioning in mixtures over the wide range of length and time scales encountered during planetary impact events and identify the current challenges in calculating the volume of melted ice. In some cases, the criteria for shock-induced melting of ice in a mixture are the same as for pure ice. Shock-induced melting of H 2 O ice during impact cratering events is an important planetary phenomenon. As relatively low shock pressures are required to melt ice (Stewart et al., 2008), large volumes of melt may be produced during impact events. …