“…The fact that glycine and other prebiotically relevant species were detected in non-negligible amounts in some comets, such as Halley, Hyakutake, Tempel-1, Giacobini–Zinner, Hartley 2 and Hale–Bopp, 81P/Wild 2 [ 105 , 106 , 107 , 108 , 109 , 110 , 111 ], indirectly suggested the possibility to observe and reproduce a relatively complex chemistry when high-energy impacts take place. In fact, many interesting experimental and computational results emerge from disparate investigations of the catalytic effects produced by violent mechanical stresses acting on simple inorganic systems [ 7 , 16 , 18 , 36 , 39 , 42 , 104 , 112 , 113 , 114 , 115 , 116 , 117 , 118 , 119 , 120 , 120 ]. As an example, Martins et al [ 16 ] created several icy bullets composed of simple compounds ubiquitous in cometary ices such as ammonium hydroxide (NH 4 OH), carbon dioxide (CO 2 ), and methanol (CH 3 OH), which were impacted on a series of rocky surfaces—mimicking planetary surfaces—by using a light gas gun available at an important facility located at the University of Kent [ 121 ].…”