Burchell Mark J, Bowden Stephen A, Cole Michael, Price Mark C, Parnell John
1 School for Physical Sciences, University of Kent , Canterbury, UK .
Astrobiology. 2014 Jun;14(6):473-85. doi: 10.1089/ast.2013.1007. Epub 2014 Jun 5.
The survival of organic molecules in shock impact events has been investigated in the laboratory. A frozen mixture of anthracene and stearic acid, solvated in dimethylsulfoxide (DMSO), was fired in a two-stage light gas gun at speeds of ~2 and ~4 km s(-1) at targets that included water ice, water, and sand. This involved shock pressures in the range of 2-12 GPa. It was found that the projectile materials were present in elevated quantities in the targets after impact and in some cases in the crater ejecta as well. For DMSO impacting water at 1.9 km s(-1) and 45° incidence, we quantify the surviving fraction after impact as 0.44±0.05. This demonstrates successful transfer of organic compounds from projectile to target in high-speed impacts. The range of impact speeds used covers that involved in impacts of terrestrial meteorites on the Moon, as well as impacts in the outer Solar System on icy bodies such as Pluto. The results provide laboratory evidence that suggests that exogenous delivery of complex organic molecules from icy impactors is a viable source of such material on target bodies.
实验室已对冲击事件中有机分子的存活情况展开研究。将溶解于二甲基亚砜(DMSO)中的蒽和硬脂酸的冷冻混合物,以约2千米/秒和约4千米/秒的速度,用两级轻气炮射向包括水冰、水和沙子在内的靶标。这涉及2 - 12吉帕的冲击压力。研究发现,撞击后靶标中以及某些情况下弹坑喷出物中均存在数量增加的抛射物材料。对于DMSO以1.9千米/秒的速度、45°入射角撞击水的情况,我们将撞击后的存活分数量化为0.44±0.05。这表明在高速撞击中有机化合物成功地从抛射物转移到了靶标。所使用的撞击速度范围涵盖了地球陨石撞击月球以及太阳系外层冰质天体(如冥王星)上的撞击情况。这些结果提供了实验室证据,表明来自冰质撞击体的复杂有机分子的外源输送是靶标天体上此类物质的一个可行来源。