1 00:00:05,269 --> 00:00:02,710 hypervelocity impacts are often 2 00:00:08,310 --> 00:00:05,279 considered as catastrophic events 3 00:00:10,390 --> 00:00:08,320 that tend to destroy life however 4 00:00:12,629 --> 00:00:10,400 previous studies have synthesized 5 00:00:13,589 --> 00:00:12,639 essential organic compounds using source 6 00:00:16,470 --> 00:00:13,599 of carbon and 7 00:00:20,550 --> 00:00:16,480 nitrogen in primitive atmospheres via 8 00:00:22,230 --> 00:00:20,560 simulated hypervelocity impact events 9 00:00:24,230 --> 00:00:22,240 whether the carbon and the nitrogen 10 00:00:27,029 --> 00:00:24,240 stored in the primitive crust 11 00:00:28,390 --> 00:00:27,039 could also synthesize organics via hyper 12 00:00:31,910 --> 00:00:28,400 velocity impacts 13 00:00:35,910 --> 00:00:34,470 in these studies we simulate the impact 14 00:00:37,990 --> 00:00:35,920 event via high power 15 00:00:39,830 --> 00:00:38,000 pose later ablation and the physical 16 00:00:43,670 --> 00:00:39,840 bombardment of carbon 60 17 00:00:44,630 --> 00:00:43,680 onto a target we observe molecular 18 00:00:47,670 --> 00:00:44,640 recombination 19 00:00:50,470 --> 00:00:47,680 of cn and cmo in the plasma plume 20 00:00:52,630 --> 00:00:50,480 where only geological matrices are used 21 00:00:55,350 --> 00:00:52,640 as the starting materials 22 00:00:57,990 --> 00:00:55,360 this result indicates that carbon and 23 00:01:01,189 --> 00:00:58,000 nitrogen stored in the early earth crust 24 00:01:05,350 --> 00:01:01,199 could have contributed significantly to 25 00:01:07,429 --> 00:01:05,360 prebiotic inventory in early earth 26 00:01:09,429 --> 00:01:07,439 further interaction of the prebiotic 27 00:01:10,070 --> 00:01:09,439 organics with the resource around the 28 00:01:11,830 --> 00:01:10,080 craters 29 00:01:13,230 --> 00:01:11,840 could have synthesized essential 30 00:01:16,070 --> 00:01:13,240 monomers promote 31 00:01:18,149 --> 00:01:16,080 polymerization and provide habitats that