1 00:00:00,010 --> 00:00:04,130 Since the beginning of the 2 00:00:04,150 --> 00:00:08,310 space age NASA has explored our solar system, bringing back 3 00:00:08,330 --> 00:00:12,480 unprecedented scientific knowledge, but only a handful of missions 4 00:00:12,500 --> 00:00:16,680 over the past 50 years have actually collected and returned samples 5 00:00:16,700 --> 00:00:20,870 from these far off places. Astronauts 6 00:00:20,890 --> 00:00:25,020 on the Apollo program traveled to our Moon, bringing back over 800 lbs 7 00:00:25,040 --> 00:00:29,530 of moon rock. Stardust was an unmanned mission that collected samples 8 00:00:29,550 --> 00:00:33,700 from the coma of comet Wild 2 before returning them to Earth for in-depth 9 00:00:33,720 --> 00:00:37,860 scientific study. OSIRIS-Rex is the most recently funded 10 00:00:37,880 --> 00:00:42,010 sample return mission that will launch in 2016 and return surface 11 00:00:42,030 --> 00:00:46,190 samples from an asteroid in 2023. 12 00:00:46,210 --> 00:00:50,320 The Comet Nucleus Sample Return mission will collect subsurface samples 13 00:00:50,340 --> 00:00:54,430 from a comet and return them to Earth. Comets and Asteroids are 14 00:00:54,450 --> 00:00:58,530 leftover remnants from the early solar system and by studying samples from these 15 00:00:58,550 --> 00:01:02,620 objects, we can learn more about the formation of our solar system and 16 00:01:02,640 --> 00:01:06,680 may find clues to the origin of life on Earth. Collecting a sample 17 00:01:06,700 --> 00:01:10,710 from a comet is a challenging feat for many reasons, including how far 18 00:01:10,730 --> 00:01:14,730 away they are from Earth and how little gravity they provide. In our 19 00:01:14,750 --> 00:01:18,910 concept, harpoons are used to collect and retrieve samples from interesting locations 20 00:01:18,930 --> 00:01:23,090 on these exotic objects. Traditionally, 21 00:01:23,110 --> 00:01:27,270 when collecting samples on Earth, we use scoops, shovels, or coring drills, 22 00:01:27,290 --> 00:01:31,450 but on comets and asteroids there is so little gravity that you would 23 00:01:31,470 --> 00:01:35,640 push yourself off the surface if you used one of these methods. Harpoons allow 24 00:01:35,660 --> 00:01:39,860 you to grapple to the surface while taking a sample, allowing rapid sample collection 25 00:01:39,880 --> 00:01:43,990 and retrieval. First, we choose a specific interesting 26 00:01:44,010 --> 00:01:48,200 area to take a sample from and then fire a sample collecting harpoon into that 27 00:01:48,220 --> 00:01:52,330 spot. As the harpoon penetrates into the comet, it fills its inner sample 28 00:01:52,350 --> 00:01:56,440 cartridge with subsurface material as it goes deeper. When it reaches its 29 00:01:56,460 --> 00:02:00,550 maximum depth the sample cartridge closure mechanism shuts, trapping all 30 00:02:00,570 --> 00:02:04,640 the material inside it. The sample cartridge is then with drawn from the outer harpoon 31 00:02:04,660 --> 00:02:08,700 sheath and pulled back into the space craft. The sample is 32 00:02:08,720 --> 00:02:12,750 then brought back to a terrestrial laboratory where scientists examine the collected 33 00:02:12,770 --> 00:02:16,790 samples in a pristine environment. 34 00:02:16,810 --> 00:02:20,970 Before we journey here, we need to work here 35 00:02:20,990 --> 00:02:25,150 in the lab, studying comet and asteroid analogs. 36 00:02:25,170 --> 00:02:29,320 In order to determine how much energy is required to penetrate different depths 37 00:02:29,340 --> 00:02:33,500 in various density material, we’ve designed and built a harpoon 38 00:02:33,520 --> 00:02:37,670 test laboratory. Although the actual mission will use a cannon, 39 00:02:37,690 --> 00:02:41,860 for safety reasons, we’ve employed a ballista to fire the harpoons. 40 00:02:41,880 --> 00:02:46,040 By correlating the imparted energy versus the penetration depth, we will 41 00:02:46,060 --> 00:02:50,190 know how to size the explosive charge for the actual mission. 42 00:02:50,210 --> 00:02:54,340 The harpoon lab also allows us to study how the tip geometry, cross 43 00:02:54,360 --> 00:02:58,500 section and mass of the harpoon affect its penetration. 44 00:02:58,520 --> 00:03:02,610 This has allowed us to optimize the harpoon sheath for a range of 45 00:03:02,630 --> 00:03:06,700 possible comet densities. Although sample return missions can be quite 46 00:03:06,720 --> 00:03:10,770 costly and complex, they offer important advantages over missions 47 00:03:10,790 --> 00:03:14,820 that study their subjects from a distance. Sample return missions allow 48 00:03:14,840 --> 00:03:18,860 terrestrial laboratories to study in far greater detail, with a variety