1 00:00:19,990 --> 00:00:18,390 [Music] 2 00:00:22,070 --> 00:00:20,000 the first thing we do is we put it in 3 00:00:23,990 --> 00:00:22,080 this catapult looking device that you 4 00:00:25,670 --> 00:00:24,000 see here we call it the rocket launcher 5 00:00:27,349 --> 00:00:25,680 the end caps are taken off of the drive 6 00:00:29,109 --> 00:00:27,359 tube and then 7 00:00:31,109 --> 00:00:29,119 threaded metal rods with plates on the 8 00:00:32,790 --> 00:00:31,119 end were actually inserted into either 9 00:00:34,549 --> 00:00:32,800 end then the sample is picked up from 10 00:00:37,030 --> 00:00:34,559 the rocket launcher and it's put into 11 00:00:39,830 --> 00:00:37,040 this device over here with the wheel on 12 00:00:42,389 --> 00:00:39,840 it as that wheel gets turned very slowly 13 00:00:46,389 --> 00:00:42,399 the threads engage and the rod starts to 14 00:00:50,869 --> 00:00:48,069 that core 15 00:00:53,990 --> 00:00:50,879 was collected by gene cernan 16 00:00:55,990 --> 00:00:54,000 as i was working on the edge of a of a 17 00:00:57,670 --> 00:00:56,000 crater nearby 18 00:00:59,270 --> 00:00:57,680 one of the most important tools that we 19 00:01:02,630 --> 00:00:59,280 had was this 20 00:01:04,869 --> 00:01:02,640 core tube a double drive tube and you 21 00:01:06,870 --> 00:01:04,879 could drive these into the surface now 22 00:01:08,390 --> 00:01:06,880 still very difficult 23 00:01:12,149 --> 00:01:08,400 it was the best we had and we got a 24 00:01:14,870 --> 00:01:12,159 quite a number of very good cores that 25 00:01:17,190 --> 00:01:14,880 are giving us new information not only 26 00:01:19,670 --> 00:01:17,200 about the nature of this debris layer 27 00:01:23,030 --> 00:01:19,680 but also within those cores is a history 28 00:01:26,390 --> 00:01:24,950 it was anticipated early on in the 29 00:01:27,429 --> 00:01:26,400 apollo program 30 00:01:30,550 --> 00:01:27,439 that 31 00:01:33,030 --> 00:01:30,560 analytical technology would mature would 32 00:01:35,030 --> 00:01:33,040 become much more sophisticated with time 33 00:01:37,350 --> 00:01:35,040 that we could gain new information from 34 00:01:39,590 --> 00:01:37,360 the same old samples it makes it 35 00:01:41,749 --> 00:01:39,600 very very exciting for everybody in fact 36 00:01:43,510 --> 00:01:41,759 apollo never ended for lunar scientists 37 00:01:45,190 --> 00:01:43,520 our analytical techniques have gotten to 38 00:01:47,350 --> 00:01:45,200 the point where we can actually detect 39 00:01:49,270 --> 00:01:47,360 the water that is in some of these 40 00:01:51,030 --> 00:01:49,280 ancient ludar rocks we've actually been 41 00:01:52,710 --> 00:01:51,040 able to constrain 42 00:01:54,469 --> 00:01:52,720 that there is a common history and a 43 00:01:56,149 --> 00:01:54,479 common source between the earthman 44 00:01:58,230 --> 00:01:56,159 system which is what we have learned 45 00:02:00,550 --> 00:01:58,240 previously by other studies of the 46 00:02:03,350 --> 00:02:00,560 apollo lunar samples that we have 47 00:02:06,069 --> 00:02:03,360 x-ray computed tomography or xct now 48 00:02:07,910 --> 00:02:06,079 this is a way for us to actually look at 49 00:02:13,510 --> 00:02:07,920 the three-dimensional structure of a 50 00:02:17,510 --> 00:02:15,430 there's a whole industry of engineers 51 00:02:19,670 --> 00:02:17,520 who are studying how to extract 52 00:02:21,030 --> 00:02:19,680 resources from the moon and so one of 53 00:02:22,630 --> 00:02:21,040 the things that we want to do during 54 00:02:24,790 --> 00:02:22,640 artemis is actually test out some of 55 00:02:26,470 --> 00:02:24,800 these new technologies and see how 56 00:02:28,470 --> 00:02:26,480 effective they are at extracting the 57 00:02:30,470 --> 00:02:28,480 water and these other materials thinking 58 00:02:33,110 --> 00:02:30,480 forward to mars we've only ever sent 59 00:02:35,030 --> 00:02:33,120 robotic missions to mars and so when we 60 00:02:36,790 --> 00:02:35,040 send people to mars these are things 61 00:02:39,670 --> 00:02:36,800 we're going to have to consider so this 62 00:02:41,750 --> 00:02:39,680 core has a multitude of the information 63 00:02:43,750 --> 00:02:41,760 to give us and we're as you can tell i 64 00:02:45,589 --> 00:02:43,760 think all of us are very excited about 65 00:02:47,750 --> 00:02:45,599 getting a chance to work on it there's a 66 00:02:49,910 --> 00:02:47,760 lot we don't know about the rest of the 67 00:02:51,750 --> 00:02:49,920 moon and there's a lot we don't know 68 00:02:54,390 --> 00:02:51,760 about in between these various sites 69 00:02:56,550 --> 00:02:54,400 that apollo landed at and so gathering 70 00:02:58,070 --> 00:02:56,560 new information uh particularly from the 71 00:03:00,390 --> 00:02:58,080 south pole but there are many other 72 00:03:03,509 --> 00:03:00,400 areas on the far side that will start to 73 00:03:06,070 --> 00:03:03,519 define much more uh give us much more 74 00:03:07,589 --> 00:03:06,080 information about lunar science you have 75 00:03:09,350 --> 00:03:07,599 to remember that everything we're 76 00:03:11,589 --> 00:03:09,360 learning about the moon 77 00:03:13,670 --> 00:03:11,599 relates to the very early history of the 78 00:03:17,190 --> 00:03:13,680 solar system and particularly to the 79 00:03:31,430 --> 00:03:17,200 very early history of the earth 80 00:03:34,050 --> 00:03:32,390 subscribe