1 00:00:01,030 --> 00:00:03,180 [music] 2 00:00:03,200 --> 00:00:05,210 [robotic voice] 3, 2, 1... 3 00:00:05,230 --> 00:00:08,210 [Dana Hurley] I think that it's in human nature to explore. 4 00:00:11,260 --> 00:00:16,350 [Rich Vondrak] Understanding the moon better, will help us to understand our neighbors in the solar system. 5 00:00:17,500 --> 00:00:20,550 [Ashwin Vasavada] We're exploring the solar system here and not just the moon. 6 00:00:20,560 --> 00:00:23,610 [Cathy Peddie] The moon is the natural next step 7 00:00:23,630 --> 00:00:26,710 in our exploration of our own universe. 8 00:00:26,730 --> 00:00:29,780 [drum beats] 9 00:00:34,860 --> 00:00:36,850 [Craig Tooley] The Lunar Reconnaissance Orbiter 10 00:00:36,860 --> 00:00:40,029 is as its namesake says, a reconnaissance mission to the moon. 11 00:00:40,030 --> 00:00:44,059 Our job is to take a suite of very powerful scientific instruments and make 12 00:00:44,060 --> 00:00:48,059 an atlas of the entire moon, in some place in very great detail. 13 00:00:48,060 --> 00:00:52,080 Topography, mountain heights, minerology, temperatures, 14 00:00:52,100 --> 00:00:56,080 abundances of resources, including potentially the intriguing possibility that there's water 15 00:00:56,100 --> 00:01:00,110 at the moon. We put all this together into a dataset by flying low over the moon for a year, 16 00:01:00,130 --> 00:01:04,150 and this is the data that the people designing the systems, picking the sites, 17 00:01:04,160 --> 00:01:06,310 need to take us back to the moon. 18 00:01:06,330 --> 00:01:10,450 [Rich Vondrak] Well, we learned much about the moon from the Apollo Program, 19 00:01:10,460 --> 00:01:14,610 but now we want to return to the moon for a more intensive study. 20 00:01:14,630 --> 00:01:18,710 We want to be able to go back to the moon so that we can live there for longer 21 00:01:18,730 --> 00:01:21,810 periods and work on the moon, so we need a mission 22 00:01:21,830 --> 00:01:24,810 that can help us find the best places to go 23 00:01:24,830 --> 00:01:28,680 and determine how to go back there safely. 24 00:01:30,130 --> 00:01:31,250 [muffled] "it's a nice place to land" 25 00:01:31,260 --> 00:01:34,310 [Cathy Peddie] We know that, you know, Neil Armstrong and some of the others had 26 00:01:34,330 --> 00:01:37,510 a difficult time finding a safe landing site. 27 00:01:37,530 --> 00:01:41,580 The didn't see it until they got there. But now with our instruments, we'll be able to 28 00:01:41,600 --> 00:01:43,780 tell people ahead of time, "look, don't go there." 29 00:01:43,800 --> 00:01:47,780 [Rich Vondrak] LRO will have a laser system that will give 30 00:01:47,800 --> 00:01:51,980 us a high resolution topographic map of the moon. 31 00:01:52,000 --> 00:01:56,180 It als has high resolution cameras that will identify 32 00:01:56,200 --> 00:02:00,380 objects that are only a foot or two in size so that we know where there are 33 00:02:00,400 --> 00:02:04,380 no large boulders that could be a risk to astronauts. 34 00:02:04,400 --> 00:02:08,510 [Craig Tooley] So our job is to literally complete the job of mapping the moon, do it at high resolutions, and then 35 00:02:08,530 --> 00:02:11,610 enable the designers of the human systems 36 00:02:11,630 --> 00:02:14,680 the atlas they need to pick the safe places to go 37 00:02:14,700 --> 00:02:17,710 the beneficial places to go and where it's most fruitful to go. 38 00:02:20,930 --> 00:02:25,980 [Cathy Peddie] In addition to the safe landing sites, LRO is looking for potential resources, and now 39 00:02:26,000 --> 00:02:30,080 why are we doing that? Because it's really hard to carry all your supplies 40 00:02:30,100 --> 00:02:34,180 with you, I mean, you can do it, but really spend a lot of 41 00:02:34,200 --> 00:02:38,310 not only fuel, but cargo space. So it'd be really nice to go to a place that 42 00:02:38,330 --> 00:02:42,480 already has the resources, whether it's water ice to have water, 43 00:02:42,500 --> 00:02:46,580 or potential minerals that we could use as raw materials, 44 00:02:46,600 --> 00:02:48,780 to make into things that we would need. 45 00:02:48,800 --> 00:02:52,780 [Rich Vondrak] We think the most interesting parts of the moon may be polar 46 00:02:52,800 --> 00:02:56,780 regions of the moon because there could be resources there. 47 00:02:56,800 --> 00:03:00,950 And so we're going to study intesively the polar regions 48 00:03:00,960 --> 00:03:01,950 with LRO. 49 00:03:01,960 --> 00:03:05,080 [Craig Tooley] From the Apollo era we chose to go for good reasons, because 50 00:03:05,100 --> 00:03:08,180 it was literally the easiest, to go to the equatorial regions, and 51 00:03:08,200 --> 00:03:11,250 stay a very short time, and it was a very ambitious program but 52 00:03:11,260 --> 00:03:14,480 when you look at where would like to go and 53 00:03:14,500 --> 00:03:17,680 stay for awhile on the moon, you begin to realize that 54 00:03:17,700 --> 00:03:20,810 probably the poles are the most interesting place. 55 00:03:20,830 --> 00:03:23,910 [John Keller] Access to solar power, continuously, that may be 56 00:03:23,930 --> 00:03:27,950 the first and most important reason over, you know, the near term 57 00:03:27,960 --> 00:03:31,180 And then the possibility of resources being there. 58 00:03:31,200 --> 00:03:34,310 Those may take much longer time 59 00:03:34,330 --> 00:03:37,410 before we're able to really exploit those, but the solar power 60 00:03:37,430 --> 00:03:39,680 is something that we can exploit right away. 61 00:03:40,730 --> 00:03:44,710 [Rich Vondrak] The second big resource on the moon, may be water ice. 62 00:03:44,730 --> 00:03:48,750 There's evidence from early missions, that in dark places at the 63 00:03:48,760 --> 00:03:52,750 poles, there may be water at the surface or below. 64 00:03:52,760 --> 00:03:55,950 the surface in the form of ice crystals. 65 00:03:55,960 --> 00:03:59,110 If it is abundant, astronauts could use 66 00:03:59,130 --> 00:04:02,180 this for both human consumption 67 00:04:02,200 --> 00:04:05,210 and as a source of rocket fuel. 68 00:04:08,430 --> 00:04:12,580 LRO will measure for the first time, this very energetic component 69 00:04:12,600 --> 00:04:16,680 of the space radiation environment, in order to see whether it 70 00:04:16,700 --> 00:04:18,880 is going to be a problems or not. 71 00:04:18,900 --> 00:04:23,910 [Craig Tooley] It was one thing to go for a handful of days in Apollo, and go when 72 00:04:23,930 --> 00:04:27,080 we knew that the Sun was quiet, or you hope the Sun stayed quiet, 73 00:04:27,100 --> 00:04:31,210 and you took the risk, you calculated the risk of cancer and 74 00:04:31,230 --> 00:04:35,310 such and you made a short mission. If you're going to live there longer, you need to 75 00:04:35,330 --> 00:04:39,410 understand it enough to go, "Here's what I need to do to protect myself." 76 00:04:39,430 --> 00:04:43,480 [Cathy Peddie] One of the things that we're looking for in the LRO mission is 77 00:04:43,500 --> 00:04:47,550 how the high radiation environment effects 78 00:04:47,560 --> 00:04:51,610 our ability to explore. So if we bring cameras or 79 00:04:51,630 --> 00:04:55,780 communication devices, you know, how will they be impacted by 80 00:04:55,800 --> 00:05:00,810 the cosmic radiation? We need to protect our equipment as well as ourselves. 81 00:05:05,830 --> 00:05:07,910 [music ramps up] 82 00:05:07,930 --> 00:05:12,059 [Craig Tooley] When we look back at what we did in LRO and 83 00:05:12,060 --> 00:05:15,059 we look at what followed, I think we'll see a profound impact. We'll see 84 00:05:15,060 --> 00:05:18,280 this as really being the small first step 85 00:05:18,300 --> 00:05:22,510 where we have human beings permanently off this planet. 86 00:05:22,530 --> 00:05:25,710 Beginning to the move out of the solar system, starting with the moon, as that pans out 87 00:05:25,730 --> 00:05:28,850 I think we'll be a small part of a profound 88 00:05:28,860 --> 00:05:32,910 development that when history looks back they'll say, "This time we went back to the moon. This time 89 00:05:32,930 --> 00:05:37,059 we stayed, and then we moved on from there."