WEBVTT FILE 1 00:00:00.000 --> 00:00:03.990 No sound 2 00:00:04.010 --> 00:00:08.010 On Sunday night 3 00:00:08.030 --> 00:00:12.050 we have two cool events that are happening at the same time. We have a lunar 4 00:00:12.070 --> 00:00:16.240 eclipse, when the moon passes into the shadow of the Earth. So we'll go 5 00:00:16.260 --> 00:00:20.270 from being very bright to turning this beautiful red color. The effect of the sunrises 6 00:00:20.290 --> 00:00:24.290 and sunsets of the Earth being projected onto the lunar surface. We also have a supermoon 7 00:00:24.310 --> 00:00:28.310 the closest full moon of the year. So those two events are occuring at the same time. 8 00:00:28.330 --> 00:00:32.340 And that's a very rare event. Hasn't happened since 1982, won't happen 9 00:00:32.360 --> 00:00:36.530 again until 2033. So Sunday night's a really great opportunity to go out 10 00:00:36.550 --> 00:00:40.610 and see a beautiful moon change right before your eyes. It's going to be a 11 00:00:40.630 --> 00:00:44.660 beautiful show. 12 00:00:44.680 --> 00:00:48.690 No sound 13 00:00:48.710 --> 00:00:52.700 The moon will be fairly high in the sky when it goes into eclipse. 14 00:00:52.720 --> 00:00:56.730 You don't need to worry about too far away from trees, but you want to be able to have a pretty good 15 00:00:56.750 --> 00:01:00.760 view to the sky and just sit back and enjoy the show. 16 00:01:00.780 --> 00:01:04.790 No sound 17 00:01:04.810 --> 00:01:08.820 No sound 18 00:01:08.840 --> 00:01:12.870 Measuring the temperature of the surface of the moon especially during the eclipse is a really 19 00:01:12.890 --> 00:01:16.890 important thing because with that measurement we can learn about the 20 00:01:16.910 --> 00:01:20.940 characteristics, the properties of the surface of the moon. And particularly during an eclipse 21 00:01:20.960 --> 00:01:25.140 we learn about the upper, upper most surface. So what we see is that surface 22 00:01:25.160 --> 00:01:29.170 that stays warm longer generally have larger blocks or 23 00:01:29.190 --> 00:01:33.230 smaller pebbles and things like that. Where surfaces that cool off very quickly have 24 00:01:33.250 --> 00:01:37.300 smaller sand-sized particals and so by measuring how the surface 25 00:01:37.320 --> 00:01:41.480 of the moon, the temperature of the surface of the moon changes during an eclipse, we learn about 26 00:01:41.500 --> 00:01:45.520 the makeup of the surface of the moon. How the structure 27 00:01:45.540 --> 00:01:49.540 of the surface. And we can't do that normally. So it's these 28 00:01:49.560 --> 00:01:53.730 eclipses that give us a really, really unique opportunity to make specific 29 00:01:53.750 --> 00:01:57.750 measurements about the surface that we just can't do at any other time. 30 00:01:57.770 --> 00:02:01.780 No sound 31 00:02:01.800 --> 00:02:05.780 So the Lunar Reconnaissance 32 00:02:05.800 --> 00:02:09.970 Orbiter has been at the moon now for over six years. And in those six years we've 33 00:02:09.990 --> 00:02:13.970 learned an incredible amount about the surface of the moon and the lunar 34 00:02:13.990 --> 00:02:18.000 environment. What we've seen that's most surprising that the moon is in fact a dynamic place 35 00:02:18.020 --> 00:02:22.190 We're seeing changes on the surface on the moon that are occuring in the time that LRO has been 36 00:02:22.210 --> 00:02:26.230 at the moon. We're seeing new impact craters that have formed in the six years that we've been there. 37 00:02:26.250 --> 00:02:30.420 We're seeing the evidence of migrating water across the surface 38 00:02:30.440 --> 00:02:34.450 Not a lot of water. A small amount of water. But still the view that the moon is a 39 00:02:34.470 --> 00:02:38.460 static unchanging place is now completely different. 40 00:02:38.480 --> 00:02:42.470 With the eyes of LRO right at the surface of the moon, we're able to see that 41 00:02:42.490 --> 00:02:46.520 there are incredible amount of changes going on revealing that the moon is 42 00:02:46.540 --> 00:02:50.710 far more dynamic than we ever knew before. 43 00:02:50.730 --> 00:02:54.710 No sound 44 00:02:54.730 --> 00:02:58.740 Some of the coolest things that we've learned about the moon is that there's been 45 00:02:58.760 --> 00:03:02.760 evidence for volcanism that occured on the moon far more recently than 46 00:03:02.780 --> 00:03:06.770 we ever knew before. So for instance before LRO launched we thought that 47 00:03:06.790 --> 00:03:10.770 volcanism on the moon ended about a billion years ago. Now we have evidence for 48 00:03:10.790 --> 00:03:16.600 that volcanism may have occured as recently as recently as a hundred million year ago or perhaps even 49 00:03:16.620 --> 00:03:20.630 more recently than that. And that's surprising because that changes our entire view of how the interior heat 50 00:03:20.650 --> 00:03:24.820 of the moon has disapated over time. 51 00:03:24.840 --> 00:03:28.840 No sound 52 00:03:28.860 --> 00:03:32.870 LRO data and the results from LRO have completely rewritten 53 00:03:32.890 --> 00:03:36.900 the textbooks of what we know about the moon. I think the moon 54 00:03:36.920 --> 00:03:40.920 that we knew before LRO is now completely different. Of course the moon hasn't changed it's just 55 00:03:40.940 --> 00:03:44.940 our understanding of it. But the data that we've gotten from LRO 56 00:03:44.960 --> 00:03:49.120 has led to profound changes in how we view the moon and how 57 00:03:49.140 --> 00:03:53.130 view the moon in the future. And you know the great thing about 58 00:03:53.150 --> 00:03:57.160 the LRO data is that we're studying it now, but it's going to be 59 00:03:57.180 --> 00:04:01.170 a data set and a legacy that will last for generations to come in our understanding 60 00:04:01.190 --> 00:04:05.190 of the moon. 61 00:04:05.210 --> 00:04:09.380 No sound 62 00:04:09.400 --> 00:04:13.410 People should care about the moon because it's our neighbor 63 00:04:13.430 --> 00:04:17.460 in the sky. It's actually very close to the Earth compared to the 64 00:04:17.480 --> 00:04:21.600 distances to other objects in the solar system. And by studying the moon we can learn a lot 65 00:04:21.620 --> 00:04:25.800 about the history of the Earth. You know if you look surface of the moon there are 66 00:04:25.820 --> 00:04:29.830 places on the moon where we have rocks that are four-and-a-half billion 67 00:04:29.850 --> 00:04:33.850 years old. And so by looking at the moon we can learn about the earliest history of the solar 68 00:04:33.870 --> 00:04:37.880 system. The record of that portion of time in our solar system is almost all but 69 00:04:37.900 --> 00:04:41.900 gone from the Earth. So in order to understand what was happening just after the 70 00:04:41.920 --> 00:04:45.950 planets formed studying the surface of the moon is one of the most interesting and best 71 00:04:45.970 --> 00:04:49.970 places to do that. So when we look at moon we're really looking into 72 00:04:49.990 --> 00:04:53.980 the deep history of the Earth as well and I think from that we can learn a lot about 73 00:04:54.000 --> 00:04:59.012 how our planet has changed and how all planets have changed over time.