WEBVTT FILE 1 00:00:00.020 --> 00:00:04.030 [slate] 2 00:00:04.050 --> 00:00:08.100 A supermoon is quite easily the 3 00:00:08.120 --> 00:00:12.170 closest full moon of the year. As we know, the moon's orbit around the 4 00:00:12.190 --> 00:00:16.300 Earth is not a perfect circle. And so sometimes it's closer 5 00:00:16.320 --> 00:00:20.490 to the Earth and sometimes it's further away. And when we get both a full moon and the closest 6 00:00:20.510 --> 00:00:24.560 approach of the moon to the Earth, we get a supermoon. 7 00:00:24.580 --> 00:00:28.660 This is going to be a particularly important supermoon because it'll be the closest the moon has been to the Earth since January 8 00:00:28.680 --> 00:00:32.770 of 1948. And so it should be a spectacular show. 9 00:00:32.790 --> 00:00:36.810 [slate] 10 00:00:36.830 --> 00:00:40.960 You don't have to be out in any particular instant in time to see 11 00:00:40.980 --> 00:00:45.030 this. So any clear night over the weekend and into early next 12 00:00:45.050 --> 00:00:49.150 week you'll be able to see a full moon that's going to be brighter and larger 13 00:00:49.170 --> 00:00:53.320 than the average full moon. The supermoon which itself happens on Monday 14 00:00:53.340 --> 00:00:57.370 will appear to be about 14 percent larger and 30 percent 15 00:00:57.390 --> 00:01:01.410 brighter than the smallest full moon that we get. So really anytime at night 16 00:01:01.430 --> 00:01:05.490 if it's clear, you'll get a spectacular show and you'll get to see our beautiful moon 17 00:01:05.510 --> 00:01:09.520 in the sky. 18 00:01:09.540 --> 00:01:13.700 [slate] Over the seven 19 00:01:13.720 --> 00:01:17.740 years of the life of the LRO mission we've learned a lot about the moon. And I think for me 20 00:01:17.760 --> 00:01:21.800 one of the biggest surprises is how dynamic the moon is. 21 00:01:21.820 --> 00:01:25.890 That we're able to measure the changes that have occurred on the lunar surface 22 00:01:25.910 --> 00:01:30.040 as a result of impact craters that have formed. And that constant bombardment of 23 00:01:30.060 --> 00:01:34.230 the lunar surface actually erodes the surfaces quite faster than we expected 24 00:01:34.250 --> 00:01:38.250 before. Before LRO we thought that the boot prints that the astronauts left 25 00:01:38.270 --> 00:01:42.340 on the moon during the Apollo program would be around for millions of years. 26 00:01:42.360 --> 00:01:46.480 And recent results from LRO show that those boot prints may be erased 27 00:01:46.500 --> 00:01:50.630 much faster, over several tens of thousands of years. So we're learning the moon 28 00:01:50.650 --> 00:01:54.700 is a much more changing place, much more dynamic place than we ever imaged 29 00:01:54.720 --> 00:01:58.730 before. [slate] 30 00:01:58.750 --> 00:02:02.830 [slate] One of the great things about 31 00:02:02.850 --> 00:02:06.970 the moon is that we use it, our understanding of the moon as a cornerstone 32 00:02:06.990 --> 00:02:11.150 for understanding all of the other objects in the solar system. So for instance when we got the 33 00:02:11.170 --> 00:02:15.220 beautiful images of Pluto, we learned that the surface of Pluto has areas that are 34 00:02:15.240 --> 00:02:19.330 very smooth, that have little impact craters on them. Or few impact craters on them. 35 00:02:19.350 --> 00:02:23.470 And so one of the things that we can do is estimate the ages of those surfaces. 36 00:02:23.490 --> 00:02:27.550 It turns out that Pluto has very young surfaces. And the reason that we know that is because of our 37 00:02:27.570 --> 00:02:31.590 studies of the moon. So for any object in the solar system, the basis of 38 00:02:31.610 --> 00:02:35.680 our understanding comes from our knowledge of the moon. And so our continued studying 39 00:02:35.700 --> 00:02:39.800 of the moon tells us more about not only how the moon has evolved, but also how all of the 40 00:02:39.820 --> 00:02:43.820 solar system objects have evolved. 41 00:02:43.840 --> 00:02:48.020 [slate] 42 00:02:48.040 --> 00:02:52.070 To learn more about the LRO mission, you can go to NASA.gov/LRO. 43 00:02:52.090 --> 00:02:56.140 Follow us on Twitter @LRO_NASA. 44 00:02:56.160 --> 00:03:00.230 And of course you can also post pictures of the supermoon using the hashtag 45 00:03:00.250 --> 00:03:02.562 #NASASupermoon.