1 00:00:10,385 --> 00:00:13,471 So a total lunar eclipse happens when the sun, the Earth, 2 00:00:13,471 --> 00:00:15,140 and the moon are aligned. 3 00:00:15,140 --> 00:00:18,977 The moon goes around the Earth once a month, but we don't get an eclipse 4 00:00:18,977 --> 00:00:19,519 every month. 5 00:00:19,519 --> 00:00:22,522 Because the moon's orbit is a little bit tilted. 6 00:00:23,231 --> 00:00:26,067 We get that alignment about every six months. 7 00:00:26,067 --> 00:00:31,156 And so the Earth's shadow stretches across 240,000 8 00:00:31,156 --> 00:00:34,117 miles and lands on the moon. 9 00:00:41,833 --> 00:00:44,586 The great thing about a lunar eclipse is that you don't need 10 00:00:44,586 --> 00:00:48,131 special equipment, and you don't need to be in a particular location. 11 00:00:48,173 --> 00:00:51,217 Everybody in the United States is going to be able to see this. 12 00:00:51,593 --> 00:00:54,596 They just need to go outside and locate the moon. 13 00:01:03,021 --> 00:01:04,355 So Lunar Reconnaissance Orbiter, 14 00:01:04,355 --> 00:01:08,109 or LRO, has been in orbit around the moon since 2009. 15 00:01:08,401 --> 00:01:12,363 It's been making global maps of the color and the shape of the moon. 16 00:01:12,655 --> 00:01:16,367 The temperature for, some forms of radiation from the moon. 17 00:01:16,701 --> 00:01:21,414 And so we're learning a lot about what it's made of, more 18 00:01:21,414 --> 00:01:23,124 about where it came from. 19 00:01:23,124 --> 00:01:26,127 And therefore where the earth, how it formed. 20 00:01:26,294 --> 00:01:30,006 And we're also learning the shape of the terrain 21 00:01:30,006 --> 00:01:34,677 to a level of detail that will allow us to land there safely and explore. 22 00:01:42,894 --> 00:01:43,269 Well, 23 00:01:43,269 --> 00:01:46,397 I'm maybe you can tell I'm old enough to remember the Apollo era. 24 00:01:46,397 --> 00:01:48,525 And we went there for a few years. 25 00:01:48,525 --> 00:01:50,068 We landed astronauts on the moon. 26 00:01:50,068 --> 00:01:53,071 We gathered a bunch of really important samples. 27 00:01:53,321 --> 00:01:55,990 And then there was sort of a quiet period for a while. 28 00:01:55,990 --> 00:01:59,786 We're now going back with, not only NASA itself, 29 00:01:59,786 --> 00:02:04,290 but its commercial partners to sample the surface and explore. 30 00:02:05,208 --> 00:02:09,212 And the moon is a great destination for this 31 00:02:09,212 --> 00:02:13,007 because it remembers everything that has happened over 32 00:02:13,007 --> 00:02:16,594 the 4.6 billion years the solar system has been in existence. 33 00:02:16,970 --> 00:02:21,432 This is how we can find out where we came from, where the earth came from, 34 00:02:21,432 --> 00:02:24,435 where the moon came from, how the solar system formed. 35 00:02:24,769 --> 00:02:27,105 And so I think that's really exciting. 36 00:02:36,990 --> 00:02:37,699 We've only 37 00:02:37,699 --> 00:02:41,077 landed people in 5 or 6 different places 38 00:02:41,077 --> 00:02:44,122 on the moon, and those places were all near the equator. 39 00:02:44,455 --> 00:02:49,085 We're now sending both people and robots to all kinds of places, 40 00:02:49,085 --> 00:02:52,755 including the South Pole, that we haven't explored yet at all. 41 00:02:53,590 --> 00:02:56,009 The great thing about the South Pole is that it 42 00:02:56,009 --> 00:02:59,012 can trap, volatiles like water. 43 00:02:59,053 --> 00:03:03,016 Trap it is ice that may have been there for a billion years. 44 00:03:03,683 --> 00:03:06,978 And this is a great way to sample the history of the solar system. 45 00:03:07,687 --> 00:03:11,566 But it also means that we might be able to find ways to sustain 46 00:03:11,566 --> 00:03:14,569 a human presence on the surface. 47 00:03:20,950 --> 00:03:21,784 Right, exactly. 48 00:03:21,784 --> 00:03:25,955 So in order for us to create a sustain presence on the moon with people, 49 00:03:26,247 --> 00:03:29,667 we need to know as much as possible about what it's like there. 50 00:03:30,418 --> 00:03:33,046 What resources are available? 51 00:03:33,046 --> 00:03:37,550 What the illumination is going to be like if we land at the South Pole? 52 00:03:37,550 --> 00:03:41,387 The sun is never more than a degree and a half above the the horizon. 53 00:03:42,180 --> 00:03:45,141 The lighting situation is very unusual there. 54 00:03:45,141 --> 00:03:51,022 So we need to gather as much information as we can in order to plan those missions 55 00:03:51,022 --> 00:03:55,026 and make them as productive and survivable as possible. 56 00:04:05,495 --> 00:04:08,998 So pi is this incredibly important number in mathematics and science. 57 00:04:09,040 --> 00:04:12,794 It's just the ratio of the circumference of a circle to its diameter. 58 00:04:13,169 --> 00:04:15,505 But it shows up in all kinds of other places. 59 00:04:15,505 --> 00:04:18,591 So when I do eclipse calculations to figure out 60 00:04:18,591 --> 00:04:22,220 where the shadow is going to fall, that involves trigonometry. 61 00:04:22,220 --> 00:04:25,223 And all of trigonometry is built on pi. 62 00:04:26,349 --> 00:04:29,435 Now Pi Day is March 14th. 63 00:04:29,477 --> 00:04:34,148 It just so happens that the first three digits of pi or 3.14 64 00:04:34,148 --> 00:04:38,444 and so the third month and the 14th day becomes pi day. 65 00:04:38,820 --> 00:04:42,240 And this lunar eclipse is going to happen on Pi Day. 66 00:04:43,199 --> 00:04:46,828 That happens once every 350 years or so. 67 00:04:46,869 --> 00:04:49,080 So it's quite unusual. 68 00:04:49,080 --> 00:04:52,834 It's a fun way to celebrate not just the moon, 69 00:04:52,834 --> 00:04:55,837 but, math and pi. 70 00:04:56,170 --> 00:04:57,755 Of both kinds. 71 00:04:57,755 --> 00:05:01,634 So think of fruit pies and pizza pies and all kinds of things, 72 00:05:03,052 --> 00:05:04,178 that you can 73 00:05:04,178 --> 00:05:09,142 add to your observation of the moon and your celebration of science. 74 00:05:17,150 --> 00:05:18,860 So I mentioned this before. 75 00:05:18,860 --> 00:05:22,780 The eclipses don't happen every month because the moon's orbit is tilted 76 00:05:22,780 --> 00:05:24,157 by about five degrees. 77 00:05:24,157 --> 00:05:28,536 And so some months during the full moon, it's going to pass a little bit 78 00:05:28,536 --> 00:05:30,038 above the Earth's shadow. 79 00:05:30,038 --> 00:05:33,041 And some months it's going to pass a little bit below. 80 00:05:33,333 --> 00:05:36,711 But about once every six months it actually passes through the Earth's 81 00:05:36,711 --> 00:05:37,754 shadow. 82 00:05:37,754 --> 00:05:40,840 Now, it doesn't hit the middle of that shadow every time. 83 00:05:40,840 --> 00:05:43,509 So some lunar eclipses are just partial. 84 00:05:43,509 --> 00:05:47,889 But every year or year and a half, we on average, 85 00:05:47,889 --> 00:05:51,476 we get a total lunar eclipse where the moon passes through the center 86 00:05:51,476 --> 00:05:55,605 of the Earth's shadow, and every part of the moon is blocked from the sun. 87 00:06:05,198 --> 00:06:08,201 I will absolutely be outside watching this eclipse. 88 00:06:08,618 --> 00:06:11,621 The best thing about a lunar eclipse is that it's beautiful. 89 00:06:11,662 --> 00:06:17,001 So the moon during totality will turn shades of orange and red and brown. 90 00:06:17,335 --> 00:06:22,507 It's being, hit by all of the sunrises and sunsets projected from the Earth. 91 00:06:23,383 --> 00:06:26,386 And those colors will change over time. 92 00:06:27,011 --> 00:06:29,180 And the moon will be dim enough 93 00:06:29,180 --> 00:06:32,183 that it kind of looks almost transparent. 94 00:06:32,475 --> 00:06:36,187 This is something I've noticed over, watching the past few. 95 00:06:36,729 --> 00:06:39,399 Total lunar eclipse is that it almost seems to be disappearing 96 00:06:39,399 --> 00:06:41,192 like the Cheshire Cat. 97 00:06:41,192 --> 00:06:44,195 So it's an unusual thing to watch. 98 00:06:44,487 --> 00:06:45,405 It's. 99 00:06:45,405 --> 00:06:48,783 It lasts for an hour, so you have plenty of time 100 00:06:48,783 --> 00:06:51,786 to look around and see what other effects there are. 101 00:06:52,370 --> 00:06:56,457 And it makes you think about our place in the solar system. 102 00:06:56,499 --> 00:06:58,543 I mean, we're standing at night. 103 00:06:58,543 --> 00:07:00,503 Every night we're standing in the shadow of the earth. 104 00:07:00,503 --> 00:07:04,006 But on this particular night, we get to see that shadow 105 00:07:04,757 --> 00:07:08,678 its extent all the way across space from here to the moon. 106 00:07:08,678 --> 00:07:11,681 And so it's a it's just a lovely thing to watch and to think about. 107 00:07:18,855 --> 00:07:21,858 The moon remembers everything. 108 00:07:22,358 --> 00:07:25,820 You know, on the Earth, all of this is erased by weather 109 00:07:25,820 --> 00:07:29,073 and tectonics and all kinds of things that make, 110 00:07:29,740 --> 00:07:32,743 cratering events and other things, just go away. 111 00:07:32,952 --> 00:07:34,704 But all of that's remembered on the moon. 112 00:07:34,704 --> 00:07:39,667 And so we can look at craters that were formed three and 4 billion years ago 113 00:07:39,667 --> 00:07:42,795 and learn about what was going on in the early solar system from that. 114 00:07:42,795 --> 00:07:45,756 And I think that's just very cool. 115 00:07:51,345 --> 00:07:52,763 To learn more about the moon 116 00:07:52,763 --> 00:07:56,142 and about this eclipse, go to science dot nasa.gov slash moon.