WEBVTT FILE 1 00:00:11.803 --> 00:00:13.555 So during a solar 2 00:00:13.555 --> 00:00:17.392 eclipse, the sun, moon and earth are lined up 3 00:00:17.392 --> 00:00:22.605 so that the sun shines on the moon, which then casts a shadow on the earth. 4 00:00:22.897 --> 00:00:26.651 And so in the United States, in the contiguous United States, 5 00:00:26.651 --> 00:00:31.740 everyone will have an opportunity to see at least a partial solar eclipse. 6 00:00:32.073 --> 00:00:35.201 And so that's when the moon moves across 7 00:00:35.201 --> 00:00:38.204 and partially blocks out the sun's disk. 8 00:00:38.496 --> 00:00:42.959 There is also a narrow path that moves from Texas 9 00:00:43.209 --> 00:00:47.380 up to New England, where you can experience totality. 10 00:00:47.505 --> 00:00:51.426 So for a brief period of time as that shadow is moving across, 11 00:00:51.926 --> 00:00:55.722 you will see the moon completely BLOCK the sun out. 12 00:00:55.972 --> 00:01:00.101 And that then reveals the sun's outer atmosphere called the corona. 13 00:01:00.393 --> 00:01:04.355 The rest of the time, it's still a partial eclipse, 14 00:01:04.814 --> 00:01:08.318 but in that narrow time period, that's 15 00:01:08.318 --> 00:01:13.073 when you can experience the full aspect of what is a total solar eclipse. 16 00:01:22.499 --> 00:01:23.124 Well, 17 00:01:23.124 --> 00:01:26.127 yeah, so there's a couple of ways we can do that. 18 00:01:26.169 --> 00:01:30.840 So except for that narrow time, when you're in totality, 19 00:01:31.257 --> 00:01:32.759 the rest of the time is what we call 20 00:01:32.759 --> 00:01:35.804 a partial eclipse, where the sun is only partially blocked 21 00:01:36.012 --> 00:01:41.226 and it's always, always too bright to look at just normally like the sun. 22 00:01:41.392 --> 00:01:45.271 So what you want to do is if you want to look at it directly, you want to have safe 23 00:01:45.271 --> 00:01:48.316 solar viewing glasses or eclipse glasses, 24 00:01:48.608 --> 00:01:52.445 and then you're able to look up and safely see it. 25 00:01:52.695 --> 00:01:56.199 Now, if you don't have solar viewing glasses, 26 00:01:56.407 --> 00:02:00.829 then what you can do is you can create a projector which projects 27 00:02:00.870 --> 00:02:05.166 the sun's image onto a piece of paper or the ground, or you can even take 28 00:02:05.166 --> 00:02:09.629 a piece of paper with holes punched in it, which makes a pinhole camera 29 00:02:09.921 --> 00:02:14.092 that allows you to see the sun the crescents cast onto the ground. 30 00:02:14.300 --> 00:02:19.514 You can even take your hands, do them like this with the sun behind you. 31 00:02:19.722 --> 00:02:21.516 And that creates a little pinholes. 32 00:02:21.516 --> 00:02:22.809 And it's actually much like 33 00:02:22.809 --> 00:02:26.604 what happens with the leaves in the trees, which is just an amazing thing to see. 34 00:02:36.614 --> 00:02:37.323 Well, 35 00:02:37.323 --> 00:02:40.535 I am really, really, really stoked to see the corona. 36 00:02:40.577 --> 00:02:43.246 I mean, the corona, the outer part of the sun's atmosphere 37 00:02:43.246 --> 00:02:48.585 is what I've been studying for 20 years, but I have always studied it from space. 38 00:02:49.002 --> 00:02:52.630 When you can't actually see this part of the atmosphere 39 00:02:53.006 --> 00:02:57.886 and the only time you can see it is when you're in totality on the ground. 40 00:02:57.886 --> 00:03:03.433 So I will see the part of the sun I study with my own eyes. 41 00:03:03.641 --> 00:03:07.729 But you know more than that, it's a really amazing experience. 42 00:03:07.729 --> 00:03:10.899 Once I first saw a total solar eclipse, I was hooked. 43 00:03:11.107 --> 00:03:15.111 And I'm really excited because I will get to experience this with my wife. 44 00:03:15.320 --> 00:03:18.323 And this is just such an amazing opportunity 45 00:03:18.406 --> 00:03:21.826 to share and with all of the people around you. 46 00:03:33.796 --> 00:03:36.507 Well, this is a really amazing opportunity. 47 00:03:36.507 --> 00:03:40.929 Nature is giving us a laboratory to study many aspects. 48 00:03:41.846 --> 00:03:45.350 One, of course, is the corona, which is very, very important. 49 00:03:45.642 --> 00:03:50.104 It's much, much hotter by 100 times than the surface of the sun. 50 00:03:50.480 --> 00:03:54.150 And it is where solar activity and space weather 51 00:03:54.150 --> 00:03:57.654 comes from huge explosions that send out solar material. 52 00:03:57.904 --> 00:04:00.907 And so this is a really important opportunity to study that. 53 00:04:01.115 --> 00:04:05.995 But also as we study that shadow moving across the country 54 00:04:06.621 --> 00:04:10.833 and we see the change in light in the atmosphere, 55 00:04:10.959 --> 00:04:16.005 it allows us to study the lower atmosphere, clouds and temperature, 56 00:04:16.214 --> 00:04:21.302 and it also allows us to study the very important upper atmosphere 57 00:04:21.302 --> 00:04:26.557 called the ionosphere, which is critical for our daily communications. 58 00:04:26.683 --> 00:04:30.561 And this is giving scientists a really special opportunity 59 00:04:30.770 --> 00:04:35.525 to do an experiment that can only be done during a total solar eclipse. 60 00:04:45.493 --> 00:04:48.371 Well, the sun has an activity cycle. 61 00:04:48.371 --> 00:04:50.957 It gets magnetically excited. 62 00:04:50.957 --> 00:04:53.960 The magnets, the magnetism builds up in it 63 00:04:54.043 --> 00:04:57.714 and it releases energy as it gets more and more twisted. 64 00:04:57.714 --> 00:05:02.218 So we go from very low activity or solar min [minimum] to high activity. 65 00:05:02.218 --> 00:05:04.095 Solar maximum back down to low. 66 00:05:04.095 --> 00:05:09.350 We are currently either in or getting close to solar maximum. 67 00:05:09.350 --> 00:05:11.811 So this is the most activity, 68 00:05:11.811 --> 00:05:15.231 most space weather we could possibly see will be happening. 69 00:05:15.398 --> 00:05:20.320 And this is a great time to study that because it has such a huge impact 70 00:05:20.320 --> 00:05:24.157 on our society and scientists will take this opportunity 71 00:05:24.324 --> 00:05:28.036 to learn more about our own star and how it affects our daily 72 00:05:28.036 --> 00:05:31.039 lives. 73 00:05:40.214 --> 00:05:42.967 It's an amazing achievement for humanity. 74 00:05:42.967 --> 00:05:47.847 This is the fastest are totally autonomous spacecraft 75 00:05:47.889 --> 00:05:53.019 it's ever been created, and it's already, since 2018, 76 00:05:53.144 --> 00:05:56.814 been traveling, orbiting the sun, getting closer and closer. 77 00:05:56.981 --> 00:06:00.943 It's already started flying through the sun's corona, this part 78 00:06:00.943 --> 00:06:03.071 that we see during a total solar eclipse. 79 00:06:03.071 --> 00:06:06.991 And on December 24th, it will make its closest approach. 80 00:06:06.991 --> 00:06:11.954 It will be less than 4 million miles from the surface of the sun. 81 00:06:12.121 --> 00:06:15.917 Now, this doesn't seem like that's very, very close. 82 00:06:15.917 --> 00:06:21.255 But remember, the sun is 93 million miles away, so this is less than 4% 83 00:06:21.547 --> 00:06:25.301 a distance, allowing us to study this really important 84 00:06:25.301 --> 00:06:26.719 part of the sun's atmosphere. 85 00:06:36.354 --> 00:06:37.146 Well, yeah. 86 00:06:37.146 --> 00:06:40.733 So there's been a huge explosion in our ability 87 00:06:40.733 --> 00:06:44.404 to make better predictions, which also includes making better maps. 88 00:06:44.612 --> 00:06:48.908 And one of the keys to this is the data that we get 89 00:06:48.908 --> 00:06:51.077 from the Lunar Reconnaissance Orbiter. 90 00:06:51.077 --> 00:06:54.372 This is providing an incredibly detailed 91 00:06:54.372 --> 00:06:57.667 profile of the edge of the moon, 92 00:06:57.917 --> 00:07:01.546 which has a huge impact on how the shadow 93 00:07:01.546 --> 00:07:05.133 is cast on earth and the structure of that shadow and the timing. 94 00:07:05.299 --> 00:07:08.594 We've also used data about the Earth itself. 95 00:07:08.594 --> 00:07:13.182 So combining the the the changes in the Earth 96 00:07:13.433 --> 00:07:18.521 as well as the structure of the moon, has given us unprecedented abilities 97 00:07:18.521 --> 00:07:22.275 to predict the timing, as well as the maps 98 00:07:22.275 --> 00:07:25.278 that we use to know where and when the eclipse will be. 99 00:07:35.455 --> 00:07:37.165 Yeah, so a transit is 100 00:07:37.165 --> 00:07:41.377 when a planet, for example, moves in front of a star. 101 00:07:41.419 --> 00:07:44.547 Now, of course, for the eclipses we're talking about, 102 00:07:44.839 --> 00:07:48.885 the moon is moving in front of the sun and completely blocking it out. 103 00:07:49.177 --> 00:07:53.806 But distant stars have little planets that are moving in front of them. 104 00:07:53.931 --> 00:07:58.728 And by looking at how the light changes as the planet moves across it 105 00:07:58.728 --> 00:08:02.607 very subtly, we can see the size of the planet. 106 00:08:02.607 --> 00:08:05.234 The bigger the drop, the bigger the planet. 107 00:08:05.234 --> 00:08:08.070 But we can also look at the different colors of light 108 00:08:08.070 --> 00:08:11.991 that are coming through the edge of that planet, which is allowing us to 109 00:08:12.033 --> 00:08:15.036 to study the atmospheres of those planets. 110 00:08:15.077 --> 00:08:18.664 This is something that's happening with James Webb Space Telescope, 111 00:08:18.915 --> 00:08:22.335 and we will be building even better instruments in the future 112 00:08:22.668 --> 00:08:27.882 to help us figure out if life is possible or maybe even if life 113 00:08:27.882 --> 00:08:31.844 exists on other planets outside of our own solar system. 114 00:08:41.187 --> 00:08:42.188 Well, there are a lot of 115 00:08:42.188 --> 00:08:45.983 great tips, participatory science opportunities. 116 00:08:46.317 --> 00:08:51.656 Now, NASA has created a several apps that you can download for your phone. 117 00:08:51.822 --> 00:08:55.409 One is called Globe Observer, which is a yearlong project, 118 00:08:55.409 --> 00:08:58.454 but they have a special Eclipse app that during the eclipse 119 00:08:58.621 --> 00:09:03.125 you can participate and take measurements of temperature and clouds. 120 00:09:03.459 --> 00:09:06.128 There's also one called Sun Sketcher, 121 00:09:06.128 --> 00:09:10.633 which is allowing you to sketch and to take images of the corona. 122 00:09:11.008 --> 00:09:14.679 And Eclipse Soundscapes is allowing 123 00:09:14.679 --> 00:09:19.475 people to take sounds to record sounds that are happening as the 124 00:09:19.559 --> 00:09:24.146 the wildlife changes during the eclipse and bring back that data 125 00:09:24.313 --> 00:09:27.567 to allow NASA's scientists, but also to have 126 00:09:28.192 --> 00:09:32.863 the public participate as a scientist to help us gather more data 127 00:09:33.072 --> 00:09:34.740 so that we can better understand 128 00:09:34.740 --> 00:09:38.619 all of the amazing things that we can learn during a solar eclipse. 129 00:09:48.129 --> 00:09:50.423 Well, it wasn't too long 130 00:09:50.423 --> 00:09:53.759 after Einstein had proposed his theory of general relativity, 131 00:09:53.884 --> 00:09:56.804 which basically says that a massive object 132 00:09:56.804 --> 00:10:00.516 like the sun literally bends space. 133 00:10:00.516 --> 00:10:05.146 And a consequence of that is this light travels through that bent space. 134 00:10:05.354 --> 00:10:06.897 The light itself bends. 135 00:10:06.897 --> 00:10:10.776 And so the gravity of the sun acts like a lens 136 00:10:10.901 --> 00:10:13.779 and bends starlight when it travels around it. 137 00:10:13.779 --> 00:10:17.533 So during a total solar eclipse, when the bright disk 138 00:10:17.533 --> 00:10:20.536 is blocked out, we can see background stars. 139 00:10:20.703 --> 00:10:24.373 But the positions of those stars are slightly shifted 140 00:10:24.582 --> 00:10:27.710 because of the bending of the light going around the sun. 141 00:10:27.877 --> 00:10:30.087 So we know exactly where they are. 142 00:10:30.087 --> 00:10:34.091 We see them in a different location and that allows us to 143 00:10:34.759 --> 00:10:38.054 confirm the results of what general relativity 144 00:10:38.054 --> 00:10:42.058 predicts will happen when that star star's light passes the Sun. 145 00:10:51.776 --> 00:10:53.527 Well, the viewers can go to 146 00:10:53.527 --> 00:10:57.907 go that NASA dot gov slash eclipse 2024 [go.nasa.gov/eclipse2024]. 147 00:10:58.157 --> 00:11:00.701 And there you can find out about the citizen science. 148 00:11:00.701 --> 00:11:04.789 You can participate in see live feeds across the country 149 00:11:04.955 --> 00:11:08.959 and find out about all of the opportunities so that you can participate, 150 00:11:08.959 --> 00:11:11.545 whether you're in the path or out of the path. 151 00:11:11.545 --> 00:11:14.382 There are lots of things that people can enjoy 152 00:11:14.382 --> 00:11:19.303 and take that experience and have it be something unique, 153 00:11:19.303 --> 00:11:23.974 something that they can experience and share with all of the people around them.