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.