1 00:00:11,094 --> 00:00:11,386 Yeah. 2 00:00:11,386 --> 00:00:13,513 So a total solar eclipse happens 3 00:00:13,513 --> 00:00:17,017 when the moon passes between us here on the earth and the sun. 4 00:00:17,350 --> 00:00:20,353 And for those people who are in the path of totality, 5 00:00:20,353 --> 00:00:24,190 it will block out the moon will block out the main body of the sun, 6 00:00:24,190 --> 00:00:27,193 and you'll get to see the corona or the atmosphere 7 00:00:27,193 --> 00:00:30,196 of the sun peeking out around the moon. 8 00:00:30,488 --> 00:00:34,659 Now, everybody in the contiguous United States will get to see 9 00:00:34,659 --> 00:00:37,912 at least a partial solar eclipse, which means that the moon will block out 10 00:00:38,079 --> 00:00:41,082 part of the sun, but not all of it. 11 00:00:47,922 --> 00:00:48,423 That's right. 12 00:00:48,423 --> 00:00:49,883 Never look directly at the sun, 13 00:00:49,883 --> 00:00:53,887 but there are three safe ways to view the solar eclipse. 14 00:00:54,304 --> 00:00:57,766 The first is with special solar viewers. 15 00:00:57,974 --> 00:01:02,645 These glasses have special filters in front of them so that it is 16 00:01:02,645 --> 00:01:07,358 safe to view the sun always, but during the partial phases of the eclipse as well. 17 00:01:08,109 --> 00:01:12,572 If you're in the path of totality, then during that total phase 18 00:01:12,572 --> 00:01:15,950 of the eclipse, when the moon totally blocks out the main body of the sun, 19 00:01:16,242 --> 00:01:19,120 then it's safe to look directly at the corona, 20 00:01:19,120 --> 00:01:22,332 which is the part of the sun that peeks out during totality. 21 00:01:22,749 --> 00:01:25,251 The third way is to make a pinhole projector. 22 00:01:25,251 --> 00:01:26,836 You can make them. You can also 23 00:01:28,254 --> 00:01:28,880 get one of the 24 00:01:28,880 --> 00:01:31,883 ones that we're using for our punch outreach. 25 00:01:32,050 --> 00:01:33,885 They're just simple holes. 26 00:01:33,885 --> 00:01:35,887 You stand with the sun behind you. 27 00:01:35,887 --> 00:01:40,225 You project the image then of the moon coming between us 28 00:01:40,225 --> 00:01:43,895 and the sun down onto the ground in front of you, 29 00:01:43,895 --> 00:01:46,898 through the holes. 30 00:01:53,947 --> 00:01:55,240 I am so excited 31 00:01:55,240 --> 00:01:58,868 to get to see the solar corona, the atmosphere of the sun. 32 00:01:58,868 --> 00:02:02,747 That's the part of the sun that peeks out around the moon 33 00:02:03,373 --> 00:02:06,668 during the total the totality phase of solar eclipse. 34 00:02:06,918 --> 00:02:09,838 That's the part of the sun that I study all the time, 35 00:02:09,838 --> 00:02:12,882 and I'm so excited to actually get to see it with my own eyes. 36 00:02:20,890 --> 00:02:24,727 This one is different than the one in 2017 for a few reasons. 37 00:02:24,936 --> 00:02:28,064 I got to see the one in 2017, so it was so amazing. 38 00:02:29,107 --> 00:02:31,234 The first is that 39 00:02:31,234 --> 00:02:35,655 the path of totality is coming over where more people live, and so more 40 00:02:35,655 --> 00:02:39,701 people will have the opportunity to see the total phase of the eclipse. 41 00:02:40,243 --> 00:02:44,706 The second thing is that the totality phase is going to last longer 42 00:02:44,706 --> 00:02:48,084 this time than in 2017, almost twice as long. 43 00:02:48,084 --> 00:02:51,921 This one will last for 4 minutes in the central line of totality there. 44 00:02:52,839 --> 00:02:55,925 And the third thing is the sun is more active right now. 45 00:02:56,426 --> 00:03:00,680 So in 2017, there was some activity, The corona had some structure. 46 00:03:01,055 --> 00:03:04,809 But in this phase, the sun is more active. 47 00:03:04,809 --> 00:03:06,811 So that corona, the atmosphere of the sun, 48 00:03:06,811 --> 00:03:10,064 is going to have more complexity and we might even get to see 49 00:03:10,523 --> 00:03:14,402 a magnetic explosion happening on the sun during the eclipse. 50 00:03:24,287 --> 00:03:25,872 Yeah, there's a lot of ways 51 00:03:25,872 --> 00:03:29,209 that anybody can get involved in the science of the eclipse. 52 00:03:29,918 --> 00:03:33,755 One is called Globe Observer, where you can use your cell phone 53 00:03:33,755 --> 00:03:35,215 to measure the cloud coverage 54 00:03:35,215 --> 00:03:38,676 and how the temperature feels during the eclipse. 55 00:03:38,676 --> 00:03:42,764 Because the moon is blocking the sunlight and so the temperature 56 00:03:42,764 --> 00:03:44,891 actually decreases. 57 00:03:44,891 --> 00:03:48,686 There's also a project called Sun Sketcher where you can use your phone 58 00:03:48,686 --> 00:03:52,565 to actually look at the shape of the sun during the eclipse. 59 00:03:52,941 --> 00:03:54,734 The third one is called Soundscape. 60 00:03:54,734 --> 00:03:58,238 So that's one where you can actually record the sounds of the animals 61 00:03:58,238 --> 00:04:00,031 during the eclipse, because the animals are going 62 00:04:00,031 --> 00:04:03,618 to think that it's nighttime, it feels like nighttime and it's dark 63 00:04:03,618 --> 00:04:06,621 like nighttime, and the animals respond to that. 64 00:04:14,003 --> 00:04:14,212 Yeah. 65 00:04:14,212 --> 00:04:18,716 So during the eclipse, the moon is blocking out the sunlight. 66 00:04:18,716 --> 00:04:21,552 And so it feels like dawn or dusk to the animals. 67 00:04:21,552 --> 00:04:24,514 And so they will start to respond like it's nighttime. 68 00:04:24,514 --> 00:04:25,932 You'll hear different sounds 69 00:04:26,933 --> 00:04:30,853 and it's with soundscapes, you can actually record that 70 00:04:30,853 --> 00:04:33,856 and actually help the scientists take data on that. 71 00:04:41,948 --> 00:04:45,994 So during a total solar eclipse, when we can see the solar corona, 72 00:04:45,994 --> 00:04:49,747 the outer atmosphere of the sun, scientists are looking at that corona. 73 00:04:49,747 --> 00:04:53,710 There are a lot of mysteries about how the energy gets into the corona 74 00:04:53,710 --> 00:04:56,921 and how that energy gets from the corona out into the solar system. 75 00:04:57,338 --> 00:05:01,342 The other thing we're looking at is how that energy from the sun impacts 76 00:05:01,509 --> 00:05:02,677 Earth's atmosphere. 77 00:05:02,677 --> 00:05:06,639 And so we're flying experiments sounding rockets to look at how 78 00:05:06,681 --> 00:05:09,684 Earth's atmosphere responds to that decrease in sunlight. 79 00:05:18,484 --> 00:05:19,694 Yeah, women have been 80 00:05:19,694 --> 00:05:22,655 a part of solar studies for a long time. 81 00:05:22,739 --> 00:05:24,824 Two fun examples are Maria mitchell 82 00:05:24,824 --> 00:05:28,161 and Cecilia Payne, who are part of their 1869 83 00:05:28,578 --> 00:05:31,956 total solar eclipse campaigns that came here in the United States. 84 00:05:32,498 --> 00:05:35,293 But here at NASA, we're just so lucky that women 85 00:05:35,293 --> 00:05:39,130 get to be a part of and lead so many solar missions. 86 00:05:39,130 --> 00:05:43,009 Mission development, science studies all throughout Heliophysics. 87 00:05:52,935 --> 00:05:53,353 Yeah. 88 00:05:53,353 --> 00:05:56,564 So during the eclipse, these students are going 89 00:05:56,564 --> 00:06:00,443 to launch balloons with instruments to measure 90 00:06:00,443 --> 00:06:04,238 how the atmosphere responds during the total solar eclipse. 91 00:06:04,238 --> 00:06:09,077 Because during the eclipse, the moon blocks out the main body of the sun. 92 00:06:09,077 --> 00:06:13,039 And so the light coming to the earth and how the atmosphere responds 93 00:06:13,039 --> 00:06:16,042 will be really interesting to study. 94 00:06:16,042 --> 00:06:19,045 And those students are going to be a part of that science. 95 00:06:27,762 --> 00:06:27,929 Yeah, 96 00:06:27,929 --> 00:06:33,476 so you can learn more by going to go dot nasa.gov slash Eclipse 2024. [ go.nasa.gov/eclipse2024 ]