1 00:00:00,050 --> 00:00:03,070 [slate] 2 00:00:03,070 --> 00:00:06,090 [slate] 3 00:00:06,090 --> 00:00:09,120 Text on screen: What will we experience on August 21? 4 00:00:09,120 --> 00:00:12,180 5 00:00:12,180 --> 00:00:15,290 We are so excited for August 21. 6 00:00:15,290 --> 00:00:18,420 What is going to happen is the moon is going to cross 7 00:00:18,420 --> 00:00:21,630 in between the sun and the Earth and we're going to be treated 8 00:00:21,630 --> 00:00:24,810 to a spectacular show as that shadow goes across the 9 00:00:24,810 --> 00:00:27,860 Earth. Everywhere in North America, Central America 10 00:00:27,860 --> 00:00:30,940 and even bits of South America will get to see some 11 00:00:30,940 --> 00:00:34,070 portion of the eclipse - either partial or total. 12 00:00:34,070 --> 00:00:37,260 If you're in the path of totality that's going to be 13 00:00:37,260 --> 00:00:40,440 especially amazing because what happens is the moon will totally 14 00:00:40,440 --> 00:00:43,620 block out the main body of the sun and you'll get to 15 00:00:43,620 --> 00:00:46,710 see the sun's atmosphere, the solar corona, around the moon. 16 00:00:46,710 --> 00:00:49,740 And it's just going to be amazing. 17 00:00:49,740 --> 00:00:52,770 Text on screen: We've been told never to look directly at the sun (even with sunglasses!). 18 00:00:52,770 --> 00:00:55,970 Text on screen cont.: How can we enjoy this eclipse safely? 19 00:00:55,970 --> 00:00:59,040 That's correct, never look directly at the 20 00:00:59,040 --> 00:01:02,210 sun even with sunglasses on. What you want are 21 00:01:02,210 --> 00:01:05,380 safety eclipse glasses like these. And you can check to 22 00:01:05,380 --> 00:01:08,470 make sure that your eclipse glasses really are safety 23 00:01:08,470 --> 00:01:11,680 eclipse glasses by going to our webpage 24 00:01:11,680 --> 00:01:14,740 eclipse2017.nasa.gov. And on that webpage 25 00:01:14,740 --> 00:01:17,820 we have information of how to check. So, for example you want 26 00:01:17,820 --> 00:01:20,930 to look for an ISO number, cross check that 27 00:01:20,930 --> 00:01:24,120 with what we have on our webpage, and a manufacturer - again, cross check 28 00:01:24,120 --> 00:01:27,310 that with our webpage. During totality, 29 00:01:27,310 --> 00:01:30,360 if you are in that path you can take off your glasses and look 30 00:01:30,360 --> 00:01:33,420 directly at the sun during those couple of minutes. 31 00:01:33,420 --> 00:01:36,510 The other thing you can do is indirectly view the eclipse. 32 00:01:36,510 --> 00:01:39,620 So you can do that by creating a pinhole projection. 33 00:01:39,620 --> 00:01:42,640 You can do that with your hands and create a little pinhole with your fingers there. 34 00:01:42,640 --> 00:01:45,820 You want to stand with the sun at your back. Let 35 00:01:45,820 --> 00:01:48,930 the sun shine through your pinhole and then 36 00:01:48,930 --> 00:01:52,130 the image of the sun and the moon taking a bite out of the sun 37 00:01:52,130 --> 00:01:55,220 will be projected down on the ground in front of 38 00:01:55,220 --> 00:01:58,240 you. 39 00:01:58,240 --> 00:02:01,330 Text on screen: For those in the path of totality - when is it safe to finally take off our solar glasses? 40 00:02:01,330 --> 00:02:04,390 You can take 41 00:02:04,390 --> 00:02:07,480 off your solar glasses when you don't see anything 42 00:02:07,480 --> 00:02:10,590 any longer. That means that the moon has 43 00:02:10,590 --> 00:02:13,750 blocked out the main body of the sun at the atmosphere around it 44 00:02:13,750 --> 00:02:16,950 is now visible. Then, as soon as you start to see 45 00:02:16,950 --> 00:02:20,130 the sun peeking around the moon again you need to put those 46 00:02:20,130 --> 00:02:23,140 glasses right back on. 47 00:02:23,140 --> 00:02:26,170 Text on screen: We're not in the path of totality - what interesting things should we lookout for? 48 00:02:26,170 --> 00:02:29,210 So if you're 49 00:02:29,210 --> 00:02:32,280 not in the path of totality and you're going to get a 50 00:02:32,280 --> 00:02:35,380 partial eclipse, that is still really amazing. What's going to happen is 51 00:02:35,380 --> 00:02:38,540 the moon is going to go across the sun and take a 52 00:02:38,540 --> 00:02:41,720 bite out of the sun, creating crescent shaped 53 00:02:41,720 --> 00:02:44,890 shadows and uh - you'll be able to see those with 54 00:02:44,890 --> 00:02:47,940 a pinhole projector. You can also see those 55 00:02:47,940 --> 00:02:51,010 even if you stand in front of a tree. The shadow as 56 00:02:51,010 --> 00:02:54,130 it goes through the tree - the tree acts like a pinhole projector - 57 00:02:54,130 --> 00:02:57,300 you'll get images of the 58 00:02:57,300 --> 00:03:00,490 moon going across the sun in the shadow 59 00:03:00,490 --> 00:03:03,670 of tree and you'll be able to see that. 60 00:03:03,670 --> 00:03:06,690 Text on screen: Why are you excited for this eclipse? 61 00:03:06,690 --> 00:03:09,850 62 00:03:09,850 --> 00:03:13,020 I am so excited about this eclipse because I 63 00:03:13,020 --> 00:03:16,220 study the solar corona. The solar corona is the part 64 00:03:16,220 --> 00:03:19,270 of the sun that we get to see during a total solar 65 00:03:19,270 --> 00:03:22,350 eclipse. It is the atmosphere of the sun and it's 66 00:03:22,350 --> 00:03:25,460 much less bright than the photosphere - the main body of the sun. 67 00:03:25,460 --> 00:03:28,620 So we usually don't get to see it. I get to 68 00:03:28,620 --> 00:03:31,790 study it with a NASA spacecraft that watches the sun all the 69 00:03:31,790 --> 00:03:34,990 time. But this total solar eclipse, getting to see it in person 70 00:03:34,990 --> 00:03:38,080 and getting to see it in this particular way, is so 71 00:03:38,080 --> 00:03:41,190 exciting to me. 72 00:03:41,190 --> 00:03:44,220 Text on screen: How can we watch the eclipse if the weather isn't on our side on August 21? 73 00:03:44,220 --> 00:03:47,290 74 00:03:47,290 --> 00:03:50,380 nasa.gov/eclipselive 75 00:03:50,380 --> 00:03:53,520 is doing live coverage of the 76 00:03:53,520 --> 00:03:56,720 eclipse - of the path of totality. We have stations 77 00:03:56,720 --> 00:03:59,910 all across the country watching the total solar 78 00:03:59,910 --> 00:04:02,980 eclipse, and we have airplane coverage of 79 00:04:02,980 --> 00:04:06,070 the total solar eclipse. So, whoever gets 80 00:04:06,070 --> 00:04:09,210 to see the eclipse, we will be covering and we'll have 81 00:04:09,210 --> 00:04:12,400 coverage of that. So if you're in the partial phases 82 00:04:12,400 --> 00:04:15,590 of the eclipse or if it was clouded out in your area, check us 83 00:04:15,590 --> 00:04:18,620 out and watch our live coverage of the eclipse. 84 00:04:18,620 --> 00:04:21,640 Text on screen: Why does an eclipse only last for a few minutes? 85 00:04:21,640 --> 00:04:24,840 86 00:04:24,840 --> 00:04:27,860 An eclipse 87 00:04:27,860 --> 00:04:31,060 only lasts for a couple of minutes because of the precise geometry. 88 00:04:31,060 --> 00:04:34,260 We have to get this perfect geometry - this perfect lineup 89 00:04:34,260 --> 00:04:37,330 between the sun, the moon and the Earth. And to get that 90 00:04:37,330 --> 00:04:40,470 to line up just exactly perfect, the shadow 91 00:04:40,470 --> 00:04:43,610 at a given place on the Earth only lasts a 92 00:04:43,610 --> 00:04:46,720 couple of minutes. 93 00:04:46,720 --> 00:04:49,760 Text on screen: What happens to Earth during the eclipse? 94 00:04:49,760 --> 00:04:52,960 95 00:04:52,960 --> 00:04:56,150 As the eclipse happens, it's effectively 96 00:04:56,150 --> 00:04:59,230 turning into night in just a small location 97 00:04:59,230 --> 00:05:02,340 on the Earth for just a brief period of time. 98 00:05:02,340 --> 00:05:05,360 And that's really strange. The atmosphere is 99 00:05:05,360 --> 00:05:08,560 going to respond and become cooler. 100 00:05:08,560 --> 00:05:11,750 The cloud coverage could change. The ionosphere 101 00:05:11,750 --> 00:05:14,800 could change. And we have um an App called Globe 102 00:05:14,800 --> 00:05:17,870 Observer App and we are encouraging citizen scientists to 103 00:05:17,870 --> 00:05:20,970 tell us what is going on - what they are observing 104 00:05:20,970 --> 00:05:24,130 as the eclipse is happening. So if you have a thermometer 105 00:05:24,130 --> 00:05:27,330 and get the Globe Observer App on your phone then 106 00:05:27,330 --> 00:05:30,520 you too can be a citizen scientist and help NASA 107 00:05:30,520 --> 00:05:33,580 collect data on how the Earth is responding 108 00:05:33,580 --> 00:05:36,670 to the eclipse. 109 00:05:36,670 --> 00:05:39,870 Text on screen: If you were looking back at Earth during the eclipse what would you see? 110 00:05:39,870 --> 00:05:43,010 111 00:05:43,010 --> 00:05:46,200 In fact we do 112 00:05:46,200 --> 00:05:49,380 look back at the Earth during the eclipse. 113 00:05:49,380 --> 00:05:52,430 Uh - spacecraft, one of them is called DSCOVR, 114 00:05:52,430 --> 00:05:55,490 and it sits in-between the sun and the Earth, watching 115 00:05:55,490 --> 00:05:58,570 the Earth and it will watch the eclipse as it happens. 116 00:05:58,570 --> 00:06:01,670 It will watch the shadow of the moon cast 117 00:06:01,670 --> 00:06:04,840 across the Earth and go across the Earth. 118 00:06:04,840 --> 00:06:08,030 The Lunar Reconnaissance Orbiter is another mission that usually watches 119 00:06:08,030 --> 00:06:11,230 the moon, but for this eclipse it is going to point and look 120 00:06:11,230 --> 00:06:14,290 at the Earth and watch the shadow of the moon go across the Earth. 121 00:06:14,290 --> 00:06:17,390 And the International Space Station is also going to get to see 122 00:06:17,390 --> 00:06:20,540 the shadow of the moon across the Earth. 123 00:06:20,540 --> 00:06:23,580 124 00:06:23,580 --> 00:06:26,590 Text on screen: How has our precise mapping of the moon helped us predict the path of eclipses? 125 00:06:26,590 --> 00:06:29,770 The Lunar Reconnaissance 126 00:06:29,770 --> 00:06:32,960 Orbiter has taken very precise measurements of the 127 00:06:32,960 --> 00:06:36,030 moon. It has precise measurements of the topography - 128 00:06:36,030 --> 00:06:39,140 the mountains, the valleys, the craters. Because the moon 129 00:06:39,140 --> 00:06:42,330 is not a perfect sphere, and so that shadow that it casts down 130 00:06:42,330 --> 00:06:45,510 onto the Earth is not a perfect circle. The details of 131 00:06:45,510 --> 00:06:48,700 the topography are what help us know exactly what that shadow is 132 00:06:48,700 --> 00:06:51,790 going to look like when it hits the Earth. 133 00:06:51,790 --> 00:06:54,820 Text on screen: Where can we learn more? 134 00:06:54,820 --> 00:06:58,010 135 00:06:58,010 --> 00:07:01,100 You can learn more at 136 00:07:01,100 --> 00:07:04,210 eclipse2017.nasa.gov - that's where we have 137 00:07:04,210 --> 00:07:07,360 all sorts of information. Everything from safety, 138 00:07:07,360 --> 00:07:10,550 to detailed maps of what you're going to see in 139 00:07:10,550 --> 00:07:13,720 your area. We also have 140 00:07:13,720 --> 00:07:16,760 event information, uh, local 141 00:07:16,760 --> 00:07:19,840 libraries, zoos, museums, things like that, are hosting 142 00:07:19,840 --> 00:07:22,950 eclipse parties. And you can find out what events 143 00:07:22,950 --> 00:07:26,110 are going on in your area. 144 00:07:26,110 --> 00:07:26,463