1 00:00:08,019 --> 00:00:05,830 people have been observing the Sun for 2 00:00:10,299 --> 00:00:08,029 thousands of years many cultures 3 00:00:12,489 --> 00:00:10,309 believed in a Sun Goddess and they 4 00:00:14,850 --> 00:00:12,499 thought of the Sun as the perfect object 5 00:00:17,170 --> 00:00:14,860 as soon as the telescope was invented 6 00:00:19,330 --> 00:00:17,180 people pointed it pretty much anything 7 00:00:20,860 --> 00:00:19,340 they could think of and they discovered 8 00:00:23,820 --> 00:00:20,870 that the Sun is actually not that 9 00:00:26,290 --> 00:00:23,830 perfect they were able to see sunspots 10 00:00:29,110 --> 00:00:26,300 today we know that the Sun is very 11 00:00:31,780 --> 00:00:29,120 dynamic and it has the largest eruptions 12 00:00:34,060 --> 00:00:31,790 in the solar system it's important for 13 00:00:36,819 --> 00:00:34,070 us to be able to predict solar weather 14 00:00:39,220 --> 00:00:36,829 using NASA satellites to help us look 15 00:00:42,369 --> 00:00:39,230 inside the Sun and better understand 16 00:00:45,040 --> 00:00:42,379 this giant violent star without the Sun 17 00:00:47,319 --> 00:00:45,050 life on the wouldn't exist the Sun is 18 00:00:50,079 --> 00:00:47,329 the big anchor that keeps our planet and 19 00:00:53,559 --> 00:00:50,089 the other planets of the solar system in 20 00:00:55,270 --> 00:00:53,569 a small area of space rather than just 21 00:00:57,340 --> 00:00:55,280 flying off into the rest of the universe 22 00:00:58,569 --> 00:00:57,350 since this is part of our everyday life 23 00:01:00,430 --> 00:00:58,579 I think this is something very 24 00:01:11,410 --> 00:01:00,440 fundamental to mankind just to 25 00:01:14,109 --> 00:01:11,420 understand what we are looking at hi my 26 00:01:16,690 --> 00:01:14,119 name is my Jordan and I'm student here 27 00:01:19,719 --> 00:01:16,700 at Parkland magnet Middle School in 28 00:01:22,060 --> 00:01:19,729 Rockville Maryland one of the cool 29 00:01:25,569 --> 00:01:22,070 things we study in astronomy class is 30 00:01:27,370 --> 00:01:25,579 actually the Sun and how we study it is 31 00:01:29,380 --> 00:01:27,380 we use the Sun spotter 32 00:01:33,069 --> 00:01:29,390 the Sun spotters actually show you a 33 00:01:35,289 --> 00:01:33,079 flexion or shadow of the Sun and you 34 00:01:39,010 --> 00:01:35,299 trace it and then over time we collect 35 00:01:42,300 --> 00:01:39,020 the papers and we can compare them to 36 00:01:46,050 --> 00:01:42,310 see how the sunspot heptane 37 00:01:48,139 --> 00:01:46,060 they move sunspots are regions on the 38 00:01:50,810 --> 00:01:48,149 Sun that are cooler than the surrounding 39 00:01:54,779 --> 00:01:50,820 areas in the sun's photosphere 40 00:01:57,630 --> 00:01:54,789 ruk is that the Sun yet we were so we 41 00:01:59,460 --> 00:01:57,640 invited NASA scientists 10 and Daniel to 42 00:02:00,840 --> 00:01:59,470 come and talk with the students about 43 00:02:02,669 --> 00:02:00,850 the Sun and help them with their 44 00:02:06,570 --> 00:02:02,679 calculations you know how to average 45 00:02:08,279 --> 00:02:06,580 these numbers together the final mean 46 00:02:10,169 --> 00:02:08,289 you add these numbers up and divide by 47 00:02:12,330 --> 00:02:10,179 the number of numbers the Sun is an 48 00:02:15,330 --> 00:02:12,340 active star that goes through regular 49 00:02:17,970 --> 00:02:15,340 cycles of maximum and minimum activity 50 00:02:20,250 --> 00:02:17,980 the students are calculating the solar 51 00:02:23,009 --> 00:02:20,260 maximum and solar minimum by looking at 52 00:02:25,320 --> 00:02:23,019 data over the last 50 years that covers 53 00:02:27,539 --> 00:02:25,330 how many sunspots occurred during every 54 00:02:29,550 --> 00:02:27,549 decade and it's and some of the really 55 00:02:30,780 --> 00:02:29,560 big sunspots you can easily see if you 56 00:02:33,630 --> 00:02:30,790 look at the Sun with the naked eye 57 00:02:36,300 --> 00:02:33,640 they're that big I think these sunspots 58 00:02:39,000 --> 00:02:36,310 were about you know 30 times as big as 59 00:02:42,690 --> 00:02:39,010 the earth they were just huge exactly 60 00:02:45,630 --> 00:02:42,700 how walking sunspots you look at the 61 00:02:46,890 --> 00:02:45,640 surface of the Sun and it's about 5,700 62 00:02:49,770 --> 00:02:46,900 degrees Kelvin 63 00:02:53,340 --> 00:02:49,780 I think the coolest sunspot goes down 64 00:02:56,160 --> 00:02:53,350 maybe 2000 to 2500 degrees cooler than 65 00:03:00,060 --> 00:02:56,170 that one of the most important things is 66 00:03:01,710 --> 00:03:00,070 that the Sun is a star it's the nearest 67 00:03:03,870 --> 00:03:01,720 example that we have in the entire 68 00:03:05,370 --> 00:03:03,880 universe what those little points of 69 00:03:08,250 --> 00:03:05,380 light in the sky are that we see at 70 00:03:09,660 --> 00:03:08,260 night the Sun is a very dynamic star and 71 00:03:11,520 --> 00:03:09,670 it changes all the time 72 00:03:14,640 --> 00:03:11,530 did you know it has the largest 73 00:03:17,220 --> 00:03:14,650 eruptions in all of the solar system we 74 00:03:19,380 --> 00:03:17,230 call these coronal mass ejections and 75 00:03:22,050 --> 00:03:19,390 they have an impact on us here on earth 76 00:03:24,210 --> 00:03:22,060 that's called solar weather in looking 77 00:03:26,340 --> 00:03:24,220 at that image do you guys have a 78 00:03:29,460 --> 00:03:26,350 prediction about which of those areas 79 00:03:35,190 --> 00:03:29,470 would be most likely to cause a coronal 80 00:03:37,849 --> 00:03:35,200 mass ejection yeah okay over here sir we 81 00:03:40,289 --> 00:03:37,859 care about solar weather because any 82 00:03:43,170 --> 00:03:40,299 communication devices that rely on 83 00:03:45,270 --> 00:03:43,180 transmitting information continuously 84 00:03:46,830 --> 00:03:45,280 can be affected high-precision 85 00:03:48,830 --> 00:03:46,840 electronics like electronics for 86 00:03:51,770 --> 00:03:48,840 high-speed trains can be affected by it 87 00:03:53,990 --> 00:03:51,780 and since high-speed train at 200 miles 88 00:03:57,199 --> 00:03:54,000 per hour is it is a pretty dangerous 89 00:03:59,960 --> 00:03:57,209 thing if it just runs loose so we want 90 00:04:01,940 --> 00:03:59,970 to know what's going on here the earth 91 00:04:04,280 --> 00:04:01,950 has its own way of protecting us from 92 00:04:06,259 --> 00:04:04,290 solar storms and solar weather it's 93 00:04:09,199 --> 00:04:06,269 something called a magnetic field you 94 00:04:13,040 --> 00:04:09,209 can imagine the earth magnetic field a 95 00:04:16,759 --> 00:04:13,050 bit like an egg shell around neck so 96 00:04:18,440 --> 00:04:16,769 without this shell we would be fried and 97 00:04:20,780 --> 00:04:18,450 what about if we were on the moon yeah 98 00:04:22,879 --> 00:04:20,790 if you're on the moon you would be fried 99 00:04:25,070 --> 00:04:22,889 as well so what you would have to do is 100 00:04:28,190 --> 00:04:25,080 go in your little spaceship wait until 101 00:04:29,960 --> 00:04:28,200 the storm is over today scientists are 102 00:04:32,750 --> 00:04:29,970 learning about solar weather using 103 00:04:35,030 --> 00:04:32,760 satellites that go around the Sun one of 104 00:04:37,790 --> 00:04:35,040 those satellites Soho is celebrating its 105 00:04:40,940 --> 00:04:37,800 10-year anniversary European Space 106 00:04:43,879 --> 00:04:40,950 Agency scientists Daniel came in to tell 107 00:04:45,680 --> 00:04:43,889 us how the Soho satellite is unique when 108 00:04:48,740 --> 00:04:45,690 compared to other satellites that use 109 00:04:51,860 --> 00:04:48,750 silver data the satellite the spacecraft 110 00:04:53,420 --> 00:04:51,870 contains twelve different experiments so 111 00:04:56,270 --> 00:04:53,430 we collect images of the Sun in 112 00:04:58,820 --> 00:04:56,280 different colors or different wavelength 113 00:05:00,350 --> 00:04:58,830 it is just very fascinating to look at 114 00:05:02,330 --> 00:05:00,360 the Sun and if you look at these images 115 00:05:04,670 --> 00:05:02,340 you'll see the Sun as most of us have 116 00:05:07,540 --> 00:05:04,680 never seen it before and you realize 117 00:05:10,760 --> 00:05:07,550 that this is a star that is violent and 118 00:05:12,800 --> 00:05:10,770 dynamic before the launch of Soho all we 119 00:05:15,529 --> 00:05:12,810 knew about space weather was from 120 00:05:19,730 --> 00:05:15,539 satellites in near Earth orbit and now 121 00:05:21,770 --> 00:05:19,740 we actually see the origin of stormy 122 00:05:24,640 --> 00:05:21,780 weather out in space this way we get a 123 00:05:29,000 --> 00:05:24,650 two to three days notice for 124 00:05:31,879 --> 00:05:29,010 disturbances that propagate to us and so 125 00:05:33,620 --> 00:05:31,889 the phrase that NASA invented that we 126 00:05:35,900 --> 00:05:33,630 are living with a star is actually true 127 00:05:37,070 --> 00:05:35,910 since this is part of our everyday life 128 00:05:38,930 --> 00:05:37,080 I think this is something very 129 00:05:41,690 --> 00:05:38,940 fundamental to mankind just to 130 00:05:44,330 --> 00:05:41,700 understand what we are looking at our 131 00:05:46,219 --> 00:05:44,340 teachers tell us every day that there 132 00:05:49,400 --> 00:05:46,229 are less and less scientists to discover 133 00:05:53,540 --> 00:05:49,410 new things when I go to college I am 134 00:05:56,570 --> 00:05:53,550 going to major in aerospace engineering 135 00:05:58,280 --> 00:05:56,580 and hopefully I will get a job for NASA 136 00:06:00,740 --> 00:05:58,290 and the 137 00:06:03,230 --> 00:06:00,750 spacecraft my personal goal is I just 138 00:06:04,730 --> 00:06:03,240 love to instill in them curiosity 139 00:06:06,830 --> 00:06:04,740 so I hope I'm raising the next 140 00:06:09,710 --> 00:06:06,840 generation of scientists and I hope that