1 00:00:06,389 --> 00:00:04,070 from a spy glass to satellites our 2 00:00:09,430 --> 00:00:06,399 backyard to the very edge of our solar 3 00:00:11,350 --> 00:00:09,440 system every culture on every continent 4 00:00:12,870 --> 00:00:11,360 has observed the sun 5 00:00:15,190 --> 00:00:12,880 we have been searching for the answers 6 00:00:17,269 --> 00:00:15,200 to the mysteries of time and the seasons 7 00:00:19,429 --> 00:00:17,279 the web of life on earth 8 00:00:21,750 --> 00:00:19,439 and our place in the universe 9 00:00:23,750 --> 00:00:21,760 our sun has always been more than a ball 10 00:00:25,750 --> 00:00:23,760 of heat and light 11 00:00:28,390 --> 00:00:25,760 our sun through curious minds and 12 00:00:30,630 --> 00:00:28,400 innovative technology has allowed us to 13 00:00:33,510 --> 00:00:30,640 explore how the northern lights dance 14 00:00:50,790 --> 00:00:33,520 and how our solar system may have formed 15 00:00:55,270 --> 00:00:52,869 before sophisticated satellites brought 16 00:00:58,069 --> 00:00:55,280 us vibrant images and wavelengths beyond 17 00:00:59,110 --> 00:00:58,079 our senses people simply looked at the 18 00:01:01,430 --> 00:00:59,120 sun 19 00:01:05,030 --> 00:01:01,440 although he was not alone in his pursuit 20 00:01:07,590 --> 00:01:05,040 in 1609 galileo galilei pioneered the 21 00:01:10,950 --> 00:01:07,600 use of the telescope in order to observe 22 00:01:16,789 --> 00:01:13,350 his detailed sketches produced over the 23 00:01:19,190 --> 00:01:16,799 summer in 1612 revealed that the sun was 24 00:01:23,510 --> 00:01:19,200 not a static orb in the sky but a 25 00:01:28,310 --> 00:01:26,070 galileo's solar discoveries sparked an 26 00:01:29,990 --> 00:01:28,320 academic interest in the sun leading 27 00:01:32,390 --> 00:01:30,000 astronomers around the world to 28 00:01:33,670 --> 00:01:32,400 investigate how the sun shapes life on 29 00:01:35,990 --> 00:01:33,680 earth 30 00:01:38,710 --> 00:01:36,000 400 years later astronomers with 31 00:01:40,870 --> 00:01:38,720 increasingly complex satellite imagers 32 00:01:48,630 --> 00:01:40,880 investigate the origins and effects of 33 00:01:52,870 --> 00:01:50,789 there must be something in a sunspot 34 00:01:54,710 --> 00:01:52,880 that opens up a wealth of knowledge and 35 00:01:56,789 --> 00:01:54,720 even more questions 36 00:01:59,190 --> 00:01:56,799 like galileo before him german 37 00:02:01,670 --> 00:01:59,200 astronomer samuel heinrich schwab became 38 00:02:04,709 --> 00:02:01,680 fascinated with sunspots from careful 39 00:02:07,030 --> 00:02:04,719 observation over 17 years schwab found a 40 00:02:08,389 --> 00:02:07,040 periodic cycling of the average number 41 00:02:10,469 --> 00:02:08,399 of sunspots 42 00:02:12,470 --> 00:02:10,479 in the mid-1800s he and other 43 00:02:15,030 --> 00:02:12,480 astronomers found that the sun has about 44 00:02:16,949 --> 00:02:15,040 an 11-year cycle between the times when 45 00:02:18,390 --> 00:02:16,959 we can observe the most and the least 46 00:02:20,550 --> 00:02:18,400 sunspots 47 00:02:22,550 --> 00:02:20,560 understanding the 11-year solar cycle 48 00:02:24,229 --> 00:02:22,560 becomes very crucial in understanding 49 00:02:26,630 --> 00:02:24,239 the effects of space weather here at 50 00:02:29,030 --> 00:02:26,640 earth because it really dictates how 51 00:02:40,949 --> 00:02:29,040 often solar storms will occur and how 52 00:02:45,589 --> 00:02:43,270 we often underestimate how beautiful a 53 00:02:47,430 --> 00:02:45,599 scientific discovery can be 54 00:02:50,070 --> 00:02:47,440 when the themis satellite fleet launched 55 00:02:53,110 --> 00:02:50,080 in 2007 the mission set out to 56 00:02:55,430 --> 00:02:53,120 investigate what triggers substorms 57 00:02:57,589 --> 00:02:55,440 substorms are atmospheric events visible 58 00:02:59,830 --> 00:02:57,599 in the northern hemisphere as a sudden 59 00:03:03,589 --> 00:02:59,840 brightening of the northern lights or 60 00:03:09,430 --> 00:03:06,949 one such substorm in march 2008 produced 61 00:03:12,949 --> 00:03:09,440 lightning fast aurora with the energy of 62 00:03:17,110 --> 00:03:14,949 nasa scientists found the answer to this 63 00:03:20,229 --> 00:03:17,120 mysterious behavior and massive energy 64 00:03:22,869 --> 00:03:20,239 in giant magnetic ropes 65 00:03:24,550 --> 00:03:22,879 these can be as wide as the earth itself 66 00:03:26,390 --> 00:03:24,560 serve as conduits for solar wind 67 00:03:28,710 --> 00:03:26,400 particles which collide with the earth's 68 00:03:31,910 --> 00:03:28,720 magnetic field and charge the 69 00:03:33,589 --> 00:03:31,920 spectacular substorms and auroras these 70 00:03:35,270 --> 00:03:33,599 ropes are evidence of a direct 71 00:03:37,430 --> 00:03:35,280 connection between the sun and the 72 00:03:39,910 --> 00:03:37,440 earth's upper atmosphere 73 00:03:41,990 --> 00:03:39,920 it is when these ropes form and unravel 74 00:03:44,229 --> 00:03:42,000 that the highly energetic solar wind 75 00:03:46,470 --> 00:03:44,239 ignites the earth's magnetic field and 76 00:03:48,789 --> 00:03:46,480 lights up the northern sky providing a 77 00:04:02,229 --> 00:03:48,799 celestial dance that has captivated 78 00:04:06,390 --> 00:04:04,470 sometimes a great discovery is a new 79 00:04:09,509 --> 00:04:06,400 perspective on the universe we thought 80 00:04:13,589 --> 00:04:11,350 as the voyager spacecraft's near the 81 00:04:16,310 --> 00:04:13,599 edge of our sun's reach scientists are 82 00:04:19,590 --> 00:04:16,320 getting a new look at the expanse and 83 00:04:22,469 --> 00:04:19,600 shape of the solar system 84 00:04:27,430 --> 00:04:22,479 over 30 years ago voyager 1 and 2 set 85 00:04:31,670 --> 00:04:29,510 now as the twin spacecrafts explore the 86 00:04:33,749 --> 00:04:31,680 outer reaches some nine billion miles 87 00:04:36,310 --> 00:04:33,759 away from earth they have crossed the 88 00:04:39,909 --> 00:04:36,320 heliosphere the bubble of supersonic 89 00:04:43,749 --> 00:04:41,909 however when voyager 2 crossed this 90 00:04:46,150 --> 00:04:43,759 boundary much closer to the sun than 91 00:04:48,870 --> 00:04:46,160 expected we received a picture of a 92 00:04:50,070 --> 00:04:48,880 squashed heliosphere rather than a round 93 00:04:51,590 --> 00:04:50,080 bubble 94 00:04:53,670 --> 00:04:51,600 the squashed heliosphere helps 95 00:04:56,150 --> 00:04:53,680 scientists build up a picture of how the 96 00:04:58,150 --> 00:04:56,160 sun interacts with the space outside of 97 00:05:00,310 --> 00:04:58,160 our solar system 98 00:05:02,469 --> 00:05:00,320 when the recently launched ibex or 99 00:05:04,870 --> 00:05:02,479 interstellar boundary explorer reaches 100 00:05:06,390 --> 00:05:04,880 the very distant limits it will further 101 00:05:08,710 --> 00:05:06,400 the study of how the solar wind 102 00:05:17,430 --> 00:05:08,720 interacts with the cold gas between 103 00:05:21,670 --> 00:05:19,510 it's hard to imagine weather being more 104 00:05:22,790 --> 00:05:21,680 than rain on our weekend or ice on our 105 00:05:25,510 --> 00:05:22,800 roads 106 00:05:27,749 --> 00:05:25,520 but space weather can affect the globe 107 00:05:29,510 --> 00:05:27,759 especially in the way we communicate and 108 00:05:31,270 --> 00:05:29,520 power our world 109 00:05:33,590 --> 00:05:31,280 space weather is the environmental 110 00:05:35,670 --> 00:05:33,600 conditions outside of our planet 111 00:05:38,230 --> 00:05:35,680 originating from the massively energetic 112 00:05:40,469 --> 00:05:38,240 output of the sun the solar wind is 113 00:05:42,390 --> 00:05:40,479 primarily comprised of protons and 114 00:05:44,469 --> 00:05:42,400 electrons they're streaming outward from 115 00:05:47,029 --> 00:05:44,479 the sun at speeds of up to a million 116 00:05:50,710 --> 00:05:47,039 miles an hour and they're constantly 117 00:05:52,390 --> 00:05:50,720 bombarding the earth's magnetic field 118 00:05:55,029 --> 00:05:52,400 satellites have been launched to study 119 00:06:01,510 --> 00:05:55,039 solar wind solar flares coronal mass 120 00:06:07,510 --> 00:06:03,909 these phenomena impact our atmosphere 121 00:06:10,230 --> 00:06:07,520 sometimes with devastating force 122 00:06:13,029 --> 00:06:10,240 so space weather includes power outages 123 00:06:15,430 --> 00:06:13,039 in high latitude power grids includes 124 00:06:17,590 --> 00:06:15,440 disruption of spacecraft includes 125 00:06:18,469 --> 00:06:17,600 radiation that can harm astronauts in 126 00:06:21,990 --> 00:06:18,479 space 127 00:06:23,990 --> 00:06:22,000 with any weather prediction is the goal 128 00:06:26,150 --> 00:06:24,000 these missions will all add to the