1 00:00:13,430 --> 00:00:11,030 between the earth and the sun we tend to 2 00:00:15,110 --> 00:00:13,440 imagine empty space 3 00:00:18,390 --> 00:00:15,120 but every day 4 00:00:23,269 --> 00:00:18,400 every moment solar forces fill the void 5 00:00:28,070 --> 00:00:25,429 the grey mesh you see here is the 6 00:00:30,470 --> 00:00:28,080 magnetosphere it's effectively a bubble 7 00:00:33,430 --> 00:00:30,480 around the earth created by our planet's 8 00:00:35,910 --> 00:00:33,440 magnetic field squashed and elongated as 9 00:00:37,430 --> 00:00:35,920 intensely energized solar particles 10 00:00:39,990 --> 00:00:37,440 collide with it without the 11 00:00:40,869 --> 00:00:40,000 magnetosphere life on earth would likely 12 00:00:42,869 --> 00:00:40,879 cease 13 00:00:45,510 --> 00:00:42,879 naturally we want to know more about it 14 00:00:47,750 --> 00:00:45,520 so let's start close to home 15 00:00:50,069 --> 00:00:47,760 these near-earth satellites monitor 16 00:00:52,470 --> 00:00:50,079 solar activity interactions with our 17 00:00:54,150 --> 00:00:52,480 planet's atmosphere and other aspects of 18 00:00:55,830 --> 00:00:54,160 the sun's condition 19 00:00:58,389 --> 00:00:55,840 you'll notice how they orbit the earth 20 00:00:59,430 --> 00:00:58,399 quickly about once every 90 minutes or 21 00:01:01,910 --> 00:00:59,440 so 22 00:01:03,830 --> 00:01:01,920 remember this because the rate of times 23 00:01:06,550 --> 00:01:03,840 passage will change as we move through 24 00:01:08,789 --> 00:01:06,560 the solar system 25 00:01:10,469 --> 00:01:08,799 further away we see satellites measuring 26 00:01:12,710 --> 00:01:10,479 the three-dimensional boundaries of the 27 00:01:14,870 --> 00:01:12,720 magnetosphere as it interacts with the 28 00:01:17,270 --> 00:01:14,880 solar wind 29 00:01:19,109 --> 00:01:17,280 and let's be clear this is more than an 30 00:01:21,270 --> 00:01:19,119 academic exercise 31 00:01:23,670 --> 00:01:21,280 nasa's fleet of research satellites 32 00:01:26,149 --> 00:01:23,680 gathers vital information solar 33 00:01:27,910 --> 00:01:26,159 phenomena can jeopardize astronauts and 34 00:01:29,830 --> 00:01:27,920 provoke dramatic challenges to 35 00:01:32,789 --> 00:01:29,840 communications systems and the 36 00:01:35,749 --> 00:01:32,799 electrical grid on the ground 37 00:01:37,910 --> 00:01:35,759 time speeds up as we move out more space 38 00:01:40,069 --> 00:01:37,920 between objects means we have to travel 39 00:01:43,510 --> 00:01:40,079 greater distances and our tour of the 40 00:01:45,270 --> 00:01:43,520 heliosphere only lasts a few minutes 41 00:01:47,030 --> 00:01:45,280 while we're traveling take note of 42 00:01:48,069 --> 00:01:47,040 something you might not have considered 43 00:01:50,710 --> 00:01:48,079 before 44 00:01:53,270 --> 00:01:50,720 not all orbits look the same 45 00:01:54,630 --> 00:01:53,280 in close satellite paths essentially 46 00:01:57,030 --> 00:01:54,640 circle the earth 47 00:01:59,590 --> 00:01:57,040 but farther away we begin to encounter a 48 00:02:01,429 --> 00:01:59,600 wider variety of orbits designed for 49 00:02:03,350 --> 00:02:01,439 varying purposes 50 00:02:05,190 --> 00:02:03,360 the cluster vehicles are on a high 51 00:02:09,029 --> 00:02:05,200 elliptical flight path 52 00:02:11,270 --> 00:02:09,039 geotale makes a lazy loop all alone 53 00:02:13,589 --> 00:02:11,280 the two stereo satellites fly in 54 00:02:15,910 --> 00:02:13,599 relatively close formation but they 55 00:02:18,070 --> 00:02:15,920 won't stay that way for long 56 00:02:20,869 --> 00:02:18,080 i'll show you how in a moment but the 57 00:02:24,229 --> 00:02:20,879 point is navigation out here is harder 58 00:02:26,470 --> 00:02:24,239 than it looks a vehicle can't simply fly 59 00:02:29,830 --> 00:02:26,480 from place to place but for some 60 00:02:31,910 --> 00:02:29,840 missions like stereo precise position 61 00:02:32,869 --> 00:02:31,920 makes all the difference 62 00:02:35,350 --> 00:02:32,879 why 63 00:02:38,070 --> 00:02:35,360 the two stereo satellites will deliver 64 00:02:41,350 --> 00:02:38,080 3d pictures of the sun similar to the 65 00:02:43,190 --> 00:02:41,360 way your two eyes perceive 3d 66 00:02:45,190 --> 00:02:43,200 remember i said to keep an eye on 67 00:02:47,670 --> 00:02:45,200 stereo's flight path 68 00:02:49,589 --> 00:02:47,680 watch as one of the two stereo vehicles 69 00:02:50,550 --> 00:02:49,599 intercepts the moon's orbit a second 70 00:02:52,150 --> 00:02:50,560 time 71 00:02:53,750 --> 00:02:52,160 here it comes 72 00:02:55,990 --> 00:02:53,760 as they close the distance the 73 00:02:58,630 --> 00:02:56,000 spacecraft uses the moon's gravity to 74 00:03:00,869 --> 00:02:58,640 execute a cool maneuver like a roller 75 00:03:03,190 --> 00:03:00,879 coaster zooming up and into a corkscrew 76 00:03:04,869 --> 00:03:03,200 just after hitting a big drop 77 00:03:06,390 --> 00:03:04,879 now the vehicles are headed to their 78 00:03:08,470 --> 00:03:06,400 final orbits 79 00:03:11,190 --> 00:03:08,480 tight loops around the earth loose 80 00:03:13,910 --> 00:03:11,200 orbits out into space bank shots off the 81 00:03:16,710 --> 00:03:13,920 moon there are many ways to travel from 82 00:03:20,309 --> 00:03:16,720 place to place but sometimes travel is 83 00:03:22,470 --> 00:03:20,319 not the goal sometimes it pays to park 84 00:03:25,350 --> 00:03:22,480 welcome to a lagrange point 85 00:03:27,350 --> 00:03:25,360 this one l1 in space speak denotes a 86 00:03:29,589 --> 00:03:27,360 relative position between the earth and 87 00:03:32,550 --> 00:03:29,599 the sun where the gravitational pull of 88 00:03:35,589 --> 00:03:32,560 each object is in approximate balance 89 00:03:37,750 --> 00:03:35,599 these so-called halo orbits around l1 90 00:03:40,070 --> 00:03:37,760 make good places for hovering spacecraft 91 00:03:41,190 --> 00:03:40,080 to take observations of either the earth 92 00:03:42,949 --> 00:03:41,200 or sun 93 00:03:44,550 --> 00:03:42,959 we find a number of observatories 94 00:03:46,710 --> 00:03:44,560 patrolling out here 95 00:03:49,110 --> 00:03:46,720 including an extremely famous and 96 00:03:50,550 --> 00:03:49,120 extremely successful solar observatory 97 00:03:52,949 --> 00:03:50,560 called soho 98 00:03:55,509 --> 00:03:52,959 notice how l1 exists well in front of 99 00:03:58,149 --> 00:03:55,519 the magnetosphere this part of the solar 100 00:03:59,750 --> 00:03:58,159 system is fully bathed in the solar wind 101 00:04:01,190 --> 00:03:59,760 without the protection of earth's 102 00:04:03,429 --> 00:04:01,200 magnetic shield 103 00:04:05,589 --> 00:04:03,439 therefore it's extremely useful for 104 00:04:10,789 --> 00:04:05,599 studying solar activity without 105 00:04:16,069 --> 00:04:13,030 let's briefly revisit the area around 106 00:04:18,710 --> 00:04:16,079 the earth simulated time slows again as 107 00:04:20,870 --> 00:04:18,720 the distance between objects shrinks 108 00:04:23,030 --> 00:04:20,880 but as we once again approach our home 109 00:04:24,550 --> 00:04:23,040 you'll notice the calendar has advanced 110 00:04:26,629 --> 00:04:24,560 two years 111 00:04:29,270 --> 00:04:26,639 new satellites have entered the dance 112 00:04:31,030 --> 00:04:29,280 including the five themis vehicles 113 00:04:33,749 --> 00:04:31,040 the near-earth fleet of satellites 114 00:04:35,990 --> 00:04:33,759 swarms like bees around a hive some 115 00:04:37,990 --> 00:04:36,000 ranging out beyond the magnetosphere 116 00:04:40,310 --> 00:04:38,000 some well inside 117 00:04:42,870 --> 00:04:40,320 it's provocative to consider that all 118 00:04:46,150 --> 00:04:42,880 this activity takes place in space 119 00:04:49,110 --> 00:04:46,160 something we generally perceive as empty 120 00:04:51,590 --> 00:04:49,120 but what we find instead from light to 121 00:04:53,909 --> 00:04:51,600 charged particles to magnetic fields 122 00:04:55,830 --> 00:04:53,919 demonstrates a strange and wonderful 123 00:04:57,990 --> 00:04:55,840 solar vitality 124 00:04:59,830 --> 00:04:58,000 in fact there's a particular scientific 125 00:05:01,350 --> 00:04:59,840 discipline that describes the study of 126 00:05:03,990 --> 00:05:01,360 these things 127 00:05:06,310 --> 00:05:04,000 it's heliophysics from the greek word 128 00:05:08,830 --> 00:05:06,320 for sun combined with the word used to 129 00:05:11,350 --> 00:05:08,840 describe the study of matter and 130 00:05:13,749 --> 00:05:11,360 energy heliophysics studies how the 131 00:05:16,390 --> 00:05:13,759 sun's sphere of influence interacts with 132 00:05:19,350 --> 00:05:16,400 planets and the interstellar medium the 133 00:05:22,790 --> 00:05:19,360 barely tangible stuff that fills what we 134 00:05:25,029 --> 00:05:22,800 typically regard as empty space 135 00:05:26,790 --> 00:05:25,039 almost done but we've got to get moving 136 00:05:29,029 --> 00:05:26,800 if we're going to see the full extent of 137 00:05:31,510 --> 00:05:29,039 the sun's influence 138 00:05:34,469 --> 00:05:31,520 pulling way way back earth's 139 00:05:36,950 --> 00:05:34,479 magnetosphere effectively disappears 140 00:05:39,670 --> 00:05:36,960 almost all of our solar observing fleet 141 00:05:43,189 --> 00:05:39,680 shrinks like boats on the horizon 142 00:05:46,710 --> 00:05:43,199 almost but not all 143 00:05:49,749 --> 00:05:46,720 two legendary spacecraft voyager 1 and 2 144 00:05:51,830 --> 00:05:49,759 are out there still taking measurements 145 00:05:53,670 --> 00:05:51,840 notice the gravity assist bank shots and 146 00:05:57,110 --> 00:05:53,680 their flight paths 147 00:05:59,430 --> 00:05:57,120 launched in 1977 the voyager spacecraft 148 00:06:01,749 --> 00:05:59,440 are the most distant artifacts humanity 149 00:06:05,029 --> 00:06:01,759 has ever cast out into space 150 00:06:07,110 --> 00:06:05,039 time capsules from a small blue planet 151 00:06:09,430 --> 00:06:07,120 they are also the first human objects to 152 00:06:11,670 --> 00:06:09,440 encounter the sun's termination shock 153 00:06:13,430 --> 00:06:11,680 the area where the solar wind slows down 154 00:06:15,430 --> 00:06:13,440 enough to be affected by the flow of 155 00:06:17,110 --> 00:06:15,440 interstellar particles 156 00:06:18,790 --> 00:06:17,120 in a couple of decades one of the 157 00:06:21,189 --> 00:06:18,800 voyager crafts should pass the 158 00:06:23,749 --> 00:06:21,199 heliopause the zone where the sun's 159 00:06:25,270 --> 00:06:23,759 influence meets the interstellar medium 160 00:06:27,830 --> 00:06:25,280 years later it should encounter the 161 00:06:29,990 --> 00:06:27,840 so-called bow shock that's the wake in 162 00:06:31,830 --> 00:06:30,000 flowing interstellar particles as they 163 00:06:34,629 --> 00:06:31,840 move around the bubble of energy and 164 00:06:37,189 --> 00:06:34,639 particles emanating from our star 165 00:06:39,670 --> 00:06:37,199 our star the sun 166 00:06:41,029 --> 00:06:39,680 neither particularly large nor powerful 167 00:06:43,350 --> 00:06:41,039 as stars go 168 00:06:45,670 --> 00:06:43,360 stretches itself out further than even 169 00:06:47,909 --> 00:06:45,680 our most distant probes 170 00:06:50,309 --> 00:06:47,919 as we discover how to coexist with our 171 00:06:53,270 --> 00:06:50,319 own solar dynamo we stretch our