1 00:00:05,349 --> 00:00:03,030 there's one thing that stands between us 2 00:00:07,430 --> 00:00:05,359 and the harsh environment of space our 3 00:00:10,549 --> 00:00:07,440 atmosphere the part of earth that 4 00:00:12,709 --> 00:00:10,559 sustains all life 5 00:00:17,430 --> 00:00:12,719 but here in the closest town to the 6 00:00:19,590 --> 00:00:17,440 north pole it's slowly leaking away 7 00:00:21,429 --> 00:00:19,600 a team headed there to launch rockets 8 00:00:23,429 --> 00:00:21,439 into the leak but it's not the lack of 9 00:00:25,589 --> 00:00:23,439 atmosphere that they're concerned about 10 00:00:27,670 --> 00:00:25,599 the leak is a natural process that will 11 00:00:30,230 --> 00:00:27,680 take billions of years so we're not 12 00:00:32,310 --> 00:00:30,240 going to run out anytime soon it's part 13 00:00:34,790 --> 00:00:32,320 of the larger story of how a planet's 14 00:00:36,630 --> 00:00:34,800 atmosphere changes over time a key 15 00:00:39,750 --> 00:00:36,640 factor in the search for life on other 16 00:00:45,270 --> 00:00:42,869 we have 35 residents and 60 of our team 17 00:00:46,869 --> 00:00:45,280 together in a town that is completely 18 00:00:49,029 --> 00:00:46,879 isolated there's a plane twice a week 19 00:00:49,990 --> 00:00:49,039 and there's a thousand polar bears 20 00:00:52,630 --> 00:00:50,000 nearby 21 00:00:54,869 --> 00:00:52,640 this is doug roland a nasa scientist 22 00:00:56,790 --> 00:00:54,879 who's taken his team to niallison on the 23 00:00:58,790 --> 00:00:56,800 island of svalbard 24 00:01:00,790 --> 00:00:58,800 the island lies beneath one of two 25 00:01:01,830 --> 00:01:00,800 regions near earth's poles called the 26 00:01:03,910 --> 00:01:01,840 cusps 27 00:01:05,990 --> 00:01:03,920 it's where we can access space directly 28 00:01:08,630 --> 00:01:06,000 and where a hundred tons of atmosphere 29 00:01:10,630 --> 00:01:08,640 escapes into space each day this escape 30 00:01:12,950 --> 00:01:10,640 gives clues to how long an atmosphere 31 00:01:15,510 --> 00:01:12,960 will last and ultimately whether it 32 00:01:17,429 --> 00:01:15,520 stays around long enough to sustain life 33 00:01:19,510 --> 00:01:17,439 we're trying to understand is how did 34 00:01:21,190 --> 00:01:19,520 earth's atmosphere evolve over time and 35 00:01:23,190 --> 00:01:21,200 how do other planets that might be like 36 00:01:25,990 --> 00:01:23,200 earth or more dissimilar to earth how 37 00:01:28,870 --> 00:01:26,000 did their atmospheres evolve 38 00:01:31,109 --> 00:01:28,880 so doug joined forces with joran mohan a 39 00:01:33,350 --> 00:01:31,119 professor at the university of oslo who 40 00:01:34,310 --> 00:01:33,360 started the grand challenge initiative 41 00:01:36,310 --> 00:01:34,320 cusp 42 00:01:38,469 --> 00:01:36,320 it's an international mission to launch 43 00:01:41,270 --> 00:01:38,479 12 rockets into the earth's northern 44 00:01:42,710 --> 00:01:41,280 cusp and doug he's the mission leader 45 00:01:43,630 --> 00:01:42,720 for the first two rockets of the 46 00:01:48,870 --> 00:01:43,640 campaign 47 00:01:50,469 --> 00:01:48,880 [Music] 48 00:01:51,910 --> 00:01:50,479 we don't want to waste our rocket it 49 00:01:53,510 --> 00:01:51,920 takes three years to make the rocket 50 00:01:56,069 --> 00:01:53,520 only 15 minutes to use it and i don't 51 00:01:57,510 --> 00:01:56,079 waste my shot here he's using a sounding 52 00:01:59,510 --> 00:01:57,520 rocket which is different from the 53 00:02:01,510 --> 00:01:59,520 bigger rockets that carry satellites and 54 00:02:03,670 --> 00:02:01,520 humans into space it's a small 55 00:02:05,990 --> 00:02:03,680 suborbital rocket that flies briefly 56 00:02:08,150 --> 00:02:06,000 into space collects real-time data for 57 00:02:09,029 --> 00:02:08,160 around 15 minutes then falls back to 58 00:02:11,430 --> 00:02:09,039 earth 59 00:02:13,750 --> 00:02:11,440 it's affordable quick to build and can 60 00:02:15,990 --> 00:02:13,760 launch towards a precise point the major 61 00:02:18,229 --> 00:02:16,000 advantage is that you can launch 62 00:02:20,390 --> 00:02:18,239 into a target on the sky but there's a 63 00:02:23,910 --> 00:02:20,400 limited launch window and only one 64 00:02:27,670 --> 00:02:26,150 we have these unguided rockets 65 00:02:28,710 --> 00:02:27,680 they go where you point them unless the 66 00:02:30,070 --> 00:02:28,720 wind is blowing because the wind 67 00:02:31,509 --> 00:02:30,080 literally just blows them over we don't 68 00:02:33,430 --> 00:02:31,519 launch when there's high wind so to 69 00:02:36,150 --> 00:02:33,440 measure the winds they launch balloons 70 00:02:38,630 --> 00:02:36,160 with gps trackers they're released every 71 00:02:40,949 --> 00:02:38,640 15 to 30 minutes and then they're 72 00:02:46,309 --> 00:02:40,959 monitored to see how fast the winds are 73 00:02:53,670 --> 00:02:49,509 the ground winds were 12 13 meters per 74 00:02:55,110 --> 00:02:53,680 second gusting 17 which is way off 75 00:02:57,190 --> 00:02:55,120 you're filled with trepidation oh my 76 00:03:02,790 --> 00:02:57,200 gosh this thing that i built is it going 77 00:03:05,350 --> 00:03:04,149 so i think we're going to scrub for 78 00:03:06,630 --> 00:03:05,360 today 79 00:03:09,430 --> 00:03:06,640 i'd like to thank everyone i think it 80 00:03:11,430 --> 00:03:09,440 was a great performance thanks a lot 81 00:03:13,910 --> 00:03:11,440 this means that we are scrubbing this 82 00:03:18,149 --> 00:03:13,920 operation for today and try again 83 00:03:23,589 --> 00:03:20,550 the mission is named visualizing ion 84 00:03:25,910 --> 00:03:23,599 outflow via neutral atom sensing 2 or 85 00:03:28,229 --> 00:03:25,920 visions 2. in short they're looking at 86 00:03:30,229 --> 00:03:28,239 how oxygen is getting enough energy to 87 00:03:32,390 --> 00:03:30,239 escape it's a good test of how 88 00:03:34,550 --> 00:03:32,400 atmospheric escape works earth's gravity 89 00:03:37,030 --> 00:03:34,560 should hold on to the oxygen and yet we 90 00:03:38,390 --> 00:03:37,040 see this gas shooting off into space 91 00:03:40,710 --> 00:03:38,400 we're trying to figure out how that 92 00:03:41,830 --> 00:03:40,720 works that is a science question that 93 00:03:44,229 --> 00:03:41,840 has been 94 00:03:46,550 --> 00:03:44,239 hanging around for four decades 95 00:03:48,949 --> 00:03:46,560 fortunately anyone can see atmospheric 96 00:03:50,710 --> 00:03:48,959 escape at the right place and time in 97 00:03:54,229 --> 00:03:50,720 svalbard we have the so-called polar 98 00:03:56,789 --> 00:03:54,239 night it's dark all 24 hours his 99 00:03:59,750 --> 00:03:56,799 continual darkness is key for witnessing 100 00:04:01,750 --> 00:03:59,760 this this is the cuspara it's a type of 101 00:04:04,309 --> 00:04:01,760 northern lights that appears between 8 102 00:04:06,149 --> 00:04:04,319 am and noon and you can only see it when 103 00:04:07,910 --> 00:04:06,159 it's dark during the day it looks 104 00:04:10,149 --> 00:04:07,920 similar to the aurora that occurs at 105 00:04:12,789 --> 00:04:10,159 night but when these iridescent colors 106 00:04:15,589 --> 00:04:12,799 dance at this hour each day 100 tons of 107 00:04:17,110 --> 00:04:15,599 oxygen escapes from earth's atmosphere 108 00:04:19,349 --> 00:04:17,120 into space 109 00:04:21,509 --> 00:04:19,359 this is our sport node to 110 00:04:24,469 --> 00:04:21,519 to chase the aurora 111 00:04:26,710 --> 00:04:24,479 working with them is the iscat radar and 112 00:04:28,310 --> 00:04:26,720 chell henriksen observatory they have 113 00:04:29,350 --> 00:04:28,320 additional instruments to find the 114 00:04:32,310 --> 00:04:29,360 aurora 115 00:04:35,749 --> 00:04:32,320 sometimes it's cloudy so we use radars 116 00:04:38,469 --> 00:04:35,759 to track the cusp we can give advice 117 00:04:40,790 --> 00:04:38,479 that this is the right type of aurora 118 00:04:42,550 --> 00:04:40,800 this is the wall of science a collection 119 00:04:44,390 --> 00:04:42,560 of data from satellites and ground 120 00:04:46,469 --> 00:04:44,400 instruments that helps them predict 121 00:04:47,749 --> 00:04:46,479 where the cusp aurora will be 122 00:04:49,270 --> 00:04:47,759 so the cusp 123 00:04:50,870 --> 00:04:49,280 actually isn't a fixed point in space it 124 00:04:53,110 --> 00:04:50,880 kind of moves around 125 00:04:55,749 --> 00:04:53,120 what's controlling the cusps movement is 126 00:04:58,070 --> 00:04:55,759 the sun interacting with earth 127 00:04:59,909 --> 00:04:58,080 our planet is surrounded by a magnetic 128 00:05:01,990 --> 00:04:59,919 field that helps us hold on to our 129 00:05:04,550 --> 00:05:02,000 atmosphere but at the north and south 130 00:05:06,390 --> 00:05:04,560 poles the magnetic field bends inwards 131 00:05:07,430 --> 00:05:06,400 creating a corridor between earth and 132 00:05:10,390 --> 00:05:07,440 space 133 00:05:12,950 --> 00:05:10,400 when energy is released from the sun via 134 00:05:14,469 --> 00:05:12,960 a solar flare or coronal mass ejection 135 00:05:16,710 --> 00:05:14,479 all of that energy in the form of 136 00:05:18,870 --> 00:05:16,720 radiation rides down the magnetic field 137 00:05:21,670 --> 00:05:18,880 lines of the earth and is transferred 138 00:05:23,510 --> 00:05:21,680 and dumped into the earth's atmosphere 139 00:05:25,830 --> 00:05:23,520 electrons cascade into earth's 140 00:05:28,230 --> 00:05:25,840 atmosphere they accelerate and collide 141 00:05:30,710 --> 00:05:28,240 with oxygen particles giving them energy 142 00:05:32,150 --> 00:05:30,720 to release light and sometimes enough 143 00:05:35,029 --> 00:05:32,160 energy to escape 144 00:05:37,670 --> 00:05:35,039 collectively this forms the cusp aurora 145 00:05:40,790 --> 00:05:37,680 and streams of escaping oxygen 146 00:05:42,310 --> 00:05:40,800 this cusp is in constant motion and 147 00:05:44,230 --> 00:05:42,320 we've got a fixed trajectory we really 148 00:05:45,670 --> 00:05:44,240 can't aim where the cusp is we have to 149 00:05:47,830 --> 00:05:45,680 wait for the cusp to come across our 150 00:05:49,189 --> 00:05:47,840 line of sight can you guys hear gelimer 151 00:05:50,390 --> 00:05:49,199 we'd like you as soon as you see an 152 00:05:52,390 --> 00:05:50,400 indication that crosstalk is moving 153 00:05:55,270 --> 00:05:52,400 close to move it the radar dish if we 154 00:06:02,629 --> 00:05:55,280 can this is ice cat it's been very quiet 155 00:06:02,639 --> 00:06:08,070 do you think 156 00:06:08,080 --> 00:06:14,790 probably about a 60 chance of launching 157 00:06:18,309 --> 00:06:16,150 when we started seeing this really good 158 00:06:20,469 --> 00:06:18,319 data this clock started counting down 159 00:06:23,110 --> 00:06:20,479 and that's when everyone realized this 160 00:06:25,510 --> 00:06:23,120 is going to happen we're going to launch 161 00:06:27,510 --> 00:06:25,520 we're doing everything we can to to get 162 00:06:28,710 --> 00:06:27,520 that launch off before the aurora goes 163 00:06:30,950 --> 00:06:28,720 away 164 00:06:32,950 --> 00:06:30,960 it is really really challenging and 165 00:06:36,150 --> 00:06:32,960 nerve-racking at that point 166 00:06:37,670 --> 00:06:36,160 you can see the tension just rise 167 00:06:40,469 --> 00:06:37,680 and everybody when that when that 168 00:06:42,469 --> 00:06:40,479 happens and so everyone's watching their 169 00:06:44,790 --> 00:06:42,479 instruments getting really excited and 170 00:06:45,830 --> 00:06:44,800 then at t minus one minute 171 00:06:48,000 --> 00:06:45,840 all of us 172 00:06:58,950 --> 00:06:48,010 ran out to go see the launch happen 173 00:07:00,870 --> 00:06:58,960 [Music] 174 00:07:03,029 --> 00:07:00,880 then we immediately turned around and 175 00:07:05,270 --> 00:07:03,039 ran right back in to look at all the 176 00:07:07,350 --> 00:07:05,280 data that was coming back from the 177 00:07:09,909 --> 00:07:07,360 instruments 178 00:07:11,749 --> 00:07:09,919 you know how much time and effort went 179 00:07:13,749 --> 00:07:11,759 into it because 180 00:07:14,950 --> 00:07:13,759 we all worked on it and there's just 181 00:07:17,270 --> 00:07:14,960 nothing 182 00:07:19,110 --> 00:07:17,280 that compares to that feeling 183 00:07:22,070 --> 00:07:19,120 everybody in every one of those little 184 00:07:24,550 --> 00:07:22,080 places you know really just so happy to 185 00:07:25,430 --> 00:07:24,560 contribute to uh to getting the science 186 00:07:28,469 --> 00:07:25,440 uh 187 00:07:30,390 --> 00:07:28,479 it's really an incredible experience 188 00:07:32,550 --> 00:07:30,400 this is a story about what it takes to 189 00:07:34,309 --> 00:07:32,560 launch science instruments into space 190 00:07:36,070 --> 00:07:34,319 but the real adventure will be in the 191 00:07:37,749 --> 00:07:36,080 data they sent back 192 00:07:40,469 --> 00:07:37,759 hidden within the numbers will be 193 00:07:42,150 --> 00:07:40,479 answers that reach far beyond earth 194 00:07:44,629 --> 00:07:42,160 shedding light on how atmospheres 195 00:07:46,150 --> 00:07:44,639 throughout the universe change evolve 196 00:07:48,010 --> 00:07:46,160 and perhaps