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These are the user uploaded subtitles that are being translated: 1 00:00:00,000 --> 00:00:04,440 NASA's revolutionary Juno probe 2 00:00:04,520 --> 00:00:07,880 is on a daring voyage to Jupiter. 3 00:00:07,960 --> 00:00:13,720 Its goal, to reveal the deepest mysteries of our solar system. 4 00:00:13,800 --> 00:00:16,560 Everything we see in the solar system today 5 00:00:16,640 --> 00:00:20,200 is affected by Jupiter somehow, in the past or now. 6 00:00:20,280 --> 00:00:25,600 All the asteroids, all the planets, the moons, the comets...everything. 7 00:00:25,680 --> 00:00:28,320 So in many ways, Juno is actually giving us a view 8 00:00:28,400 --> 00:00:31,720 into the history of our planetary system, even the history of Earth. 9 00:00:32,960 --> 00:00:35,360 Juno's mission is risky. 10 00:00:35,440 --> 00:00:38,480 Jupiter could eat the spacecraft...like that. 11 00:00:38,560 --> 00:00:43,520 But by diving perilously close to this monstrous world, 12 00:00:43,600 --> 00:00:48,000 Juno could change everything we know about our solar system. 13 00:00:48,080 --> 00:00:51,720 If you want to know what's happening, you got to get up-close and personal. 14 00:01:07,040 --> 00:01:10,280 Independence day, 2016... 15 00:01:10,360 --> 00:01:14,520 Juno arrives at Jupiter and gets to work. 16 00:01:14,600 --> 00:01:17,640 The probe angles its high-resolution camera 17 00:01:17,720 --> 00:01:20,320 towards this stormy world. 18 00:01:20,400 --> 00:01:23,480 Juno's snaps don't disappoint. 19 00:01:28,760 --> 00:01:32,160 The images returned from Juno are just beautiful. 20 00:01:42,960 --> 00:01:46,360 Suddenly you have this magnificent mosaic of this planet. 21 00:01:52,000 --> 00:01:54,560 As a human being, I'm like, Oh, my gosh, look at this. 22 00:01:54,640 --> 00:01:57,120 "This is amazing. This is coming back from Jupiter." 23 00:01:58,600 --> 00:02:01,360 These are the closest-ever views of Jupiter, 24 00:02:01,440 --> 00:02:04,440 a world 500 million miles away. 25 00:02:14,640 --> 00:02:17,960 But we didn't send Juno just to take pictures. 26 00:02:19,080 --> 00:02:24,400 One of its main goals is to peer deep into Jupiter's dark heart. 27 00:02:24,480 --> 00:02:27,160 One of the big questions we have about Jupiter is, 28 00:02:27,240 --> 00:02:29,360 does it have a core? 29 00:02:29,440 --> 00:02:32,360 And you'd think, well, of course every planet has a core. 30 00:02:32,440 --> 00:02:34,960 The Earth has a core. Everything does. 31 00:02:35,040 --> 00:02:37,040 Well, it turns out, Jupiter might not. 32 00:02:39,440 --> 00:02:41,880 Knowing what lies at a planet's core 33 00:02:41,960 --> 00:02:46,520 allows scientists to wind back the clock billions of years 34 00:02:46,600 --> 00:02:48,760 to the formation of the planets. 35 00:02:49,880 --> 00:02:53,640 If Juno can reveal what lies deep within Jupiter, 36 00:02:53,720 --> 00:02:55,920 it could change our understanding 37 00:02:56,000 --> 00:02:59,040 of how the gas giant formed. 38 00:02:59,120 --> 00:03:01,920 If Juno finds a solid core, 39 00:03:02,000 --> 00:03:06,560 it could mean Jupiter first formed as a rocky planet like Earth, 40 00:03:06,640 --> 00:03:09,040 then kept growing. 41 00:03:09,120 --> 00:03:11,440 But if Juno finds no core, 42 00:03:11,520 --> 00:03:14,720 it could mean that Jupiter skipped the rocky stage 43 00:03:14,800 --> 00:03:17,840 and formed straight from a cloud of gas. 44 00:03:19,040 --> 00:03:22,360 Answering this question could shine a light 45 00:03:22,440 --> 00:03:24,440 on other mysteries, too. 46 00:03:25,920 --> 00:03:28,000 If we can figure out how Jupiter formed, 47 00:03:28,080 --> 00:03:31,720 we can figure out the rest of the story of the solar system. 48 00:03:34,240 --> 00:03:37,240 So how do you probe down into the interior of a planet 49 00:03:37,320 --> 00:03:40,400 when all you can really see are the very tops of the clouds? 50 00:03:40,480 --> 00:03:43,040 Well, incredibly, you can use gravity. 51 00:03:43,120 --> 00:03:47,240 As Juno orbits Jupiter, 52 00:03:47,320 --> 00:03:51,880 it can sense in its orbit tiny little variations 53 00:03:51,960 --> 00:03:55,280 in the gravitational pull of Jupiter. 54 00:03:55,360 --> 00:03:57,920 As Juno speeds towards Jupiter, 55 00:03:58,000 --> 00:04:01,080 gravitational spikes tug at the craft. 56 00:04:01,160 --> 00:04:06,040 It turns out, some parts of Jupiter are denser than others. 57 00:04:06,120 --> 00:04:09,760 If Jupiter were some solid ball, then as Juno passes by it, 58 00:04:09,840 --> 00:04:12,560 as it passes very close above its cloud tops, 59 00:04:12,640 --> 00:04:15,400 the orbit, the trajectory, would be very smooth. 60 00:04:15,480 --> 00:04:18,160 But in fact, if Jupiter has layers 61 00:04:18,240 --> 00:04:20,440 or places where there's more mass 62 00:04:20,520 --> 00:04:23,760 and places where there's less, then it's gonna pull on Juno 63 00:04:23,840 --> 00:04:25,840 a little bit differently. 64 00:04:25,920 --> 00:04:29,000 Passing over areas of concentrated mass 65 00:04:29,080 --> 00:04:31,200 gives Juno a speed boost. 66 00:04:32,240 --> 00:04:34,880 So what they do is, the engineers back on Earth 67 00:04:34,960 --> 00:04:38,080 can basically just say, "How fast is it moving right now? 68 00:04:38,160 --> 00:04:40,160 How about now? How about now?" 69 00:04:40,240 --> 00:04:44,440 And you build up a map of where the mass is in Jupiter 70 00:04:44,520 --> 00:04:47,560 underneath the spacecraft as it passes around. 71 00:04:50,640 --> 00:04:54,880 Juno's instruments begin to map out the heart of gas giant, 72 00:04:54,960 --> 00:04:59,560 revealing the mysterious core for the first time. 73 00:04:59,640 --> 00:05:02,080 What Juno found was this amorphous mass, 74 00:05:02,160 --> 00:05:04,800 a fuzzy thing in the centre of Jupiter. 75 00:05:04,880 --> 00:05:07,440 It's not as solid as we expected 76 00:05:07,520 --> 00:05:09,520 if it were just a metal and rock core, 77 00:05:09,600 --> 00:05:11,600 but there is something there. 78 00:05:12,920 --> 00:05:14,920 In the centre of the planet, 79 00:05:15,000 --> 00:05:17,640 Juno detects hydrogen and rocky material 80 00:05:17,720 --> 00:05:20,240 dissolved and blended together. 81 00:05:20,320 --> 00:05:24,600 It's a type of planetary core we've never seen before. 82 00:05:24,680 --> 00:05:28,240 Astronomers are describing it as fuzzy. 83 00:05:29,240 --> 00:05:31,240 We thought we were gonna find an avocado. 84 00:05:31,320 --> 00:05:33,800 Instead we found a bowl of chili. 85 00:05:33,880 --> 00:05:37,560 It's a hydrogen fluid chili con carne. 86 00:05:40,040 --> 00:05:43,880 So none of our models of the interior of Jupiter turned out to be correct. 87 00:05:43,960 --> 00:05:46,520 That means we have to go back to the drawing board. 88 00:05:47,960 --> 00:05:51,600 One theory is that Jupiter didn't form from rocks or gas 89 00:05:51,680 --> 00:05:54,920 but from tiny pebbles less than an inch wide, 90 00:05:55,000 --> 00:06:00,600 strewn across the early solar system 4.6 billion years ago. 91 00:06:01,720 --> 00:06:04,520 These pebbles came together. They accreted 92 00:06:04,600 --> 00:06:06,600 to form a massive object 93 00:06:06,680 --> 00:06:09,520 that was the sort of seed, the core of Jupiter. 94 00:06:10,520 --> 00:06:12,800 The swarm of pebbles clumped together 95 00:06:12,880 --> 00:06:15,080 to form one giant core 96 00:06:15,160 --> 00:06:17,720 twenty times the mass of Earth. 97 00:06:17,800 --> 00:06:22,760 But these pebbles can't sustain this growing planet for long. 98 00:06:22,840 --> 00:06:26,440 Eventually, we need to make a jump from those centimetre-size particles 99 00:06:26,520 --> 00:06:29,640 up to really large things, like 100-kilometer planetesimals, 100 00:06:29,720 --> 00:06:32,520 to really kick-start growth of a planet. 101 00:06:34,520 --> 00:06:39,600 As Jupiter grows, its appetite becomes insatiable. 102 00:06:39,680 --> 00:06:42,680 The cores of other would-be planets are drawn in 103 00:06:42,760 --> 00:06:46,520 by its immense pull and absorbed on impact, 104 00:06:46,600 --> 00:06:49,760 causing Jupiter's core to transform. 105 00:06:49,840 --> 00:06:53,680 Huge chunks of incoming rock are mixed up with gas 106 00:06:53,760 --> 00:06:57,240 and the pebbles that originally built the core. 107 00:06:58,240 --> 00:07:01,520 We think that the core material that might've been there is actually 108 00:07:01,600 --> 00:07:05,600 dissolved and mixed in with the rest of the planet. 109 00:07:05,680 --> 00:07:08,000 This mix of rock, gas, and pebbles 110 00:07:08,080 --> 00:07:10,640 leaves the core in a strange state. 111 00:07:10,720 --> 00:07:13,120 Somewhere between solid and liquid 112 00:07:13,200 --> 00:07:15,320 or, in other words, fuzzy. 113 00:07:16,400 --> 00:07:19,520 Once Jupiter's core reaches a critical mass, 114 00:07:19,600 --> 00:07:24,560 its gravity starts sucking in all nearby hydrogen gas... 115 00:07:24,640 --> 00:07:27,240 building the iconic Jovian atmosphere 116 00:07:27,320 --> 00:07:29,320 and leaving the fuzzy core 117 00:07:29,400 --> 00:07:33,640 trapped beneath thousands of miles of thick clouds. 118 00:07:33,720 --> 00:07:37,960 And that is what formed Jupiter as we know and love it today. 119 00:07:38,040 --> 00:07:42,360 Juno's discovery of Jupiter's fuzzy core could rewrite the book 120 00:07:42,440 --> 00:07:44,960 on Jupiter's early years. 121 00:07:45,040 --> 00:07:47,360 But Juno is just getting started. 122 00:07:47,440 --> 00:07:49,800 We haven't even scratched the surface 123 00:07:49,880 --> 00:07:53,440 of the number of mysteries there are. 124 00:07:53,520 --> 00:07:56,280 There's more to Jupiter than meets the eye 125 00:07:56,360 --> 00:08:00,800 as Juno's instruments begin to reveal a darker side 126 00:08:00,880 --> 00:08:03,200 to this giant world. 127 00:08:03,280 --> 00:08:08,040 Jupiter's environment is one of the most vicious in the solar system, 128 00:08:08,120 --> 00:08:12,320 and that's because of its incredibly strong magnetic field. 129 00:08:12,400 --> 00:08:16,080 And Juno is caught right in the middle of it. 130 00:08:20,560 --> 00:08:22,600 The gas giant, Jupiter, 131 00:08:22,680 --> 00:08:26,880 holds clues to the mysteries of our solar system. 132 00:08:26,960 --> 00:08:29,400 And in 2011, NASA launches 133 00:08:29,480 --> 00:08:32,360 a billion-dollar mission to uncover them. 134 00:08:32,440 --> 00:08:36,480 MAN: Three, two, one, ignition. 135 00:08:36,560 --> 00:08:42,000 And lift-off of the Atlas V with Juno on a trek to Jupiter. 136 00:08:43,800 --> 00:08:47,800 To reach its target, Juno embarks on a five-year journey. 137 00:08:50,800 --> 00:08:54,600 Sending any spacecraft to another planet is gonna be tough, 138 00:08:54,680 --> 00:08:58,800 but sending one to Jupiter is really pushing things pretty hard. 139 00:09:00,280 --> 00:09:02,640 Juno weaves through the solar system 140 00:09:02,720 --> 00:09:04,720 with extreme precision. 141 00:09:04,800 --> 00:09:08,000 The craft battles violent temperature changes 142 00:09:08,080 --> 00:09:11,600 and navigates carefully through the asteroid belt. 143 00:09:11,680 --> 00:09:14,360 If there's a fleck of dust in your path 144 00:09:14,440 --> 00:09:16,440 and that thing slams into your spacecraft, 145 00:09:16,520 --> 00:09:19,160 it could do significant damage. 146 00:09:19,240 --> 00:09:22,400 1.7 billion miles into its mission, 147 00:09:22,480 --> 00:09:25,360 Juno finally nears its target, 148 00:09:25,440 --> 00:09:28,000 but the probe is hurtling towards Jupiter 149 00:09:28,080 --> 00:09:31,520 at 165,000 miles per hour. 150 00:09:33,240 --> 00:09:35,240 Juno is moving really fast. 151 00:09:35,320 --> 00:09:37,920 It's one of the fastest spacecraft ever. 152 00:09:38,000 --> 00:09:39,720 You need to go fast enough to get there 153 00:09:39,800 --> 00:09:43,400 but then you need to be slow enough to be captured by the gravity of the planet. 154 00:09:43,480 --> 00:09:46,200 You need to get it just right. 155 00:09:46,280 --> 00:09:49,720 Get it wrong and Juno could slam into the planet 156 00:09:49,800 --> 00:09:52,240 or drift out into deep space. 157 00:09:57,080 --> 00:10:00,640 To successfully get Juno to enter a stable orbit around Jupiter... 158 00:10:00,720 --> 00:10:02,720 it's almost the same as, say, 159 00:10:02,800 --> 00:10:04,800 shooting a basketball from London 160 00:10:04,880 --> 00:10:07,400 and having it on the land on the front of the rim in New York 161 00:10:07,480 --> 00:10:09,480 and just sitting there balanced. 162 00:10:09,560 --> 00:10:14,320 I could do it... but can NASA do it with Juno? 163 00:10:14,400 --> 00:10:16,400 (LAUGHING) 164 00:10:18,200 --> 00:10:20,360 NASA has a neat game plan. 165 00:10:20,440 --> 00:10:22,720 Juno performs a backflip in space 166 00:10:22,800 --> 00:10:25,800 and fires its thruster towards Jupiter. 167 00:10:25,880 --> 00:10:27,880 Everything is going smoothly. 168 00:10:27,960 --> 00:10:30,560 We're continuing to burn and change our velocity. 169 00:10:31,640 --> 00:10:35,000 The rocket burns for 35 nail-biting minutes, 170 00:10:35,080 --> 00:10:39,160 reducing the craft's speed by 1,200 miles per hour. 171 00:10:44,600 --> 00:10:45,600 (CHEERING) 172 00:10:45,680 --> 00:10:48,480 Finally the probe achieves orbit around Jupiter. 173 00:10:49,640 --> 00:10:53,080 Right on July 4th, during the fireworks, we just got into orbit. 174 00:10:53,160 --> 00:10:55,800 In many ways, we're firing a rocket motor. 175 00:10:55,880 --> 00:10:57,880 I mean, it is fireworks. 176 00:11:00,400 --> 00:11:03,840 Safe in orbit, Juno turns its instruments to the planet 177 00:11:03,920 --> 00:11:06,080 for a critical part of the mission... 178 00:11:06,160 --> 00:11:08,840 Investigating Jupiter's magnetic field. 179 00:11:11,520 --> 00:11:13,800 Deep below the stormy surface, 180 00:11:13,880 --> 00:11:18,400 liquid metallic hydrogen flows endlessly around the planet, 181 00:11:18,480 --> 00:11:21,520 producing a huge magnetic field. 182 00:11:21,600 --> 00:11:26,240 This magnetosphere stretches over 600 million miles 183 00:11:26,320 --> 00:11:30,200 beyond the planet, reaching all the way to Saturn. 184 00:11:35,240 --> 00:11:38,520 To reveal the true scale of Jupiter's magnetosphere, 185 00:11:38,600 --> 00:11:42,000 planetary scientist Jani Radebaugh hits the beach. 186 00:11:43,000 --> 00:11:45,040 I've made a little solar system. 187 00:11:45,120 --> 00:11:47,120 So we'll start here at the sun. 188 00:11:47,200 --> 00:11:49,360 We come out here to the Earth. 189 00:11:49,440 --> 00:11:51,800 And now we're going to skip a few and go out to Jupiter. 190 00:11:51,880 --> 00:11:55,200 And Jupiter is five times as far away from the sun as the Earth. 191 00:11:55,280 --> 00:11:57,280 Now, we'll go out to Saturn. 192 00:11:58,280 --> 00:12:01,520 Saturn here is ten times as far away from the sun as the Earth. 193 00:12:01,600 --> 00:12:04,360 And we want to look at the size of Jupiter's magnetic field. 194 00:12:04,440 --> 00:12:07,280 So we want to draw out the magnetic field of Jupiter. 195 00:12:07,360 --> 00:12:09,680 It arches around like this... 196 00:12:09,760 --> 00:12:13,440 away from the sun because the solar wind is impacting the magnetic field, 197 00:12:13,520 --> 00:12:15,520 dragging it downwind. 198 00:12:15,600 --> 00:12:18,840 So here it comes downwind. 199 00:12:18,920 --> 00:12:20,920 On both sides. 200 00:12:21,000 --> 00:12:23,160 All the way out to the orbit of Saturn. 201 00:12:25,320 --> 00:12:27,320 Jupiter's magnetosphere stretches 202 00:12:27,400 --> 00:12:30,320 over 600 million miles beyond the planet. 203 00:12:31,360 --> 00:12:33,920 When you think about structures in our solar system, 204 00:12:34,000 --> 00:12:35,840 of course, you think of the giant sun, 205 00:12:35,920 --> 00:12:38,000 you think of massive planets like Jupiter... 206 00:12:38,080 --> 00:12:42,200 But what if the largest things in the solar system are things we really can't see. 207 00:12:42,280 --> 00:12:44,280 And in fact the magnetic field of Jupiter 208 00:12:44,360 --> 00:12:46,360 and all of the particles trapped in it 209 00:12:46,440 --> 00:12:49,160 are one of the largest things the solar system has to offer. 210 00:12:49,240 --> 00:12:52,600 If your eyes could actually see Jupiter's magnetosphere 211 00:12:52,680 --> 00:12:55,440 and you tried to look at it while standing on Earth, 212 00:12:55,520 --> 00:12:58,160 it would look about as big in the sky as the moon. 213 00:12:59,720 --> 00:13:02,040 And within this magnetic field, 214 00:13:02,120 --> 00:13:04,480 Juno faces an invisible threat. 215 00:13:06,280 --> 00:13:09,560 Jupiter has an enormous magnetic field. 216 00:13:09,640 --> 00:13:12,840 It is so enormous in terms of space, 217 00:13:12,920 --> 00:13:14,920 but also in terms of power. 218 00:13:15,440 --> 00:13:18,400 As Jupiter is bombarded by the solar wind, 219 00:13:18,480 --> 00:13:20,480 high-energy particles from the sun 220 00:13:20,560 --> 00:13:23,320 are funnelled into deadly radiation belts, 221 00:13:23,400 --> 00:13:27,120 guided by the giant planet's magnetic field. 222 00:13:27,200 --> 00:13:31,360 The magnetic field traps charged particles coming from the sun 223 00:13:31,440 --> 00:13:34,200 and circulates them around that system 224 00:13:34,280 --> 00:13:37,480 and just bombards anything in the vicinity, 225 00:13:37,560 --> 00:13:40,320 including our fragile little spacecraft. 226 00:13:42,360 --> 00:13:46,360 Close to the planet, radiation levels are up to 30 times greater 227 00:13:46,440 --> 00:13:48,440 than inside the reactor core room 228 00:13:48,520 --> 00:13:51,200 during the Chernobyl disaster. 229 00:13:51,280 --> 00:13:53,280 This is radiation. 230 00:13:53,360 --> 00:13:56,600 This is bad news. These particles, they would hit you. 231 00:13:56,680 --> 00:13:59,760 They would rupture your DNA, rupture your cell structures, 232 00:13:59,840 --> 00:14:01,840 and you would die. 233 00:14:03,280 --> 00:14:08,440 This blistering radiation is bad news for the spacecraft too. 234 00:14:08,520 --> 00:14:10,680 The charged particles threaten to destroy 235 00:14:10,760 --> 00:14:13,440 electronic and navigational systems, 236 00:14:13,520 --> 00:14:16,240 but Juno has armoured up. 237 00:14:17,280 --> 00:14:21,120 It's not some delicate, beautiful, gossamer thing 238 00:14:21,200 --> 00:14:23,360 that you are sending to orbit Jupiter. 239 00:14:23,440 --> 00:14:25,440 It's more like a tank. 240 00:14:25,520 --> 00:14:27,520 You have to protect this thing or else 241 00:14:27,600 --> 00:14:29,600 it's not going to last very long at all. 242 00:14:31,160 --> 00:14:34,400 We've got a couple hundred pounds of titanium 243 00:14:34,480 --> 00:14:36,680 on the spacecraft just trying to shield us 244 00:14:36,760 --> 00:14:39,000 from what Jupiter might throw at us. 245 00:14:39,080 --> 00:14:42,200 So it is, in a sense, like an armoured tank going into war. 246 00:14:43,640 --> 00:14:46,560 Lightweight titanium is tough. 247 00:14:46,640 --> 00:14:50,080 Juno's half inch thick shielding blocks 99% 248 00:14:50,160 --> 00:14:52,440 of Jupiter's vicious radiation. 249 00:14:52,520 --> 00:14:54,520 But even at this reduced rate, 250 00:14:54,600 --> 00:14:57,000 Juno can't survive the bombardment for long. 251 00:14:57,080 --> 00:15:00,480 So the craft sets itself on a unique orbit 252 00:15:00,560 --> 00:15:02,680 around the gas giant. 253 00:15:06,960 --> 00:15:09,240 It actually has a very long orbit 254 00:15:09,320 --> 00:15:11,880 where it spends most of its time far away. 255 00:15:11,960 --> 00:15:14,440 And then every once in a while dives in and goes, 256 00:15:14,520 --> 00:15:16,520 "Oh, hot, hot, hot. I zoomed in too much," 257 00:15:16,600 --> 00:15:19,080 and then goes safely away to communicate and process 258 00:15:19,160 --> 00:15:21,160 and then back in again. 259 00:15:23,160 --> 00:15:25,160 Juno takes a mighty gamble 260 00:15:25,240 --> 00:15:27,600 diving deep into these radiation belts 261 00:15:27,680 --> 00:15:30,320 to achieve one of its key objectives, 262 00:15:30,400 --> 00:15:33,800 mapping Jupiter's giant magnetic field. 263 00:15:33,880 --> 00:15:36,880 And as Juno swoops around the planet, 264 00:15:36,960 --> 00:15:40,840 it reveals something scientists have never seen before. 265 00:15:42,520 --> 00:15:45,800 Planetary scientist Dan Durda demonstrates. 266 00:15:45,880 --> 00:15:49,920 We can use a pretty simple, even elementary school level experiment 267 00:15:50,000 --> 00:15:52,600 of the structure of the Earth's magnetic field 268 00:15:52,680 --> 00:15:55,200 by shaking some iron filings 269 00:15:55,280 --> 00:15:57,320 across the surface 270 00:15:57,400 --> 00:15:59,760 of very simple bar magnet with a north and south pole. 271 00:15:59,840 --> 00:16:03,800 Earth's magnetic field forms a perfect bubble around our planet, 272 00:16:03,880 --> 00:16:06,880 protecting us from solar radiation and cosmic rays. 273 00:16:06,960 --> 00:16:09,520 If I can get these little iron fillings to come out here... 274 00:16:09,600 --> 00:16:12,200 And already I can see, 275 00:16:12,280 --> 00:16:14,920 the sort of classic outlines 276 00:16:15,000 --> 00:16:19,120 of the north and south magnetic field lines that are coming out of our planet. 277 00:16:19,200 --> 00:16:23,920 The Earth's magnetic field is pretty well behaved in this way. It's what we call a dipolar field. 278 00:16:24,000 --> 00:16:27,960 It has a very distinct north and south magnetic pole. 279 00:16:28,040 --> 00:16:31,800 Lucky for us, Earth's magnetic field is pretty stable. 280 00:16:31,880 --> 00:16:36,640 But new results from Juno suggests that Jupiter may not be so fortunate. 281 00:16:37,840 --> 00:16:40,920 Jupiter's magnetic field is much more complex than this. 282 00:16:41,000 --> 00:16:43,040 Jupiter is not going to play by those rules. 283 00:16:43,120 --> 00:16:46,920 Its magnetic fields are going to do whatever it wants. 284 00:16:47,000 --> 00:16:50,680 And the generation of that magnetic field 285 00:16:50,760 --> 00:16:53,760 is so complex and so twisted and and so wild 286 00:16:53,840 --> 00:16:58,400 that the magnetic field is gonna have very strange shapes 287 00:16:58,480 --> 00:17:00,720 that we're just now beginning to understand. 288 00:17:00,800 --> 00:17:04,200 When you look at the Earth, we have a fairly simple magnetic field. 289 00:17:04,280 --> 00:17:08,120 It's like a giant bar magnet with a north and south magnetic pole. 290 00:17:08,200 --> 00:17:10,200 Well, Jupiter has that as well. 291 00:17:10,280 --> 00:17:13,520 This is called a dipolar field. It's got two poles. 292 00:17:13,600 --> 00:17:16,080 But it also has a third pole. 293 00:17:17,960 --> 00:17:19,960 Juno's magnetic field maps 294 00:17:20,040 --> 00:17:22,040 shows a north and south pole 295 00:17:22,120 --> 00:17:25,720 and a bizarre magnetic disturbance at Jupiter's equator. 296 00:17:25,800 --> 00:17:29,320 And it's like Jupiter just sprouted a third arm, 297 00:17:29,400 --> 00:17:31,400 and that's kind of mysterious. 298 00:17:32,440 --> 00:17:34,440 On magnetic field maps, 299 00:17:34,520 --> 00:17:38,080 north poles show up red and south poles blue. 300 00:17:38,160 --> 00:17:40,920 So scientists are calling this second south pole 301 00:17:41,000 --> 00:17:43,000 the Great Blue Spot. 302 00:17:43,080 --> 00:17:45,640 Everyone knows about the Great Red Spot, 303 00:17:45,720 --> 00:17:49,080 but Jupiter now has a Great Blue Spot as well. 304 00:17:49,160 --> 00:17:51,560 This magnetic disturbance reflects 305 00:17:51,640 --> 00:17:53,960 Jupiter's stormy interior. 306 00:17:54,040 --> 00:17:57,800 You have these fast-moving winds blowing on the magnetic field, 307 00:17:57,880 --> 00:18:01,760 and they're actually shearing it apart and moving the field around. 308 00:18:01,840 --> 00:18:04,520 It's not necessarily a storm, although it could be. 309 00:18:04,600 --> 00:18:07,320 It maybe is better to think of it as a magnetic storm. 310 00:18:10,480 --> 00:18:12,600 Turbulence inside Jupiter could be 311 00:18:12,680 --> 00:18:16,400 twisting up the magnetic field to drive the Great Blue Spot 312 00:18:16,480 --> 00:18:18,480 and the deadly radiation belts 313 00:18:18,560 --> 00:18:21,520 that Juno must navigate through. 314 00:18:21,600 --> 00:18:26,680 Unlike Earth, Jupiter is not really a solid mass for the most part. 315 00:18:26,760 --> 00:18:29,520 So all of its clouds and gases 316 00:18:29,600 --> 00:18:32,000 are moving at slightly different rates 317 00:18:32,080 --> 00:18:34,520 and that actually makes the magnetic field 318 00:18:34,600 --> 00:18:39,240 that's generated very variable and highly changing. 319 00:18:39,320 --> 00:18:42,160 For us to have a variable magnetic field like Jupiter does, 320 00:18:42,240 --> 00:18:44,400 the entire Earth would have to be molten. 321 00:18:44,480 --> 00:18:46,480 We really don't want that to happen. 322 00:18:46,560 --> 00:18:48,560 With each orbit of Jupiter, 323 00:18:48,640 --> 00:18:52,040 Juno unravels more mysteries of this giant planet. 324 00:18:52,120 --> 00:18:54,120 But Jupiter's deepest secret 325 00:18:54,200 --> 00:18:57,560 could shine a light on our own origins. 326 00:18:57,640 --> 00:19:00,960 If we want to understand the Earth and our place in the solar system, 327 00:19:01,040 --> 00:19:03,360 Juno has found that a lot of those mysteries 328 00:19:03,440 --> 00:19:05,440 are locked up there in Jupiter. 329 00:19:11,000 --> 00:19:14,680 The Juno spacecraft is uncovering the secrets of Jupiter 330 00:19:14,760 --> 00:19:18,400 from its swirling cloud tops to its dark heart. 331 00:19:18,480 --> 00:19:23,160 But Juno's discoveries go beyond the gas giant itself. 332 00:19:23,240 --> 00:19:28,160 They could answer mysteries about our own planet. 333 00:19:28,240 --> 00:19:32,960 Jupiter is the key to the formation of the solar system, 334 00:19:33,040 --> 00:19:35,120 which means it's the key to understanding 335 00:19:35,200 --> 00:19:37,520 how the Earth formed. 336 00:19:37,600 --> 00:19:40,960 Juno is actually giving us a view into the history of our planetary system, 337 00:19:41,040 --> 00:19:43,680 even the history of Earth. 338 00:19:43,760 --> 00:19:46,680 4.6 billion years ago, 339 00:19:46,760 --> 00:19:52,680 a mammoth cloud of hydrogen gas and cosmic dust collapses, 340 00:19:52,760 --> 00:19:55,640 sparking nuclear fusion. 341 00:19:55,720 --> 00:19:57,720 From the resulting chaos, 342 00:19:57,800 --> 00:20:00,640 one star, four rocky worlds, 343 00:20:00,720 --> 00:20:03,600 and four gassy giants are born 344 00:20:03,680 --> 00:20:06,040 to form our solar system. 345 00:20:08,400 --> 00:20:10,760 There's these distinct zones of the solar system... 346 00:20:10,840 --> 00:20:12,560 rocky and metallic in the inner part, 347 00:20:12,640 --> 00:20:14,760 gaseous and water-rich in the outer part. 348 00:20:14,840 --> 00:20:17,520 And even without thinking about that too hard, 349 00:20:17,600 --> 00:20:21,400 it kind of makes sense cos getting close to the sun, it's warmer. 350 00:20:21,480 --> 00:20:23,840 Out farther away from the sun, it's cooler. 351 00:20:26,040 --> 00:20:28,640 But the Earth breaks the mould. 352 00:20:28,720 --> 00:20:33,520 Our planet has far more life-giving water than theories predict. 353 00:20:33,600 --> 00:20:35,840 The Earth formed in a part of the solar system that, 354 00:20:35,920 --> 00:20:38,240 you'd think normally should be probably pretty dry 355 00:20:38,320 --> 00:20:40,320 cos it was pretty close to the sun. 356 00:20:40,400 --> 00:20:45,280 Our planet is just 150 million miles from the sun, 357 00:20:45,360 --> 00:20:49,680 putting us inside what scientists call the snow line. 358 00:20:49,760 --> 00:20:53,160 Inside this line, the sun is powerful enough 359 00:20:53,240 --> 00:20:56,640 to evaporate water during a planet's formation. 360 00:20:58,320 --> 00:21:00,880 Inside the snow line, the temperatures are high 361 00:21:00,960 --> 00:21:03,560 and there's a lot of energy from the sun nearby. 362 00:21:03,640 --> 00:21:05,840 Too close to the sun, those gaseous 363 00:21:05,920 --> 00:21:08,520 and ice-rich materials just can't exist. 364 00:21:08,600 --> 00:21:10,760 They're evaporated away by the heat of the sun. 365 00:21:12,400 --> 00:21:15,880 Our watery world should be a dry rock in space. 366 00:21:17,120 --> 00:21:19,640 Understanding how water got to the Earth is so important 367 00:21:19,720 --> 00:21:22,520 because it wouldn't be there in the very, very beginning. 368 00:21:23,960 --> 00:21:27,280 But Jupiter could hold the answer to this mystery. 369 00:21:28,520 --> 00:21:30,760 To solve the riddle of Earth's water, 370 00:21:30,840 --> 00:21:33,840 Juno aims to discover where Jupiter was born. 371 00:21:35,680 --> 00:21:40,320 Understanding how and where and when Jupiter formed is critical. 372 00:21:40,400 --> 00:21:44,600 Because it has really dominated the entire evolution of the solar system. 373 00:21:44,680 --> 00:21:46,680 It's the biggest planet by far. 374 00:21:46,760 --> 00:21:51,040 It's the biggest thing out there, that's moving everything around. 375 00:21:51,120 --> 00:21:53,480 Any water in the early solar system 376 00:21:53,560 --> 00:21:57,200 could have been moved around by Jupiter's mighty gravity. 377 00:21:57,280 --> 00:22:00,200 So if Juno can trace Jupiter's history, 378 00:22:00,280 --> 00:22:03,040 that could explain why we find H2O 379 00:22:03,120 --> 00:22:05,440 where it's least expected. 380 00:22:05,520 --> 00:22:09,280 We know that planets can move closer to the sun and farther out 381 00:22:09,360 --> 00:22:11,880 while they're forming and even after they form. 382 00:22:11,960 --> 00:22:15,520 So how do we figure out where Jupiter formed? 383 00:22:15,600 --> 00:22:20,200 The key is how much water is locked up inside Jupiter. 384 00:22:20,280 --> 00:22:23,120 If we can understand how Jupiter 385 00:22:23,200 --> 00:22:25,200 built a relationship with water, 386 00:22:25,280 --> 00:22:27,280 we can understand how water got 387 00:22:27,360 --> 00:22:31,200 distributed all throughout the solar system including here on Earth. 388 00:22:34,080 --> 00:22:37,120 If Juno can measure the water content of Jupiter, 389 00:22:37,200 --> 00:22:39,480 it will solve a 20 year old mystery. 390 00:22:42,360 --> 00:22:45,000 December, 1995. 391 00:22:45,080 --> 00:22:49,920 NASA's Galileo probe begins a fatal dive into Jupiter's atmosphere. 392 00:22:51,680 --> 00:22:54,760 When it did, it was able to measure 393 00:22:54,840 --> 00:22:57,320 the atmosphere around it and detect water. 394 00:22:57,400 --> 00:22:59,600 And the thing is, it didn't. 395 00:22:59,680 --> 00:23:02,720 Didn't find any, and that's weird. 396 00:23:02,800 --> 00:23:04,960 Everything was bone dry. 397 00:23:05,040 --> 00:23:07,640 So why in the world did Jupiter's atmosphere look dry? 398 00:23:08,880 --> 00:23:12,000 If the results from the Galileo probe are correct, 399 00:23:12,080 --> 00:23:14,280 Then 4.6 billion years ago 400 00:23:14,360 --> 00:23:16,560 Jupiter formed closer to the sun. 401 00:23:18,320 --> 00:23:20,960 But that's not the whole story. 402 00:23:21,040 --> 00:23:25,160 20 years later, NASA sends Juno to get a second opinion. 403 00:23:26,440 --> 00:23:30,600 Juno is an orbiter so it's loaded with instruments and detectors 404 00:23:30,680 --> 00:23:34,320 to look down on Jupiter and try to figure out everything going on. 405 00:23:35,800 --> 00:23:40,200 Juno doesn't have to risk it's life to hunt for water. 406 00:23:40,280 --> 00:23:42,880 The craft pierced through Jupiter's thick clouds 407 00:23:42,960 --> 00:23:45,320 using a microwave radiometer 408 00:23:45,400 --> 00:23:48,560 - to detect H2 - O from a safe distance. 409 00:23:48,640 --> 00:23:50,640 Using these microwaves, 410 00:23:50,720 --> 00:23:53,800 Juno builds up a global map of Jupiter's water. 411 00:23:54,800 --> 00:23:59,200 What Juno has found is, yeah, there's plenty of water in Jupiter. 412 00:23:59,280 --> 00:24:02,440 It's just that Galileo happened to hit a dry spot. 413 00:24:02,520 --> 00:24:05,080 But, in fact, if it had come in almost anywhere else, 414 00:24:05,160 --> 00:24:07,160 it would've seen plenty of water. 415 00:24:09,040 --> 00:24:11,960 Juno's findings may give scientists a clue 416 00:24:12,040 --> 00:24:14,800 to understanding where Jupiter originally formed. 417 00:24:16,080 --> 00:24:19,080 It seems apparent now that Jupiter 418 00:24:19,160 --> 00:24:22,800 didn't form in its present location. 419 00:24:22,880 --> 00:24:27,440 The leading theory is that Jupiter formed just beyond the Snow line - 420 00:24:27,520 --> 00:24:30,360 the boundary between the dry inner solar system 421 00:24:30,440 --> 00:24:32,800 and the wet outer solar system. 422 00:24:32,880 --> 00:24:35,960 But we find Jupiter is twice as far away from the sun 423 00:24:36,040 --> 00:24:38,320 as where that original Snow line would've been. 424 00:24:38,400 --> 00:24:40,520 So this is telling us something interesting. 425 00:24:42,640 --> 00:24:45,960 Jupiter may have wandered from its original position, 426 00:24:46,040 --> 00:24:48,040 causing unimaginable chaos. 427 00:24:49,040 --> 00:24:51,400 As Jupiter moved around, things got hit 428 00:24:51,480 --> 00:24:53,560 and knocked out of the solar system. 429 00:24:53,640 --> 00:24:56,040 It essentially scatters everything in its path. 430 00:24:56,120 --> 00:24:58,760 It's the biggest player. It's the biggest planet. 431 00:24:58,840 --> 00:25:00,840 Everything moves for it. 432 00:25:02,240 --> 00:25:06,360 As Jupiter bulldozes towards the outer solar system, 433 00:25:06,440 --> 00:25:09,360 it slings ice ridged asteroids and comets 434 00:25:09,440 --> 00:25:12,440 in towards the sun and towards Earth. 435 00:25:15,920 --> 00:25:17,920 Jupiter would literally, in some sense, 436 00:25:18,000 --> 00:25:20,920 have snow ploughed into the inner solar system. 437 00:25:21,000 --> 00:25:23,080 A whole wave of water rich planetesimals 438 00:25:23,160 --> 00:25:26,680 that would've delivered much of our Earth's oceans. 439 00:25:28,160 --> 00:25:31,240 Juno has helped answer why Earth is habitable 440 00:25:31,320 --> 00:25:34,120 despite being so close to the sun. 441 00:25:34,200 --> 00:25:36,600 So it was worth going all that distance, 442 00:25:36,680 --> 00:25:39,560 sending Juno all the way out there to get that closer look. 443 00:25:43,400 --> 00:25:45,440 Our solar system plays host 444 00:25:45,520 --> 00:25:48,400 to some epic natural wonders. 445 00:25:48,480 --> 00:25:51,080 The ice geysers of Enceladus, 446 00:25:51,160 --> 00:25:53,360 the giant rings of Saturn, 447 00:25:53,440 --> 00:25:57,400 the Martian mega volcano, Olympus Mons. 448 00:25:57,480 --> 00:25:59,880 But in July, 2017, 449 00:25:59,960 --> 00:26:03,680 NASA's Juno probe skims the surface of Jupiter 450 00:26:03,760 --> 00:26:07,440 and photographs the most famous natural wonder. 451 00:26:07,520 --> 00:26:10,480 A fierce hurricane-like storm 452 00:26:10,560 --> 00:26:13,600 that's been raging for hundreds of years. 453 00:26:15,400 --> 00:26:19,120 When you think of Jupiter, one of the most visually stunning, 454 00:26:19,200 --> 00:26:23,200 most iconic features of the atmosphere is the Great Red Spot. 455 00:26:23,280 --> 00:26:26,680 There is nothing like Jupiter's Red Spot in our entire solar system. 456 00:26:27,680 --> 00:26:30,960 As Juno soars over the Great Red Spot, 457 00:26:31,040 --> 00:26:33,240 it looks down onto a storm 458 00:26:33,320 --> 00:26:36,120 over 10,000 miles across. 459 00:26:39,360 --> 00:26:41,520 This is the most extreme storm. 460 00:26:41,600 --> 00:26:44,560 The winds are blowing continuously at 400 miles an hour. 461 00:26:48,560 --> 00:26:52,160 Earth's most powerful Category Five hurricanes 462 00:26:52,240 --> 00:26:56,160 are less than half as powerful as the storm on Jupiter. 463 00:26:57,920 --> 00:27:00,080 The Great Red Spot is the 464 00:27:00,160 --> 00:27:02,440 greatest hurricane that you've ever imagined. 465 00:27:02,520 --> 00:27:04,840 But that's not all. 466 00:27:04,920 --> 00:27:08,360 Juno's microwave radiometer allows scientists to see through 467 00:27:08,440 --> 00:27:11,680 Jupiter's cloud layers for the first time. 468 00:27:12,920 --> 00:27:16,400 Juno has instrumentation that's able to look underneath. 469 00:27:16,480 --> 00:27:20,600 So one of the things we did was, we looked at how deep are the roots? 470 00:27:20,680 --> 00:27:24,760 Juno peers down into the eye of this monster storm. 471 00:27:24,840 --> 00:27:29,560 It spots temperature changes that follow the storm's iconic shape. 472 00:27:29,640 --> 00:27:32,160 Tracing the roots of the Great Red Spot 473 00:27:32,240 --> 00:27:34,440 deep into the Jovian atmosphere. 474 00:27:35,560 --> 00:27:40,720 They found out that it goes down over 200 miles deep into the atmosphere. 475 00:27:40,800 --> 00:27:43,200 There's nothing like that on Earth 476 00:27:43,280 --> 00:27:46,440 Weather satellites circling the Earth show the greatest 477 00:27:46,520 --> 00:27:49,280 cyclones of our planet can reach heights 478 00:27:49,360 --> 00:27:51,520 of around ten miles. 479 00:27:51,600 --> 00:27:55,520 But Jupiter's Great Red Spot is 20 times taller. 480 00:27:56,760 --> 00:27:58,960 I think that really brings into perspective 481 00:27:59,040 --> 00:28:01,200 the massive scale of this planet. 482 00:28:02,520 --> 00:28:05,360 The dizzying depths of the storm is made possible 483 00:28:05,440 --> 00:28:07,800 by Jupiter's vast hidden atmosphere. 484 00:28:07,880 --> 00:28:10,200 A seemingly endless spinning mass 485 00:28:10,280 --> 00:28:13,200 made up of hydrogen and helium. 486 00:28:13,280 --> 00:28:17,960 Jupiter doesn't have a solid surface like the Earth does. 487 00:28:18,040 --> 00:28:21,400 And so right away, if you were to dive into Jupiter's clouds 488 00:28:21,480 --> 00:28:25,040 things are gonna be really different. This atmosphere's tremendously thick. 489 00:28:25,120 --> 00:28:27,440 As you're going in the pressure is going up. 490 00:28:28,920 --> 00:28:31,760 As soon as you start plunging down into that atmosphere 491 00:28:31,840 --> 00:28:34,680 there's more and more. There's not just a 100 miles of air, 492 00:28:34,760 --> 00:28:38,320 there's a 1,000 miles of air, 10,000 miles of air above you. 493 00:28:38,400 --> 00:28:42,240 And not only would your ears pop deep in the Jovian atmosphere, 494 00:28:42,320 --> 00:28:44,520 your entire body would pop 495 00:28:44,600 --> 00:28:47,800 and, in fact, all of your molecules would pop. 496 00:28:49,760 --> 00:28:52,280 Juno's vast turbulent atmosphere 497 00:28:52,360 --> 00:28:56,880 hosts the deepest storm mankind has ever seen. 498 00:28:56,960 --> 00:28:58,960 And Juno's discoveries 499 00:28:59,040 --> 00:29:01,240 gets scientists wondering... 500 00:29:01,320 --> 00:29:03,320 Could the Great Red Spot 501 00:29:03,400 --> 00:29:06,280 be behind another of Jupiter's mysteries, 502 00:29:06,360 --> 00:29:09,840 the planet's surprisingly warm atmosphere? 503 00:29:12,440 --> 00:29:15,080 Jupiter lurks out in our outer solar system, 504 00:29:15,160 --> 00:29:17,720 where everything is very cold, the sun is very dim 505 00:29:17,800 --> 00:29:20,320 when you get that far away. 506 00:29:20,400 --> 00:29:23,280 Jupiter is five times farther from the sun than we are. 507 00:29:23,360 --> 00:29:26,160 So it's only getting four percent of the amount of energy 508 00:29:26,240 --> 00:29:27,680 from the sun that we do. 509 00:29:27,760 --> 00:29:30,720 But there's something heating up the atmosphere of Jupiter. 510 00:29:30,800 --> 00:29:34,720 There are parts of it that are many times warmer than we can explain with sunlight. 511 00:29:34,800 --> 00:29:37,680 The question is, of course, where is that energy coming from? 512 00:29:39,240 --> 00:29:42,200 Juno swoops in for another pass on Jupiter, 513 00:29:42,280 --> 00:29:46,040 turning its high resolution cameras on the raging storm below. 514 00:29:48,440 --> 00:29:50,840 The storm unleashes vicious turbulence 515 00:29:50,920 --> 00:29:53,080 into the surrounding atmosphere, 516 00:29:53,160 --> 00:29:55,360 giving scientists the clue they need 517 00:29:55,440 --> 00:29:57,960 to explain the planet's high temperature. 518 00:29:59,200 --> 00:30:02,360 The Great Red Spot is a giant hurricane 519 00:30:02,440 --> 00:30:06,880 that's powered by heat deep in the core of Jupiter. 520 00:30:06,960 --> 00:30:10,880 But it has such violent and chaotic motion, 521 00:30:10,960 --> 00:30:13,000 it's mixing up the atmosphere around it. 522 00:30:16,760 --> 00:30:20,520 The thunder storms on Jupiter are gonna be generating booming thunder 523 00:30:20,600 --> 00:30:22,720 just the same way they do here on the Earth. 524 00:30:24,680 --> 00:30:26,800 Thunder clouds and sound waves 525 00:30:26,880 --> 00:30:28,880 rippling through the storm. 526 00:30:31,720 --> 00:30:34,680 A sound wave is 527 00:30:34,760 --> 00:30:37,680 a wave of pressure, of compression, 528 00:30:37,760 --> 00:30:42,240 where air molecules or water molecules get compacted. 529 00:30:42,320 --> 00:30:45,440 They get squeezed together. When you squeeze something together, 530 00:30:45,520 --> 00:30:48,480 they are lot closer together and they're gonna get pretty hot. 531 00:30:51,240 --> 00:30:55,200 These sound waves shoot up 500 miles above the storm 532 00:30:56,440 --> 00:30:59,440 where they break, converting sound energy into heat. 533 00:31:00,840 --> 00:31:03,600 The sound waves, they crash together 534 00:31:03,680 --> 00:31:07,000 creating tremendous amount of energy, heating the gases around them. 535 00:31:09,600 --> 00:31:12,760 The Great Red Spot has helped heat the Jovian atmosphere 536 00:31:12,840 --> 00:31:14,840 for hundreds of years. 537 00:31:14,920 --> 00:31:19,280 But new images suggest that this may be about to change. 538 00:31:20,600 --> 00:31:25,560 Jupiter's red spot is so big, it's bigger than Earth by a long shot. 539 00:31:25,640 --> 00:31:28,680 It seems like it would be an incredibly stable thing. 540 00:31:28,760 --> 00:31:31,960 It's just there and it's always been there and it always will be. 541 00:31:32,040 --> 00:31:34,120 Recently we've seen it changing. 542 00:31:36,040 --> 00:31:40,600 When NASA's Voyager Space Probe visited Jupiter in 1979, 543 00:31:40,680 --> 00:31:44,800 it observed a storm twice the diameter of the Earth. 544 00:31:44,880 --> 00:31:46,880 In 2017, 545 00:31:46,960 --> 00:31:49,800 Juno's images showed the Great Red Spot 546 00:31:49,880 --> 00:31:52,760 has lost one-third of its width. 547 00:31:52,840 --> 00:31:54,840 But that's not all. 548 00:31:54,920 --> 00:31:57,760 Despite the storm's shrinking size, 549 00:31:57,840 --> 00:32:00,640 it's actually getting taller. 550 00:32:00,720 --> 00:32:03,560 The Great Red Spot is being stretched and forced 551 00:32:03,640 --> 00:32:06,640 into Jupiter's upper atmosphere. 552 00:32:06,720 --> 00:32:09,440 The storms in the Great Red Spot is kind of like 553 00:32:09,520 --> 00:32:11,600 the clay on a potter's wheel where, 554 00:32:11,680 --> 00:32:14,880 as you bring your hands closer together to draw the clay in, 555 00:32:14,960 --> 00:32:18,080 the closer your hands are, the taller the pottery becomes. 556 00:32:18,160 --> 00:32:21,760 And similarly for the storm, as it becomes smaller at the base 557 00:32:21,840 --> 00:32:24,040 it raises taller to the upper atmosphere. 558 00:32:25,480 --> 00:32:29,920 It's getting taller. And we see storms do the same thing on Earth and when it does that 559 00:32:30,000 --> 00:32:33,760 the wind shear will take the top of the storm off and drag it apart. 560 00:32:33,840 --> 00:32:36,320 So we'll be watching it over the next few years 561 00:32:36,400 --> 00:32:38,920 to see if that's what happens on Jupiter as well. 562 00:32:40,640 --> 00:32:44,400 It may be only a matter of time before Jupiter's high altitude winds 563 00:32:44,480 --> 00:32:47,440 tear the iconic storm to shreds. 564 00:32:47,520 --> 00:32:52,480 The most famous storm of our solar system may soon disappear. 565 00:32:52,560 --> 00:32:55,040 But Juno reveals other storms 566 00:32:55,120 --> 00:32:57,960 hidden in the strangest of places. 567 00:33:04,160 --> 00:33:06,520 NASA's Juno probe has voyaged 568 00:33:06,600 --> 00:33:09,600 billions of miles across the solar system, 569 00:33:09,680 --> 00:33:12,960 to reveal the mysteries of gas giant Jupiter. 570 00:33:13,040 --> 00:33:18,000 But there's one part of Jupiter that has remained hidden until now. 571 00:33:18,080 --> 00:33:20,880 Before Juno, our view of Jupiter was very limited. 572 00:33:20,960 --> 00:33:23,120 We'd never actually flown over the poles. 573 00:33:23,200 --> 00:33:25,560 It's something that's very hard to do on Jupiter. 574 00:33:25,640 --> 00:33:28,520 We don't have other missions that have done this. 575 00:33:28,600 --> 00:33:30,920 In August, 2016, 576 00:33:31,000 --> 00:33:35,400 Juno's flight plan takes the spacecraft into unknown territory 577 00:33:35,480 --> 00:33:39,960 to reveal Jupiter's mysterious Polar regions for the first time. 578 00:33:41,120 --> 00:33:43,320 The first time we looked at the pole, 579 00:33:43,400 --> 00:33:46,360 it didn't look anything like the Jupiter we knew. 580 00:33:48,880 --> 00:33:50,880 We never would've guessed that was Jupiter 581 00:33:50,960 --> 00:33:52,960 if somebody had shown that to us. 582 00:33:55,240 --> 00:33:59,640 Juno's camera reveals a strange blue expanse that puzzle scientists. 583 00:34:02,640 --> 00:34:06,880 The electric colour could be due to chemical changes in the clouds 584 00:34:06,960 --> 00:34:09,200 brought on by a lack of sunlight. 585 00:34:09,280 --> 00:34:13,280 But what Juno spots inside the blue clouds is even stranger. 586 00:34:16,840 --> 00:34:19,560 Giant central cyclones spin around each pole 587 00:34:19,640 --> 00:34:22,000 at 200 miles per hour. 588 00:34:22,080 --> 00:34:26,680 With these cyclones surrounded by eight stormy vortices in the North, 589 00:34:26,760 --> 00:34:28,760 and five in the South. 590 00:34:31,720 --> 00:34:35,240 There are these weird cyclones, gigantic swirls, 591 00:34:35,320 --> 00:34:38,760 vortices of gas swirling around Jupiter's poles 592 00:34:38,840 --> 00:34:41,160 and they're clearly forming patterns. 593 00:34:42,200 --> 00:34:44,240 It's hard to get a sense of scale here. 594 00:34:44,320 --> 00:34:47,720 The North Polar central cyclone, that one right at the pole, 595 00:34:47,800 --> 00:34:50,200 that's 2,500 miles across. 596 00:34:50,280 --> 00:34:53,600 That is almost as big as the Continental United States. 597 00:34:53,680 --> 00:34:55,880 What is going on there? 598 00:34:55,960 --> 00:34:58,280 This is nothing like what we see on Earth. 599 00:35:01,200 --> 00:35:03,200 On Earth our weather is 600 00:35:03,280 --> 00:35:05,360 driven by heat from the sun. 601 00:35:05,440 --> 00:35:07,840 It hits our planet at the equator 602 00:35:07,920 --> 00:35:10,680 and flows across the surface. 603 00:35:10,760 --> 00:35:14,400 Powerful cyclones form over tropical waters 604 00:35:14,480 --> 00:35:16,920 and move around the planet. 605 00:35:17,000 --> 00:35:20,880 But the polar regions receive less energy from the sun, 606 00:35:20,960 --> 00:35:23,640 so cyclones can't form at the poles. 607 00:35:24,640 --> 00:35:28,200 We see that if you're at the equator, it's warmer, it's stormier. 608 00:35:28,280 --> 00:35:31,960 If you're at the poles, where the sun is slightly harder to see, 609 00:35:32,040 --> 00:35:34,480 that activity goes away. 610 00:35:34,560 --> 00:35:38,520 But the weather on Jupiter couldn't be more different. 611 00:35:38,600 --> 00:35:40,760 We see lightning and convective thunderstorms 612 00:35:40,840 --> 00:35:43,080 at the poles of Jupiter but not at the equator. 613 00:35:43,160 --> 00:35:45,840 That's sort of the opposite of what we see on the Earth. 614 00:35:45,920 --> 00:35:48,680 Question is, what's driving Jupiter's storms? 615 00:35:50,880 --> 00:35:54,680 Jupiter is five times further from the sun than the Earth 616 00:35:54,760 --> 00:35:57,960 and receives only a fraction of the sun's energy. 617 00:35:58,040 --> 00:36:01,160 And unlike Earth, Jupiter's polar regions 618 00:36:01,240 --> 00:36:03,640 seem to be where the action is. 619 00:36:03,720 --> 00:36:07,200 Something is driving the planet's weird weather 620 00:36:07,280 --> 00:36:11,240 and Juno's scans of the giant planet's thermo emissions 621 00:36:11,320 --> 00:36:14,400 suggest it could be Jupiter itself. 622 00:36:14,480 --> 00:36:19,000 You can actually see the internal heat of Jupiter coming right up through. 623 00:36:19,080 --> 00:36:23,360 And so, Jupiter will look very bright in areas where we can see that heat. 624 00:36:24,680 --> 00:36:29,720 Juno detects searing heat beneath Jupiter's cloud bands. 625 00:36:29,800 --> 00:36:31,800 Jupiter has so much material. 626 00:36:31,880 --> 00:36:34,440 So much mass, so much gravity that the interior 627 00:36:34,520 --> 00:36:37,160 is incredibly dense and very, very hot. 628 00:36:37,240 --> 00:36:40,160 At the core it's probably many thousands of degrees hotter 629 00:36:40,240 --> 00:36:42,240 than the surface of the sun. 630 00:36:43,280 --> 00:36:46,760 This fiery inferno buried in Jupiter's dark heart 631 00:36:46,840 --> 00:36:48,880 is a relic from its birth, 632 00:36:48,960 --> 00:36:50,960 billions of years ago. 633 00:36:51,040 --> 00:36:53,760 The violent collisions that formed the planet 634 00:36:53,840 --> 00:36:56,320 leave its core seething hot, 635 00:36:56,400 --> 00:36:58,720 a heat that remains to this day, 636 00:36:58,800 --> 00:37:02,760 buried under thousands of miles of insulating gas. 637 00:37:02,840 --> 00:37:05,480 As the heat slowly leaks outwards, 638 00:37:05,560 --> 00:37:08,040 Jupiter's fast rotating atmosphere 639 00:37:08,120 --> 00:37:12,920 gets churned up into vicious cyclones and thunderstorms. 640 00:37:13,000 --> 00:37:15,480 That's what's really driving most of the weather. 641 00:37:15,560 --> 00:37:17,840 It's not the sun, it's Jupiter itself. 642 00:37:19,840 --> 00:37:22,560 And as Juno soars above the planet, 643 00:37:22,640 --> 00:37:25,200 it reveals another weather mystery. 644 00:37:25,280 --> 00:37:28,320 The craft detects bursts of radio waves, 645 00:37:28,400 --> 00:37:31,720 spiking up to four times a second, 646 00:37:31,800 --> 00:37:35,920 a tell-tale sign of ferocious lightning strikes. 647 00:37:38,440 --> 00:37:41,760 Clouds are moving around in the atmosphere, building up electric charge 648 00:37:41,840 --> 00:37:44,120 and causing bolts of lightning to form. 649 00:37:44,200 --> 00:37:47,800 And we've actually seen this with the Juno spacecraft. 650 00:37:47,880 --> 00:37:50,200 These are mega-storms, 651 00:37:50,280 --> 00:37:52,520 orders of magnitude bigger than here on Earth. 652 00:37:56,840 --> 00:38:00,600 And Juno finds that there's more to these thunderclouds 653 00:38:00,680 --> 00:38:03,120 than just flashes of light, 654 00:38:03,200 --> 00:38:06,440 giant icy hail stones of water and ammonia, 655 00:38:06,520 --> 00:38:11,520 that chemical which gives Jupiter's clouds their orange colour. 656 00:38:15,120 --> 00:38:18,080 High up in Jupiter's atmosphere, the ammonia 657 00:38:18,160 --> 00:38:20,440 is mixing with the water 658 00:38:20,520 --> 00:38:25,280 and it becomes a liquid ball that starts to collect ice around it 659 00:38:25,360 --> 00:38:27,600 and it will fall like hail does, 660 00:38:27,680 --> 00:38:29,800 deep into Jupiter's atmosphere. 661 00:38:31,280 --> 00:38:33,840 On Earth hail falls to the ground. 662 00:38:33,920 --> 00:38:36,520 But on Jupiter, there is no ground. 663 00:38:38,160 --> 00:38:41,280 It gets lifted in the atmosphere because of an updraft 664 00:38:41,360 --> 00:38:43,400 and then more ice and it builds bigger 665 00:38:43,480 --> 00:38:46,120 and then it falls down and then it gets carried back up. 666 00:38:46,200 --> 00:38:49,760 So hail's often many layers being built. 667 00:38:51,720 --> 00:38:55,000 These icy balls grow layer by layer 668 00:38:55,080 --> 00:38:57,440 as they soar up and down the atmosphere. 669 00:38:57,520 --> 00:39:00,120 If they formed in storms here on Earth, 670 00:39:00,200 --> 00:39:02,200 they'd cause some serious damage. 671 00:39:03,840 --> 00:39:06,240 So if you were buzzing around Jupiter 672 00:39:06,320 --> 00:39:09,000 and you were near where these storms were, 673 00:39:09,080 --> 00:39:12,040 you might get hit by hail coming up or going down. 674 00:39:13,040 --> 00:39:15,040 This is one of the most 675 00:39:15,120 --> 00:39:19,320 violent energetic atmospheres in the entire solar system. 676 00:39:21,280 --> 00:39:25,000 Juno is revealing Jupiter's hidden secrets. 677 00:39:30,600 --> 00:39:34,720 On Earth dazzling auroras light up the skies 678 00:39:34,800 --> 00:39:37,080 as charged particles from the sun 679 00:39:37,160 --> 00:39:40,040 interact with atoms high in the atmosphere. 680 00:39:41,320 --> 00:39:43,600 Deep in the outer solar system, 681 00:39:43,680 --> 00:39:45,880 Jupiter's too far from the sun 682 00:39:45,960 --> 00:39:49,000 for strong auroras to form in this way. 683 00:39:49,080 --> 00:39:52,560 But high above the giant planet's poles, 684 00:39:52,640 --> 00:39:56,640 Juno spots a seemingly impossible light show. 685 00:39:58,960 --> 00:40:00,960 The auroras of Jupiter are 686 00:40:01,040 --> 00:40:03,840 tremendously larger than the ones we find here on Earth. 687 00:40:03,920 --> 00:40:08,200 In fact, the aurora rings at the poles are bigger than our planet itself. 688 00:40:08,280 --> 00:40:12,000 Jupiter's auroras emit primarily ultraviolet and X-ray light. 689 00:40:12,080 --> 00:40:14,480 So you can't see it with the naked human eye. 690 00:40:14,560 --> 00:40:17,480 But if you could see them and you were at Jupiter, 691 00:40:17,560 --> 00:40:20,360 that would be an amazing light show. 692 00:40:20,440 --> 00:40:23,160 Because those auroras are strong. 693 00:40:26,000 --> 00:40:28,280 These glowing displays are evidence of 694 00:40:28,360 --> 00:40:31,480 charged particles slamming into Jupiter's atmosphere. 695 00:40:33,160 --> 00:40:35,680 But if they're not coming from the sun... 696 00:40:35,760 --> 00:40:38,160 where are they coming from? 697 00:40:38,240 --> 00:40:40,280 Hunting for an answer 698 00:40:40,360 --> 00:40:43,360 Juno snaps an image of Jupiter's southern lights 699 00:40:43,440 --> 00:40:46,680 with its ultraviolet imaging spectrometer. 700 00:40:46,760 --> 00:40:50,440 Inside the aurora it glimpses something strange. 701 00:40:51,720 --> 00:40:56,200 When Juno studied the lights coming from the aurora on Jupiter, 702 00:40:56,280 --> 00:40:59,480 it found that they were even stronger than expected. 703 00:40:59,560 --> 00:41:02,760 And, in fact, when you look at Jupiter's poles in wavelengths 704 00:41:02,840 --> 00:41:05,600 that our eyes can't see, for example ultraviolet, 705 00:41:05,680 --> 00:41:07,680 you see a hot spot. 706 00:41:08,800 --> 00:41:11,200 This hot spot marks the point where 707 00:41:11,280 --> 00:41:13,840 huge concentrations of charged particles 708 00:41:13,920 --> 00:41:15,920 strike Jupiter's atmosphere. 709 00:41:16,000 --> 00:41:18,000 Tracing their trajectory 710 00:41:18,080 --> 00:41:21,920 reveals the culprit of Jupiter's dazzling light shows, 711 00:41:22,000 --> 00:41:24,840 the volcanoes of Jupiter's powerful moons. 712 00:41:27,360 --> 00:41:31,880 Jupiter's moon Io has hundreds of active volcanoes spewing out materials 713 00:41:31,960 --> 00:41:33,960 way out into space and many of those get 714 00:41:34,040 --> 00:41:36,840 trapped by the magnetic fired of Jupiter. 715 00:41:36,920 --> 00:41:38,960 Io's volcanoes 716 00:41:39,040 --> 00:41:41,520 fire out jets of charged particles 717 00:41:41,600 --> 00:41:45,480 which are swept up by the giant planet's magnetic field. 718 00:41:45,560 --> 00:41:49,360 It's funnelling those particles down and slamming into specific spots 719 00:41:49,440 --> 00:41:51,920 in Jupiter's atmosphere. 720 00:41:52,000 --> 00:41:54,760 But Io isn't the only moon responsible for 721 00:41:54,840 --> 00:41:57,360 Jupiter's polar light show. 722 00:41:57,440 --> 00:41:59,680 If we go further out, Europa, 723 00:41:59,760 --> 00:42:02,400 Ganymede, Callisto, those are more icy, 724 00:42:02,480 --> 00:42:05,240 don't necessarily have volcanoes. 725 00:42:05,320 --> 00:42:09,160 These icy moons twist up Jupiter's magnetic field. 726 00:42:10,160 --> 00:42:12,200 Some of these moons have magnetic fields 727 00:42:12,280 --> 00:42:14,400 that interact with Jupiter's magnetic field. 728 00:42:14,480 --> 00:42:18,200 And that actually intensifies the aurora display on Jupiter. 729 00:42:19,680 --> 00:42:22,200 Jupiter's moons work together to energise 730 00:42:22,280 --> 00:42:25,880 the greatest northern lights in the solar system. 731 00:42:25,960 --> 00:42:28,320 But in these beautiful displays 732 00:42:28,400 --> 00:42:32,120 is a stark reminder of the danger Juno faces. 733 00:42:32,200 --> 00:42:35,600 When you look at these pictures of the aurora on Jupiter and you think, 734 00:42:35,680 --> 00:42:38,440 "That's beautiful. Wouldn't it be great to see in person?" 735 00:42:38,520 --> 00:42:42,360 The answer is, "No. No, it wouldn't. Because they would kill you." 736 00:42:42,440 --> 00:42:44,480 What's causing these displays 737 00:42:44,560 --> 00:42:48,560 are subatomic particles accelerated to tremendously high speeds 738 00:42:48,640 --> 00:42:51,000 by the magnetic fields involved. 739 00:42:52,080 --> 00:42:54,920 The radiation around Jupiter is lethal. 740 00:42:56,600 --> 00:42:58,600 The lifetime of the Juno mission is 741 00:42:58,680 --> 00:43:02,160 very limited by the extreme conditions it has to survive in. 742 00:43:02,240 --> 00:43:04,600 We think that in the future all of the instruments 743 00:43:04,680 --> 00:43:07,120 will be so radiated they won't really work any more. 744 00:43:09,320 --> 00:43:11,800 When Juno's titanium armour fails, 745 00:43:11,880 --> 00:43:15,840 Jupiter's deadly radiation will damage the craft beyond repair. 746 00:43:18,120 --> 00:43:20,880 So the team plans to go out with a bang, 747 00:43:20,960 --> 00:43:24,000 thrusting Juno into Jupiter's atmosphere 748 00:43:24,080 --> 00:43:26,080 where the craft will be torn apart. 749 00:43:27,640 --> 00:43:30,960 Eventually it will be drawn down into Jupiter's depths 750 00:43:31,040 --> 00:43:33,080 and become a part of the planet itself. 751 00:43:34,320 --> 00:43:37,920 Before then, Juno has many more mysteries to unlock. 752 00:43:39,280 --> 00:43:42,280 We'll answer some questions and we'll raise some more, 753 00:43:42,360 --> 00:43:45,880 that's what I expect, and we'll get some fantastic images. 754 00:43:47,520 --> 00:43:50,240 Every single thing has turned out to be a surprise. 755 00:43:50,320 --> 00:43:53,240 There're so many things that Juno has opened our eyes to 756 00:43:53,320 --> 00:43:56,400 that I can't imagine having not sent it. 757 00:43:56,480 --> 00:43:58,480 So we're in for at least a year more 758 00:43:58,560 --> 00:44:01,640 of the most profound surprises about Jupiter. 759 00:44:01,720 --> 00:44:04,680 What we're learning, what we're unlocking, 760 00:44:04,760 --> 00:44:08,240 not just about Jupiter, but the formation of the solar system 761 00:44:08,320 --> 00:44:11,320 and the potential formation of life itself here on Earth... 762 00:44:11,680 --> 00:44:12,680 It's mind-blowing. 763 00:44:12,760 --> 00:44:14,760 subtitles by Deluxe 64152

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