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These are the user uploaded subtitles that are being translated: 1 00:00:03,520 --> 00:00:05,896 NASA's revolutionary Juno probe 2 00:00:05,920 --> 00:00:08,006 is on a daring voyage to Jupiter. 3 00:00:08,030 --> 00:00:10,936 Its goal... to reveal the the deepest mysteries 4 00:00:10,960 --> 00:00:14,176 of our solar system. 5 00:00:14,200 --> 00:00:17,006 Everything we see in the solar system today 6 00:00:17,030 --> 00:00:20,776 is affected by Jupiter somehow in the past or now, 7 00:00:20,800 --> 00:00:22,816 all the asteroids, all the planets, 8 00:00:22,840 --> 00:00:26,016 the moons, the comets, everything. 9 00:00:26,040 --> 00:00:28,656 So in many ways, Juno is actually giving us a view 10 00:00:28,680 --> 00:00:30,626 into the history of our planetary system, 11 00:00:30,650 --> 00:00:33,256 even the history of Earth. 12 00:00:33,280 --> 00:00:35,696 Juno's mission is risky. 13 00:00:35,720 --> 00:00:39,466 Jupiter could eat the spacecraft like that. 14 00:00:39,490 --> 00:00:41,536 But by diving perilously close 15 00:00:41,560 --> 00:00:43,566 to this monstrous world, 16 00:00:43,590 --> 00:00:48,306 Juno could change everything we know about our solar system. 17 00:00:48,330 --> 00:00:49,746 If you want to know what's happening, 18 00:00:49,770 --> 00:00:51,600 you got to get up close and personal. 19 00:00:59,640 --> 00:01:02,686 Captions by vitac... www.vitac.com 20 00:01:02,710 --> 00:01:05,710 captions paid for by discovery communications 21 00:01:07,220 --> 00:01:10,726 Independence day, 2016... 22 00:01:10,750 --> 00:01:13,496 Juno arrives at Jupiter 23 00:01:13,520 --> 00:01:15,766 and gets to work. 24 00:01:15,790 --> 00:01:18,036 The probe angles its high-resolution camera 25 00:01:18,060 --> 00:01:21,206 towards this stormy world. 26 00:01:21,230 --> 00:01:24,700 Juno's snaps do not disappoint. 27 00:01:29,110 --> 00:01:32,610 The images returned from Juno are just beautiful. 28 00:01:43,150 --> 00:01:45,496 Suddenly you have this magnificent mosaic 29 00:01:45,520 --> 00:01:46,620 of this planet. 30 00:01:52,460 --> 00:01:54,806 As a human being, I'm like, "oh, my gosh, look at this. 31 00:01:54,830 --> 00:01:58,316 This is amazing. This is coming back from Jupiter." 32 00:01:58,340 --> 00:02:00,616 These are the closest-ever views 33 00:02:00,640 --> 00:02:05,010 of Jupiter, a world 500 million miles away. 34 00:02:15,020 --> 00:02:19,236 But we didn't send Juno just to take pictures. 35 00:02:19,260 --> 00:02:24,936 One of its main goals is to peer deep into Jupiter's dark heart. 36 00:02:24,960 --> 00:02:27,606 One of the big questions we have about Jupiter is, 37 00:02:27,630 --> 00:02:29,706 does it have a core? 38 00:02:29,730 --> 00:02:31,306 And you'd think, well, of course it has a core 39 00:02:31,330 --> 00:02:32,716 like every planet has a core. 40 00:02:32,740 --> 00:02:35,316 The Earth has a core. Everything does. 41 00:02:35,340 --> 00:02:40,086 Well, it turns out, Jupiter might not. 42 00:02:40,110 --> 00:02:42,126 Knowing what lies at a planet's core 43 00:02:42,150 --> 00:02:46,156 allows scientists to wind back the clock billions of years 44 00:02:46,180 --> 00:02:50,566 to the formation of the planets. 45 00:02:50,590 --> 00:02:54,236 If Juno can reveal what lies deep within Jupiter, 46 00:02:54,260 --> 00:02:56,136 it could change our understanding 47 00:02:56,160 --> 00:03:00,476 of how the gas giant formed. 48 00:03:00,500 --> 00:03:03,776 If Juno finds a solid core, it could mean 49 00:03:03,800 --> 00:03:07,246 Jupiter first formed as a rocky planet like earth 50 00:03:07,270 --> 00:03:09,816 then kept growing, 51 00:03:09,840 --> 00:03:12,786 but if Juno finds no core, 52 00:03:12,810 --> 00:03:15,826 it could mean that Jupiter skipped the rocky stage 53 00:03:15,850 --> 00:03:18,680 and formed straight from a cloud of gas. 54 00:03:20,920 --> 00:03:23,666 Answering this question could shine a light 55 00:03:23,690 --> 00:03:26,136 on other mysteries, too. 56 00:03:26,160 --> 00:03:28,336 If we can figure out how Jupiter formed, 57 00:03:28,360 --> 00:03:32,030 we can figure out the rest of the story of the solar system. 58 00:03:34,500 --> 00:03:37,676 So how do you probe down into the interior of a planet 59 00:03:37,700 --> 00:03:40,746 when all you can really see are the very tops of the clouds? 60 00:03:40,770 --> 00:03:43,446 Well, incredibly, you can use gravity. 61 00:03:43,470 --> 00:03:47,556 As Juno orbits Jupiter, 62 00:03:47,580 --> 00:03:50,486 it can sense in its orbit 63 00:03:50,510 --> 00:03:52,196 tiny little variations 64 00:03:52,220 --> 00:03:56,196 in the gravitational pull of Jupiter. 65 00:03:56,220 --> 00:03:58,336 As Juno speeds around Jupiter, 66 00:03:58,360 --> 00:04:01,566 gravitational spikes tug on the craft. 67 00:04:01,590 --> 00:04:06,606 Turns out, some parts of Jupiter are denser than others. 68 00:04:06,630 --> 00:04:10,106 If Jupiter were some solid ball, then as Juno passes by it, 69 00:04:10,130 --> 00:04:13,046 as it passes very close above its cloud tops, 70 00:04:13,070 --> 00:04:15,816 the orbit, the trajectory would be very smooth, 71 00:04:15,840 --> 00:04:18,516 but in fact, if Jupiter has layers, 72 00:04:18,540 --> 00:04:20,786 or places where there is more mass 73 00:04:20,810 --> 00:04:23,956 and places where there's less, then it's gonna pull on Juno 74 00:04:23,980 --> 00:04:26,356 a little bit differently. 75 00:04:26,380 --> 00:04:29,296 Passing over areas of concentrated mass 76 00:04:29,320 --> 00:04:32,636 gives Juno a speed boost. 77 00:04:32,660 --> 00:04:35,166 So what they do is, the engineers back on earth 78 00:04:35,190 --> 00:04:36,406 can basically just say, 79 00:04:36,430 --> 00:04:38,376 "how fast is it moving right now? 80 00:04:38,400 --> 00:04:40,036 How about now? How about now?" 81 00:04:40,060 --> 00:04:44,846 And you build up a map of where the mass is in Jupiter 82 00:04:44,870 --> 00:04:50,086 underneath the spacecraft as it passes around. 83 00:04:50,110 --> 00:04:52,316 Juno's instruments begin to map out 84 00:04:52,340 --> 00:04:55,026 the heart of gas giant, 85 00:04:55,050 --> 00:04:59,996 revealing the mysterious core for the first time. 86 00:05:00,020 --> 00:05:02,496 What Juno found was this amorphous mass, 87 00:05:02,520 --> 00:05:05,036 a fuzzy thing in the center of Jupiter. 88 00:05:05,060 --> 00:05:07,796 It's not as solid as we expected 89 00:05:07,820 --> 00:05:10,066 if it were just a metal and rock core, 90 00:05:10,090 --> 00:05:13,876 but there is something there. 91 00:05:13,900 --> 00:05:15,376 In the center of the planet, 92 00:05:15,400 --> 00:05:18,316 Juno detects hydrogen and rocky material 93 00:05:18,340 --> 00:05:22,086 dissolved and blended together. 94 00:05:22,110 --> 00:05:25,786 It's a type of planetary core we've never seen before. 95 00:05:25,810 --> 00:05:29,426 Astronomers describe it as fuzzy. 96 00:05:29,450 --> 00:05:31,356 We thought we were gonna find an avocado. 97 00:05:31,380 --> 00:05:34,326 Instead, we found a bowl of chili. 98 00:05:34,350 --> 00:05:37,820 It's a hydrogen fluid chili con carne. 99 00:05:40,320 --> 00:05:42,806 So none of our models of the interior of Jupiter 100 00:05:42,830 --> 00:05:44,266 turned out to be correct. 101 00:05:44,290 --> 00:05:48,346 That means we have to go back to the drawing board. 102 00:05:48,370 --> 00:05:50,106 One theory is that Jupiter 103 00:05:50,130 --> 00:05:53,176 didn't form from rocks or gas 104 00:05:53,200 --> 00:05:56,416 but from tiny pebbles less than an inch wide strewn 105 00:05:56,440 --> 00:06:02,126 across the early solar system 4.6 billion years ago. 106 00:06:02,150 --> 00:06:03,626 These pebbles came together. 107 00:06:03,650 --> 00:06:06,956 They accreted to form a massive object 108 00:06:06,980 --> 00:06:11,396 that was the sort of seed, the core of Jupiter. 109 00:06:11,420 --> 00:06:12,836 The swarm of pebbles 110 00:06:12,860 --> 00:06:16,266 clumped together to form one giant core 111 00:06:16,290 --> 00:06:18,836 20 times the mass of Earth, 112 00:06:18,860 --> 00:06:23,246 but these pebbles can't sustain this growing planet for long. 113 00:06:23,270 --> 00:06:24,476 Eventually, we need to make a jump 114 00:06:24,500 --> 00:06:26,146 from those centimeter-size particles 115 00:06:26,170 --> 00:06:30,016 up to really large things, like 100-kilometer planetesimals, 116 00:06:30,040 --> 00:06:32,870 to really kick-start growth of a planet. 117 00:06:35,750 --> 00:06:40,356 As Jupiter grows, its appetite becomes insatiable. 118 00:06:40,380 --> 00:06:42,866 The cores of other would-be planets are drawn in 119 00:06:42,890 --> 00:06:46,666 by its immense pull and absorb on impact, 120 00:06:46,690 --> 00:06:51,136 causing Jupiter's core to transform. 121 00:06:51,160 --> 00:06:54,976 Huge chunks of incoming rock are mixed up with gas 122 00:06:55,000 --> 00:06:58,576 and the pebbles that originally built the core. 123 00:06:58,600 --> 00:07:01,886 We think that core material that might've been there is actually 124 00:07:01,910 --> 00:07:05,856 dissolved and mixed in with the rest of the planet. 125 00:07:05,880 --> 00:07:08,856 This mix of rock, gas, and pebbles 126 00:07:08,880 --> 00:07:11,626 leaves the core in a strange state 127 00:07:11,650 --> 00:07:14,926 somewhere between solid and liquid 128 00:07:14,950 --> 00:07:17,896 or, in other words, fuzzy. 129 00:07:17,920 --> 00:07:20,436 Once Jupiter's core reaches a critical mass, 130 00:07:20,460 --> 00:07:24,936 its gravity pulls in all nearby hydrogen gas, 131 00:07:24,960 --> 00:07:27,806 building the Jovian atmosphere 132 00:07:27,830 --> 00:07:30,106 and leaving the fuzzy core 133 00:07:30,130 --> 00:07:34,146 trapped beneath thousands of miles of thick clouds. 134 00:07:34,170 --> 00:07:38,786 And that is what formed Jupiter as we know and love it today. 135 00:07:38,810 --> 00:07:41,716 Juno's discovery of Jupiter's fuzzy core 136 00:07:41,740 --> 00:07:43,186 could rewrite the book on 137 00:07:43,210 --> 00:07:47,796 Jupiter's early years, but Juno is just getting started. 138 00:07:47,820 --> 00:07:50,166 We haven't even scratched the surface 139 00:07:50,190 --> 00:07:54,996 of the number of mysteries there are. 140 00:07:55,020 --> 00:07:57,406 There's more to Jupiter than meets the eye 141 00:07:57,430 --> 00:08:01,436 as Juno's instruments begin to reveal a darker side 142 00:08:01,460 --> 00:08:03,746 to this giant world. 143 00:08:03,770 --> 00:08:06,816 Jupiter's environment is one of the most vicious 144 00:08:06,840 --> 00:08:09,246 in the solar system, and that's because 145 00:08:09,270 --> 00:08:12,686 of its incredibly strong magnetic field. 146 00:08:12,710 --> 00:08:17,680 And Juno is caught right in the middle of it. 147 00:08:30,360 --> 00:08:31,736 The gas giant Jupiter 148 00:08:31,760 --> 00:08:36,476 holds clues to the mysteries of our solar system, 149 00:08:36,500 --> 00:08:38,176 and in 2011, 150 00:08:38,200 --> 00:08:41,886 NASA launched a billion-dollar mission to uncover them. 151 00:08:41,910 --> 00:08:46,156 Three, two, one, ignition. 152 00:08:46,180 --> 00:08:49,086 And liftoff of the Atlas V 153 00:08:49,110 --> 00:08:53,226 with Juno on a trek to Jupiter. 154 00:08:53,250 --> 00:08:54,556 To reach its target, 155 00:08:54,580 --> 00:08:57,250 Juno embarks on a five-year journey. 156 00:09:00,360 --> 00:09:02,666 Sending any spacecraft to another planet 157 00:09:02,690 --> 00:09:05,876 is gonna be tough, but sending one to Jupiter 158 00:09:05,900 --> 00:09:10,246 is really pushing things pretty hard. 159 00:09:10,270 --> 00:09:12,646 Juno weaves through the solar system 160 00:09:12,670 --> 00:09:15,286 with extreme precision. 161 00:09:15,310 --> 00:09:18,046 The craft battles violent temperature changes 162 00:09:18,070 --> 00:09:21,186 and navigates carefully through the asteroid belt. 163 00:09:21,210 --> 00:09:23,956 If there's a fleck of dust in your path 164 00:09:23,980 --> 00:09:26,026 and that thing slams into your spacecraft, 165 00:09:26,050 --> 00:09:28,766 it could do significant damage. 166 00:09:28,790 --> 00:09:31,796 1.7 billion miles into its mission, 167 00:09:31,820 --> 00:09:36,336 Juno finally nears its target, 168 00:09:36,360 --> 00:09:39,736 but the probe is hurtling towards Jupiter 169 00:09:39,760 --> 00:09:42,546 at 165,000 miles an hour. 170 00:09:42,570 --> 00:09:44,846 Juno is moving really fast. 171 00:09:44,870 --> 00:09:47,546 It's one of the fastest spacecraft ever. 172 00:09:47,570 --> 00:09:50,016 You need to go fast enough to get there, but then you need 173 00:09:50,040 --> 00:09:52,886 to be slow enough to be captured by the gravity of the planet. 174 00:09:52,910 --> 00:09:55,426 You need to get it just right. 175 00:09:55,450 --> 00:09:56,656 Entering orbit around 176 00:09:56,680 --> 00:09:59,456 Jupiter is the trickiest part of the mission. 177 00:09:59,480 --> 00:10:02,766 Get it wrong and Juno could slam into the planet 178 00:10:02,790 --> 00:10:06,566 or drift out into deep space. 179 00:10:06,590 --> 00:10:09,506 To successfully get Juno to enter a stable orbit around 180 00:10:09,530 --> 00:10:12,176 Jupiter as almost the same as, say, 181 00:10:12,200 --> 00:10:14,176 shooting a basketball from London 182 00:10:14,200 --> 00:10:16,846 and having it on the land on the front of the rim in New York 183 00:10:16,870 --> 00:10:19,116 and just sitting there balanced. 184 00:10:19,140 --> 00:10:23,440 I could do it, but can NASA do it with Juno? 185 00:10:27,480 --> 00:10:29,586 NASA has a neat game plan. 186 00:10:29,610 --> 00:10:32,326 Juno performs a backflip in space 187 00:10:32,350 --> 00:10:35,466 and fires its thruster towards Jupiter. 188 00:10:35,490 --> 00:10:37,096 Everything is going smoothly. 189 00:10:37,120 --> 00:10:41,166 We're continuing to burn and change our velocity. 190 00:10:41,190 --> 00:10:44,706 The rocket burns for 35 nail-biting minutes, 191 00:10:44,730 --> 00:10:49,060 reducing the craft's speed by 1,200 miles an hour. 192 00:10:55,300 --> 00:10:59,016 Finally, the probe achieves orbit around Jupiter. 193 00:10:59,040 --> 00:11:01,416 Right on July 4th during the fireworks 194 00:11:01,440 --> 00:11:02,686 we just got into orbit. 195 00:11:02,710 --> 00:11:05,326 In many ways, we're firing a rocket motor. 196 00:11:05,350 --> 00:11:09,826 I mean, it is fireworks. 197 00:11:09,850 --> 00:11:10,996 Safe in orbit, 198 00:11:11,020 --> 00:11:13,236 Juno turns its instruments to the planet 199 00:11:13,260 --> 00:11:15,666 for a crucial part of the mission... 200 00:11:15,690 --> 00:11:18,290 investigating Jupiter's magnetic field. 201 00:11:22,530 --> 00:11:26,316 Deep below the stormy surface, liquid metallic hydrogen 202 00:11:26,340 --> 00:11:28,686 flows endlessly around the planet, 203 00:11:28,710 --> 00:11:33,286 producing a huge magnetic field. 204 00:11:33,310 --> 00:11:36,986 This magnetosphere stretches over 600 million miles 205 00:11:37,010 --> 00:11:41,956 beyond the planet, reaching all the way to Saturn. 206 00:11:41,980 --> 00:11:45,366 If your eyes could actually see Jupiter's magnetosphere 207 00:11:45,390 --> 00:11:48,196 and you tried to look at it while standing on earth, 208 00:11:48,220 --> 00:11:52,406 it would look about as big in the sky as the moon. 209 00:11:52,430 --> 00:11:54,706 And within this magnetic field, 210 00:11:54,730 --> 00:11:58,916 Juno faces an invisible threat. 211 00:11:58,940 --> 00:12:02,386 Jupiter has an enormous magnetic field. 212 00:12:02,410 --> 00:12:05,486 It is so enormous in terms of space, 213 00:12:05,510 --> 00:12:09,626 but also in terms of power. 214 00:12:09,650 --> 00:12:12,256 High-energy particles from the Sun 215 00:12:12,280 --> 00:12:14,926 are funneled into deadly radiation belts 216 00:12:14,950 --> 00:12:19,866 guided by the giant planet's magnetic field. 217 00:12:19,890 --> 00:12:24,106 The magnetic field traps charged particles coming from the Sun 218 00:12:24,130 --> 00:12:26,936 and circulates them around that system 219 00:12:26,960 --> 00:12:30,206 and just bombards anything in the vicinity, 220 00:12:30,230 --> 00:12:34,576 including our fragile little spacecraft. 221 00:12:34,600 --> 00:12:36,086 Closer to the planet, 222 00:12:36,110 --> 00:12:38,716 radiation levels are up to 30 times greater 223 00:12:38,740 --> 00:12:41,416 than they were inside the reactor core room 224 00:12:41,440 --> 00:12:44,086 during the Chernobyl disaster. 225 00:12:44,110 --> 00:12:45,856 This is radiation. 226 00:12:45,880 --> 00:12:47,596 This is bad news. 227 00:12:47,620 --> 00:12:49,296 These particles, they would hit you. 228 00:12:49,320 --> 00:12:52,536 They would rupture your DNA, rupture your cell structures, 229 00:12:52,560 --> 00:12:55,396 and you would die. 230 00:12:55,420 --> 00:12:57,836 This blistering radiation is bad news 231 00:12:57,860 --> 00:13:01,276 for the spacecraft as well. 232 00:13:01,300 --> 00:13:04,376 The charged particles threaten to destroy electronic 233 00:13:04,400 --> 00:13:09,846 and navigational systems, but Juno has armored up. 234 00:13:09,870 --> 00:13:13,856 It's not some delicate, beautiful, gossamer thing 235 00:13:13,880 --> 00:13:16,356 that you are sending to orbit Jupiter. 236 00:13:16,380 --> 00:13:18,186 It's more like a tank. 237 00:13:18,210 --> 00:13:20,096 You have to protect this thing or else 238 00:13:20,120 --> 00:13:24,026 it's not going to last very long at all. 239 00:13:24,050 --> 00:13:27,166 We've got a couple hundred pounds of titanium 240 00:13:27,190 --> 00:13:29,536 on the spacecraft just trying to shield us 241 00:13:29,560 --> 00:13:31,736 from what Jupiter might throw at us, 242 00:13:31,760 --> 00:13:36,076 so it is in a sense we're like an armored tank going into war. 243 00:13:36,100 --> 00:13:40,476 Lightweight titanium is tough. 244 00:13:40,500 --> 00:13:44,046 Juno's 1/2-inch-thick shielding blocks 99% 245 00:13:44,070 --> 00:13:48,116 of Jupiter's vicious radiation. 246 00:13:48,140 --> 00:13:49,726 But even at this reduced rate, 247 00:13:49,750 --> 00:13:53,456 Juno can't survive the bombardment for long, 248 00:13:53,480 --> 00:13:56,796 so the craft sets itself on a unique orbit 249 00:13:56,820 --> 00:13:59,566 around the gas giant. 250 00:13:59,590 --> 00:14:01,966 It actually has a very long orbit 251 00:14:01,990 --> 00:14:04,636 where it spends most of its time far away, 252 00:14:04,660 --> 00:14:07,276 and then every once in a while dives in and goes, 253 00:14:07,300 --> 00:14:09,076 "oh, hot, hot, hot, hot. I zoomed in too much," 254 00:14:09,100 --> 00:14:11,776 and then goes safely away to communicate and process 255 00:14:11,800 --> 00:14:15,516 and then back in again. 256 00:14:15,540 --> 00:14:17,316 Juno takes a mighty gamble 257 00:14:17,340 --> 00:14:20,016 diving deep into these radiation belts 258 00:14:20,040 --> 00:14:22,856 to achieve one of its key objectives... 259 00:14:22,880 --> 00:14:26,826 mapping Jupiter's giant magnetic field, 260 00:14:26,850 --> 00:14:29,696 and as Juno swoops around the planet, 261 00:14:29,720 --> 00:14:35,466 it reveals something scientists have never seen before. 262 00:14:35,490 --> 00:14:36,636 When you look at the Earth, 263 00:14:36,660 --> 00:14:38,906 we have a fairly simple magnetic field. 264 00:14:38,930 --> 00:14:40,836 It's like a giant bar magnet with a north 265 00:14:40,860 --> 00:14:42,876 and south magnetic pole. 266 00:14:42,900 --> 00:14:44,876 Well, Jupiter has that as well. 267 00:14:44,900 --> 00:14:46,676 This is called a dipolar field. 268 00:14:46,700 --> 00:14:51,546 It's got two poles, but it also has a third pole. 269 00:14:51,570 --> 00:14:53,886 Juno's magnetic field maps 270 00:14:53,910 --> 00:14:56,356 show a north and south pole 271 00:14:56,380 --> 00:15:00,456 and a bizarre magnetic disturbance at the equator. 272 00:15:00,480 --> 00:15:04,066 And it's like Jupiter just sprouted a third arm, 273 00:15:04,090 --> 00:15:06,866 and that's kind of mysterious. 274 00:15:06,890 --> 00:15:08,396 On magnetic field maps, 275 00:15:08,420 --> 00:15:11,966 north poles show up red and south poles blue, 276 00:15:11,990 --> 00:15:15,646 so scientists are calling this second south pole 277 00:15:15,670 --> 00:15:17,876 the great blue spot. 278 00:15:17,900 --> 00:15:20,516 Everyone knows about the Great Red Spot, 279 00:15:20,540 --> 00:15:24,046 but Jupiter now has a great blue spot as well. 280 00:15:24,070 --> 00:15:26,256 This magnetic disturbance reflects 281 00:15:26,280 --> 00:15:28,716 Jupiter's stormy interior. 282 00:15:28,740 --> 00:15:32,496 You have these fast-moving winds blowing on the magnetic field, 283 00:15:32,520 --> 00:15:34,896 and they're actually shearing it apart 284 00:15:34,920 --> 00:15:36,526 and moving the field around. 285 00:15:36,550 --> 00:15:38,026 It's not necessarily a storm, 286 00:15:38,050 --> 00:15:39,436 although it could be. 287 00:15:39,460 --> 00:15:41,990 It maybe is better to think of it as a magnetic storm. 288 00:15:44,630 --> 00:15:46,806 Turbulence inside Jupiter could be 289 00:15:46,830 --> 00:15:51,346 twisting up the magnetic field to drive the great blue spot 290 00:15:51,370 --> 00:15:56,316 and the deadly radiation belts that Juno must navigate through. 291 00:15:56,340 --> 00:16:00,216 Unlike earth, Jupiter is not really a solid mass 292 00:16:00,240 --> 00:16:04,286 for the most part, so all of its clouds and gases 293 00:16:04,310 --> 00:16:06,696 are moving at slightly different rates, 294 00:16:06,720 --> 00:16:09,226 and that actually makes the magnetic field 295 00:16:09,250 --> 00:16:14,066 that's generated very variable and highly changing. 296 00:16:14,090 --> 00:16:15,596 For us to have a variable magnetic field 297 00:16:15,620 --> 00:16:17,166 like Jupiter does, 298 00:16:17,190 --> 00:16:19,336 the entire earth would have to be molten. 299 00:16:19,360 --> 00:16:21,776 We really don't want that to happen. 300 00:16:21,800 --> 00:16:25,106 With each orbit, Juno unravels more mysteries 301 00:16:25,130 --> 00:16:29,316 of this giant planet, but Jupiter's deepest secret 302 00:16:29,340 --> 00:16:32,316 could shine a light on our own origins. 303 00:16:32,340 --> 00:16:33,986 If we want to understand the Earth 304 00:16:34,010 --> 00:16:35,656 and our place in the solar system, 305 00:16:35,680 --> 00:16:38,156 Juno has found that a lot of those mysteries 306 00:16:38,180 --> 00:16:39,580 are locked up there in Jupiter. 307 00:16:53,630 --> 00:16:55,106 The Juno spacecraft 308 00:16:55,130 --> 00:16:57,806 is uncovering the secrets of Jupiter 309 00:16:57,830 --> 00:17:02,346 from its swirling cloud tops to its dark heart, 310 00:17:02,370 --> 00:17:07,156 but Juno's discoveries go beyond the gas giant itself. 311 00:17:07,180 --> 00:17:12,026 They could also solve mysteries surrounding our own planet. 312 00:17:12,050 --> 00:17:14,456 Jupiter is the key 313 00:17:14,480 --> 00:17:16,796 to the formation of the solar system, 314 00:17:16,820 --> 00:17:18,866 which means it's the key to understanding 315 00:17:18,890 --> 00:17:21,366 how the Earth formed. 316 00:17:21,390 --> 00:17:22,966 Juno is actually giving us a view 317 00:17:22,990 --> 00:17:24,936 into the history of our planetary system, 318 00:17:24,960 --> 00:17:28,676 even the history of earth. 319 00:17:28,700 --> 00:17:31,076 4.6 billion years ago, 320 00:17:31,100 --> 00:17:35,146 a cloud of hydrogen gas and cosmic dust collapses, 321 00:17:35,170 --> 00:17:38,716 sparking nuclear fusion. 322 00:17:38,740 --> 00:17:41,186 From the resulting chaos, 323 00:17:41,210 --> 00:17:44,326 one star, four rocky worlds, 324 00:17:44,350 --> 00:17:47,126 and four gassy giants are born 325 00:17:47,150 --> 00:17:52,266 and form our solar system. 326 00:17:52,290 --> 00:17:54,466 There's these distinct zones of the solar system... 327 00:17:54,490 --> 00:17:56,336 rocky and metallic in the inner part, 328 00:17:56,360 --> 00:17:58,606 gaseous and water-rich in the outer part, 329 00:17:58,630 --> 00:18:01,306 and even without thinking about that too hard, 330 00:18:01,330 --> 00:18:04,376 it kind of makes sense because in close to the Sun, 331 00:18:04,400 --> 00:18:05,646 it's warmer. 332 00:18:05,670 --> 00:18:09,116 Out farther away from the Sun, it's cooler. 333 00:18:09,140 --> 00:18:12,616 But the Earth breaks the mold. 334 00:18:12,640 --> 00:18:17,626 Our planet has far more water than theories predict. 335 00:18:17,650 --> 00:18:19,696 The Earth formed in a part of the solar system that, 336 00:18:19,720 --> 00:18:21,756 well, you'd think normally should be probably pretty dry 337 00:18:21,780 --> 00:18:24,326 because it was pretty close to the Sun. 338 00:18:24,350 --> 00:18:28,036 Our planet is just 150 million miles from the Sun, 339 00:18:28,060 --> 00:18:33,376 putting us inside what scientists call the snow line. 340 00:18:33,400 --> 00:18:36,306 Inside this line, the Sun is powerful enough 341 00:18:36,330 --> 00:18:42,176 to evaporate water during a planet's formation. 342 00:18:42,200 --> 00:18:44,546 Inside the snow line, the temperatures are high, 343 00:18:44,570 --> 00:18:47,486 and there's a lot of energy from the Sun nearby. 344 00:18:47,510 --> 00:18:48,916 Too close to the Sun, 345 00:18:48,940 --> 00:18:52,286 those gaseous and ice-rich materials just can't exist. 346 00:18:52,310 --> 00:18:55,596 They're evaporate away by the heat of the Sun. 347 00:18:55,620 --> 00:19:00,866 Our watery world should be a dry rock in space. 348 00:19:00,890 --> 00:19:03,466 Understanding how water got to the Earth is so important 349 00:19:03,490 --> 00:19:07,536 because it wouldn't be there in the very, very beginning. 350 00:19:07,560 --> 00:19:11,906 But Jupiter could hold the answer to this mystery. 351 00:19:11,930 --> 00:19:14,446 To solve the riddle of earth's water, 352 00:19:14,470 --> 00:19:19,416 Juno aims to discover where our Jupiter was born. 353 00:19:19,440 --> 00:19:21,716 Understanding how and where 354 00:19:21,740 --> 00:19:24,156 and when Jupiter formed is critical 355 00:19:24,180 --> 00:19:25,626 because it has really dominated 356 00:19:25,650 --> 00:19:28,456 the entire evolution of the solar system. 357 00:19:28,480 --> 00:19:30,296 It's the biggest planet by far. 358 00:19:30,320 --> 00:19:34,766 It's the biggest thing out there that's moving everything around. 359 00:19:34,790 --> 00:19:36,906 Any water in the early solar system 360 00:19:36,930 --> 00:19:40,536 could've been moved around by Jupiter's mighty gravity, 361 00:19:40,560 --> 00:19:44,506 so if Juno can trace the history of this giant planet, 362 00:19:44,530 --> 00:19:49,316 that could explain why we find H2O where it's least expected. 363 00:19:49,340 --> 00:19:51,986 We know that planets can move closer to the Sun 364 00:19:52,010 --> 00:19:53,856 and farther out while they're forming 365 00:19:53,880 --> 00:19:55,656 and even after they form, 366 00:19:55,680 --> 00:19:59,086 so how do we figure out where Jupiter formed? 367 00:19:59,110 --> 00:20:01,326 The key is how much water is 368 00:20:01,350 --> 00:20:04,026 locked up inside Jupiter. 369 00:20:04,050 --> 00:20:09,166 If we can understand how Jupiter built a relationship with water, 370 00:20:09,190 --> 00:20:11,666 we can understand how water got distributed 371 00:20:11,690 --> 00:20:17,106 all throughout the solar system, including here on earth. 372 00:20:17,130 --> 00:20:20,446 If Juno can measure the water content of Jupiter, 373 00:20:20,470 --> 00:20:23,870 it will solve a 20-year-old mystery. 374 00:20:25,870 --> 00:20:28,456 December 1995... 375 00:20:28,480 --> 00:20:32,126 NASA's Galileo probe begins a fatal dive 376 00:20:32,150 --> 00:20:35,296 into Jupiter's atmosphere. 377 00:20:35,320 --> 00:20:39,496 When it did, it was able to measure the atmosphere around it 378 00:20:39,520 --> 00:20:43,206 and detect water, and the thing is... it didn't. 379 00:20:43,230 --> 00:20:46,436 It didn't find any, and that's weird. 380 00:20:46,460 --> 00:20:49,546 Everything was bone-dry, so why in the world 381 00:20:49,570 --> 00:20:52,506 did Jupiter's atmosphere look dry? 382 00:20:52,530 --> 00:20:55,576 If the results from the Galileo probe are correct, 383 00:20:55,600 --> 00:20:58,046 then 4.6 billion years ago, 384 00:20:58,070 --> 00:21:02,116 Jupiter formed closer to the Sun, 385 00:21:02,140 --> 00:21:04,486 but that's not the whole story. 386 00:21:04,510 --> 00:21:10,126 20 years later, NASA sends Juno to get a second opinion. 387 00:21:10,150 --> 00:21:13,566 Juno is an orbiter, and so it is loaded with instruments 388 00:21:13,590 --> 00:21:15,696 and detectors to look down on Jupiter 389 00:21:15,720 --> 00:21:19,536 and try to figure out everything that's going on. 390 00:21:19,560 --> 00:21:21,206 Juno doesn't have to risk 391 00:21:21,230 --> 00:21:24,076 its life to hunt for water. 392 00:21:24,100 --> 00:21:26,946 The craft peers through Jupiter's thick clouds 393 00:21:26,970 --> 00:21:32,716 using a microwave radiometer to detect H2O from a safe distance. 394 00:21:32,740 --> 00:21:34,356 Using these microwaves, 395 00:21:34,380 --> 00:21:38,456 Juno builds up a global map of Jupiter's water. 396 00:21:38,480 --> 00:21:39,926 What Juno has found is, yeah, 397 00:21:39,950 --> 00:21:42,926 there's plenty of water in Jupiter, 398 00:21:42,950 --> 00:21:46,196 it's just that Galileo happened to hit a dry spot, 399 00:21:46,220 --> 00:21:48,996 but in fact, if it had come in almost anywhere else, 400 00:21:49,020 --> 00:21:53,006 it would've seen plenty of water. 401 00:21:53,030 --> 00:21:55,576 Juno's findings may give a clue 402 00:21:55,600 --> 00:21:59,716 to where Jupiter originally formed. 403 00:21:59,740 --> 00:22:02,816 It seems apparent now that Jupiter 404 00:22:02,840 --> 00:22:06,856 didn't form in its present location. 405 00:22:06,880 --> 00:22:08,056 The leading theory is that 406 00:22:08,080 --> 00:22:10,886 Jupiter formed just beyond the snow line, 407 00:22:10,910 --> 00:22:14,156 the boundary between the dry inner solar system 408 00:22:14,180 --> 00:22:16,626 and the wet outer solar system. 409 00:22:16,650 --> 00:22:19,796 But we find Jupiter is twice as far away from the Sun 410 00:22:19,820 --> 00:22:22,636 as where that original snow line would've been, 411 00:22:22,660 --> 00:22:26,506 so this is telling us something interesting. 412 00:22:26,530 --> 00:22:27,676 Jupiter may have wandered from 413 00:22:27,700 --> 00:22:29,546 its original position, 414 00:22:29,570 --> 00:22:33,046 causing unimaginable chaos. 415 00:22:33,070 --> 00:22:35,216 As Jupiter moved around, things got hit 416 00:22:35,240 --> 00:22:37,416 and knocked out of the solar system. 417 00:22:37,440 --> 00:22:39,716 It essentially scatters everything in its path. 418 00:22:39,740 --> 00:22:42,516 It's the biggest player. It's the biggest planet. 419 00:22:42,540 --> 00:22:44,656 Everything moves for it. 420 00:22:44,680 --> 00:22:48,126 As Jupiter bulldozes toward the outer solar system, 421 00:22:48,150 --> 00:22:50,226 it slings ice-rich asteroids 422 00:22:50,250 --> 00:22:55,390 and comets in towards the Sun and towards the Earth. 423 00:22:59,930 --> 00:23:01,636 Jupiter would literally in some sense 424 00:23:01,660 --> 00:23:04,746 have snowplowed into the inner solar system 425 00:23:04,770 --> 00:23:06,846 a whole wave of water-rich planetesimals 426 00:23:06,870 --> 00:23:11,846 that would've delivered much of our Earth's oceans. 427 00:23:11,870 --> 00:23:15,356 Juno has helped answer why our Earth is habitable 428 00:23:15,380 --> 00:23:17,956 despite being so close to the Sun. 429 00:23:17,980 --> 00:23:20,256 So it was worth going all that distance, 430 00:23:20,280 --> 00:23:23,220 sending Juno all the way out there to get that closer look. 431 00:23:26,760 --> 00:23:28,466 Juno continues to explore 432 00:23:28,490 --> 00:23:33,076 Jupiter's mysteries and its famous features. 433 00:23:33,100 --> 00:23:35,376 There is nothing more iconic about Jupiter 434 00:23:35,400 --> 00:23:37,376 than the Great Red Spot. 435 00:23:37,400 --> 00:23:41,646 And Juno reveals that this 300-year-old cyclone 436 00:23:41,670 --> 00:23:44,700 may soon vanish. 437 00:23:57,290 --> 00:23:59,096 Our solar system plays host 438 00:23:59,120 --> 00:24:01,466 to some epic natural wonders... 439 00:24:01,490 --> 00:24:03,536 the ice geysers of Enceladus, 440 00:24:03,560 --> 00:24:06,676 the giant rings of Saturn, 441 00:24:06,700 --> 00:24:10,646 the martian mega volcano Olympus Mons, 442 00:24:10,670 --> 00:24:13,176 but in July of 2017, 443 00:24:13,200 --> 00:24:17,016 NASA's Juno probe skims the surface of Jupiter 444 00:24:17,040 --> 00:24:22,186 and photographs the most famous natural wonder... 445 00:24:22,210 --> 00:24:24,726 a fierce, hurricane-like storm 446 00:24:24,750 --> 00:24:29,026 that's been raging for hundreds of years. 447 00:24:29,050 --> 00:24:30,326 When you think of Jupiter, 448 00:24:30,350 --> 00:24:32,626 one of the most visually stunning 449 00:24:32,650 --> 00:24:34,836 and most iconic features of the atmosphere 450 00:24:34,860 --> 00:24:36,836 is that Great Red Spot. 451 00:24:36,860 --> 00:24:38,666 There is nothing like Jupiter's red spot 452 00:24:38,690 --> 00:24:42,076 in our entire solar system. 453 00:24:42,100 --> 00:24:45,006 As Juno soars over the Great Red Spot, 454 00:24:45,030 --> 00:24:49,470 it looks down onto a storm over 10,000 miles across. 455 00:24:53,010 --> 00:24:55,016 This is the most extreme storm. 456 00:24:55,040 --> 00:24:56,726 The winds are blowing continuously 457 00:24:56,750 --> 00:24:59,956 at 400 miles an hour. 458 00:24:59,980 --> 00:25:03,566 On earth, the most powerful category 5 hurricanes 459 00:25:03,590 --> 00:25:06,536 can unleash almost total destruction, 460 00:25:06,560 --> 00:25:09,466 but these are less than half as powerful 461 00:25:09,490 --> 00:25:11,766 as the storm on Jupiter. 462 00:25:11,790 --> 00:25:14,336 The Great Red Spot is the greatest hurricane 463 00:25:14,360 --> 00:25:16,406 that you've ever imagined. 464 00:25:16,430 --> 00:25:17,876 But that's not all. 465 00:25:17,900 --> 00:25:22,416 Juno's microwave radiometer allows scientists to see through 466 00:25:22,440 --> 00:25:26,456 Jupiter's cloud layers for the first time. 467 00:25:26,480 --> 00:25:30,156 Juno has instrumentation that's able to look underneath, 468 00:25:30,180 --> 00:25:31,586 so one of the things we did was we looked 469 00:25:31,610 --> 00:25:33,556 at how deep are the roots. 470 00:25:33,580 --> 00:25:35,796 Juno peers down into the eye 471 00:25:35,820 --> 00:25:37,526 of this monstrous storm. 472 00:25:37,550 --> 00:25:40,796 It spots temperature changes far below the surface 473 00:25:40,820 --> 00:25:43,466 that follow the storm's iconic shape, 474 00:25:43,490 --> 00:25:46,506 tracing the roots of the Great Red Spot 475 00:25:46,530 --> 00:25:49,176 deep into the Jovian atmosphere. 476 00:25:49,200 --> 00:25:50,806 They found out that it goes down over 477 00:25:50,830 --> 00:25:54,346 200 miles deep into the atmosphere. 478 00:25:54,370 --> 00:25:56,270 There's nothing like that on Earth. 479 00:25:59,580 --> 00:26:02,216 The greatest cyclones of our own planet 480 00:26:02,240 --> 00:26:05,426 can reach heights of around 10 miles, 481 00:26:05,450 --> 00:26:10,596 but Jupiter's Great Red Spot is over 20 times taller. 482 00:26:10,620 --> 00:26:12,666 I think that really brings into perspective 483 00:26:12,690 --> 00:26:14,790 the massive scale of this planet. 484 00:26:18,090 --> 00:26:20,606 Jupiter's vast, turbulent atmosphere 485 00:26:20,630 --> 00:26:24,246 hosts the deepest storm mankind has ever seen, 486 00:26:24,270 --> 00:26:28,376 and Juno's discoveries get scientists wondering. 487 00:26:28,400 --> 00:26:31,316 Could the Great Red Spot help explain 488 00:26:31,340 --> 00:26:34,116 another of Jupiter's mysteries, 489 00:26:34,140 --> 00:26:39,386 the planet's surprisingly warm atmosphere? 490 00:26:39,410 --> 00:26:42,226 Jupiter looks out in our outer solar system 491 00:26:42,250 --> 00:26:43,696 where everything is very cold. 492 00:26:43,720 --> 00:26:47,366 The Sun is very dim when you get that far away. 493 00:26:47,390 --> 00:26:50,436 Jupiter is five times farther from the Sun than we are, 494 00:26:50,460 --> 00:26:52,166 so it's only getting 4% 495 00:26:52,190 --> 00:26:54,736 of the amount of energy from the Sun that we do. 496 00:26:54,760 --> 00:26:56,006 But there's something heating up 497 00:26:56,030 --> 00:26:57,346 the atmosphere of Jupiter. 498 00:26:57,370 --> 00:27:00,346 There are parts of it that are many times warmer 499 00:27:00,370 --> 00:27:01,846 than we could explain with sunlight. 500 00:27:01,870 --> 00:27:03,586 The question is, of course, where is that energy 501 00:27:03,610 --> 00:27:06,286 coming from? 502 00:27:06,310 --> 00:27:09,356 Juno swoops in for another pass on Jupiter, 503 00:27:09,380 --> 00:27:11,626 turning its high-resolution cameras 504 00:27:11,650 --> 00:27:16,256 on the raging storm below. 505 00:27:16,280 --> 00:27:18,526 The storm unleashes vicious turbulence 506 00:27:18,550 --> 00:27:20,436 into the surrounding atmosphere, 507 00:27:20,460 --> 00:27:22,936 giving scientists the clue they need 508 00:27:22,960 --> 00:27:26,236 to explain the planet's high temperature. 509 00:27:26,260 --> 00:27:29,476 The Great Red Spot is a giant hurricane 510 00:27:29,500 --> 00:27:34,016 that's powered by heat deep in the core of Jupiter, 511 00:27:34,040 --> 00:27:37,816 but it has such violent and chaotic motion, 512 00:27:37,840 --> 00:27:40,310 it's mixing up the atmosphere around it. 513 00:27:43,810 --> 00:27:46,026 The thunderstorms on Jupiter are gonna be generating 514 00:27:46,050 --> 00:27:48,026 booming thunder just the same way 515 00:27:48,050 --> 00:27:52,166 that they do here on the Earth. 516 00:27:52,190 --> 00:27:54,336 Thunderclouds send sound waves 517 00:27:54,360 --> 00:27:58,966 rippling through the storm. 518 00:27:58,990 --> 00:28:03,546 A sound wave is a wave of pressure, 519 00:28:03,570 --> 00:28:06,616 of compression where air molecules 520 00:28:06,640 --> 00:28:09,316 or water molecules get compacted. 521 00:28:09,340 --> 00:28:10,746 They get squeezed together, 522 00:28:10,770 --> 00:28:12,716 and when you squeeze something together, 523 00:28:12,740 --> 00:28:14,016 they're a lot closer together 524 00:28:14,040 --> 00:28:15,480 and they're gonna get pretty hot. 525 00:28:18,250 --> 00:28:20,056 These sounds waves shoot up 526 00:28:20,080 --> 00:28:23,426 500 miles above the storm 527 00:28:23,450 --> 00:28:26,836 where they break, converting sound energy into heat. 528 00:28:26,860 --> 00:28:30,706 These sound waves, they crash together, 529 00:28:30,730 --> 00:28:32,766 creating a tremendous amount of energy 530 00:28:32,790 --> 00:28:36,976 and heating the gases around them. 531 00:28:37,000 --> 00:28:39,576 Jupiter's great red spot has helped heat 532 00:28:39,600 --> 00:28:42,476 the Jovian atmosphere for hundreds of years, 533 00:28:42,500 --> 00:28:48,286 but new images suggest that this may be about to change. 534 00:28:48,310 --> 00:28:50,186 Jupiter's red spot is so big, 535 00:28:50,210 --> 00:28:53,356 I mean, it's bigger than earth by a long shot. 536 00:28:53,380 --> 00:28:56,396 It seems like it would be an incredibly stable thing. 537 00:28:56,420 --> 00:28:59,796 It's just there and it's always been there and always will be. 538 00:28:59,820 --> 00:29:03,506 Recently, we've seen it changing. 539 00:29:03,530 --> 00:29:05,806 When NASA's Voyager space probe visited 540 00:29:05,830 --> 00:29:07,936 Jupiter in 1979, 541 00:29:07,960 --> 00:29:11,200 it observed a storm twice the diameter of Earth. 542 00:29:15,700 --> 00:29:20,186 In 2017, Juno's images show the Great Red Spot 543 00:29:20,210 --> 00:29:24,626 has lost a third of its width, but that's not all. 544 00:29:24,650 --> 00:29:28,856 Despite the storm shrinking, it's actually getting taller. 545 00:29:28,880 --> 00:29:31,726 The Great Red Spot is being stretched and forced 546 00:29:31,750 --> 00:29:34,796 into Jupiter's upper atmosphere. 547 00:29:34,820 --> 00:29:36,366 The storms in the Great Red Spot, 548 00:29:36,390 --> 00:29:39,036 it's kind of like the clay on a potter's wheel, 549 00:29:39,060 --> 00:29:41,176 where as you bring your hands closer together 550 00:29:41,200 --> 00:29:43,906 to draw the clay in, the closer your hands are, 551 00:29:43,930 --> 00:29:47,246 the taller the pottery becomes, and similarly, for the storm, 552 00:29:47,270 --> 00:29:49,616 as it becomes smaller at the base, 553 00:29:49,640 --> 00:29:53,456 it raises taller toward the upper atmosphere. 554 00:29:53,480 --> 00:29:55,316 It's getting taller, and we see storms 555 00:29:55,340 --> 00:29:57,686 do the same thing on earth, and when it does that, 556 00:29:57,710 --> 00:30:00,196 the wind shear will actually take the top of the storm off 557 00:30:00,220 --> 00:30:02,496 and drag it apart, and so we'll be watching it 558 00:30:02,520 --> 00:30:04,026 very intently over the next few years 559 00:30:04,050 --> 00:30:08,566 to see if that's what happens on Jupiter as well. 560 00:30:08,590 --> 00:30:10,366 It may be only a matter of time 561 00:30:10,390 --> 00:30:13,406 before Jupiter's high-altitude winds 562 00:30:13,430 --> 00:30:16,306 tear this iconic storm to shreds. 563 00:30:16,330 --> 00:30:18,506 The most famous storm of the solar system 564 00:30:18,530 --> 00:30:20,476 may soon disappear, 565 00:30:20,500 --> 00:30:23,046 but Juno reveals other storms 566 00:30:23,070 --> 00:30:26,786 hidden in the strangest of places. 567 00:30:26,810 --> 00:30:29,156 The storm in the Great Red Spot is one, 568 00:30:29,180 --> 00:30:32,780 but not the only, giant storm that's happening on Jupiter. 569 00:30:49,230 --> 00:30:52,806 NASA's Juno probe has traveled billions of miles 570 00:30:52,830 --> 00:30:54,546 across the solar system 571 00:30:54,570 --> 00:30:58,486 to reveal the mysteries of gas giant Jupiter, 572 00:30:58,510 --> 00:31:00,916 but there's one part of Jupiter 573 00:31:00,940 --> 00:31:04,686 that has remained hidden until now. 574 00:31:04,710 --> 00:31:07,496 Before Juno, our view of Jupiter was very limited. 575 00:31:07,520 --> 00:31:10,366 We'd never actually flown over the poles. 576 00:31:10,390 --> 00:31:12,066 It's something that's very hard to do on Jupiter. 577 00:31:12,090 --> 00:31:15,536 We don't have other missions that have done this. 578 00:31:15,560 --> 00:31:19,206 In August of 2016, Juno's flight plan takes 579 00:31:19,230 --> 00:31:22,576 the spacecraft into unknown territory to reveal 580 00:31:22,600 --> 00:31:27,976 Jupiter's mysterious polar regions for the first time. 581 00:31:28,000 --> 00:31:29,616 Well, and the first time we looked at the pole, 582 00:31:29,640 --> 00:31:31,940 it didn't look anything like the Jupiter we knew. 583 00:31:35,640 --> 00:31:37,326 We never would've guessed that was Jupiter 584 00:31:37,350 --> 00:31:38,630 if somebody had shown that to us. 585 00:31:42,420 --> 00:31:46,196 Juno's camera reveals a strange blue expanse 586 00:31:46,220 --> 00:31:49,096 that puzzles scientists. 587 00:31:49,120 --> 00:31:50,266 The electronic color 588 00:31:50,290 --> 00:31:52,936 could be due to chemical changes in the clouds 589 00:31:52,960 --> 00:31:56,876 brought on by a lack of sunlight, 590 00:31:56,900 --> 00:32:00,276 but what Juno spots inside the blue clouds 591 00:32:00,300 --> 00:32:03,386 is even stranger... 592 00:32:03,410 --> 00:32:08,186 giant central cyclones spin around each pole at 200 miles 593 00:32:08,210 --> 00:32:10,456 an hour, with these cyclones 594 00:32:10,480 --> 00:32:14,956 surrounded by eight stormy vortices in the north 595 00:32:14,980 --> 00:32:18,296 and five in the south. 596 00:32:18,320 --> 00:32:21,596 There are these weird cyclones, gigantic swirls, 597 00:32:21,620 --> 00:32:25,566 vortices of gas swirling around Jupiter's poles, 598 00:32:25,590 --> 00:32:28,906 and they're clearly forming patterns. 599 00:32:28,930 --> 00:32:30,846 It's hard to get a sense of scale here. 600 00:32:30,870 --> 00:32:32,906 Now the north polar central cyclone, 601 00:32:32,930 --> 00:32:36,816 that one right at the pole, that's 2,500 miles across. 602 00:32:36,840 --> 00:32:40,616 That is almost as big as the continental United States. 603 00:32:40,640 --> 00:32:42,086 What is going on there? 604 00:32:42,110 --> 00:32:44,780 This is nothing like what we see on earth. 605 00:32:47,820 --> 00:32:51,826 On earth, our weather is driven by heat from the Sun 606 00:32:51,850 --> 00:32:53,796 that hits our planet at the equator 607 00:32:53,820 --> 00:32:57,206 and flows across the surface. 608 00:32:57,230 --> 00:33:00,476 Powerful cyclones form over tropical waters 609 00:33:00,500 --> 00:33:04,346 and move around the planet, 610 00:33:04,370 --> 00:33:07,516 but the polar regions receive less energy from the Sun, 611 00:33:07,540 --> 00:33:11,246 so cyclones can't form at the poles. 612 00:33:11,270 --> 00:33:13,356 We see that if you're at the equator, 613 00:33:13,380 --> 00:33:14,586 it's warmer and it's stormier. 614 00:33:14,610 --> 00:33:15,986 If you're at the poles, 615 00:33:16,010 --> 00:33:20,996 where the Sun is slightly harder to see, that activity goes away. 616 00:33:21,020 --> 00:33:22,756 But the weather on Jupiter 617 00:33:22,780 --> 00:33:25,126 couldn't be more different. 618 00:33:25,150 --> 00:33:27,366 We see lightning and convective thunderstorms 619 00:33:27,390 --> 00:33:29,596 at the poles of Jupiter but not at the equator, 620 00:33:29,620 --> 00:33:32,366 and that's sort of the opposite of what we see on the Earth. 621 00:33:32,390 --> 00:33:36,846 The question is, what's driving Jupiter's storms? 622 00:33:36,870 --> 00:33:38,406 Jupiter is five times further 623 00:33:38,430 --> 00:33:40,516 away from the Sun than the Earth 624 00:33:40,540 --> 00:33:44,946 and receives only a fraction of the Sun's energy. 625 00:33:44,970 --> 00:33:47,986 Unlike earth, Jupiter's polar regions 626 00:33:48,010 --> 00:33:50,586 seem to be where the action is. 627 00:33:50,610 --> 00:33:53,926 Something is driving the planet's weird weather, 628 00:33:53,950 --> 00:33:57,596 and Juno's scans of the giant planet's thermal emissions 629 00:33:57,620 --> 00:34:01,696 suggests it could be Jupiter itself. 630 00:34:01,720 --> 00:34:04,436 We can actually see the internal heat of Jupiter 631 00:34:04,460 --> 00:34:05,806 coming right up through, 632 00:34:05,830 --> 00:34:08,036 and so Jupiter will look very bright in areas 633 00:34:08,060 --> 00:34:11,276 where we can see that heat. 634 00:34:11,300 --> 00:34:13,416 Juno detects searing heat 635 00:34:13,440 --> 00:34:16,416 beneath Jupiter's cloud bands. 636 00:34:16,440 --> 00:34:19,186 Jupiter has so much material, so much mass, 637 00:34:19,210 --> 00:34:22,056 so much gravity that the interior is incredibly dense 638 00:34:22,080 --> 00:34:23,756 and very, very hot. 639 00:34:23,780 --> 00:34:26,726 At the core, it's probably at many thousands of degrees hotter 640 00:34:26,750 --> 00:34:29,626 than the surface of the Sun. 641 00:34:29,650 --> 00:34:33,836 This fiery inferno buried in Jupiter's dark heart 642 00:34:33,860 --> 00:34:37,436 is a relic from its birth billions of years ago. 643 00:34:37,460 --> 00:34:40,206 The violent collisions that formed the planet 644 00:34:40,230 --> 00:34:42,736 left its core seething hot, 645 00:34:42,760 --> 00:34:45,646 a heat that remains to this day, 646 00:34:45,670 --> 00:34:50,116 buried under thousands of miles of insulating gas. 647 00:34:50,140 --> 00:34:52,786 As the heat slowly leaks outward, 648 00:34:52,810 --> 00:34:55,716 Jupiter's fast-rotating atmosphere 649 00:34:55,740 --> 00:34:59,456 creates vicious cyclones and thunderstorms. 650 00:34:59,480 --> 00:35:02,226 And that's what's really driving most of the weather. 651 00:35:02,250 --> 00:35:06,266 It's not the Sun. It's Jupiter itself. 652 00:35:06,290 --> 00:35:08,866 And as Juno soars over the planet, 653 00:35:08,890 --> 00:35:13,136 it reveals another weather mystery. 654 00:35:13,160 --> 00:35:16,106 The craft detects bursts of radio waves 655 00:35:16,130 --> 00:35:19,846 spiking up to four times a second... 656 00:35:19,870 --> 00:35:24,846 the telltale sign of ferocious lightning strikes. 657 00:35:24,870 --> 00:35:26,486 Clouds are moving around in the atmosphere 658 00:35:26,510 --> 00:35:28,356 and building up electric charge 659 00:35:28,380 --> 00:35:30,886 and causing bolts of lightning to form, 660 00:35:30,910 --> 00:35:35,126 and we've actually seen this with the Juno spacecraft. 661 00:35:35,150 --> 00:35:38,196 These are mega storms orders of magnitude bigger 662 00:35:38,220 --> 00:35:39,550 than here on Earth. 663 00:35:43,530 --> 00:35:46,636 And Juno finds there's more to these thunderclouds 664 00:35:46,660 --> 00:35:50,006 than just flashes of light... 665 00:35:50,030 --> 00:35:54,316 giant icy hailstones of water and ammonia, 666 00:35:54,340 --> 00:35:57,016 the chemical which gives Jupiter's clouds 667 00:35:57,040 --> 00:36:01,716 their orange color. 668 00:36:01,740 --> 00:36:03,356 High up in Jupiter's atmosphere, 669 00:36:03,380 --> 00:36:07,026 the ammonia is mixing with the water, 670 00:36:07,050 --> 00:36:09,226 and it becomes a liquid ball 671 00:36:09,250 --> 00:36:11,896 that starts to collect ice around it, 672 00:36:11,920 --> 00:36:17,106 and it will fall like hail does deep into Jupiter's atmosphere. 673 00:36:17,130 --> 00:36:20,976 On earth, hail falls to the ground and melts, 674 00:36:21,000 --> 00:36:24,676 but on Jupiter, there is no ground. 675 00:36:24,700 --> 00:36:26,916 And it gets lifted in the atmosphere 676 00:36:26,940 --> 00:36:29,076 because of an updraft and then more ice, 677 00:36:29,100 --> 00:36:31,316 and it builds bigger, and then it falls down, 678 00:36:31,340 --> 00:36:32,686 and then it gets carried back up, 679 00:36:32,710 --> 00:36:38,056 and so hail is often many layers being built. 680 00:36:38,080 --> 00:36:41,696 These ice balls grow layer by layer as they soar up 681 00:36:41,720 --> 00:36:44,726 and down the atmosphere. 682 00:36:44,750 --> 00:36:47,266 If they formed in storms here on earth, 683 00:36:47,290 --> 00:36:50,536 they'd cause some serious damage. 684 00:36:50,560 --> 00:36:52,966 So if you were buzzing around Jupiter 685 00:36:52,990 --> 00:36:55,606 and you were near where these storms were, 686 00:36:55,630 --> 00:36:59,976 you might get hit by hail coming up or going down. 687 00:37:00,000 --> 00:37:04,116 This is one of the most violent, energetic atmospheres 688 00:37:04,140 --> 00:37:07,816 in the entire solar system. 689 00:37:07,840 --> 00:37:09,886 Juno is revealing the secrets 690 00:37:09,910 --> 00:37:12,656 that Jupiter has hidden for decades, 691 00:37:12,680 --> 00:37:17,326 including the mystery of Jupiter's northern lights. 692 00:37:17,350 --> 00:37:19,796 When Juno studied the lights 693 00:37:19,820 --> 00:37:21,896 coming from the aurora on Jupiter, 694 00:37:21,920 --> 00:37:24,920 it found that something really weird is going on. 695 00:37:42,840 --> 00:37:46,426 On earth, dazzling auroras light up the skies 696 00:37:46,450 --> 00:37:48,626 as charged particles from the Sun 697 00:37:48,650 --> 00:37:51,280 interact with atoms high in the atmosphere. 698 00:37:54,660 --> 00:37:58,736 Deep in the outer solar system, Jupiter is too far from the Sun 699 00:37:58,760 --> 00:38:01,806 for strong auroras to form in this way, 700 00:38:01,830 --> 00:38:05,046 but high above the giant planet's poles, 701 00:38:05,070 --> 00:38:09,140 Juno spots a seemingly impossible light show. 702 00:38:11,370 --> 00:38:14,356 The auroras of Jupiter are tremendously larger 703 00:38:14,380 --> 00:38:15,916 than the ones that we find here on Earth. 704 00:38:15,940 --> 00:38:17,956 In fact, the auroral rings near the poles 705 00:38:17,980 --> 00:38:20,426 are bigger than our planet itself. 706 00:38:20,450 --> 00:38:21,726 Jupiter's auroras emit 707 00:38:21,750 --> 00:38:24,166 primarily ultraviolet and X-ray light, 708 00:38:24,190 --> 00:38:26,626 so you can't see it with the naked human eye, 709 00:38:26,650 --> 00:38:29,596 but if you could see them and you were at Jupiter, 710 00:38:29,620 --> 00:38:32,506 that would be an amazing light show 711 00:38:32,530 --> 00:38:37,646 because those auroras are strong. 712 00:38:37,670 --> 00:38:39,046 These glowing displays are 713 00:38:39,070 --> 00:38:41,746 evidence of charged particles 714 00:38:41,770 --> 00:38:45,216 slamming into Jupiter's atmosphere. 715 00:38:45,240 --> 00:38:47,616 But if they're not coming from the Sun, 716 00:38:47,640 --> 00:38:50,326 where are they coming from? 717 00:38:50,350 --> 00:38:52,856 Hunting for an answer, Juno snaps an image 718 00:38:52,880 --> 00:38:54,496 of Jupiter's southern lights 719 00:38:54,520 --> 00:38:59,466 with its ultraviolet imaging spectrometer. 720 00:38:59,490 --> 00:39:03,866 Inside the aurora, it glimpses something strange. 721 00:39:03,890 --> 00:39:06,266 When Juno studied the lights 722 00:39:06,290 --> 00:39:08,336 coming from the aurora on Jupiter, 723 00:39:08,360 --> 00:39:11,606 it found that they were even stronger than expected, 724 00:39:11,630 --> 00:39:13,246 and in fact, when you look at 725 00:39:13,270 --> 00:39:15,976 Jupiter's poles in wavelengths that our eyes can't see, 726 00:39:16,000 --> 00:39:20,286 for example, ultraviolet, you see a hot spot. 727 00:39:20,310 --> 00:39:22,456 This hot spot marks the point 728 00:39:22,480 --> 00:39:25,756 where huge concentrations of charged particles 729 00:39:25,780 --> 00:39:28,756 strike Jupiter's atmosphere. 730 00:39:28,780 --> 00:39:31,796 Tracing their trajectory reveals the culprit 731 00:39:31,820 --> 00:39:34,396 of Jupiter's dazzling light shows... 732 00:39:34,420 --> 00:39:36,990 the volcanoes of Jupiter's moons. 733 00:39:39,730 --> 00:39:42,576 Jupiter's moon, Io has hundreds of active volcanoes 734 00:39:42,600 --> 00:39:45,106 spewing out materials way out into space, 735 00:39:45,130 --> 00:39:49,376 and many of those get trapped by the magnetic field of Jupiter. 736 00:39:49,400 --> 00:39:53,386 Io's volcanoes fire out jets of charged particles, 737 00:39:53,410 --> 00:39:57,556 which are swept by the giant planet's magnetic field. 738 00:39:57,580 --> 00:39:59,126 It's funneling those particles down 739 00:39:59,150 --> 00:40:04,166 and slamming into specific spots in Jupiter's atmosphere. 740 00:40:04,190 --> 00:40:06,426 But Io isn't the only moon responsible 741 00:40:06,450 --> 00:40:09,436 for Jupiter's polar light show. 742 00:40:09,460 --> 00:40:12,766 If we go further out, Europa, Ganymede, 743 00:40:12,790 --> 00:40:14,106 Callisto, those are more icy. 744 00:40:14,130 --> 00:40:16,906 They don't necessarily have volcanoes. 745 00:40:16,930 --> 00:40:18,906 These icy moons twist up 746 00:40:18,930 --> 00:40:22,276 Jupiter's magnetic field in their own way. 747 00:40:22,300 --> 00:40:24,846 Some of these moons have magnetic fields that interact 748 00:40:24,870 --> 00:40:26,446 with Jupiter's magnetic field, 749 00:40:26,470 --> 00:40:31,756 and that actually intensifies the aurora display on Jupiter. 750 00:40:31,780 --> 00:40:33,626 Jupiter's moons work together 751 00:40:33,650 --> 00:40:37,926 to energize the greatest auroras in the solar system, 752 00:40:37,950 --> 00:40:40,126 but in these beautiful displays 753 00:40:40,150 --> 00:40:45,136 is a stark reminder of the danger Juno faces. 754 00:40:45,160 --> 00:40:47,276 When you look at these pictures of the aurora on Jupiter, 755 00:40:47,300 --> 00:40:48,536 and you think, oh, that's beautiful. 756 00:40:48,560 --> 00:40:49,976 Wouldn't it be great to see that in person? 757 00:40:50,000 --> 00:40:52,506 The answer is no, no, it wouldn't 758 00:40:52,530 --> 00:40:54,416 because they will kill you. 759 00:40:54,440 --> 00:40:57,916 What's causing these displays are subatomic particles 760 00:40:57,940 --> 00:41:00,786 accelerated to tremendously high speeds 761 00:41:00,810 --> 00:41:03,516 by the magnetic fields involved. 762 00:41:03,540 --> 00:41:06,626 The radiation around Jupiter is lethal 763 00:41:06,650 --> 00:41:08,956 and not just for humans. 764 00:41:08,980 --> 00:41:11,526 The lifetime of the Juno mission is very limited 765 00:41:11,550 --> 00:41:14,496 by the extreme conditions it has to survive in. 766 00:41:14,520 --> 00:41:15,866 We think that in the future, 767 00:41:15,890 --> 00:41:17,636 a lot of the instruments will be so irradiated, 768 00:41:17,660 --> 00:41:21,276 they won't really work anymore. 769 00:41:21,300 --> 00:41:23,976 When Juno's titanium armor finally fails, 770 00:41:24,000 --> 00:41:29,646 Jupiter's deadly radiation will damage the craft beyond repair, 771 00:41:29,670 --> 00:41:32,716 so the team plan to go out with a bang, 772 00:41:32,740 --> 00:41:36,456 thrusting Juno into Jupiter's atmosphere, 773 00:41:36,480 --> 00:41:39,556 where the craft will be torn to pieces. 774 00:41:39,580 --> 00:41:42,856 Eventually, it'll be drawn down into Jupiter's depths 775 00:41:42,880 --> 00:41:45,996 and become a part of the planet itself. 776 00:41:46,020 --> 00:41:47,596 But before then, 777 00:41:47,620 --> 00:41:51,306 Juno has many more mysteries to unlock. 778 00:41:51,330 --> 00:41:54,306 We'll answer some questions, and we'll raise some more. 779 00:41:54,330 --> 00:41:56,076 That's what I expect 780 00:41:56,100 --> 00:41:59,606 and we'll get some fantastic images. 781 00:41:59,630 --> 00:42:03,046 Every single thing has turned out to be a surprise. 782 00:42:03,070 --> 00:42:05,516 There are so many things that Juno has opened our eyes to that 783 00:42:05,540 --> 00:42:08,486 I can't imagine having not sent it. 784 00:42:08,510 --> 00:42:10,086 So we're in for at least a year 785 00:42:10,110 --> 00:42:13,826 more of the most profound surprises about Jupiter. 786 00:42:13,850 --> 00:42:16,796 What we're learning, what we're unlocking, 787 00:42:16,820 --> 00:42:18,296 not just about Jupiter, 788 00:42:18,320 --> 00:42:20,266 but the formation of the solar system 789 00:42:20,290 --> 00:42:23,236 and potential formation of life itself 790 00:42:23,260 --> 00:42:24,966 here on earth, 791 00:42:24,990 --> 00:42:26,130 it's mind-blowing. 62982

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