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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:01,933 --> 00:00:04,463 Jupiter... Our largest planetary neighbor. 2 00:00:04,469 --> 00:00:05,699 Jupiter is the king of the planets for a good reason. 3 00:00:05,703 --> 00:00:08,372 It's the biggest. 4 00:00:08,373 --> 00:00:12,373 It dominated the evolution of the solar system. 5 00:00:12,377 --> 00:00:14,907 Jupiter is a violent world of radiation and storms 6 00:00:14,913 --> 00:00:17,381 on an epic scale. 7 00:00:17,382 --> 00:00:19,612 The interior of Jupiter is kind of hard to imagine. 8 00:00:19,617 --> 00:00:21,147 There may be a layer inside Jupiter 9 00:00:22,821 --> 00:00:25,151 where you get diamond rain. 10 00:00:25,156 --> 00:00:29,493 Today, NASA's Juno mission 11 00:00:29,494 --> 00:00:32,724 is unraveling Jupiter's deepest secrets. 12 00:00:32,730 --> 00:00:34,730 What forces shape its mysterious storms 13 00:00:34,732 --> 00:00:37,901 and cause volcanic eruptions 14 00:00:37,902 --> 00:00:40,902 that jet lava deep into space? 15 00:00:40,905 --> 00:00:42,773 Jupiter actually has more in common with our sun 16 00:00:42,774 --> 00:00:44,274 than it does with any of the other planets 17 00:00:44,275 --> 00:00:47,544 in the solar system. 18 00:00:47,545 --> 00:00:49,475 We venture deep inside the most extreme planet 19 00:00:49,480 --> 00:00:52,816 in the solar system 20 00:00:52,817 --> 00:00:58,057 to reveal its inner secrets and investigate 21 00:01:00,959 --> 00:01:04,928 if Jupiter could actually be the sun's secret twin. 22 00:01:04,929 --> 00:01:06,496 Have you ever dreamed about traveling out of this world? 23 00:01:06,497 --> 00:01:09,127 My name is Mike Massimino, 24 00:01:09,133 --> 00:01:11,933 and I turned that fantasy into a reality 25 00:01:11,936 --> 00:01:15,005 when I space-walked to repair the Hubble space telescope. 26 00:01:15,006 --> 00:01:17,836 Great job, Mike. 27 00:01:17,842 --> 00:01:20,772 Now as we expand our knowledge of our solar system 28 00:01:20,778 --> 00:01:23,148 from Mercury to the cosmic unknowns, 29 00:01:25,116 --> 00:01:28,116 I want to take you on a personal journey to... 30 00:01:28,119 --> 00:01:31,119 Captions by vitac... www.Vitac.Com 31 00:01:31,122 --> 00:01:32,789 captions paid for by discovery communications 32 00:01:32,790 --> 00:01:34,658 welcome to "the planets." 33 00:01:34,659 --> 00:01:36,989 I'm Mike Massimino. 34 00:01:36,995 --> 00:01:41,064 Of all the planets in our solar system, 35 00:01:41,065 --> 00:01:45,065 Jupiter is hands-down the biggest and the baddest. 36 00:01:45,069 --> 00:01:46,869 It's a beast of a world full of radiation and violent storms. 37 00:01:46,871 --> 00:01:49,971 It's got so much power, 38 00:01:49,974 --> 00:01:54,011 it's basically its own mini-solar system. 39 00:01:54,012 --> 00:01:55,812 And thanks to the new amazing high-resolution images 40 00:01:55,813 --> 00:02:00,483 from NASA's Juno mission, 41 00:02:00,485 --> 00:02:04,885 more of Jupiter's secrets are being revealed. 42 00:02:04,889 --> 00:02:08,659 Jupiter... The fifth planet from the sun 43 00:02:08,660 --> 00:02:11,890 and the largest in the solar system. 44 00:02:11,896 --> 00:02:17,434 Made almost entirely of hydrogen and helium, 45 00:02:17,435 --> 00:02:19,703 Jupiter stretches more than 85,000 miles across. 46 00:02:19,704 --> 00:02:23,874 It's unfathomably big. 47 00:02:23,875 --> 00:02:26,205 You know, you can fit 1,000 earths inside. 48 00:02:26,210 --> 00:02:27,377 Now scientists have launched a mission 49 00:02:27,378 --> 00:02:29,646 to study Jupiter 50 00:02:29,647 --> 00:02:33,016 in more detail than ever before. 51 00:02:33,017 --> 00:02:37,187 The Juno spacecraft that launched in 2011 52 00:02:37,188 --> 00:02:42,388 reached Jupiter's orbit in 2016, 53 00:02:42,393 --> 00:02:46,163 where it is capturing close-up images and collecting data. 54 00:02:46,164 --> 00:02:49,664 And these newest findings from Juno show a unique 55 00:02:49,667 --> 00:02:51,835 and extraordinarily complex world. 56 00:02:51,836 --> 00:02:53,836 Jupiter has 67 known moons 57 00:02:53,838 --> 00:02:55,368 and probably a giant number of ones 58 00:02:55,373 --> 00:02:57,703 that are not yet known. 59 00:02:57,709 --> 00:03:00,777 It's like a miniature solar system all of its own. 60 00:03:00,778 --> 00:03:05,178 It's a whole environment, a whole ecosystem. 61 00:03:05,183 --> 00:03:08,413 The conditions on and around Jupiter are extreme. 62 00:03:10,121 --> 00:03:12,821 It doesn't behave like an ordinary planet. 63 00:03:12,824 --> 00:03:16,393 Formed at the beginning of the solar system 64 00:03:16,394 --> 00:03:19,730 from the same stuff as the sun, 65 00:03:19,731 --> 00:03:22,399 Jupiter is an enigma. 66 00:03:22,400 --> 00:03:25,600 Is it hiding a secret history? 67 00:03:25,603 --> 00:03:28,673 Could Jupiter be a star in disguise? 68 00:03:31,576 --> 00:03:36,376 Spread across 50 square miles 69 00:03:36,381 --> 00:03:38,248 of baking sand in the scorching Mojave desert, 70 00:03:38,249 --> 00:03:40,979 these giant telescopes 71 00:03:43,888 --> 00:03:46,618 listen for radio signals in outer space. 72 00:03:46,624 --> 00:03:49,292 NASA's Steve Levin is on the front line, 73 00:03:49,293 --> 00:03:51,923 unlocking the secrets of Jupiter. 74 00:03:51,929 --> 00:03:53,497 We've known about Jupiter for thousands of years, 75 00:03:53,498 --> 00:03:54,664 and we've studied it with telescopes 76 00:03:54,665 --> 00:03:56,765 for hundreds of years. 77 00:03:56,768 --> 00:03:59,136 In fact, Jupiter was one of the very first objects 78 00:03:59,137 --> 00:04:01,805 in the sky that was studied with telescopes. 79 00:04:01,806 --> 00:04:05,442 But when we started using radio telescopes, 80 00:04:05,443 --> 00:04:09,413 we learned a lot of surprises about Jupiter. 81 00:04:09,414 --> 00:04:11,344 These telescopes observe space by looking at radio waves 82 00:04:11,349 --> 00:04:13,717 rather than visible light. 83 00:04:13,718 --> 00:04:17,454 And the radio waves that come from Jupiter 84 00:04:17,455 --> 00:04:20,724 aren't what scientists expect to see from a planet. 85 00:04:20,725 --> 00:04:23,193 One of the surprises was this enormous bright radio source 86 00:04:23,194 --> 00:04:26,094 that turned out to be Jupiter. 87 00:04:26,097 --> 00:04:28,267 Jupiter gives off a huge radio signal 88 00:04:30,001 --> 00:04:31,768 far too bright for its size. 89 00:04:31,769 --> 00:04:34,638 Scientists think these signals 90 00:04:34,639 --> 00:04:38,175 are created by small, charged particles 91 00:04:38,176 --> 00:04:40,844 interacting with a magnetic field. 92 00:04:40,845 --> 00:04:45,615 Most planets have a magnetic field, 93 00:04:45,616 --> 00:04:48,146 but Jupiter's is far larger than any other. 94 00:04:48,152 --> 00:04:49,920 In fact, the Juno spacecraft proved 95 00:04:49,921 --> 00:04:54,891 that Jupiter's magnetic field 96 00:04:54,892 --> 00:05:00,030 is 10 times stronger than that of the earth. 97 00:05:00,031 --> 00:05:02,631 So what is causing Jupiter's huge magnetic field? 98 00:05:02,633 --> 00:05:06,303 Scientists believe the answer might lie 99 00:05:08,339 --> 00:05:11,908 within alien chemistry deep within the planet. 100 00:05:11,909 --> 00:05:16,279 More than 300 million miles from earth, 101 00:05:16,280 --> 00:05:20,780 Jupiter is an unimaginably different world. 102 00:05:20,785 --> 00:05:23,985 It's a planet that astronomers call a "gas giant." 103 00:05:23,988 --> 00:05:28,125 It's made almost entirely from hydrogen, 104 00:05:28,126 --> 00:05:33,926 the same material that forms stars like the sun. 105 00:05:33,931 --> 00:05:38,301 But beneath its cloudy surface, a darkness looms. 106 00:05:38,302 --> 00:05:40,670 Scientists believe a thick, black liquid swirls below, 107 00:05:40,671 --> 00:05:45,771 where intense pressures and temperatures 108 00:05:45,776 --> 00:05:48,812 transform hydrogen into a strange new substance. 109 00:05:48,813 --> 00:05:53,713 The secret of Jupiter's giant magnetic field 110 00:05:53,718 --> 00:05:56,218 may lie within this abyss. 111 00:05:56,220 --> 00:05:59,420 Scientists in Edinburgh are conducting 112 00:05:59,423 --> 00:06:01,491 a remarkable experiment to find out. 113 00:06:01,492 --> 00:06:03,660 So, we call Jupiter a gas giant, 114 00:06:03,661 --> 00:06:05,328 but beneath the clouds of Jupiter, 115 00:06:05,329 --> 00:06:08,029 the planet's not really made of gas. 116 00:06:08,032 --> 00:06:12,202 It's made of something much, much stranger. 117 00:06:16,807 --> 00:06:18,675 Scientists know that Jupiter is 90% hydrogen. 118 00:06:18,676 --> 00:06:20,706 Let's go. Things work fast 119 00:06:20,711 --> 00:06:23,211 when they work here. 120 00:06:23,214 --> 00:06:26,683 This equipment can recreate some of the 121 00:06:26,684 --> 00:06:28,852 incredibly high pressures found inside Jupiter, 122 00:06:28,853 --> 00:06:32,753 to find out what happens to a gas 123 00:06:32,757 --> 00:06:35,926 under the extreme conditions deep inside the planet. 124 00:06:35,927 --> 00:06:37,257 In the bottom of the ocean, the pressure from all the water 125 00:06:37,261 --> 00:06:40,230 that's on top of you 126 00:06:40,231 --> 00:06:42,031 is about 1,000 times earth's atmospheric pressure. 127 00:06:42,033 --> 00:06:43,833 And in the center of the earth, 128 00:06:43,834 --> 00:06:45,664 it's about a million times. 129 00:06:45,670 --> 00:06:47,470 But in the center of Jupiter, 130 00:06:47,471 --> 00:06:49,371 it's almost a billion times 131 00:06:49,373 --> 00:06:51,673 the pressure of earth's atmosphere. 132 00:06:51,676 --> 00:06:53,476 Stewart is going to expose a gas 133 00:06:53,477 --> 00:06:56,613 more commonly found on earth 134 00:06:56,614 --> 00:06:59,950 to the pressures found deep within Jupiter. 135 00:06:59,951 --> 00:07:02,219 He uses oxygen because it's easier to control 136 00:07:02,220 --> 00:07:04,150 in the lab, yet reacts to pressure 137 00:07:04,155 --> 00:07:07,085 in the same way as hydrogen. 138 00:07:07,091 --> 00:07:08,591 Oxygen is very similar to hydrogen, 139 00:07:08,593 --> 00:07:11,962 and so, they have similar properties 140 00:07:11,963 --> 00:07:15,932 when you put them under pressure inside a planet. 141 00:07:15,933 --> 00:07:17,933 At low pressures, light can easily pass through the sample. 142 00:07:17,935 --> 00:07:19,835 If I put my hand behind the sample, 143 00:07:19,837 --> 00:07:22,467 the light goes away. 144 00:07:22,473 --> 00:07:25,273 So, we're seeing light, now, coming through oxygen, 145 00:07:25,276 --> 00:07:27,406 and we're able to see right through it. 146 00:07:27,411 --> 00:07:30,480 And of course, oxygen, like hydrogen, 147 00:07:30,481 --> 00:07:33,881 when you squeeze on it, it starts to change. 148 00:07:33,884 --> 00:07:35,714 Stewart begins to squeeze the gas. 149 00:07:35,720 --> 00:07:37,920 Under extreme pressures, 150 00:07:37,922 --> 00:07:42,692 the structure of oxygen transforms. 151 00:07:42,693 --> 00:07:45,362 - 62, 63. - There it goes. 152 00:07:45,363 --> 00:07:48,999 The oxygen has now just turned solid, 153 00:07:49,000 --> 00:07:52,000 and crystals are starting to form in the system. 154 00:07:52,003 --> 00:07:55,272 The oxygen becomes opaque. 155 00:07:55,273 --> 00:07:56,940 It's beginning to change its structure. 156 00:07:56,941 --> 00:08:00,441 We're starting to see, the oxygen's beginning 157 00:08:00,444 --> 00:08:03,680 to turn a little bit darker and a little more orange, 158 00:08:03,681 --> 00:08:05,849 and there it goes. 159 00:08:05,850 --> 00:08:09,350 We've turned, now, our oxygen sample 160 00:08:09,353 --> 00:08:10,853 into a totally black substance here. 161 00:08:10,855 --> 00:08:14,324 We were trying to shine light through it, 162 00:08:14,325 --> 00:08:17,825 and it's being totally absorbed inside the oxygen. 163 00:08:17,828 --> 00:08:20,828 Stewart believes his experiments prove that the pressure 164 00:08:20,831 --> 00:08:23,361 within Jupiter transforms hydrogen gas 165 00:08:23,367 --> 00:08:25,567 into a new, different state. 166 00:08:25,569 --> 00:08:28,305 But this isn't enough to explain 167 00:08:28,306 --> 00:08:32,676 Jupiter's enormous magnetic field. 168 00:08:32,677 --> 00:08:34,477 An even stranger force must be at work. 169 00:08:34,478 --> 00:08:36,508 Deeper inside the planet, 170 00:08:39,383 --> 00:08:41,313 the conditions intensify. 171 00:08:41,319 --> 00:08:45,188 Beneath the dark hydrogen, 172 00:08:45,189 --> 00:08:49,089 scientists think there's an even more bizarre layer... 173 00:08:49,093 --> 00:08:53,930 An ocean of liquid, metallic hydrogen, 174 00:08:53,931 --> 00:08:59,231 an exotic state of hydrogen that doesn't exist on earth. 175 00:08:59,236 --> 00:09:02,806 12,000 miles deep, this metallic ocean transforms the planet 176 00:09:02,807 --> 00:09:05,807 into an enormous dynamo. 177 00:09:05,810 --> 00:09:11,147 As it spins, it creates a magnetic field 178 00:09:11,148 --> 00:09:14,888 that extends nearly 4 million miles around Jupiter, 179 00:09:17,588 --> 00:09:20,688 the biggest planetary structure in the solar system. 180 00:09:20,691 --> 00:09:23,560 Scientists now believe metallic hydrogen 181 00:09:23,561 --> 00:09:27,897 powers Jupiter's magnetic field. 182 00:09:27,898 --> 00:09:30,367 But in the lab, it's proving difficult to make. 183 00:09:30,368 --> 00:09:33,068 The only possible explanation for that magnetic field 184 00:09:33,070 --> 00:09:35,438 is the existence of a metallic state of hydrogen 185 00:09:35,439 --> 00:09:38,375 deep within Jupiter. And so, it's really... 186 00:09:38,376 --> 00:09:41,776 Experiments are trying to catch up to nature. 187 00:09:41,779 --> 00:09:44,979 The pressure inside Jupiter is unrivaled 188 00:09:44,982 --> 00:09:48,082 by the other planets in our solar system. 189 00:09:48,085 --> 00:09:50,954 Only the sun creates a greater force. 190 00:09:50,955 --> 00:09:54,555 Jupiter is so big, so massive that, 191 00:09:54,558 --> 00:09:55,988 we know, as you descend into the interior of Jupiter, 192 00:09:55,993 --> 00:09:58,393 you will reach pressures 193 00:09:58,396 --> 00:09:59,826 where an element like hydrogen 194 00:09:59,830 --> 00:10:03,330 doesn't just liquify. 195 00:10:03,334 --> 00:10:06,302 It actually begins to behave like a metal. 196 00:10:06,303 --> 00:10:09,033 Now, the reason a metal is shiny is that, 197 00:10:09,039 --> 00:10:11,469 metal atoms actually share electrons. 198 00:10:11,475 --> 00:10:12,775 And with the hydrogen compressed so close together, 199 00:10:12,777 --> 00:10:14,777 the same thing happens, 200 00:10:14,779 --> 00:10:17,079 and you get metallic hydrogen. 201 00:10:17,081 --> 00:10:18,748 This metallic hydrogen is something 202 00:10:18,749 --> 00:10:21,649 that is very difficult to make. 203 00:10:21,652 --> 00:10:24,952 But because Jupiter is so powerful, it's so cool, 204 00:10:24,955 --> 00:10:28,691 and it has such awesome gravity, 205 00:10:28,692 --> 00:10:32,962 it can create metallic hydrogen. 206 00:10:36,333 --> 00:10:40,033 Jupiter's magnetic field reaches out deep into space. 207 00:10:40,037 --> 00:10:41,767 When tiny charged particles come into contact with it, 208 00:10:41,772 --> 00:10:45,208 they produce radio waves 209 00:10:45,209 --> 00:10:48,509 that telescopes can detect on earth. 210 00:10:48,512 --> 00:10:50,480 Scientists observing Jupiter in ultraviolet light 211 00:10:50,481 --> 00:10:53,611 can see an extraordinary phenomena 212 00:10:53,617 --> 00:10:56,017 caused by the magnetic field... 213 00:10:56,020 --> 00:10:58,750 Huge auroras, 214 00:10:58,756 --> 00:11:00,186 the brightest and biggest in the solar system. 215 00:11:00,191 --> 00:11:01,658 The auroras here on earth, 216 00:11:01,659 --> 00:11:04,089 our northern and Southern lights, 217 00:11:04,094 --> 00:11:05,994 are caused by the interaction of our magnetic field 218 00:11:05,996 --> 00:11:08,565 with particles from the sun. 219 00:11:08,566 --> 00:11:10,996 Well, Jupiter's magnetic field is so extreme, 220 00:11:11,001 --> 00:11:14,637 it actually generates auroras all by itself. 221 00:11:14,638 --> 00:11:18,408 But the unparalleled brightness of Jupiter's auroras 222 00:11:18,409 --> 00:11:22,549 can't be explained by its magnetic field alone. 223 00:11:28,157 --> 00:11:30,487 What awesome power is fueling Jupiter's auroras? 224 00:11:30,493 --> 00:11:31,893 When I first travelled to the Hubble space telescope 225 00:11:31,894 --> 00:11:35,530 as an astronaut, 226 00:11:35,531 --> 00:11:38,800 I was mesmerized by how bright the colors in space were. 227 00:11:38,801 --> 00:11:41,801 The sun's light was the whitest white I had ever seen. 228 00:11:41,804 --> 00:11:43,572 I can only imagine how bright the massive auroras around 229 00:11:43,573 --> 00:11:46,942 Jupiter look from space. 230 00:11:46,943 --> 00:11:50,613 But what's causing this majestic light show around Jupiter? 231 00:11:52,815 --> 00:11:55,183 NASA's Juno spacecraft is on the mission to find out. 232 00:11:55,184 --> 00:11:58,120 Jupiter behaves more like a star 233 00:11:58,121 --> 00:12:02,557 than an ordinary planet, like earth. 234 00:12:02,558 --> 00:12:05,427 It's made from the same stuff as the sun, 235 00:12:05,428 --> 00:12:10,598 and supercharged auroras suggest 236 00:12:10,600 --> 00:12:15,100 that extremely powerful radiation surrounds Jupiter. 237 00:12:15,104 --> 00:12:17,234 This makes getting near to the planet very difficult. 238 00:12:17,240 --> 00:12:18,707 Trying to get anywhere close to Jupiter 239 00:12:18,708 --> 00:12:21,338 is really, really hard 240 00:12:21,344 --> 00:12:22,874 because of the intense radiation of the magnetic field. 241 00:12:22,879 --> 00:12:25,409 So, when you send a spacecraft, 242 00:12:25,415 --> 00:12:27,783 you understand it's not gonna live for very long. 243 00:12:27,784 --> 00:12:31,784 We've not been to Jupiter that many times, 244 00:12:33,156 --> 00:12:35,386 which is one reason NASA's Juno mission is so exciting. 245 00:12:35,391 --> 00:12:38,221 The Juno spacecraft has been sent 246 00:12:38,227 --> 00:12:40,627 right into the heart of Jupiter's auroras 247 00:12:40,630 --> 00:12:42,097 to discover the secrets behind the radiation 248 00:12:42,098 --> 00:12:44,298 that causes them. 249 00:12:44,300 --> 00:12:48,537 Launched in 2011, 250 00:12:48,538 --> 00:12:51,468 Juno traveled at more than 124,000 miles per hour, 251 00:12:51,474 --> 00:12:53,674 to reach Jupiter in 2016. 252 00:12:53,676 --> 00:12:57,946 It's currently orbiting the planet, 253 00:12:57,947 --> 00:13:01,516 and will circle it 37 times during its mission. 254 00:13:01,517 --> 00:13:03,985 While in orbit, Juno is sending back images of Jupiter 255 00:13:03,986 --> 00:13:08,023 like we've never seen before. 256 00:13:08,024 --> 00:13:12,194 This first-ever infrared image of Jupiter's Southern lights 257 00:13:12,195 --> 00:13:16,731 shows off its incredible auroras. 258 00:13:16,732 --> 00:13:19,568 This is NASA's jet propulsion laboratory in California. 259 00:13:19,569 --> 00:13:21,036 It's the nerve center for the Juno mission. 260 00:13:21,037 --> 00:13:23,637 The data's looking amazing. 261 00:13:23,639 --> 00:13:26,308 All the scientists are incredibly excited. 262 00:13:26,309 --> 00:13:29,109 Heidi Becker is studying the radiation environment 263 00:13:29,111 --> 00:13:30,911 around Jupiter using Juno. 264 00:13:30,913 --> 00:13:33,181 When Juno went through the really nasty 265 00:13:33,182 --> 00:13:38,482 radiation environment for the first time, 266 00:13:38,488 --> 00:13:41,988 it's kind of an edge-of-your-seat-type moment. 267 00:13:41,991 --> 00:13:44,159 Heidi measures the strength of radiation around Jupiter 268 00:13:44,160 --> 00:13:47,429 by looking at photographs of stars 269 00:13:47,430 --> 00:13:49,660 taken by the Juno spacecraft. 270 00:13:49,665 --> 00:13:51,365 This is a regular, 271 00:13:51,367 --> 00:13:55,067 radiation-free image 272 00:13:55,071 --> 00:13:57,939 collected by Juno's star tracker. 273 00:13:57,940 --> 00:14:01,376 The stars appear like points of light, 274 00:14:01,377 --> 00:14:04,746 like you're used to when you look up at the stars at night. 275 00:14:04,747 --> 00:14:07,347 The stars are constant points of light in the photograph, 276 00:14:07,350 --> 00:14:10,480 but when radiation particles hit the camera, 277 00:14:10,486 --> 00:14:12,216 they appear, suddenly, as additional white spots 278 00:14:12,221 --> 00:14:15,991 and streaks of light. 279 00:14:15,992 --> 00:14:17,792 So, each of these frames is another level of radiation. 280 00:14:17,793 --> 00:14:19,893 And all of these squiggles and holes 281 00:14:19,896 --> 00:14:22,296 that are being added to this star field, 282 00:14:22,298 --> 00:14:24,165 that's the radiation signature. 283 00:14:24,166 --> 00:14:26,935 These are the radiation particles 284 00:14:26,936 --> 00:14:30,036 that create Jupiter's auroras. 285 00:14:30,039 --> 00:14:32,207 The particles are kind of like machine-gun fire, 286 00:14:32,208 --> 00:14:34,976 creating bullet holes in an image. 287 00:14:34,977 --> 00:14:36,677 And so, we can count those individual bullet holes, 288 00:14:36,679 --> 00:14:38,146 and that's what helps me understand 289 00:14:38,147 --> 00:14:43,447 the radiation environment. 290 00:14:43,452 --> 00:14:46,388 So, one person's noise is another person's music or data. 291 00:14:46,389 --> 00:14:48,419 This data from Juno allows scientists 292 00:14:48,424 --> 00:14:51,393 to map the planet's radiation. 293 00:14:51,394 --> 00:14:54,794 The radiation fields of Jupiter are so intense, 294 00:14:54,797 --> 00:14:57,766 we know they're going to eventually fry our spacecraft. 295 00:14:57,767 --> 00:15:00,997 Juno has on the order of about a 2-year lifetime. 296 00:15:01,003 --> 00:15:05,203 We understand that. 297 00:15:05,207 --> 00:15:07,075 This intense radiation lights up Jupiter's auroras, 298 00:15:07,076 --> 00:15:12,576 but where does it come from? 299 00:15:12,582 --> 00:15:16,051 What's feeding Jupiter's magnetic field with radiation? 300 00:15:16,052 --> 00:15:18,682 Scientists looking for evidence have spotted clues 301 00:15:18,688 --> 00:15:21,218 in a mysterious bright spot 302 00:15:24,093 --> 00:15:25,523 tracing a path across the lights. 303 00:15:25,528 --> 00:15:28,258 They now think that lo, 304 00:15:28,264 --> 00:15:31,600 one of the 67 moons that orbit Jupiter, 305 00:15:31,601 --> 00:15:34,069 holds the key to the planet's auroras. 306 00:15:34,070 --> 00:15:35,800 There's this very intense magnetic interaction 307 00:15:35,805 --> 00:15:38,035 between Jupiter and its moons, 308 00:15:38,040 --> 00:15:41,240 and you can actually see this in the Aurora. 309 00:15:41,243 --> 00:15:42,643 And you see a glowing spot moving around in the auroras. 310 00:15:42,645 --> 00:15:45,675 And one of the most dramatic ones, 311 00:15:45,681 --> 00:15:50,151 the most dramatic footprints to see, is that of lo. 312 00:15:50,152 --> 00:15:53,752 Io orbits at 217,000 miles from Jupiter, 313 00:15:53,756 --> 00:15:57,125 held in place by the planet's massive gravity. 314 00:15:57,126 --> 00:15:59,856 It's nothing like the moon that orbits earth. 315 00:15:59,862 --> 00:16:02,530 When we sent our first spacecraft, 316 00:16:02,531 --> 00:16:04,461 we saw, amazingly, 317 00:16:04,467 --> 00:16:06,597 volcanoes going off. 318 00:16:06,602 --> 00:16:11,372 Could these remote volcanoes 319 00:16:15,811 --> 00:16:19,011 be the source of Jupiter's supercharged auroras? 320 00:16:19,014 --> 00:16:21,944 On my second mission on space shuttle Atlantis, 321 00:16:21,950 --> 00:16:23,950 we brought a replica of Galileo's telescope 322 00:16:23,952 --> 00:16:28,122 just like the one that he used to discover 323 00:16:28,123 --> 00:16:30,323 Jupiter's four largest moons, including lo. 324 00:16:30,325 --> 00:16:33,094 In Galileo's wildest dreams, 325 00:16:33,095 --> 00:16:35,425 he probably never would've theorized that volcanoes 326 00:16:35,430 --> 00:16:37,430 on lo would be playing a role in 327 00:16:37,432 --> 00:16:39,600 Jupiter's stunning auroras. 328 00:16:39,601 --> 00:16:41,371 But that's just what some scientists 329 00:16:43,038 --> 00:16:46,138 are on the hunt to prove. 330 00:16:46,141 --> 00:16:49,009 Scientists at Syracuse university in New York 331 00:16:49,010 --> 00:16:52,010 are investigating if volcanoes on lo 332 00:16:52,013 --> 00:16:54,243 are the cause of Jupiter's magnificent auroras 333 00:16:54,249 --> 00:16:56,517 by making their own volcano. 334 00:16:56,518 --> 00:16:59,148 I've poured lava over 1,000 times, 335 00:16:59,154 --> 00:17:01,454 and probably have seen more lava 336 00:17:01,456 --> 00:17:05,456 than a lot of volcanologists. 337 00:17:05,460 --> 00:17:08,290 Professor Bob Wysocki runs the lava project. 338 00:17:08,296 --> 00:17:11,832 He uses his homemade furnace to replicate 339 00:17:11,833 --> 00:17:14,263 the geological conditions on other worlds. 340 00:17:14,269 --> 00:17:17,669 Tonight, he's gearing up to investigate 341 00:17:17,672 --> 00:17:20,508 how volcanic activity on one of Jupiter's moons 342 00:17:20,509 --> 00:17:23,239 might fuel the planet's deadly radiation 343 00:17:23,245 --> 00:17:26,445 and light up its auroras. 344 00:17:26,448 --> 00:17:30,684 Bob heats basalt rock until it melts. 345 00:17:30,685 --> 00:17:32,785 The furnace burns at 2,300 degrees Fahrenheit. 346 00:17:32,787 --> 00:17:35,317 It takes an immense amount of energy 347 00:17:35,323 --> 00:17:37,923 to melt even a small amount of rock. 348 00:17:37,926 --> 00:17:40,256 So, where does lo get the energy 349 00:17:40,262 --> 00:17:44,832 to fuel its volcanoes? 350 00:17:44,833 --> 00:17:46,133 All signs point to lo's immense immense and malevolent neighbor, 351 00:17:46,134 --> 00:17:49,970 Jupiter. 352 00:17:49,971 --> 00:17:52,301 The planet traps lo in a gravitational tug-of-war 353 00:17:52,307 --> 00:17:56,076 with other orbiting moons. 354 00:17:56,077 --> 00:17:59,677 Inside lo, the relentless push and pull from Jupiter 355 00:17:59,681 --> 00:18:03,251 heats up the interior to melting point, 356 00:18:05,420 --> 00:18:06,750 creating smoldering currents beneath the surface. 357 00:18:06,755 --> 00:18:10,325 As the pressure builds, 358 00:18:12,827 --> 00:18:15,327 the lava finally erupts through the moon's crust. 359 00:18:15,330 --> 00:18:18,199 It shoots scorching fountains of lava 360 00:18:18,200 --> 00:18:21,700 up to half-a-mile high 361 00:18:25,373 --> 00:18:27,741 and floods the frozen surface with molten rock. 362 00:18:27,742 --> 00:18:31,212 - Okay, Jeff, you ready to go? - Yeah. 363 00:18:31,213 --> 00:18:33,213 In Syracuse, Bob is ready to pour the lava. 364 00:18:33,215 --> 00:18:35,945 We are just that one step below 365 00:18:35,951 --> 00:18:40,187 what comes out of a volcano 366 00:18:40,188 --> 00:18:41,988 and making and replicating what happens in nature. 367 00:18:41,990 --> 00:18:43,620 Well, we're doing an experiment today 368 00:18:43,625 --> 00:18:46,725 to try to better understand 369 00:18:46,728 --> 00:18:49,728 what happens when ice meets lava. 370 00:18:49,731 --> 00:18:54,201 Geologist Jeff Karson is joining Bob 371 00:18:54,202 --> 00:18:56,870 to see what happens when volcanoes erupt on lo. 372 00:18:56,871 --> 00:19:02,409 Io is extremely cold. 373 00:19:02,410 --> 00:19:05,140 Its surface is made from sulfur dioxide that is frozen solid. 374 00:19:05,146 --> 00:19:09,146 Bob monitors the furnace, while Jeff examines 375 00:19:09,150 --> 00:19:12,219 how lava interacts with the ice. 376 00:19:12,220 --> 00:19:15,289 The physics that govern the way the lava flows form, 377 00:19:15,290 --> 00:19:18,020 the way they cool, the shapes they take on, 378 00:19:18,026 --> 00:19:21,695 these are all the same on other planetary objects, 379 00:19:21,696 --> 00:19:23,996 but the same basic physics applies. 380 00:19:23,999 --> 00:19:26,229 Scientists believe that the hot lava 381 00:19:26,234 --> 00:19:27,901 pouring out of lo's volcanoes 382 00:19:27,902 --> 00:19:31,072 onto its icy surface 383 00:19:33,575 --> 00:19:35,975 has a direct effect on Jupiter's radiation. 384 00:19:35,977 --> 00:19:37,444 Moving onto the ice, 385 00:19:37,445 --> 00:19:39,775 a bunch of bubbles are starting to form. 386 00:19:39,781 --> 00:19:42,349 You see a completely different style 387 00:19:42,350 --> 00:19:43,550 of behavior of the lava here. 388 00:19:43,551 --> 00:19:47,151 I'm gonna step back, actually, 389 00:19:47,155 --> 00:19:48,585 'cause I can feel the heat so intensely here. 390 00:19:48,590 --> 00:19:51,358 But those bubbles are forming 391 00:19:51,359 --> 00:19:53,389 because water vapor is being produced, 392 00:19:53,395 --> 00:19:55,325 boiling the water in the ice. 393 00:19:55,330 --> 00:19:58,830 The vapor is escaping through the lava 394 00:19:58,833 --> 00:20:00,233 and blowing these beautiful bubbles. 395 00:20:00,235 --> 00:20:02,765 It's a really good analog 396 00:20:02,771 --> 00:20:05,839 for what could be happening on other planetary objects, 397 00:20:05,840 --> 00:20:08,440 like on lo. 398 00:20:08,443 --> 00:20:12,313 The hot lava causes the frozen ice 399 00:20:12,314 --> 00:20:13,714 to instantly vaporize into clouds of steam. 400 00:20:13,715 --> 00:20:17,051 On a place like lo, 401 00:20:17,052 --> 00:20:19,482 it would be sulfur that's being vaporized, 402 00:20:19,487 --> 00:20:22,387 and sulfur dioxide making bubbles 403 00:20:22,390 --> 00:20:26,560 and being released into the atmosphere. 404 00:20:26,561 --> 00:20:27,728 Scientists now think that vaporized sulfur dioxide 405 00:20:27,729 --> 00:20:32,566 is the key ingredient 406 00:20:32,567 --> 00:20:36,967 to explain Jupiter's extraordinary auroras. 407 00:20:36,971 --> 00:20:42,209 Io's volcanoes vaporize the toxic sulfur dioxide. 408 00:20:42,210 --> 00:20:47,047 They blast it into a nearly 50-mile umbrella plume. 409 00:20:47,048 --> 00:20:49,416 One ton every second flies into orbit around Jupiter. 410 00:20:49,417 --> 00:20:52,217 The sulfur dioxide supercharges 411 00:20:52,220 --> 00:20:54,820 the deadly radiation belt around the planet 412 00:20:54,823 --> 00:20:57,453 with a lethal particle storm. 413 00:20:57,459 --> 00:20:59,389 Jupiter's magnetic field then captures 414 00:20:59,394 --> 00:21:01,894 the sulfur dioxide particles 415 00:21:01,896 --> 00:21:04,996 and accelerates them to the poles of the planet 416 00:21:04,999 --> 00:21:07,067 at almost the speed of light. 417 00:21:07,068 --> 00:21:10,738 They strike Jupiter's atmosphere 418 00:21:10,739 --> 00:21:13,439 and create the spectacular Aurora patterns, 419 00:21:13,441 --> 00:21:16,410 over 100 times more energetic 420 00:21:16,411 --> 00:21:18,911 than the northern lights on earth. 421 00:21:18,913 --> 00:21:22,013 And now, thanks to Juno imagery, 422 00:21:22,016 --> 00:21:26,253 scientists have confirmed that lo's volcanoes 423 00:21:26,254 --> 00:21:28,384 are indeed contributing to this massive light show. 424 00:21:28,390 --> 00:21:33,660 These eruptions on Jupiter's moon 425 00:21:33,661 --> 00:21:37,561 help generate a lethal radiation engulfing the whole planet. 426 00:21:37,565 --> 00:21:41,535 But it's not just radiation that makes Jupiter so extreme. 427 00:21:41,536 --> 00:21:43,904 Deadly storms rage on the surface. 428 00:21:43,905 --> 00:21:46,373 Today, Juno is sending back photos 429 00:21:46,374 --> 00:21:49,174 of unimaginable weather systems, 430 00:21:49,177 --> 00:21:53,113 enormously more powerful than even the most 431 00:21:53,114 --> 00:21:56,014 terrifying hurricanes on earth. 432 00:21:56,017 --> 00:21:58,185 The weather on Jupiter is pretty darn extreme. 433 00:21:58,186 --> 00:22:00,116 There are these belts that have winds 434 00:22:00,121 --> 00:22:02,221 that are zooming around very quickly, 435 00:22:02,223 --> 00:22:04,023 and then in one direction in one 436 00:22:04,025 --> 00:22:06,193 and then the other direction in the other. 437 00:22:06,194 --> 00:22:07,794 Among all the swirling bands, 438 00:22:07,796 --> 00:22:10,796 there's an enigma, 439 00:22:10,799 --> 00:22:14,769 one feature that doesn't seem to change... 440 00:22:20,471 --> 00:22:23,640 Jupiter's famous great red spot. 441 00:22:23,641 --> 00:22:26,071 When I space-walked for the first time in 2002 442 00:22:26,076 --> 00:22:28,506 to help repair the Hubble space telescope, 443 00:22:28,512 --> 00:22:30,342 I just couldn't believe how incredible the earth 444 00:22:30,347 --> 00:22:33,647 looked from outer space. 445 00:22:33,651 --> 00:22:36,481 One of the coolest sights were the lightning storms. 446 00:22:36,487 --> 00:22:38,955 But the storms on earth are nothing compared to 447 00:22:38,956 --> 00:22:42,156 the ferocious ones on Jupiter. 448 00:22:42,159 --> 00:22:44,089 And as scientists find out more about these storms, 449 00:22:44,094 --> 00:22:48,264 they're unlocking the secrets 450 00:22:48,265 --> 00:22:53,265 to the planet's mysterious red spot. 451 00:22:53,270 --> 00:22:55,438 Jupiter... more than 1,000 times larger than the earth. 452 00:22:55,439 --> 00:22:57,839 It's the biggest and baddest planet 453 00:22:57,841 --> 00:23:00,641 in the solar system. 454 00:23:00,644 --> 00:23:04,580 It's so deadly, it seems to have more in common 455 00:23:04,581 --> 00:23:06,881 with the sun than a planet like earth. 456 00:23:06,884 --> 00:23:09,384 Jupiter has single storms 457 00:23:09,386 --> 00:23:11,716 that are larger than its neighboring planets. 458 00:23:11,722 --> 00:23:14,290 They rage for centuries and create 459 00:23:14,291 --> 00:23:16,091 its unmistakable appearance. 460 00:23:16,093 --> 00:23:18,093 If you were to go to Jupiter, you'd be in for 461 00:23:18,095 --> 00:23:20,225 some very serious weather. 462 00:23:20,230 --> 00:23:22,660 But, hey, maybe the kitesurfing would be good, 463 00:23:22,666 --> 00:23:26,302 or the parachuting, because you have to deal with 464 00:23:26,303 --> 00:23:31,773 some serious winds and some serious storms. 465 00:23:31,775 --> 00:23:35,645 In 2017, the Juno mission sent back photos of Jupiter's poles, 466 00:23:35,646 --> 00:23:38,046 which were covered in dense, massive storms. 467 00:23:38,048 --> 00:23:40,616 The Southern pole boasts cyclones 468 00:23:40,617 --> 00:23:43,786 that are 600 miles in diameter, 469 00:23:43,787 --> 00:23:46,187 the size of Texas. 470 00:23:46,190 --> 00:23:50,827 And close to Jupiter's northern pole, 471 00:23:50,828 --> 00:23:53,896 this anti-cyclonic storm is 3,700 miles long, 472 00:23:53,897 --> 00:23:56,065 bigger than the entire U.S. 473 00:23:56,066 --> 00:23:58,696 But even this storm doesn't compare 474 00:23:58,702 --> 00:24:00,202 to Jupiter's great red spot. 475 00:24:00,204 --> 00:24:03,034 The great red spot 476 00:24:03,040 --> 00:24:06,109 is this gigantic swirling storm 477 00:24:06,110 --> 00:24:08,810 that has lasted for hundreds of years. 478 00:24:08,812 --> 00:24:11,481 You know, storms on earth don't last that long. 479 00:24:11,482 --> 00:24:14,612 Jupiter's great red spot is one of the biggest 480 00:24:14,618 --> 00:24:17,987 and oldest storms in the solar system. 481 00:24:17,988 --> 00:24:20,618 The Juno cam captured the closest-ever photos of the spot 482 00:24:20,624 --> 00:24:25,194 on July 10, 2017, 483 00:24:25,195 --> 00:24:28,795 recording storm clouds moving at over 350 miles per hour. 484 00:24:30,134 --> 00:24:33,664 But the mystery remains. What keeps it spinning? 485 00:24:33,670 --> 00:24:38,670 Scientists at UCLA's spinlab in California 486 00:24:38,675 --> 00:24:41,175 are trying to understand Jupiter's extreme weather. 487 00:24:41,178 --> 00:24:42,908 It would be impossible for us to get to Jupiter and survive, 488 00:24:42,913 --> 00:24:45,543 so we have the next best thing. Here at spinlab, 489 00:24:45,549 --> 00:24:48,017 we do simulations of Jupiter in the lab. 490 00:24:48,018 --> 00:24:50,418 Juan Lora has a surprising tool 491 00:24:50,420 --> 00:24:52,450 to understand Jupiter's atmosphere... 492 00:24:52,456 --> 00:24:53,886 A tank of water. 493 00:24:53,891 --> 00:24:56,991 With this setup here, 494 00:24:56,994 --> 00:24:59,024 we are simulating a planetary atmosphere in the lab. 495 00:24:59,029 --> 00:25:01,529 I know it doesn't look much like a planet, 496 00:25:01,532 --> 00:25:04,332 but imagine just looking down at the center of the table, 497 00:25:04,334 --> 00:25:05,764 and that represents the polar region of the planet. 498 00:25:05,769 --> 00:25:08,599 The table will spin. 499 00:25:08,605 --> 00:25:12,805 So, as you head out to the edges of the table, 500 00:25:12,810 --> 00:25:15,110 that represents lower latitudes on the planet. 501 00:25:15,112 --> 00:25:19,081 Jupiter is the fastest spinning planet 502 00:25:19,082 --> 00:25:23,482 in the solar system. 503 00:25:23,487 --> 00:25:25,587 A day on Jupiter lasts only 10 hours. 504 00:25:25,589 --> 00:25:27,256 The fluid in the table is now spinning 505 00:25:27,257 --> 00:25:28,757 like a planetary atmosphere would be. 506 00:25:28,759 --> 00:25:30,389 So, now, we're gonna add some dye, 507 00:25:30,394 --> 00:25:33,763 and let's see what happens. 508 00:25:33,764 --> 00:25:35,694 The colored fluids represent different cloud systems. 509 00:25:35,699 --> 00:25:37,867 This experiment should reveal clues 510 00:25:37,868 --> 00:25:40,268 about how they interact. 511 00:25:40,270 --> 00:25:42,338 Adding any sort of turbulence to a rotating fluid 512 00:25:42,339 --> 00:25:46,909 will create some interesting dynamics. 513 00:25:46,910 --> 00:25:49,278 Juan stirs the water to create turbulence. 514 00:25:49,279 --> 00:25:51,609 Turbulence occurs in Jupiter's atmosphere 515 00:25:51,615 --> 00:25:53,315 when gasses of different temperatures and speeds 516 00:25:53,317 --> 00:25:55,284 come together. 517 00:25:55,285 --> 00:25:57,285 Once you get turbulence, and you disturb a fluid 518 00:25:57,287 --> 00:26:00,223 that is rotating quickly, 519 00:26:00,224 --> 00:26:02,924 like this tank and like Jupiter, then you get these vortices. 520 00:26:02,926 --> 00:26:06,426 And the vortices are very stable, 521 00:26:06,430 --> 00:26:08,830 and they like to interact with each other sometimes. 522 00:26:08,832 --> 00:26:10,399 This is like the red spot. 523 00:26:10,400 --> 00:26:12,430 As soon as it was formed, 524 00:26:12,436 --> 00:26:14,303 it is able to be maintained 525 00:26:14,304 --> 00:26:17,704 by the rotation of Jupiter. 526 00:26:17,708 --> 00:26:20,038 Jupiter's rotation energizes the great red spot 527 00:26:20,043 --> 00:26:23,213 and keeps it spinning. 528 00:26:24,748 --> 00:26:28,885 But how did it get so large in the first place? 529 00:26:28,886 --> 00:26:34,086 The great red spot is larger than whole planets. 530 00:26:34,091 --> 00:26:37,731 Winds whip around it at over 400 miles per hour to form a cyclone 531 00:26:39,863 --> 00:26:42,899 that rises nearly 5 miles above the clouds. 532 00:26:42,900 --> 00:26:46,500 The striking red color is believed to be the gas 533 00:26:46,503 --> 00:26:49,103 reacting with the sun's rays. 534 00:26:49,106 --> 00:26:53,242 Behind the sunburnt surface, 535 00:26:53,243 --> 00:26:55,511 these twisting clouds remain gray inside. 536 00:26:55,512 --> 00:26:58,681 As smaller storms approach, 537 00:26:58,682 --> 00:26:59,882 they are ruthlessly cannibalized by the giant. 538 00:26:59,883 --> 00:27:04,353 Their energy and spin 539 00:27:04,354 --> 00:27:08,324 add to the great red spot's size and power. 540 00:27:08,325 --> 00:27:13,125 Is this superstorm destined to rage forever? 541 00:27:13,130 --> 00:27:14,297 Today, scientists can see something strange is happening. 542 00:27:14,298 --> 00:27:15,498 Jupiter's great red spot 543 00:27:15,499 --> 00:27:18,067 has been changing over the past 20 years. 544 00:27:18,068 --> 00:27:19,468 So, here, an image taken in 1995, 545 00:27:19,469 --> 00:27:21,569 where you can see that the great red spot 546 00:27:21,571 --> 00:27:24,740 is quite large and oval-shaped. 547 00:27:24,741 --> 00:27:26,809 If you compare this image to one taken in 2009, 548 00:27:26,810 --> 00:27:28,678 the spot has become more circular, 549 00:27:28,679 --> 00:27:30,979 and it's also smaller in size. 550 00:27:30,981 --> 00:27:33,211 And then, from 2014, shows, again, 551 00:27:34,952 --> 00:27:39,488 a further shrinkage of the spot. 552 00:27:39,489 --> 00:27:45,695 These NASA photos show just how much the spot has changed 553 00:27:45,696 --> 00:27:50,132 from 1994 to the newest image in 2017. 554 00:27:50,133 --> 00:27:51,463 The great red spot feeds on other storms to survive. 555 00:27:51,468 --> 00:27:54,236 It consumes them, 556 00:27:54,237 --> 00:27:57,137 absorbing their energy to keep spinning. 557 00:27:57,140 --> 00:27:59,640 And if it's not fed, it'll starve. 558 00:27:59,643 --> 00:28:02,043 It's possible that, in the past 20 years, 559 00:28:02,045 --> 00:28:03,375 fewer of those vortices have come into contact 560 00:28:03,380 --> 00:28:06,449 with the great red spot. 561 00:28:06,450 --> 00:28:09,780 Scientists also think that some smaller storms 562 00:28:09,786 --> 00:28:12,786 could actually damage the great red spot. 563 00:28:12,789 --> 00:28:15,989 Another possibility is that it's eating, 564 00:28:15,993 --> 00:28:17,259 if you will, vortices that are spinning more slowly 565 00:28:17,260 --> 00:28:19,330 than it is spinning, 566 00:28:21,198 --> 00:28:25,698 and therefore, there's a net loss of spin. 567 00:28:25,702 --> 00:28:29,102 Storms that move more slowly or spin in the opposite direction 568 00:28:30,440 --> 00:28:33,270 could be putting the brakes on the great red spot. 569 00:28:33,276 --> 00:28:35,244 Its extraordinary longevity could simply be 570 00:28:35,245 --> 00:28:37,513 an exceptional streak of luck 571 00:28:37,514 --> 00:28:39,782 that's only now running out. 572 00:28:39,783 --> 00:28:41,583 The fact that it's changing, and so quickly, 573 00:28:41,585 --> 00:28:43,815 and so dramatically, after being stable 574 00:28:43,820 --> 00:28:46,150 for so long, does suggest that, maybe, 575 00:28:46,156 --> 00:28:48,786 something is taking place. 576 00:28:48,792 --> 00:28:51,092 Maybe it will shrink till the point we can't see it. 577 00:28:51,094 --> 00:28:54,330 We don't know. We have to keep watching. 578 00:28:54,331 --> 00:28:57,600 Only time will tell if Jupiter's most famous feature 579 00:28:57,601 --> 00:28:59,301 will survive another 100 years. 580 00:28:59,302 --> 00:29:04,240 The extreme physics on Jupiter 581 00:29:04,241 --> 00:29:06,371 creates unparalleled weather systems visible from space, 582 00:29:06,376 --> 00:29:10,046 and scientists are just beginning to understand 583 00:29:10,047 --> 00:29:13,647 the conditions inside the planet's clouds. 584 00:29:13,650 --> 00:29:14,880 What they're finding is extraordinary. 585 00:29:14,885 --> 00:29:16,585 One of the big surprises 586 00:29:16,586 --> 00:29:20,856 when we got to Jupiter with a spacecraft, 587 00:29:20,857 --> 00:29:23,357 was to see that there was lightning on the dark side. 588 00:29:23,360 --> 00:29:28,397 These images taken by NASA spacecraft 589 00:29:28,398 --> 00:29:31,667 are evidence of lightning strikes in Jupiter's atmosphere. 590 00:29:31,668 --> 00:29:36,638 They could trigger an astonishing chemical reaction 591 00:29:36,640 --> 00:29:39,809 deep inside Jupiter's colorful clouds. 592 00:29:39,810 --> 00:29:44,547 A thick fog of gas surrounds Jupiter. 593 00:29:44,548 --> 00:29:47,378 Friction in the clouds generates super bolts of lightning. 594 00:29:47,384 --> 00:29:49,114 These strikes are many times more powerful 595 00:29:51,888 --> 00:29:55,324 than lightning on earth. 596 00:29:55,325 --> 00:29:59,195 62 miles beneath the surface, 597 00:29:59,196 --> 00:30:02,096 the clouds harbor methane, as well as hydrogen. 598 00:30:02,099 --> 00:30:03,899 When the superheated electric shock 599 00:30:03,900 --> 00:30:05,700 rips through the atmosphere, 600 00:30:05,702 --> 00:30:08,402 the conditions are perfect 601 00:30:08,405 --> 00:30:11,435 for an extraordinary chemical reaction 602 00:30:17,104 --> 00:30:20,973 unlike anything else in the solar system. 603 00:30:20,974 --> 00:30:24,644 There's no question that 85,000 miles across, 604 00:30:24,645 --> 00:30:28,145 Jupiter is the king of all planets in the solar system. 605 00:30:28,148 --> 00:30:32,748 And the amazing forces at play on this hostile planet 606 00:30:32,753 --> 00:30:34,783 can create millions of jewels fit for a crown. 607 00:30:34,788 --> 00:30:37,288 Jupiter's lightning bolts are stronger 608 00:30:37,291 --> 00:30:39,358 than anything we've witnessed on earth, 609 00:30:39,359 --> 00:30:42,559 and the resulting chemical reaction 610 00:30:42,563 --> 00:30:46,093 unleashes a shower of unimaginable riches. 611 00:30:46,099 --> 00:30:48,468 The lightning transforms the elements into diamonds. 612 00:30:48,469 --> 00:30:50,499 Jupiter keeps its bling on the inside, 613 00:30:50,504 --> 00:30:52,034 because it may be raining diamonds. 614 00:30:52,039 --> 00:30:54,769 Now, think about this. 615 00:30:54,775 --> 00:30:57,243 Jupiter has incredibly strong winds, 616 00:30:57,244 --> 00:31:01,080 and diamonds are really hard. 617 00:31:01,081 --> 00:31:03,349 So, talk about a hail storm. 618 00:31:03,350 --> 00:31:04,850 Scientists at Cardiff university 619 00:31:04,852 --> 00:31:10,322 are trying to understand 620 00:31:10,324 --> 00:31:13,024 how diamonds might be created out of thin air on Jupiter. 621 00:31:13,026 --> 00:31:16,996 Professor Oliver Williams simulates Jupiter's 622 00:31:16,997 --> 00:31:20,166 lightning-charged atmosphere in the lab. 623 00:31:20,167 --> 00:31:21,797 I'm using an airtight chamber that I've sucked all the air out 624 00:31:21,802 --> 00:31:25,302 to make a vacuum. 625 00:31:25,305 --> 00:31:27,705 I'm flowing in 99% hydrogen and 1% methane, 626 00:31:27,708 --> 00:31:30,877 and this is like the atmosphere of Jupiter. 627 00:31:30,878 --> 00:31:34,308 But the experiment really begins when Oliver adds 628 00:31:34,314 --> 00:31:37,014 the final ingredient... Lightning. 629 00:31:37,017 --> 00:31:38,347 I'm gonna break this gas down using high-power microwaves. 630 00:31:38,352 --> 00:31:40,782 This is very like lightning, 631 00:31:40,787 --> 00:31:42,826 where the high electric field is breaking down the air 632 00:31:44,825 --> 00:31:47,393 and making these lightning bolts. 633 00:31:47,394 --> 00:31:51,464 Microwaves, like lightning on Jupiter, 634 00:31:51,465 --> 00:31:55,101 break down hydrogen and methane gas. 635 00:31:55,102 --> 00:31:57,902 It glows purple as the atoms break apart. 636 00:31:57,905 --> 00:32:01,105 So, diamond is fundamentally made out of carbon. 637 00:32:01,108 --> 00:32:04,038 Methane is actually carbon with four hydrogen atoms, 638 00:32:04,044 --> 00:32:07,680 and we're able to strip these hydrogen away. 639 00:32:07,681 --> 00:32:11,381 The microwaves release carbon atoms from methane gas. 640 00:32:11,385 --> 00:32:13,152 The atoms join together to form a diamond. 641 00:32:13,153 --> 00:32:16,923 Inside this chamber, 642 00:32:16,924 --> 00:32:19,792 a slice of diamond literally grows out of thin air. 643 00:32:19,793 --> 00:32:21,693 So, what we've done is, we've broken down these gasses 644 00:32:21,695 --> 00:32:23,695 that you do see in places like Jupiter. 645 00:32:23,697 --> 00:32:27,066 And from this chemistry, we've grown a crystalline form 646 00:32:27,067 --> 00:32:30,667 of carbon, which is diamond. 647 00:32:30,671 --> 00:32:33,201 Experiments like this suggest diamonds form like hail 648 00:32:33,206 --> 00:32:36,106 in Jupiter's lightning storms. 649 00:32:36,109 --> 00:32:38,539 But something even more extraordinary happens 650 00:32:38,545 --> 00:32:41,581 as they fall. 651 00:32:41,582 --> 00:32:42,882 As the diamonds are zapped into existence, 652 00:32:42,883 --> 00:32:47,820 they begin to descend 653 00:32:47,821 --> 00:32:50,121 through the atmosphere as diamond hail stones. 654 00:32:50,123 --> 00:32:53,823 They plummet thousands of miles 655 00:32:53,827 --> 00:32:58,364 through Jupiter's atmosphere, towards the core, 656 00:32:58,365 --> 00:33:01,901 racing into higher and higher pressures and temperatures. 657 00:33:01,902 --> 00:33:07,172 When they hit 14,400 degrees, 658 00:33:07,174 --> 00:33:08,404 they melt, creating a shower of liquid diamond raindrops. 659 00:33:08,408 --> 00:33:12,244 But what comes next 660 00:33:12,245 --> 00:33:14,245 is an even more bizarre theoretical possibility. 661 00:33:14,247 --> 00:33:17,917 Diamond rain could lead 662 00:33:17,918 --> 00:33:22,188 to a sparkling diamond ocean far below. 663 00:33:24,157 --> 00:33:26,157 Jupiter's world may be stranger than science fiction. 664 00:33:28,857 --> 00:33:30,011 The extreme physics on Jupiter 665 00:33:32,092 --> 00:33:33,939 creates weather totally unlike anything on earth. 666 00:33:34,768 --> 00:33:36,345 The tremendous forces forge a unique world 667 00:33:38,238 --> 00:33:39,008 in our solar system. 668 00:33:41,508 --> 00:33:43,047 In fact, Jupiter behaves more like a star 669 00:33:46,108 --> 00:33:53,109 than a mere planet. 670 00:33:56,239 --> 00:33:58,047 Could Jupiter actually be the sun's secret twin? 671 00:33:59,045 --> 00:34:00,661 Jupiter and earth are almost nothing alike. 672 00:34:02,418 --> 00:34:04,111 In fact, Jupiter doesn't share many qualities 673 00:34:06,518 --> 00:34:08,172 with any of the planets in our solar system. 674 00:34:10,392 --> 00:34:12,431 What if Jupiter wasn't supposed to be a planet at all? 675 00:34:14,830 --> 00:34:16,292 What if it's really a star in disguise? 676 00:34:18,230 --> 00:34:20,230 Images captured from NASA's Juno mission in 2017 show 677 00:34:21,834 --> 00:34:23,219 that Jupiter is a planet of extremes. 678 00:34:25,237 --> 00:34:27,084 It dwarfs every other planet in the solar system. 679 00:34:27,441 --> 00:34:28,604 So, was Jupiter meant to be a star? 680 00:34:28,611 --> 00:34:30,342 Just as the sun is made primarily of hydrogen, 681 00:34:30,411 --> 00:34:30,950 so is Jupiter. 682 00:34:32,081 --> 00:34:33,197 And so, it looks like a star, 683 00:34:34,411 --> 00:34:35,642 only it's one that's not burning. 684 00:34:36,346 --> 00:34:37,346 Jupiter is really massive, 685 00:34:38,982 --> 00:34:40,213 and it's held onto its hydrogen. 686 00:34:40,888 --> 00:34:42,658 So, that's kind of unusual in the solar system, 687 00:34:44,790 --> 00:34:46,175 is to have a planet made of hydrogen. 688 00:34:46,623 --> 00:34:48,692 Scientists are beginning to understand how Jupiter formed 689 00:34:48,699 --> 00:34:52,768 by investigating what happened 690 00:34:54,298 --> 00:34:55,298 in the early solar system. 691 00:34:57,743 --> 00:35:00,409 They're hunting for clues 692 00:35:02,709 --> 00:35:04,440 by observing the birth of other distant stars. 693 00:35:06,711 --> 00:35:07,942 Deep in the deserts of California 694 00:35:10,885 --> 00:35:12,385 sits the Owens valley radio observatory. 695 00:35:13,686 --> 00:35:15,686 These dishes make up the Carma radio telescope array. 696 00:35:18,928 --> 00:35:20,313 This location is absolutely gorgeous. 697 00:35:22,358 --> 00:35:23,857 Astronomer John Tobin scans the skies for newborn stars. 698 00:35:23,864 --> 00:35:25,826 Rather than building one really big radio telescope, 699 00:35:26,135 --> 00:35:27,289 which is very difficult to do, 700 00:35:27,435 --> 00:35:28,666 they built a lot of small dishes. 701 00:35:29,236 --> 00:35:30,429 Then they linked them together. 702 00:35:30,768 --> 00:35:32,115 And the further apart you move them, 703 00:35:32,773 --> 00:35:33,927 the higher resolution you get, 704 00:35:35,705 --> 00:35:37,359 which means it acts like a bigger telescope, 705 00:35:38,881 --> 00:35:39,974 and you can see finer detail. 706 00:35:39,981 --> 00:35:41,174 John is looking for protostars, 707 00:35:41,882 --> 00:35:42,459 brand-new stars 708 00:35:45,521 --> 00:35:46,637 that are only just condensing 709 00:35:48,051 --> 00:35:49,398 from a vast cloud of gas and debris. 710 00:35:50,787 --> 00:35:51,941 A protostar is a newborn star, 711 00:35:52,593 --> 00:35:54,055 so it's still in the process of forming 712 00:35:54,163 --> 00:35:55,125 and building up its mass. 713 00:35:56,031 --> 00:35:57,031 And in interstellar space, 714 00:36:00,731 --> 00:36:01,962 there are clouds of gas and dust, 715 00:36:04,536 --> 00:36:06,190 and at the center, a protostar will be born. 716 00:36:07,270 --> 00:36:09,347 Jupiter was formed from the same clouds of hydrogen gas 717 00:36:10,376 --> 00:36:11,415 and dust that formed stars. 718 00:36:13,549 --> 00:36:14,973 Could it have formed like a protostar? 719 00:36:16,349 --> 00:36:18,388 John is finding evidence thousands of light-years away 720 00:36:18,752 --> 00:36:20,099 that explains how star systems form. 721 00:36:20,784 --> 00:36:21,746 This image is showing you 722 00:36:23,589 --> 00:36:24,820 that the black and the contours, 723 00:36:25,661 --> 00:36:27,085 they're the intensity of the radiation 724 00:36:27,630 --> 00:36:28,991 that we're detecting from this protostar. 725 00:36:28,998 --> 00:36:30,191 There's not just one protostar, 726 00:36:31,728 --> 00:36:32,767 but there's two protostars. 727 00:36:34,803 --> 00:36:36,573 So, these two peaks that you see here and here, 728 00:36:38,703 --> 00:36:40,088 those are the two forming protostars. 729 00:36:42,144 --> 00:36:43,305 It's a solar system very different from our own. 730 00:36:43,312 --> 00:36:44,851 And my first reaction to this was, "wow." 731 00:36:46,977 --> 00:36:48,093 I couldn't believe the detail 732 00:36:49,551 --> 00:36:51,051 that we were seeing towards this object. 733 00:36:52,151 --> 00:36:54,190 Because previously, we knew there was one thing there, 734 00:36:55,084 --> 00:36:56,313 but then we found out that there looks like 735 00:36:56,320 --> 00:36:57,818 there's at least two objects around this protostar. 736 00:36:57,825 --> 00:36:58,902 And so, that was unexpected. 737 00:37:00,396 --> 00:37:02,050 We didn't know that we were gonna find that, 738 00:37:05,734 --> 00:37:06,965 and so that was a surprise to us. 739 00:37:09,604 --> 00:37:11,643 Could Jupiter have once stood toe-to-toe with the sun? 740 00:37:14,205 --> 00:37:16,205 From the outside, each young star system looks alike, 741 00:37:18,847 --> 00:37:20,709 starting life as a spiraling disc of dust and gas. 742 00:37:20,716 --> 00:37:22,447 But what evolves inside can be very different. 743 00:37:22,985 --> 00:37:24,178 Deep in the middle of the disc, 744 00:37:26,585 --> 00:37:28,009 turbulence can cause the central cloud 745 00:37:29,588 --> 00:37:33,562 to split into two and collapse into not one, 746 00:37:37,900 --> 00:37:39,247 but two shining stars in the center. 747 00:37:39,830 --> 00:37:41,600 The stars orbit each other in a hypnotic dance. 748 00:37:43,772 --> 00:37:44,734 Born from the same cloud, 749 00:37:48,042 --> 00:37:50,779 this solar system has twin stars. 750 00:37:56,418 --> 00:37:58,457 Any dust and gas left over will go on to form planets. 751 00:37:58,987 --> 00:38:01,026 In our solar system, the sun is the only shining star. 752 00:38:03,926 --> 00:38:05,273 But another massive ball of hydrogen 753 00:38:08,564 --> 00:38:09,911 quietly orbits from afar... Jupiter. 754 00:38:10,794 --> 00:38:12,948 Could this planet be the sun's double that didn't ignite? 755 00:38:13,869 --> 00:38:15,254 Scientists believe that solar systems 756 00:38:16,839 --> 00:38:18,032 with twin suns are very common. 757 00:38:20,639 --> 00:38:22,832 Well, since that first result using these telescopes here, 758 00:38:24,242 --> 00:38:25,939 we've been carrying out a much larger survey of protostars, 759 00:38:25,946 --> 00:38:27,641 in order to see just how many star systems form with two 760 00:38:27,648 --> 00:38:28,533 or three or more stars. 761 00:38:31,649 --> 00:38:33,534 And we're finding that a surprisingly large number 762 00:38:35,053 --> 00:38:36,746 of star systems form with more than one star. 763 00:38:37,657 --> 00:38:39,619 John wants to try to discover the precise conditions 764 00:38:40,396 --> 00:38:41,858 that create these binary solar systems, 765 00:38:44,833 --> 00:38:46,064 where two stars orbit each other. 766 00:38:47,533 --> 00:38:49,259 We've been putting together a compendium of images 767 00:38:49,266 --> 00:38:50,843 of young star systems in order to find out 768 00:38:52,741 --> 00:38:54,011 which ones are binary or multiple. 769 00:38:55,271 --> 00:38:56,656 So, this one is a single-star system. 770 00:38:57,307 --> 00:38:58,307 This one here is a double. 771 00:38:59,982 --> 00:39:01,059 As many as half of all stars 772 00:39:03,419 --> 00:39:04,766 in the universe have a partner star, 773 00:39:04,987 --> 00:39:06,718 both formed from a single disc of gas and dust 774 00:39:07,156 --> 00:39:07,849 that breaks apart. 775 00:39:09,856 --> 00:39:11,818 The system we were looking at is located right here, 776 00:39:11,858 --> 00:39:14,243 where the clouds of gas are kind of stretched out and extended. 777 00:39:15,197 --> 00:39:16,813 There might be multiple centers of collapse 778 00:39:18,297 --> 00:39:20,297 that can lead to the formation of more than one star. 779 00:39:20,769 --> 00:39:22,462 A cloud of gas and dust that is stretched out 780 00:39:22,869 --> 00:39:24,369 will likely collapse into multiple stars 781 00:39:24,740 --> 00:39:25,702 very close to each other. 782 00:39:27,640 --> 00:39:28,717 John thinks our solar system 783 00:39:29,973 --> 00:39:31,320 must have formed in a different way. 784 00:39:32,178 --> 00:39:33,409 So, we think our own solar system 785 00:39:36,018 --> 00:39:37,711 may have looked something more like this one, 786 00:39:38,618 --> 00:39:40,580 where you have just one star surrounded by its disc, 787 00:39:41,990 --> 00:39:43,414 and then the disc itself is lower mass 788 00:39:44,460 --> 00:39:46,460 and is not going to fragment into more than one star. 789 00:39:46,790 --> 00:39:48,483 Scientists believe the type of hydrogen cloud 790 00:39:51,465 --> 00:39:52,735 that gave rise to our solar system 791 00:39:54,497 --> 00:39:56,113 cut short Jupiter's quest to become a star. 792 00:40:00,542 --> 00:40:02,389 In its race to grow up, the sun got a head start, 793 00:40:05,842 --> 00:40:08,073 sucking up 99% of all the matter in the young solar system. 794 00:40:10,648 --> 00:40:12,418 When it reached 27 million degrees, it ignited. 795 00:40:13,322 --> 00:40:15,361 Meanwhile, the same cloud was condensing into Jupiter, 796 00:40:16,422 --> 00:40:17,961 rapidly snowballing to collect two-thirds 797 00:40:18,325 --> 00:40:19,402 of all the matter left over. 798 00:40:21,657 --> 00:40:23,004 But there was not enough matter left 799 00:40:24,700 --> 00:40:26,200 for Jupiter to get big enough to ignite, 800 00:40:27,269 --> 00:40:28,193 so it became a gas giant 801 00:40:30,806 --> 00:40:32,399 more than double the mass of all other planets 802 00:40:32,406 --> 00:40:33,522 in the solar system combined. 803 00:40:36,245 --> 00:40:36,899 No normal planet, 804 00:40:37,412 --> 00:40:38,836 Jupiter is the star's younger sibling. 805 00:40:39,812 --> 00:40:40,928 It would make sense to think, 806 00:40:43,185 --> 00:40:44,762 "well, where is the sun's binary partner?" 807 00:40:45,085 --> 00:40:46,662 And immediately, the mind goes to Jupiter. 808 00:40:47,256 --> 00:40:48,564 If Jupiter had gathered enough mass 809 00:40:50,726 --> 00:40:51,573 to ignite into a star, 810 00:40:54,026 --> 00:40:55,552 it's unlikely that the earth would have ever been formed. 811 00:40:55,559 --> 00:40:57,367 The solar system would be a very different place 812 00:41:01,336 --> 00:41:01,913 with twin suns. 813 00:41:02,936 --> 00:41:04,898 Instead, Jupiter became the most extraordinary world 814 00:41:05,107 --> 00:41:05,877 in the solar system. 815 00:41:08,337 --> 00:41:09,684 Everything about Jupiter is extreme. 816 00:41:11,380 --> 00:41:13,111 Its mass is more than 300 times that of earth. 817 00:41:13,310 --> 00:41:15,195 You could fit 1,000 earths inside this one planet. 818 00:41:15,284 --> 00:41:16,592 It has a magnetic field so intense, 819 00:41:18,654 --> 00:41:20,039 it would kill you with the radiation. 820 00:41:22,791 --> 00:41:24,330 Its winds blow at over 400 miles an hour. 821 00:41:25,121 --> 00:41:26,814 I mean, can you imagine a more extreme place? 822 00:41:27,757 --> 00:41:28,719 To me, Jupiter is perhaps 823 00:41:30,332 --> 00:41:31,893 the most fascinating object in our solar system. 824 00:41:31,900 --> 00:41:33,054 It's certainly the most alien. 825 00:41:34,700 --> 00:41:35,393 It is an enormous, 826 00:41:40,342 --> 00:41:41,419 strange ball of swirling gas 827 00:41:43,272 --> 00:41:45,119 surrounded by its own miniature planetary system. 828 00:41:46,108 --> 00:41:47,916 Formed at the very beginning of the solar system 829 00:41:50,714 --> 00:41:51,984 from the same material as the sun, 61844

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