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These are the user uploaded subtitles that are being translated: 1 00:00:01,140 --> 00:00:02,260 The Sun, 2 00:00:02,260 --> 00:00:05,120 smooth and round and peaceful. 3 00:00:05,560 --> 00:00:11,040 Except when it suddenly vomits radiation and plasma in random directions. 4 00:00:11,540 --> 00:00:15,580 These solar flares and coronal mass ejections, or CMEs, 5 00:00:15,580 --> 00:00:19,340 can hit Earth and have serious consequences for humanity. 6 00:00:19,860 --> 00:00:21,540 How exactly do they work? 7 00:00:21,540 --> 00:00:23,140 How bad could they be? 8 00:00:23,140 --> 00:00:25,020 And can we prepare for them? 9 00:00:25,620 --> 00:00:31,500 [Intro music] 10 00:00:33,520 --> 00:00:37,880 While the Sun seems pretty solid, it's actually like a very hot ocean. 11 00:00:38,120 --> 00:00:44,380 So hot that it rips atoms into electrons and nuclei, all flowing around each other in a plasma. 12 00:00:44,740 --> 00:00:49,100 This plasma is pushed around and shaped by the Sun's magnetic field. 13 00:00:49,300 --> 00:00:54,520 Similar to how the Sun's gravitational field reaches out to the planets and shapes their orbits. 14 00:00:54,800 --> 00:00:57,760 But magnetism is very different from gravity. 15 00:00:58,000 --> 00:01:01,960 Magnetism is one part of a dual force: Electromagnetism. 16 00:01:02,460 --> 00:01:07,940 Electricity creates magnetic fields, and magnetic fields create electricity. 17 00:01:08,120 --> 00:01:12,240 On the Sun, the plasma—made of electrically charged protons and electrons— 18 00:01:12,240 --> 00:01:14,700 creates a magnetic field as they move, 19 00:01:14,700 --> 00:01:17,980 and this magnetic field then shapes the flow of particles. 20 00:01:18,460 --> 00:01:22,180 They're stuck in a dynamic feedback loop called a dynamo, 21 00:01:22,180 --> 00:01:24,620 which keeps the sun's magnetic field alive. 22 00:01:25,240 --> 00:01:28,960 This magnetic field stores enormous amounts of energy 23 00:01:28,960 --> 00:01:31,120 and leaks out over the Solar System. 24 00:01:31,520 --> 00:01:36,820 It carries with it a constant trickle of solar plasma, like a light rain, known as the solar wind, 25 00:01:36,820 --> 00:01:38,720 creating a sort of space weather. 26 00:01:39,600 --> 00:01:41,660 But it isn't always calm and smooth. 27 00:01:41,800 --> 00:01:44,900 As the sun's plasma churns and flows around itself, 28 00:01:44,900 --> 00:01:47,860 its magnetic field gets all kinked and twisted. 29 00:01:48,080 --> 00:01:52,100 This creates magnetic knots that build up enormous amounts of energy. 30 00:01:52,500 --> 00:01:56,600 When the magnetic knots break—like a tangle of springs exploding outwards— 31 00:01:56,600 --> 00:02:00,720 the Sun can vomit plasma and other awful things into the Solar System. 32 00:02:01,300 --> 00:02:03,920 These solar storms come in many types, 33 00:02:03,920 --> 00:02:07,540 like solar flares; a tidal wave of high-energy radiation. 34 00:02:08,080 --> 00:02:12,840 They race through the solar system at the speed of light, sweeping up protons in the solar wind, 35 00:02:12,840 --> 00:02:16,520 accelerating them into a high-speed solar-proton storm. 36 00:02:17,320 --> 00:02:19,660 Then, there are coronal mass ejections, 37 00:02:19,660 --> 00:02:23,940 which rip millions or billions of tons of plasma from the Sun's atmosphere, 38 00:02:23,940 --> 00:02:29,120 catapulting it through the solar system at speeds of up to 9 million km/h. 39 00:02:29,880 --> 00:02:33,300 When these monsters hit us, nothing happens on Earth. 40 00:02:33,660 --> 00:02:36,420 While even smaller storms can damage satellites, 41 00:02:36,420 --> 00:02:38,020 affect radio communication, 42 00:02:38,020 --> 00:02:39,740 or be dangerous to astronauts, 43 00:02:39,740 --> 00:02:42,540 for people on the surface, space weather is harmless. 44 00:02:43,000 --> 00:02:46,660 Earth's atmosphere protects us from the worst effects of a solar flare 45 00:02:46,660 --> 00:02:49,880 by absorbing the blast of X-rays high up in the atmosphere, 46 00:02:49,880 --> 00:02:51,920 well before it reaches the surface. 47 00:02:52,440 --> 00:02:57,200 The electrified plasma from a CME is deflected by the Earth's magnetic field, 48 00:02:57,200 --> 00:03:00,340 diverting the energy storm to the North and South Poles, 49 00:03:00,340 --> 00:03:02,940 where energetic particles fall into the atmosphere, 50 00:03:02,940 --> 00:03:07,100 causing the atmosphere to glow and creating beautiful auroras. 51 00:03:07,860 --> 00:03:11,400 As with any sort of weather— most of the time, things are fine. 52 00:03:11,920 --> 00:03:14,340 Sometimes, there are hurricanes, though. 53 00:03:14,440 --> 00:03:17,580 Or in the case of the Sun, solar superstorms. 54 00:03:18,080 --> 00:03:21,320 And we know that they happen once or twice every century. 55 00:03:21,680 --> 00:03:25,740 If one were to happen today, we would first detect strong solar flares, 56 00:03:25,740 --> 00:03:28,840 a sort of flash before the much more dangerous thunder. 57 00:03:29,400 --> 00:03:34,640 The thunder is a CME, consisting of billions of tons of hot magnetic plasma 58 00:03:34,640 --> 00:03:38,800 that crosses the 150 million kilometers between the Sun and Earth 59 00:03:38,800 --> 00:03:40,040 in less than a day. 60 00:03:40,740 --> 00:03:46,140 When it arrives, it causes a shockwave that violently compresses the Earth's magnetic field 61 00:03:46,140 --> 00:03:48,720 and transfers energy into the magnetosphere. 62 00:03:49,060 --> 00:03:50,519 But it can get worse. 63 00:03:50,840 --> 00:03:54,800 If the magnetic field of the CME is aligned to Earth's in just the right way, 64 00:03:54,800 --> 00:03:56,800 the two magnetic fields merge. 65 00:03:57,220 --> 00:04:02,220 As the magnetic cloud passes over Earth, it stretches the Earth's field into a long tail. 66 00:04:02,740 --> 00:04:06,600 Eventually, the energy stored in the tail becomes too much to contain. 67 00:04:06,840 --> 00:04:10,760 It snaps and explosively releases its energy towards Earth. 68 00:04:11,120 --> 00:04:14,040 A geomagnetic storm has begun. 69 00:04:14,840 --> 00:04:17,720 A few hundred years ago, nobody would have cared. 70 00:04:17,940 --> 00:04:22,620 This storm gushing over the Earth is not relevant for machines made out of meat and bones. 71 00:04:22,900 --> 00:04:26,800 But it's very relevant for machines made out of metal and wire. 72 00:04:27,300 --> 00:04:28,640 Remember the dynamo? 73 00:04:28,820 --> 00:04:31,480 Magnetism creates electric currents. 74 00:04:31,540 --> 00:04:37,240 Earth in the 21st century is covered in millions of kilometers of wires, transporting electricity, 75 00:04:37,240 --> 00:04:41,480 and a complex grid of machines, like transformers, that make this transfer possible. 76 00:04:42,040 --> 00:04:47,360 A CME's energy can induce currents in our power grid that can either completely shut it down, 77 00:04:47,360 --> 00:04:51,640 or worse, destroy the transformer stations that keep our grid running. 78 00:04:52,080 --> 00:04:53,800 This has happened already, 79 00:04:53,800 --> 00:04:58,300 like when the Quebec power grid failed after a strong solar storm in 1989. 80 00:04:58,880 --> 00:05:02,360 But in general, our engineers know how to deal with these storms, 81 00:05:02,360 --> 00:05:04,580 and so we usually don't even notice. 82 00:05:05,100 --> 00:05:09,580 The last time a solar hurricane washed over Earth was in 1859: 83 00:05:09,760 --> 00:05:11,140 The Carrington Event, 84 00:05:11,140 --> 00:05:14,580 the largest geomagnetic storms ever observed on Earth. 85 00:05:15,160 --> 00:05:18,560 Massive auroras occurred as far south as the Caribbean. 86 00:05:19,140 --> 00:05:22,240 In some places, they were so bright that people got up, 87 00:05:22,240 --> 00:05:23,840 thinking the Sun was rising. 88 00:05:24,240 --> 00:05:27,440 Luckily, we only had one sort of modern technology: 89 00:05:27,440 --> 00:05:28,740 telegraph systems. 90 00:05:29,200 --> 00:05:31,080 They failed all over the world, 91 00:05:31,080 --> 00:05:33,880 shocking their operators and chucking out sparks. 92 00:05:34,400 --> 00:05:36,940 Today, we have a tad more technology, 93 00:05:36,940 --> 00:05:39,140 and our luck may run out soon. 94 00:05:39,420 --> 00:05:42,660 Another bad solar storm is bound to happen eventually. 95 00:05:43,200 --> 00:05:48,180 A storm as strong as the Carrington Event missed earth only by a small margin in 2012. 96 00:05:48,780 --> 00:05:53,500 Studies projected that it would've inflicted serious damage to electronic systems globally, 97 00:05:53,500 --> 00:05:57,540 costing up to $2.6 trillion to the US alone. 98 00:05:57,840 --> 00:06:03,180 The time to replace all the damaged systems was estimated at between 4 and 10 years. 99 00:06:03,400 --> 00:06:05,660 It's hard to say how bad it could have been. 100 00:06:05,900 --> 00:06:07,420 Experts disagreed. 101 00:06:07,480 --> 00:06:09,880 Some assumed there would just be temporary blackouts, 102 00:06:09,880 --> 00:06:12,080 but others worried it could be much worse. 103 00:06:12,280 --> 00:06:15,840 We won't know for sure until a big solar hurricane hits us. 104 00:06:16,200 --> 00:06:20,680 The probability of such an event is estimated to be 12% per decade. 105 00:06:20,840 --> 00:06:25,160 That's about a 50/50 chance of at least one in the next 50 years. 106 00:06:25,360 --> 00:06:28,300 And, there is more unsettling news. 107 00:06:28,500 --> 00:06:32,500 A 2019 paper found that even calm stars, like our Sun, 108 00:06:32,500 --> 00:06:35,860 can create superflares every few thousand years. 109 00:06:36,380 --> 00:06:39,680 Eruptions orders of magnitude stronger than the strongest storms 110 00:06:39,680 --> 00:06:41,680 we have observed in the Solar System. 111 00:06:42,060 --> 00:06:46,680 If such a storm hits us unprepared, the consequences could be catastrophic. 112 00:06:47,100 --> 00:06:50,600 It's hard to overstate how much we depend on electricity. 113 00:06:50,820 --> 00:06:52,580 It's not just the lights at home. 114 00:06:52,580 --> 00:06:54,100 It means no computers, 115 00:06:54,100 --> 00:06:55,400 no communication, 116 00:06:55,400 --> 00:06:56,720 no navigation. 117 00:06:56,860 --> 00:07:01,200 A sustained power outage might lead to a breakdown of the supply chain, 118 00:07:01,200 --> 00:07:03,020 water supply systems failing 119 00:07:03,020 --> 00:07:05,560 and hospital generators running dry, 120 00:07:05,880 --> 00:07:07,900 supermarkets not being refilled 121 00:07:07,900 --> 00:07:10,000 while food rots in the fields. 122 00:07:10,280 --> 00:07:14,500 The lack of power might make it extremely hard to reboot our broken power grid, 123 00:07:14,500 --> 00:07:18,920 taking years or decades to restart our starving civilization. 124 00:07:19,280 --> 00:07:21,280 Okay, time to panic? 125 00:07:21,580 --> 00:07:26,100 As much as daily newspapers might like for solar storms to send us back to the Stone Age, 126 00:07:26,100 --> 00:07:27,360 they probably won't. 127 00:07:27,640 --> 00:07:30,700 Fortunately, even though solar storms aren't preventable, 128 00:07:30,700 --> 00:07:33,440 virtually all of their nasty side effects are. 129 00:07:33,880 --> 00:07:39,340 Scientists observing the Sun have a few hours up to a few days to see a CME coming. 130 00:07:39,620 --> 00:07:42,920 And the engineers working the systems that keep the world running 131 00:07:42,920 --> 00:07:46,120 are well aware of the risks posed by solar storms. 132 00:07:46,640 --> 00:07:50,100 Transformers and substations can be taken offline— 133 00:07:50,100 --> 00:07:52,000 short preventative blackouts— 134 00:07:52,000 --> 00:07:54,420 or in other words, by unplugging stuff. 135 00:07:54,920 --> 00:07:58,300 Engineers can open up extra lines to dissipate the extra power. 136 00:07:58,420 --> 00:08:03,500 And with investment and upgrades cheap compared to those other natural disasters require, 137 00:08:03,500 --> 00:08:07,820 we could protect the world's electric grid against even the nastiest of storms. 138 00:08:08,040 --> 00:08:10,240 But we do need to prepare. 139 00:08:10,500 --> 00:08:13,040 While the risk is manageable, it is real. 140 00:08:13,540 --> 00:08:16,960 For while our Sun bathes us in warm and pleasant light, 141 00:08:16,960 --> 00:08:19,960 one day, it might send a monster our way 142 00:08:19,960 --> 00:08:21,820 that we better be ready for. 143 00:08:23,360 --> 00:08:26,000 This video was sponsored by...you! 144 00:08:26,480 --> 00:08:30,200 Kurzgesagt videos are only possible thanks to your direct support. 145 00:08:30,420 --> 00:08:34,600 For example, if you want to stare at our smooth and round Sun for a little longer, 146 00:08:34,600 --> 00:08:37,080 we've made two minimal infographic posters: 147 00:08:37,080 --> 00:08:40,580 one about the scale of the Sun, and one about the age of the universe. 148 00:08:40,700 --> 00:08:42,940 Both should make you feel sufficiently tiny 149 00:08:42,940 --> 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