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These are the user uploaded subtitles that are being translated: 1 00:00:01,934 --> 00:00:06,167 The sun, our nuclear powerhouse. 2 00:00:07,135 --> 00:00:16,231 Our star, its light powers our world...and us. 3 00:00:16,264 --> 00:00:19,632 Without light, we would not be alive. 4 00:00:20,698 --> 00:00:23,898 Starting deep inside the sun, 5 00:00:23,931 --> 00:00:26,131 We follow the brutal journey 6 00:00:26,163 --> 00:00:31,462 Of a single, tiny package of light -- A photon. 7 00:00:31,495 --> 00:00:34,663 The ride that any photon takes to get to my eyes 8 00:00:34,694 --> 00:00:37,294 When i look up at the sun is an amazing one. 9 00:00:37,328 --> 00:00:39,794 From its ancient birth in the sun's core 10 00:00:39,828 --> 00:00:41,861 To its escape from the surface. 11 00:00:44,327 --> 00:00:45,961 The light reaching me from the sun 12 00:00:45,993 --> 00:00:48,726 Was produced before there was even human civilization. 13 00:00:48,760 --> 00:00:50,028 It's an incredible idea. 14 00:00:51,992 --> 00:00:53,459 Join our photon 15 00:00:53,492 --> 00:00:56,559 On its incredible million-Year journey 16 00:00:56,593 --> 00:01:01,624 Through the most hostile environment in the solar system 17 00:01:01,659 --> 00:01:05,124 To bring light and life to earth. 18 00:01:20,953 --> 00:01:25,720 The universe, home to billions of galaxies... 19 00:01:27,786 --> 00:01:30,719 ...each made of billions of stars. 20 00:01:33,885 --> 00:01:38,251 And, in an unremarkable corner of our galaxy, the milky way, 21 00:01:38,284 --> 00:01:42,051 Lies the sun, our closest star... 22 00:01:43,950 --> 00:01:48,149 ...a dazzling sphere of intense light, 23 00:01:48,182 --> 00:01:49,883 Too bright for the naked eye. 24 00:01:51,849 --> 00:01:57,149 But strip away that glare, and the sun transforms 25 00:01:57,182 --> 00:01:59,147 Into a giant ball 26 00:01:59,182 --> 00:02:03,982 Of super heated gas dominating our cosmic stage. 27 00:02:07,613 --> 00:02:09,612 The sun is really the star of the show. 28 00:02:09,647 --> 00:02:13,179 The sun is the parent of the whole solar system. 29 00:02:13,212 --> 00:02:16,712 It provides its children, the planets, 30 00:02:16,745 --> 00:02:18,178 With everything they need. 31 00:02:18,212 --> 00:02:22,177 We depend on the sun for energy, for light, for warmth. 32 00:02:22,211 --> 00:02:24,810 We would not exist without the sun. 33 00:02:27,509 --> 00:02:30,275 The sun generates heat and light, 34 00:02:30,310 --> 00:02:32,942 The energy source for all life on earth. 35 00:02:32,975 --> 00:02:36,942 All of the energy that my body uses, 36 00:02:36,974 --> 00:02:39,275 Literally what i'm doing to talk to you right now, 37 00:02:39,307 --> 00:02:40,707 Came from the sun. 38 00:02:40,741 --> 00:02:43,741 The sun truly is the creator of all of the life around us. 39 00:02:45,407 --> 00:02:48,106 The sun is a constantly exploding 40 00:02:48,139 --> 00:02:51,506 Nuclear bomb, violent and essential. 41 00:02:53,938 --> 00:02:57,737 Our entire existence is powered by the energy 42 00:02:57,771 --> 00:02:59,770 Emitted in those nuclear reactions in the sun. 43 00:02:59,805 --> 00:03:02,870 We are here because of the light from the sun. 44 00:03:02,903 --> 00:03:05,037 We are here because of those nuclear reactions, 45 00:03:05,070 --> 00:03:07,703 And no aspect of our existence could persist 46 00:03:07,736 --> 00:03:08,969 If it wasn't there. 47 00:03:11,735 --> 00:03:14,501 Light is one of the basic building blocks 48 00:03:14,536 --> 00:03:15,569 Of the universe. 49 00:03:20,301 --> 00:03:22,900 I find light to be probably 50 00:03:22,932 --> 00:03:24,566 The most amazing thing in the universe. 51 00:03:24,599 --> 00:03:26,599 It's so important in everything. 52 00:03:26,633 --> 00:03:28,933 I mean, it's everything. It's everywhere. 53 00:03:28,966 --> 00:03:32,466 So, it's such a fundamental part of everything that exists. 54 00:03:32,498 --> 00:03:37,597 Fundamental and fast. 55 00:03:37,630 --> 00:03:39,830 The fastest thing in the cosmos... 56 00:03:41,796 --> 00:03:45,829 ...traveling at 186,000 miles per second. 57 00:03:47,962 --> 00:03:50,428 The sun is about 93 million miles away from us. 58 00:03:50,462 --> 00:03:52,594 So, going at 186,000 miles per second, 59 00:03:52,628 --> 00:03:53,728 That's about eight minutes. 60 00:03:53,761 --> 00:03:55,594 But those eight minutes 61 00:03:55,629 --> 00:03:59,262 Are just the brief last leg of its incredible journey. 62 00:04:04,194 --> 00:04:06,926 It may have taken the light as much as a million years 63 00:04:06,958 --> 00:04:09,326 To escape from the sun's raging interior... 64 00:04:12,992 --> 00:04:15,758 ...which means the light we're seeing right now 65 00:04:15,790 --> 00:04:17,992 Was created long before 66 00:04:18,023 --> 00:04:20,158 Our ancestors left the plains of africa. 67 00:04:23,557 --> 00:04:25,323 When i first learned this fact, 68 00:04:25,357 --> 00:04:27,356 I was already a practicing scientist. 69 00:04:27,389 --> 00:04:29,355 I had never really thought about that, 70 00:04:29,388 --> 00:04:31,922 And on first glance, it just blew me away. 71 00:04:31,954 --> 00:04:34,088 Right now the light reaching me from the sun 72 00:04:34,122 --> 00:04:37,021 Was produced before there was even human civilization. 73 00:04:37,054 --> 00:04:39,388 And yet, the minute it gets to the surface of the sun, 74 00:04:39,422 --> 00:04:42,521 It races away and is here eight minutes after that. 75 00:04:42,554 --> 00:04:45,687 It's an incredible idea. 76 00:04:45,720 --> 00:04:48,619 The ride that any photon takes to get to my eyes 77 00:04:48,653 --> 00:04:52,086 When i look up at the sun is an amazing one. 78 00:04:52,119 --> 00:04:55,419 That ride starts deep in the belly of our star. 79 00:04:56,817 --> 00:04:59,983 If we could open up the sun, 80 00:05:00,017 --> 00:05:03,650 We'd see layers of dense hydrogen gas 81 00:05:03,683 --> 00:05:07,248 Hundreds of thousands of miles deep. 82 00:05:07,283 --> 00:05:12,315 And at its center, the core, the sun gives birth to light... 83 00:05:16,947 --> 00:05:19,479 ...forged in one of the most violent reactions 84 00:05:19,512 --> 00:05:23,280 In the universe, nuclear fusion. 85 00:05:29,646 --> 00:05:32,812 The specific nuclear reaction that powers the sun is fusion, 86 00:05:32,846 --> 00:05:34,812 Fusion of hydrogen into helium. 87 00:05:34,845 --> 00:05:37,377 You take two hydrogen atoms, you ram them together, 88 00:05:37,410 --> 00:05:39,778 And what's left over is a helium atom. 89 00:05:39,810 --> 00:05:41,575 It sounds simple enough, 90 00:05:41,610 --> 00:05:43,877 But it's not. 91 00:05:43,910 --> 00:05:46,410 It's actually hard to get two atoms to fuse. 92 00:05:46,442 --> 00:05:48,175 Two photons have the same charge. 93 00:05:48,209 --> 00:05:50,909 They're both positively charged. They want to repel each other. 94 00:05:52,608 --> 00:05:54,973 Protons don't like to get close together. 95 00:05:55,007 --> 00:05:57,341 They have to come together with a huge amount 96 00:05:57,374 --> 00:05:59,640 Of energy or velocity 97 00:05:59,673 --> 00:06:01,673 To get close enough to begin to fuse, 98 00:06:01,706 --> 00:06:04,605 And that's very, very rare. 99 00:06:04,639 --> 00:06:06,805 To force protons together 100 00:06:06,838 --> 00:06:09,939 Takes immense amounts of heat and pressure... 101 00:06:11,937 --> 00:06:15,903 ...generated by the invisible hand of gravity. 102 00:06:15,937 --> 00:06:19,536 The sun contains 99.8% of all the matter 103 00:06:19,571 --> 00:06:21,037 In the solar system. 104 00:06:23,670 --> 00:06:25,968 That's a lot of mass. 105 00:06:26,002 --> 00:06:28,835 All that mass pulls the sun together 106 00:06:28,867 --> 00:06:31,868 With unimaginable gravitational force. 107 00:06:34,267 --> 00:06:36,333 With gravity crushing things down, 108 00:06:36,367 --> 00:06:38,734 Things get close enough together and nuclear fusion happens. 109 00:06:39,967 --> 00:06:43,233 In this nuclear compactor, 110 00:06:43,265 --> 00:06:44,898 Hydrogen atoms slam together 111 00:06:44,933 --> 00:06:49,466 100 million quadrillion quadrillion times each second. 112 00:06:53,698 --> 00:06:59,198 Some of these collisions are so powerful that atoms fuse, 113 00:06:59,230 --> 00:07:01,162 Releasing energy. 114 00:07:01,196 --> 00:07:04,996 When the protons come together to bind together, 115 00:07:05,030 --> 00:07:06,662 They lose a little bit of mass, 116 00:07:06,695 --> 00:07:08,995 And that mass gets converted into energy. 117 00:07:09,027 --> 00:07:11,660 And every second of every day, 118 00:07:11,695 --> 00:07:17,560 About five million tons of stuff is being converted to energy. 119 00:07:17,594 --> 00:07:19,227 It's amazing. 120 00:07:24,426 --> 00:07:28,092 Each collision creates a tiny burst of energy, 121 00:07:28,124 --> 00:07:34,057 A packet of light impossibly small and incredibly powerful. 122 00:07:36,790 --> 00:07:40,889 Somehow, our photon will deliver its energy to earth 123 00:07:40,924 --> 00:07:46,121 Where it will power the planet and make life possible. 124 00:07:46,155 --> 00:07:50,388 But right now it's nothing like the light we see. 125 00:07:50,422 --> 00:07:55,421 It has massive amounts of energy, and it's deadly. 126 00:08:06,951 --> 00:08:11,451 The light we see from our star is old... 127 00:08:11,484 --> 00:08:13,284 much older than the eight minutes it takes 128 00:08:13,316 --> 00:08:15,184 To get from the sun to earth. 129 00:08:17,615 --> 00:08:22,116 That short leap across space is the end of a long, hard journey 130 00:08:22,149 --> 00:08:24,449 That starts deep inside our sun. 131 00:08:24,482 --> 00:08:26,114 When we look at the sun, 132 00:08:26,149 --> 00:08:29,782 We say, "how beautiful, how elegant, and how simple." 133 00:08:29,814 --> 00:08:30,914 Light is formed in the sun, 134 00:08:30,947 --> 00:08:33,780 And it shines and lights up our world. 135 00:08:33,814 --> 00:08:35,247 Well, not so fast. 136 00:08:35,280 --> 00:08:37,146 It's actually very complex. 137 00:08:38,978 --> 00:08:40,112 The journey starts 138 00:08:40,146 --> 00:08:42,779 In the immense heat of the sun's core. 139 00:08:48,478 --> 00:08:52,143 Crushed together by the sun's enormous gravity, 140 00:08:52,176 --> 00:08:54,944 Atoms smash into each other and fuse... 141 00:08:56,476 --> 00:09:01,775 ...releasing a tiny packet of energy, photon of light... 142 00:09:03,742 --> 00:09:07,974 ...far smaller than an atom with no mass. 143 00:09:08,007 --> 00:09:10,874 Photons travel faster than anything else, 144 00:09:10,906 --> 00:09:15,607 And they never stop moving. 145 00:09:20,338 --> 00:09:24,039 Photons don't just come from the core of stars. 146 00:09:26,205 --> 00:09:27,538 So, where does light come from? 147 00:09:27,572 --> 00:09:30,405 The short answer is, matter makes it, 148 00:09:30,438 --> 00:09:32,271 And the amount of light that it creates 149 00:09:32,304 --> 00:09:33,571 Depends on its temperature. 150 00:09:34,803 --> 00:09:36,670 Every piece of matter in the universe 151 00:09:36,704 --> 00:09:39,170 Above absolute zero degrees 152 00:09:39,204 --> 00:09:42,003 Produces light, including humans. 153 00:09:43,701 --> 00:09:46,200 We humans are emitting light all the time 154 00:09:46,234 --> 00:09:49,633 Because we're alive, we're warm, we're not at a zero temperature. 155 00:09:49,667 --> 00:09:52,967 So, in fact we are emitting infrared radiation, 156 00:09:53,000 --> 00:09:54,999 Often called heat radiation. 157 00:09:55,032 --> 00:09:57,398 But all matter emits light. 158 00:09:57,431 --> 00:10:00,633 Even someone as cool as me, i'm creating light right now. 159 00:10:02,931 --> 00:10:04,464 The light we see 160 00:10:04,498 --> 00:10:06,797 Can be split into the colors of the rainbow. 161 00:10:06,830 --> 00:10:09,330 Each color is photons of light 162 00:10:09,364 --> 00:10:12,230 With slightly different amounts of energy. 163 00:10:15,196 --> 00:10:16,562 And what we can see 164 00:10:16,595 --> 00:10:18,864 Is only a fraction of the light spectrum. 165 00:10:21,027 --> 00:10:23,327 Our eyes are actually imperfect detectors. 166 00:10:23,360 --> 00:10:24,628 We know about visible light, 167 00:10:24,662 --> 00:10:26,927 The type of light that our eyes are sensitive to, 168 00:10:26,960 --> 00:10:28,693 But that's only a small range of energies. 169 00:10:28,728 --> 00:10:33,327 Light comes at higher and lower energies than we can detect. 170 00:10:33,359 --> 00:10:34,759 Using special cameras, 171 00:10:34,792 --> 00:10:38,393 We can see the infrared light that humans emit. 172 00:10:39,993 --> 00:10:41,825 This infrared light 173 00:10:41,859 --> 00:10:44,825 Has less energy than the visible light we see. 174 00:10:48,224 --> 00:10:52,924 Some light is too energetic to see, 175 00:10:52,956 --> 00:10:56,989 Like ultraviolets, x-Rays, and gamma rays. 176 00:11:01,689 --> 00:11:07,187 The vast, hot sun generates all forms of light. 177 00:11:07,221 --> 00:11:10,787 But in the nuclear furnace of the sun's core, 178 00:11:10,819 --> 00:11:14,718 Every photon starts out as a gamma ray, 179 00:11:14,752 --> 00:11:19,451 The most energetic form of light in the universe. 180 00:11:19,484 --> 00:11:20,619 And when a nuclear reaction happens, 181 00:11:20,652 --> 00:11:22,951 It emits an amazing amount of energy, 182 00:11:22,984 --> 00:11:25,651 The energy much, much bigger than visible light -- 183 00:11:25,684 --> 00:11:28,218 Gamma rays, we call them. 184 00:11:28,251 --> 00:11:30,617 Literally almost a million times 185 00:11:30,650 --> 00:11:35,449 Or at least 10,000 times the energy of the light we see. 186 00:11:35,782 --> 00:11:39,015 Gamma rays can transform and even kill. 187 00:11:39,149 --> 00:11:40,649 There's a reason why gamma rays 188 00:11:40,682 --> 00:11:42,481 Turned bruce banner into the hulk. 189 00:11:42,514 --> 00:11:45,147 Gamma rays are a very dangerous form of light. 190 00:11:45,179 --> 00:11:46,813 They can travel into your body 191 00:11:46,846 --> 00:11:48,414 And when they interact with the matter, 192 00:11:48,447 --> 00:11:51,278 They can break apart atoms. 193 00:11:51,312 --> 00:11:53,080 Fortunately for us, 194 00:11:53,113 --> 00:11:57,079 Our gamma-Ray photon can't head straight out of the sun. 195 00:12:04,110 --> 00:12:07,211 If the sun were not this hot ball of gas, 196 00:12:07,245 --> 00:12:09,076 Then upon being created, 197 00:12:09,110 --> 00:12:12,576 A photon would immediately escape from the sun 198 00:12:12,609 --> 00:12:14,043 And it would be a gamma-Ray photon, 199 00:12:14,076 --> 00:12:19,109 A very energetic photon, not very good for life on earth. 200 00:12:19,142 --> 00:12:21,709 After its birth as a gamma ray, 201 00:12:21,743 --> 00:12:25,075 Our photon starts to race out from the sun's core 202 00:12:25,107 --> 00:12:26,141 At the speed of light. 203 00:12:30,440 --> 00:12:34,474 But it encounters an obstacle course of epic proportions. 204 00:12:36,273 --> 00:12:38,639 A journey that should take seconds 205 00:12:38,672 --> 00:12:40,904 Slows to a cosmic crawl. 206 00:12:42,403 --> 00:12:46,571 It takes on average about 100,000 years 207 00:12:46,604 --> 00:12:49,737 For a photon to make it from the middle of the sun, 208 00:12:49,770 --> 00:12:52,471 Where it was created, to the outermost edge, 209 00:12:52,504 --> 00:12:55,802 Where it gets emitted into space -- 100,000 years. 210 00:12:55,836 --> 00:12:58,768 If it had traveled in a straight line unimpeded, 211 00:12:58,801 --> 00:13:00,968 It would have taken two seconds. 212 00:13:01,001 --> 00:13:04,334 What could possibly slow a photon 213 00:13:04,368 --> 00:13:08,001 Moving at the speed of light? 214 00:13:08,033 --> 00:13:16,533 Something slams on the brakes -- Huge, hot, dense. 215 00:13:16,566 --> 00:13:21,465 So powerful, it doesn't just slow light, 216 00:13:21,498 --> 00:13:23,165 It transforms it. 217 00:13:34,994 --> 00:13:36,863 In the sun's core, 218 00:13:36,896 --> 00:13:41,428 Nuclear fusion releases a tiny bundle of energy... 219 00:13:43,594 --> 00:13:45,660 ...a photon of light. 220 00:13:46,560 --> 00:13:51,426 It races outwards at 186,000 miles per second. 221 00:13:54,825 --> 00:13:57,526 At that speed, it should take two seconds 222 00:13:57,557 --> 00:14:00,591 To travel through the sun's interior to the surface. 223 00:14:04,724 --> 00:14:09,689 But something turns seconds into an eternity. 224 00:14:09,723 --> 00:14:11,090 The sun is so dense 225 00:14:11,123 --> 00:14:13,689 That to get through all of the different layers of gas, 226 00:14:13,723 --> 00:14:16,189 This poor little piece of light takes hundreds of thousands, 227 00:14:16,221 --> 00:14:18,254 If not a million years, to get to the surface. 228 00:14:20,888 --> 00:14:22,687 So, when you're looking at the sun, 229 00:14:22,720 --> 00:14:23,921 You're looking at the light 230 00:14:23,953 --> 00:14:27,252 Emitted from reactions a million years ago. 231 00:14:27,285 --> 00:14:28,752 Our newborn photon 232 00:14:28,787 --> 00:14:30,586 Leaves the core at the speed of light 233 00:14:30,620 --> 00:14:33,885 Only to run smack into a dense soup 234 00:14:33,918 --> 00:14:37,918 Of hydrogen atoms, a photon's nightmare, 235 00:14:37,951 --> 00:14:42,984 That stretches for over 400,000 miles. 236 00:14:43,018 --> 00:14:45,350 If you're a photon born in the center of the sun, 237 00:14:45,383 --> 00:14:47,550 You have a heck of a journey ahead of you. 238 00:14:47,582 --> 00:14:48,916 It's actually pretty hard 239 00:14:48,950 --> 00:14:51,749 For light generated in the core of the sun to get out 240 00:14:51,782 --> 00:14:54,083 Because there's a lot of sun in the way, 241 00:14:54,115 --> 00:14:55,581 And it's extremely dense. 242 00:14:55,615 --> 00:14:59,914 The radiation zone surrounds the core of the sun. 243 00:15:02,913 --> 00:15:05,646 The zone is made of hydrogen gas, 244 00:15:05,679 --> 00:15:07,912 But not a gas as we think of it. 245 00:15:10,379 --> 00:15:13,346 The sheer weight of all the material above 246 00:15:13,379 --> 00:15:18,711 Compresses the radiation zone until it's denser than lead 247 00:15:18,745 --> 00:15:21,077 And nearly impossible to pass through. 248 00:15:24,876 --> 00:15:27,242 A photon produced in the center of the sun 249 00:15:27,275 --> 00:15:29,142 Knows where it wants to go. 250 00:15:29,175 --> 00:15:32,009 It wants to go to the edge where it's cool, 251 00:15:32,043 --> 00:15:33,875 And it wants to get out. 252 00:15:33,909 --> 00:15:36,842 But it's got 400,000 miles 253 00:15:36,875 --> 00:15:39,775 Of all these opaque gases blocking its way. 254 00:15:39,808 --> 00:15:45,206 These gases aren't just dense -- They're hot, 255 00:15:45,240 --> 00:15:50,639 Superheated to over 12 1/2 million degrees fahrenheit. 256 00:15:50,672 --> 00:15:52,606 The gas in the radiation zone 257 00:15:52,640 --> 00:15:56,739 Is transformed into what scientists call plasma. 258 00:15:59,669 --> 00:16:02,871 Plasma is the fourth state of matter. 259 00:16:02,904 --> 00:16:07,703 Atoms in normal matter have a nucleus with orbiting electrons. 260 00:16:07,836 --> 00:16:11,169 In plasma, the atoms have been torn apart 261 00:16:11,202 --> 00:16:15,035 And the electrons ripped away. 262 00:16:15,068 --> 00:16:19,067 Here on earth, we're familiar with the three main states 263 00:16:19,101 --> 00:16:21,168 Of matter that we're taught in school -- 264 00:16:21,201 --> 00:16:23,834 Solids, liquids, and gases. 265 00:16:23,866 --> 00:16:27,000 You know, we have the atmosphere as a gas, the oceans are water, 266 00:16:27,033 --> 00:16:29,533 The ground that i stand on is solid. 267 00:16:29,566 --> 00:16:31,433 But in fact, most of the universe, 268 00:16:31,466 --> 00:16:35,265 Including stars, consists of plasma. 269 00:16:37,831 --> 00:16:39,664 Compared to the rest of the universe, 270 00:16:39,698 --> 00:16:43,063 Earth is a calm place. 271 00:16:43,096 --> 00:16:44,396 Most of the time, 272 00:16:44,429 --> 00:16:47,663 It's not hot or violent enough here to create plasma. 273 00:16:49,928 --> 00:16:54,694 The best place to witness the power of plasma on earth 274 00:16:54,728 --> 00:16:56,395 Is inside a lightning strike. 275 00:16:59,427 --> 00:17:05,658 Temperatures inside a bolt can reach 53,000 degrees fahrenheit, 276 00:17:05,693 --> 00:17:08,725 Enough to momentarily rip a few atoms apart. 277 00:17:10,759 --> 00:17:13,258 The plasma lasts an instant. 278 00:17:13,291 --> 00:17:17,059 Then the electrons rebind and it's gone. 279 00:17:19,890 --> 00:17:22,355 But in our massive sun, 280 00:17:22,390 --> 00:17:25,290 The plasma lasts for billions of years 281 00:17:25,323 --> 00:17:26,489 And makes up 282 00:17:26,524 --> 00:17:30,089 The entire 200,000-Mile-Deep radiation zone. 283 00:17:32,588 --> 00:17:34,688 Worse for our photon, 284 00:17:34,720 --> 00:17:40,253 The plasma is electrically charged, forming a cosmic trap. 285 00:17:43,953 --> 00:17:46,418 And a plasma is opaque to radiation 286 00:17:46,452 --> 00:17:49,385 Because light interacts much more strongly 287 00:17:49,417 --> 00:17:51,083 With electronically charged objects 288 00:17:51,118 --> 00:17:52,783 Than with neutral objects. 289 00:17:52,818 --> 00:17:54,318 So, when you have a neutral atom, 290 00:17:54,350 --> 00:17:56,217 Light in general can pass by. 291 00:17:56,251 --> 00:17:57,817 But when you separated the charges 292 00:17:57,850 --> 00:17:59,284 And you have positive and negative charges 293 00:17:59,318 --> 00:18:03,384 Located everywhere, the light can't make it through. 294 00:18:03,417 --> 00:18:06,215 Our photon, in the form of a gamma ray, 295 00:18:06,248 --> 00:18:08,181 Has entered the radiation zone 296 00:18:08,215 --> 00:18:11,881 And smashed into a charged plasma particle. 297 00:18:11,915 --> 00:18:13,380 For a fraction of a second, 298 00:18:13,415 --> 00:18:18,347 The particle absorbs the photon, then spits it back out, 299 00:18:18,379 --> 00:18:22,113 And the photon collides with another particle. 300 00:18:25,244 --> 00:18:27,513 Every time it goes a little bit of a distance, 301 00:18:27,545 --> 00:18:29,245 It basically slams into an atom, 302 00:18:29,279 --> 00:18:32,545 Is absorbed and readmitted in some random direction. 303 00:18:32,579 --> 00:18:34,378 So, instead of just flying out, 304 00:18:34,410 --> 00:18:37,443 It's bouncing around countless, countless, countless times 305 00:18:37,476 --> 00:18:39,277 Until finally, it reaches the edge of the star. 306 00:18:40,776 --> 00:18:44,042 It's an atomic game of basketball 307 00:18:44,074 --> 00:18:47,975 With a court representing the radiation zone. 308 00:18:48,009 --> 00:18:51,942 The players stand in for the particles and the plasma 309 00:18:51,975 --> 00:18:53,774 And the ball is the photon. 310 00:18:55,406 --> 00:18:56,941 So, the basketball 311 00:18:56,973 --> 00:19:00,840 Is being thrown from one player to another seemingly randomly. 312 00:19:00,874 --> 00:19:04,173 It's not making a lot of progress down the court, 313 00:19:04,205 --> 00:19:07,173 But it is gradually making progress. 314 00:19:07,205 --> 00:19:09,438 Gradually over time, it is going 315 00:19:09,472 --> 00:19:12,538 From the hotter parts of the core outward 316 00:19:12,570 --> 00:19:14,503 Toward cooler temperatures. 317 00:19:14,537 --> 00:19:16,271 That's where it wants to get. 318 00:19:16,303 --> 00:19:18,204 It's a random-Looking process, 319 00:19:18,238 --> 00:19:22,736 But it's directed in a certain direction with time. 320 00:19:25,901 --> 00:19:28,468 The photon wants to go straight up the court -- 321 00:19:28,502 --> 00:19:31,435 Its quickest route -- 322 00:19:31,467 --> 00:19:34,033 But is bounced and thrown around the radiation zone, 323 00:19:34,068 --> 00:19:36,268 Slowing to a crawl. 324 00:19:38,899 --> 00:19:43,864 This bruising process transforms the photon. 325 00:19:43,898 --> 00:19:45,931 When a photon, a little packet of light, 326 00:19:45,965 --> 00:19:47,665 Is created in the center of the star, 327 00:19:47,697 --> 00:19:50,931 It's actually a gamma ray, super high energy bit of light. 328 00:19:50,965 --> 00:19:53,898 And it can't go very far because as soon as it does, 329 00:19:53,932 --> 00:19:56,365 Boom, it hits another atom and gets absorbed. 330 00:19:58,663 --> 00:19:59,797 Every time it does this, 331 00:19:59,830 --> 00:20:02,629 It loses a little bit of that energy. 332 00:20:04,628 --> 00:20:06,462 Over several hundred thousand years, 333 00:20:06,495 --> 00:20:10,794 Sometimes even a million, the photon keeps bouncing 334 00:20:10,829 --> 00:20:15,128 Through the dense radiation zone. 335 00:20:15,160 --> 00:20:20,059 Each collision saps a tiny bit of energy, 336 00:20:20,092 --> 00:20:23,560 Transforming it from a lethal gamma-Ray photon 337 00:20:23,592 --> 00:20:25,627 To a lower energy x-Ray. 338 00:20:27,825 --> 00:20:31,292 Nearly a million years after its creation in the core, 339 00:20:31,325 --> 00:20:35,789 The photon has made it through the radiation zone, 340 00:20:35,824 --> 00:20:38,690 But its quest to escape is not over yet. 341 00:20:40,655 --> 00:20:42,822 It's about to hitch a wild ride 342 00:20:42,856 --> 00:20:46,189 On the sun's ferocious internal roller coaster... 343 00:20:47,922 --> 00:20:51,621 ...a place so violent, it makes the sun roar. 344 00:21:10,850 --> 00:21:14,282 A photon, nature's energy-Delivery system, 345 00:21:14,317 --> 00:21:16,717 Has spent up to a million years 346 00:21:16,750 --> 00:21:18,715 In the maze of the sun's interior 347 00:21:18,748 --> 00:21:20,782 On its journey toward the earth. 348 00:21:23,015 --> 00:21:27,114 The photon has fought its way through 3/4 of the sun's radius. 349 00:21:29,647 --> 00:21:31,848 Battered and sapped of energy, 350 00:21:31,880 --> 00:21:35,281 It is morphed from a deadly gamma ray to an x-Ray. 351 00:21:37,980 --> 00:21:42,412 But now it enters the mysterious boiling layer of the sun, 352 00:21:42,444 --> 00:21:44,146 The convection zone. 353 00:21:48,310 --> 00:21:51,711 The convection zone lies between the radiation zone 354 00:21:51,744 --> 00:21:57,309 And the sun's surface and is 125,000 miles deep. 355 00:21:59,542 --> 00:22:03,408 We can't see the convection zone directly. 356 00:22:03,442 --> 00:22:08,406 This region of the sun is still opaque to our telescopes, 357 00:22:08,441 --> 00:22:10,475 But we can hear it. 358 00:22:14,573 --> 00:22:19,805 Nasa's solar dynamics observatory listens to the sun. 359 00:22:19,839 --> 00:22:23,771 The sound it picks up is too deep for humans to hear, 360 00:22:23,805 --> 00:22:27,338 But if you speed up 40 days' recording 361 00:22:27,370 --> 00:22:31,503 Into a few seconds, this is what you get. 362 00:22:35,236 --> 00:22:38,603 It's the sound of chaos. 363 00:22:41,567 --> 00:22:43,968 Since we can't see into the sun, 364 00:22:44,001 --> 00:22:46,769 Its sound is vital to scientists. 365 00:22:50,000 --> 00:22:55,165 When a gun fires, the bullet rushes out and smashes into air, 366 00:22:55,199 --> 00:22:57,767 Creating waves of turbulence. 367 00:23:00,897 --> 00:23:02,865 When we hear the gun firing, 368 00:23:02,898 --> 00:23:06,231 These waves vibrate our eardrums. 369 00:23:09,396 --> 00:23:11,931 What we see here is sound. 370 00:23:11,962 --> 00:23:16,696 The sun works the same way on a much larger scale. 371 00:23:18,996 --> 00:23:21,961 When we see these waves moving across, 372 00:23:21,995 --> 00:23:24,962 What we're looking at is when material moves up 373 00:23:24,995 --> 00:23:27,562 From inside the sun and it makes noise. 374 00:23:27,594 --> 00:23:29,026 It just, like, ran into a surface. 375 00:23:29,059 --> 00:23:32,259 It just ran into a wall, and it generates sound. 376 00:23:32,294 --> 00:23:35,826 And we see that sound moving all around the sun. 377 00:23:35,860 --> 00:23:38,659 Sound waves crashing through the plasma 378 00:23:38,691 --> 00:23:42,124 Create ripples in the sun's surface. 379 00:23:42,159 --> 00:23:44,425 And all we see are these ripples. 380 00:23:44,458 --> 00:23:47,325 Those are the actual sound waves of the sun, 381 00:23:47,357 --> 00:23:49,356 And they move around the entire sun. 382 00:23:49,390 --> 00:23:50,956 They move down inside the sun. 383 00:23:50,989 --> 00:23:52,923 They move back up to the surface. 384 00:23:52,956 --> 00:23:54,956 By tracking the sound, 385 00:23:54,990 --> 00:23:57,489 Scientists can see the invisible. 386 00:23:59,954 --> 00:24:01,521 They pick up sound waves 387 00:24:01,553 --> 00:24:04,021 Smashing against the sun's surface 388 00:24:04,055 --> 00:24:06,988 And resonating throughout the solar interior... 389 00:24:08,886 --> 00:24:12,587 ...revealing a violent, boiling convection zone. 390 00:24:16,786 --> 00:24:20,485 The sun can be said to be ringing. 391 00:24:20,518 --> 00:24:22,818 You have this hot gas rising. 392 00:24:22,851 --> 00:24:24,716 You have cool gas falling. 393 00:24:24,750 --> 00:24:26,517 You have all this turbulence. 394 00:24:26,550 --> 00:24:30,050 You have so much action going on that it causes the sun to ring. 395 00:24:30,082 --> 00:24:34,182 Columns of gases rise and fall, 396 00:24:34,215 --> 00:24:39,281 Churned by heat from below. 397 00:24:39,315 --> 00:24:40,948 If you look at water boiling, 398 00:24:40,981 --> 00:24:44,881 Bubbles of gas or water are rising up because they're hot. 399 00:24:44,915 --> 00:24:47,047 And then they cool off, and then they sink back down. 400 00:24:47,079 --> 00:24:49,512 And if you look at a pot of boiling water, 401 00:24:49,546 --> 00:24:52,547 That's the same phenomena that's going on the sun, 402 00:24:52,579 --> 00:24:55,878 But with hot plasma instead of water. 403 00:24:55,913 --> 00:24:58,245 At the bottom of the convection zone, 404 00:24:58,279 --> 00:25:01,612 Photons smash into atoms in the plasma, 405 00:25:01,645 --> 00:25:03,212 Heating them to a boil. 406 00:25:04,244 --> 00:25:07,644 But this time, the photons are absorbed by the atoms. 407 00:25:09,510 --> 00:25:12,609 The hot atoms ride the boiling current to the top, 408 00:25:12,641 --> 00:25:15,142 Dragging the photons with them. 409 00:25:18,242 --> 00:25:21,207 So, it's almost like this conveyor belt of material. 410 00:25:21,241 --> 00:25:24,141 Photons are actually hitchhiking a ride on the atoms 411 00:25:24,174 --> 00:25:27,574 That are traveling upward through this heat transfer. 412 00:25:27,607 --> 00:25:29,906 So, it's a much easier ride in the convection layer 413 00:25:29,939 --> 00:25:31,639 Than it is in the radiation zone. 414 00:25:36,473 --> 00:25:39,338 It's as if our photon were now in the hands 415 00:25:39,371 --> 00:25:42,404 Of a single player making a fast break. 416 00:25:44,704 --> 00:25:48,735 In the convection layer, it's a direct path. 417 00:25:48,770 --> 00:25:52,235 One player can actually hold on to this basketball or photon 418 00:25:52,269 --> 00:25:54,636 For a lot longer in a direct path. 419 00:25:56,901 --> 00:25:58,134 By not passing, 420 00:25:58,167 --> 00:26:01,135 The atom takes the ball quickly up the court. 421 00:26:04,167 --> 00:26:06,766 The photon's journey through the convection zone 422 00:26:06,801 --> 00:26:09,699 Takes just one week. 423 00:26:09,733 --> 00:26:13,565 But in that time, the photon is transformed. 424 00:26:13,599 --> 00:26:16,165 The bottom of the convection zone 425 00:26:16,197 --> 00:26:20,065 Is around 360,000 degrees fahrenheit. 426 00:26:20,996 --> 00:26:23,264 The top -- Just 10,000. 427 00:26:26,630 --> 00:26:31,529 So, as the photon rises up, it cools, losing energy, 428 00:26:31,562 --> 00:26:35,262 Changing from an energetic x-Ray to visible light. 429 00:26:39,626 --> 00:26:42,161 So, it starts as a high-Energy x-Ray 430 00:26:42,194 --> 00:26:44,792 At the bottom of the convection zone, moves its way up, 431 00:26:44,827 --> 00:26:46,827 It loses a little bit of that energy. 432 00:26:46,859 --> 00:26:48,225 By the time it leaves there, 433 00:26:48,259 --> 00:26:50,527 It's closer to the kind of light that we see, 434 00:26:50,559 --> 00:26:51,826 Which is visible light. 435 00:26:55,492 --> 00:26:57,524 At the top of the convection zone, 436 00:26:57,558 --> 00:26:59,825 The atom releases the photon, 437 00:26:59,857 --> 00:27:02,823 Which shoots out as visible light. 438 00:27:04,490 --> 00:27:05,990 This cools the atoms, 439 00:27:06,023 --> 00:27:09,223 Which fall back down to absorb more photons, 440 00:27:09,257 --> 00:27:11,190 Heat up, and rise again. 441 00:27:12,889 --> 00:27:16,289 The photon is now just below the sun's surface. 442 00:27:18,854 --> 00:27:24,252 But the churning convection zone unleashes another force -- 443 00:27:24,285 --> 00:27:27,152 A force that powers huge storms, 444 00:27:27,187 --> 00:27:31,386 Detonates bombs, and threatens to stop light's escape. 445 00:27:48,916 --> 00:27:51,649 In the sun's core, 446 00:27:51,682 --> 00:27:54,414 Nuclear fusion has created a photon, a packet of light. 447 00:27:54,848 --> 00:27:58,780 It has battled through the radiation zone, 448 00:27:58,815 --> 00:28:01,581 Been dragged up through the convection zone 449 00:28:01,614 --> 00:28:06,614 On columns of hot plasma, hurdling towards its escape. 450 00:28:09,546 --> 00:28:11,712 On this million-Year journey, 451 00:28:11,744 --> 00:28:16,411 The photon has changed from an invisible deadly gamma ray 452 00:28:16,444 --> 00:28:19,811 To the kind of life-Giving light we see here on earth. 453 00:28:24,942 --> 00:28:29,241 Finally, it has reached the surface -- 454 00:28:29,276 --> 00:28:32,975 The visible shell of the sun, the photosphere. 455 00:28:35,773 --> 00:28:36,974 The photosphere, 456 00:28:37,008 --> 00:28:38,575 Which is basically the visible part of the sun, 457 00:28:38,607 --> 00:28:42,140 Or the surface, is what we see when we look up at the sun. 458 00:28:42,174 --> 00:28:45,240 We're seeing visible light coming from that very layer, 459 00:28:45,273 --> 00:28:46,339 The photosphere. 460 00:28:49,472 --> 00:28:52,904 The ball of blinding light we perceive 461 00:28:52,938 --> 00:28:57,472 Hides a spectacular and savage world. 462 00:28:59,971 --> 00:29:03,537 The sun from a distance looks quiet and serene, 463 00:29:03,569 --> 00:29:06,636 But if you take a close-Up of the surface of the sun, 464 00:29:06,668 --> 00:29:09,602 You see that it's churning with activity. 465 00:29:11,402 --> 00:29:14,869 It's beautiful and terrifying at the same time -- 466 00:29:14,902 --> 00:29:18,034 Huge storms of material bubbling and boiling. 467 00:29:18,067 --> 00:29:19,534 It looks like a witch's brew, 468 00:29:19,568 --> 00:29:21,567 Except the bubbles in the witch's brew 469 00:29:21,600 --> 00:29:23,632 Are larger than the size of the earth. 470 00:29:25,567 --> 00:29:28,933 The surface of the sun is a turbulent barrier. 471 00:29:30,799 --> 00:29:34,764 And once again, our photon gets taken hostage. 472 00:29:44,996 --> 00:29:48,561 At kitt peak observatory in arizona, 473 00:29:48,594 --> 00:29:53,060 Solar astronomer matt penn studies this solar surface 474 00:29:53,093 --> 00:29:57,093 To discover how photons of light get trapped. 475 00:29:57,127 --> 00:29:58,860 There's a bunch of cirrus today, 476 00:29:58,894 --> 00:30:00,694 But hopefully, we'll get some data. 477 00:30:04,627 --> 00:30:06,592 Using the mcmath-Pierce telescope, 478 00:30:06,626 --> 00:30:10,759 He focuses the sun's light to scan the photosphere in detail. 479 00:30:11,991 --> 00:30:14,491 So, what we've got are a few small sun spots 480 00:30:14,525 --> 00:30:15,824 On a disc of the sun. 481 00:30:15,857 --> 00:30:19,255 We've got two sun spots, two large ones. 482 00:30:19,289 --> 00:30:20,822 They're heading off to the edge of the sun, 483 00:30:20,855 --> 00:30:22,289 To the limb of the sun. 484 00:30:22,323 --> 00:30:24,723 But they're all accompanied by a smaller sun spots, 485 00:30:24,756 --> 00:30:26,390 Groups of smaller ones, following them. 486 00:30:29,189 --> 00:30:32,721 Sun spots mark areas where light is trapped. 487 00:30:34,886 --> 00:30:36,986 So, a sun spot forms a dark spot 488 00:30:37,020 --> 00:30:39,421 By removing energy from that part of the sun. 489 00:30:39,453 --> 00:30:42,052 It's blocking the convective flows that transport the heat 490 00:30:42,086 --> 00:30:44,519 And the light from inside the sun to space. 491 00:30:44,553 --> 00:30:46,320 So, what we see then is a cooler region 492 00:30:46,353 --> 00:30:47,786 That appears dark to us. 493 00:30:50,385 --> 00:30:54,750 A powerful force stops our photon dead in its tracks, 494 00:30:54,784 --> 00:30:58,651 Preventing its light and energy from leaving the sun's surface. 495 00:31:00,983 --> 00:31:03,384 That force is magnetism. 496 00:31:07,615 --> 00:31:10,814 Sun spots take shape where intense magnetism 497 00:31:10,849 --> 00:31:15,548 From deep inside the sun blasts up through the photosphere. 498 00:31:19,514 --> 00:31:22,647 The magnetic fields are so strong that it actually 499 00:31:22,679 --> 00:31:27,411 Stops the convective motion of hot inner material 500 00:31:27,445 --> 00:31:28,678 From flowing to the surface. 501 00:31:28,711 --> 00:31:31,010 So, you actually get what looks like a cool spot 502 00:31:31,044 --> 00:31:32,111 On the surface of the sun. 503 00:31:32,943 --> 00:31:34,776 They can be huge, 504 00:31:34,809 --> 00:31:37,844 The largest over 10 times the size of earth. 505 00:31:44,642 --> 00:31:47,275 The magnetism that generates these sun spots 506 00:31:47,308 --> 00:31:50,541 Forms field lines covering the sun. 507 00:31:50,575 --> 00:31:53,440 On our solid earth, the whole planet 508 00:31:53,473 --> 00:31:59,207 Rotates together, including its magnetic field. 509 00:31:59,240 --> 00:32:02,605 But the sun is a big ball of gas, 510 00:32:02,640 --> 00:32:05,505 And the same rules don't apply. 511 00:32:05,538 --> 00:32:07,837 You see, there's nothing solid about the sun. 512 00:32:07,871 --> 00:32:09,038 It's a big ball of gas. 513 00:32:09,072 --> 00:32:10,872 It turns on its axis, 514 00:32:10,904 --> 00:32:13,537 But the equator rotates faster than the poles. 515 00:32:13,571 --> 00:32:14,937 The sun twists itself up, 516 00:32:14,970 --> 00:32:17,238 And the magnetic field twists with it. 517 00:32:18,903 --> 00:32:22,935 It rotates faster at the equator than at the poles, 518 00:32:22,969 --> 00:32:26,235 Twisting and tangling its magnetic field 519 00:32:26,269 --> 00:32:27,902 With each rotation. 520 00:32:29,201 --> 00:32:33,067 The result -- Magnetic mayhem. 521 00:32:36,866 --> 00:32:39,765 So, when these fields emerge from the surface of the sun, 522 00:32:39,798 --> 00:32:41,866 They have all this stored energy in them. 523 00:32:41,998 --> 00:32:43,932 They're, like, all twisted and knotted, 524 00:32:43,966 --> 00:32:45,998 Like rubber bands you just twist and knot 525 00:32:46,032 --> 00:32:47,332 With all this energy in it. 526 00:32:47,364 --> 00:32:48,931 If you ever twist and twist and twist a rubber band 527 00:32:48,965 --> 00:32:50,097 And pull it straight, 528 00:32:50,131 --> 00:32:52,532 You can tell, you can feel that tension in it. 529 00:32:54,796 --> 00:32:57,262 Where the magnetic lines twist, 530 00:32:57,296 --> 00:33:00,329 Flows of plasma containing our photon 531 00:33:00,363 --> 00:33:01,863 Can't reach the surface. 532 00:33:03,662 --> 00:33:05,961 So, what happens is you have these packets of gas 533 00:33:05,995 --> 00:33:08,661 Which reach the surface, cool off, 534 00:33:08,694 --> 00:33:11,061 But are trapped right there by the magnetism. 535 00:33:13,994 --> 00:33:15,993 A patch of the sun goes dark 536 00:33:16,026 --> 00:33:18,759 Where light can't escape. 537 00:33:18,794 --> 00:33:20,794 A sun spot is born. 538 00:33:22,393 --> 00:33:24,926 But in that tangle of magnetic lines, 539 00:33:24,960 --> 00:33:26,691 Something eventually has to snap. 540 00:33:26,925 --> 00:33:29,990 The magnetic fields are very unhappy. 541 00:33:30,023 --> 00:33:31,656 They don't like the state that they're in, 542 00:33:31,689 --> 00:33:33,890 And all they want to do is unravel. 543 00:33:38,356 --> 00:33:40,655 Huge loops of magnetic energy 544 00:33:40,689 --> 00:33:43,056 Arch out over the sun spots. 545 00:33:46,023 --> 00:33:50,421 Twisted and unstable, desperate to spew their energy, 546 00:33:50,454 --> 00:33:54,820 They create a magnetic bomb primed to explode. 547 00:33:56,919 --> 00:33:58,852 And so, if one magnetic field with stored energy 548 00:33:58,886 --> 00:34:02,451 Sees another magnetic field, those two look at each other 549 00:34:02,486 --> 00:34:05,786 And say, "hey, if we connect, we can get rid of a lot of energy." 550 00:34:05,819 --> 00:34:07,151 They do so, they reconnect. 551 00:34:07,183 --> 00:34:08,618 Baddow! 552 00:34:18,082 --> 00:34:21,115 It's a huge explosion, and we call it a solar flare. 553 00:34:23,515 --> 00:34:27,147 And this can be equivalent to millions of nuclear weapons 554 00:34:27,181 --> 00:34:29,915 Exploding simultaneously. 555 00:34:31,213 --> 00:34:35,945 Solar flares erupt outwards into space 556 00:34:35,980 --> 00:34:38,579 At up to 4 1/2 million miles an hour... 557 00:34:40,646 --> 00:34:43,079 ...releasing massive amounts of energy. 558 00:34:47,411 --> 00:34:49,311 Magnetic fields are throwing plasma 559 00:34:49,344 --> 00:34:51,443 From the surface of the sun. 560 00:34:51,476 --> 00:34:54,010 Suddenly, there's a large outpouring of light. 561 00:34:57,710 --> 00:34:59,442 After nearly a million years, 562 00:34:59,476 --> 00:35:02,675 Our packet of light finally makes its escape. 563 00:35:06,907 --> 00:35:08,174 It's free, 564 00:35:08,206 --> 00:35:12,940 Catapulting out along with trillions of other photons, 565 00:35:12,974 --> 00:35:15,574 But their journey is far from over. 566 00:35:17,206 --> 00:35:22,072 Most hurdle onwards to the far reaches of the cosmos, 567 00:35:22,105 --> 00:35:24,771 To strange, new worlds. 568 00:35:34,401 --> 00:35:38,368 After a nearly million-Year journey 569 00:35:38,401 --> 00:35:42,968 Through the most hostile environment in the solar system, 570 00:35:43,001 --> 00:35:45,801 Tiny parcels of light -- 571 00:35:45,834 --> 00:35:49,667 Photons -- Finally burst from the sun's surface. 572 00:35:56,464 --> 00:35:57,999 They're free. 573 00:35:58,033 --> 00:36:01,931 They basically are free to leave this arduous journey 574 00:36:01,964 --> 00:36:03,464 That they've been on in the sun. 575 00:36:03,497 --> 00:36:05,830 And then they fly out at the speed of light. 576 00:36:07,997 --> 00:36:11,763 So, it's kind of a "breaking out of prison" type of feeling 577 00:36:11,796 --> 00:36:13,595 For those poor photons. 578 00:36:14,996 --> 00:36:17,961 They speed out into empty space 579 00:36:17,994 --> 00:36:21,028 At 186,000 miles per second. 580 00:36:22,960 --> 00:36:26,327 And just 8.3 minutes after it leaves the sun, 581 00:36:26,360 --> 00:36:28,592 Our photon reaches earth. 582 00:36:28,626 --> 00:36:30,858 The next time you look at a star in the sky, 583 00:36:30,893 --> 00:36:33,425 You might consider the amazing journey 584 00:36:33,458 --> 00:36:37,058 The photons have taken on their way to reaching your eye. 585 00:36:40,291 --> 00:36:42,525 They were created by nuclear reactions 586 00:36:42,557 --> 00:36:46,458 Deep in the core of the stars, and then they bounced around 587 00:36:46,490 --> 00:36:50,422 And got degraded into lower energy photons. 588 00:36:50,456 --> 00:36:52,523 And then in the convective zone, 589 00:36:52,556 --> 00:36:55,855 They were carried by mass motions of gas. 590 00:36:55,889 --> 00:36:59,122 And finally, at the edge, they were set free. 591 00:37:02,155 --> 00:37:07,121 And they traveled unimpeded and finally reached your eyes. 592 00:37:08,919 --> 00:37:12,252 Our photon finally arrives, 593 00:37:12,287 --> 00:37:16,752 Smashes into a leaf, and passes on its energy. 594 00:37:16,785 --> 00:37:18,885 This is photosynthesis, 595 00:37:18,919 --> 00:37:21,252 The fundamental link in our food chain. 596 00:37:25,151 --> 00:37:29,450 Finally, carrying energy born inside the sun's core, 597 00:37:29,482 --> 00:37:32,415 Our photon and billions like it 598 00:37:32,448 --> 00:37:36,914 Ignite the primal fires of life on our planet. 599 00:37:36,948 --> 00:37:42,247 The sun's light creates our fuel, drives our weather, 600 00:37:42,281 --> 00:37:43,680 Churns our seas. 601 00:37:46,913 --> 00:37:50,246 Every single day, enough photons hit the earth 602 00:37:50,279 --> 00:37:53,245 To power our civilization for 27 years. 603 00:37:55,346 --> 00:37:59,210 The sun's light is more than just warmth and heat. 604 00:37:59,243 --> 00:38:02,910 It provides everything we need to survive. 605 00:38:02,944 --> 00:38:06,476 Without light, we are nothing. 606 00:38:06,511 --> 00:38:09,543 All of the energy that powers our biology, 607 00:38:09,576 --> 00:38:12,243 The thing that makes our planet warm, that makes life possible, 608 00:38:12,275 --> 00:38:13,808 That all comes from the sun. 609 00:38:16,340 --> 00:38:20,241 Trillions of photons hit the earth every second, 610 00:38:20,273 --> 00:38:22,473 Each delivering life-Giving energy. 611 00:38:25,974 --> 00:38:30,039 But for the unimaginable number who pass us by, 612 00:38:30,072 --> 00:38:33,239 The journey is far from over. 613 00:38:33,273 --> 00:38:36,472 Around 80 minutes after leaving the sun, 614 00:38:36,505 --> 00:38:38,903 They reach saturn. 615 00:38:38,938 --> 00:38:41,371 After four hours, neptune. 616 00:38:43,771 --> 00:38:46,070 Once a photon leaves the surface of the sun, 617 00:38:46,103 --> 00:38:48,470 It's free to travel as far as it can, 618 00:38:48,503 --> 00:38:52,001 And as far as it can can be literally across the universe, 619 00:38:52,034 --> 00:38:54,301 Billions of light years away. 620 00:38:55,668 --> 00:38:57,468 They shoot past the outer reaches 621 00:38:57,501 --> 00:39:01,534 Of our solar system in just 18 hours. 622 00:39:01,567 --> 00:39:06,300 Here, the sun is a dim speck in the distance. 623 00:39:06,333 --> 00:39:10,865 But the photons keep on going, out into deep space. 624 00:39:13,931 --> 00:39:16,564 In 1,200 years, some of the photons 625 00:39:16,598 --> 00:39:21,065 Reach the red dwarf star system kepler-62, 626 00:39:21,096 --> 00:39:25,529 A solar system with potentially habitable earth-Like planets. 627 00:39:25,563 --> 00:39:28,330 In our galaxy, 628 00:39:28,362 --> 00:39:32,628 There are billions of earth-Like planets. 629 00:39:32,661 --> 00:39:37,994 If there is life out there, can it see the light from our sun? 630 00:39:38,029 --> 00:39:39,993 If aliens exist out there, 631 00:39:40,027 --> 00:39:42,560 They could easily see the light from our sun. 632 00:39:42,594 --> 00:39:44,525 If they're sufficiently nearby, 633 00:39:44,560 --> 00:39:48,058 The sun might be a naked-Eye star in their sky 634 00:39:48,092 --> 00:39:49,426 Or with telescopes, 635 00:39:49,458 --> 00:39:51,058 They would be able to detect the sun 636 00:39:51,092 --> 00:39:53,725 Even from vastly greater distances. 637 00:39:53,757 --> 00:39:55,725 So, there's a distinct possibility 638 00:39:55,757 --> 00:40:00,656 That aliens are studying our sun right now without realizing 639 00:40:00,690 --> 00:40:03,790 That we're here trying to study the universe, as well. 640 00:40:05,855 --> 00:40:07,322 Hurdling on, 641 00:40:07,355 --> 00:40:12,656 The photons pass the horsehead nebula in 1,500 years 642 00:40:12,688 --> 00:40:15,721 And the pillars of creation in 7,000. 643 00:40:17,822 --> 00:40:20,387 At these distances, the light from our star 644 00:40:20,420 --> 00:40:23,721 Is too small to be seen with the naked eye, 645 00:40:23,753 --> 00:40:26,219 But it would be visible with a powerful telescope. 646 00:40:26,253 --> 00:40:27,952 And with the biggest telescopes 647 00:40:27,985 --> 00:40:29,885 That we can create here on earth or in space, 648 00:40:29,918 --> 00:40:32,550 We can actually see the light from stars 649 00:40:32,585 --> 00:40:34,217 At the other end of the universe, 650 00:40:34,251 --> 00:40:36,184 Over 10 billion light years away. 651 00:40:36,217 --> 00:40:40,050 And so the light from our sun is traveling across the universe. 652 00:40:42,384 --> 00:40:43,682 So, the light from our sun, 653 00:40:43,715 --> 00:40:47,014 The light from the earth, travels essentially forever. 654 00:40:47,048 --> 00:40:49,481 The next time you're out under a clear sky 655 00:40:49,516 --> 00:40:50,749 And you look up, 656 00:40:50,782 --> 00:40:52,980 You might want to wave because somebody out there 657 00:40:53,014 --> 00:40:55,349 Might be able to see you and wave back. 658 00:40:57,648 --> 00:41:01,847 Our tiny star is visible across the universe 659 00:41:01,880 --> 00:41:04,380 If someone is looking. 660 00:41:04,413 --> 00:41:07,778 There isn't a single place in our visible universe 661 00:41:07,813 --> 00:41:09,813 That you wouldn't be able to see the sun from, 662 00:41:09,846 --> 00:41:11,445 And maybe that's heartening. 663 00:41:11,478 --> 00:41:13,510 Maybe there's some evidence of our existence 664 00:41:13,545 --> 00:41:14,677 At the other end of the universe. 665 00:41:14,711 --> 00:41:16,577 Won't get there for billions of years, 666 00:41:16,610 --> 00:41:19,277 But at least maybe we won't be forgotten. 667 00:41:19,311 --> 00:41:24,143 A journey that started deep inside the core of the sun 668 00:41:24,177 --> 00:41:27,309 With a photon, a million-Year struggle 669 00:41:27,342 --> 00:41:29,708 To finally escape the sun's grip. 670 00:41:32,442 --> 00:41:34,641 Once free, our photon 671 00:41:34,675 --> 00:41:39,307 Brought energy, heat, and life to our world. 672 00:41:41,574 --> 00:41:47,338 Light from our sun joins light from trillions of other stars 673 00:41:47,371 --> 00:41:49,806 Journeying through the universe, 674 00:41:49,838 --> 00:41:53,072 Spreading energy throughout the cosmos. 53664

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