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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:01,640 --> 00:00:06,280 Humans can survive in this universe as long as we have an energy source. 2 00:00:06,840 --> 00:00:13,000 Unfortunately, the universe will die. It will happen slowly, over many billions of years, 3 00:00:13,320 --> 00:00:18,760 but it will happen. On a universal time scale, stars like our sun will be gone in no time. 4 00:00:19,740 --> 00:00:24,080 Luckily, there are places that will exist practically forever from a human perspective: 5 00:00:25,120 --> 00:00:27,120 the corpses of dead stars... 6 00:00:27,480 --> 00:00:29,260 white dwarfs. 7 00:00:29,260 --> 00:00:34,100 They could be humanity's last home right before the death of the universe. 8 00:00:35,120 --> 00:00:39,180 What are these strange things and what happens when they finally die? 9 00:00:49,280 --> 00:00:51,880 How long stars live varies drastically, 10 00:00:52,140 --> 00:00:54,140 depending on how massive they are. 11 00:00:54,340 --> 00:01:01,940 For example, really massive stars burn hot and fast, dying violently in supernovae a few million years after birth. 12 00:01:02,760 --> 00:01:04,500 But they're the exception. 13 00:01:04,780 --> 00:01:08,880 97% of all stars will end their existence as white dwarfs. 14 00:01:09,620 --> 00:01:11,220 There are two ways this can happen: 15 00:01:11,980 --> 00:01:18,760 Small stars - so-called red dwarfs - burn out over trillions of years until they eventually quietly turn into white dwarfs. 16 00:01:20,140 --> 00:01:22,700 Medium-sized stars like our Sun are more interesting. 17 00:01:23,400 --> 00:01:29,520 Imagine the sun as a huge pressure cooker that fuses hydrogen into helium in its core through its gravity. 18 00:01:30,400 --> 00:01:33,420 The fusion of elements releases extreme amounts of energy, 19 00:01:33,620 --> 00:01:37,840 that pushes outwards and stabilizes the star, keeping it in a delicate balance. 20 00:01:38,660 --> 00:01:42,040 When the Sun is old, the hydrogen in the core is exhausted, 21 00:01:42,180 --> 00:01:45,140 and the Sun will begin to burn helium into heavier elements. 22 00:01:46,000 --> 00:01:48,560 While doing so, it will shed its outer layers. 23 00:01:49,480 --> 00:01:54,900 When this process is over more than half of the Sun's mass will be lost into space as a spectacular 24 00:01:55,080 --> 00:01:57,860 planetary nebula millions of kilometers across. 25 00:01:58,460 --> 00:02:00,740 What remains will be its former core: 26 00:02:01,640 --> 00:02:04,760 A white dwarf is born, a star corpse. 27 00:02:05,180 --> 00:02:08,880 While its former self was about 100 times its diameter, now 28 00:02:08,900 --> 00:02:13,360 it's only about as big as Earth, but still with about half of its former mass. 29 00:02:14,600 --> 00:02:20,720 This means it's extremely dense, a teaspoon of white dwarf is about as massive as a car. 30 00:02:21,640 --> 00:02:25,800 Its surface gravity is over 100,000 times higher than Earth's. 31 00:02:27,500 --> 00:02:31,820 If you tried to land on it, you'd immediately be compressed into a steaming puddle. 32 00:02:34,140 --> 00:02:37,600 Life around a white dwarf is very unlikely, but possible. 33 00:02:38,360 --> 00:02:44,860 Most of them that exist now were former stars that, well, died, which probably ruined any planets they once had. 34 00:02:45,300 --> 00:02:48,600 But that's not all: since they are so small, 35 00:02:48,600 --> 00:02:53,660 a planet would need to orbit them about 75 times closer than Earth is to the Sun to have liquid water. 36 00:02:55,020 --> 00:02:57,560 This proximity has up- and downsides: 37 00:02:57,600 --> 00:03:02,340 for one, it would tidally lock the planet giving it a permanent day and permanent night. 38 00:03:04,500 --> 00:03:07,860 At the edges of these day and night zones life could be possible. 39 00:03:08,860 --> 00:03:11,600 But white dwarfs have a very stable energy output, 40 00:03:11,600 --> 00:03:14,580 so they might actually be safer to live around than many red dwarfs. 41 00:03:15,100 --> 00:03:17,020 This is still speculation at this point, 42 00:03:17,020 --> 00:03:20,620 but if we could find the white dwarf with the right conditions to settle around, 43 00:03:20,740 --> 00:03:23,240 we could have a home for many billions of years. 44 00:03:24,540 --> 00:03:27,660 But why do they shine so much longer than other star types? 45 00:03:28,640 --> 00:03:32,980 White dwarfs are very, very hot - up to 40 times hotter than our Sun - 46 00:03:33,280 --> 00:03:35,580 ranking among the hottest objects in the universe. 47 00:03:36,020 --> 00:03:38,020 But they are not incredibly active. 48 00:03:38,360 --> 00:03:41,240 All the heat inside of them is trapped and has nowhere to go. 49 00:03:41,360 --> 00:03:44,100 Only on its outer layer can it escape into space. 50 00:03:44,620 --> 00:03:48,920 But space is mostly empty, so heat can't be transferred by conduction. 51 00:03:49,660 --> 00:03:52,540 The only way energy can escape is by radiation. 52 00:03:53,380 --> 00:03:57,920 This is so inefficient that white dwarfs will take trillions of years to cool down, 53 00:03:58,120 --> 00:04:01,040 which may make them humanity's last refuge. 54 00:04:01,660 --> 00:04:05,560 They might be the last sources of light and energy in a dying universe. 55 00:04:06,120 --> 00:04:11,680 According to some estimates white dwarfs might shine as long as 100 billion billion years, 56 00:04:11,880 --> 00:04:19,180 ten billion times longer than the universe has existed. So far into the future that no regular stars will shine any more, 57 00:04:20,100 --> 00:04:22,100 galaxies will have evaporated, and 58 00:04:22,380 --> 00:04:26,340 only then will the first white dwarf turn into the first black dwarf. 59 00:04:27,240 --> 00:04:30,500 When this happens the last hope for life will die off. 60 00:04:31,440 --> 00:04:34,960 Black dwarfs will be inactive spheres with no energy left to give, 61 00:04:35,880 --> 00:04:38,440 still massive enough to kill you if you get too close. 62 00:04:38,920 --> 00:04:43,540 So cold that they'll be near the coldest possible temperature in the universe, 63 00:04:43,560 --> 00:04:46,720 so dark that they are practically invisible. 64 00:04:47,900 --> 00:04:54,100 The universe will enter its last stage - heat death - which will leave the universe unrecognizable, 65 00:04:55,020 --> 00:04:58,100 an absolutely dark and cold graveyard, 66 00:04:58,340 --> 00:05:02,460 with black holes and black dwarfs scattered over trillions of lightyears. 67 00:05:03,380 --> 00:05:06,480 We don't know for sure what will happen with black dwarfs in the end. 68 00:05:06,840 --> 00:05:11,000 If the proton - one of the fundamental parts of atoms - has a limited lifespan, 69 00:05:11,180 --> 00:05:14,500 black dwarfs will slowly evaporate over many trillions of years. 70 00:05:14,920 --> 00:05:16,980 If the proton does not decay, 71 00:05:17,080 --> 00:05:22,160 black dwarfs will probably turn into spheres of pure ion via quantum tunneling, over a timespan 72 00:05:22,180 --> 00:05:26,520 so obscenely gigantic that calling it forever is okay. 73 00:05:27,160 --> 00:05:31,500 These ion spheres will then travel completely alone through a dark universe. 74 00:05:32,110 --> 00:05:34,199 Nothing new will happen anymore... 75 00:05:34,810 --> 00:05:36,039 forever. 76 00:05:36,039 --> 00:05:43,589 While this may sound kind of dark, this is so far away that for our purposes today, it might as well not happen at all. 77 00:05:43,720 --> 00:05:47,180 It doesn't matter what happens in a billion trillion years. 78 00:05:47,420 --> 00:05:50,980 Right now, we happen to exist at an excellent time, 79 00:05:50,980 --> 00:05:57,300 able to be in awe about a universe filled with endless stars and light and planets. 80 00:05:57,300 --> 00:06:00,090 And enough time to visit them one day. 81 00:06:02,900 --> 00:06:08,229 Our music is finally available on Spotify and iTunes. it's composed by our good friends at Epic Mountain, 82 00:06:08,479 --> 00:06:10,929 two guys with a studio who make music for a living. 83 00:06:11,449 --> 00:06:16,089 You can check them out here, and follow them on Facebook and Twitter. And if you like our videos, 84 00:06:16,090 --> 00:06:18,159 please consider supporting us on Patreon. 85 00:06:18,160 --> 00:06:21,260 It really would be extremely helpful. 86 00:06:21,260 --> 00:06:26,300 If you need an excuse to delay work a little bit longer, here's a playlist with more space videos.8539

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