All language subtitles for The Most Dangerous Stuff in the Universe - Strange Stars Explained

af Afrikaans
sq Albanian
am Amharic
ar Arabic
hy Armenian
az Azerbaijani
eu Basque
be Belarusian
bn Bengali
bs Bosnian
bg Bulgarian
ca Catalan
ceb Cebuano
ny Chichewa
zh-CN Chinese (Simplified)
zh-TW Chinese (Traditional)
co Corsican
hr Croatian
cs Czech
da Danish
nl Dutch
en English
eo Esperanto
et Estonian
tl Filipino
fi Finnish
fr French
fy Frisian
gl Galician
ka Georgian
de German
el Greek
gu Gujarati
ht Haitian Creole
ha Hausa
haw Hawaiian
iw Hebrew
hi Hindi
hmn Hmong
hu Hungarian Download
is Icelandic
ig Igbo
id Indonesian
ga Irish
it Italian
ja Japanese
jw Javanese
kn Kannada
kk Kazakh
km Khmer
ko Korean
ku Kurdish (Kurmanji)
ky Kyrgyz
lo Lao
la Latin
lv Latvian
lt Lithuanian
lb Luxembourgish
mk Macedonian
mg Malagasy
ms Malay
ml Malayalam
mt Maltese
mi Maori
mr Marathi
mn Mongolian
my Myanmar (Burmese)
ne Nepali
no Norwegian
ps Pashto
fa Persian
pl Polish
pt Portuguese
pa Punjabi
ro Romanian
ru Russian
sm Samoan
gd Scots Gaelic
sr Serbian
st Sesotho
sn Shona
sd Sindhi
si Sinhala
sk Slovak
sl Slovenian
so Somali
es Spanish
su Sundanese
sw Swahili
sv Swedish
tg Tajik
ta Tamil
te Telugu
th Thai
tr Turkish
uk Ukrainian
ur Urdu
uz Uzbek
vi Vietnamese
cy Welsh
xh Xhosa
yi Yiddish
yo Yoruba
zu Zulu
or Odia (Oriya)
rw Kinyarwanda
tk Turkmen
tt Tatar
ug Uyghur
Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:00,820 --> 00:00:04,660 Neutron stars are the densest things that are not black holes. 2 00:00:05,380 --> 00:00:09,780 In their cores, we might find the most dangerous substance in existence: 3 00:00:10,340 --> 00:00:11,840 Strange matter. 4 00:00:11,840 --> 00:00:14,320 A bizarre thing so extreme, 5 00:00:14,320 --> 00:00:16,420 that it bends the rules of the universe 6 00:00:16,420 --> 00:00:20,740 and could infect and destroy everything it comes into contact with-- 7 00:00:20,860 --> 00:00:24,100 --or it could teach us about how the universe began. 8 00:00:24,560 --> 00:00:25,840 Maybe both. 9 00:00:29,900 --> 00:00:34,000 [Intro music] 10 00:00:36,480 --> 00:00:41,420 To understand how extreme strange matter really is, we first need to get a few basics. 11 00:00:41,780 --> 00:00:46,780 What is a neutron star, and how does strange matter break the rules of the universe? 12 00:00:47,260 --> 00:00:51,460 To get all of this into one video, we'll grossly oversimplify a few things, 13 00:00:51,460 --> 00:00:54,760 but we'll provide you with further reading if you want more details. 14 00:00:55,260 --> 00:01:00,620 A neutron star is what remains after a very massive star explodes in a supernova. 15 00:01:01,080 --> 00:01:05,040 When this happens, the star's core collapses under its own gravity 16 00:01:05,040 --> 00:01:09,920 with such a strong inward force that it squeezes nuclei and particles together violently. 17 00:01:10,940 --> 00:01:15,260 Electrons are pushed into protons, so they merge and turn into neutrons. 18 00:01:15,820 --> 00:01:19,920 All the "nothing" inside of atoms is suddenly completely filled with particles 19 00:01:19,920 --> 00:01:23,300 that really don't want to be close to each other, but have no choice. 20 00:01:23,720 --> 00:01:27,500 They desperately push back against gravity, against the collapse. 21 00:01:27,720 --> 00:01:30,580 If gravity wins, they will become a black hole. 22 00:01:30,860 --> 00:01:33,480 If they win, they become a neutron star. 23 00:01:34,220 --> 00:01:38,900 This makes neutron stars like giant atomic nuclei the size of a city, 24 00:01:38,900 --> 00:01:40,800 but holding the mass of our Sun. 25 00:01:41,260 --> 00:01:43,500 And here, things get weird. 26 00:01:43,780 --> 00:01:49,700 The environment in the core of neutron stars is so extreme that the rules of nuclear physics change. 27 00:01:50,080 --> 00:01:54,500 And this could lead to a strange and extremely dangerous substance. 28 00:01:54,980 --> 00:01:57,140 But let's not get ahead of ourselves. 29 00:01:57,600 --> 00:02:01,160 We first need to know the rules before we learn how they can be broken. 30 00:02:02,020 --> 00:02:05,420 Protons and neutrons, the particles making up the nuclei of atoms, 31 00:02:05,420 --> 00:02:08,420 are made up of smaller particles called quarks. 32 00:02:09,020 --> 00:02:11,300 Quarks really don't want to be alone. 33 00:02:11,300 --> 00:02:13,300 They are what we call confined. 34 00:02:14,000 --> 00:02:15,660 You can try to separate them, 35 00:02:15,660 --> 00:02:19,520 but the harder you pull, the harder they try to pull themselves back together. 36 00:02:19,860 --> 00:02:24,380 If you use a lot of energy, they just use this energy to create new quarks. 37 00:02:24,740 --> 00:02:28,520 Quarks only exist together as the building blocks of other particles 38 00:02:28,520 --> 00:02:30,880 and have never been observed by themselves. 39 00:02:31,440 --> 00:02:35,340 They come in many types, but only two appear to make stable matter: 40 00:02:35,340 --> 00:02:39,320 the 'up' and 'down' quarks found in protons and neutrons. 41 00:02:39,620 --> 00:02:42,660 All other quarks seem to decay away quickly, 42 00:02:42,660 --> 00:02:44,120 but this may be different inside neutron stars. 43 00:02:44,120 --> 00:02:47,360 The forces operating in their cores are so extreme 44 00:02:49,700 --> 00:02:53,680 that they are actually similar to the universe shortly after the Big Bang. 45 00:02:54,500 --> 00:02:59,900 Neutron star cores are like fossils, which can let us peer back in time to the beginning of everything. 46 00:03:00,540 --> 00:03:03,760 So learning how quarks behave inside a neutron star 47 00:03:03,760 --> 00:03:07,740 is a way of understanding the very nature of the universe itself. 48 00:03:08,300 --> 00:03:14,240 One hypothesis is that, inside a neutron star core, protons and neutrons deconfine. 49 00:03:14,640 --> 00:03:20,260 All the particles crammed shoulder-to-shoulder dissolve and melt into a sort of bath of quarks. 50 00:03:20,960 --> 00:03:26,740 Uncountable numbers of particles become one giant thing made purely from quarks: 51 00:03:26,740 --> 00:03:27,740 Quark matter. 52 00:03:28,560 --> 00:03:31,300 A star made from this is called a Quark Star. 53 00:03:31,400 --> 00:03:35,380 Though from the outside, it may not look any different than a regular neutron star. 54 00:03:36,620 --> 00:03:39,980 Now, we can finally talk about the most dangerous substance. 55 00:03:40,120 --> 00:03:44,660 If the pressure inside a quark star is great enough, it may get stranger, 56 00:03:45,120 --> 00:03:46,000 literally. 57 00:03:47,060 --> 00:03:52,000 In the cores of neutron stars, some of the quarks may be converted into 'strange' quarks. 58 00:03:52,560 --> 00:03:55,340 Strange quarks have bizarre nuclear properties, 59 00:03:55,340 --> 00:03:59,500 and they are heavier, and for the lack of a better word, stronger. 60 00:03:59,760 --> 00:04:02,600 If they turn up, they could create strange matter. 61 00:04:03,140 --> 00:04:06,440 Strange matter might be the ideal state of matter, 62 00:04:06,440 --> 00:04:09,880 perfectly dense, perfectly stable, indestructible, 63 00:04:10,220 --> 00:04:13,260 more stable than any other matter in the universe. 64 00:04:13,460 --> 00:04:17,460 So stable that it can exist outside neutron stars. 65 00:04:18,000 --> 00:04:20,620 If this is the case, we have a problem. 66 00:04:20,780 --> 00:04:22,340 It might be infectious. 67 00:04:22,680 --> 00:04:26,700 Every piece of matter it touches might be so impressed by its stability 68 00:04:26,700 --> 00:04:29,560 that it would immediately turn into strange matter, too. 69 00:04:30,560 --> 00:04:34,740 Protons and neutrons would dissolve and become part of the quark bath, 70 00:04:34,740 --> 00:04:37,880 which frees energy and creates more strange matter. 71 00:04:38,840 --> 00:04:42,400 The only way to get rid of it would be to throw it into a black hole. 72 00:04:42,880 --> 00:04:44,920 But then again, who cares? 73 00:04:45,020 --> 00:04:47,120 All of it is inside neutron stars, 74 00:04:47,580 --> 00:04:52,200 except when neutron stars collide with other neutron stars or black holes. 75 00:04:52,200 --> 00:04:55,060 They spew out tremendous amounts of their insides, 76 00:04:55,060 --> 00:04:59,540 some of which could include little droplets of strange matter called strangelets. 77 00:05:00,160 --> 00:05:03,280 Strangelets are as dense as the core of a neutron star. 78 00:05:04,060 --> 00:05:07,200 They could be really small, maybe even subatomic, 79 00:05:07,200 --> 00:05:10,740 but even the largest strangelets wouldn't be any bigger than a rocket. 80 00:05:11,280 --> 00:05:15,280 These strangelets would drift through the galaxy for millions or billions of years 81 00:05:15,280 --> 00:05:18,000 until they meet a star or planet by chance. 82 00:05:18,580 --> 00:05:23,600 If one were to strike earth, it would immediately start converting it into strange matter. 83 00:05:23,920 --> 00:05:26,340 The more it converts, the more it would grow. 84 00:05:26,660 --> 00:05:30,160 Ultimately, all of the atoms making up earth would be converted. 85 00:05:30,700 --> 00:05:35,020 Earth would become a hot clump of strange matter, the size of an asteroid. 86 00:05:35,800 --> 00:05:40,220 If a strangelet strikes the sun, it would collapse into a strange star, 87 00:05:40,220 --> 00:05:42,800 eating through it like fire through a dry forest. 88 00:05:43,540 --> 00:05:45,960 This would not change the Sun's mass much, 89 00:05:45,960 --> 00:05:47,820 but it would become way less bright. 90 00:05:47,820 --> 00:05:49,520 So Earth would freeze to death. 91 00:05:50,040 --> 00:05:54,160 And like a tiny virus, we'd have no way to see a strangelet coming. 92 00:05:54,760 --> 00:05:59,100 Worse still, some theories suggest strangelets are more than common, 93 00:05:59,100 --> 00:06:01,460 outnumbering all stars in the galaxy. 94 00:06:02,240 --> 00:06:05,400 The strangelets could've formed very early after the Big Bang, 95 00:06:05,400 --> 00:06:08,820 when it was as hot and dense as a neutron star core everywhere. 96 00:06:09,580 --> 00:06:12,360 They might be clumping around the gravity of galaxies 97 00:06:12,360 --> 00:06:15,080 as the universe expanded and evolved. 98 00:06:15,680 --> 00:06:18,800 Strangelets could even be so numerous and massive, 99 00:06:18,800 --> 00:06:22,960 that they might actually be the dark matter we suspect holds galaxies together. 100 00:06:23,520 --> 00:06:25,380 But then again, maybe not. 101 00:06:25,920 --> 00:06:27,180 This is speculation. 102 00:06:27,280 --> 00:06:29,900 And the Earth and Sun and planets haven't been consumed 103 00:06:29,900 --> 00:06:32,980 in a wildfire of strangelets in the past few billion years. 104 00:06:32,980 --> 00:06:36,220 So the odds seem good that it won't happen any time soon. 105 00:06:37,900 --> 00:06:40,400 Understanding these strange objects today 106 00:06:40,400 --> 00:06:43,280 may be the key to understanding the birth of our universe, 107 00:06:43,280 --> 00:06:45,760 and why it grew to look the way it does now. 108 00:06:46,660 --> 00:06:51,760 When scientists first started playing with magnets and wires and thinking about electrons, 109 00:06:51,760 --> 00:06:55,660 they had no idea how technology would evolve in the next hundred years. 110 00:06:56,320 --> 00:07:00,680 The scientists thinking about the cause of neutron stars and strange matter today 111 00:07:00,680 --> 00:07:05,500 may be setting up humans for a future beyond our wildest imaginations 112 00:07:05,860 --> 00:07:06,860 ...or maybe not. 113 00:07:07,260 --> 00:07:08,240 Time will tell... 114 00:07:09,840 --> 00:07:13,080 So, while you're waiting to see if the universe gets destroyed, 115 00:07:13,080 --> 00:07:15,420 you might still want to find out more about it. 116 00:07:15,960 --> 00:07:16,760 We've got you. 117 00:07:16,760 --> 00:07:21,780 Our friends from Brilliant can be your insight into a whole world of science, black holes and all. 118 00:07:22,020 --> 00:07:25,380 Brilliant is a website that helps you tackle science in a practical way, 119 00:07:25,380 --> 00:07:30,720 with interactive problem-solving courses and daily challenges in maths, logic, and engineering. 120 00:07:30,800 --> 00:07:34,920 Each problem gives you all the tools you'll need to crack complex topics all by yourself. 121 00:07:35,060 --> 00:07:36,420 It's learning by doing, 122 00:07:36,420 --> 00:07:38,540 but with your brain, instead of your hands. 123 00:07:38,960 --> 00:07:42,700 Use your curiosity to get to the bottom of puzzles and courses about things 124 00:07:42,700 --> 00:07:47,040 like classical mechanics, astronomy, gravitational physics, and much more. 125 00:07:47,540 --> 00:07:51,520 If you click the link in the description or visit brilliant.org/nutshell, 126 00:07:51,520 --> 00:07:54,960 you can sign up for free and learn more things than you can imagine. 127 00:07:55,820 --> 00:07:58,280 And there's an extra perk for Kurzgesagt viewers. 128 00:07:58,400 --> 00:08:03,920 The first 688 people to use the link get 20% off their annual membership, 129 00:08:03,920 --> 00:08:08,200 which lets you view all the daily problems in the archives and unlock every course. 130 00:08:09,460 --> 00:08:12,460 Brilliant helps you end your day a little smarter. 131 00:08:12,680 --> 00:08:15,100 You might get hooked on the experience. 132 00:08:16,460 --> 00:08:26,440 [Outro music]12157

Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.