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Sagittarius A* Is Far More Dangerous Than You Think — Transcript

by Flippo Explains · 1,897 words · 314 segments · language en · Watch on YouTube

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  1. 0:00The stars are too close. That is your
  2. 0:02first thought when the engines go quiet.
  3. 0:04Through the front window, the sky is not
  4. 0:06black. It is crowded. Stars everywhere.
  5. 0:09Big ones, bright ones, white, yellow,
  6. 0:12orange.
  7. 0:14They are packed so tightly they look
  8. 0:16like spilled sugar. There is no night
  9. 0:18here. There is barely any dark. You are
  10. 0:21at the center of the Milky Way, about
  11. 0:2326,000 light-years from home. How you
  12. 0:26got here is a different problem.
  13. 0:28Today, you only have one job. You are
  14. 0:30going to try to land on Sagittarius A*
  15. 0:33the giant black hole at the heart of our
  16. 0:35galaxy. It has about 4 million times the
  17. 0:38mass of the Sun. And that brings you to
  18. 0:40the first problem with your mission.
  19. 0:42A black hole has no ground. No rocks, no
  20. 0:45dust, no surface at all. You are trying
  21. 0:48to land on something that does not have
  22. 0:49a floor. Mission control knew this. They
  23. 0:52sent you anyway. That tells you
  24. 0:54something about mission control.
  25. 0:56From Earth, nobody has ever seen this
  26. 0:58view with their own eyes. Huge clouds of
  27. 1:01dust sit between Earth and the galactic
  28. 1:03center. They block almost all of its
  29. 1:05visible light. You are the first one to
  30. 1:08just look out of the window.
  31. 1:10Back home, the nearest star is more than
  32. 1:12four light-years away. Here, neighboring
  33. 1:14stars can be hundreds of times closer
  34. 1:16than that. You start searching for the
  35. 1:18black hole. You check every direction.
  36. 1:20Nothing.
  37. 1:21Between them, long glowing streams of
  38. 1:23gas curl slowly inward. They look like
  39. 1:26the arms of a lazy whirlpool. But at the
  40. 1:28center of that whirlpool, you see
  41. 1:30nothing at all. That makes sense. A
  42. 1:33black hole does not shine.
  43. 1:35It swallows light. So, you cannot look
  44. 1:38for it directly. You have to look for
  45. 1:40what it does to everything else.
  46. 1:42Then you notice one star moving faster
  47. 1:44than the others. Much faster.
  48. 1:47It is swinging around an empty patch of
  49. 1:49sky. Like a stone on a string. Except
  50. 1:52there is no string. And there is nothing
  51. 1:54in the middle. That star is called S2.
  52. 1:57At its closest pass, it moves over 7,000
  53. 2:00km per second.
  54. 2:02That is fast enough to cross the Earth
  55. 2:04in under 2 seconds.
  56. 2:06And it repeats this loop roughly every
  57. 2:0716 years.
  58. 2:09Something invisible is pulling it
  59. 2:10around. Something incredibly heavy.
  60. 2:13Packed into a tiny space.
  61. 2:15Back on Earth, astronomers tracked stars
  62. 2:18like this for decades. That is how they
  63. 2:20knew this black hole existed. It is also
  64. 2:23how they knew where to send you. S2 even
  65. 2:25carries a message about what is coming.
  66. 2:28As its light climbs away from the black
  67. 2:29hole, it gets stretched. The light
  68. 2:32shifts slightly toward red. Gravity is
  69. 2:34not just pulling on the star. It is
  70. 2:36pulling on its light. You make a mental
  71. 2:38note. That seems important.
  72. 2:41You point the capsule at the empty patch
  73. 2:43and you go.
  74. 2:44As you get closer, the empty patch is
  75. 2:46not completely empty.
  76. 2:48There is a faint glow around it.
  77. 2:50Thin, hot gas swirls inward in a slow
  78. 2:53spiral.
  79. 2:54Most famous black holes are messy
  80. 2:56eaters.
  81. 2:57This one barely eats.
  82. 2:59Sagittarius A* is one of the dimmest
  83. 3:02giant black holes we know.
  84. 3:04Most of the time, it is starving.
  85. 3:06That sounds reassuring. It is not.
  86. 3:09Because it has not always been this
  87. 3:11calm.
  88. 3:12Clouds of gas near the center still glow
  89. 3:14with old reflected X-ray light. That
  90. 3:16echo suggests it flared much brighter a
  91. 3:18few centuries ago.
  92. 3:20So, you have arrived during a quiet
  93. 3:21period. You decide not to mention this
  94. 3:24to the black hole.
  95. 3:25Because even quiet, the gas it does eat
  96. 3:28is ferociously hot. We are talking
  97. 3:30billions of degrees. But it glows with
  98. 3:33radio waves and it can blast out X-rays.
  99. 3:36Your radiation alarm starts beeping.
  100. 3:38Quietly at first.
  101. 3:40You raise the shielding. You remind
  102. 3:42yourself this is the calm version.
  103. 3:44Then the black hole flares.
  104. 3:46Without warning, the glow brightens. A
  105. 3:49burst of X-rays ripples out from the
  106. 3:50center.
  107. 3:51Flares like this happen roughly once a
  108. 3:53day.
  109. 3:55Nobody fully knows what triggers them.
  110. 3:57Your alarm stops beeping politely. It
  111. 3:59starts screaming. Your shielding holds,
  112. 4:02barely.
  113. 4:03You make a note. Mission Control's
  114. 4:05definition of quiet needs work.
  115. 4:07The flare fades.
  116. 4:09The glow settles down.
  117. 4:10And now you are close enough to see the
  118. 4:12dark spot itself. A round black shadow
  119. 4:15surrounded by a ring of glowing gas.
  120. 4:17Astronomers revealed a picture of this
  121. 4:19ring in 2022. It was blurry, orange,
  122. 4:23taken from 26,000 light years away.
  123. 4:26Now you are looking at the real thing,
  124. 4:27up close.
  125. 4:29Somewhere inside that black shadow is
  126. 4:30the event horizon. The edge of no
  127. 4:32return.
  128. 4:33Anything that crosses it, even light,
  129. 4:35can never come back out.
  130. 4:37The event horizon is roughly 18 times
  131. 4:40wider than the sun. The glowing ring
  132. 4:42around it would fit inside the orbit of
  133. 4:44Mercury. That is not a planet. That is
  134. 4:46not a star. That is a hole in the rules.
  135. 4:50Then the sky starts to bend.
  136. 4:52Stars behind the black hole do not
  137. 4:53disappear.
  138. 4:54They smear.
  139. 4:56Their light curves around the edge of
  140. 4:57the shadow.
  141. 4:58One star turns into two copies. Then
  142. 5:01into a thin glowing arc.
  143. 5:03You can see stars that should be hidden
  144. 5:04behind the black hole. Gravity here is
  145. 5:07bending light like a giant lens. The
  146. 5:09whole sky looks like it is being pulled
  147. 5:11into a funnel.
  148. 5:12Your eyes say everything is moving. Your
  149. 5:14instruments say it is just the light.
  150. 5:16You trust the instruments, mostly.
  151. 5:19If you're enjoying this video, please
  152. 5:21hit the subscribe button. It genuinely
  153. 5:23helps keep the channel alive. So far you
  154. 5:26have been falling freely. Now you try
  155. 5:28the sensible thing. You decide to orbit
  156. 5:30first. Circle the target. Find a good
  157. 5:32spot to land.
  158. 5:34At first, this works.
  159. 5:36At about three times the radius of the
  160. 5:37event horizon, something strange
  161. 5:39happens.
  162. 5:40Your orbit stops being stable.
  163. 5:42The tiniest nudge, and you start sliding
  164. 5:44inward.
  165. 5:46Closer than this, there are no safe
  166. 5:47circles left. There is no parking spot.
  167. 5:50You can either fall in or fire your
  168. 5:52engines very, very hard. You keep going.
  169. 5:55Now you reach a place where gravity can
  170. 5:57bend light into a circle.
  171. 5:59Light can actually orbit the black hole
  172. 6:01here.
  173. 6:02Light leaving the back of your capsule
  174. 6:04can travel all the way around and come
  175. 6:06back to you from the front.
  176. 6:08In principle, you could look ahead and
  177. 6:10see your own ship's back.
  178. 6:13The universe has turned into a hall of
  179. 6:14mirrors
  180. 6:15with you as the only exhibit. So you try
  181. 6:18plan B. If you cannot orbit, maybe you
  182. 6:21can hover. You point the engines down.
  183. 6:23You fire. And you discover what hovering
  184. 6:25here actually costs.
  185. 6:27To hold still this close, your engines
  186. 6:30must push incredibly hard.
  187. 6:32We are talking hundreds of thousands of
  188. 6:33times Earth's gravity.
  189. 6:35At that force, you would not be sitting
  190. 6:37in your seat.
  191. 6:39You would become part of your seat. You
  192. 6:40turn the engines off
  193. 6:42and you let yourself fall.
  194. 6:44Before you go further, you check on your
  195. 6:46backup plan.
  196. 6:47Far behind you, you left a small
  197. 6:49observer probe. It is parked a safe
  198. 6:51distance away.
  199. 6:52Its only job is to watch you.
  200. 6:55Your capsule sends it a blinking signal,
  201. 6:57one flash every second. At first, the
  202. 6:59probe receives one flash every second.
  203. 7:02Then something strange happens. The
  204. 7:04flashes start arriving further apart. 1
  205. 7:07second, then two, then 10.
  206. 7:11From the probe's point of view, your
  207. 7:12clock is slowing down. Your capsule is
  208. 7:15changing color, too. Its light shifts
  209. 7:17toward red, then deeper red, then into
  210. 7:20colors no human eye can see.
  211. 7:22To the probe, you are slowing down,
  212. 7:25fading,
  213. 7:26getting dimmer.
  214. 7:27But inside the capsule, nothing feels
  215. 7:29different. Your watch ticks normally.
  216. 7:32Your heart beats normally.
  217. 7:34Time is not broken. It is just running
  218. 7:37differently for the two of you.
  219. 7:38By now, you are falling incredibly fast.
  220. 7:41The black shadow fills most of your
  221. 7:43window.
  222. 7:44The rest of the universe is squeezed
  223. 7:46into a bright ring around it, and then
  224. 7:48you reach the event horizon. You brace
  225. 7:50for impact. Nothing happens. No wall.
  226. 7:54No flash, no bump, you just pass
  227. 7:56through. You might expect the edge of a
  228. 7:58black hole to tear you apart. But for a
  229. 8:01black hole this big, the event horizon
  230. 8:03is surprisingly gentle.
  231. 8:05Gravity pulls on your feet a little
  232. 8:06harder than on your head.
  233. 8:08But near the horizon of this giant, that
  234. 8:10difference is tiny. Far too small to
  235. 8:12feel. Smaller black holes are the
  236. 8:14dangerous ones at the edge. A small one
  237. 8:17would stretch you apart before you
  238. 8:18reached its horizon. This giant lets you
  239. 8:20in politely.
  240. 8:22It is the most polite trap in the
  241. 8:23universe. Because something has changed.
  242. 8:26You just cannot see it yet. You look
  243. 8:28back. The stars are still there. Light
  244. 8:31from outside keeps pouring in behind
  245. 8:32you.
  246. 8:33But nothing you send can get out. Your
  247. 8:36blinking signals no longer reach the
  248. 8:38probe. So you try the last escape plan
  249. 8:40you have. You turn the capsule around.
  250. 8:43Full thrust, away from the center.
  251. 8:46It does not help.
  252. 8:47Inside the event horizon, outward is no
  253. 8:49longer a direction you can go. Space and
  254. 8:52time are so twisted here. The center is
  255. 8:54not just ahead of you, it is your
  256. 8:56future. Every path you could take leads
  257. 8:59there.
  258. 9:00The same way every day, no matter what
  259. 9:02you do, leads to tomorrow.
  260. 9:04And here is the cruel twist.
  261. 9:06Firing your engines does not buy you
  262. 9:08time. It makes you reach the center
  263. 9:10sooner.
  264. 9:11The way to last longest in here is to do
  265. 9:13nothing at all.
  266. 9:15Just fall.
  267. 9:16For a black hole this size, that means
  268. 9:18roughly a minute, probably less.
  269. 9:20The best survival strategy is to relax,
  270. 9:23which is not something your body is
  271. 9:24currently interested in.
  272. 9:25The seconds tick by.
  273. 9:27Then you start to feel it. Your feet are
  274. 9:30being pulled slightly harder than your
  275. 9:31head.
  276. 9:32Then harder, then much harder. Your body
  277. 9:35is being stretched along its length, and
  278. 9:37squeezed in from the sides.
  279. 9:40Physicists have a word for this,
  280. 9:41spaghettification. It is a silly word
  281. 9:44for something deeply unpleasant. In a
  282. 9:46giant like this, it only happens at the
  283. 9:48very end. In the final fraction of a
  284. 9:50second. What happens after that, nobody
  285. 9:53knows.
  286. 9:54At the very center, our best theory of
  287. 9:56gravity breaks down. It predicts a point
  288. 9:59where density becomes infinite. Most
  289. 10:01physicists think that means the theory
  290. 10:03is incomplete there. Not that infinity
  291. 10:05is actually real.
  292. 10:07Your trip ends at the one place where
  293. 10:09physics runs out of answers. Now, back
  294. 10:12to the probe. It is still parked far
  295. 10:14away, still watching. And from its point
  296. 10:17of view, you never arrive. It sees your
  297. 10:20capsule creep closer to the horizon.
  298. 10:23Slower and slower. Redder and dimmer.
  299. 10:27Your last flashes stretch out until they
  300. 10:29fade into nothing.
  301. 10:30To the rest of the universe, you never
  302. 10:32quite fall in. You just fade away at the
  303. 10:35edge.
  304. 10:36So, did you land on Sagittarius A*? Kind
  305. 10:39of. There was no ground to touch. No
  306. 10:42surface to plant a flag on, but you did
  307. 10:44reach it, and it kept you. Your mass now
  308. 10:47belongs to the black hole.
  309. 10:494 million suns, plus one astronaut.
  310. 10:52Slightly heavier now. Nobody will ever
  311. 10:54be able to measure the difference.
  312. 10:5526,000 light years of travel. And your
  313. 10:58biggest impact on the galaxy is a
  314. 10:59rounding error.

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