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What Would Happen If The Sun Disappeared For One Week? — Transcript

by The Last Day · 3,049 words · 550 segments · language en · Watch on YouTube

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  1. 0:00S S for sun.
  2. 0:02>> S for sun.
  3. 0:03>> Very good. And [music] the sun gives us
  4. 0:04light. It gives us everything.
  5. 0:06Oh, I've got you. I've got you. Hold on
  6. 0:08to me.
  7. 0:09>> Mama, what is it?
  8. 0:11>> Don't look at it.
  9. 0:12>> Mama, the sun.
  10. 0:15>> Right now, the sun is shining on you.
  11. 0:18Or at least, it was 8 minutes [music]
  12. 0:20ago.
  13. 0:21That is how long sunlight takes to cross
  14. 0:24the 93 million miles between the sun and
  15. 0:27the earth.
  16. 0:298 minutes and 20 [music] seconds.
  17. 0:32So, the light hitting your window at
  18. 0:33this moment left the sun's surface
  19. 0:36before you started watching [music] this
  20. 0:38video.
  21. 0:39Which means something strange and rather
  22. 0:42unsettling.
  23. 0:44If the sun vanished right now,
  24. 0:46completely and instantly,
  25. 0:48>> [music]
  26. 0:48>> you would have no idea.
  27. 0:51For 8 minutes, the sky would stay blue.
  28. 0:54Shadows would fall exactly where they
  29. 0:57always do.
  30. 0:58Birds would keep singing. Satellites
  31. 1:01would keep tracking a star that no
  32. 1:03longer exists.
  33. 1:05Every plant on earth would keep
  34. 1:08photosynthesizing [music]
  35. 1:09using light from a sun that disappeared
  36. 1:12before the sentence [music] began.
  37. 1:14And then, at 8 minutes and 20 seconds,
  38. 1:18the sky would go out.
  39. 1:20Not dim, not fade,
  40. 1:23out.
  41. 1:24So, let's run the scenario properly.
  42. 1:27The sun disappears [music] completely
  43. 1:29for exactly 7 days, then returns
  44. 1:32unchanged, exactly [music] as it was.
  45. 1:36How cold does it get?
  46. 1:38What dies first? Does anything [music]
  47. 1:41survive?
  48. 1:42And does the earth even stay where it
  49. 1:44is?
  50. 1:45Let's find out.
  51. 1:47Before anything happens, we need to be
  52. 1:50clear about the rules.
  53. 1:52The sun does two things for earth.
  54. 1:55It provides light and heat, [music] and
  55. 1:58it provides gravity.
  56. 2:00Its gravitational pull is what holds our
  57. 2:03planet in [music] orbit, and both of
  58. 2:05those things travel at the same speed.
  59. 2:08The speed of light.
  60. 2:10This is one of the [music] most
  61. 2:11important results in physics.
  62. 2:14Gravity is not instantaneous.
  63. 2:17When Einstein published general [music]
  64. 2:19relativity, one of its predictions was
  65. 2:22that changes in gravity propagate
  66. 2:24[music] outward at exactly the speed of
  67. 2:26light, no faster.
  68. 2:29That prediction was confirmed [music] in
  69. 2:312015, when detectors on Earth measured
  70. 2:34gravitational [music] waves from two
  71. 2:36black holes colliding over a billion
  72. 2:39light-years away, arriving precisely as
  73. 2:42the theory said they should.
  74. 2:45So, in our scenario, the light and the
  75. 2:47gravity [music] disappear together. And
  76. 2:50they both stop reaching us after the
  77. 2:52same delay.
  78. 2:548 minutes and 20 seconds [music] of a
  79. 2:56completely normal afternoon.
  80. 2:59Then, everything changes at once.
  81. 3:03At 8 minutes and 20 seconds, [music]
  82. 3:05the last photons from the Sun arrive at
  83. 3:08Earth.
  84. 3:09And then, nothing.
  85. 3:11For anyone standing [music] on the
  86. 3:13daylight side of the planet, the
  87. 3:15experience would be instant and total.
  88. 3:19The sky does [music] not darken
  89. 3:20gradually because there is no light left
  90. 3:23to scatter.
  91. 3:25The blue sky you see is sunlight
  92. 3:27bouncing off air molecules.
  93. 3:29Remove the source, and the sky simply
  94. 3:32stops [music] existing as a bright
  95. 3:34thing.
  96. 3:36Daylight becomes night in less than a
  97. 3:38second.
  98. 3:39But here is the detail almost nobody
  99. 3:42expects. [music]
  100. 3:44It would not be properly dark.
  101. 3:47Because the stars are still there.
  102. 3:50Without the Sun washing out the sky, you
  103. 3:53would see the full night sky in the
  104. 3:55middle of the afternoon. And it would be
  105. 3:57the clearest, most brilliant sky any
  106. 4:00human has ever seen outside [music] a
  107. 4:03desert at new moon.
  108. 4:05You would also see the planets still
  109. 4:07shining. Venus, Jupiter, Mars, all of
  110. 4:12them still lit.
  111. 4:14For about 8 minutes, because sunlight
  112. 4:16[music] takes different amounts of time
  113. 4:18to reach each of them, and then to
  114. 4:20bounce back to us.
  115. 4:22So, the planets would go out one by one
  116. 4:25in order of their distance, like someone
  117. 4:28walking down a corridor switching off
  118. 4:30lamps.
  119. 4:32The moon would be the first to go within
  120. 4:34a second or two.
  121. 4:36Venus a few minutes later, then Mars,
  122. 4:39then Jupiter half an hour or more after
  123. 4:42the sun vanished.
  124. 4:44Imagine standing outside and watching
  125. 4:46the planets extinguish one at a time in
  126. 4:50a sky full of stars.
  127. 4:52It would be the most beautiful thing any
  128. 4:55human being will ever see.
  129. 4:58Now, the other half of the problem. The
  130. 5:01sun's [music] gravity is gone, too.
  131. 5:04And at that same instant, Earth stops
  132. 5:07orbiting.
  133. 5:08Here is [music] what people usually get
  134. 5:10wrong. The Earth does not fall toward
  135. 5:13where the sun used to be, and it does
  136. 5:16not fly away at random.
  137. 5:18It simply obeys Newton's first law.
  138. 5:22An object in motion stays in motion
  139. 5:25unless a force acts on it.
  140. 5:28The force is [music] gone.
  141. 5:30So, the Earth travels in a perfectly
  142. 5:32straight line in whatever direction it
  143. 5:35happened to [music] be moving at that
  144. 5:37moment at the speed it was already
  145. 5:39going.
  146. 5:41That speed is about 30 [music] km/s,
  147. 5:44roughly 107,000
  148. 5:46km/h.
  149. 5:49We would be flying off at a tangent
  150. 5:51[music]
  151. 5:51straight out of the solar system.
  152. 5:54But over the course of 1 week, [music]
  153. 5:56how far is that?
  154. 5:58About 18 million kilometers.
  155. 6:01Which sounds enormous, but in solar
  156. 6:04system [music] terms, it is nothing.
  157. 6:06It is around 12% of the distance to the
  158. 6:09sun.
  159. 6:10Not far enough to matter [music] for
  160. 6:12temperature because the sun is gone
  161. 6:15anyway.
  162. 6:16So, after 7 days, we are 18 million
  163. 6:20kilometers off course, moving in a
  164. 6:22straight line through empty space, and
  165. 6:25we would need the sun to come back in
  166. 6:27exactly the right [music] place to
  167. 6:29resume our orbit. In our scenario, it
  168. 6:32does, but hold that thought because it
  169. 6:35becomes important later.
  170. 6:37Meanwhile, on the surface, nobody is
  171. 6:39thinking about orbital mechanics. They
  172. 6:42are thinking about the temperature. This
  173. 6:44is the question everyone asks, and the
  174. 6:46answer is more [music] interesting than
  175. 6:48you might expect because the cooling is
  176. 6:50not steady at all. Earth's surface stays
  177. 6:54warm in two ways. It absorbs sunlight,
  178. 6:57and it is wrapped in an atmosphere and
  179. 6:59oceans that store enormous [music]
  180. 7:02amounts of heat. Remove the sunlight and
  181. 7:04the planet starts radiating its stored
  182. 7:07heat [music] into space without anything
  183. 7:09replacing it.
  184. 7:10Within the first 24 hours, average
  185. 7:13global surface temperature would drop by
  186. 7:15roughly [music] 18° C.
  187. 7:19That is a dramatic fall,
  188. 7:22>> [music]
  189. 7:22>> but it is survivable almost everywhere.
  190. 7:25A warm summer day [music] becomes a cold
  191. 7:27winter day.
  192. 7:29And here is where the cooling slows
  193. 7:31down. As the surface gets colder, it
  194. 7:34radiates heat more slowly. The rate of
  195. 7:37heat loss depends very strongly [music]
  196. 7:38on temperature, so the colder Earth
  197. 7:41becomes, the longer it takes to lose the
  198. 7:43next degree. [music]
  199. 7:45So, the first day is brutal. The second
  200. 7:48day is worse. But, after that, the curve
  201. 7:50starts to flatten. Estimates [music]
  202. 7:53suggest that within a week, average
  203. 7:55surface temperatures would fall to
  204. 7:57somewhere around -40°C.
  205. 8:00[music]
  206. 8:01Within a year, somewhere around -70.
  207. 8:05So, let's be precise about our scenario.
  208. 8:087 days without the sun
  209. 8:09>> [music]
  210. 8:10>> does not freeze the Earth solid. It does
  211. 8:12not boil off the atmosphere [music] or
  212. 8:15turn the oceans to ice. What it does is
  213. 8:18deliver the most severe [music] and
  214. 8:20sudden winter in the history of the
  215. 8:22planet. And that is more than enough.
  216. 8:25In the first hours, the most dangerous
  217. 8:28thing is not the cold. It is the
  218. 8:30darkness
  219. 8:31>> [music]
  220. 8:31>> arriving instantly across half the
  221. 8:33world. Every aircraft in flight on the
  222. 8:36daylight side loses visual reference
  223. 8:39without warning.
  224. 8:40>> [music]
  225. 8:41>> Every road suddenly has no light. Power
  226. 8:44grids face an immediate and catastrophic
  227. 8:46problem because solar generation
  228. 8:49vanishes worldwide in the same [music]
  229. 8:51second. And demand for heating and
  230. 8:53lighting spikes at once. Grids are
  231. 8:56balancing acts. A sudden massive
  232. 8:59imbalance triggers protective [music]
  233. 9:01shutdowns, and those cascade. Large
  234. 9:04portions of the world lose power within
  235. 9:07hours. Meanwhile, [music]
  236. 9:09the temperature is dropping by roughly a
  237. 9:11degree every 80 minutes. By the end of
  238. 9:14the first day, surviving in most of the
  239. 9:16world means having heat that does not
  240. 9:18[music] depend on the grid. Gas, wood,
  241. 9:22oil, anything that burns. And something
  242. 9:25else is happening quietly that will
  243. 9:27matter enormously later. Photosynthesis
  244. 9:31has stopped. Every plant on Earth, every
  245. 9:34tree, every crop, every blade of grass,
  246. 9:38and critically, every microscopic plant
  247. 9:40[music] in the ocean has stopped
  248. 9:42converting light into energy.
  249. 9:45The entire food [music] chain of this
  250. 9:46planet has been unplugged at the source.
  251. 9:50Plants do not die [music] immediately.
  252. 9:52Most can survive days of darkness using
  253. 9:55stored energy. A week of [music]
  254. 9:57darkness alone would not kill a mature
  255. 9:59tree.
  256. 10:01But the cold is a different matter.
  257. 10:03By the second day, average temperatures
  258. 10:05[music]
  259. 10:05are approaching minus 20.
  260. 10:08Something is now happening to the
  261. 10:10weather that is genuinely strange. Our
  262. 10:13atmosphere moves because of uneven
  263. 10:15heating. The equator receives more
  264. 10:18energy than the poles. Warm air rises,
  265. 10:21cold air sinks, [music] and the whole
  266. 10:23system churns. Every wind, every storm,
  267. 10:28every weather system on this planet is
  268. 10:30ultimately driven by sunlight. With the
  269. 10:33sun gone, that engine switches off. The
  270. 10:37existing weather does not stop instantly
  271. 10:39because the atmosphere still holds
  272. 10:41momentum, and the oceans still hold
  273. 10:44heat. But the temperature difference
  274. 10:46that drives it begins to collapse,
  275. 10:49>> [music]
  276. 10:49>> and the global circulation starts
  277. 10:51winding down. In many places, [music]
  278. 10:54the wind simply dies.
  279. 10:56Alongside that, something else begins.
  280. 11:00The oceans are [music] now far warmer
  281. 11:02than the air above them, and that
  282. 11:04difference drives enormous evaporation
  283. 11:06and condensation.
  284. 11:08Heavy snowfall would develop over
  285. 11:10coastal regions and [music] across the
  286. 11:12seas as warm ocean moisture meets
  287. 11:15freezing air.
  288. 11:17Here is where we need to be honest about
  289. 11:20casualties, [music]
  290. 11:21and the order may surprise you.
  291. 11:24The first things to go [music] in large
  292. 11:26numbers are the smallest. Phytoplankton,
  293. 11:29the microscopic photosynthetic life in
  294. 11:31the ocean surface waters are responsible
  295. 11:34for a huge proportion of the planet's
  296. 11:36oxygen production and sit at the base of
  297. 11:39the marine food web.
  298. 11:41Many have very short lifespans measured
  299. 11:44[music] in days.
  300. 11:46A week without light causes a severe
  301. 11:48collapse in their numbers.
  302. 11:50On land, most plants survive a week of
  303. 11:53darkness, but not necessarily a week of
  304. 11:55[music] extreme cold.
  305. 11:57Tropical plants, which have no
  306. 11:59adaptation to frost at all, would be
  307. 12:01devastated. Crops in the field would
  308. 12:04[music] be lost worldwide.
  309. 12:06Temperate and polar plants, already
  310. 12:09built for winter,
  311. 12:10>> [music]
  312. 12:10>> would mostly survive.
  313. 12:12Insects, being small and cold-blooded,
  314. 12:15would suffer enormously outside of
  315. 12:17shelter.
  316. 12:18Large mammals, including humans, are in
  317. 12:21a strange position.
  318. 12:23We can survive minus 40 as long as we
  319. 12:26[music] have insulation and heat. Our
  320. 12:28problem is not biology. It is
  321. 12:31infrastructure.
  322. 12:33And here is the point worth dwelling on.
  323. 12:36Where you are matters far more than what
  324. 12:39you are.
  325. 12:40If you are in the deep ocean, nothing
  326. 12:42happens.
  327. 12:43The abyss [music] is permanently dark
  328. 12:45and close to freezing already.
  329. 12:48Life down there, much of which depends
  330. 12:50on chemical energy from hydrothermal
  331. 12:52vents rather than sunlight,
  332. 12:54>> [music]
  333. 12:54>> would not register the event at all.
  334. 12:57If you are in a cave system, [music] in
  335. 12:59deep soil, or in a hot spring, you would
  336. 13:02likely be fine.
  337. 13:04If you are a microbe several kilometers
  338. 13:06underground, drawing energy from rock
  339. 13:08chemistry, the sun disappearing is not
  340. 13:11an event in your life.
  341. 13:13Those organisms would never know.
  342. 13:16>> [music]
  343. 13:16>> The deeper and darker your home, the
  344. 13:19safer you are.
  345. 13:20By day four, average [music]
  346. 13:22temperatures are falling toward minus
  347. 13:2430.
  348. 13:25The oceans are now doing something
  349. 13:26[music] important, and it is the reason
  350. 13:29the Earth does not simply freeze.
  351. 13:32Water has an extraordinarily high heat
  352. 13:34capacity. It takes an enormous amount of
  353. 13:37energy to change its temperature, which
  354. 13:40means it also releases that energy
  355. 13:42slowly.
  356. 13:43The oceans hold a vast reservoir of heat
  357. 13:46accumulated over a very long time, and
  358. 13:49they do not give it up quickly.
  359. 13:51Sea ice begins forming far outside its
  360. 13:54usual range, spreading across the
  361. 13:56surface [music] of seas that have never
  362. 13:58frozen.
  363. 13:59But that ice then acts as insulation,
  364. 14:02slowing further heat loss from the water
  365. 14:04below.
  366. 14:05So, beneath the ice, the ocean stays
  367. 14:08liquid and [music] relatively warm.
  368. 14:10Life in the water column continues, for
  369. 14:13now.
  370. 14:14On land, by day [music] six and seven,
  371. 14:17we are approaching minus 40 on average,
  372. 14:20far colder in continental interiors.
  373. 14:23>> [music]
  374. 14:23>> This is comparable to an Antarctic
  375. 14:25winter, except it is everywhere at once.
  376. 14:29Anyone still alive is alive because they
  377. 14:32have fuel, shelter, and [music] food
  378. 14:34stored indoors, and because they stopped
  379. 14:36relying on anything that requires
  380. 14:38electricity days ago.
  381. 14:41The night sky is still spectacular.
  382. 14:42[music]
  383. 14:44That has not changed.
  384. 14:46Seven days of the clearest stars ever
  385. 14:48seen from the surface of this planet,
  386. 14:51over a world that is slowly freezing
  387. 14:53beneath them.
  388. 14:55On day seven, the sun comes back, and it
  389. 14:58does not announce itself.
  390. 15:00For 8 minutes [music] and 20 seconds,
  391. 15:03nothing happens, because the light is
  392. 15:05still in [music] transit.
  393. 15:07The world remains dark and frozen, while
  394. 15:1093 million kilometers away, a star is
  395. 15:13already shining.
  396. 15:15Then dawn arrives everywhere at once, in
  397. 15:18the middle of whatever hour it happens
  398. 15:20to be, [music]
  399. 15:21with no warning and no horizon glow.
  400. 15:25The sky simply switches back on.
  401. 15:28It would be the single most emotional
  402. 15:29moment in human history.
  403. 15:32But the return is not gentle. [music]
  404. 15:35The planet is now covered in fresh snow
  405. 15:37and ice over an enormous area.
  406. 15:40And ice reflects sunlight rather [music]
  407. 15:42than absorbing it.
  408. 15:44This is called albedo.
  409. 15:46A bright planet absorbs less energy than
  410. 15:48a dark one. Which means the newly frozen
  411. 15:51Earth would warm back up more slowly
  412. 15:53than it cooled.
  413. 15:55At the same time, the atmosphere that
  414. 15:57had wound down is suddenly given energy
  415. 16:00again. And the temperature differences
  416. 16:02driving circulation are now extreme and
  417. 16:05chaotic.
  418. 16:07The restart would bring violent storms
  419. 16:09worldwide. Recovery to normal global
  420. 16:12temperatures would take weeks to months,
  421. 16:15not days.
  422. 16:16And the ecological damage would last
  423. 16:18[music] far longer.
  424. 16:20A collapsed plankton population takes
  425. 16:23time to rebuild. A lost global harvest
  426. 16:26means [music] a food crisis that
  427. 16:28outlives the event by a year or more.
  428. 16:31The week [music] of darkness ends. The
  429. 16:34consequences do not.
  430. 16:36Now the detail that makes this [music]
  431. 16:38scenario genuinely strange, and it has
  432. 16:41nothing to do with temperature.
  433. 16:45>> [music]
  434. 16:48>> When the sun reappears, its gravity has
  435. 16:50to travel to us as well, taking another
  436. 16:538 minutes to arrive.
  437. 16:55And when it does, Earth is in the wrong
  438. 16:57place, moving in the wrong direction.
  439. 17:01We would not simply resume our old
  440. 17:03orbit. We would fall into a new one, an
  441. 17:07[music] ellipse shaped by our position
  442. 17:09and velocity at that moment.
  443. 17:12Depending on the direction we happen
  444. 17:13[music] to be traveling when the sun
  445. 17:15vanished, that new orbit could bring us
  446. 17:17closer to the Sun at some points and
  447. 17:19further away at others.
  448. 17:22In other words, a week without the Sun
  449. 17:24>> [music]
  450. 17:24>> would permanently change the shape of
  451. 17:26our year.
  452. 17:28The seasons would be different. The
  453. 17:30length of the year would be different.
  454. 17:33Not catastrophically, perhaps, but
  455. 17:35measurably and forever.
  456. 17:38And we would not be alone. Every planet,
  457. 17:41every moon, every asteroid in the solar
  458. 17:45system would have done the same thing.
  459. 17:47Each flying off on its own tangent for a
  460. 17:50week before being recaptured into a new
  461. 17:53orbit.
  462. 17:54The entire solar system would be
  463. 17:56reshuffled and the long-term [music]
  464. 17:58stability of those new orbits would be
  465. 18:00an open question.
  466. 18:02The Sun returning would not restore the
  467. 18:04solar system. It would create a new one.
  468. 18:08No.
  469. 18:08>> [music]
  470. 18:09>> And the reason is worth explaining.
  471. 18:11Mass cannot simply vanish.
  472. 18:14Conservation of energy is one of the
  473. 18:16most thoroughly tested principles in all
  474. 18:18of physics and nothing in the known
  475. 18:21universe allows an object of 2 billion
  476. 18:24billion billion tons to stop existing.
  477. 18:28The Sun also cannot switch off. It
  478. 18:31shines because of nuclear fusion in its
  479. 18:33core, converting hydrogen into helium
  480. 18:36and releasing energy. And that process
  481. 18:39is self-regulating and remarkably
  482. 18:41stable.
  483. 18:42It has been running for around 4 and 1/2
  484. 18:45billion years and has roughly 5 billion
  485. 18:48left. And even if fusion somehow stopped
  486. 18:51today, the Sun [music] would not go
  487. 18:53dark.
  488. 18:55The energy generated in its core takes
  489. 18:57an extraordinarily long time to work its
  490. 19:00way to the surface [music]
  491. 19:01with estimates ranging from thousands to
  492. 19:04hundreds of thousands of years.
  493. 19:07The Sun would keep shining for a very
  494. 19:09long time on energy [music] already in
  495. 19:12transit.
  496. 19:13There is also no plausible way to remove
  497. 19:16its gravity. Gravity is produced by
  498. 19:18mass, and the mass is not going
  499. 19:21anywhere.
  500. 19:22So, the sun disappearing is not a risk.
  501. 19:25It is a thought experiment, and a useful
  502. 19:28one, because it reveals how much of our
  503. 19:30world is quietly held up by something 93
  504. 19:33million kilometers away.
  505. 19:36Here is what I find remarkable about
  506. 19:38this scenario. We tend to think of the
  507. 19:41sun as something that lights our days, a
  508. 19:44thing that rises and sets and makes the
  509. 19:46[music] weather pleasant.
  510. 19:48It is not. It is the engine that runs
  511. 19:51this entire planet.
  512. 19:54Every wind that has ever blown was
  513. 19:56driven by solar heating. Every ocean
  514. 19:59current, every storm, every rain shower,
  515. 20:03every plant, every animal, and every
  516. 20:06human being on Earth runs on energy that
  517. 20:09originated in that star.
  518. 20:12The food you ate today was sunlight a
  519. 20:14few months ago. The fuel in a car was
  520. 20:17sunlight that fell on this planet
  521. 20:19hundreds of millions of years ago.
  522. 20:22Take it away for 1 week,
  523. 20:24>> [music]
  524. 20:24>> and the planet does not explode or
  525. 20:26shatter. It simply stops.
  526. 20:29The wind drops, [music]
  527. 20:30the temperature falls, the food chain
  528. 20:33unplugs at the base, and the Earth
  529. 20:35drifts off in a straight line through
  530. 20:38the dark.
  531. 20:39And the most unsettling part is the
  532. 20:41[music] 8-minutes.
  533. 20:43The gap between the sun ending and us
  534. 20:46finding out, a window in which
  535. 20:48everything is already over and nothing
  536. 20:51has happened yet.
  537. 20:53>> [music]
  538. 20:53>> So, the next time you step outside and
  539. 20:55feel the warmth on your face, remember
  540. 20:57that it is 8-minutes old, that it
  541. 21:00traveled 93 million miles to reach you,
  542. 21:03and that it is doing far more than
  543. 21:06keeping you warm.
  544. 21:07It is holding the entire system
  545. 21:09together.
  546. 21:11Thanks for watching. If you enjoyed
  547. 21:14this, subscribe [music]
  548. 21:15and let us know in the comments which
  549. 21:17impossible scenario we should explore
  550. 21:19next.

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