What Would Happen If The Sun Disappeared For One Week? — Transcript
Full transcript
- 0:00S S for sun.
- 0:02>> S for sun.
- 0:03>> Very good. And [music] the sun gives us
- 0:04light. It gives us everything.
- 0:06Oh, I've got you. I've got you. Hold on
- 0:08to me.
- 0:09>> Mama, what is it?
- 0:11>> Don't look at it.
- 0:12>> Mama, the sun.
- 0:15>> Right now, the sun is shining on you.
- 0:18Or at least, it was 8 minutes [music]
- 0:20ago.
- 0:21That is how long sunlight takes to cross
- 0:24the 93 million miles between the sun and
- 0:27the earth.
- 0:298 minutes and 20 [music] seconds.
- 0:32So, the light hitting your window at
- 0:33this moment left the sun's surface
- 0:36before you started watching [music] this
- 0:38video.
- 0:39Which means something strange and rather
- 0:42unsettling.
- 0:44If the sun vanished right now,
- 0:46completely and instantly,
- 0:48>> [music]
- 0:48>> you would have no idea.
- 0:51For 8 minutes, the sky would stay blue.
- 0:54Shadows would fall exactly where they
- 0:57always do.
- 0:58Birds would keep singing. Satellites
- 1:01would keep tracking a star that no
- 1:03longer exists.
- 1:05Every plant on earth would keep
- 1:08photosynthesizing [music]
- 1:09using light from a sun that disappeared
- 1:12before the sentence [music] began.
- 1:14And then, at 8 minutes and 20 seconds,
- 1:18the sky would go out.
- 1:20Not dim, not fade,
- 1:23out.
- 1:24So, let's run the scenario properly.
- 1:27The sun disappears [music] completely
- 1:29for exactly 7 days, then returns
- 1:32unchanged, exactly [music] as it was.
- 1:36How cold does it get?
- 1:38What dies first? Does anything [music]
- 1:41survive?
- 1:42And does the earth even stay where it
- 1:44is?
- 1:45Let's find out.
- 1:47Before anything happens, we need to be
- 1:50clear about the rules.
- 1:52The sun does two things for earth.
- 1:55It provides light and heat, [music] and
- 1:58it provides gravity.
- 2:00Its gravitational pull is what holds our
- 2:03planet in [music] orbit, and both of
- 2:05those things travel at the same speed.
- 2:08The speed of light.
- 2:10This is one of the [music] most
- 2:11important results in physics.
- 2:14Gravity is not instantaneous.
- 2:17When Einstein published general [music]
- 2:19relativity, one of its predictions was
- 2:22that changes in gravity propagate
- 2:24[music] outward at exactly the speed of
- 2:26light, no faster.
- 2:29That prediction was confirmed [music] in
- 2:312015, when detectors on Earth measured
- 2:34gravitational [music] waves from two
- 2:36black holes colliding over a billion
- 2:39light-years away, arriving precisely as
- 2:42the theory said they should.
- 2:45So, in our scenario, the light and the
- 2:47gravity [music] disappear together. And
- 2:50they both stop reaching us after the
- 2:52same delay.
- 2:548 minutes and 20 seconds [music] of a
- 2:56completely normal afternoon.
- 2:59Then, everything changes at once.
- 3:03At 8 minutes and 20 seconds, [music]
- 3:05the last photons from the Sun arrive at
- 3:08Earth.
- 3:09And then, nothing.
- 3:11For anyone standing [music] on the
- 3:13daylight side of the planet, the
- 3:15experience would be instant and total.
- 3:19The sky does [music] not darken
- 3:20gradually because there is no light left
- 3:23to scatter.
- 3:25The blue sky you see is sunlight
- 3:27bouncing off air molecules.
- 3:29Remove the source, and the sky simply
- 3:32stops [music] existing as a bright
- 3:34thing.
- 3:36Daylight becomes night in less than a
- 3:38second.
- 3:39But here is the detail almost nobody
- 3:42expects. [music]
- 3:44It would not be properly dark.
- 3:47Because the stars are still there.
- 3:50Without the Sun washing out the sky, you
- 3:53would see the full night sky in the
- 3:55middle of the afternoon. And it would be
- 3:57the clearest, most brilliant sky any
- 4:00human has ever seen outside [music] a
- 4:03desert at new moon.
- 4:05You would also see the planets still
- 4:07shining. Venus, Jupiter, Mars, all of
- 4:12them still lit.
- 4:14For about 8 minutes, because sunlight
- 4:16[music] takes different amounts of time
- 4:18to reach each of them, and then to
- 4:20bounce back to us.
- 4:22So, the planets would go out one by one
- 4:25in order of their distance, like someone
- 4:28walking down a corridor switching off
- 4:30lamps.
- 4:32The moon would be the first to go within
- 4:34a second or two.
- 4:36Venus a few minutes later, then Mars,
- 4:39then Jupiter half an hour or more after
- 4:42the sun vanished.
- 4:44Imagine standing outside and watching
- 4:46the planets extinguish one at a time in
- 4:50a sky full of stars.
- 4:52It would be the most beautiful thing any
- 4:55human being will ever see.
- 4:58Now, the other half of the problem. The
- 5:01sun's [music] gravity is gone, too.
- 5:04And at that same instant, Earth stops
- 5:07orbiting.
- 5:08Here is [music] what people usually get
- 5:10wrong. The Earth does not fall toward
- 5:13where the sun used to be, and it does
- 5:16not fly away at random.
- 5:18It simply obeys Newton's first law.
- 5:22An object in motion stays in motion
- 5:25unless a force acts on it.
- 5:28The force is [music] gone.
- 5:30So, the Earth travels in a perfectly
- 5:32straight line in whatever direction it
- 5:35happened to [music] be moving at that
- 5:37moment at the speed it was already
- 5:39going.
- 5:41That speed is about 30 [music] km/s,
- 5:44roughly 107,000
- 5:46km/h.
- 5:49We would be flying off at a tangent
- 5:51[music]
- 5:51straight out of the solar system.
- 5:54But over the course of 1 week, [music]
- 5:56how far is that?
- 5:58About 18 million kilometers.
- 6:01Which sounds enormous, but in solar
- 6:04system [music] terms, it is nothing.
- 6:06It is around 12% of the distance to the
- 6:09sun.
- 6:10Not far enough to matter [music] for
- 6:12temperature because the sun is gone
- 6:15anyway.
- 6:16So, after 7 days, we are 18 million
- 6:20kilometers off course, moving in a
- 6:22straight line through empty space, and
- 6:25we would need the sun to come back in
- 6:27exactly the right [music] place to
- 6:29resume our orbit. In our scenario, it
- 6:32does, but hold that thought because it
- 6:35becomes important later.
- 6:37Meanwhile, on the surface, nobody is
- 6:39thinking about orbital mechanics. They
- 6:42are thinking about the temperature. This
- 6:44is the question everyone asks, and the
- 6:46answer is more [music] interesting than
- 6:48you might expect because the cooling is
- 6:50not steady at all. Earth's surface stays
- 6:54warm in two ways. It absorbs sunlight,
- 6:57and it is wrapped in an atmosphere and
- 6:59oceans that store enormous [music]
- 7:02amounts of heat. Remove the sunlight and
- 7:04the planet starts radiating its stored
- 7:07heat [music] into space without anything
- 7:09replacing it.
- 7:10Within the first 24 hours, average
- 7:13global surface temperature would drop by
- 7:15roughly [music] 18° C.
- 7:19That is a dramatic fall,
- 7:22>> [music]
- 7:22>> but it is survivable almost everywhere.
- 7:25A warm summer day [music] becomes a cold
- 7:27winter day.
- 7:29And here is where the cooling slows
- 7:31down. As the surface gets colder, it
- 7:34radiates heat more slowly. The rate of
- 7:37heat loss depends very strongly [music]
- 7:38on temperature, so the colder Earth
- 7:41becomes, the longer it takes to lose the
- 7:43next degree. [music]
- 7:45So, the first day is brutal. The second
- 7:48day is worse. But, after that, the curve
- 7:50starts to flatten. Estimates [music]
- 7:53suggest that within a week, average
- 7:55surface temperatures would fall to
- 7:57somewhere around -40°C.
- 8:00[music]
- 8:01Within a year, somewhere around -70.
- 8:05So, let's be precise about our scenario.
- 8:087 days without the sun
- 8:09>> [music]
- 8:10>> does not freeze the Earth solid. It does
- 8:12not boil off the atmosphere [music] or
- 8:15turn the oceans to ice. What it does is
- 8:18deliver the most severe [music] and
- 8:20sudden winter in the history of the
- 8:22planet. And that is more than enough.
- 8:25In the first hours, the most dangerous
- 8:28thing is not the cold. It is the
- 8:30darkness
- 8:31>> [music]
- 8:31>> arriving instantly across half the
- 8:33world. Every aircraft in flight on the
- 8:36daylight side loses visual reference
- 8:39without warning.
- 8:40>> [music]
- 8:41>> Every road suddenly has no light. Power
- 8:44grids face an immediate and catastrophic
- 8:46problem because solar generation
- 8:49vanishes worldwide in the same [music]
- 8:51second. And demand for heating and
- 8:53lighting spikes at once. Grids are
- 8:56balancing acts. A sudden massive
- 8:59imbalance triggers protective [music]
- 9:01shutdowns, and those cascade. Large
- 9:04portions of the world lose power within
- 9:07hours. Meanwhile, [music]
- 9:09the temperature is dropping by roughly a
- 9:11degree every 80 minutes. By the end of
- 9:14the first day, surviving in most of the
- 9:16world means having heat that does not
- 9:18[music] depend on the grid. Gas, wood,
- 9:22oil, anything that burns. And something
- 9:25else is happening quietly that will
- 9:27matter enormously later. Photosynthesis
- 9:31has stopped. Every plant on Earth, every
- 9:34tree, every crop, every blade of grass,
- 9:38and critically, every microscopic plant
- 9:40[music] in the ocean has stopped
- 9:42converting light into energy.
- 9:45The entire food [music] chain of this
- 9:46planet has been unplugged at the source.
- 9:50Plants do not die [music] immediately.
- 9:52Most can survive days of darkness using
- 9:55stored energy. A week of [music]
- 9:57darkness alone would not kill a mature
- 9:59tree.
- 10:01But the cold is a different matter.
- 10:03By the second day, average temperatures
- 10:05[music]
- 10:05are approaching minus 20.
- 10:08Something is now happening to the
- 10:10weather that is genuinely strange. Our
- 10:13atmosphere moves because of uneven
- 10:15heating. The equator receives more
- 10:18energy than the poles. Warm air rises,
- 10:21cold air sinks, [music] and the whole
- 10:23system churns. Every wind, every storm,
- 10:28every weather system on this planet is
- 10:30ultimately driven by sunlight. With the
- 10:33sun gone, that engine switches off. The
- 10:37existing weather does not stop instantly
- 10:39because the atmosphere still holds
- 10:41momentum, and the oceans still hold
- 10:44heat. But the temperature difference
- 10:46that drives it begins to collapse,
- 10:49>> [music]
- 10:49>> and the global circulation starts
- 10:51winding down. In many places, [music]
- 10:54the wind simply dies.
- 10:56Alongside that, something else begins.
- 11:00The oceans are [music] now far warmer
- 11:02than the air above them, and that
- 11:04difference drives enormous evaporation
- 11:06and condensation.
- 11:08Heavy snowfall would develop over
- 11:10coastal regions and [music] across the
- 11:12seas as warm ocean moisture meets
- 11:15freezing air.
- 11:17Here is where we need to be honest about
- 11:20casualties, [music]
- 11:21and the order may surprise you.
- 11:24The first things to go [music] in large
- 11:26numbers are the smallest. Phytoplankton,
- 11:29the microscopic photosynthetic life in
- 11:31the ocean surface waters are responsible
- 11:34for a huge proportion of the planet's
- 11:36oxygen production and sit at the base of
- 11:39the marine food web.
- 11:41Many have very short lifespans measured
- 11:44[music] in days.
- 11:46A week without light causes a severe
- 11:48collapse in their numbers.
- 11:50On land, most plants survive a week of
- 11:53darkness, but not necessarily a week of
- 11:55[music] extreme cold.
- 11:57Tropical plants, which have no
- 11:59adaptation to frost at all, would be
- 12:01devastated. Crops in the field would
- 12:04[music] be lost worldwide.
- 12:06Temperate and polar plants, already
- 12:09built for winter,
- 12:10>> [music]
- 12:10>> would mostly survive.
- 12:12Insects, being small and cold-blooded,
- 12:15would suffer enormously outside of
- 12:17shelter.
- 12:18Large mammals, including humans, are in
- 12:21a strange position.
- 12:23We can survive minus 40 as long as we
- 12:26[music] have insulation and heat. Our
- 12:28problem is not biology. It is
- 12:31infrastructure.
- 12:33And here is the point worth dwelling on.
- 12:36Where you are matters far more than what
- 12:39you are.
- 12:40If you are in the deep ocean, nothing
- 12:42happens.
- 12:43The abyss [music] is permanently dark
- 12:45and close to freezing already.
- 12:48Life down there, much of which depends
- 12:50on chemical energy from hydrothermal
- 12:52vents rather than sunlight,
- 12:54>> [music]
- 12:54>> would not register the event at all.
- 12:57If you are in a cave system, [music] in
- 12:59deep soil, or in a hot spring, you would
- 13:02likely be fine.
- 13:04If you are a microbe several kilometers
- 13:06underground, drawing energy from rock
- 13:08chemistry, the sun disappearing is not
- 13:11an event in your life.
- 13:13Those organisms would never know.
- 13:16>> [music]
- 13:16>> The deeper and darker your home, the
- 13:19safer you are.
- 13:20By day four, average [music]
- 13:22temperatures are falling toward minus
- 13:2430.
- 13:25The oceans are now doing something
- 13:26[music] important, and it is the reason
- 13:29the Earth does not simply freeze.
- 13:32Water has an extraordinarily high heat
- 13:34capacity. It takes an enormous amount of
- 13:37energy to change its temperature, which
- 13:40means it also releases that energy
- 13:42slowly.
- 13:43The oceans hold a vast reservoir of heat
- 13:46accumulated over a very long time, and
- 13:49they do not give it up quickly.
- 13:51Sea ice begins forming far outside its
- 13:54usual range, spreading across the
- 13:56surface [music] of seas that have never
- 13:58frozen.
- 13:59But that ice then acts as insulation,
- 14:02slowing further heat loss from the water
- 14:04below.
- 14:05So, beneath the ice, the ocean stays
- 14:08liquid and [music] relatively warm.
- 14:10Life in the water column continues, for
- 14:13now.
- 14:14On land, by day [music] six and seven,
- 14:17we are approaching minus 40 on average,
- 14:20far colder in continental interiors.
- 14:23>> [music]
- 14:23>> This is comparable to an Antarctic
- 14:25winter, except it is everywhere at once.
- 14:29Anyone still alive is alive because they
- 14:32have fuel, shelter, and [music] food
- 14:34stored indoors, and because they stopped
- 14:36relying on anything that requires
- 14:38electricity days ago.
- 14:41The night sky is still spectacular.
- 14:42[music]
- 14:44That has not changed.
- 14:46Seven days of the clearest stars ever
- 14:48seen from the surface of this planet,
- 14:51over a world that is slowly freezing
- 14:53beneath them.
- 14:55On day seven, the sun comes back, and it
- 14:58does not announce itself.
- 15:00For 8 minutes [music] and 20 seconds,
- 15:03nothing happens, because the light is
- 15:05still in [music] transit.
- 15:07The world remains dark and frozen, while
- 15:1093 million kilometers away, a star is
- 15:13already shining.
- 15:15Then dawn arrives everywhere at once, in
- 15:18the middle of whatever hour it happens
- 15:20to be, [music]
- 15:21with no warning and no horizon glow.
- 15:25The sky simply switches back on.
- 15:28It would be the single most emotional
- 15:29moment in human history.
- 15:32But the return is not gentle. [music]
- 15:35The planet is now covered in fresh snow
- 15:37and ice over an enormous area.
- 15:40And ice reflects sunlight rather [music]
- 15:42than absorbing it.
- 15:44This is called albedo.
- 15:46A bright planet absorbs less energy than
- 15:48a dark one. Which means the newly frozen
- 15:51Earth would warm back up more slowly
- 15:53than it cooled.
- 15:55At the same time, the atmosphere that
- 15:57had wound down is suddenly given energy
- 16:00again. And the temperature differences
- 16:02driving circulation are now extreme and
- 16:05chaotic.
- 16:07The restart would bring violent storms
- 16:09worldwide. Recovery to normal global
- 16:12temperatures would take weeks to months,
- 16:15not days.
- 16:16And the ecological damage would last
- 16:18[music] far longer.
- 16:20A collapsed plankton population takes
- 16:23time to rebuild. A lost global harvest
- 16:26means [music] a food crisis that
- 16:28outlives the event by a year or more.
- 16:31The week [music] of darkness ends. The
- 16:34consequences do not.
- 16:36Now the detail that makes this [music]
- 16:38scenario genuinely strange, and it has
- 16:41nothing to do with temperature.
- 16:45>> [music]
- 16:48>> When the sun reappears, its gravity has
- 16:50to travel to us as well, taking another
- 16:538 minutes to arrive.
- 16:55And when it does, Earth is in the wrong
- 16:57place, moving in the wrong direction.
- 17:01We would not simply resume our old
- 17:03orbit. We would fall into a new one, an
- 17:07[music] ellipse shaped by our position
- 17:09and velocity at that moment.
- 17:12Depending on the direction we happen
- 17:13[music] to be traveling when the sun
- 17:15vanished, that new orbit could bring us
- 17:17closer to the Sun at some points and
- 17:19further away at others.
- 17:22In other words, a week without the Sun
- 17:24>> [music]
- 17:24>> would permanently change the shape of
- 17:26our year.
- 17:28The seasons would be different. The
- 17:30length of the year would be different.
- 17:33Not catastrophically, perhaps, but
- 17:35measurably and forever.
- 17:38And we would not be alone. Every planet,
- 17:41every moon, every asteroid in the solar
- 17:45system would have done the same thing.
- 17:47Each flying off on its own tangent for a
- 17:50week before being recaptured into a new
- 17:53orbit.
- 17:54The entire solar system would be
- 17:56reshuffled and the long-term [music]
- 17:58stability of those new orbits would be
- 18:00an open question.
- 18:02The Sun returning would not restore the
- 18:04solar system. It would create a new one.
- 18:08No.
- 18:08>> [music]
- 18:09>> And the reason is worth explaining.
- 18:11Mass cannot simply vanish.
- 18:14Conservation of energy is one of the
- 18:16most thoroughly tested principles in all
- 18:18of physics and nothing in the known
- 18:21universe allows an object of 2 billion
- 18:24billion billion tons to stop existing.
- 18:28The Sun also cannot switch off. It
- 18:31shines because of nuclear fusion in its
- 18:33core, converting hydrogen into helium
- 18:36and releasing energy. And that process
- 18:39is self-regulating and remarkably
- 18:41stable.
- 18:42It has been running for around 4 and 1/2
- 18:45billion years and has roughly 5 billion
- 18:48left. And even if fusion somehow stopped
- 18:51today, the Sun [music] would not go
- 18:53dark.
- 18:55The energy generated in its core takes
- 18:57an extraordinarily long time to work its
- 19:00way to the surface [music]
- 19:01with estimates ranging from thousands to
- 19:04hundreds of thousands of years.
- 19:07The Sun would keep shining for a very
- 19:09long time on energy [music] already in
- 19:12transit.
- 19:13There is also no plausible way to remove
- 19:16its gravity. Gravity is produced by
- 19:18mass, and the mass is not going
- 19:21anywhere.
- 19:22So, the sun disappearing is not a risk.
- 19:25It is a thought experiment, and a useful
- 19:28one, because it reveals how much of our
- 19:30world is quietly held up by something 93
- 19:33million kilometers away.
- 19:36Here is what I find remarkable about
- 19:38this scenario. We tend to think of the
- 19:41sun as something that lights our days, a
- 19:44thing that rises and sets and makes the
- 19:46[music] weather pleasant.
- 19:48It is not. It is the engine that runs
- 19:51this entire planet.
- 19:54Every wind that has ever blown was
- 19:56driven by solar heating. Every ocean
- 19:59current, every storm, every rain shower,
- 20:03every plant, every animal, and every
- 20:06human being on Earth runs on energy that
- 20:09originated in that star.
- 20:12The food you ate today was sunlight a
- 20:14few months ago. The fuel in a car was
- 20:17sunlight that fell on this planet
- 20:19hundreds of millions of years ago.
- 20:22Take it away for 1 week,
- 20:24>> [music]
- 20:24>> and the planet does not explode or
- 20:26shatter. It simply stops.
- 20:29The wind drops, [music]
- 20:30the temperature falls, the food chain
- 20:33unplugs at the base, and the Earth
- 20:35drifts off in a straight line through
- 20:38the dark.
- 20:39And the most unsettling part is the
- 20:41[music] 8-minutes.
- 20:43The gap between the sun ending and us
- 20:46finding out, a window in which
- 20:48everything is already over and nothing
- 20:51has happened yet.
- 20:53>> [music]
- 20:53>> So, the next time you step outside and
- 20:55feel the warmth on your face, remember
- 20:57that it is 8-minutes old, that it
- 21:00traveled 93 million miles to reach you,
- 21:03and that it is doing far more than
- 21:06keeping you warm.
- 21:07It is holding the entire system
- 21:09together.
- 21:11Thanks for watching. If you enjoyed
- 21:14this, subscribe [music]
- 21:15and let us know in the comments which
- 21:17impossible scenario we should explore
- 21:19next.
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