쉐도잉 연습: What Would Happen If an Asteroid Hit the Ocean? - 영상으로 영어 말하기 배우기

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70 % of this planet is water, which means that if something falls out of the sky and hits us,
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the odds are overwhelmingly that it lands in the ocean rather than on land.
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Most people find that reassuring.
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The ocean feels like a cushion.
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It is deep, it is empty, and there are no cities out there to destroy.
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If a mountain of rock is going to fall on the earth,
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surely the middle of the Pacific is the best possible place for it to land.
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That instinct is completely understandable, and it is wrong in a way that took scientists a surprisingly long time to work out.
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Because water does not absorb an impact like that.
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Water does something far worse.
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It takes the energy, holds onto it and then carries it thousands of kilometers to a coastline where people actually live.
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And that is only the first of the three separate disasters an ocean impact sets in motion.
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And it is not the one that kills the most people.
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By the end of this you will understand why the ocean is not a cushion at all.
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It is a delivery system.
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Before we drop anything, we have to be honest about scale.
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Because asteroid hits the ocean covers an enormous range of outcomes, from nothing at all to the end of civilization.
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Small objects hit our atmosphere constantly.
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Every single day, tons of material from space runs into the Earth, and almost all of it burns up long before it reaches the surface.
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Those are the shooting stars you see on a clear night, and they pose no threat to anyone.
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Push the scale up to a few meters across, and you get the events that occasionally make the news.
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An object explodes in the upper atmosphere, produces a spectacular fireball, rattles some windows,
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and scatters fragments across a landscape.
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Anything landing in the ocean at that size vanishes without a single person noticing.
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The situation changes at somewhere in the region of a hundred meters.
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An object that size carries enough energy to survive the atmosphere and deliver a serious impact.
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And if it lands in water, it starts generating waves that matter.
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At around a kilometer, you are looking at a genuine global threat, regardless of where it hits.
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And at 10 to 15 kilometers, which is roughly the size of the object that ended the dinosaurs, the location almost stops mattering.
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That is not a regional disaster, that is a planetary reset.
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For most of this video, we are going to focus on the range that is actually most likely to happen in a human lifetime,
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which is the few hundred meter object, because that is where the odds and the consequences intersect most uncomfortably.
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But we will come back to the big one, because the day the dinosaurs died was an ocean impact,
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and what happened next is genuinely difficult to imagine.
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Picture a rocky object 300 meters across on a collision course with the middle of an ocean.
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It is traveling somewhere in the region of 20 kilometers per second.
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The first thing to understand is that at that speed our atmosphere barely exists.
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A hundred kilometers of air, the thing that protects every living creature on this planet, is crossed in a handful of seconds.
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The object compresses the air in front of it so violently that the air itself glows white -hot,
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and anyone within sight of the sky sees a light brighter than the sun tearing across it.
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Then it reaches the water and here is where our intuition fails us completely.
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When you imagine something falling into the sea, you probably picture a splash.
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Something enters, water parts, water closes over it, ripples spread out.
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That image is based on a lifetime of watching objects drop into water at ordinary speeds.
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At 20 km per second, water does not behave like a liquid at all.
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It does not have time to flow out of the way.
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On the time scale of the impact,
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seawater behaves more like a solid and the collision is closer to rock striking rock than to a stone hitting a pond.
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The object does not sink.
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It is.. destroyed.
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It is annihilated on contact, converting an enormous quantity of kinetic energy into heat and pressure in an instant,
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and in the process it vaporizes a colossal volume of seawater around it.
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What opens up in the ocean at that moment is not a splash.
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It is a crater in the water itself, A transient cavity that can be several kilometers across and,
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in deeper water, may reach all the way to the sea floor.
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For a brief moment, there is a hole in the ocean with steam -filled walls, and you could look down through it and see the seabed.
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The ocean, of course, does not tolerate that for long.
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The cavity begins collapsing almost immediately, and this is the moment that creates the disaster.
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Billions of tons of seawater rush inward from every direction to fill the hole.
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And all of that water arrives at the center at the same time, with nowhere left to go but up.
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It rebounds, forming an enormous column of water that rises high into the atmosphere before falling back and collapsing again.
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near the impact point we are potentially talking about waves hundreds of meters high
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now this is the point where most explanations of ocean impacts go badly wrong
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and I want to correct it carefully because the correction is actually more interesting than the myth
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The common claim is that an ocean impact produces a wall of water hundreds of meters tall
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that sweeps across the entire ocean and washes over continents.
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That version is not what the physics predicts, and it is worth understanding exactly why.
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Impact waves and earthquake tsunamis are not the same animal.
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An earthquake tsunami is generated when a long section of the seafloor, sometimes hundreds of kilometers of it, shifts vertically all at once.
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That displaces an enormous volume of water along a very long front, and it produces a wave with a very long wavelength.
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Long wavelength waves are extraordinarily efficient at crossing oceans, losing very little energy on the way,
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which is why a quake off one coast can devastate a shoreline on the far side of the world many hours later.
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An impact wave is generated by a single point and the waves it produces have much shorter wavelengths.
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Short wavelength waves lose energy far more rapidly as they spread.
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The wavefront expands outward as a growing circle and the same energy is distributed across an ever larger circumference,
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so the height falls off quickly with distance.
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So the honest picture is this.
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Close to the impact, the waves are apocalyptic and nothing survives.
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At intermediate distances, they are still catastrophic, and by the time they reach a distant continent, they may be far smaller than the myth suggests,
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though still large enough to be a serious coastal disaster.
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That sounds like good news, and up to a point it is, but there is a detail hiding in that reassurance that turns it around completely,
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and it has to do with where we choose to live.
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Here is the uncomfortable arithmetic.
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Something in the region of 40 % of humanity lives within 100 kilometers of a coast.
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The great cities of the world are overwhelmingly coastal because for the whole of human history,
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access to the sea has meant access to trade, food and travel.
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We built our civilization at the water's edge on purpose.
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That means the specific weakness of an ocean impact, its ability to convert energy into moving water,
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is aimed directly at where we keep almost half our population and a large fraction of our infrastructure.
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And there is a second problem that makes the wave heights out in the open ocean misleading.
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When a wave moves into shallow water near a coastline, it slows down and the energy it carries has to go somewhere.
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It goes upward.
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The wave grows dramatically as it approaches the shore, a process called shoaling.
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A wave that seems modest in deep water can become something entirely different when it arrives at a continental shelf.
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Local geography then makes it worse or better in ways that are extremely difficult to predict.
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A wave funneled into a narrowing bay is amplified.
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A wave arriving at a gently sloping shelf pushes much further inland.
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A map meeting a steep coastline may reflect and dissipate.
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So the real answer to how bad an ocean impact would be depends enormously on where in the ocean it lands,
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which coastlines face it, and the shape of the seabed leading up to them.
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An impact in the middle of the South Pacific and an impact in the North Atlantic are entirely different events for humanity.
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And all of that is still only the first of the three disasters.
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Because there is something else coming out of that impact site, and unlike the waves, it does not weaken with distance.
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Remember what happened in the first second.
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A colossal volume of seawater was vaporized instantly.
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That water does not disappear.
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It is thrown into the atmosphere as steam, along with pulverized rock and dust, and, if the impact reaches the sea floor,
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material excavated from the crust itself.
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An ocean impact injects an enormous quantity of water vapor into the upper atmosphere.
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Water vapor is a greenhouse gas.
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Large quantities of it high in the atmosphere can affect the planet's energy balance, and researchers studying ocean impacts have pointed out
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that this is a genuinely distinctive feature of a water strike compared to a land strike.
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There is also the question of what such an injection does to the ozone layer, which shields the surface from ultraviolet radiation.
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So you get competing effects, and the net outcome depends on the size of the impact and the specific conditions.
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The exact magnitude of all this is an area of active research rather than settled fact, And the honest position is
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that the climate consequences of a mid -sized ocean impact are less well understood than the wave effects.
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But the principle is clear.
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An ocean impact is not just a wave -making machine.
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It is also an atmospheric event, and the atmosphere does not stop at any coastline.
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And then there is the third disaster,
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which is the one that would probably kill the most people and it involves no water and no dust at all.
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Imagine the wave has come and gone.
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Imagine it struck a stretch of coastline somewhere in the world, destroying ports, cities, refineries, airports and rail links.
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Now think about what a modern civilization actually is.
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It is a network.
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Food is grown in one place and eaten thousands of kilometers away.
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Medicines are manufactured in a handful of facilities and distributed globally.
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Fuel moves by sea.
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Electronics move by sea.
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A staggering share of everything you own passed through a port at some point.
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And those ports are precisely what a tsunami destroys most efficiently.
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Modern supply chains are also optimized for efficiency rather than resilience.
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Most of what you buy is not sitting in a warehouse waiting for you.
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It is scheduled to arrive shortly before it is needed, because storage costs money.
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That system is extraordinarily efficient and extraordinarily fragile.
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Take out a cluster of major ports on one side of an ocean
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and the effects propagate through that network in ways
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that reach people who never saw the wave and live nowhere near the sea.
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Shortages appear in places that were physically untouched.
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Prices spike.
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Manufacturing stalls because a single component is no longer available.
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We have watched smaller versions of this happen in living memory,
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when a single blocked shipping route or one disrupted factory sent measurable ripples through the global economy for months.
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So the death toll from an ocean impact is not really a question about the height of a wave.
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It is a question about how well a globally interconnected civilization handles losing a section of its coastline.
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And the honest answer is that we do not know, because we have never tested it.
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Now, let us go back to the one that we know actually happened.
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66 million years ago, an object somewhere in the range of 10 to 15 km
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across across struck the earth near what is now the Yucatan Peninsula.
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That was an ocean impact.
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It landed in a shallow sea.
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At that scale, everything I have described stops being a regional disaster and becomes something else entirely.
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The waves generated were beyond anything in human experience,
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and evidence of enormous disturbance in the sediments around the Gulf region records their passage.
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But the waves were not what ended the dinosaurs, and this is the detail that matters most for understanding impact risk.
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The rock at that particular site was rich in sulfur -bearing minerals, and the impact vaporized it and threw it into the atmosphere,
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where it formed a haze that reflected sunlight away from the surface.
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Combined with soot from global wildfires and enormous quantities of dust, the result was a collapse in the sunlight reaching the ground.
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When sunlight fails, photosynthesis fails.
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And when photosynthesis fails, every food chain on the planet that depends on it comes apart from the bottom up.
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Around three -quarters of species on Earth died and every dinosaur larger than a house cat disappeared.
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So the lesson from the only large ocean impact in the record is a strange one.
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The water was not the main weapon, the atmosphere was.
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And that is worth holding on to because it means that when we assess the risk from a future impact,
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the question of what the object hits and what that material does
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when it is thrown into the sky may matter more than whether it lands on land or at sea.
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Here is the genuinely hopeful part, and it is not a small one.
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We are, as far as we know, the first species in the history of this planet with the ability to see one of these coming
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and do something about it.
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There are ongoing
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The following survey programs mapping near -earth objects and the large ones, the civilization -ending kilometer -plus objects,
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are the easiest to find because they are the brightest.
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A substantial proportion of that population has been catalogued
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and none of the known ones are on a collision course in the foreseeable future.
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Objects in the 100 to 300 meter range are much harder to spot, far more numerous and entirely capable of destroying a coastline.
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Those are the ones that could genuinely surprise us.
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That is not a complete planetary defense system, but it is a proof of concept,
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and it moves the whole problem out of the category of things we simply endure.
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The catch is time.
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Deflection works by making a very small change to an object's path a very long way in advance
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so that the tiny nudge compounds into a large miss by the time it reaches us.
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That requires years of warning, which requires finding the object first,
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which brings the entire subject back to something unglamorous.
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The single most valuable thing we can do about asteroid impacts is not build weapons.
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It is look.
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So what would happen if an asteroid hit the ocean.
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For a small object, nothing at all, and nobody would ever know.
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For something a few hundred meters across, a regional catastrophe aimed squarely at the coastlines where we have concentrated our cities,
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our ports, and nearly half of our species,
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followed by an economic disruption that would reach far inland to people who never saw a drop of the water.
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If you enjoyed this, subscribe, because we are only getting started.
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And tell us in the comments whether you think we would actually be ready.
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Watch next as we reconstruct the day the dinosaurs died, hour by hour.

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이 레슨의 어휘와 말하기 포인트

이 말하기 레슨은 영상 “What Would Happen If an Asteroid Hit the Ocean?”을(를) 바탕으로 합니다. 가장 자주 반복되는 단어는 다음과 같습니다: impact, ocean, wave, object, atmosphere. 이 영상에는 섀도잉할 문장 193개와 단어 2662개가 있습니다. 말하는 구간의 길이는 19:59입니다. 화자는 분당 약 133단어의 일정한 속도로 말해서 섀도잉하기에 편한 속도입니다. 영어에서 가장 많이 쓰이는 3,000단어에 속하는 단어가 79%뿐이라 어휘가 어려운 편입니다.

이 영상의 핵심 어휘

영상에 나오는 익혀 둘 만한 단어 15개를 발음, 뜻과 함께 정리했습니다.

단어발음뜻
atmosphere 명사/ˈætməsˌfɪɹ/대기, 대기권
disaster 명사/dɪˈzɑːs.təː/재난, 재앙
enormous 형용사/ɪˈnɔː.məs/거대하다
meter 명사/ˈmitəɹ/계량기
civilization 명사/ˌsɪv.ɪ.laɪˈzeɪ.ʃən/문명
arrive 동사/əˈɹaɪv/도착하다
quantity 명사/ˈkwɑn(t)ɪti/양, 량
dinosaur 명사/ˈdaɪnəsoɹ/공룡
dust 명사/dʌst/먼지, 흙
collision 명사/kəˈlɪʒn̩/충돌
sunlight 명사/ˈsʌnˌlaɪt/햇빛, 일광
asteroid 명사/ˈæst(ə)ɹɔɪd/소행성
efficient 형용사/ɪˈfɪʃənt/효율적인
nowhere 부사/ˈnoʊ.(h)wɛɹ/아무데도
reflect 동사/ɹɪˈflɛkt/반사(反射)하다

영상에 나오는 구동사

단어뜻
point out 동사가리키다

이 영상의 문법

화자가 가장 많이 쓰는 문형을 영상 속 실제 표현과 함께 정리했습니다.

문형영상 속 표현
수동태 be + 과거분사 — 누가 하는지보다 무슨 일이 일어나는지에 초점is crossed · is based · is annihilated
현재완료 have/has + 과거분사 — 과거의 일이 지금도 관련이 있을 때has meant · have pointed · has come
관계절 who / which + 절 — 사람이나 사물에 대한 추가 정보water, which means · kilometers, which is · people who never

주의할 발음

  • “th” 소리: earthquake /ˈɝθkweɪk/, myth /mɪθ/, wavelength /ˈweɪvˌlɛŋ(k)θ/, photosynthesis /ˌfoʊ.toʊˈsɪn.θə.sɪs/
  • “sh”와 “zh” 소리: civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, collision /kəˈlɪʒn̩/, efficient /ɪˈfɪʃənt/, shallow /ˈʃæloʊ/, shelf /ʃɛlf/
  • 긴 단어 — 강세 위치에 주의: civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, genuinely /ˈd͡ʒɛn.ju.ɪn.li/, humanity /hjuˈmænɪti/, planetary /ˈplænɪˌtɛəri/, overwhelmingly /ˌəʊ.vəˈwɛl.mɪŋ.lɪ/

한국어 화자가 어려워하는 소리:

  • /f/ — ㅍ(/p/)으로 바꾸지 말고 윗니를 아랫입술에 대기: atmosphere /ˈætməsˌfɪɹ/, efficient /ɪˈfɪʃənt/, lifetime /ˈlaɪf.taɪm/, reflect /ɹɪˈflɛkt/, handful /ˈhæn(d)fʊl/
  • /v/ — ㅂ(/b/)과 구별하기: civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, arrive /əˈɹaɪv/, cavity /ˈkæv.ɪt.i/, vapor /ˈveɪpɚ/, overwhelmingly /ˌəʊ.vəˈwɛl.mɪŋ.lɪ/
  • /z/ — ㅈ이 아니라 성대를 울리는 /s/: disaster /dɪˈzɑːs.təː/, civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, physics /ˈfɪz.ɪks/, physically /ˈfɪz.ɪ.kli/, pose /poʊz/

이 영상으로 연습하는 방법

  1. 먼저 말하지 않고 영상을 끝까지 듣고 모르는 단어를 적어 둡니다.
  2. 보통 속도로 한 문장씩 섀도잉하고, 화자의 리듬과 맞을 때까지 반복합니다.
  3. 자신의 목소리를 녹음해 원본과 비교하고, atmosphere, disaster, enormous 같은 단어에 특히 주의합니다.

쉐도잉이란? 영어 실력을 빠르게 키우는 과학적 방법

쉐도잉(Shadowing)은 원래 전문 통역사 훈련을 위해 개발된 언어 학습 기법으로, 다언어 학자인 Dr. Alexander Arguelles에 의해 대중화된 방법입니다. 핵심 원리는 간단하지만 매우 강력합니다: 원어민의 영어를 들으면서 1~2초의 짧은 지연으로 즉시 소리 내어 따라 말하는 것——마치 '그림자(shadow)'처럼 화자를 따라가는 것입니다. 문법 공부나 수동적인 청취와 달리, 쉐도잉은 뇌와 입 근육이 동시에 실시간으로 영어를 처리하고 재현하도록 훈련합니다. 연구에 따르면 이 방법은 발음 정확도, 억양, 리듬, 연음, 청취력, 말하기 유창성을 크게 향상시킵니다. IELTS 스피킹 준비와 자연스러운 영어 소통을 원하는 분들에게 특히 효과적입니다.

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