WEBVTT - Natural Risks

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<v Speaker 1>Existential risks aren't new to us. Ever since our species

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<v Speaker 1>was born. There have always been lots of catastrophes ready

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<v Speaker 1>and waiting to wipe the human race off the face

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<v Speaker 1>of the earth. It's just that these risks are of

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<v Speaker 1>our own making. The history of humanity is relatively brief,

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<v Speaker 1>and we've been fortunate to have come along during a

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<v Speaker 1>period of relative calm in Earth's history. Maybe we couldn't

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<v Speaker 1>have come along had things been more tumultuous. Who knows,

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<v Speaker 1>but there's something to bear in mind that pops up

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<v Speaker 1>a lot when you look into existential threats. Whatever lessons

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<v Speaker 1>the past may offer, it doesn't teach us enough about

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<v Speaker 1>the future. Just because things have gone smoothly so far

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<v Speaker 1>doesn't mean they will always go that way. Every so often,

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<v Speaker 1>some massive catastrophe happens on Earth that brings life to

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<v Speaker 1>the brink of extinction. There are a lot of things

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<v Speaker 1>in space and on Earth that can devastate life. We

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<v Speaker 1>call these natural existential risks. It's worth noting that we

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<v Speaker 1>humans pose an existential threat to just about every other

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<v Speaker 1>species that we share the planet with, but there are

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<v Speaker 1>also natural catastrophes that pose a threat to all of us.

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<v Speaker 1>Creatures living on Earth, including us humans. In this episode,

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<v Speaker 1>we'll look at a few of them to get a

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<v Speaker 1>feel for just how badly things can go on Earth.

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<v Speaker 1>Let's travel back to one particular day during the most

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<v Speaker 1>strictan age of the Upper Cretaceous period, about sixty six

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<v Speaker 1>million years ago, give or take three hundred thousand years,

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<v Speaker 1>and on this day, a light streaks across the sky

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<v Speaker 1>above Earth. That light, it turns out, is an asteroid,

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<v Speaker 1>six miles across, about the size of downtown Los Angeles,

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<v Speaker 1>is traveling at about forty four thousand miles per hour,

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<v Speaker 1>times faster than a bullet when it passes through the

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<v Speaker 1>Earth's atmosphere as if it's not even there, and strikes

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<v Speaker 1>the planet. The impact creates a blast with one hundred

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<v Speaker 1>million megatons of energy. For comparison, the Czar BOMBA, the

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<v Speaker 1>largest nuclear bomb that humans have ever detonated, was fifty megatons.

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<v Speaker 1>One got past Jupiter, you could say. The asteroid strikes

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<v Speaker 1>the Earth along what is now called the Yucatan, the

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<v Speaker 1>spur like peninsula that juts out of southern Mexico into

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<v Speaker 1>the Gulf. It drives itself into the Earth, digging out

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<v Speaker 1>a crater a hundred and ten miles in diameter and

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<v Speaker 1>nine miles deep, so deep, in fact, it nearly punctures

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<v Speaker 1>a hole all the way through the crust. The impact

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<v Speaker 1>is felt all over the world as enormous shocks of

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<v Speaker 1>energy that travel along the borders between tectonic plates. This

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<v Speaker 1>sets off earthquakes and volcanoes across Earth unimaginably large tsunamis

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<v Speaker 1>from the Gulf of Mexico Wash as far north as St. Louis.

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<v Speaker 1>The impact kicks a tremendous amount of earth and sea

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<v Speaker 1>into the air. Boulders the size of cars are launched

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<v Speaker 1>hundreds of miles from the impact site, as far away

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<v Speaker 1>as Believes. The pressure and heat from the collision is

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<v Speaker 1>so great that it instantly melts the rocky earth below.

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<v Speaker 1>That melted rock sprays into the air, where it turns

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<v Speaker 1>to glass before it can reach the ground. Continents away.

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<v Speaker 1>Quartz is pressed into crazy angles, and minerals into tiny

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<v Speaker 1>spheres of metal, And when the heavier bits among all

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<v Speaker 1>that kicked up dirt and rock and metal come back down,

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<v Speaker 1>it heats up. It brings a tremendous amount of energy

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<v Speaker 1>with it, flash heating the Earth's surface, embroiling alive anything

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<v Speaker 1>that can't take cover underground or underwater. And as the

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<v Speaker 1>earthquakes and tsunamis raging across the Earth and the fire

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<v Speaker 1>raining from the sky begin to subside, things go from

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<v Speaker 1>bad to worse. The finer particles from all that pulverized

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<v Speaker 1>earth and liquefied rock launched into space stay aloft, forming

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<v Speaker 1>a vast globe spanning shroud that blocks out the Sun

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<v Speaker 1>for months. Photosynthesis grants to a halt back on Earth.

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<v Speaker 1>The world's plants can no longer make their food, and

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<v Speaker 1>since they, in one way or another, feed the rest

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<v Speaker 1>of life on Earth, everything is still alive begins to starve.

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<v Speaker 1>But as bad as the asteroid makes things for life

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<v Speaker 1>on Earth, it is made even worse by a fluke,

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<v Speaker 1>a stroke of sheer bad luck. The Yucatan, the area

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<v Speaker 1>where the asteroid strikes, is one of the most sulfur

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<v Speaker 1>rich areas on Earth, and when that asteroid hit, as

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<v Speaker 1>much as five hundred billion metric tons of sulfur instantly

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<v Speaker 1>rose from deep inside the Earth up into the atmosphere,

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<v Speaker 1>like dust rising from a table when a heavy book

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<v Speaker 1>is dropped on it. In the sky, that sulfur mixes

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<v Speaker 1>with water vapor and is bombarded by ultra violet radiation

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<v Speaker 1>from the sun, so it becomes sulfur aerosol, the type

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<v Speaker 1>of atmospheric pollution that just happens to be the most

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<v Speaker 1>efficient at absorbing sunlight and blocking it from reaching the Earth.

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<v Speaker 1>The sudden presence of aerosols in the sky makes the

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<v Speaker 1>darkness complete. Sulfur aerosols also form acid rain and freshwater

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<v Speaker 1>lakes and the surface of the oceans are poisoned by it.

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<v Speaker 1>Life on Earth comes disturbingly close to total extinction. Millions

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<v Speaker 1>of years later, humans will call this cataclysmic event the

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<v Speaker 1>Cretaceous Tertiary extinction. It had such a profoundly colossal effect

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<v Speaker 1>on the planet that it serves as the sudden and

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<v Speaker 1>abrupt dividing line between one geological age, the Cretaceous, and

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<v Speaker 1>the one that followed it, the Tertiary or Paleogene, as

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<v Speaker 1>it's called these days. Around of the species alive on

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<v Speaker 1>Earth at the time died during the event and the

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<v Speaker 1>hard times that followed the asteroid's arrival. Three out of

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<v Speaker 1>four species death swept across Earth and waves that lasted

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<v Speaker 1>for tens of thousands of years. Those species that did

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<v Speaker 1>manage to survive had an extremely hard time of it.

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<v Speaker 1>They hung on by a thread. In many cases, they

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<v Speaker 1>were whittled down to just a few individuals that were

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<v Speaker 1>somehow able to carry on their species. Animals that were

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<v Speaker 1>able to burrow to feed off the carcasses of the

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<v Speaker 1>unlucky ones, and whatever plants still reached upward towards a

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<v Speaker 1>sun that no longer shown. Those are the ancestors of

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<v Speaker 1>everything alive on Earth today. We are descended from the

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<v Speaker 1>toughest band of animals that ever lived. But for most

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<v Speaker 1>species of dinosaurs, the asteroid was the end of the line,

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<v Speaker 1>the Kuda grass. They succumbed to their existential threat. We

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<v Speaker 1>know all of this thanks to a father's son science

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<v Speaker 1>team known as Luis and Walter Alvarez. As a geologist

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<v Speaker 1>working in Italy in the seventies, Walter Alvarez found a

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<v Speaker 1>thin layer of clay dating back to around sixty five

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<v Speaker 1>million years before. It was peculiar because immediately below the

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<v Speaker 1>strip of clay there was a wide variety of fossils

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<v Speaker 1>of different types of forums, tiny single celled organisms that

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<v Speaker 1>have shells, but right above the clay there was only

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<v Speaker 1>one type. Forums are an excellent indicator species They eat

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<v Speaker 1>plants and animals that degrade on the seafloor, and they

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<v Speaker 1>are very sensitive to changes in the environment. If something

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<v Speaker 1>happens to forums, it means that something happened to everything else,

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<v Speaker 1>and something definitely did seem to have happened to the

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<v Speaker 1>forums around the time that clay strip was deposited that

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<v Speaker 1>drastically reduced their diversity. There was something similar among plants too.

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<v Speaker 1>Just below the clay strip were fossils of a wide

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<v Speaker 1>variety of plants, where just above there were only fern spores.

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<v Speaker 1>Walter would have been surprised to know that the strip

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<v Speaker 1>of clay he was scraping at with his trowel in

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<v Speaker 1>the center of Italy was actually from Mexico. Walter had

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<v Speaker 1>a very famous scientist, Dad Louise, a physicist who developed

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<v Speaker 1>the first atomic bombs for the US, among many other things.

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<v Speaker 1>By the late seventies. When Walter approached his father with

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<v Speaker 1>the curious find of the clay strip, Louise worked at

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<v Speaker 1>one of the national labs where he had some colleagues

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<v Speaker 1>who ran a mess spectrometer. He asked them to take

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<v Speaker 1>a look at the samples of the clay layer. What

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<v Speaker 1>they found was surprising the clay layer contained about six

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<v Speaker 1>hundred times more iridium than the layer above or below

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<v Speaker 1>the clay. This is very weird because i ridium, which

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<v Speaker 1>is a metal in the platinum family, isn't found much

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<v Speaker 1>in Earth's crust. It certainly isn't found at six hundred

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<v Speaker 1>times the background amount. It is, however, found in abundance

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<v Speaker 1>on things like asteroids. As Walter started looking around the world,

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<v Speaker 1>he found that same clay layer at other sites, and

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<v Speaker 1>it had all the same characteristics as the first site

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<v Speaker 1>in Italy. Iridium in aces in abrupt shift in diversity.

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<v Speaker 1>By that time, paleontologists had already established that the dinosaurs

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<v Speaker 1>had died out around sixty five or so million years earlier.

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<v Speaker 1>The clay layers geological age matched that extinction precisely, But

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<v Speaker 1>at the time, the prevailing theory was that it had

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<v Speaker 1>been a million year period of volcanic activity that had

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<v Speaker 1>been responsible for killing off the dinosaurs, all that gas

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<v Speaker 1>erupting and poisoning the air and rain. But what the

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<v Speaker 1>Alvarez Boys were seeing suggested an asteroid, a colossal one,

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<v Speaker 1>one so colossal it had brought the Earth to the

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<v Speaker 1>brink of near total extinction, and in their theory got

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<v Speaker 1>a shot in the arm with the discovery of the

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<v Speaker 1>chick s Aloub Crater on the Yukatamp Peninsula, the site

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<v Speaker 1>of the destruction sixty six million years before. Eventually, the

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<v Speaker 1>debate was laid to rest. In two thousand ten forty

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<v Speaker 1>one scientists and fields like paleontology, astronomy, geology, and others

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<v Speaker 1>released a review of the literature on the KT extinction

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<v Speaker 1>in the astro evidence and concluded that it was in

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<v Speaker 1>fact an asteroid that killed off the dinosaurs. It's as

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<v Speaker 1>close as science comes to being settled. There's something that

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<v Speaker 1>gets overshadowed by the story of the dinosaurs extinction. That

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<v Speaker 1>life on Earth rebounded. Those smaller animals that could burrow

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<v Speaker 1>and dive held fast and among all the darkness and death,

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<v Speaker 1>they continued on. They reproduced and raised their young, and

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<v Speaker 1>as the Earth slowly shook off that extraordinarily bad day,

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<v Speaker 1>it became again a fertile place, a place friendly to life,

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<v Speaker 1>and that bottle that created by the asteroid open wide,

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<v Speaker 1>and life spread again and grew diverse. And from that

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<v Speaker 1>calamity we humans arose amid the vacuum left by the

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<v Speaker 1>sudden loss of life. The dinosaurs existential catastrophe proved to

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<v Speaker 1>be our existential triumph, which is to say that life

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<v Speaker 1>is tough and it is very, very difficult to extinguish

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<v Speaker 1>it entirely in the coming centuries. That will be a

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<v Speaker 1>mark in its favor. M hm hm. We humans are

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<v Speaker 1>an earth bound species, and so whatever happens to Earth

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<v Speaker 1>happens to us. Like the dinosaurs, we live under the

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<v Speaker 1>threat of death from huge rocks traveling at unimaginable speeds

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<v Speaker 1>hurtling toward us. But unlike the dinosaurs, we are in

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<v Speaker 1>a position to do something about it. In the coming years.

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<v Speaker 1>Is our technology to travel through space develops and we

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<v Speaker 1>become capable of spreading out around our solar system and

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<v Speaker 1>eventually our galaxy, we will have made the biggest shift

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<v Speaker 1>in our species since at least when we settled down

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<v Speaker 1>and began raising crops. That see change in human ecology.

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<v Speaker 1>The advent of agriculture led to sweeping changes for humans.

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<v Speaker 1>It was, as Nick Bostrom would put it, a pan

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<v Speaker 1>generational change in how humans lived. By coaxing food from

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<v Speaker 1>the ground on a predictable schedule, and by taming animals

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<v Speaker 1>and creating a reliable supply of meat and milk. We

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<v Speaker 1>changed a lot about ourselves, our bones, the shapes of

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<v Speaker 1>our skulls, the workings of our guts, the color of

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<v Speaker 1>our skin. And it changed our culture too. As anthropologist

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<v Speaker 1>Jared Diamond points out in his nine seven essay The

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<v Speaker 1>Worst Mistake in the History of the Human Race, about

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<v Speaker 1>the advent of agriculture, we started to have a surplus

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<v Speaker 1>of food, something that our hunter gatherer ancestors never would

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<v Speaker 1>have experienced. This meant that some people had more than others,

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<v Speaker 1>which creates an imbalance and power, and hence agriculture also

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<v Speaker 1>led to things like kings and armies and social classes.

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<v Speaker 1>When we settled down our cities developed. Agriculture can support

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<v Speaker 1>more people than hunting and gathering, and the more people

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<v Speaker 1>there are, the more brilliant ideas there are too, so

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<v Speaker 1>our civilization began to advance by leaps and bounds in

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<v Speaker 1>the last nine or ten thousand years. Ideas spread more

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<v Speaker 1>quickly among those people who lived together in those new cities,

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<v Speaker 1>so innovations were able to develop over the span of

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<v Speaker 1>a handful of years rather than millennia. Almost everything we

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<v Speaker 1>have in the world today can be traced back to

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<v Speaker 1>our collective decision to settle down and raise crops. It was,

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<v Speaker 1>to say the least, a sweeping change for us humans.

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<v Speaker 1>With our next great leap spreading out into space, we

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<v Speaker 1>are effectively doing the opposite of when we settled down

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<v Speaker 1>into cities. Rather than contracting, we will be expanding from

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<v Speaker 1>that huge coming together, we will spread out. Over time,

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<v Speaker 1>humans will begin to colonize other planets, and generations of

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<v Speaker 1>little human babies will be borne on planets other than Earth.

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<v Speaker 1>They will be shaped by forces and experiences that no

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<v Speaker 1>earth bound human will have ever encountered, and they will

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<v Speaker 1>learn to adapt to their home planet just like we did.

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<v Speaker 1>We are quite capable of becoming all the things that

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<v Speaker 1>it's possible to become. Life that starts from us and

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<v Speaker 1>radiates out can not only spread to different places, it

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<v Speaker 1>can create different styles and techniques and cultures and approaches.

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<v Speaker 1>All of the life that you see on Earth started

0:14:17.240 --> 0:14:19.800
<v Speaker 1>out from a much smaller amount of variation, but with

0:14:19.880 --> 0:14:23.120
<v Speaker 1>time it could explore lots of different niches and ways

0:14:23.120 --> 0:14:26.760
<v Speaker 1>of living. And that's probably what would happen to us too.

0:14:26.800 --> 0:14:29.400
<v Speaker 1>If we're the only life around it, we can survive,

0:14:30.040 --> 0:14:33.880
<v Speaker 1>We will radiate, We will become diverse and different and

0:14:33.960 --> 0:14:38.320
<v Speaker 1>fill thousand million billion different niches of different ways of being.

0:14:38.920 --> 0:14:41.760
<v Speaker 1>Over time, perhaps their physical connection to humans on Earth

0:14:41.800 --> 0:14:45.520
<v Speaker 1>will become distant enough that new species of humans will form,

0:14:45.560 --> 0:14:47.360
<v Speaker 1>and the universe will be home to more than one

0:14:47.400 --> 0:14:51.160
<v Speaker 1>species of human again, just as it was fifty years ago.

0:14:52.080 --> 0:14:55.680
<v Speaker 1>We will become the aliens we seek, and later on

0:14:56.480 --> 0:14:58.600
<v Speaker 1>they might be surprised to learn that they came from

0:14:58.640 --> 0:15:02.240
<v Speaker 1>something that was simple and not as very It's odd

0:15:02.240 --> 0:15:05.680
<v Speaker 1>to think of, but humans are in an evolutionary bottleneck

0:15:05.760 --> 0:15:09.360
<v Speaker 1>of our own. Right now. There's only one species of us,

0:15:09.840 --> 0:15:12.480
<v Speaker 1>and with the exception of maybe half a dozen astronauts

0:15:12.520 --> 0:15:15.760
<v Speaker 1>on the International Space Station at any given time, we

0:15:15.840 --> 0:15:20.600
<v Speaker 1>are all stranded on this island Earth. Those astronauts aboard

0:15:20.600 --> 0:15:23.400
<v Speaker 1>the I s S showed just the faintest beginnings of

0:15:23.440 --> 0:15:27.440
<v Speaker 1>our future. If we become a space faring species, all

0:15:27.480 --> 0:15:30.400
<v Speaker 1>of humanities eggs will no longer be in just the

0:15:30.480 --> 0:15:34.360
<v Speaker 1>one basket of Earth. Should some catastrophe befall those of

0:15:34.440 --> 0:15:37.360
<v Speaker 1>us here on Earth, there will be other humans living

0:15:37.400 --> 0:15:40.920
<v Speaker 1>elsewhere to carry on. We will begin to trickle from

0:15:40.920 --> 0:15:44.400
<v Speaker 1>our bottle neck and spread throughout the universe, and when

0:15:44.400 --> 0:15:47.480
<v Speaker 1>we do, we will have made it through the Great Filter.

0:15:48.840 --> 0:15:51.680
<v Speaker 1>Colonizing beyond Earth is something we should begin working on

0:15:51.960 --> 0:15:55.160
<v Speaker 1>as soon as we can, because Earth is vulnerable to

0:15:55.280 --> 0:15:59.280
<v Speaker 1>a wide variety of catastrophes that are pretty hostile to life,

0:16:00.080 --> 0:16:04.000
<v Speaker 1>things like exploding stars, the death of our Sun, even

0:16:04.080 --> 0:16:08.400
<v Speaker 1>Earth's zone systems going haywire. Take our son for starters.

0:16:09.080 --> 0:16:12.800
<v Speaker 1>Remember that Goldilocks zone, that habitable area around a star

0:16:12.880 --> 0:16:15.840
<v Speaker 1>where a planet can sustain life. Earth is in the

0:16:15.880 --> 0:16:20.320
<v Speaker 1>Sun's Goldilocks zone, but it's not a permanent position as

0:16:20.320 --> 0:16:23.120
<v Speaker 1>a star. The Sun is currently in its main sequence.

0:16:23.760 --> 0:16:26.120
<v Speaker 1>It has plenty of hydrogen atoms in its core that

0:16:26.160 --> 0:16:29.960
<v Speaker 1>it fuses into helium, and these constant nuclear reactions release

0:16:30.040 --> 0:16:33.560
<v Speaker 1>tremendous amounts of energy, which we gratefully accept as light

0:16:33.640 --> 0:16:37.120
<v Speaker 1>and heat here on Earth. But the Sun is slowly

0:16:37.200 --> 0:16:40.640
<v Speaker 1>using up its available fuel, and as it does, its

0:16:40.720 --> 0:16:44.920
<v Speaker 1>core shrinks in size. That smaller core means that it's

0:16:44.960 --> 0:16:47.680
<v Speaker 1>closer to the center of the Sun, which means that

0:16:47.720 --> 0:16:51.640
<v Speaker 1>gravity exerts more force on it, making it denser. All

0:16:51.680 --> 0:16:54.480
<v Speaker 1>of this is what one would expect, but we're talking

0:16:54.480 --> 0:16:57.680
<v Speaker 1>about cosmic stuff here, and as with all cosmic stuff,

0:16:57.960 --> 0:17:02.360
<v Speaker 1>something weird always happens to because the core grows denser

0:17:02.400 --> 0:17:05.199
<v Speaker 1>as it grows smaller. That means more fuel is closer

0:17:05.240 --> 0:17:07.640
<v Speaker 1>at hand for the Sun to burn, so its main

0:17:07.680 --> 0:17:11.280
<v Speaker 1>sequence begins to speed up. It uses fuel more quickly,

0:17:11.640 --> 0:17:14.879
<v Speaker 1>actually shortening its own lifespan, at least compared to what

0:17:14.920 --> 0:17:17.040
<v Speaker 1>it would be if it managed to maintain a slow,

0:17:17.080 --> 0:17:20.879
<v Speaker 1>steady burn during its entire life. As the Sun burns

0:17:20.920 --> 0:17:23.840
<v Speaker 1>through its fuel supply more quickly, it's actually going to

0:17:23.880 --> 0:17:28.240
<v Speaker 1>grow larger, much much larger, and about one point one

0:17:28.280 --> 0:17:30.399
<v Speaker 1>billion years, the Earth will no longer be in the

0:17:30.400 --> 0:17:34.240
<v Speaker 1>Sun's goldilocks song. It will be a lot closer, and

0:17:34.320 --> 0:17:38.240
<v Speaker 1>it will keep getting closer from there. This is estrophysicist

0:17:38.280 --> 0:17:41.600
<v Speaker 1>Ian O'Neill. When it goes through this end stage, when

0:17:41.640 --> 0:17:43.639
<v Speaker 1>it starts to turn, is what's called a red giant,

0:17:43.840 --> 0:17:46.280
<v Speaker 1>and it's pretty much a red giant is pretty descriptive.

0:17:46.280 --> 0:17:49.200
<v Speaker 1>A boy, what's going to be. It will expand, possibly

0:17:49.280 --> 0:17:52.080
<v Speaker 1>out to the orbit of Earth. So this the Sun

0:17:52.119 --> 0:17:55.879
<v Speaker 1>will basically fill up our entire, our entire sky. You

0:17:55.880 --> 0:17:57.639
<v Speaker 1>look out the window, it will just be a big

0:17:58.720 --> 0:18:02.439
<v Speaker 1>seething mess of of star. So you can imagine that

0:18:02.480 --> 0:18:04.520
<v Speaker 1>with the Sun right on top of Earth, there won't

0:18:04.520 --> 0:18:07.879
<v Speaker 1>be much room for life, but billions of years before

0:18:07.920 --> 0:18:10.280
<v Speaker 1>that point, the biggest issue will have to deal with

0:18:10.440 --> 0:18:14.040
<v Speaker 1>is the increase in solar radiation. Sure, things will get

0:18:14.119 --> 0:18:17.080
<v Speaker 1>much much hotter on Earth than they are today, but

0:18:17.160 --> 0:18:20.040
<v Speaker 1>as with the fallout from the kt asteroid, there are

0:18:20.040 --> 0:18:25.440
<v Speaker 1>places that some life could go underground, deep underwater. Sorry cows,

0:18:25.720 --> 0:18:29.920
<v Speaker 1>sorry elephants, sorry feral pigs. Sure, but as we've seen,

0:18:30.000 --> 0:18:33.120
<v Speaker 1>life is persistent. If anything, it would almost certainly find

0:18:33.119 --> 0:18:35.440
<v Speaker 1>a way to adapt to the changes from the increased

0:18:35.480 --> 0:18:40.200
<v Speaker 1>heat on Earth, at least at first. But the radiation

0:18:40.320 --> 0:18:42.960
<v Speaker 1>from the growing Sun will be so intense that it

0:18:42.960 --> 0:18:46.320
<v Speaker 1>will tear apart the very molecules that make up Earth's atmosphere.

0:18:47.000 --> 0:18:51.480
<v Speaker 1>All aerobic life. Life that breathes oxygen would die, obviously,

0:18:52.000 --> 0:18:55.200
<v Speaker 1>but even anaerobic life would find it impossible to continue

0:18:55.200 --> 0:18:59.119
<v Speaker 1>on Earth without an atmosphere to regulate temperatures. The wild

0:18:59.160 --> 0:19:02.320
<v Speaker 1>swings between tense heat and cold on a daily basis

0:19:02.480 --> 0:19:06.080
<v Speaker 1>would evaporate the oceans, leaving Earth a dead, lifeless rock.

0:19:06.840 --> 0:19:11.280
<v Speaker 1>A planet without an atmosphere is a dead planet. So

0:19:11.320 --> 0:19:13.640
<v Speaker 1>we have a billion years to figure out either how

0:19:13.680 --> 0:19:16.480
<v Speaker 1>to slow the Sun's burn right and vastly extend its

0:19:16.480 --> 0:19:19.919
<v Speaker 1>main sequence, or how to live away from Earth, and

0:19:20.000 --> 0:19:22.399
<v Speaker 1>the odds aren't that bad actually that we may be

0:19:22.480 --> 0:19:28.040
<v Speaker 1>able to do both within that time. That same issue,

0:19:28.240 --> 0:19:31.080
<v Speaker 1>a star reaching the end of its productive life poses

0:19:31.119 --> 0:19:34.439
<v Speaker 1>another natural threat to Earth as well. Depending on the

0:19:34.600 --> 0:19:38.159
<v Speaker 1>size or the type of the star, could explode at

0:19:38.200 --> 0:19:42.320
<v Speaker 1>the end of its life. As a star nears the

0:19:42.440 --> 0:19:44.880
<v Speaker 1>end of its life and its fuel core becomes denser

0:19:44.880 --> 0:19:47.880
<v Speaker 1>and denser, the force of gravity acts ever more strongly

0:19:47.960 --> 0:19:50.280
<v Speaker 1>on it, and just the same way as the singularity

0:19:50.280 --> 0:19:53.280
<v Speaker 1>of a black hole. But a black hole singularity is

0:19:53.320 --> 0:19:56.240
<v Speaker 1>so massive and so dense that the force of gravity

0:19:56.280 --> 0:19:59.159
<v Speaker 1>acting on it actually presses it into the fabric of

0:19:59.160 --> 0:20:03.400
<v Speaker 1>space time, creating a bottomless depression. Not all stars are

0:20:03.440 --> 0:20:06.560
<v Speaker 1>as massive as this, though, so there are other outcomes

0:20:06.560 --> 0:20:08.919
<v Speaker 1>that it can have within a black hole. One of

0:20:08.920 --> 0:20:13.680
<v Speaker 1>those is a supernova. Over the star's lifespan, the nuclear

0:20:13.720 --> 0:20:17.520
<v Speaker 1>fusion reactions that carried out left behind his byproducts increasingly

0:20:17.600 --> 0:20:22.560
<v Speaker 1>heavier elements hydrogen fused into helium, helium fused into oxygen,

0:20:22.760 --> 0:20:26.360
<v Speaker 1>oxygen fused into neon, and so on, until the elements

0:20:26.400 --> 0:20:28.399
<v Speaker 1>the star burned towards the end of its life become

0:20:28.480 --> 0:20:32.359
<v Speaker 1>heavy metals like iron and nickel, so eventually it will

0:20:32.400 --> 0:20:34.480
<v Speaker 1>start to try and burn elements as big as a

0:20:34.720 --> 0:20:39.359
<v Speaker 1>iron and any star the stars to try to fuse

0:20:39.520 --> 0:20:43.240
<v Speaker 1>iron is basically on this deathbed. The force that holds

0:20:43.280 --> 0:20:45.800
<v Speaker 1>the nuclei of these types of atoms together is so

0:20:45.840 --> 0:20:49.399
<v Speaker 1>strong that they can't be fused together even by something

0:20:49.440 --> 0:20:52.800
<v Speaker 1>like a star. But the force that gravity exerts on

0:20:52.840 --> 0:20:56.240
<v Speaker 1>this extraordinarily dense core of iron and nickel is strong

0:20:56.400 --> 0:21:00.760
<v Speaker 1>enough that it actually compresses the individual atoms, pushing them

0:21:00.760 --> 0:21:04.159
<v Speaker 1>into tight, tiny balls. When the atoms that make up

0:21:04.200 --> 0:21:07.960
<v Speaker 1>the core shrink, the core itself does as well, becoming denser,

0:21:08.359 --> 0:21:10.800
<v Speaker 1>and so the force of gravity acts even more strongly

0:21:10.840 --> 0:21:14.119
<v Speaker 1>on it, creating a feedback loop. The star's core, in

0:21:14.119 --> 0:21:17.679
<v Speaker 1>other words, suddenly collapses. And all of this happens in

0:21:17.720 --> 0:21:20.879
<v Speaker 1>the fraction of a second. So is this weird point

0:21:20.920 --> 0:21:25.960
<v Speaker 1>where as soon as you hit iron, almost immediately within milliseconds,

0:21:26.000 --> 0:21:29.760
<v Speaker 1>the star just fulls apart. It just the whole system

0:21:29.760 --> 0:21:32.919
<v Speaker 1>in this core breaks down and it will undergo a

0:21:32.960 --> 0:21:36.119
<v Speaker 1>core collapse. But since the star isn't massive enough to

0:21:36.160 --> 0:21:38.480
<v Speaker 1>become a black hole, since one of the laws of

0:21:38.480 --> 0:21:41.199
<v Speaker 1>physics is that matter cannot occupy the same space at

0:21:41.200 --> 0:21:44.040
<v Speaker 1>the same time. There's a limit to how tightly packed

0:21:44.040 --> 0:21:47.080
<v Speaker 1>the iron atoms at the star's core can become. When

0:21:47.160 --> 0:21:50.480
<v Speaker 1>they reached that limit, the collapse suddenly stops, kind of

0:21:50.520 --> 0:21:53.359
<v Speaker 1>like hitting a brick wall. All that force of the

0:21:53.400 --> 0:21:56.800
<v Speaker 1>collapsing core has to go somewhere, though, and it reverberates

0:21:56.840 --> 0:22:00.520
<v Speaker 1>back outward. Exploding in a supernova one of the most

0:22:00.560 --> 0:22:04.560
<v Speaker 1>fantastic displays in the universe. All of the mass that

0:22:04.720 --> 0:22:08.000
<v Speaker 1>star sheds is shot outward as energy, so much in fact,

0:22:08.240 --> 0:22:11.400
<v Speaker 1>that planets that orbited the star just moments before may

0:22:11.400 --> 0:22:14.479
<v Speaker 1>be blown out of their solar system into space if

0:22:14.480 --> 0:22:18.920
<v Speaker 1>they're not outright destroyed. That is, tremendous amounts of light

0:22:18.960 --> 0:22:21.879
<v Speaker 1>and heat are released. For a few minutes, the dying

0:22:21.920 --> 0:22:25.360
<v Speaker 1>star can shine brighter than the combined luminosity of an

0:22:25.520 --> 0:22:29.879
<v Speaker 1>entire galaxy. The explosion since tremendous amounts of heat and

0:22:30.000 --> 0:22:34.960
<v Speaker 1>radiation spewing into space, bathing anything nearby with The only

0:22:35.000 --> 0:22:38.840
<v Speaker 1>explosion in our universe larger than a supernova was the

0:22:38.880 --> 0:22:44.560
<v Speaker 1>Big Bang. Sometimes, if the supernova is large enough, it

0:22:44.600 --> 0:22:48.119
<v Speaker 1>can emit a gamma ray burst. Gamma radiation is the

0:22:48.160 --> 0:22:52.480
<v Speaker 1>most energetic type of radiation on the electromagnetic spectrum. Gamma

0:22:52.560 --> 0:22:55.359
<v Speaker 1>rays are so energetic that they excite any atom they

0:22:55.400 --> 0:22:58.520
<v Speaker 1>come in contact with, causing the atom to move temporarily

0:22:58.560 --> 0:23:01.680
<v Speaker 1>to its higher energy state, causing its a release energy

0:23:01.720 --> 0:23:04.520
<v Speaker 1>itself as it moves back to its normal ground state.

0:23:05.440 --> 0:23:08.199
<v Speaker 1>It's like gamma rays get everybody else wound up, and

0:23:08.240 --> 0:23:11.080
<v Speaker 1>to calm down, everyone has to let out a little shout.

0:23:12.840 --> 0:23:16.080
<v Speaker 1>Just thinking about this happening to an individual atom sounds

0:23:16.119 --> 0:23:19.080
<v Speaker 1>like chaos. So you can imagine what a burst big

0:23:19.200 --> 0:23:22.520
<v Speaker 1>enough to flood an entire planet with gamma radiation might be. Like,

0:23:24.200 --> 0:23:27.000
<v Speaker 1>let's say, for argument's sake, that Earth just happens to

0:23:27.000 --> 0:23:29.480
<v Speaker 1>be in the path of that beam of energy. A

0:23:29.560 --> 0:23:32.480
<v Speaker 1>sudden flood of gamma radiation would burn those of us

0:23:32.480 --> 0:23:35.639
<v Speaker 1>walking around on Earth's surface to a crisp Sadly, we

0:23:35.640 --> 0:23:40.280
<v Speaker 1>would probably not all be transformed into incredible hulks. The

0:23:40.359 --> 0:23:42.840
<v Speaker 1>life that did manage to survive the initial burst would

0:23:42.840 --> 0:23:46.000
<v Speaker 1>have a rough time of it afterward. Gamma radiation is

0:23:46.040 --> 0:23:49.800
<v Speaker 1>particularly good at burning away the ozone layer, the protective

0:23:49.800 --> 0:23:52.560
<v Speaker 1>blanket of O three atoms that reflects most of the

0:23:52.560 --> 0:23:56.680
<v Speaker 1>Sun's radiation. When flooded with energetic gamma rays, those O

0:23:56.880 --> 0:24:00.920
<v Speaker 1>three molecules would destabilize and the ozone layer would deteriorate,

0:24:01.320 --> 0:24:04.240
<v Speaker 1>leaving Earth exposed to the full brunt of ultra violet

0:24:04.359 --> 0:24:07.760
<v Speaker 1>radiation from the Sun. UV from the Sun could be

0:24:07.760 --> 0:24:11.040
<v Speaker 1>bad enough with the folows on layer, without it, it

0:24:11.040 --> 0:24:15.000
<v Speaker 1>would be utterly catastrophic. The intensity of the UV would

0:24:15.040 --> 0:24:19.240
<v Speaker 1>prove too much for even photosynthesis and plants, so, following

0:24:19.240 --> 0:24:22.040
<v Speaker 1>the blueprints of the KT extinction, in a matter of

0:24:22.119 --> 0:24:25.000
<v Speaker 1>days or weeks, the bottom of the food chain would collapse,

0:24:25.359 --> 0:24:27.800
<v Speaker 1>and everything else above it would starve. As a result,

0:24:28.560 --> 0:24:31.080
<v Speaker 1>the oceans too would be crippled by the increase in UV.

0:24:31.600 --> 0:24:33.960
<v Speaker 1>It would destroy the plankton that makes up the basis

0:24:34.000 --> 0:24:37.720
<v Speaker 1>of the marine food webs. The effect would be pronounced

0:24:37.800 --> 0:24:40.280
<v Speaker 1>enough that a gamma ray burst is considered to be

0:24:40.320 --> 0:24:43.119
<v Speaker 1>able to sterilize a planet close enough in its path,

0:24:44.880 --> 0:24:47.840
<v Speaker 1>and it's possible that the Earth has experienced them before.

0:24:48.720 --> 0:24:52.080
<v Speaker 1>One theory for the Ordovician extinction four hundred and forty

0:24:52.119 --> 0:24:54.400
<v Speaker 1>million years ago is that Earth got in the way

0:24:54.440 --> 0:24:58.560
<v Speaker 1>of a gamma ray bursts. As majestically dangerous as they

0:24:58.600 --> 0:25:01.440
<v Speaker 1>are gamma ray burst upened in the universe once a

0:25:01.520 --> 0:25:05.520
<v Speaker 1>day at least, well that's how often we noticed them

0:25:05.560 --> 0:25:08.760
<v Speaker 1>since the nineteen sixties. I should say humans have been

0:25:08.800 --> 0:25:12.399
<v Speaker 1>aware of supernova for thousands of years, first noting the

0:25:12.440 --> 0:25:15.440
<v Speaker 1>appearance of bright new stars in China almost two thousand

0:25:15.520 --> 0:25:18.679
<v Speaker 1>years ago. But we spent the entire lifespan of our

0:25:18.720 --> 0:25:23.200
<v Speaker 1>species up until the nineteen sixties blissfully unaware that invisible

0:25:23.240 --> 0:25:26.040
<v Speaker 1>death rays went off in our universe at all. It

0:25:26.080 --> 0:25:28.080
<v Speaker 1>was all because of the Cold War that we ever

0:25:28.119 --> 0:25:32.800
<v Speaker 1>found them. In ninety three, the US the USS are

0:25:33.200 --> 0:25:36.439
<v Speaker 1>in Great Britain signed a treaty banning nuclear detonations in

0:25:36.480 --> 0:25:40.960
<v Speaker 1>the atmosphere, underwater or in outer space. But we didn't

0:25:41.000 --> 0:25:44.159
<v Speaker 1>precisely trust our comrades, and so the US launched the

0:25:44.200 --> 0:25:48.200
<v Speaker 1>satellite capable of detecting large sudden spikes and nuclear radiation,

0:25:48.920 --> 0:25:51.800
<v Speaker 1>and the satellite found it. But it wasn't from nuclear

0:25:51.840 --> 0:25:55.840
<v Speaker 1>tests that satellite provided the first evidence of gamma ray bursts,

0:25:56.480 --> 0:25:58.960
<v Speaker 1>and since then we found that they are extremely common.

0:25:59.520 --> 0:26:06.520
<v Speaker 1>Stars collapse all the time. It seems the universe is

0:26:06.560 --> 0:26:10.159
<v Speaker 1>full of rocks and collapsing stars and gamma ray bursts,

0:26:10.680 --> 0:26:12.760
<v Speaker 1>which by the way. It can also form from two

0:26:12.760 --> 0:26:15.960
<v Speaker 1>black holes merging, or from the hiccup of an exotic

0:26:16.000 --> 0:26:19.280
<v Speaker 1>and frightening type of star called magnet Or, which is

0:26:19.320 --> 0:26:22.199
<v Speaker 1>a type of dwarf star made of nickel. It's been

0:26:22.359 --> 0:26:26.000
<v Speaker 1>hundreds of times per second and produces the strongest magnetic

0:26:26.040 --> 0:26:28.760
<v Speaker 1>field in the universe. This is a dangerous place out there.

0:26:28.760 --> 0:26:32.200
<v Speaker 1>I mean that the universe is has got no care

0:26:32.320 --> 0:26:36.920
<v Speaker 1>for life on Earth, and and I think that it's

0:26:36.960 --> 0:26:39.160
<v Speaker 1>worth remembering that when you look up in the nice sky,

0:26:39.320 --> 0:26:43.080
<v Speaker 1>when it looks very you know, peaceful and static, and

0:26:43.080 --> 0:26:52.479
<v Speaker 1>and it's unlook particularly dangerous. Being alive in the twenty

0:26:52.480 --> 0:26:55.640
<v Speaker 1>one century. You're probably fairly well versed in the basics

0:26:55.680 --> 0:26:59.080
<v Speaker 1>of climate change. We all are, and whether you believe

0:26:59.160 --> 0:27:01.919
<v Speaker 1>humans contribute to it or not, it's plain to everyone

0:27:02.000 --> 0:27:04.960
<v Speaker 1>that has advanced as we've become, we are still very

0:27:05.040 --> 0:27:08.439
<v Speaker 1>much at the mercy of the Earth's climate. All of

0:27:08.480 --> 0:27:12.240
<v Speaker 1>the bad news about climate change, though it seems incremental,

0:27:12.840 --> 0:27:15.639
<v Speaker 1>a few degrees increase in temperature here, a couple of

0:27:15.640 --> 0:27:19.080
<v Speaker 1>feet of sea level rise there, it just seems so well,

0:27:19.119 --> 0:27:22.400
<v Speaker 1>I hate to say it, but distant, distant and sort

0:27:22.440 --> 0:27:25.960
<v Speaker 1>of non threatening. Now there's a whole series I could

0:27:25.960 --> 0:27:28.160
<v Speaker 1>do just on how those sentiments aren't correct at all.

0:27:28.640 --> 0:27:31.240
<v Speaker 1>But enough doubt has been sown that it feels like

0:27:31.320 --> 0:27:34.240
<v Speaker 1>we have the luxury of time to keep arguing about

0:27:34.280 --> 0:27:36.840
<v Speaker 1>something as silly as whether humans are contributing in a

0:27:36.920 --> 0:27:39.959
<v Speaker 1>climate change or not, but whether you believe we do

0:27:40.280 --> 0:27:43.800
<v Speaker 1>or not, and we definitely do, there's something you should

0:27:43.800 --> 0:27:47.320
<v Speaker 1>know about climate change. Earth has a point of no

0:27:47.480 --> 0:27:50.960
<v Speaker 1>return climate wise, and should we find that we've pushed

0:27:51.000 --> 0:27:53.639
<v Speaker 1>it past that point, we would also find, to our

0:27:53.720 --> 0:27:56.920
<v Speaker 1>great peril that the changing climate would be neither distant

0:27:57.280 --> 0:28:03.000
<v Speaker 1>nor non threatening. With an overabundance of carbon dioxide, the

0:28:03.080 --> 0:28:06.160
<v Speaker 1>atmosphere could become a blanket that traps heat from escaping

0:28:06.200 --> 0:28:11.160
<v Speaker 1>into space, heating Earth up to an unbearable degree. Literally,

0:28:12.040 --> 0:28:15.879
<v Speaker 1>it's called a runaway greenhouse effect. If you were alive

0:28:15.920 --> 0:28:18.680
<v Speaker 1>in the nineties, you were introduced to the greenhouse effected

0:28:18.800 --> 0:28:21.720
<v Speaker 1>byproduct of climate change that can lead to global warming.

0:28:22.440 --> 0:28:25.480
<v Speaker 1>The basics are that as we burn more fossil fuels,

0:28:25.480 --> 0:28:28.439
<v Speaker 1>we contribute new large amounts of carbon dioxide to the

0:28:28.480 --> 0:28:31.280
<v Speaker 1>atmosphere that wouldn't otherwise be there. They would still be

0:28:31.320 --> 0:28:35.440
<v Speaker 1>locked underground as deposits of oil and gas. When sunlight

0:28:35.480 --> 0:28:38.200
<v Speaker 1>shines on Earth, the planet absorbs some of it and

0:28:38.320 --> 0:28:41.040
<v Speaker 1>is warmed by it, but it also re emits some

0:28:41.080 --> 0:28:44.760
<v Speaker 1>of it back into space as infrared heat. The trouble

0:28:44.880 --> 0:28:48.120
<v Speaker 1>is CO two is an extremely efficient absorber of that

0:28:48.200 --> 0:28:50.880
<v Speaker 1>infrared heat. When there's a lot of CO two in

0:28:50.920 --> 0:28:54.720
<v Speaker 1>the atmosphere, the atmosphere is a whole warms, so we

0:28:54.840 --> 0:28:57.440
<v Speaker 1>end up with a warm planet and a warmer than

0:28:57.480 --> 0:29:02.720
<v Speaker 1>normal atmosphere. Things become warmer all around, but when temperatures

0:29:02.800 --> 0:29:06.240
<v Speaker 1>rise on Earth, the planet just releases more radiated heat,

0:29:06.720 --> 0:29:09.880
<v Speaker 1>and so eventually temperature is cool again. It's as if

0:29:09.920 --> 0:29:12.800
<v Speaker 1>Earth overwhelms the CEO two in the atmosphere with sheer

0:29:12.880 --> 0:29:16.080
<v Speaker 1>multitudes of infrared. There's just not enough CEO two to

0:29:16.160 --> 0:29:19.440
<v Speaker 1>trap it all, and the planet overcomes the greenhouse effect

0:29:19.680 --> 0:29:23.040
<v Speaker 1>easy peasy. But there's a limit to how much heat

0:29:23.120 --> 0:29:26.280
<v Speaker 1>Earth can release into space, and so once the planet

0:29:26.280 --> 0:29:28.760
<v Speaker 1>reaches the point where it can emit no more infrared.

0:29:29.160 --> 0:29:32.080
<v Speaker 1>As c O two levels continue to rise, the tables

0:29:32.120 --> 0:29:34.880
<v Speaker 1>can turn, and it can be the carbon dioxide that

0:29:34.920 --> 0:29:40.080
<v Speaker 1>overwhelms Earth. A runaway greenhouse effect is triggered when a

0:29:40.120 --> 0:29:44.320
<v Speaker 1>positive feedback loop arises. As the planet grows warmer, more

0:29:44.360 --> 0:29:47.920
<v Speaker 1>water evaporates from the surface of the oceans. Water vapor

0:29:48.040 --> 0:29:51.840
<v Speaker 1>is also particularly good at absorbing reflected heat and trapping

0:29:51.840 --> 0:29:55.360
<v Speaker 1>it in the atmosphere, So the atmosphere goes even warmer,

0:29:55.800 --> 0:29:58.960
<v Speaker 1>causing more of the oceans to evaporate, adding more water

0:29:59.040 --> 0:30:02.800
<v Speaker 1>vapor to the atmosphere, trapping more escaping heat, warming the

0:30:02.800 --> 0:30:07.280
<v Speaker 1>planet even more and evaporating more of the oceans. Eventually,

0:30:07.480 --> 0:30:10.080
<v Speaker 1>it reaches a point where the entire planet becomes so

0:30:10.160 --> 0:30:15.360
<v Speaker 1>hot that the oceans boil off. You will be relieved

0:30:15.360 --> 0:30:17.600
<v Speaker 1>to hear that there is a point where the feedback

0:30:17.640 --> 0:30:21.120
<v Speaker 1>loop is broken and the runaway greenhouse effect ends. But

0:30:21.360 --> 0:30:23.640
<v Speaker 1>I regret to say that that doesn't happen until the

0:30:23.720 --> 0:30:27.880
<v Speaker 1>atmospheric temperature reaches about three thousand degrees fahrenheit, when the

0:30:27.920 --> 0:30:30.680
<v Speaker 1>emitted heat moves to a wavelength that water vapor is

0:30:30.680 --> 0:30:35.080
<v Speaker 1>incapable of absorbing. Long before that we humans would have

0:30:35.120 --> 0:30:39.280
<v Speaker 1>ceased to exist, and eventually, with the oceans boiled off,

0:30:39.320 --> 0:30:41.280
<v Speaker 1>any life hanging on in the seas would meet the

0:30:41.320 --> 0:30:45.520
<v Speaker 1>same fate as us. This is what astronomers believe happened

0:30:45.520 --> 0:30:48.680
<v Speaker 1>to Venus Venus is about the same size as Earth,

0:30:48.760 --> 0:30:50.880
<v Speaker 1>but it's far closer to the Sun, and it's not

0:30:50.960 --> 0:30:54.320
<v Speaker 1>within the Goldilocks zone. It's not the closest planet to

0:30:54.360 --> 0:30:57.240
<v Speaker 1>the Sun. That distinction goes to Mercury, but it is

0:30:57.280 --> 0:30:59.880
<v Speaker 1>the hottest planet in the entire Solar System by far,

0:31:00.000 --> 0:31:03.960
<v Speaker 1>are despite being almost twenty eight million miles further away

0:31:03.960 --> 0:31:07.040
<v Speaker 1>from the Sun than Mercury is. Venus is average surface

0:31:07.040 --> 0:31:10.480
<v Speaker 1>temperature of eight hundred and sixty four degrees fahrenheit is

0:31:10.560 --> 0:31:13.640
<v Speaker 1>hundreds of degrees hotter than Mercuries, hot enough to melt

0:31:13.720 --> 0:31:18.320
<v Speaker 1>let that's because Venus has an atmosphere thick with CEO two.

0:31:18.880 --> 0:31:21.560
<v Speaker 1>On the surface of the planet. The atmospheric pressure is

0:31:21.600 --> 0:31:24.280
<v Speaker 1>almost a hundred times that of Earth's at sea level,

0:31:24.640 --> 0:31:27.680
<v Speaker 1>about what you would experienced three thousand feet underwater in

0:31:27.720 --> 0:31:31.560
<v Speaker 1>one of Earth's oceans. There's no surface water on Venus

0:31:31.600 --> 0:31:35.080
<v Speaker 1>that evaporated away eons ago, but at some point in

0:31:35.120 --> 0:31:44.200
<v Speaker 1>its distant past, Venus may have been habitable. It is

0:31:44.240 --> 0:31:47.840
<v Speaker 1>to our great fortune that natural existential risks seem to

0:31:47.880 --> 0:31:53.160
<v Speaker 1>be rare. This is philosopher Toby ord. Humanity has survived

0:31:53.280 --> 0:31:57.040
<v Speaker 1>about two thousand centuries so far, so that's two thousand

0:31:57.120 --> 0:32:04.160
<v Speaker 1>centuries worth of natural risk. Asteroid comments, supervolcanos, supernovas, everything

0:32:04.320 --> 0:32:08.960
<v Speaker 1>put together that could have killed humanity. We've survived two

0:32:09.000 --> 0:32:12.840
<v Speaker 1>thousand centuries of that risk. UH. And this, this fact

0:32:13.040 --> 0:32:15.600
<v Speaker 1>allows us to put a bound on how much risk

0:32:15.720 --> 0:32:18.520
<v Speaker 1>these natural things could be causing UH. And if you

0:32:18.560 --> 0:32:21.520
<v Speaker 1>do the mathematics on this, you can show that it

0:32:21.600 --> 0:32:24.600
<v Speaker 1>can't be much higher than about one in a thousand

0:32:25.200 --> 0:32:29.760
<v Speaker 1>chance of extinction per century from natural causes, which works

0:32:29.760 --> 0:32:33.080
<v Speaker 1>out to a point zero zero one percent chance of

0:32:33.160 --> 0:32:36.960
<v Speaker 1>humanity going extinct from natural risks during any given year,

0:32:37.600 --> 0:32:42.600
<v Speaker 1>a thousandth of a percent, not too menacing. Most atmospheric

0:32:42.640 --> 0:32:46.520
<v Speaker 1>models show that human contributed CEO two definitely exacerbates the

0:32:46.520 --> 0:32:50.000
<v Speaker 1>greenhouse effect, but that it would be extremely unlikely that

0:32:50.040 --> 0:32:53.760
<v Speaker 1>we humans could push it into a runaway greenhouse. In

0:32:53.800 --> 0:32:57.080
<v Speaker 1>the paper where they introduced the world to the concept

0:32:57.080 --> 0:33:00.120
<v Speaker 1>of a dinosaur killing asteroid, the alvarez Is and their

0:33:00.160 --> 0:33:04.320
<v Speaker 1>colleagues calculated how frequently such a catastrophic event might take place.

0:33:05.080 --> 0:33:08.160
<v Speaker 1>They concluded that an asteroid with that scope of devastation

0:33:08.240 --> 0:33:11.840
<v Speaker 1>might come along once every hundred million years, which would

0:33:11.880 --> 0:33:14.400
<v Speaker 1>leave us with around thirty four million years left on

0:33:14.440 --> 0:33:18.120
<v Speaker 1>the clock before we can expect a similarly destructive asteroid.

0:33:18.440 --> 0:33:23.320
<v Speaker 1>With something approaching certainty. A gamma ray burst close enough

0:33:23.360 --> 0:33:26.120
<v Speaker 1>to Earth to cause a mass extinction might happen once

0:33:26.160 --> 0:33:29.280
<v Speaker 1>every billion years, and Earth would have to be lined

0:33:29.360 --> 0:33:31.600
<v Speaker 1>up in the path of the relatively narrow beam of

0:33:31.640 --> 0:33:35.840
<v Speaker 1>gamma radiation to experience the full effect. There are stars

0:33:35.880 --> 0:33:39.000
<v Speaker 1>nearby that could collapse in supernova, but the closest I

0:33:39.160 --> 0:33:43.160
<v Speaker 1>k pegasy A isn't expected to for another five million years.

0:33:44.000 --> 0:33:47.680
<v Speaker 1>The next two closest and Terris and Beetlejuice, could explode

0:33:47.680 --> 0:33:50.160
<v Speaker 1>at any time in the next million years, but it

0:33:50.200 --> 0:33:53.320
<v Speaker 1>should be too far away to damage Earth. And again,

0:33:53.480 --> 0:33:55.720
<v Speaker 1>the Sun has more than a billion years before it

0:33:55.760 --> 0:33:58.360
<v Speaker 1>reaches the end of its main sequence and begins to

0:33:58.400 --> 0:34:02.440
<v Speaker 1>grow unbearably hot for us. But it pays to keep

0:34:02.440 --> 0:34:06.280
<v Speaker 1>an open mind. It is entirely possible that our current

0:34:06.320 --> 0:34:10.319
<v Speaker 1>understanding of these risks is flawed in some way or incomplete,

0:34:10.880 --> 0:34:13.120
<v Speaker 1>that there's some factor we're not aware of yet that

0:34:13.160 --> 0:34:16.040
<v Speaker 1>could make any one of these disasters much more likely.

0:34:16.960 --> 0:34:20.799
<v Speaker 1>In that slight, limital space of uncertainty is where existential

0:34:20.920 --> 0:34:25.400
<v Speaker 1>risks live. The chances of them happening are minuscule, but

0:34:25.480 --> 0:34:29.080
<v Speaker 1>the consequences they bring if they do, are so catastrophic

0:34:29.480 --> 0:34:34.040
<v Speaker 1>that they demand to be taken into account. Atmospheric scientists,

0:34:34.080 --> 0:34:38.040
<v Speaker 1>for example, don't understand the extraordinarily complex interactions that make

0:34:38.120 --> 0:34:42.320
<v Speaker 1>up Earth's atmosphere, and so maybe we could accidentally trigger

0:34:42.400 --> 0:34:46.799
<v Speaker 1>a runaway greenhouse effect by burning fossil fuels. It's unlikely,

0:34:47.320 --> 0:34:51.400
<v Speaker 1>but it's unlikely under our current understanding, and with the

0:34:51.440 --> 0:34:57.360
<v Speaker 1>addition of information that understanding can change. Human misunderstanding doesn't

0:34:57.360 --> 0:35:01.799
<v Speaker 1>prevent calamity. In fact, it makes it like clear. But

0:35:01.880 --> 0:35:06.000
<v Speaker 1>here's the thing about natural existential risks. Being earth bound,

0:35:06.080 --> 0:35:09.200
<v Speaker 1>we can't do much about them right now. In the future,

0:35:09.239 --> 0:35:12.600
<v Speaker 1>we will, our artificial intelligence will be able to predict

0:35:12.640 --> 0:35:15.719
<v Speaker 1>gamma ray bursts to give us plenty of warning. Our

0:35:15.760 --> 0:35:18.800
<v Speaker 1>spacecraft will be able to ferry us around a safer planets,

0:35:19.440 --> 0:35:22.319
<v Speaker 1>and maybe we'll build structures to capture the energy from

0:35:22.320 --> 0:35:25.719
<v Speaker 1>those bursts and store it for later. But so long

0:35:25.760 --> 0:35:28.880
<v Speaker 1>as we remain bound to Earth, we will be vulnerable

0:35:28.960 --> 0:35:32.200
<v Speaker 1>to the same threats that it is. More so, really,

0:35:32.680 --> 0:35:35.920
<v Speaker 1>Earth is likelier to bounce back from a cataclysmic asteroid

0:35:36.000 --> 0:35:39.480
<v Speaker 1>or a gamma ray burst than we are. But there's

0:35:39.520 --> 0:35:43.319
<v Speaker 1>an entirely different class of existential risks, ones that we

0:35:43.400 --> 0:35:46.279
<v Speaker 1>have a much greater chance of controlling because they are

0:35:46.320 --> 0:35:50.600
<v Speaker 1>of our own making, but also ones that pose significantly

0:35:50.640 --> 0:35:57.680
<v Speaker 1>greater danger. These are anthropogenic existential risks. Anthropogenic risks. However,

0:35:58.320 --> 0:36:01.879
<v Speaker 1>um we can't apply such an argument to bound the probabilities,

0:36:01.920 --> 0:36:04.200
<v Speaker 1>and to show that there must be quite small. I

0:36:04.239 --> 0:36:07.000
<v Speaker 1>would say that there's maybe something like if there was

0:36:07.200 --> 0:36:12.319
<v Speaker 1>something like a risk of extinction from anthropogenic causes in

0:36:12.360 --> 0:36:15.800
<v Speaker 1>the twentieth century, this century, I think it's it's growing.

0:36:16.360 --> 0:36:18.720
<v Speaker 1>My best guest would be something like one and six

0:36:18.960 --> 0:36:23.120
<v Speaker 1>Russian Roulette, and then next century, well, if we don't

0:36:23.120 --> 0:36:27.120
<v Speaker 1>get our act together even higher. Those technologies that pose

0:36:27.160 --> 0:36:30.920
<v Speaker 1>an anthropogenic risk to us, we're beginning to develop them

0:36:31.000 --> 0:36:35.120
<v Speaker 1>right now. Some are already here and almost know what

0:36:35.840 --> 0:36:39.759
<v Speaker 1>is paying attention to the danger they are bringing our way.

0:36:44.960 --> 0:36:47.040
<v Speaker 1>On the next episode of the End of the World

0:36:47.040 --> 0:36:50.360
<v Speaker 1>with Josh Clark, it was a cold, windy day in

0:36:50.440 --> 0:36:54.440
<v Speaker 1>January nine when the robots took their first human life.

0:36:55.480 --> 0:36:58.560
<v Speaker 1>As we create more intelligent algorithms that are capable of

0:36:58.600 --> 0:37:01.919
<v Speaker 1>improving themselves, we run the risk that they may take

0:37:01.960 --> 0:37:05.760
<v Speaker 1>over their own development and quickly evolved beyond our control.

0:37:06.800 --> 0:37:09.240
<v Speaker 1>There is no good outcome for us if that happens.