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Speaker 1: Welcome to Thrilling Threads.

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Speaker 2: Today, we're doing something a little different. We are staring

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directly into the terrifying physics of planetary failure, just examining

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the absolute limits of what the universe can throw at us.

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Speaker 1: That's right. Our mission today is to go through a

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stack of worst case scenarios, detailing the top ways the

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world could go spectacularly immediately wrong.

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Speaker 2: And we're not just you know, listing disasters.

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Speaker 1: Now, we are extracting the science behind the catastrophe, really

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analyzing the sheer scale and the frankly terrifying velocity of

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these events.

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Speaker 2: And while these scenarios are hypothetical, a kind of cosmic

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hit list for twenty twenty six, if you will, the

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underlying science.

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Speaker 1: Is anything, but it's all real.

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Speaker 2: It's all real. We're looking at measurable forces, kinetic energy,

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orbital mechanics, planetary chemistry, the sheer density of astronomical objects.

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It's an intense exercise in understanding not just how fragile

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Earth is, but also it's surprising resilience in some cases.

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Speaker 1: And for you listening, this is your shortcut to being

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well informed about the ultimate threats. We're going from rogue

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comets that are literally older than our Sun, all the

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way to the complete sudden disappearance of the air we breathe.

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Speaker 2: It's a lot to process, it is.

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Speaker 1: So let's unpack this and let's start with the fastest,

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most violent threats, the speed demons that come howling in

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from outside our own solar system.

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Speaker 2: It's a sobering thought, isn't it that not all planet

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killers originate in our neighborhood. For well, for millennia, astronomers

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only dealt with objects bound by the Sun's gravity.

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Speaker 1: Right, things from the asteroid belt, the Kuiper Belt are.

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Speaker 2: Stuff exactly our stuff. Now we have to account for

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the astounding reality of interstellar objects or ISOs.

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Speaker 1: I find the whole idea of ISOs just fascinating. They're

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essentially galacta kitchhikers, right. They get flung out of their

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own systems by gravitational chaos, and then they just travel

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through the void for what millions.

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Speaker 2: Of years billions sometimes until they briefly slice through our domain.

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Speaker 1: And for decades they were just theoretical. It was just

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an idea that all changed with our first confirmed visitor.

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Speaker 2: That would be one I twenty seventeen U, one which

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we all know.

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Speaker 1: As um oh moa such a great name.

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Speaker 2: It's perfect. The Hawaiian name means a messenger from Afar,

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arriving first. It really captures the surprise and the significance

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of its arrival. It was truly the first confirmed object

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we knew was not born here.

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Speaker 1: Okay, so how did we know that so definitively? I mean,

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what was the dead giveaway?

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Speaker 2: It all came down to speed, pure and simple. Most

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comets and asteroids that are local to us, they're moving

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at a pretty constrained velocity, maybe around twenty kilometers per second.

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Speaker 1: Which is still incredibly fast, Oh.

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Speaker 2: Incredibly fast. Yeah, But Umua was traveling at speed so

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far above that. We're talking at eighty seven kilometers per

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second up on leaving the Solar System. That's fifty four

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miles a second, a speed so high that it couldn't

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possibly be gravitationally bound to our son. That non local velocity.

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That was the immediate tip off. It was just visiting.

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Speaker 1: But the speed was just the beginning of a mystery,

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wasn't it, Because then there was the shape.

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Speaker 2: The shape, Yes, it was unlike anything else we routinely see.

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Astronomers started describing it as cigar shaped or you know, cylindrical.

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Speaker 1: Hot dog, a cosmic hot dog, a.

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Speaker 2: Cosmic hot dog exactly, an object that was estimated to

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be ten times longer than it was wide. That geometry

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is completely atypical compared to the you know, lumpy potato

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shaped rocks and ice chunks that we see all the time.

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Speaker 1: So you have this weird shape. Plus something else happened

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that caused this huge flurry of speculation, and that was

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its acceleration.

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Speaker 2: Right as Umwa Mus sped past the Sun. It didn't

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slow down exactly as Newton's laws predicted. It sped up

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just a little, but more than gravity alone could explain.

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Speaker 1: And that's where the alien theories started.

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Speaker 2: That's where the initial highly dramatic alien hypothesis came from.

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Some scientists seriously speculated that this acceleration must be artificial,

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like it had engines, or a light sale or solar

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sale functioning as a massive thin propulsion system or some

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kind of probe. It seemed incredible that our very first

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can firmed visitor from beyond might be an engineered craft.

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Speaker 1: It really speaks to the human psyche though face, with

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something truly new that our physics can't immediately explain. We

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just leaped to the most spectacular conclusion possible, of course.

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Speaker 2: But after a lot of rigorous scientific scrutiny, the consensus

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shifted back toward a natural explanation.

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Speaker 1: A less exciting one, but probably more likely.

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Speaker 2: Well, it's still pretty exciting. The scientific conclusion confirms it's

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almost certainly a comet, but one that uses a very

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subtle form of propulsion we rarely get to see. The

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acceleration was likely due to hydrogen outgassing.

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Speaker 1: Okay, so what does that mean?

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Speaker 2: Because onlya had been tumbling through the incredibly cold interstellar

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void for millions, maybe billions of years, a layer of

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frozen molecular hydrogen likely built up just beneath its surface.

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Speaker 1: And as it got close to our sun, that hydrogen

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it heated up and vaporized.

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Speaker 2: Precisely, that vaporization that outgassing, It acted like a tiny

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invisible thruster, pushing it just enough to account for that

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extra acceleration.

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Speaker 1: And that would also explain why we never saw tail,

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which is what you expect from a comet, exactly.

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Speaker 2: The comets we usually see outgas things like water or

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carbon monoxide ice, which reflects sunlight and create that big

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visible coma and tail Oumua's propulsion was silent and nearly invisible.

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It was an enigma, but ultimately a natural one.

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Speaker 1: So that was the strange fast messenger. But now let's

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talk about the real planetbuster in this scenario, the one

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that missed us by the smallest of cosmic margins, Comet

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three ie at.

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Speaker 2: Lists Atlas, the third ISO discovered logged in twenty twenty five.

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This one introduced a completely different level of well, frankly

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pure terror as a threat.

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Speaker 1: Model ooh Mua was small and weird, Atlas was big.

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Speaker 2: Atlas was much larger, some estimates say up to five

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point six kilometers wide. And it appears to be incredibly ancient.

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Speaker 1: And we have to just pause on that for a second.

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The age of this thing, our entire Solar system Earth included,

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is about four point five.

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Speaker 2: Billion years years old and three iatlis.

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Speaker 1: The sources suggest it originated in the Milky Ways thick

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disc of stars and could be as old as seven

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billion years So.

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Speaker 2: It's billions of years older than our Sun.

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Speaker 1: Think about that, A visitor that predates the Sun arriving

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from the you know, the ultraviolent primeval chaos of the

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early galaxy. It's basically a fossil from the Milky Ways creation.

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Speaker 2: And that extreme age is key to its weird composition.

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Scientists detected high levels of puzzling nickel and iron in

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the gases around it, a metal rich signature that's highly unusual.

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Speaker 1: But it still looked like a comet, right it had

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a tail it did.

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Speaker 2: It displayed classic cometary features, a visible coma and tail

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formed by outgassing water and carbon dioxide ice, a very

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strange mix.

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Speaker 1: So it's metal rich CO two rich, incredibly old, and

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it missed.

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Speaker 2: Us, thankfully, Yes, mercifully. Its closest pass was in December

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twenty twenty five, a distance of about two hundred and

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seventy million.

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Speaker 3: Kilometers, which sounds like a lot.

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Speaker 2: It is, but in cosmic terms, that was near miss.

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It passed within Mars's orbit, missing Mars by a mere

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twenty eight million kilometers. We are talking about the difference

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of a few degrees of trajectory separating Earth from just

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utter annihilation.

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Speaker 1: Okay, let's go there. Let's step into the hypothetical scenario.

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What if three I Atlas had been on a collision course.

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The benchmark for this stuff is always the chicksalub asteroid,

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the one that killed the dinosaurs.

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Speaker 2: Right, chicks Alub was estimated to be around ten kilometers wide.

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A massive piece of rock three atlas is roughly half

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that size at its maximum estimate maybe five point six kilometers.

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Speaker 1: So you'd think, okay, half the size, half the damage.

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Speaker 2: That would be the logical assumption. But it assumes they're

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moving at the same speed.

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Speaker 1: And this is where the terror of an ISO really

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comes into play. The physics of kinetic energy the energy

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of motion.

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Speaker 2: The equation is E equals one half envy squared, velocity

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is squared. That means if you double the velocity, you

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quadruple the energy.

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Speaker 1: And chicks a Lub was a local object, so it

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was moving at what twenty kilometers a second roughly, yes.

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Speaker 2: But three ialyis being in interstellar traveler was moving three

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times faster, sixty one kilometers per second.

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Speaker 1: Three times faster. So that's nine times the energy just

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from the speed.

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Speaker 2: Well, you have a smaller object, but because the velocity

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is so high, the impact would strike Earth with four

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and a half times the kinetic energy of the chiseel of.

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Speaker 1: Impact, four and a half times the dinosaur killer exactly.

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Speaker 2: That is a true difference between a local planet killer

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and an interstellar one.

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Speaker 1: That kind of energy releases just it's beyond human comprehension.

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It would be like detonating hundreds of millions of mega

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tons of TNT all at once.

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Speaker 2: The impact would punch through the atmosphere and barely more

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than a second, just vaporizing rock instantly, and.

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Speaker 1: The immediate destruction. The sources detail this pretty graphically.

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Speaker 2: Yes, the impact point would become a superheated core of plasma.

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The initial shock wave would generate super hurricane winds of

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a thousand kilometers per hour.

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Speaker 1: One thousand kilometers an hour. That's what does that even do?

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Speaker 2: It flattens everything, every tree, every building, every life and

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form for thousands of kilometers wiped clean.

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Speaker 1: And that's before we even get to what happens next.

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The material launched into the atmosphere.

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Speaker 2: Trillions of tons of molten material, vaporized rock magma would

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be launched high above the atmosphere. As this stuff ranged

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back down across the globe, the entire planet would just

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erupt into firestorms. The heat pulse alone would incinerate every

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exposed living thing.

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Speaker 1: At the same time, the seismic consequences would be just

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as bad overwhelming.

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Speaker 2: That impact energy would propagate through the planet, causing worldwide

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earthquakes that register beyond anything on the conventional Richter scale.

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Tectonic plates would shift, triggering massive global volcanic.

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Speaker 1: Eruptions, and the tsunamis.

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Speaker 2: Gigantic flooding continents hundreds of kilometers inland. It's a full

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planetary reset.

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Speaker 1: But if you somehow miraculously survived the firestorms, the tsunamis,

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and the global convulsion, the long term catastrophe would seal

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your fate. The impact winter, a multi year, maybe even

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decade long winter.

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Speaker 2: All that debris cast into the atmosphere soot, water, vapor,

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pulverized rock. It would form a dense, persistent cloud layer.

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It would block sunlight for years.

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Speaker 1: So photosynthesis would just stop.

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Speaker 2: It would hault entirely. Yeah, the global food chain collapses.

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On top of that. The atmospheric debris would combine with

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water vapor and fall back down as highly corrosive acid rain,

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poisoning fresh water systems and frying any surviving plants.

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Speaker 1: It's a double layered extinction. The blast kills the unprepared,

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and then the cold and darkness starved the survivors.

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Speaker 2: But there's a final terrifying chapter in this atlas an area.

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We have to remember what it was made of. It

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was rich in carbon dioxide.

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Speaker 1: Ice, right the CO two.

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Speaker 2: Upon impact, all that CO two ice would vaporize instantly,

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released into the atmosphere with all the rock and water.

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So once the sky is finally cleared and the impact

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winter started.

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Speaker 1: To subside, all that CO two would still be there.

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A massive greenhouse gas.

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Speaker 2: Trap, a colossal trap. So you shift from a deep

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global nuclear winter freeze to a long scorching recover, a

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runaway greenhouse.

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Speaker 1: Effect, a total environmental reversal. The few survivors who managed

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to cling on through the winter would then face a

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hyper scorching planet. It's a complete cycle of destruction.

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Speaker 2: The key takeaway here for you is that the true

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terror of these interstellar objects isn't their size. It's the

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compounding effect of velocity, turning a smaller object into an

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existential threat far greater than a local one. We really

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dodged a seven billion year old bullet with that one,

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all right.

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Speaker 1: So if the last segment was about the speed of

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cosmic objects, this one is about the slow, but ultimately

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catastrophic creep of things on our own planet. We're shifting

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focus from the void to a colossal ice mass sitting

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right here.

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Speaker 2: We're talking about the Thwaits Glacier.

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Speaker 1: In West Antarctica. Its nickname is not comforting.

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Speaker 2: No, it's aptly called the doomsday glacier. It's an enormous

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slab of ice, roughly the size of Florida, holding an

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estimated twenty five million cubic kilometers of ice, and the.

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Speaker 1: Source is called it a loaded trap, which I think

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is a fitting description.

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Speaker 2: It's very fitting because of its structure. It rests on

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a bedrock slope that dips inward toward the continent. That

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makes it uniquely unstable and very vulnerable to warm ocean

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water getting underneath it.

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Speaker 1: And it's already melting. It's not a future problem, it's

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a now problem exactly.

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Speaker 2: It currently sheds fifty billion tons of icy year that

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contributes a measurable four percent to global sea level rise today.

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Speaker 1: But what's the doomsday scenario? What happens if this whole

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colossal structure gives way suddenly?

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Speaker 2: The sources outline the immediate crisis if th Waits were

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to melt completely, that event, just to weights alone, would

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cause global sea levels to rise by sixty.

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Speaker 1: Centimeters, so about two feet instantly.

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Speaker 2: Now two feet might not sound like complete global annihilation,

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but it is enough to make major low lying coastal

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cities San Francisco, Miami, New Orleans, huge parts of Bangladesh

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instantly uninhabitable.

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Speaker 1: You'd trigger the largest forced migration in human history overnight.

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Speaker 2: An overwhelming strain on global infrastructure. But that's sixty centime

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is just the appetizer.

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Speaker 1: Because SWAITES is like a cork in a bottle.

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Speaker 2: It's the cork holding back the rest of the West

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Antarctic ice sheet. And if we consider the cascading effect

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of total Antarctic ice loss, well that's the seventy meter catastrophe.

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Speaker 1: Seventy meters, that's over two hundred feet.

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Speaker 2: Antarctica holds ninety percent of the planet's ice. If that

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entire twenty five million cubic kilometers of ice surges into

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the oceans, sea levels would rise by that shocking seventy meters.

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Speaker 1: The scale of that is just it's unimaginable.

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Speaker 2: It really is. Forty percent of the world's population, over

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three billion people live in coastal regions that would be

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permanently submerged global cities like London, Shanghai, Mumbai, they would

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just cease to exist. They'd become shallow seas.

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Speaker 1: And you'd had the contamination issue, right, all that salt

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water getting into the underground aquifers, poisoning freshwater sources, a.

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Speaker 2: Global crisis over drinking water that would affect even elevated

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inland communities.

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Speaker 1: But this is where we get into some really bizarre physics,

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the gravitational paradise.

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Speaker 2: Okay, let's unpack this for the listener. Yeah, because this

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is strange. Sea levels don't rise.

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Speaker 1: Uniformly, not when you're dealing with an object as massive

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as the Antarctic ice sheet, which weighs twenty four billion megatons.

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So how does its weight change the local sea level?

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Speaker 2: Think of it this way. That immense weight creates its

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own gravitational poll. It's a tiny local gravity well, and

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it's drawing the surrounding seawater toward the ice mass. It's

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like how the moon creates tides, but constant.

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Speaker 1: Okay, so the ice is literally holding the water close

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to it.

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Speaker 2: Exactly when the ice sheet disappears, that local gravitational pole vanishes.

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Speaker 1: Instantly and the water that was being held there is

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suddenly released and it flows away.

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Speaker 2: It flows away to find a new equilibrium across the planet.

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So while distant cities like New York and Rotterdam flood catastrophically,

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the sea level right near Antarctica would actually fall.

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Speaker 1: That's so counterintuitive.

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Speaker 2: It's a strange local counter effect of mass loss amidst

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the global deluge. It's a good reminder that the mass

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and gravity are the ultimate drivers here, not just volume.

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Speaker 1: And beyond the water itself, the melt exposes hidden horrors.

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We're not just releasing water, We're releasing millions of years

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of biological history locked in the ice in the permafrost.

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Speaker 2: The thawing permafrost is a terrifying dual biological threat. You

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have ancient bacteria and ancient viruses.

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Speaker 1: The bacteria are a concern because of antibiotic resistance right right.

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Speaker 2: The sources raise concerns about bacteria that have evolved traits

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dangerous to us, including some strains linked to diseases like

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cystic fibrosis. But the real issue is that these microbes,

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isolated for millennia, could transfer resistance genes to modern bacteria.

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Speaker 1: So you could suddenly face a global pandemic where common

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infections are completely untreatable. That's a nightmare scenario on top

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of an environmental catastrophe.

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Speaker 2: And then there's the virus threat. Scientists that document a

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DNA viruses that have been frozen for over forty thousand years,

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perfectly preserved in the permafrost. As the ground thaws, these viruses,

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potentially still viable.

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Speaker 1: Get released, a new ancient global pandemic.

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Speaker 2: It's a very real biological hazard. But the meltdown also

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triggers a massive global climate chain reaction, and this enters

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on the ocean circulatory.

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Speaker 1: System, the oceanic conveyor belt, the Gulf Stream exactly.

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Speaker 2: That influx of cold, fresh melt water directly disrupts it.

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The conveyor belt is critical because it transports warm, salty

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water from the equator up to the northern latitudes, keeping

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places like Europe much warmer than they would otherwise be.

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Speaker 1: And the freshwater being less dense. It just sits on

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top like a cap and stops the whole system.

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Speaker 2: That's the problem. It jams the entire heat transport mechanism.

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It causes a radical shift in climate. And this is

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where the paradox.

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Speaker 3: Comes in, because global warming could cause an ice age,

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it could while the melting causes global sea level rise,

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The disruption of the Gulf Stream could trigger a rapid

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ice age in North America and Western Europe, turning productive

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regions into frigid wastelands in a single decade.

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Speaker 1: It also starves the ocean.

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Speaker 2: The conveyer built doesn't just move heat, it moves nutrients.

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It brings nutrient rich water up from the deep ocean floor,

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which is vital for phytoplankton, the foundation of the entire

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ocean food chain. Less circulation means massive ecosystem collapse.

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Speaker 1: Okay, so let's briefly touch on the ultimate terrestrial disruption,

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the magnitude twenty earthquake.

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Speaker 2: Just as a benchmark, a magnitude twenty is a theoretical event.

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Geologists consider anything over a ten physically impossible from plate tectonics,

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because the earth crust just isn't rigid enough to store

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that much energy.

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Speaker 1: So to get to a twenty you need an outside force.

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Speaker 2: You need something like that three I atless impact we

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were just talking about. The energy release would cause a

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five full minute convulsion of the ground, ripping continents apart,

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initiating global tsunamis and totally transforming Earth's geography.

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Speaker 1: It's a vivid picture of planetary instability.

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Speaker 2: But it reminds us that while Earth's systems are fragile,

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ice sheets melt, current stall, the true immediate existential threats

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the ones that can crack the whole planet. They come

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from the overwhelming energy of the cosmos.

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Speaker 1: We've covered high speed impacts and slow terrestrial collapse. Now

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let's explore threats that operate on the scale of gravity itself.

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Scenarios that could destabilize our orbit, physically stretch the planet,

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or just erase it.

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Speaker 2: We are delving into the theoretical black.

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Speaker 1: Hole fly by, and what's so unsettling about black holes

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is the way their size their event horizon can be

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so deceptive compared to their mass.

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Speaker 2: Right, we need to distinguish between different classes of black

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holes and the specific way each one would annihilate our planet,

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because even a near miss can instantly ruin our year.

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Speaker 1: Let's start with the smallest hypothetical nightmare, a primordial black hole,

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one with the exact mass of Earth.

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Speaker 2: Okay, so, despite having the gravity of an entire planet,

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this black hole would have an event horizon of just

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under two centimeters. It's smaller than a coin. Wow. But

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if this tiny hyper dense object were to fly by,

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its concentrated gravity would exert mass massive tidal forces.

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Speaker 1: And tidal forces are differential gravity. Right, the near side

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of the Earth gets pulled harder than the far side.

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Speaker 2: Exactly, and that strain would rip the crust, triggering massive tsunamis,

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worldwide earthquakes, and volcanic chaos. But the worst impact would

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be orbital.

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Speaker 1: It would just yank us out of place, like.

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Speaker 2: A massive gravitational slingshot. It would instantaneously yank Earth out

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of its current life sustaining orbit would either be thrown

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inward toward the Sun to be fried, or flung outward

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to the asteroid belt for a deep freeze. Either way,

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life ends okay.

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Speaker 1: Moving up the scale, a stellar mass black hole born

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from a giant star, Let's say one that's ten times

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the mass of our Sun. It would be about fifty

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nine kilometers wide.

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Speaker 2: This is the equivalent of a gravitational bullet. If one

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were detected entering the outer edge of our solar system

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the Kuiper Belt, astronomers would have only five and a

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half hours until total chaos.

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Speaker 1: Five and a half hours, what would The.

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Speaker 2: First signs be gravitational anomalies near Jupiter and Mars planets

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suddenly veering off corres, maybe even being torn apart. For Earth,

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it would start with a subtle distortion of the night

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sky from gravitational lensing, the gravity bending the light around it.

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Speaker 1: And then almost instantly, the tidal forces would hit.

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Speaker 2: The planet would crack across continents, violent gravity driven tides

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washing across the land, global earthquakes erupting all at once.

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A flyby is damaging enough, but a direct hit is

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one of the most terrifying instantaneous endings imaginable.

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Speaker 1: A direct hit from this thing would just pierce the

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planet like a needle.

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Speaker 2: It wouldn't even slow down. The mass is so immense

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and the velocity so high. It would rip straight through

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the crust the mantle of the core.

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Speaker 1: And how long would that take?

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Speaker 2: The timeline is chilling, Just point zero zero four seconds

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later it emerges on the other side. The black hole

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just leaves, and what's left behind a tunnel of superheated

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collapsing matter. The sudden removal of the core would cause

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the planet to rapidly implode and rupture. The shock waves

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would ignite the atmosphere, boil the oceans, and leave Earth

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fundamentally to formed hemorrhaging into space.

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Speaker 1: The integrity of the planet would just be gone completely.

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Speaker 2: Now, let's consider the next step up, an intermediate mass

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black hole, maybe a thousand times the mass of the Sun,

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about half the size of Earth itself.

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Speaker 1: With this one, a direct hit isn't a piercing it's

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an erasure.

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Speaker 2: It wouldn't hit Earth like a rock. It would simply

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replace this space where Earth used to be. The moment

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the planet approached the event horizon, it would be subjected

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to those immense tidal forces spaghetification, instant spaghetification, the entire

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core gone in an instant, and Earth would just collapse

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inward under its own residual gravity.

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Speaker 1: And finally, the true celestial monster, Phoenix a star, a

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supermassive black hole with a mass of one hundred billion suns.

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Speaker 2: The scale of this justifies visualization. Its event horizon is

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one hundred times wider than Pluto's entire.

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Speaker 1: Orbit, So even before this thing reaches the Kuiper Belt,

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its gravity would be warping the fabric of space.

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Speaker 2: Neptune and Uranus would start to drest the Sun's hold

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on the entire Solar's and would be compromised.

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Speaker 1: And at its closest pass, its gravity would overpower the suns.

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Speaker 2: Even if just for a few seconds. And this is

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where the truly strange effects happen. For that fleeting moment,

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the side of Earth facing the black hole would experience

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impossible continent high tides.

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Speaker 1: But also everything on Earth would feel weightless for a second.

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Speaker 2: A momentary sense of free fall. Yes, as the powerful

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localized poll temporarily cancels out the planet's own gravity.

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Speaker 1: It sounds almost whimsical, but it quickly ends.

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Speaker 2: The momentary tidal strain would cause global earthquakes beyond measurement,

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shattering the crust, and as the black hole races on

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it permanently shatters the Solar System's orbital balance. Earth would

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be violently flung out into the.

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Speaker 1: Void, ejected to become a rogue planet, drifting toward an

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inevitable deep preeze.

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Speaker 2: And that brings us to rogue planets themselves, objects not

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tied to a star, ejected from their own systems. There

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are billions of them in the Milky Way alone.

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Speaker 1: A Jupiter sized rogue flying by would be catastrophic. The

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gravity would cause massive tidal waves, deep cracking of the

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Earth's surface, widespread volcanic eruptions.

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Speaker 2: It's a planet size gravitational bomb. Passing by.

470
00:23:10,400 --> 00:23:13,640
Speaker 1: Even a smaller ones, say a mercury sized rogue, would

471
00:23:13,680 --> 00:23:16,079
do immense damage if it passed close enough.

472
00:23:16,160 --> 00:23:18,400
Speaker 2: If it passed at half the distance of our own moon,

473
00:23:18,799 --> 00:23:22,000
you'd have tides eight times higher than today and land

474
00:23:22,000 --> 00:23:26,599
strain causing intense earthquakes and volcanoes. Globally, the whole planet

475
00:23:26,599 --> 00:23:28,839
would feel like it was being squeezed in a colossal

476
00:23:28,880 --> 00:23:29,759
invisible vice.

477
00:23:30,240 --> 00:23:33,839
Speaker 1: And the scenario of two equally massive earths passing close

478
00:23:33,880 --> 00:23:36,480
by that one is almost poetically devastating.

479
00:23:36,880 --> 00:23:40,000
Speaker 2: A brief zero gravity environment, you'd lose the atmosphere and

480
00:23:40,039 --> 00:23:41,880
then an eventual slow motion collision.

481
00:23:42,039 --> 00:23:46,240
Speaker 1: But the source material offer one really captivating whimsical possibility,

482
00:23:46,880 --> 00:23:47,880
the horseshoe orbit.

483
00:23:48,200 --> 00:23:50,519
Speaker 2: This is a real thing. We see it with Saturn's

484
00:23:50,519 --> 00:23:54,440
moons Janus and Epimetheus. Two bodies share the same orbit

485
00:23:54,519 --> 00:23:57,759
without colliding. They continually approach each other then.

486
00:23:57,680 --> 00:24:01,240
Speaker 1: Retreat, So in this fantasy scenario two earths, they would

487
00:24:01,240 --> 00:24:02,480
just forever chase each other.

488
00:24:02,559 --> 00:24:04,680
Speaker 2: It could lead to orbital dynamics where one side of

489
00:24:04,720 --> 00:24:09,599
the planet might experience perpetual summer. It's a marvelous thought experiment,

490
00:24:09,880 --> 00:24:12,880
a travel destination fantasy born from catastrophe.

491
00:24:12,920 --> 00:24:15,319
Speaker 1: But regardless of the size of the rogue, the greatest

492
00:24:15,359 --> 00:24:17,119
hazard is always ejection.

493
00:24:17,440 --> 00:24:21,480
Speaker 2: Always a rogue planet passes by imparts just enough momentum

494
00:24:21,519 --> 00:24:24,680
and shoves Earth out of its orbit entirely. That means

495
00:24:24,759 --> 00:24:27,640
either rapid deep freezing in the blackness of deep space

496
00:24:28,160 --> 00:24:31,519
or incinerating closer to the Sun. The orbital order of

497
00:24:31,519 --> 00:24:34,000
our Solar system is just exquisitely fragile.

498
00:24:34,160 --> 00:24:38,640
Speaker 1: We've explored destruction on astronomical and planetary scales. Now let's

499
00:24:38,640 --> 00:24:41,599
shift to a purely physics based threat that shows how

500
00:24:41,680 --> 00:24:44,799
mass combined with extreme speed can weaponize even the most

501
00:24:44,799 --> 00:24:46,359
innocuous object.

502
00:24:46,039 --> 00:24:48,079
Speaker 2: A tiny needle traveling at near light speed.

503
00:24:48,160 --> 00:24:50,480
Speaker 1: First, we have to lay out the physics barrier here.

504
00:24:50,720 --> 00:24:54,160
Einstein's theory of relativity says achieving one hundred percent light

505
00:24:54,200 --> 00:24:55,279
speed is impossible.

506
00:24:55,680 --> 00:25:00,240
Speaker 2: Right as an object accelerates, its relativistic mass increases, so

507
00:25:00,319 --> 00:25:02,680
you'd need an infinite amount of energy to reach that

508
00:25:02,720 --> 00:25:03,559
final speed limit.

509
00:25:03,759 --> 00:25:06,160
Speaker 1: So for this scenario, we have to assume a highly

510
00:25:06,200 --> 00:25:10,319
advanced alien civilization somehow gets around this, achieving ninety nine

511
00:25:10,400 --> 00:25:12,039
point nine percent of the speed of light.

512
00:25:12,319 --> 00:25:16,279
Speaker 2: At that speed, the kinetic energy is astronomical. Again, it's

513
00:25:16,400 --> 00:25:20,880
equals one half mv squared. Since velocity is squared, its

514
00:25:20,920 --> 00:25:24,559
contribution is exponential at ninety nine point nine percent c.

515
00:25:25,119 --> 00:25:28,400
Even the tiny needle carries kinetic energy equivalent to over

516
00:25:28,440 --> 00:25:30,759
one hundred times of one megaton nuclear bomb.

517
00:25:30,880 --> 00:25:33,160
Speaker 1: It turns a piece of metal into the ultimate weapon

518
00:25:33,200 --> 00:25:33,720
of physics.

519
00:25:34,000 --> 00:25:34,559
Speaker 2: Pretty much.

520
00:25:34,680 --> 00:25:37,319
Speaker 1: Okay, let's run the first impact scenario. It lands in

521
00:25:37,359 --> 00:25:40,519
a densely populated area, say Central Park in New York.

522
00:25:40,680 --> 00:25:43,519
Speaker 2: The moment it hits the atmosphere, the friction and heat

523
00:25:43,559 --> 00:25:45,559
would be so immense that the air itself would turn

524
00:25:45,599 --> 00:25:49,640
into plasma, creating a blinding incandescent trail, and the impact

525
00:25:49,759 --> 00:25:55,119
instantaneous and apocalyptic. The energy release woul vaporize everything nearby, rock, soil, water.

526
00:25:55,440 --> 00:25:58,319
The resulting fireball and shockwave would be massive enough to

527
00:25:58,400 --> 00:26:00,920
flatten buildings and rock nearby states.

528
00:26:00,480 --> 00:26:01,880
Speaker 1: It would register as an earthquake.

529
00:26:02,200 --> 00:26:05,400
Speaker 2: Locally, it would register as a seven point three magnitude

530
00:26:05,440 --> 00:26:09,000
Richter scale quake, collapsing high rise buildings across the city.

531
00:26:09,160 --> 00:26:11,680
Speaker 1: Now, I often wonder about this. What if it plunged

532
00:26:11,720 --> 00:26:13,160
into the ocean? What would happen? Then?

533
00:26:13,599 --> 00:26:16,559
Speaker 2: It would be a spectacular event, no doubt. The explosion

534
00:26:16,559 --> 00:26:20,200
would displace a colossal amount of water, creating a gigantic

535
00:26:20,319 --> 00:26:23,200
plume similar to the one scene during the nineteen forty

536
00:26:23,200 --> 00:26:26,839
six Baker nuclear test, would shot water two kilometers into

537
00:26:26,880 --> 00:26:27,240
the sky.

538
00:26:27,680 --> 00:26:30,799
Speaker 1: So massive explosion of water, does that mean a gigantic

539
00:26:30,880 --> 00:26:32,599
world ending tsunami follows?

540
00:26:32,880 --> 00:26:36,119
Speaker 2: Counterintuitively, no, or at least not the kind of tsunami

541
00:26:36,119 --> 00:26:37,279
we saw in two thousand and four.

542
00:26:37,359 --> 00:26:40,759
Speaker 1: Okay, explain that difference. Why wouldn't one hundred megaton explosion

543
00:26:40,880 --> 00:26:42,480
create a massive wave?

544
00:26:42,720 --> 00:26:47,079
Speaker 2: Megasunamis require geological shifts, a large vertical displacement of the

545
00:26:47,079 --> 00:26:50,559
seabed over a vast area, usually from underwater earthquakes or

546
00:26:50,599 --> 00:26:54,799
massive landslides. Those processes transfer energy efficiently through the entire

547
00:26:54,920 --> 00:26:56,079
column of water.

548
00:26:55,880 --> 00:26:58,839
Speaker 1: Whereas a single point kinetic explosion a single.

549
00:26:58,559 --> 00:27:03,920
Speaker 2: Point explosion, even one this powerful, creates intense localized pressure

550
00:27:04,279 --> 00:27:09,119
and a huge splash. The energy is dissipated mostly as heat, steam,

551
00:27:09,160 --> 00:27:14,079
and localized shockwaves, not a sustained broad geological movement. Mother

552
00:27:14,200 --> 00:27:17,319
Nature is still far more efficient and moving water across continents.

553
00:27:17,440 --> 00:27:20,440
Speaker 1: That's a tiny shred of comfort. However, there's one location

554
00:27:20,480 --> 00:27:23,759
where this needle strike would guarantee a global extinction event, a.

555
00:27:23,759 --> 00:27:25,839
Speaker 2: Direct hit on an active supervolcano.

556
00:27:26,000 --> 00:27:28,839
Speaker 1: This is the ultimate purely physics driven extinction.

557
00:27:29,119 --> 00:27:32,119
Speaker 2: The needle strike would breach the Earth's crust, releasing all

558
00:27:32,200 --> 00:27:35,440
the pent up magma pressure within a massive volcanic system.

559
00:27:36,079 --> 00:27:39,160
The impact would trigger a series of cataclysmic mass volcanic

560
00:27:39,279 --> 00:27:40,559
eruptions globally.

561
00:27:40,279 --> 00:27:42,079
Speaker 1: So we're talking about an event on the scale of

562
00:27:42,119 --> 00:27:45,319
the Toba eruptions seventy four thousand years ago, which nearly

563
00:27:45,400 --> 00:27:46,480
wiped out humanity.

564
00:27:46,599 --> 00:27:50,559
Speaker 2: In this hypervelocity scenario, volcanic ash and sulfur dioxide would

565
00:27:50,559 --> 00:27:53,799
be thrown miles high into the atmosphere, creating a persistent

566
00:27:53,839 --> 00:27:57,160
global stratospheric aerosol layer that would linger for ten years

567
00:27:57,279 --> 00:27:58,160
or more, blocking the.

568
00:27:58,119 --> 00:28:01,640
Speaker 1: Sun, which brings us back to that decade long nuclear winter.

569
00:28:02,319 --> 00:28:07,119
Global temperatures plummet, crops fail, global starvation would be the

570
00:28:07,200 --> 00:28:08,000
ultimate killer.

571
00:28:08,279 --> 00:28:10,960
Speaker 2: The only grim solace in this whole scenario is the

572
00:28:11,000 --> 00:28:13,880
personal takeaway. If you were in the path of that needle,

573
00:28:14,119 --> 00:28:16,480
you'd be instantly incinerated.

574
00:28:15,880 --> 00:28:18,200
Speaker 1: Death would be instantaneous and painless.

575
00:28:18,240 --> 00:28:21,359
Speaker 2: You would not witness the agonizing aftermath. It's perhaps the

576
00:28:21,359 --> 00:28:25,000
most immediate total obliteration scenario we've covered.

577
00:28:25,200 --> 00:28:29,319
Speaker 1: We've looked at external and physical threats. Now, let's examine

578
00:28:29,319 --> 00:28:33,119
the ultimate internal collapse, the sudden disappearance of the air

579
00:28:33,160 --> 00:28:36,839
we breathe. A scenario where Earth starts losing one percent

580
00:28:36,880 --> 00:28:39,000
of its atmospheric oxygen every second.

581
00:28:39,519 --> 00:28:42,960
Speaker 2: And this is terrifying precisely because of its speed. It's

582
00:28:43,000 --> 00:28:45,799
not a slow change that allows for adaptation. This is

583
00:28:45,839 --> 00:28:48,440
an immediate physiological and industrial crisis.

584
00:28:48,480 --> 00:28:51,000
Speaker 1: Okay, let's track the timeline. Thirty seconds in twenty six

585
00:28:51,039 --> 00:28:54,200
percent of our oxygen is gone, leaving a sixteen percent concentration.

586
00:28:54,440 --> 00:28:58,160
Speaker 2: Physiologically, you would feel extreme exhaustion, a desperate gasping for air,

587
00:28:58,480 --> 00:29:02,480
like sudden high altitude sickness. But the immediate systemic catastrophe

588
00:29:02,519 --> 00:29:05,880
is industrial combustion engines. They need about twenty one percent

589
00:29:05,960 --> 00:29:10,640
oxygen to function. At sixteen percent, cars stall, heavy machinery

590
00:29:10,680 --> 00:29:14,240
grinds to a halt, and most critically, planes fall out

591
00:29:14,240 --> 00:29:19,599
of the sky. The world's transportation system just stops dead.

592
00:29:19,680 --> 00:29:23,279
Speaker 1: And since less oxygen means less fire. Electrical grids would

593
00:29:23,279 --> 00:29:25,960
fail as fossil fuel power plants sputter and die.

594
00:29:26,240 --> 00:29:29,839
Speaker 2: Hospitals would face an immediate crisis. People with respiratory and

595
00:29:29,880 --> 00:29:33,519
cardiovascular issues would die instantly as their hearts fail trying

596
00:29:33,519 --> 00:29:34,599
to oxygenate the body.

597
00:29:34,640 --> 00:29:37,279
Speaker 1: Now, let's fast forward to the one minute mark. Fifty

598
00:29:37,279 --> 00:29:40,599
percent of the oxygen is gone, leaving an eleven percent concentration.

599
00:29:40,880 --> 00:29:46,920
Speaker 2: This induces severe hypoxia, universal gasping, short shallow breaths, poor judgment, staggering.

600
00:29:47,480 --> 00:29:50,039
Mass chaos erupts if people realize the air itself is.

601
00:29:49,960 --> 00:29:51,640
Speaker 1: Toxic and what's happening in the oceans.

602
00:29:51,960 --> 00:29:55,720
Speaker 2: The drop in atmosphere pressure causes the oceans to begin degassing,

603
00:29:56,079 --> 00:30:00,440
releasing dissolved gases, including oxygen. This starts killing marine life versly,

604
00:30:00,680 --> 00:30:01,680
creating mass.

605
00:30:01,440 --> 00:30:03,680
Speaker 1: Die offs, and at the same time, the ozone layer,

606
00:30:03,759 --> 00:30:06,599
which is made of oxygen, begins to deplete rapidly.

607
00:30:06,559 --> 00:30:10,279
Speaker 2: Exposing any potential survivors to harmful uv ras, though few

608
00:30:10,279 --> 00:30:11,680
would live long enough for that to matter.

609
00:30:11,799 --> 00:30:14,240
Speaker 1: By the two minute mark, seventy percent of the oxygen

610
00:30:14,319 --> 00:30:17,640
is gone, a mere six percent concentration is left.

611
00:30:17,759 --> 00:30:22,559
Speaker 2: At this point, you have mass fainting unconsciousness, faces turn

612
00:30:22,599 --> 00:30:23,279
ash colored.

613
00:30:23,519 --> 00:30:27,599
Speaker 1: But the sources also explore the absolute extreme, the ultimate

614
00:30:27,640 --> 00:30:31,480
wipeout scenario, not just losing the atmosphere, but the chemical

615
00:30:31,519 --> 00:30:34,720
removal of all oxygen molecules from Earth.

616
00:30:35,039 --> 00:30:39,400
Speaker 2: This collapses life in chemistry instantaneously. Because oxygen is the

617
00:30:39,480 --> 00:30:41,440
chemical backbone of the entire planet.

618
00:30:41,559 --> 00:30:44,480
Speaker 1: The human body is sixty five percent oxygen.

619
00:30:44,559 --> 00:30:47,799
Speaker 2: Every molecule, from water H two oz to the silicon

620
00:30:47,839 --> 00:30:51,119
oxides in the Earth's crust depends on those oxygen bonds.

621
00:30:51,240 --> 00:30:54,440
Without them, water instantly becomes a volatile sea of hydrogen.

622
00:30:54,559 --> 00:30:57,759
Buildings held together by oxygen compounds would crumble to dust.

623
00:30:57,960 --> 00:31:00,640
Speaker 1: The Earth's crust would literally fall apart, that all living

624
00:31:00,680 --> 00:31:03,400
things would become a pulpy molecular mess as the bonds

625
00:31:03,400 --> 00:31:05,039
and our organic structures just fail.

626
00:31:05,400 --> 00:31:08,599
Speaker 2: Eight minutes after this chemical catastrophe starts, ninety nine percent

627
00:31:08,599 --> 00:31:11,319
of all oxygen is gone. The planet is chemically destroyed.

628
00:31:11,359 --> 00:31:12,440
There's no coming back from that.

629
00:31:12,599 --> 00:31:14,880
Speaker 1: But in the slightly less horrific scenario where only the

630
00:31:14,920 --> 00:31:18,759
atmosphere disappears, there are a handful of biological survival specialists.

631
00:31:19,039 --> 00:31:22,400
Speaker 2: The infamous cockroach, which can survive up to forty minutes

632
00:31:22,400 --> 00:31:26,599
without oxygen. More impressively, the naked mole rat can survive

633
00:31:26,680 --> 00:31:29,559
up to eighteen minutes using anaerobic metabolism.

634
00:31:29,720 --> 00:31:32,680
Speaker 1: And then there are the true specialists, facultative anaerobes.

635
00:31:33,079 --> 00:31:37,799
Speaker 2: These are organisms like yeasts, some bacteria, bristleworms, things that

636
00:31:37,839 --> 00:31:41,960
can switch their metabolic process from oxygen respiration to fermentation.

637
00:31:42,839 --> 00:31:45,519
These would be the key to life's potential re evolution.

638
00:31:45,720 --> 00:31:48,000
Speaker 1: But even if life could re evolve, they're facing a

639
00:31:48,039 --> 00:31:51,759
non negotiable time constraint. The Sun is aging in a.

640
00:31:51,759 --> 00:31:55,200
Speaker 2: Mere six hundred million years, its luminosity will increase by

641
00:31:55,240 --> 00:31:58,359
six percent, raising temperatures high enough to trigger a runaway

642
00:31:58,359 --> 00:32:02,039
greenhouse effect and eventually evaporate the oceans. Life would have

643
00:32:02,079 --> 00:32:03,200
to adapt all over again.

644
00:32:03,640 --> 00:32:06,720
Speaker 1: Finally, let's turn to the last great systemic threat, the

645
00:32:06,799 --> 00:32:10,559
loss of our orbital stability, specifically the Moon colliding with Earth.

646
00:32:10,920 --> 00:32:13,039
This is a scenario where the Moon starts heading toward

647
00:32:13,160 --> 00:32:14,240
us over the course of a year.

648
00:32:14,440 --> 00:32:17,079
Speaker 2: The clock starts ticking about three hundred days out when

649
00:32:17,079 --> 00:32:19,519
the Moon is two hundred and fifty thousand kilometers away.

650
00:32:20,440 --> 00:32:23,400
Even at this distance, the tidal forces would increase dramatically

651
00:32:23,960 --> 00:32:27,960
high tides rising up to five meters, instantly flooding coastal cities.

652
00:32:28,160 --> 00:32:30,960
Speaker 1: By two hundred days, the tides are reaching staggering heights

653
00:32:31,000 --> 00:32:35,319
of thirty meters. Coastal infrastructure collapses completely, and at the

654
00:32:35,319 --> 00:32:39,119
same time, the gravitational pull is putting an unimaginable strain

655
00:32:39,319 --> 00:32:40,279
on Earth's crust.

656
00:32:40,440 --> 00:32:43,400
Speaker 2: That increased tidal force on the mantle leads to worldwide

657
00:32:43,440 --> 00:32:47,240
earthquakes and hypervolcanic eruptions. The Pacific Ring of Fire would

658
00:32:47,319 --> 00:32:48,920
become intensely active, But.

659
00:32:48,839 --> 00:32:52,079
Speaker 1: The sources offer a final astonishing twist that avoids a

660
00:32:52,119 --> 00:32:56,119
total hard collision, the Roch limit. Explain the roach limit.

661
00:32:56,160 --> 00:32:58,200
Speaker 2: It's the point where the tidal force is exerted by

662
00:32:58,240 --> 00:33:01,680
a massive body, In this case, Earth overcome the self

663
00:33:01,720 --> 00:33:05,640
gravity holding a smaller body, the Moon together. For us,

664
00:33:05,640 --> 00:33:09,039
that limit is about eighteen thousand kilometers away. Before the

665
00:33:09,079 --> 00:33:11,720
Moon can hit us, Earth's gravity fights.

666
00:33:11,440 --> 00:33:13,599
Speaker 1: Back, so the Moon would rupture and disintegrate.

667
00:33:13,759 --> 00:33:16,759
Speaker 2: You'd be shattered into a colossal ring of debris, from

668
00:33:16,839 --> 00:33:20,680
tiny dust particles to asteroid sized rocks. We'd get a

669
00:33:20,680 --> 00:33:23,359
stunning chaotic ring system, just like Saturn.

670
00:33:23,480 --> 00:33:26,319
Speaker 1: But the consequences of that beautiful ring would be devastating.

671
00:33:26,640 --> 00:33:31,440
Speaker 2: First, frequent intense meteor showers of moon debris would rain

672
00:33:31,559 --> 00:33:35,720
down everywhere. Second, the debris would block out significant sunlight,

673
00:33:36,079 --> 00:33:40,440
affecting photosynthesis and causing immediate global cooling, maybe an eight

674
00:33:40,480 --> 00:33:42,000
degree celsius drop, and.

675
00:33:42,039 --> 00:33:43,920
Speaker 1: All our communication systems would be gone.

676
00:33:44,079 --> 00:33:47,200
Speaker 2: Satellites would be pulverized by the thousands of rocks in

677
00:33:47,240 --> 00:33:50,319
the ring, no GPS, no Internet, nothing.

678
00:33:50,039 --> 00:33:52,480
Speaker 1: And finally, space travel would end completely.

679
00:33:52,680 --> 00:33:56,359
Speaker 2: The Ring system would be an impenetrable high velocity barrier.

680
00:33:56,920 --> 00:34:00,839
Humanity would be permanently grounded, facing a frozen, dark planet

681
00:34:00,920 --> 00:34:04,519
with destroyed infrastructure, a true orbital cage.

682
00:34:04,759 --> 00:34:07,480
Speaker 1: We have covered an astonishing breath of catastrophe today, the

683
00:34:07,519 --> 00:34:10,199
high velocity punch of a seven billion year old comet,

684
00:34:10,519 --> 00:34:14,239
the agonizing collapse of our atmosphere, the instantaneous erasure by

685
00:34:14,239 --> 00:34:16,519
a black hole, and the orbital locked down from a

686
00:34:16,559 --> 00:34:17,199
shattered Moon.

687
00:34:17,599 --> 00:34:20,440
Speaker 2: These scenarios, while designed to push the limits of fear,

688
00:34:20,679 --> 00:34:23,920
they provide incredible insight into the physics that governs our universe.

689
00:34:24,480 --> 00:34:27,159
We see the greatest threats involve the quadratic increase of

690
00:34:27,239 --> 00:34:31,119
energy with velocity, the delicate balance of planetary chemistry, and

691
00:34:31,159 --> 00:34:32,920
the overwhelming power of gravity.

692
00:34:33,119 --> 00:34:35,920
Speaker 1: We can take a slight, almost perverse comfort in the

693
00:34:35,960 --> 00:34:39,360
fact that the most extreme threats, like the light speed

694
00:34:39,400 --> 00:34:42,920
needle or the chemical removal of oxygen, are either impossible

695
00:34:43,119 --> 00:34:44,519
or highly improbable.

696
00:34:44,639 --> 00:34:47,480
Speaker 2: But the underlying science, the rate of ice melt, the

697
00:34:47,519 --> 00:34:50,960
effect of rogue objects, the kinetic energy of ISOs is

698
00:34:51,199 --> 00:34:55,079
very real. Humanity has proven itself remarkably good at two things,

699
00:34:55,679 --> 00:34:57,880
creating disasters and surviving them.

700
00:34:58,079 --> 00:34:59,880
Speaker 1: So we want to leave you with one final, deeply

701
00:35:00,000 --> 00:35:03,440
the unsettling thought experiment that draws on everything we've just discussed.

702
00:35:03,719 --> 00:35:06,880
If you had to choose between two guaranteed scenarios for

703
00:35:06,920 --> 00:35:07,639
the end of the world.

704
00:35:07,920 --> 00:35:13,119
Speaker 2: Scenario A an instantaneous, painless obliteration like that point zero

705
00:35:13,239 --> 00:35:16,480
zero four second black hole core collapse we described, he

706
00:35:16,559 --> 00:35:19,039
simply ceased to exist before your brain could register it.

707
00:35:19,320 --> 00:35:23,199
Speaker 1: Or Scenario B, a year long conscious countdown. You know

708
00:35:23,280 --> 00:35:25,039
the end is coming from the slow creep of a

709
00:35:25,079 --> 00:35:28,039
lunar collision or the certainty of a volcanic winter. It

710
00:35:28,079 --> 00:35:30,840
allows you to prepare to say goodbye and to witness

711
00:35:30,880 --> 00:35:33,320
the slow, agonizing collapse of civilization.

712
00:35:33,719 --> 00:35:37,760
Speaker 2: Instant painless obliteration or the year long conscious countdown. What

713
00:35:37,840 --> 00:35:39,119
is your stand on that choice.

714
00:35:39,239 --> 00:35:40,800
Speaker 1: We want to know what you think. Let us know

715
00:35:40,840 --> 00:35:43,519
in the comments below. Thank you for joining us for

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00:35:43,599 --> 00:35:45,159
this edition of Thrilling Threads.

