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Speaker 1: All right, so let's try and unpack this. There's this feeling,

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you know, the one you get when a rule you

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thought was totally fixed, a law of nature almost just

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gets shattered right in front of you.

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Speaker 2: Yeah, that sense of cosmic displacement. I know exactly what

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you mean.

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Speaker 1: I had this happen to me once. I was driving

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really late at night, way out in the middle nowhere,

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and I saw this this thing on a side road,

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just a blur, a blur. Yeah, it was moving so

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fast that it just didn't make sense for the environment.

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It wasn't just a car speeding. It felt like it wasn't,

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i don't know, operating by the same rules of physics

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as everything else.

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Speaker 2: That's a perfect analogy, actually, because that feeling is exactly

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what we're talking about today, just on an astronomical scale. Okay,

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we're talking about object that show up in our solar system,

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not from around the block, cosmically speaking, but from completely

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outside the Sun's entire sphere of influence.

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Speaker 1: So they're not just running a stop sign.

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Speaker 2: Moving so fast. Yeah, the stop sign. The whole town

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doesn't even have the gravity to slow them down.

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Speaker 1: And that's the key, that distinction. We've always had theories.

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I mean, it makes sense that stuff from the void

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would pass.

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Speaker 2: Through, right, is a statistical certainty.

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Speaker 1: But to actually see one, to confirm it, and then

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to see more, that just rewrites the rule book for

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our entire cosmic neighborhood.

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Speaker 2: It does, and that's what this deep dive is all about.

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We're looking at the discovery of these interstellar visitors. We've

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got two main players on the board. It's the first messenger,

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the first confirmed messenger. Yeah, a really peculiar high speed mystery.

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And then it's much much bigger, much older cousin.

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Speaker 1: The theoretical planetbuster.

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Speaker 2: An object that carries so much velocity it becomes well

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a weapon of cosmic proportions.

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Speaker 1: So our mission today is to figure out what makes

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these things interstellar, look at the frankly insane physics of

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how they move, and then run the simulation, the thought experiment,

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the necessary thought experiment. What happens when deep time and

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that kind of deep space velocity line up with our planet.

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Speaker 2: And that word velocity is going to be the key

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to everything. Yeah, it's the one factor that turns just

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a big old rock into a threat that can reset

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the entire course of life on Earth. So to start,

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we really need to nail down the terminology. When we

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see an object is interstellar, what does that actually mean?

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Speaker 1: It means it's not from around here.

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Speaker 2: At all, exactly. It originates completely outside our solar system.

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This isn't a comet that, say, Jupiter's gravity kicked into

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a weird orbit.

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Speaker 1: Or something from the Kuiper Belt way out past Neptune.

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Speaker 2: Yeah, this is like getting mail, but the return address

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is another star system, or maybe it has no return address,

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just a drifter unattached to any star that's been wandering

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the galaxy for who knows how.

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Speaker 1: Long, and for so long. That was just a concept

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of model. We figured it had to happen. The universe

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is a messy place. But getting confirmation that was a

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huge moment.

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Speaker 2: It was, and that first visitor was named Umuah. Officially

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it's one Eye twenty seventeen U one.

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Speaker 1: That designation, the one eye. That's the important part, isn't

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it It is?

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Speaker 2: The eye stands for interstellar. It was the first of

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a completely new class of object. The moment in twenty

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seventeen when we could finally track its path with enough

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certainty to say this is not bound to our Sun

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I love.

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Speaker 1: The name though, Umumua. It's Hawaiian, right it is.

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Speaker 2: It translates to something like a messenger from Afar arriving first.

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Speaker 1: You can't get more fitting than that. It was the herald.

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It told us they were out there.

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Speaker 2: And it wasn't just that it was there, it was

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how was behaving. The initial shock was all about its speed,

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its velocity.

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Speaker 1: Okay, let's break that down, because this is where the

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whole threat discussion starts. What's like a normal speed for

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our local stuff, commets, asteroids in.

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Speaker 2: Our solar system, things are moving pretty fast, but they're

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all sort of tethered by the Sun's gravity. So you're

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typically looking at speeds around twenty kilometers a.

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Speaker 1: Second, which is about twelve miles per second. That's already

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hard to wrap your head around.

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Speaker 2: It is. It's incredibly fast, but it's the speed limit

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of our neighborhood. You could say if the speed of

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things that stuck in the Sun's gravitational well, and uh

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Mumua just blew right past that speed limit. When we

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clocked it on its way out of our solar system,

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it was still moving at eighty seven kilometers per second.

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Eighty seven fifty four miles per second.

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Speaker 1: Okay, so that's not just a little faster, that's what

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more than four times the local speed?

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Speaker 2: Yes, And that immediately tells you everything you need to

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know about its journey. That speed guarantees what we call

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a hyperbolic trajectory.

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Speaker 1: That's the key term, right.

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Speaker 2: It is if something is moving in an orbit, its

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path is an ellipse. It keeps coming back. Yeah, But

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if it's moving above a certain speed the Sun's escape velocity,

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is path is a hyperbola. It comes in, swings around

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the Sun once, and it's gone.

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Speaker 1: It's never coming back.

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Speaker 2: Never. The fact that its speed was so high meant

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it could only have come from deep space. It arrived

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here already carrying tremendous momentum from somewhere else.

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Speaker 1: So we could be talking about an object that got

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what sling shot it out of its home star system,

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maybe hundreds of light years away exactly.

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Speaker 2: Maybe it got kicked out by a giant planet or

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close pass with its star, and then it just coasted.

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It traveled through the cold dark void for maybe a

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billion years, holding onto that speed the whole time a

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billion years. That momentum was gained somewhere else in a

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totally different environment, and thankfully, I mean really thankfully, the

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calculation showed it was no threat to us.

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Speaker 1: Its trajectory was safe completely.

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Speaker 2: It cut through our system, gave us a little bit

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of a shock, and then headed back out. It's on

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its way toward the constellation Pegas is right now.

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Speaker 1: It'll just keep going for millions, maybe.

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Speaker 2: Hundreds of millions more years. We were just a tiny

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little waypoint on an absolutely epic galactic journey.

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Speaker 1: So even after we knew and Mumu was safe, the

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weirdness didn't stop. It just kept piling up.

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Speaker 2: Oh yeah, the mystery was just beginning. Long after it

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passed by, scientists were still arguing about its basic physical properties.

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Speaker 1: Starting with its shape. It wasn't the usual lumpy, potato

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shaped rock we see in the asteroid belt.

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Speaker 2: Not at all. That's what was so strange. The data

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from its light curve, how its brightness changed as it tumbled,

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suggested an extreme shape. The best estimate was that it

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was maybe ten times longer than it was wide.

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Speaker 1: Which led to all those headlines about a cosmic cigar.

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Speaker 2: Right or a cucumber or TUTSI roll. I think I

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even saw a comparison to a submarine sandwich.

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Speaker 1: A belly buster turkey and bacon sub I think was

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the specific one.

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Speaker 2: The point is its elongation was extreme. We just don't

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see objects shaped like that in our solar system.

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Speaker 1: Why not? Why are ours all lumpy?

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Speaker 2: Well, it's generally down to gravity and collisions. Over billions

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of years. Things tend to either pull themselves into a

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rough sphere if they're big enough, or they get smashed

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into irregular potato like shapes. A long, thin needle or

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cigar shape suggests a very very specific kind of formation

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or and this is where the speculation really took off.

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It suggests it's not natural, that it's an artificial construct.

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Speaker 1: And it was tumbling too, right, not just spinning neatly.

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Speaker 2: It was in a chaotic tumble, spinning on multiple axes

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as it flew. But even that wasn't the biggest mystery.

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The real hit scratcher, The thing that launched a thousand

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scientific papers was the acceleration anomaly. Okay, so what's that

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When we tracked its path past the Sun, after we

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accounted for the pull of the Sun's gravity, it was

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still moving faster than it should have been.

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Speaker 1: Something else was pushing it. A non gravitational.

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Speaker 2: Push exactly, something was giving it a little extra kick. Now,

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with comets, this is normal. We see this all the time.

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Speaker 1: Right as they get close to the sun. The ice

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heats up, turns to gas, and shoots out in jets

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like little rocket thrusters.

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Speaker 2: Precisely, that process is called outgassing, and it gives the

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comet that push. But for that to happen, you need

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to see the telltale sign of.

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Speaker 1: A comet, the coma, that big fuzzy halo of gas

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and dust around it, and the tail.

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Speaker 2: And Umu had neither no coma, no tail, nothing. It

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just looked like a dead rock, a dead rock that

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was mysteriously accelerating.

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Speaker 1: And that's the moment the alien hypothesis really took hold.

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Speaker 2: It is, if it's being propelled but not by normal

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common activity, then maybe the propulsion is deliberate.

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Speaker 1: The solar sale idea, the solar.

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Speaker 2: Sale or light sale, was the most dramatic theory put forward.

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The idea was that maybe Umamura was a piece of

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alien technology, a probe or a scoutship, or maybe just

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some space junk using the pressure from sunlight itself to accelerate.

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Speaker 1: And we should be clear that's not just science fiction.

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Solar sale technology is real. Humans have successfully launched spacecraft

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that use it.

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Speaker 2: Oh. Absolutely, the physics is sound. It was a plausible,

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if exotic explanation for what we were seeing. It was

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incredibly tantalized.

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Speaker 1: But it wasn't the consensus, was it.

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Speaker 2: No. After years of debate in analyzing the data, the

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majority of the scientific community landed on a different explanation,

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one that's still strange but natural. The conclusion was that

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probably was a comment after all, just a very very

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weird one.

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Speaker 1: Okay, But how do they explain the missing tail. If

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it's a comment and it's outgassing, where's the gas?

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Speaker 2: That's the twist. The leading theory now is hydrogen outcasting

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hydrogen ice exactly. The idea is that Umulua formed in

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a part of its home system that was so incredibly

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cold that hydrogen gas actually froze solid. It became a

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hydrogen iceberg. Wow, as a got near our sun, that

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solid hydrogen deep inside it would have started to sublimate,

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turned directly into gas. That gas would escape and provide

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the push the acceleration.

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Speaker 1: Well, why couldn't we see it?

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Speaker 2: Because hydrogen gas is transparent, It's incredibly light, and it

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would dispoose almost instantly. It wouldn't drag dust in heavier

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molecules with it to create that visible coma and tail

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that you get from water ice or carbon dioxide ice.

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Speaker 1: So it had invisible.

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Speaker 2: Jets essentially, yes, invisible propulsion. It was a unique chemical

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makeup that led to a unique physical behavior. It was

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borne in conditions so different from our own solar system

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that it broke all our existing rules for what a

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comet should look like.

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Speaker 1: So the big takeaway from MUA isn't just that these

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things exist. It's so that they can be fundamentally chemically

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different from anything we know, and that they can carry

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these immense velocities, which of course opens up the next

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big question. If a small one can do this, what

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happens if a really really big one comes along?

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Speaker 2: And that brings us directly to the ancient grandfather of

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these objects three iet lists atls.

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Speaker 1: So this was found much more recently in twenty twenty five,

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and it's already been confirmed as the third interstellar object.

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Speaker 2: That's right, And if a Wumumoo was like a speedy

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little scout three ietlesses, well, it's more like an ancient battleship.

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It's moving at similar deadly speeds, but its story is

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one of deep, deep time.

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Speaker 1: The time scale is what gets me, oohm. Ou might

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have been traveling for millions of years, which is already

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a long time, but Atlis is on another level, entirely.

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Speaker 2: A completely different scale. Yeah. The current thinking is that

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three iet Liss is almost certainly older than our entire

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solar system.

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Speaker 1: Okay, han On, let's really process that our Sun, the Earth,

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all the planets, they formed about four and a half

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billion years years ago direct and you're saying this thing

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was already out there flying through space before any of

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that existed.

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Speaker 2: That's what the evidence points to. Some estimates put its

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age at seven billion years old, maybe even older. And

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its origin story is just as fascinating.

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Speaker 1: Where did it come from?

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Speaker 2: It seems to have originated in what's called the milky

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ways thick disc. Now we live in the thin disc,

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the familiar flat spiral arms of the galaxy, right. The

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thick disc is a much older, more puffed up region

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of stars that surrounds the thin disc. It's populated by

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primeval stars, stars that formed in a much more violent,

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chaotic era of the galaxy's youth.

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Speaker 1: So we're talking about a completely different stellar environment, a

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time when the galaxy was still I don't know, settling down.

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Speaker 2: Yes, and the chemical composition of everything was different. The

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building blocks available for making planets and commets were not

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the same as the ones in the cloud that formed

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our Sun.

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Speaker 1: The elements were different.

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Speaker 2: The ratios of elements were different. The material in the

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thick disc has survived billions of years of cosmic history,

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so Atl's isn't just an object. It's a pristine time

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capsule from an age before the Earth was even a.

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Speaker 1: Speck of dust, and that ancient origin explains the weird

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data we got from its composition.

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Speaker 2: It does. As it got closer to the Sun, we

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were able to analyze the gases it was giving off,

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and they were puzzled by what they found, unusually high

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levels of nickel and.

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Speaker 1: Iron, which isn't typical for our local comets, not at all.

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Speaker 2: Our comments are mostly water, ice, dust, silicates. They have

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some metals, but not blasting out in these kinds of concentrations.

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It suggests a different kind of core, maybe denser, more

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metal rich, something forged in the conditions of that ancient

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thick disk.

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Speaker 1: So it's this ancient metal infused heart wrapped in ice

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that's been flying through space for seven billion years.

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Speaker 2: That's the picture. And what's interesting is that, unlike Umoa,

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it's actually behaving like a proper comet.

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Speaker 1: Oh so this one does have a tail.

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Speaker 2: It does a big one. The Hubble telescope got some

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great images of it in twenty twenty five. It has

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the classic coma, the halo of dust and gas, and

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the long tail. It's blasting out huge amounts of water

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and carbon dioxide ice, just like a textbook comb It should.

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Speaker 1: A very very old textbook.

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Speaker 2: A very old textbook from a different library.

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Speaker 1: Yes, okay, let's talk size, because this is where the

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fear factor really kicks in. How big are we talking?

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Speaker 2: The estimates are still a bit wide. It's hard to

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see the solid nucleus inside that huge bright coma. But

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the range we're looking at is a minimum of about

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four hundred and forty meters about a quarter of a

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mile across.

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Speaker 1: Okay, that's already pretty big.

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Speaker 2: But the maximum estimate goes all the way up to

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five point six kilometers three and a half miles in diameter.

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Speaker 1: Whoah, okay, three and a half miles wide. If Umua

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was a cosmic cucumber. Atls is a flying mountain.

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Speaker 2: At its largest estimate. Yeah, it could be up to

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fourteen times bigger than Umua. Yeah, and that size puts

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it firmly in the potential planetbuster categories, well over the

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threshold for causing a global catastrophe on impact.

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Speaker 1: Now, before we go down that rabbit hole, we have

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to be absolutely clear this specific object three I at

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less it's.

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Speaker 2: Not going to hit us, absolutely not. It is one

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hundred percent safe. We've tracked its trajectory very carefully.

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Speaker 1: We can all breathe a sigh of relief.

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Speaker 2: Yes, its closest approach to US is in December twenty

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twenty five. But it's going to be about two hundred

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and seventy million kilometers away. That's one hundred and seventy

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million miles. It's not even close.

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Speaker 1: But it is passing through the neighborhood in a pretty

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interesting way.

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Speaker 2: It is. It's actually going to pass inside the orbit

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of Mars.

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Speaker 1: Really.

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Speaker 2: Yeah, it's going to miss Mars by about twenty eight

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million kilometers, which is only eighteen million miles on a

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cosmic scale. For an object this big and this fast,

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that is an incredibly close shave.

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Speaker 1: It's a real reminder that the Solar System is a

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shooting gallery.

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Speaker 2: And of course it led to the alien hypothesis round two.

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Speaker 1: Naturally, if Umumama was a scout ship, then the giant

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metal rich Atlas must be the mother ship.

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Speaker 2: That was the suggestion for the same group of researchers. Yes,

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but again that idea is really on the fringe. The

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scientific mainstream is treating this as what it appears to be,

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an ancient, massive, and incredibly valuable natural comet. The questions

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it raises are about geology and cosmology, not technology.

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Speaker 1: But those geological questions, combined with that incredible speed, lead

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us right to the big one, the terrifying but necessary

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thought experiment.

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Speaker 2: What if the geometry had been just a little bit different.

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Speaker 1: Okay, so this is where we have to really dig

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into the physics of survival. This is hypothetical, but it's

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crucial for understanding the stakes of planetary defense. Let's set

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the stage. What if that nudge Atlas got seven billion

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years ago put it on a slightly different path. What

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if Earth was in the crosshairs.

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Speaker 2: To understand an impact of this magnitude, we have to

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start with our baseline. The most famous impact in Earth's history,

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the chixelab asteroid.

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Speaker 1: The Dinosaur Killer. Remind us of the specs on that one.

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Speaker 2: Chikisel was big, about ten kilometers one so six miles.

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It was a carbonaceous asteroid, so mostly rock, minerals and some.

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Speaker 1: Metal, and its speed.

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Speaker 2: It was coming in at a pretty standard speed for

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a Solar system object, about twenty kilometers per.

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Speaker 1: Second, and that impact at that size and speed caused

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a global extinction, wiped out seventy percent of life, left

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a crater over one hundred kilometers wide. That's our baseline.

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Speaker 2: That's the baseline. Now let's bring in three ilsts. We'll

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use the maximum size estimate of five point six.

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Speaker 1: Kilometers, so it's about half the diameter of the Dinosaur Killer.

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Speaker 2: Roughly half the diameter and probably less dense, less massive

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because it has all that ice compared to Chickalob's solid rock.

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So if you only looked at size and mass, you

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might think, okay, less destructive.

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Speaker 1: But there's the velocity problem. That's the game changer.

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Speaker 2: That's the entire game. Chick Salobe hit at twenty kilometers

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per second three ia to ls is moving at a

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minimum of sixty one kilometers.

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Speaker 1: Per second more than three times faster.

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Speaker 2: Three times faster. And this is where the math gets

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absolutely brutal. The physics is exponential.

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Speaker 1: Explain that for us. Why I speed so much more

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important than size.

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Speaker 2: Here it all comes down to the formula for kinetic energy,

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the energy of motion. It's one half mass times velocity

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squared k E equals twelve Miliva is.

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Speaker 1: Squared, the velocity is squared.

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Speaker 2: The velocity is square. That's the killer. So if you

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double the velocity, you quadruple the energy. If you triple

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the velocity like we have here, you increase the kinetic

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energy by a factor of nine.

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Speaker 1: So even though ATLS has less mass, every bit of

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that mass hits with nine times the energy because of

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the speed.

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Speaker 2: Exactly when you run all the numbers, accounting for the

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different densities and everything, the conclusion is just staggering. If

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three I addols were to hit Earth, it would impact

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with four and a half times the total energy of

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the chick slab.

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Speaker 1: Impact four and a half times.

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Speaker 2: This isn't just another mass extinction event. This is a

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planetary sterilization event. Yeah, hashtag tag tag the immediate cataclysm

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in under second.

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Speaker 1: Okay, four and a half times the energy that killed

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the dinosaurs. It's almost impossible to picture. Let's try us

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through the first few seconds of an impact like that.

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Speaker 2: At sixty one kilometers per second, it moves through our

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entire atmosphere from space to the ground in just over

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one second.

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Speaker 1: So there's no time for it to burn up or

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slow down.

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Speaker 2: The atmosphere might as well not be there. It hits

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the crust with such force that the impact site doesn't shatter,

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it vaporizes the comet and a huge chunk of the

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Earth's crust are instantly converted into a superheated plasma.

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Speaker 1: So it's not making a crater so much as it's

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creating a temporary star on the surface of the Earth.

401
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Speaker 2: That's a good way to put it. That plasma core

402
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would incinerate everything for hundreds of miles around, but the

403
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destruction spreads much faster than that through the shockwave.

404
00:18:38,119 --> 00:18:40,839
Speaker 1: A shockwave from an impact of that energy.

405
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Speaker 2: It would propagate across the continent, across the globe. The

406
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air itself becomes a weapon. The compression wave would generate

407
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winds of over one thousand kilometers per hour.

408
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Speaker 1: That's what six hundred miles an hour that's not wind,

409
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that's a solid.

410
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Speaker 2: Wall of force it is. It's a blast wave that

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would scour the landscape clean. It would flatten cities, vaporized forests,

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level mountains.

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Speaker 1: I remember feeling a minor earthquake once, just a little trimmer,

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and the terrifying thing was the ground itself feeling unreliable.

415
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Speaker 2: This would trigger earthquakes globally that would register it beyond

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anything the Richter scale was designed to measure. It would

417
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cause volcanoes to erupt on the other side of the planet.

418
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And if it hit the ocean, mile high tsunamis not

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waves that crash on the coast, but waves that would

420
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wash hundreds of kilometers inland, just erasing everything. But the

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fire is maybe the worst part. The impact would throw

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trillions of tons of molten rock ejecta back up into

423
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the atmophere on ballistic trajectories. These glowing hot beads of

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glass would rain down all over the planet.

425
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Speaker 1: So it's not just the impact site that burns.

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Speaker 2: The entire sky would heat up to the temperature of

427
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pizza oven. It'd be hot enough to ignite every forest,

428
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every blade of grass on the entire planet. A global firestorm.

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Speaker 1: So within the first hour, maybe the first day. You're

430
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dealing with a plasma blast, hypersonic shockwave, global earthquakes, megasunamis,

431
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in a planetary firestorm.

432
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Speaker 2: The chances of survival for any complex life on the

433
00:20:04,920 --> 00:20:08,400
surface are effectively zero. But that's just the opening act.

434
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The immediate cataclysm is what gives way to the real

435
00:20:11,200 --> 00:20:14,759
long term planet killer effects hashtag tag do long term

436
00:20:14,839 --> 00:20:17,880
global killer. So once the initial chaos of the impact

437
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subsides phase two begins, all that material that was blasted

438
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into the sky, the vaporized comet, the dirt, the soot

439
00:20:23,880 --> 00:20:26,119
from the fires, it doesn't just disappear.

440
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Speaker 1: It stays up there, creating a shroud around the entire planet.

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Speaker 2: A thick global shroud, and that leads directly to an

442
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impact winter, or more accurately, a nuclear winter.

443
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Speaker 1: A supercharged version of it.

444
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Speaker 2: Exactly. This cloud of dust and aerosols would be so

445
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thick it would block out the sun, not just dim it,

446
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but block it out completely. The sky would go.

447
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Speaker 1: Dark and temperatures would plummet, plunge.

448
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Speaker 2: The surface of the Earth would drop to freezing and

449
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stay there for years, possibly for decades, a deep, relentless

450
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global winter.

451
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Speaker 1: And if there's no sunlight.

452
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Speaker 2: Photosynthesis stole ops instantly, the entire foundation of the global

453
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food chain is cut off at the knees. Plants dye

454
00:21:06,839 --> 00:21:09,079
clanked in and the oceans dye, and then everything that

455
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eats them dies. Widespread global starvation is the primary killer

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00:21:13,759 --> 00:21:15,200
in the post impact world.

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Speaker 1: And the atmosphere itself becomes toxic.

458
00:21:16,799 --> 00:21:19,839
Speaker 2: It does as all that debris starts to slowly rain

459
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back down and chemically alters the air. The impact creates

460
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huge amounts of nitrogen and sulfur oxides.

461
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Speaker 1: Which means acid rain, extreme.

462
00:21:26,960 --> 00:21:30,240
Speaker 2: Acid rain, strong enough to poison the oceans and sterilize

463
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any soil that wasn't already burned or frozen. And there's more.

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The energy of the impact would blast away the ozone layer,

465
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so when the sun finally did come back, the surface

466
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would be bathed in lethal uv radiation.

467
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Speaker 1: And the colmet itself was full.

468
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Speaker 2: Of metals, right, All that nickel and iron from ATLA

469
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would rain down to leading to widespread toxic metal poisoning

470
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of whatever water was left. It's just it's a multi

471
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pronged attack on the entire biosphere. You freeze it, you

472
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starve it, you poison it, and then you radiate it

473
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hashtag tag tag the climate paradox, deep freeze, discorging recovery.

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00:22:04,240 --> 00:22:07,319
But there's one final awful twist in this story, a

475
00:22:07,319 --> 00:22:10,279
climate paradox that's specific to an impact from a comet

476
00:22:10,319 --> 00:22:11,400
like three iatl Ice.

477
00:22:11,680 --> 00:22:14,160
Speaker 1: Okay, so we have the ste freeze that last for years,

478
00:22:14,200 --> 00:22:17,200
maybe decades, caused by the dust cloud. But eventually that

479
00:22:17,279 --> 00:22:18,839
dust has to settle, right it does.

480
00:22:19,079 --> 00:22:21,599
Speaker 2: The dust and sub particles are heavy. They're what reflects

481
00:22:21,599 --> 00:22:24,440
the sunlight and causes the cooling. But over time gravity

482
00:22:24,480 --> 00:22:26,920
winds and they rain out of the atmosphere. The sky

483
00:22:26,960 --> 00:22:28,160
would slowly start to clear.

484
00:22:28,359 --> 00:22:30,839
Speaker 1: But something else was put up there that doesn't settle.

485
00:22:30,559 --> 00:22:34,279
Speaker 2: Out precisely, the comet itself. Remember three Iatla is largely

486
00:22:34,279 --> 00:22:35,920
made of carbon dioxide.

487
00:22:35,400 --> 00:22:38,279
Speaker 1: Ice, a giant block of frozen text tootda.

488
00:22:38,079 --> 00:22:40,799
Speaker 2: Which was completely vaporized in the impact. All of that

489
00:22:40,839 --> 00:22:43,640
carbon dioxide. It was released directly into the atmosphere as

490
00:22:43,640 --> 00:22:47,319
a gas, and unlike dust, text toodp gas can stay

491
00:22:47,319 --> 00:22:49,240
in the atmosphere for centuries.

492
00:22:48,920 --> 00:22:51,400
Speaker 1: And it's a greenhouse gas, a very potent.

493
00:22:51,119 --> 00:22:53,160
Speaker 2: One one of the most potent. So as the dust

494
00:22:53,160 --> 00:22:55,599
clears and the sunlight starts to get through again. You

495
00:22:55,680 --> 00:22:58,480
now have an atmosphere that's supercharged with tixto ten to two.

496
00:22:58,960 --> 00:23:01,720
It acts like a thick thermal blanket trapping the Sun's heat.

497
00:23:01,759 --> 00:23:04,480
Speaker 1: So the planet goes from one extreme to the other violently.

498
00:23:04,640 --> 00:23:07,279
Speaker 2: You go from a deep freeze, a nuclear winter that

499
00:23:07,359 --> 00:23:10,240
kills almost everything, and then as the planet tries to recover,

500
00:23:10,640 --> 00:23:13,599
it swings into a period of extreme runaway global warming.

501
00:23:13,680 --> 00:23:15,559
Speaker 1: First you freeze, then you bake.

502
00:23:15,839 --> 00:23:20,079
Speaker 2: First a deep freeze followed by a long, scorching recovery.

503
00:23:20,160 --> 00:23:22,279
It's a one to two punch that makes the planet

504
00:23:22,319 --> 00:23:26,440
completely uninhabitable for an incredibly long time. And it shows

505
00:23:26,440 --> 00:23:31,000
that this class of object, these high velocity interstellar visitors,

506
00:23:31,359 --> 00:23:33,279
they're a unique and terrifying.

507
00:23:32,880 --> 00:23:34,880
Speaker 1: Kind of threat where the speed is so much more

508
00:23:34,920 --> 00:23:36,079
important than the size.

509
00:23:36,160 --> 00:23:39,039
Speaker 2: It forces us to realize that planetary defense isn't just

510
00:23:39,079 --> 00:23:41,440
about looking for big rocks in our own backyard. It's

511
00:23:41,480 --> 00:23:44,480
about looking for these ancient messengers coming in hot from

512
00:23:44,519 --> 00:23:48,039
the depths of the galaxy hashtag tag outro So.

513
00:23:48,160 --> 00:23:53,079
Speaker 1: We circle back to the good news, the slightly boring

514
00:23:53,240 --> 00:23:57,039
but incredibly comforting reality three i E. Less is not

515
00:23:57,079 --> 00:23:58,160
going to hit us it's.

516
00:23:58,039 --> 00:24:01,640
Speaker 2: Flying safely past. The math is solid. We're fine, and.

517
00:24:01,519 --> 00:24:04,200
Speaker 1: That safety is what lets us change your perspective to

518
00:24:04,240 --> 00:24:06,599
stop looking at it as a doomsday machine and start

519
00:24:06,599 --> 00:24:07,759
looking at it as what it.

520
00:24:07,680 --> 00:24:11,799
Speaker 2: Really is, a priceless opportunity, a piece of primordial history,

521
00:24:12,160 --> 00:24:13,839
just swinging by for a brief.

522
00:24:13,680 --> 00:24:16,720
Speaker 1: Visit, a visit that's been maddeningly difficult for astronomers to

523
00:24:16,759 --> 00:24:17,440
get a good look at.

524
00:24:17,519 --> 00:24:20,640
Speaker 2: That's the irony, isn't it. This incredible object is here,

525
00:24:21,000 --> 00:24:23,279
but because of its trajectory and where it is in

526
00:24:23,319 --> 00:24:26,880
the sky relative to the Sun, getting a clear, detailed

527
00:24:26,880 --> 00:24:29,559
look at it with our telescopes is incredibly challenging.

528
00:24:29,680 --> 00:24:32,039
Speaker 1: It's like a cosmic treasure chest is floating by, but

529
00:24:32,319 --> 00:24:34,160
the keyhole is facing the wrong way.

530
00:24:34,359 --> 00:24:37,319
Speaker 2: But it's moving so fast. We only get this one

531
00:24:37,519 --> 00:24:40,279
fleeting glimpse before it disappears back into the void forever.

532
00:24:40,559 --> 00:24:42,279
We can't send a probe to it, we can't catch

533
00:24:42,359 --> 00:24:44,759
up to it. We just get this one snapshot of

534
00:24:44,799 --> 00:24:46,759
a seven billion year old traveler.

535
00:24:46,799 --> 00:24:49,799
Speaker 1: But even that snapshot is so valuable immensely.

536
00:24:50,200 --> 00:24:53,039
Speaker 2: It's a physical sample of the early universe. It's a

537
00:24:53,079 --> 00:24:56,200
time capsule from before our sun even lit up, carrying

538
00:24:56,240 --> 00:24:59,200
the raw materials from the Milky Way's thick disk that

539
00:24:59,279 --> 00:25:02,759
high nickel and i iron content. It challenges our models

540
00:25:02,799 --> 00:25:05,039
of how the building blocks of galaxies come together.

541
00:25:05,519 --> 00:25:07,799
Speaker 1: So this knowledge, this is how we learned about the

542
00:25:07,799 --> 00:25:11,799
galaxy's violent, ancient past. These objects are the.

543
00:25:11,799 --> 00:25:14,720
Speaker 2: Proof they are. They remind us that the Solar System

544
00:25:14,799 --> 00:25:17,480
isn't some isolated island. We are part of a vast,

545
00:25:17,559 --> 00:25:21,440
interconnected galaxy, and matter and energy from deep time and

546
00:25:21,519 --> 00:25:24,680
deep space are constantly flowing through our neighborhood.

547
00:25:24,759 --> 00:25:27,880
Speaker 1: Their proof of a kind of galactic connectivity, bringing the

548
00:25:27,960 --> 00:25:30,759
history of the whole Milky Way right to our front door.

549
00:25:30,680 --> 00:25:32,119
Speaker 2: Condensed into a single object.

550
00:25:32,119 --> 00:25:35,640
Speaker 1: Here and that thought of history being carried on an

551
00:25:35,640 --> 00:25:39,119
object moving at these unbelievable speeds, that gives me a

552
00:25:39,119 --> 00:25:41,759
final idea to chew on. We've just spent all this

553
00:25:41,839 --> 00:25:43,960
time talking at an object that carries the secrets of

554
00:25:44,000 --> 00:25:47,759
the galaxies primordial past seven billion years ago, tells us

555
00:25:47,799 --> 00:25:48,160
where we.

556
00:25:48,119 --> 00:25:50,480
Speaker 2: Came from, Right, It's a message from the beginning.

557
00:25:50,720 --> 00:25:54,359
Speaker 1: But if these hypervelocity objects are like cosmic time travelers,

558
00:25:55,200 --> 00:25:56,640
what about the other direction?

559
00:25:57,079 --> 00:25:57,599
Speaker 2: What do you mean?

560
00:25:57,960 --> 00:26:01,759
Speaker 1: Well, if this visitor carries in information about the galaxy's formation.

561
00:26:02,880 --> 00:26:05,759
What kind of secrets would a theoretical object from the

562
00:26:05,839 --> 00:26:09,640
end of the universe carry? Wow, Imagine something launched somehow

563
00:26:09,680 --> 00:26:12,720
from the ultimate heat death of the Cosmos five billion

564
00:26:12,799 --> 00:26:15,599
years in our future. If that object traveled back through

565
00:26:15,640 --> 00:26:17,920
time and space to us, what would it tell us

566
00:26:17,920 --> 00:26:21,359
about the fate of all matter, the final collapse of stars,

567
00:26:21,680 --> 00:26:23,079
our ultimate future, the.

568
00:26:23,039 --> 00:26:25,680
Speaker 2: Beginning and the end of the universe, both traveling at

569
00:26:25,720 --> 00:26:27,240
eighty seven kilometers per second.

570
00:26:27,359 --> 00:26:30,400
Speaker 1: Now that's the real mystery. These discoveries unlock something to

571
00:26:30,400 --> 00:26:32,039
think about until our next deep dive.

