WEBVTT

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<v Speaker 1>Welcome to Bedtime Astronomy. Explore the wonders of the cosmos

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<v Speaker 1>with our soothing Bedtime Astronomy podcast. Each episode offers a

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<v Speaker 1>gentle journey through the stars, planets, and beyond, perfect for

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<v Speaker 1>unwinding after a long day. Let's travel through the mysteries

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<v Speaker 1>of the universe as you drift off into a peaceful

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>When you picture an asteroid, I can almost guarantee what's

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<v Speaker 2>playing in your head right now. It's that iconic, totally

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<v Speaker 2>chaotic chase scene from the Empire Strikes Back.

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<v Speaker 3>Oh yeah, the Millennium Falcon, just darting through that densely

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<v Speaker 3>packed field of tumbling space rock.

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<v Speaker 2>Exactly just bouncing off each other, creating this impossible three

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<v Speaker 2>dimensional maze. And I mean it's a thrilling visual for

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<v Speaker 2>you as a viewer, but it is a complete.

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<v Speaker 3>Just massive violation of arble mechanics. It's really a masterclass

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<v Speaker 3>in terrible.

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<v Speaker 2>Astrophysics, right because the reality of the main asteroid belt

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<v Speaker 2>is well, it's profoundly lonelier than that.

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<v Speaker 3>Vastly lonelier. The objects out there are separated by these

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<v Speaker 3>just incomprehensible distances. I mean, if you were actually standing

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<v Speaker 3>on an asteroid in the main belt, you would likely

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<v Speaker 3>need a telescope just to see the next closest one.

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<v Speaker 1>Wow.

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<v Speaker 3>Yeah, it's a vast, mostly empty expanse. It is definitely

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<v Speaker 3>not a cosmic pinball machine.

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<v Speaker 2>And I think that emptiness sets us up for an

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<v Speaker 2>even bigger misconception, you know, because we just assume that

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<v Speaker 2>every single one of these sparsely distributed objects is well

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<v Speaker 2>just a dusty.

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<v Speaker 3>Gray rock, right, the standard floating rock assumption.

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<v Speaker 2>Yeah, but today we're totally dismantling that Hollywood myth because

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<v Speaker 2>out there in the dark, there is an object that

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<v Speaker 2>completely defies that assumption. It isn't rock at all. We're

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<v Speaker 2>talking about asteroid sixteen Psyche.

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<v Speaker 3>Psyche is amazing.

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<v Speaker 2>It's roughly the size of Massachusetts, right.

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<v Speaker 3>Roughly, Yeah, the Massachusetts size, kind of lumpy potato shaped

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<v Speaker 3>body that is comprised almost entirely of metal.

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<v Speaker 2>Which is just wild to think about, just a giant

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<v Speaker 2>metal potato.

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<v Speaker 3>And space iron and nickel to be specific. And the

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<v Speaker 3>working hypothesis in the planetary science community right now is

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<v Speaker 3>that sixteenth Hyche isn't just some random clump of heavy

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<v Speaker 3>metals that happened to stick together, Right, it's actually the

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<v Speaker 3>exposed frozen core of a lost protoplanet, a world was

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<v Speaker 3>violently stopped from forming during the very earliest days of

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<v Speaker 3>the Solar System.

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<v Speaker 2>So we are looking at a dead planet's heart basically.

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<v Speaker 3>Essentially, Yes, And by looking at this massive impact basin

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<v Speaker 3>on Psyche's north pole and running these incredibly complex computational

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<v Speaker 3>simulations of how that specific crater formed, we can start

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<v Speaker 3>to sort of reverse engineer the exact mechanics of the

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<v Speaker 3>demolition derby that gave rise to the planets we have today.

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<v Speaker 2>Okay, let's untack this, because if we think of the

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<v Speaker 2>early Solar System as this chaotic construction site I'm trying

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<v Speaker 2>to picture, is Psyche essentially leftover rebar?

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<v Speaker 3>I like that leftover rebar is actually a highly accurate

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<v Speaker 3>way to conceptualize the kinematics of the early Solar System.

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<v Speaker 2>Because, I mean, we know that in a fully formed planet,

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<v Speaker 2>the dense metals sink to the center to form a core, right,

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<v Speaker 2>and then the lighter silicates float up to form the

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<v Speaker 2>mantle in the crust.

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<v Speaker 3>Exactly, that's differentiation.

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<v Speaker 2>So for a planet's core to end up just floating

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<v Speaker 2>completely naked in the vacuum of space. It had to

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<v Speaker 2>have been entirely stripped of all those outer rocky layer.

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<v Speaker 3>Yeah, totally stripped, because back then we didn't have these

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<v Speaker 3>neat orderly planetary orbits the ease. Today we had a

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<v Speaker 3>swirling accretion.

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<v Speaker 2>Disk, just a mess of material.

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<v Speaker 3>A total mess. Gravity pulled gas and dust into small

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<v Speaker 3>clumps which collided to form planet tesimals. And as these

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<v Speaker 3>planet casimals accreted mass, the kinetic energy of constant impacts

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<v Speaker 3>combined with the decay of short lived radioactive isotopes like

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<v Speaker 3>aluminum twenty six, it generated immense paternal heat.

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<v Speaker 2>Right, and that heat is what triggers the differentiation you

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<v Speaker 2>mentioned exactly.

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<v Speaker 3>You get this global magma ocean phase. The iron and

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<v Speaker 3>nickel physically separate from the silicates and sink down into

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<v Speaker 3>the gravity well of the body.

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<v Speaker 2>They just dropped to the center.

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<v Speaker 3>Yes, the silicate metal partitioning. And the thing is Psyche

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<v Speaker 3>was on that exact trajectory. It had differentiated. It had

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<v Speaker 3>an iron core and a thick rocky mantle and a crust.

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<v Speaker 2>It was on its way to being a real planet.

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<v Speaker 3>It was, but the environment was defined by just catastrophic violence.

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<v Speaker 3>The prevailing model suggests Psyche was subjected to a series

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<v Speaker 3>of what we call hid and run collisions.

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<v Speaker 2>Hit and run, like they didn't just smash together and merge.

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<v Speaker 3>Not always, No, we're talking about other massive planetesimals, you know,

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<v Speaker 3>perhaps hundreds of kilometers across, slamming into it at velocities

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<v Speaker 3>of five to twenty kilometers per second.

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<v Speaker 2>Oh my god, five to twenty kilometers a second.

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<v Speaker 3>Yeah, And at those velocities, the kinetic energy transferred during

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<v Speaker 3>the impact is well, it's staggering. It wouldn't just leave

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<v Speaker 3>a crater, it would actually overcome the gravitational binding energy

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<v Speaker 3>of the mantle itself.

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<v Speaker 2>So it's hitting it so hard that the rock just

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<v Speaker 2>it can't hold on anymore.

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<v Speaker 3>The sheer physics of it are brutal. The shock waves

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<v Speaker 3>from a collision of that magnitude, they travel through the body,

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<v Speaker 3>compressing the material, and then they reflect back as rare

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<v Speaker 3>faction waves.

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<v Speaker 2>Where are faction waves?

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<v Speaker 3>Yeah, tensile waves that literally tear the rock apart from

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<v Speaker 3>the inside out. And if the impact angles oblique enough,

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<v Speaker 3>like a grazing blow rather than a dead on center mass.

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<v Speaker 2>Strike, it just takes the top right off exactly.

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<v Speaker 3>The kinetic energy shears the outer rocky layers completely off

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<v Speaker 3>the protoplanet, it accelerates that silicate debris well beyond escape velocity.

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<v Speaker 2>Wow, so the rock just flies off into space forever.

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<v Speaker 3>Right, But it leaves the much denser, highly cohesive iron

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<v Speaker 3>core intact. And if you do this a few times,

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<v Speaker 3>just strip away layer after layer, the crust and mantle

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<v Speaker 3>are gone. You're left with this unyielding metallic core totally

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<v Speaker 3>stripped of its protective layers.

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<v Speaker 2>So looking at Psyche out there and the main belt

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<v Speaker 2>is really like looking at a ghost. It's the skeletal

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<v Speaker 2>remains of a world that could have been a neighbored

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<v Speaker 2>Earth or Mars or Venus world.

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<v Speaker 3>Yeah, but from a purely scientific standpoint, this planetary casualty

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<v Speaker 3>is just a massive, massive opportunity.

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<v Speaker 2>For us because it solves that fundamental limitation we have

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<v Speaker 2>when we try to study the deep interior of our

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<v Speaker 2>own planet.

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<v Speaker 3>Yes, it's the ultimate irony of our discipline, honestly. I mean,

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<v Speaker 3>we have rovers analyzing the isotopic composition of.

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<v Speaker 2>Martian regolith right millions of miles away.

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<v Speaker 3>Millions of miles away, but we are embarrassingly ignorant about

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<v Speaker 3>the deep interior of the very sphere we are standing on.

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<v Speaker 2>I mean, if you're wondering why we don't just drill

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<v Speaker 2>down to find out what's the center of the earth,

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<v Speaker 2>the math is incredibly.

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<v Speaker 3>Humbling, extremely humbling. The distance from the surface to the

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<v Speaker 3>center of the Earth is roughly six three hundred kilometers.

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<v Speaker 2>Which is almost four thousand miles straight down.

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<v Speaker 3>Straight down. Now compare that to the deepest artificial whole

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<v Speaker 3>humanity has ever created, the Cola super deep borehole in Russia.

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<v Speaker 2>Right, how deep did they get?

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<v Speaker 3>They reached twelve point two six kilometers before the project

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<v Speaker 3>had to be abandoned.

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<v Speaker 2>Twelve point two six kilometers, So out of sixy three

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<v Speaker 2>hundred we've gone.

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<v Speaker 3>Twelve yep, which is roughly zer point two percent of

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<v Speaker 3>the way down.

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<v Speaker 2>I always think of the apple analogy. We live on

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<v Speaker 2>the absolute thinnest part of the skin of the apple,

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<v Speaker 2>and we've barely even managed to scratch that skin, let

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<v Speaker 2>alone get anywhere near the seeds in the center.

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<v Speaker 3>It's a perfect analogy. We haven't even pierced the crust entirely,

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<v Speaker 3>let alone reached the mantle of the core. And the

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<v Speaker 3>limitation isn't just a lack of engineering willpower. It's the

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<v Speaker 3>geothermal gradient and the extreme pressure.

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<v Speaker 2>Because it just gets hotter and heavier the deeper you go.

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<v Speaker 3>Right, It's a matter of fundamental thermodynamics and material science.

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<v Speaker 3>As you descend, the pressure increases to millions of atmospheres,

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<v Speaker 3>and the temperature at the core mantle boundary, it's hot

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<v Speaker 3>enough to melt literally any drill bit we could conceivably manufacture.

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<v Speaker 2>It just turns to liquid instantly yea.

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<v Speaker 3>And the rock down there it ceases to behave like

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<v Speaker 3>a brittle solid. Altogether, it acts like a highly viscous,

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<v Speaker 3>flowing plastic. We are functionally permanently locked out.

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<v Speaker 2>So if we can't physically go down there, how do

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<v Speaker 2>we know what's in our core at all?

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<v Speaker 3>We have to rely on indirect measurements, specifically seismic tomography.

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<v Speaker 3>We watch how pways and s ways from earthquakes propagate

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<v Speaker 3>and how they refract and reflect through the Earth's internal

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<v Speaker 3>layers like.

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<v Speaker 2>An ultrasound for the planet.

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<v Speaker 3>Exactly like an ultrasound. Yeah, but seismic data is essentially

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<v Speaker 3>a blurry sonogram. We can see density changes like the

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<v Speaker 3>Leman discontinuity.

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<v Speaker 2>Which is the boundary that separates the liquid outer core

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<v Speaker 2>from the solid inner core.

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<v Speaker 3>Right spot on. We can see that boundary exists, but

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<v Speaker 3>we can't sample the material. We can't put it in

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<v Speaker 3>a mass spectrometer. We are just guessing based on how

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<v Speaker 3>sound waves bend, which.

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<v Speaker 2>Makes sixteen Psyche the ultimate proxy. I mean, if we

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<v Speaker 2>can't go down into our own planet to see a core,

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<v Speaker 2>we have to look up because the universe has conveniently

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<v Speaker 2>cracked a planet open and left its core just sitting

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<v Speaker 2>in the freezer space for us to look at.

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<v Speaker 3>Yes, it's the only place in the entire Solar System

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<v Speaker 3>where we can directly observe the engine room of a planet.

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<v Speaker 3>And that is exactly why NASA launched the Psyche spacecraft

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<v Speaker 3>in late twenty twenty.

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<v Speaker 2>Three, just a mission dedicated entirely to flying alongside this

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<v Speaker 2>asteroid to take direct measurements right.

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<v Speaker 3>To finally get some ground truth data on what a

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<v Speaker 3>planetary core actually looks like up close.

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<v Speaker 2>But the wait time on orbital mechanics is just brutal.

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<v Speaker 2>I mean, the probe won't arrive until August of twenty

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<v Speaker 2>twenty nine.

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<v Speaker 3>It takes a long time to get out there.

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<v Speaker 2>So in the meantime, with the spacecraft still years away,

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<v Speaker 2>planetary scientists aren't just twiddling their thumbs waiting for photos

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<v Speaker 2>to download.

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<v Speaker 3>Oh, definitely not. We already have some ground based telescope data,

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<v Speaker 3>radar imaging, and light curve inversion.

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<v Speaker 2>Models, and that gives us a fuzzy, low resolution shape

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<v Speaker 2>model of the asteroid.

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<v Speaker 3>Very fuzzy, but we can see it's that lumpy potato shape,

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<v Speaker 3>and we can make out a massive impact basin near

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<v Speaker 3>its north polar region.

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<v Speaker 2>But trying to figure out the internal structure based on

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<v Speaker 2>a blurry silhouette millions of miles away, that requires some

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<v Speaker 2>intense computational forensics, right.

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<v Speaker 3>Exactly, And this is where they reach and break through

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<v Speaker 3>research led by Namia by All at the University of

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<v Speaker 3>Arizona really comes into play. If we can't physically sample

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<v Speaker 3>the asteroid yet, we have to use advanced hydrocodes to

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<v Speaker 3>simulate the specific impact that created that North Pole crater.

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<v Speaker 2>Okay, wait, what exactly is a hydrocode.

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<v Speaker 3>Hydrocode is a highly specialized computational tool. It's used to

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<v Speaker 3>model the behavior of continuous media under extreme conditions.

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<v Speaker 2>Like a hypervelocity asteroid impact.

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<v Speaker 3>Right, Because things don't behave normally when they hit each

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<v Speaker 3>other at ten kilometers a second, solid rock and metals

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<v Speaker 3>start acting almost like fluids, and you can't just model

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<v Speaker 3>a generic sphere colliding with a flat surface. The geometry

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<v Speaker 3>of the target dictates how the shockwave propagates.

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<v Speaker 2>Because hitting a curved ridge line on a potato shaped

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<v Speaker 2>asteroid is going to yield a completely different crater geometry

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<v Speaker 2>than hitting a flat plane.

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<v Speaker 3>Precisely so, Byell's team had to painstakingly program in Psyche's lumpy,

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<v Speaker 3>irregular shape into the simulation.

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<v Speaker 2>Wow, And they also had to test different internal structures, right,

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<v Speaker 2>since we don't know the exact composition beneath the surface.

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<v Speaker 3>Yes, they ran simulations with two very different internal models.

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<v Speaker 3>First a homogeneous model, which assumes Psyche is just a solid,

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<v Speaker 3>uniform block of iron nickel alloy all the way from

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<v Speaker 3>the surface to the center.

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<v Speaker 2>Like a giant cannon ball.

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<v Speaker 4>Right.

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<v Speaker 3>And then they also ran a layered model, testing the

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<v Speaker 3>hypothesis that maybe the core still retains a thin outer

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<v Speaker 3>shell of different material.

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<v Speaker 2>Like maybe some heavily shocked silicates or volcanic rock that

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<v Speaker 2>somehow survived those ancient hit and run collisions.

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<v Speaker 3>Exactly when they run these simulations, literally firing virtual projectiles

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<v Speaker 3>at virtual metal potatoes in a supercomputer. They are analyzing

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<v Speaker 3>the resulting creter morphology, and specifically, they are looking at

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<v Speaker 3>a metric known as the depth diameter ratio.

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<v Speaker 2>The depth diameter ratio eye. So, just to visualize this,

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<v Speaker 2>if I drop a heavy steel ball bearing into a

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<v Speaker 2>bowl of loose flour, the flower yields really easily, right,

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<v Speaker 2>and I get a deep, relatively narrow crater. Yes, But

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<v Speaker 2>if I drop that same ball bearing into a dense

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<v Speaker 2>block of wet clay, the clay resists the kinetic energy differently,

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<v Speaker 2>resulting in a wider or much shallower crater.

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<v Speaker 3>That's a great way to think about it. The physical

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<v Speaker 3>properties of the target material, its density, it's yield strength,

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<v Speaker 3>it's equation of state. Those dictate the final geometry of

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<v Speaker 3>the crater, how deep it is compared to how wide

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<v Speaker 3>it is.

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<v Speaker 2>It's like a cosmic fingerprint.

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<v Speaker 3>It really is. By altering the internal structure in the

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<v Speaker 3>hydrocode and measuring the resulting depth diameter ratio of the

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<v Speaker 3>virtual crater, Bisel's team is reverse engineering a multi billion

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<v Speaker 3>year old impact. They are hunting for the simulated interior

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<v Speaker 3>that produces a crater that perfectly matches the dim blurry

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<v Speaker 3>depression we can currently observe from Earth.

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<v Speaker 2>That is so clever. But in running these models, here's

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<v Speaker 2>where it gets really interesting. They isolated a hidden variable

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<v Speaker 2>that completely upends how we assume a solid metal asteroid

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<v Speaker 2>should behave.

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<v Speaker 3>Yes, porosity.

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<v Speaker 2>They found that porosity is actually the driving factor in

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<v Speaker 2>crater formation on Psyche.

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<v Speaker 3>Macro porosity specif the amount of empty space, deep voids

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<v Speaker 3>and internal fracturing inside the asteroid.

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<v Speaker 2>But wait, if Psyche is a metallic core that formed

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<v Speaker 2>under immense pressure at the center of a proto planet,

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<v Speaker 2>its initial state would be incredibly dense, right, like virtually

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<v Speaker 2>zero porosity.

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<v Speaker 3>It would have been pristine.

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<v Speaker 2>Yes, So why would a giant chunk of iron and

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<v Speaker 2>nickel floating in space be porous? I mean, a solid

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<v Speaker 2>block of steel doesn't avoids in it, It's solid.

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<v Speaker 3>The initial core was undoubtedly dense, But you have to

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<v Speaker 3>remember the apocalyptic violence of Psyche's history. When you slam

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<v Speaker 3>massive planet tesimols into it at ten kilometers per second,

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<v Speaker 3>the kinetic energy doesn't just vaporize the crust and.

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<v Speaker 2>Stop there, right, The energy has to go somewhere.

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<v Speaker 3>The shockwaves travel deep into the metallic core. Now, the

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<v Speaker 3>metal is incredibly strong, obviously, but it isn't invincible. These

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<v Speaker 3>impacts can actually exceed what's called the hugoniot elastic limit

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<v Speaker 3>of the iron alloy.

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<v Speaker 2>The hugonia elastic limit, meaning it hits it so hard

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<v Speaker 2>it permanently deforms or breaks the metal.

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<v Speaker 3>Brutally fractures it. It creates massive internal fault lines. The

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<v Speaker 3>metal is shattered into a tightly packed rubble pile, essentially

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<v Speaker 3>held together only by its own weak gravity.

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<v Speaker 2>Okay, so it's less like a pristine bowling ball of

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<v Speaker 2>steel and more like, I don't know, a heavily fractured

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<v Speaker 2>medieval shield that's just taken way too many hits.

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<v Speaker 3>That's yeah, exactly. It holds its macro shape. It looks

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<v Speaker 3>solid from the outside, but internally there are vast networks

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<v Speaker 3>of cracks and gaps. It's a metallic sponge.

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<v Speaker 2>A metallic sponge. Wow. And that internal empty space completely

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<v Speaker 2>changes how the material absorbs the kinetic energy of a

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<v Speaker 2>new impact.

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<v Speaker 3>It changes the energy partitioning entirely, because think about it,

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<v Speaker 3>If you strike a solid block of dense steel, the

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<v Speaker 3>energy of the blow is transmitted almost perfectly through the

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<v Speaker 3>material as an elastic wave. It just rings through it, right,

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<v Speaker 3>and much of that energy goes into excavating the crater

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<v Speaker 3>throwing material outwork.

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<v Speaker 2>Okay, But if the target is highly porous, like our

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<v Speaker 2>metallic sponge, then.

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<v Speaker 3>The energy does what we call pdvwork pressure volume work.

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<v Speaker 3>The shockwave energy is literally consumed by physically crushing the

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<v Speaker 3>voids and compressing the material inward on itself.

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<v Speaker 2>So the empty space collapses.

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<v Speaker 3>It collapses, and that.

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<v Speaker 2>Compression that generates intense localized heat.

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<v Speaker 3>Massive heat. So instead of just blasting material away and

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<v Speaker 3>excavating a deep hole, a highly porous Psyche would crush inward,

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<v Speaker 3>absorbing the blow locally, which fundamentally alters that depth diamber

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<v Speaker 3>ratio of the crater. We see.

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<v Speaker 2>It's like hitting a crumple zone in a car, exactly.

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<v Speaker 3>Like a crumple zone. And this leads to a fascinating

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<v Speaker 3>paradox regarding the fate of the impactor itself. You know,

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<v Speaker 3>the alien rock that actually crashed into Psyche's north pole

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<v Speaker 3>to make the crater.

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<v Speaker 2>Right, what happens to the bullet?

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<v Speaker 3>Well, the hydrocode simulations revealed something totally counterintuitive. A stronger,

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<v Speaker 3>more solid, low porosity interior actually preserves large amounts of

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<v Speaker 3>the impactor really, yes, while a weaker, highly porous interior

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<v Speaker 3>results in the impact or vaporizing or shattering into microscopic fragments.

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<v Speaker 2>But if the target is highly porous and crushes inward,

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<v Speaker 2>wouldn't that like trap the heat of the impact. It

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<v Speaker 2>sounds like the impactor would just be cooked inside the

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<v Speaker 2>crater rather than bouncing off.

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<v Speaker 3>That is exactly the thermodynamic mechanism at play. The crushing

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<v Speaker 3>action acts as an energy trap. The extreme heat and

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<v Speaker 3>pressure are localized right at the point of contact, enveloping

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<v Speaker 3>the impactor in the zone of extreme violence, so.

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<v Speaker 2>It just melts.

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<v Speaker 3>The temperature spikes so rapidly that the impact is subjected

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<v Speaker 3>to shock melting or outright vaporization. But if the target

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<v Speaker 3>is solid, dense metal, it cannot easily crush inward.

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<v Speaker 2>Right there are no voids to collapse, so the energy

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<v Speaker 2>propagates outward in a massive shock wave, violently excavating the crater.

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<v Speaker 3>The impactor is heavily fragmented, sure, but larger chunks of

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<v Speaker 3>it can actually survive the initial contact and become embedded

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<v Speaker 3>in the solid metal floor of the crater because that

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<v Speaker 3>localized thermal trap never formed.

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<v Speaker 4>Wow.

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<v Speaker 2>So when the Psyche spacecraft finally arrives in twenty twenty nine.

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<v Speaker 2>Its instrument payload is going to be hunting for those

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<v Speaker 2>exact fragments.

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<v Speaker 3>Yes, the probe is carrying a gamma ray and neutron spectrometer,

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<v Speaker 3>the GRNs.

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<v Speaker 2>Right, And the GRNs is a vital piece of this

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<v Speaker 2>puzzle because it detects the energy signatures of cosmic rays

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<v Speaker 2>interacting with the asteroid surface.

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<v Speaker 3>Correct Different elements emit different spectraa of gamma rays and

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<v Speaker 3>neutrons when struck by cosmic rays.

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<v Speaker 2>So by mapping those elemental signatures, the probe will be

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<v Speaker 2>able to see if there are high concentrations of exogenous

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<v Speaker 2>silicates basically alien rock, sitting in the bottom of that

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<v Speaker 2>North Pole crater exactly.

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<v Speaker 3>And if the spectrometer detects large chunks of rocky material

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<v Speaker 3>embedded in the metal, it tells.

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<v Speaker 2>Us that Psyche's interior is dense and solid.

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<v Speaker 3>Yes, But if it finds very little rocky material, it

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<v Speaker 3>tells us Psyche is a heavily fractured porous sponge that

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<v Speaker 3>vaporized its attacker.

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<v Speaker 2>It's literally planetary forensics via orbital spectrometry.

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<v Speaker 3>It's beautiful science, and the hypotheses generated by Bazal's three

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<v Speaker 3>D models are essential here because they calibrate the instruments

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<v Speaker 3>on the spacecraft. We aren't flying blind and we get

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<v Speaker 3>there in twenty twenty nine. The hydrocods tell us exactly

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<v Speaker 3>what elemental signatures and creater morphology is to look for

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<v Speaker 3>to answer these questions.

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<v Speaker 2>I mean, just studying the microscopic thermal dynamics of a

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<v Speaker 2>crater on a dead metal potato is an incredible display

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00:18:17.440 --> 00:18:19.720
<v Speaker 2>of physics on its own, it really is. But you know,

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<v Speaker 2>as we zoom out, the implications of understanding psyche stretch far,

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<v Speaker 2>far beyond just the main asteroid belt.

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<v Speaker 3>Oh definitely.

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<v Speaker 2>So what does this all mean for us? Because this

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<v Speaker 2>data actually scales up to one of the most significant

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<v Speaker 2>questions in modern astrophysics, right, the search for habitable exoplanets.

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<v Speaker 3>It does, and to understand that connection we have to

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<v Speaker 3>look at planetary geodynamos.

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00:18:40.279 --> 00:18:43.319
<v Speaker 2>Geodynamos the engines inside a planet.

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<v Speaker 3>Right, Planetary cores are not static lumps of metal deep

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<v Speaker 3>inside the Earth. The iron core is partitioned into a

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<v Speaker 3>solid inner core and a liquid outer core.

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<v Speaker 2>And the immense heat radiating from that inner core, combined

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<v Speaker 2>with the Coriolis force from the Earth spinning creates these

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<v Speaker 2>massive twisting convection currents in the liquid metal.

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00:19:03.079 --> 00:19:07.319
<v Speaker 3>Yes, magneto hydrodynamics, because the liquid metal is a conductor,

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<v Speaker 3>that turbulent churning motion generates a massive electromagnetic field that

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<v Speaker 3>extends far out into space around our planet.

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00:19:14.440 --> 00:19:17.880
<v Speaker 2>And that magnetic field is the absolute prerequisite for habitability

400
00:19:17.920 --> 00:19:19.079
<v Speaker 2>on the surface, isn't it.

401
00:19:18.960 --> 00:19:23.200
<v Speaker 3>It is the shield Space is an intensely irradiated environment.

402
00:19:23.799 --> 00:19:27.720
<v Speaker 3>Stellar winds these streams of highly energetic charged particles flowing

403
00:19:27.720 --> 00:19:30.720
<v Speaker 3>from a star. They will relentlessly strip away a planet's

404
00:19:30.720 --> 00:19:32.720
<v Speaker 3>atmosphere if it isn't deflected.

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00:19:32.279 --> 00:19:34.759
<v Speaker 2>And without an atmosphere, you can't have liquid water, you

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00:19:34.799 --> 00:19:36.319
<v Speaker 2>can't have life exactly.

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00:19:36.599 --> 00:19:39.359
<v Speaker 3>We see that exact scenario in our own solar system.

408
00:19:39.799 --> 00:19:41.839
<v Speaker 3>Mars lost as planetary dynamo.

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00:19:41.920 --> 00:19:43.119
<v Speaker 2>Its core just cooled down.

410
00:19:43.319 --> 00:19:46.599
<v Speaker 3>The core cooled, the convection stopped, and the magnetic shield

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00:19:46.599 --> 00:19:49.960
<v Speaker 3>completely collapsed. And once that shield was gone, the solar

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00:19:49.960 --> 00:19:53.519
<v Speaker 3>wind just eroded the Martian atmosphere over billions of years,

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<v Speaker 3>turning it into the irradiated desert we see today.

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<v Speaker 2>That is terrifying. So if we want to find an

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00:19:59.200 --> 00:20:03.319
<v Speaker 2>exoplanet capable of supporting complex life, particularly in the habitable

416
00:20:03.440 --> 00:20:07.039
<v Speaker 2>zones of highly active en dwarf stars, which are notorious

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<v Speaker 2>for violent stellar flares.

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00:20:08.720 --> 00:20:11.279
<v Speaker 3>We need to find planets with the right internal engines.

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00:20:11.559 --> 00:20:14.799
<v Speaker 3>They must possess a metallic core capable of generating and

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00:20:14.839 --> 00:20:17.759
<v Speaker 3>sustaining a strong geodynamo over billions of years.

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00:20:17.960 --> 00:20:21.720
<v Speaker 2>But right now, our theoretical models for how these metallic

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00:20:21.759 --> 00:20:24.640
<v Speaker 2>cores form, how their thermal evolution works, and how they

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00:20:24.680 --> 00:20:28.839
<v Speaker 2>partition light elements like sulfur or oxygen into the iron alloy.

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00:20:28.640 --> 00:20:31.480
<v Speaker 3>Are calibrated entirely on that point two percent of indirect

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00:20:31.519 --> 00:20:32.359
<v Speaker 3>data we have from.

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00:20:32.240 --> 00:20:33.759
<v Speaker 2>Earth, which is basically nothing.

427
00:20:33.839 --> 00:20:38.079
<v Speaker 3>We're guessing we are extrapolating massively from very limited data,

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00:20:38.599 --> 00:20:42.319
<v Speaker 3>But Psyche provides the missing ground truth data. By directly

429
00:20:42.400 --> 00:20:47.640
<v Speaker 3>studying an exposed core, measuring its porosity, mapping its elemental composition,

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00:20:48.079 --> 00:20:50.960
<v Speaker 3>and looking for remnant magnetic fields that might literally be

431
00:20:51.039 --> 00:20:52.759
<v Speaker 3>frozen into its crust.

432
00:20:52.559 --> 00:20:56.119
<v Speaker 2>We can physically verify our equations of state for core

433
00:20:56.200 --> 00:20:57.599
<v Speaker 2>materials exactly.

434
00:20:58.039 --> 00:21:00.319
<v Speaker 3>The data returned in twenty twenty nine will be fed

435
00:21:00.359 --> 00:21:03.960
<v Speaker 3>directly into the computational models that astronomers use to analyze

436
00:21:03.960 --> 00:21:05.839
<v Speaker 3>exoplanetary masses and densities.

437
00:21:05.920 --> 00:21:09.359
<v Speaker 2>So if we spot a super Earth fifty light years.

438
00:21:09.119 --> 00:21:11.960
<v Speaker 3>Away, the findings from Psyche will dictate our confidence in

439
00:21:12.000 --> 00:21:15.119
<v Speaker 3>whether that distant world has the internal thermal dynamics required

440
00:21:15.119 --> 00:21:18.640
<v Speaker 3>to generate a magnetic shield. We are literally analyzing the

441
00:21:18.680 --> 00:21:21.599
<v Speaker 3>anatomy of a dead world to refine our search parameters

442
00:21:21.599 --> 00:21:22.559
<v Speaker 3>for living ones.

443
00:21:22.440 --> 00:21:25.319
<v Speaker 2>Which fundamentally changes how we view this asteroid. I mean,

444
00:21:25.359 --> 00:21:27.559
<v Speaker 2>we've gone from dismissing it as just another piece of

445
00:21:27.599 --> 00:21:30.200
<v Speaker 2>space debris in an empty belt to recognizing it as

446
00:21:30.240 --> 00:21:34.200
<v Speaker 2>a critical calibration tool for the entire field of planetary science.

447
00:21:34.240 --> 00:21:37.559
<v Speaker 2>It is a keystone object, from the complex hydrocode simulations

448
00:21:37.559 --> 00:21:43.160
<v Speaker 2>of hypervelocity impacts to the totally counterintuitive thermodynamics of metallic porosity,

449
00:21:43.680 --> 00:21:47.759
<v Speaker 2>to the macro level search for habitable exoplanets. Psyche is

450
00:21:47.839 --> 00:21:50.559
<v Speaker 2>the physical bridge connecting the chaotic birth of our Solar

451
00:21:50.599 --> 00:21:53.279
<v Speaker 2>system to our understanding of the broader galaxy.

452
00:21:53.839 --> 00:21:57.960
<v Speaker 3>It is a remarkable convergence of disciplines. But I want

453
00:21:58.000 --> 00:22:00.319
<v Speaker 3>to leave you with a consideration that highlights it's the

454
00:22:00.359 --> 00:22:04.000
<v Speaker 3>inherent risk and the thrill of this type of exploration.

455
00:22:04.640 --> 00:22:07.359
<v Speaker 3>Throughout all of our modeling, the hydrocodes, the assumptions about

456
00:22:07.400 --> 00:22:11.519
<v Speaker 3>depth's diameter ratios. We are operating on a fundamental bias.

457
00:22:11.640 --> 00:22:13.359
<v Speaker 2>A bias how so, we.

458
00:22:13.319 --> 00:22:16.880
<v Speaker 3>Are assuming that Psyche's composition somewhat mirrors what we expect

459
00:22:16.880 --> 00:22:19.279
<v Speaker 3>to find deep within the Earth. We assume it is

460
00:22:19.319 --> 00:22:23.119
<v Speaker 3>primarily an ironickel alloy behaving according to the phase diagrams

461
00:22:23.160 --> 00:22:25.240
<v Speaker 3>we have constructed in our terrestrial laboratories.

462
00:22:25.279 --> 00:22:27.359
<v Speaker 2>Oh, I see, we're assuming Earth rules.

463
00:22:27.039 --> 00:22:30.559
<v Speaker 3>Apply out there exactly. But what if we are projecting

464
00:22:30.640 --> 00:22:34.200
<v Speaker 3>our Earthly expectations onto an alien body? What if the

465
00:22:34.200 --> 00:22:37.680
<v Speaker 3>spacecraft arrives in August twenty twenty nine, powers up its

466
00:22:37.680 --> 00:22:41.519
<v Speaker 3>spectrometers and discovers that this naked core is composed of

467
00:22:41.559 --> 00:22:46.880
<v Speaker 3>exotic alloys, strange isotopic ratios, or materials that behave under

468
00:22:46.920 --> 00:22:50.119
<v Speaker 3>shock pressures in ways that are entirely unaccounted for in

469
00:22:50.160 --> 00:22:52.680
<v Speaker 3>our current physics. Wow, what if the building blocks of

470
00:22:52.720 --> 00:22:55.119
<v Speaker 3>the early Solar System were far stranger than the planets

471
00:22:55.119 --> 00:22:55.839
<v Speaker 3>we ended up with.

472
00:22:56.000 --> 00:22:59.119
<v Speaker 2>That is the ultimate promise of deep space exploration. Isn't

473
00:22:59.160 --> 00:23:01.559
<v Speaker 2>it the possibilit that the universe is about to hand

474
00:23:01.640 --> 00:23:04.400
<v Speaker 2>us data that shatters our existing models, forcing us to

475
00:23:04.480 --> 00:23:07.359
<v Speaker 2>just rewrite the textbooks on planetary formation from scratch.

476
00:23:07.440 --> 00:23:08.839
<v Speaker 3>It happens more often than you think.

477
00:23:08.960 --> 00:23:10.920
<v Speaker 2>The wait until twenty twenty nine is going to be

478
00:23:11.039 --> 00:23:15.240
<v Speaker 2>absolutely agonizing, but the potential payoff is a fundamental shift

479
00:23:15.240 --> 00:23:17.279
<v Speaker 2>in how we understand the ground beneath our feet and

480
00:23:17.319 --> 00:23:20.759
<v Speaker 2>the exoplanets across the galaxy. Thank you for exploring the

481
00:23:20.799 --> 00:23:23.200
<v Speaker 2>mechanics of this lost world with us. The next time

482
00:23:23.240 --> 00:23:25.240
<v Speaker 2>you look out at the night sky, look past the

483
00:23:25.279 --> 00:23:28.319
<v Speaker 2>empty space and picture the invisible, frozen histories and the

484
00:23:28.400 --> 00:23:31.519
<v Speaker 2>poorest metallic hearts silently carrying the secrets to our past

485
00:23:31.559 --> 00:23:34.119
<v Speaker 2>in our future. Until next time, keep looking.

486
00:23:33.960 --> 00:24:00.160
<v Speaker 4>Up the

487
00:24:17.319 --> 00:24:51.440
<v Speaker 2>US Satis
