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>I want you to picture something for a second. Think

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<v Speaker 2>about the sheer kinetic reality of a major asteroid impact.

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<v Speaker 3>Yeah, it's almost impossible to truly visualize, right, because we're

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<v Speaker 3>talking about a mass of rock and iron, maybe one

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<v Speaker 3>hundred meters across, hitting the upper atmosphere at hypersonic speeds.

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<v Speaker 3>We're talking twenty to thirty kilometers per second exactly.

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<v Speaker 2>And at those velocities, the atmosphere doesn't just part for

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<v Speaker 2>the rock. It compresses so violently that the air itself

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<v Speaker 2>turns into this superheated.

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<v Speaker 3>Plasma, which is terrifying, honestly it is.

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<v Speaker 2>And when that mass finally strikes the continental crust, the

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<v Speaker 2>physics just completely defy our normal terrestrial frames of reference.

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<v Speaker 3>The pressure is so high it exceeds the structural integrity

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<v Speaker 3>of any known mineral on.

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<v Speaker 2>Earth, right, solid bedrock doesn't just crack or fracture. It

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<v Speaker 2>behaves like a fluid. It melts, a.

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<v Speaker 3>Huge portion of it literally vaporizes into a localized atmospheric

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<v Speaker 3>plume right.

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<v Speaker 2>On impact, and then you have this massive shockwave that

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<v Speaker 2>spreads outward, just instantly leveling all the topography.

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<v Speaker 3>While underneath a superheated melt sheet is forged in literal milliseconds.

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<v Speaker 2>It's the ultimate sterilization event, right, I mean, the thermal

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<v Speaker 2>radiation alone should eradicate any complex organic chemistry for miles

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<v Speaker 2>and miles.

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<v Speaker 3>That has always been the standard assumption.

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<v Speaker 2>Our whole traditional understanding of astrobiology kind of frames these

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<v Speaker 2>impacts as hard reset buttons, ye, like they are the

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<v Speaker 2>great terminators of life.

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<v Speaker 3>But what if that interpretation is just fundamentally backward.

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<v Speaker 2>Well exactly, what if the intense thermal energy and the

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<v Speaker 2>extreme pressure of an asteroid impact don't just leave a

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<v Speaker 2>sterile geological scar.

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<v Speaker 3>What if they actually synthesize the exact thermodynamic and chemical

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<v Speaker 3>conditions needed to incubate.

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<v Speaker 2>Life in a world that is otherwise completely hostile to it.

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<v Speaker 3>The paradigm in the scientific community is definitely shifting in

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<v Speaker 3>that direction right now.

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<v Speaker 2>Okay, let's unpack this because it's a massive shift.

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<v Speaker 3>For decades, we've categorized impact traders strictly through this lens

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<v Speaker 3>of catastrophic destruction.

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<v Speaker 2>Mainly because the visible macro level effects are just so

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<v Speaker 2>incredibly severe, right.

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<v Speaker 3>But when you shift the scale and you examine the

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<v Speaker 3>post impact environment geologically over tens of thousands of years,

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<v Speaker 3>the narrative totally inverts.

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<v Speaker 2>The extreme violence is actually what generates the long term

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<v Speaker 2>energy gradient you need to drive complex biogeochemical cycles.

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<v Speaker 3>Exactly, destruction and creation become two ends of the exact

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<v Speaker 3>same thermodynamic process.

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<v Speaker 2>So today we are exploring a really groundbreaking discovery from

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<v Speaker 2>South Korea that links these violent impacts to the very

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<v Speaker 2>oxygen we breathe.

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<v Speaker 3>And this earthly revelation is frankly acting like a treasure

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<v Speaker 3>map for finding life on Mars too.

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<v Speaker 2>Yeah, it's wild. The research comes from a team at

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<v Speaker 2>the Korea Institute of Geoscience and Mineral Resources led by

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<v Speaker 2>doctor Jsu Limb.

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<v Speaker 3>They've given us a completely new framework for understanding the

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<v Speaker 3>aftermath of cosmic impacts.

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<v Speaker 2>Let's ground this geographically first, because the location is super important.

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<v Speaker 2>We're talking about the Hapcheon impact crater.

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<v Speaker 3>Which is located in the Jokshan Chogi.

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<v Speaker 2>Basin, right, And this basin is a really distinct bowl

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<v Speaker 2>shaped depression on the Korean Peninsula.

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<v Speaker 3>And what's fascinating is that it's the only confirmed impact

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<v Speaker 3>crater on the entire peninsula, which.

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<v Speaker 2>Is crazy when you think about it. It's a massive

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<v Speaker 2>seven kilometer wide.

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<v Speaker 3>Structure, but it was only definitively confirmed as an impact

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<v Speaker 3>crater back in twenty twenty one.

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<v Speaker 2>How does a seven kilometer crater stay hidden until twenty

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<v Speaker 2>twenty one.

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<v Speaker 3>Well, it's a testament to how dynamic Earth's surface really is.

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<v Speaker 2>Unlike the Moon, right, where creators just sit there, perfectly

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<v Speaker 2>preserved in a vacuum forever.

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<v Speaker 3>Exactly. Earth has a very active hydrological cycle. We have

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<v Speaker 3>tectonic movement, heavy biological weathering, and the.

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<v Speaker 2>Korean Peninsula gets a lot of rainfall. Plus it has

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<v Speaker 2>incredibly dense vegetation.

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<v Speaker 3>Which is basically the perfect camouflage for geological anomalies.

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<v Speaker 2>So for decades, scientists just cataloged this basin as a

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<v Speaker 2>structurally unusual valley.

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<v Speaker 3>Yeah, it took extensive subsurface drilling to figure it out.

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<v Speaker 3>They had to look for microscopic.

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<v Speaker 2>Evidence the shocked courts right.

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<v Speaker 3>Precisely, shocked courtz only forms under the extreme instantaneous pressures

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<v Speaker 3>of a bullied impact.

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<v Speaker 2>So finding that finally proved its extraterrestrial origin.

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<v Speaker 3>But that twenty twenty one conformation just laid the groundwork.

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<v Speaker 3>The real bombshell is the twenty twenty six update, right.

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<v Speaker 2>Doctor Limb's team focused on the northwestern sector of the crater,

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<v Speaker 2>a spot they called Site str.

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<v Speaker 3>And what they found there just completely recontextualize the whole basin.

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<v Speaker 2>They discovered ancient microbial structures called stromatolites.

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<v Speaker 3>Just sitting right there in the crater.

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<v Speaker 2>Let me stop you there, because common sense is screaming

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<v Speaker 2>at me right now, I.

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<v Speaker 3>Know exactly what we're gonna ask.

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<v Speaker 2>If an asteroid vaporizes rock and creates this massive, superheated,

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<v Speaker 2>sterile crater, how do delicate microbial structures just appear there?

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<v Speaker 3>It seems like a total paradox, right.

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<v Speaker 2>How does a zone of absolute multi megaton annihilation become

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<v Speaker 2>a biological nursery.

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<v Speaker 3>It's a great question, And if you look at the

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<v Speaker 3>immediate seconds or days or even years after the impact,

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<v Speaker 3>you're totally right.

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<v Speaker 2>It's just a floor of molten glass and shocked.

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<v Speaker 3>Rock utterly sterile. But the biological incubation doesn't happen concurrently

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<v Speaker 3>with the impact.

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<v Speaker 2>Ah. Okay, so there's a timeline here.

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<v Speaker 3>Exactly, we have to introduce the concept of a post

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<v Speaker 3>impact hydrothermal lacustrine environment hydrothermal lakes.

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<v Speaker 2>Let's trace the thermodynamics of that.

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<v Speaker 3>So, the kinetic energy of the impact melts the bedrock,

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<v Speaker 3>creating this subtrane layer of superheated rock, the melt sheet.

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<v Speaker 1>Yes.

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<v Speaker 3>And because this melt sheet is buried under hundreds of

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<v Speaker 3>feet of fractured rock and insulating brescia, it cools down

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<v Speaker 3>incredibly slowly.

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<v Speaker 2>It basically acts like a giant subterranean furnace.

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<v Speaker 3>A thermal blanket.

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<v Speaker 2>Yes.

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<v Speaker 3>And then over centuries the climate stabilizes.

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<v Speaker 2>Rainwater and groundwater start to fill the crater basin.

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<v Speaker 3>Right. And as that water percolates down through the highly

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<v Speaker 3>fractured walk, it hits the residual heat of the melt sheet, it.

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<v Speaker 2>Gets superheated and rises back to the surface through convection.

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<v Speaker 3>Exactly, This creates a closed loop hydrothermal system.

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<v Speaker 2>Wow. So it's not just a warm bottle.

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<v Speaker 3>No. As the water circulates through all that pulverized bedrock,

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<v Speaker 3>the heat dramatically accelerates the dissolution of minerals.

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<v Speaker 2>The crater leg becomes a highly concentrated chemical reservoir.

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<v Speaker 3>Enriched with iron, silica, all these essential trace elements.

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<v Speaker 2>So the initial violence is actually necessary. It shatters the bedrock,

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<v Speaker 2>which increases the surface area for the water to interact.

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<v Speaker 3>With, and the sustained heat turns the whole basin into

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<v Speaker 3>a highly efficient chemical solvent.

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<v Speaker 2>Literally a self sustaining hydrothermal bioreactor.

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<v Speaker 3>That's the precise dynamic. And within this stable, warm, nutrient

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<v Speaker 3>rich spa, essentially life.

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<v Speaker 2>Thrives, specifically the cyanobacteria that build those trumatallites at cite.

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<v Speaker 2>Str let's actually.

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<v Speaker 3>Talk about what strumatallites are, because they're fascinating.

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<v Speaker 2>Oh, definitely. I like to avoid heavy jargon, so I

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<v Speaker 2>always think of them as ancient layered department buildings.

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<v Speaker 3>That's actually a fantastic analogy built.

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<v Speaker 2>By microscopic tenets the cyanobacteria, right.

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<v Speaker 3>And these cyanobacteria are photosynthetic, They eat sunlight and exhale oxygen.

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<v Speaker 2>And they have a fossil record that dates back what

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<v Speaker 2>three point five billion.

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<v Speaker 3>Years roughly, Yes, that They are some of the oldest

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<v Speaker 3>known life forms on the planet.

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<v Speaker 2>So how do they actually build these structures.

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<v Speaker 3>Well, as a colony of cyanobacteria grows, they precipitate calcium

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<v Speaker 3>carbonate as a byproduct of their metabolism, and.

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<v Speaker 2>As they do that, they trap ambient sediment from the water.

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<v Speaker 3>Exactly so they precipitate minerals in trap sediment. Building. These

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<v Speaker 3>structures up layer by micro scopic layer over very long periods.

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<v Speaker 2>Which means they aren't just fossilized microbes. They're basically biogeochemical chronometers.

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<v Speaker 3>They are literal history books made of rock because every

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<v Speaker 3>layer traps the chemical signature of the lake at the

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<v Speaker 3>exact moment that specific layer formed, like biological tree rings.

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<v Speaker 2>Yeah, I kind of picture them like a layer jawbreaker.

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<v Speaker 3>Candy and the Kigam team didn't just look at the

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<v Speaker 3>outside of the jawbreaker. They sliced it open and analyzed

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<v Speaker 3>the layers.

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<v Speaker 2>They performed really granular geochemical analyses across the cross sections

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<v Speaker 2>of these ten to twenty centimeter structures.

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<v Speaker 3>And we have to note the temporal markers here because

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<v Speaker 3>the Hapchin Crater is relatively young geologically, right.

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<v Speaker 2>It's from the late Pleistocene epic about fifty thousand years.

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<v Speaker 3>Ago, which is perfect for this kind of study because.

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<v Speaker 2>Fifty thousand years is well within the range for radiocarbon.

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<v Speaker 3>Dating, specifically carbon fourteen analysis.

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<v Speaker 2>Yeah, carbon fourteen has a half life of around five

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<v Speaker 2>seven hundred and thirty years.

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<v Speaker 3>Right exactly, So it's useless for dating billion year old

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<v Speaker 3>dinosaur bones, but it's incredible for higher resolution absolute dating

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<v Speaker 3>of the late Pleistocene.

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<v Speaker 2>So they anchored the timeline using fourteen C and then

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<v Speaker 2>map the isotopic variations across the jawbreaker layers, tracking.

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<v Speaker 3>The changing conditions of the lake from the inner core

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<v Speaker 3>of the stromatolite all the way out to its surface.

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<v Speaker 2>And the data from that isotopic gradient is basically the

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<v Speaker 2>smoking gun for this whole hydro thermal theory.

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<v Speaker 3>The signature is definitive. They looked at the ratios of

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<v Speaker 3>stable isotopes like oxygen eighteen to oxygen sixteen within those

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<v Speaker 3>carbonate layers, and.

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<v Speaker 2>They found a massive thermal gradient.

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<v Speaker 3>The inner layers, the oldest parts that formed first had

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<v Speaker 3>ratios corresponding to significantly elevated water.

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<v Speaker 2>Temperatures, proving that they formed in a highly active hydrothermal environment.

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<v Speaker 3>And then as you measure outward toward the younger layers

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<v Speaker 3>of the jawbreaker.

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<v Speaker 2>The ratios shift to show progressively cooler water.

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<v Speaker 3>Yes, what's fascinating here is this proves the structures began

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<v Speaker 3>growing during the hottest, earliest phase of the newly formed lake,

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<v Speaker 3>and they just.

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<v Speaker 2>Kept rowing as that subterranean melt sheet slowly ran out

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<v Speaker 2>of use over thousands.

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<v Speaker 3>Of years, until the hydrothermal spa eventually cooled down into

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<v Speaker 3>a standard ambient temperature lake.

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<v Speaker 2>They captured the entire thermodynamic life cycle of the IMPACT's aftermath.

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<v Speaker 2>That is incredible.

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<v Speaker 3>But wait, it gets better.

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<v Speaker 2>I'll laid on me.

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<v Speaker 3>The analysis showed that these microbial colonies were actually incorporating

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<v Speaker 3>extraterrestrial material into their structures.

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<v Speaker 2>Wait, really, remnants in the asteroid itself.

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<v Speaker 3>Yes, they mixed material from the impactor with the violently

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<v Speaker 3>altered local bedrock.

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<v Speaker 2>So they were literally metabolizing and building their homes out

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<v Speaker 2>of the fractured weapon that tried to destroy their environment.

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<v Speaker 3>It's the ultimate display of biological resourcefulness.

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<v Speaker 2>The asteroid delivered the heat, but its pulverized remains also

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<v Speaker 2>provided the exact trace minerals they needed to accelerate their.

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<v Speaker 3>Growth things like phosphorus and specific iron isotopes.

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<v Speaker 2>Okay, this force is a massive logical leap for me.

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<v Speaker 3>I think I know where you're gong with this.

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<v Speaker 2>If a local asteroid impact in South Korea fifty thousand

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<v Speaker 2>years ago can create a perfect self sustaining incubator for cyanobacteria.

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<v Speaker 3>We have to scale this up to the entire planet

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<v Speaker 3>billions of years ago.

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<v Speaker 2>Exactly, we have to talk about the Rkean eon roughly

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<v Speaker 2>two point four billion years.

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<v Speaker 3>Ago to lead up to the Great Oxidation Event or

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<v Speaker 3>the GOE.

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<v Speaker 2>Because if we connect this to the bigger picture, Earth

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<v Speaker 2>back then was completely alien.

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<v Speaker 3>It was fundamentally hostile to complex life.

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<v Speaker 2>The atmosphere had zero free oxygen. It was this toxic

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<v Speaker 2>soup of methane, ammonia and carbon.

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<v Speaker 3>Dioxide, and the global oceans were largely anoxic and highly

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<v Speaker 3>enriched and dissolved iron.

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<v Speaker 2>So if a primitive cyanobacteria colony tried to evolve and

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<v Speaker 2>photosynthesize out in the open ocean, it was basically doomed.

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<v Speaker 3>It faced an incredibly uphill.

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<v Speaker 2>Battle because any free oxygen they produced would instantly bond

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<v Speaker 2>with the ambient dissolved.

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<v Speaker 3>Iron right, Yes, it would scavenge the oxygen and precipitate

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<v Speaker 3>out as iron oxide.

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<v Speaker 2>Plus there was no ozone layer.

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<v Speaker 3>Yet, so the surface of the ocean was being continuously

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<v Speaker 3>bombarded by lethal levels of ultraviolet radiation.

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<v Speaker 2>The open ocean was a chemical sink and a radiation

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<v Speaker 2>death trap.

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<v Speaker 3>So the long standing mystery has always been how did

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<v Speaker 3>cyanobacteria ever establish a large enough population to overcome all that?

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<v Speaker 2>How did they eventually off gas enough oxygen to permanently

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<v Speaker 2>alter the atmosphere.

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<v Speaker 3>This is exactly where doctor Limb's team points to the

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<v Speaker 3>concept of the oxygen oasis.

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<v Speaker 2>And the Hapschian Crater provides the physical blueprint for it.

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<v Speaker 3>Think about the Archean eon, the Earth was experiencing a

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<v Speaker 3>vastly higher rate of asteroid bombardment.

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<v Speaker 2>Back then, the crust was just being repeatedly shattered by

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<v Speaker 2>space rocks.

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<v Speaker 3>And instead of seeing that as a series of extinction events,

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<v Speaker 3>this hydrothermal model suggests something totally different.

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<v Speaker 2>Every single impact was basically excavating a biologically optimized safe haven.

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<v Speaker 3>A crater lake offers massive advantages over the open ocean

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<v Speaker 3>on Earli Earth well.

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<v Speaker 2>First, off, the rim of the crater physically isolates the

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<v Speaker 2>lake from the global ocean.

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<v Speaker 3>Right, it acts as a bare against those turbulent iron

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<v Speaker 3>rich currents, stopping the immediate scavenging of the new oxygen.

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<v Speaker 2>And second, that hydrothermal circulation provides a constant upwelling of nutrients.

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<v Speaker 3>Right, completely independent of the nutrient starved surface waters of

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<v Speaker 3>the global ocean.

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<v Speaker 2>And third, the physical depth of a crater lake gives

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<v Speaker 2>you a thick collar of.

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<v Speaker 3>Water which attenuates and blocks that lethal UV radiation from

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<v Speaker 3>the sun.

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<v Speaker 2>Allowing the cyanobacteria to safely photosynthesize in the furtic zone.

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<v Speaker 3>So within these isolated, thermally regulated impact basins, the cyanobacteria

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<v Speaker 3>population could just absolutely boom.

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<v Speaker 2>Because it's localized. The oxygen they make eventually outpaces the

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<v Speaker 2>chemical sinks in the crater and.

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<v Speaker 3>The lake becomes completely saturated with free oxygen.

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<v Speaker 2>So are we saying that before the entire atmosphere became breathable,

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<v Speaker 2>life was essentially sheltering in these scattered asteroid made safe havens.

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<v Speaker 3>That is exactly what the data suggests.

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<v Speaker 2>Were these craters literally the localized engines that tip the

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<v Speaker 2>scale for the whole planet.

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<v Speaker 3>Yes, Once the local water column in a crater reached saturation,

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<v Speaker 3>all that excess oxygen had nowhere to go but up.

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<v Speaker 2>It would bubble up an off gas into the sky.

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<v Speaker 3>So the planetary scale transition of the Great Oxidation Event

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<v Speaker 3>probably didn't happen uniformly across the ocean.

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<v Speaker 2>It was driven by a decentralized network of millions of

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<v Speaker 2>these hydrothermal crater.

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<v Speaker 3>Lakes, all of them steadily pumping oxygen into the toxic

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<v Speaker 3>Artian sky.

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<v Speaker 2>Wow, the cosmic bombardment was literally terraforming the planet.

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<v Speaker 3>It provided the isolated, high energy sanctuaries that life required

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<v Speaker 3>to achieve critical mass.

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<v Speaker 2>The very mechanism we assume suppressed early life was actually

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<v Speaker 2>its greatest catalyst.

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<v Speaker 3>It beautifully resolves a major thermodynamic paradox in evolutionary biology.

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<v Speaker 2>Because major biological transitions require immense amounts of energy.

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<v Speaker 3>Right and highly specific stable chemical gradients.

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<v Speaker 2>Which a post impact environment provides perfectly. A massive spike

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<v Speaker 2>of kinetic energy converted into a sl low release thermal gradient.

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<v Speaker 3>Driving a localized chemical cycle for thousands and thousands of years.

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<v Speaker 2>Okay, here's where it gets really interesting.

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<v Speaker 3>Let's take it off world.

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<v Speaker 2>Exactly if this mechanism drove early life on Earth. We

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<v Speaker 2>can't just limit this to our own biosphere.

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<v Speaker 3>No, this terrestrial analog instantly becomes the ultimate diagnostic tool

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<v Speaker 3>for astrobiology.

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<v Speaker 2>Especially when we look at the planetary history of Mars.

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<v Speaker 3>When you look at the Noatian period of Mars, which

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<v Speaker 3>is roughly the same time as Earth's are Key and Eon,

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<v Speaker 3>the similarities are striking.

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<v Speaker 2>Mars had a thicker atmosphere back then, it had abundant

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<v Speaker 2>surface water.

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<v Speaker 3>And it was getting hammered by the exact same heavy

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<v Speaker 3>bombardment of asteroids that Earth was.

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<v Speaker 2>Its surface is still completely scarred with those ancient basins.

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<v Speaker 3>But unlike Earth, where plate tectonics and biological erosion have

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<v Speaker 3>wiped our early crater history clean, Mars essentially frozen place.

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<v Speaker 2>So the ancient paleo lakes of Mars are just sitting there,

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<v Speaker 2>structurally intact.

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<v Speaker 3>Which raises an important question. If impact craters on Earth

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<v Speaker 3>were the inky for microbial.

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<v Speaker 2>Life, then the dormant craters on Mars aren't just geological depressions.

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<v Speaker 3>They are the fossilized remains of potential alien nurseries.

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<v Speaker 2>And the Hapchien crater research totally alters how we investigate them.

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<v Speaker 3>Because until now, looking for life on Mars has been

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<v Speaker 3>like searching for a microscopic needle in a planetary haystack.

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00:16:19.440 --> 00:16:22.240
<v Speaker 2>We know water was there, so we send rovers to

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<v Speaker 2>ancient lake bits like the Jeesuro Crater.

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<v Speaker 3>But just knowing a basin ones held water isn't enough.

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<v Speaker 2>We need to know what specifically to look for, and

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<v Speaker 2>the hapchen stromatolites provide a literal treasure map.

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<v Speaker 3>They give us the precise isotopic fingerprint of impact driven

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<v Speaker 3>hydrothermal biology.

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<v Speaker 2>It's like a calibration tool for our rovers exactly.

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<v Speaker 3>Think about NASA's Perseverance rover driving around the Jezro crater

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<v Speaker 3>right now.

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<v Speaker 2>Jezero is an ancient impact basin that hosted a palaeolake.

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<v Speaker 3>Yes, and Perseverance has highly advanced spectroscopy instruments.

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<v Speaker 2>Like PixL, which maps the elemental composition of rocks at

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<v Speaker 2>a sub millimeter.

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00:17:00.600 --> 00:17:05.400
<v Speaker 3>Scale, and sholock, which scans for organic compounds and specific minerals.

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<v Speaker 2>But all that data requires a reference point.

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<v Speaker 3>Right if Perseverance finds a carbonate layer in the Jezro basin,

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<v Speaker 3>the hap gene study tells scientists the exact isotopic ratios

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<v Speaker 3>of carbon and oxygen to look for.

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00:17:17.359 --> 00:17:20.680
<v Speaker 2>To determine if it formed in a hot cooling hydrothermal gradient.

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<v Speaker 3>Furthermore, the South Korean data tells them to look for

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<v Speaker 3>extraterrestrial trace minerals bound within the.

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00:17:25.880 --> 00:17:29.880
<v Speaker 2>Rock, like those specific isotopes of strontium or the shocks

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00:17:29.920 --> 00:17:33.680
<v Speaker 2>toartz we talked about earlier, mixed right into the carbonate matrix.

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<v Speaker 3>We aren't just blindly looking for vague signs of past

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<v Speaker 3>water anymore.

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00:17:37.920 --> 00:17:40.839
<v Speaker 2>We know exactly what chemical fingerprints to look for when

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<v Speaker 2>the rover scrapes the dirt.

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00:17:42.319 --> 00:17:45.359
<v Speaker 3>We have the exact terrestrial reference spectrum for what a

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<v Speaker 3>microbial oasis looks like.

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<v Speaker 2>We've basically transitioned from blind exploration to highly targeted forensic geology.

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<v Speaker 3>It's a beautiful illustration of uniformitarianism in geology, but on

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<v Speaker 3>an interplanetary scale.

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<v Speaker 2>Meaning the physics that govern a crater in South Korea

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<v Speaker 2>are the same ones that operated on ancient Mars.

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<v Speaker 3>The fundamental laws of thermodynamics in geochemistry don't change just

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<v Speaker 3>because you're on another planet.

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<v Speaker 2>By rigorously studying this earthly discovery, we unlock the code

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<v Speaker 2>to hunt for astrobiology across the Solar System.

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<v Speaker 3>It's incredibly powerful let's bring.

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00:18:18.359 --> 00:18:20.680
<v Speaker 2>All these threads together, because the sheer scope of this

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00:18:20.839 --> 00:18:21.559
<v Speaker 2>is staggering.

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00:18:21.680 --> 00:18:23.799
<v Speaker 3>It really is a massive shift in perspective.

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<v Speaker 2>We start with a catastrophic event, a meteorite strike that

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<v Speaker 2>melts the crust and sterilizes the landscape.

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00:18:30.400 --> 00:18:34.400
<v Speaker 3>But beneath the destruction, a massive reservoir of heat is

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<v Speaker 3>trapped in the melt sheet.

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00:18:35.839 --> 00:18:39.920
<v Speaker 2>As water returns, that trapped heat drives a long term,

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<v Speaker 2>highly active.

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00:18:41.079 --> 00:18:46.839
<v Speaker 3>Mineral bath, turning a crater into a nutrient rich, protected bioreactor.

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00:18:46.119 --> 00:18:50.799
<v Speaker 2>Where microscopic cyanobacteria can thrive. Utilizing the minerals from the

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00:18:50.920 --> 00:18:53.240
<v Speaker 2>very asteroid that made the crater, They.

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00:18:53.039 --> 00:18:56.839
<v Speaker 3>Build their stromatolite structures, locking the thermal history of the

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00:18:56.920 --> 00:18:58.559
<v Speaker 3>lake into stone.

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00:18:58.200 --> 00:19:02.319
<v Speaker 2>And on early Earth, millions of these isolated oases pumped

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00:19:02.319 --> 00:19:06.039
<v Speaker 2>out oxygen until they literally changed the atmosphere of our planet.

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00:19:06.119 --> 00:19:09.440
<v Speaker 3>The violence of the cosmos provided the scaffolding for aerobic

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00:19:09.480 --> 00:19:10.759
<v Speaker 3>life to dominate.

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00:19:10.440 --> 00:19:13.440
<v Speaker 2>And now the chemical clues left behind in South Korea

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00:19:13.480 --> 00:19:16.480
<v Speaker 2>are guiding our rovers on Mars, telling them exactly where

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<v Speaker 2>to look for alien biology.

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00:19:18.000 --> 00:19:22.000
<v Speaker 3>It completely reframes our relationship with destructive cosmic phenomena.

399
00:19:22.200 --> 00:19:26.680
<v Speaker 2>It does it shows that complex biological systems require immense energy,

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00:19:26.960 --> 00:19:30.200
<v Speaker 2>and early on that energy is delivered through catastrophic impacts.

401
00:19:30.240 --> 00:19:34.480
<v Speaker 3>Destruction is an anomaly. It's a prerequisite step in chemical evolution.

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00:19:34.680 --> 00:19:36.599
<v Speaker 2>The next time you take a deep breath of oxygen,

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00:19:36.599 --> 00:19:37.519
<v Speaker 2>I want you to remember this.

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00:19:37.880 --> 00:19:40.680
<v Speaker 3>You owe a tiny fraction of that life giving gas

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00:19:40.960 --> 00:19:44.119
<v Speaker 3>to the cosmic violence of ancient asteroid impacts.

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00:19:44.440 --> 00:19:48.480
<v Speaker 2>The biological comfort we enjoy today is the downstream consequence

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00:19:48.559 --> 00:19:51.359
<v Speaker 2>of a terrifying era of planetary bombardment.

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00:19:51.559 --> 00:19:55.759
<v Speaker 3>We are literally breathing the biological dividends of falling stars.

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00:19:55.359 --> 00:19:58.279
<v Speaker 2>Which prompts a really provocative final thought for you to ponder.

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00:19:58.319 --> 00:19:59.559
<v Speaker 3>Oh, I'm curious where you're taking this.

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00:19:59.720 --> 00:20:02.759
<v Speaker 2>Well, if life on Earth utilize the chaotic destruction of

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00:20:02.839 --> 00:20:06.680
<v Speaker 2>asteroid impacts to build oxygen oases and terraform the.

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00:20:06.680 --> 00:20:09.559
<v Speaker 3>Planet, what other catastrophic events in the universe are doing

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00:20:09.640 --> 00:20:10.839
<v Speaker 3>the same thing Exactly?

415
00:20:11.119 --> 00:20:15.880
<v Speaker 2>What other seemingly destructive cosmic phenomena like the intense radiation

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00:20:15.920 --> 00:20:19.359
<v Speaker 2>of a nearby supernova or the tidal friction of massive

417
00:20:19.440 --> 00:20:22.519
<v Speaker 2>gas giants tearing a moon apart, are happening right now

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00:20:22.720 --> 00:20:25.960
<v Speaker 2>secretly planting the seeds for entirely new forms of life.
