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 Astronomie 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>You know, when we usually talk about the search for

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<v Speaker 2>life in the universe, we have this mental checklist. It's

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<v Speaker 2>almost like a recipe for biology.

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<v Speaker 3>Right, the standard astrobiology checklist Exactly.

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<v Speaker 2>We look for liquid water, we look for a source

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<v Speaker 2>of energy like the Sun or maybe a hot planetary core,

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<v Speaker 2>and we look for time, time for things to actually evolve.

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<v Speaker 3>And for the last twenty or thirty years, the moons

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<v Speaker 3>of Jupiter, specifically Europa, Ganymede, and Callisto, have been ticking

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<v Speaker 3>those boxes one by one.

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<v Speaker 2>They really have.

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<v Speaker 3>We've confirmed the subsurface oceans. We're pretty confident about the

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<v Speaker 3>energy sources, mainly tidal heating. They are prime real estate

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<v Speaker 3>in the astrobiology.

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<v Speaker 2>Market, time real estate. Yeah, but there's always been this

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<v Speaker 2>one nagging question mark, a gap in the resume, so

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<v Speaker 2>to speak, and that is the chemistry, specifically the.

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<v Speaker 3>Carbon, the actual stuff that life is built from.

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<v Speaker 2>Right, the building blocks. Yeah, because you can have all

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<v Speaker 2>the warm water in the universe and you can let

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<v Speaker 2>us sit there for four billion years. But if it's

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<v Speaker 2>just distilled water, you're not getting bacteria. You're just getting

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<v Speaker 2>a really excellent bath.

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<v Speaker 3>That is a very accurate, if slightly unscientific, way to

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<v Speaker 3>put it. Biology is at its core complex carbon chemistry.

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<v Speaker 2>It's not just water.

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<v Speaker 3>No, it's not. And for a long time, the prevailing

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<v Speaker 3>assumption in planetary science was that these moons formed as

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<v Speaker 3>these pristine, almost sterile.

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<v Speaker 2>Balls of ice, just pure water and rock.

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<v Speaker 3>Just water and rock frozen solid. And if you wanted

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<v Speaker 3>the good stuff, the amino acids, the complex organic molecules,

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<v Speaker 3>you essentially had to wait for delivery.

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<v Speaker 2>Like a cosmic delivery truck exactly.

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<v Speaker 3>You had to hope a comet or a carbon rich

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<v Speaker 3>asteroid would crash into the moon later on and deposit

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<v Speaker 3>those ingredients on the surface, which.

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<v Speaker 2>Is a bit of a depressing thought, isn't it. I mean,

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<v Speaker 2>it makes life feel accidental.

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<v Speaker 3>It makes it precarious.

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<v Speaker 2>Certain, Now, like you built the house, but you have

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<v Speaker 2>to wait for Amazon to deliver the furniture and the

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<v Speaker 2>driver might get completely lost.

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<v Speaker 3>It relies on chance. But the research we are doing

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<v Speaker 3>a deep dive into today completely flips that narrative on

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<v Speaker 3>its head. It suggests the furniture was built into the

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<v Speaker 3>house from day one.

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<v Speaker 2>I love that. So today we're exploring a really groundbreaking

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<v Speaker 2>set of papers. This is collaborative research from the Southwest

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<v Speaker 2>Research Institute x Marseille University in France and the Institute

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<v Speaker 2>for Advanced.

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<v Speaker 3>Studies Right they published two complementary studies, one in the

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<v Speaker 3>Planetary Science Journal and another in the Monthly Notices of

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<v Speaker 3>the Royal Astronomical Society.

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<v Speaker 2>These are major publications and their core thesis is pretty revolutionary.

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<v Speaker 2>It is they are arguing that you Ropa, Ganymede, Callisto,

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<v Speaker 2>and even Eo were not formed as clean white snowballs.

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<v Speaker 2>They argue that these loons likely accreted, meaning they gathered

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<v Speaker 2>up significant inventories of life building organic materials right from

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<v Speaker 2>the start, right as they were forming. And these materials

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<v Speaker 2>came from both the massive cloud that formed the Sun

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<v Speaker 2>and from the local disc of gas and dust spinning

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<v Speaker 2>around Jupiter itself.

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<v Speaker 3>So no waiting for a comet. The ingredients were baked.

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<v Speaker 2>In bacon and frozen in exactly before we get into

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<v Speaker 2>the how, and the how involves some incredibly cool simulation

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<v Speaker 2>work that we're going to break down. Let's define what

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<v Speaker 2>we are actually talking about here.

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<v Speaker 3>Good idea. We keep saying organics or ingredients, but I'm

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<v Speaker 3>guessing we aren't talking about, you know, sandwich meat floating

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<v Speaker 3>in space.

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<v Speaker 2>No, definitely not sandwich meat, though that would make space

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<v Speaker 2>exploration much more appetizing. We are talking about COMMS. That

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<v Speaker 2>stands for complex organic molecules COMBS.

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<v Speaker 3>Which sounds a bit like corporate jargon. But in astrobiology

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<v Speaker 3>that's a very specific term, right, It is.

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<v Speaker 2>A very specification. Now, complex is a relative term here.

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<v Speaker 2>Ahso well, in a high school biology class, complex might

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<v Speaker 2>mean a protein with thousands of atoms, a massive structure,

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<v Speaker 2>but in the context of deep space chemistry, the bar

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<v Speaker 2>is quite a bit lower. We generally define a COLM

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<v Speaker 2>as a carbon based molecule that has at least six atoms.

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<v Speaker 2>Six atoms that's the threshold, that is the magic number.

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<v Speaker 2>But crucially, it's not just carbon. It's carbon integrated with oxygen, nitrogen,

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<v Speaker 2>and hydrogen.

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<v Speaker 3>So we aren't just talking about methane, which is H four.

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<v Speaker 2>That's too simple, right, Methane is simple. We're talking about

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<v Speaker 2>things like methanol or dimethyl ether. These are molecules that

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<v Speaker 2>act as the structural precursors, the lego bricks, if you will,

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<v Speaker 2>for amino acids and nucleotides. So, if life is the castle,

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<v Speaker 2>the comms are the individual plastic bricks.

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<v Speaker 3>Precisely, you cannot build the castle without them. They form

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<v Speaker 3>the essential foundation for anything that could eventually become biological.

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<v Speaker 2>Okay, so where do these lego bricks actually come from?

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<v Speaker 2>Because space is it's space. It's a vacuum, it's freezing cold,

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<v Speaker 2>it's bombarded by radiation.

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<v Speaker 3>It's a hostile environment.

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<v Speaker 2>Yeah, it doesn't seem like a great place to do

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<v Speaker 2>delicate chemistry.

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<v Speaker 3>Yeah.

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<v Speaker 2>I usually think a chemistry happening in a beaker with

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<v Speaker 2>a Bunsen burner, not in the empty void.

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<v Speaker 3>You're entirely right. Space is a terrible place to do chemistry,

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<v Speaker 3>at least in the.

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<v Speaker 2>Gas phase, because things are too spread out.

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<v Speaker 3>Exactly, if you have two atoms floating in a vast vacuum,

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<v Speaker 3>the odds of them bumping into each other and deciding

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<v Speaker 3>to stick together to form a complex bond are astronomically low.

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<v Speaker 3>Nature needs a work space, a work.

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<v Speaker 2>Bench, and that work bench is dusty.

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<v Speaker 3>Icy grains, tiny microscopic particles. Think of them like dust bunnies,

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<v Speaker 3>but made of silicate's rock and coated in an incredibly

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<v Speaker 3>thin layers of ice.

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<v Speaker 2>Okay, so little frosted rocks.

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<v Speaker 3>Right, And in the early solar system, these grains are everywhere.

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<v Speaker 3>They are the fog that fills the protoplanetary system, and

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<v Speaker 3>the ice on them isn't just pure water ice.

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<v Speaker 2>It's dirty ice.

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<v Speaker 3>Very dirty ice contains volatiles, things like carbon monoxide, carbon dioxide,

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<v Speaker 3>and ammonia, all frozen together on the surface of this

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<v Speaker 3>tiny rock.

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<v Speaker 2>So you have a microscopic rock, it's coated in this

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<v Speaker 2>dirty ice mixture containing carbon and nitrogen. It's floating in

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<v Speaker 2>the dark. How does that turn into the precursor for

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<v Speaker 2>an amino acid. It needs a spark because otherwise it

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<v Speaker 2>would just sit there frozen forever.

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<v Speaker 3>What it needs energy. You need a catalyst to get

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<v Speaker 3>those atoms moving and rearranging themselves into new structures. The

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<v Speaker 3>research identifies two primary external stimuli that drive the synthesis.

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<v Speaker 2>In space, and the first one.

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<v Speaker 3>Is ultraviolet radiation UV photons from the young Sun. From

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<v Speaker 3>the Sun, yes, but also from the interstellar environment. In general,

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<v Speaker 3>the galaxy is full of UV radiation from massive young.

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<v Speaker 2>Stars, so the whole nebula is bathed in it exactly.

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<v Speaker 3>And when a high energy UV photon hits that icy grain,

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<v Speaker 3>it acts like a microscopic wrecking ball. It smashes into

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<v Speaker 3>the simple molecule, say a molecule of methanol frozen on

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<v Speaker 3>the surface, and it breaks the chemical bonds holding it together.

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<v Speaker 2>It snaps the legos bus, snaps them apart, and it

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<v Speaker 2>creates what we call radicals in chemistry, radicals.

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<v Speaker 3>I've heard of free radicals in health and diet discussions,

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<v Speaker 3>usually things we are told to avoid eating. But in space,

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<v Speaker 3>what are they?

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<v Speaker 2>They are essentially unhappy molecules or highly anxious molecules.

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<v Speaker 3>Unhappy molecules I like that.

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<v Speaker 2>Chemically speaking, they are fragments of molecules that have unpaired electrons.

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<v Speaker 2>Because they have an unpaired electron, they are highly aggressive.

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<v Speaker 2>They want to bond with something, anything, immediately, to stabilize themselves.

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<v Speaker 3>Okay, so you have this ice grain. The UV light hits,

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<v Speaker 3>it breaks a bunch of bonds, and suddenly you have

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<v Speaker 3>this swarm of highly reactive radicals trapped in the ice matrix.

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<v Speaker 2>And since they're trapped in the ice, they can't just

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<v Speaker 2>fly away. They grab the nearest.

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<v Speaker 3>Partner, and when they grab a partner, they build something new. Right.

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<v Speaker 3>When they recombine, they rarely go back to being the

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<v Speaker 3>simple molecule they were before. They form larger, weird chain es.

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<v Speaker 3>They form more complex structures. You smash two small things

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<v Speaker 3>and the pieces reassemble into one bigger thing. That is

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<v Speaker 3>the first mechanism for calmformation.

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<v Speaker 2>Okay, so UV light is the wrecking ball. What is

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<v Speaker 2>the second mechanism?

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<v Speaker 3>Thermal processing? Heat? But very specifically not too much heat.

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<v Speaker 3>This is a classic Goldilock situation.

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<v Speaker 2>Because if it's too hot, the ice just evaporates, right exactly.

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<v Speaker 3>If the temperature rises too much, the ice sublimates into gas.

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<v Speaker 3>The radicals fly away into the vacuum, and the chemistry stops.

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<v Speaker 3>Nothing happens.

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<v Speaker 2>But if it's too cold.

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<v Speaker 3>If it's too cold, the radicals are frozen strictly in

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<v Speaker 3>place and can't reach each other to bond. But if

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<v Speaker 3>you warm it up just enough, the ice lattice, the

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<v Speaker 3>crystal structure of the ice loosens up.

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<v Speaker 2>It gets kind of slushy.

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<v Speaker 3>At a molecular level, yes, it acts a bit like

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<v Speaker 3>a highly viscous liquid. The molecules can wiggle around. That

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<v Speaker 3>allows those trapped radicals to migrate slowly through the ice

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<v Speaker 3>and find each other to react.

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<v Speaker 2>So you need a kitchen that is irradiated by UV

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<v Speaker 2>and slightly warm, but definitely not an oven.

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<v Speaker 3>Perfect analogy, and the study points out that a protoplanetary disk,

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<v Speaker 3>which is the swirling disk of gas and dust around

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<v Speaker 3>a new born star, is basically a giant factory, perfectly

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<v Speaker 3>designed to create exactly these conditions because it's turbulent, highly

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<v Speaker 3>turbulent screens are constantly moving from cold, dark areas of

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<v Speaker 3>the disk into warmer, brighter areas and then getting swept

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<v Speaker 3>back out again.

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<v Speaker 2>Okay, so we have the mechanism, we know how to

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<v Speaker 2>make the molecules, we have the factory floor, which is

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<v Speaker 2>the disc. But the big mystery has always been how

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<v Speaker 2>do they actually get to Jupiter's mooms?

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<v Speaker 3>Right? Because Jupiter is really far out from the Sun.

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<v Speaker 2>It's far out, it's cold, and the early Solar system

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<v Speaker 2>was a chaotic mess. Just because you make a complex

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<v Speaker 2>molecule out by Neptune doesn't mean it gently lands on Europa.

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<v Speaker 3>Transport is the killer variable here, and this is where

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<v Speaker 3>the studies methodology gets really impressive. They didn't just guess

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<v Speaker 3>at how the transport happened. They built a digital time machine,

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<v Speaker 3>a computational model. Yes, but it's important under stand this

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<v Speaker 3>wasn't just one simple simulation. It was a complex coupling

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<v Speaker 3>of two massive physical models that traditionally don't even talk

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<v Speaker 3>to each other in planetary science.

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<v Speaker 2>What do you mean they don't talk to each other.

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<v Speaker 3>Well, usually in astrophysics you have research groups who model

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<v Speaker 3>the protosolar nebula that's the huge, massive disc of gas

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<v Speaker 3>and dust that formed the Sun and the entire planetary

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<v Speaker 3>system the macroscale right the grand scale, And then completely separately,

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<v Speaker 3>you have researchers who model the circumplanetary disc that is

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<v Speaker 3>the localized, much smaller subdisc spinning around Jupiter where the

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<v Speaker 3>gas giant and its specific moons formed.

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<v Speaker 2>So it's like a disc within a disc, a small

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<v Speaker 2>gear inside a massive.

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<v Speaker 3>Machine exactly, and the physics work very differently at those

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<v Speaker 3>different scales. It is notoriously difficult to simulate both at

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<v Speaker 3>the exact same time. It's akin to trying to simulate

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<v Speaker 3>the global weather patterns of the Earth and the specific

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<v Speaker 3>airflow in your living room in the same computer program.

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<v Speaker 2>That sounds computationally.

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<v Speaker 3>Expensive, dably so, but these researchers managed to do it.

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<v Speaker 3>They modeled the evolution of the massive protosolar nebula and

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<v Speaker 3>the local Jovian circumplanetary disk, and then they mathematically link

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<v Speaker 3>them together.

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<v Speaker 2>Oh kay, so they have the wind currents basically, Yeah,

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<v Speaker 2>how did they track the actual chemistry? Did they just

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<v Speaker 2>look at the average temperature of the whole system.

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<v Speaker 3>Now, they went much more granular than that. They utilized

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<v Speaker 3>a particle transport module. They essentially released thousands upon thousands

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<v Speaker 3>of digital dust grains into this massive simulation and track

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<v Speaker 3>their individual lives over millions of years.

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<v Speaker 2>Like putting tiny GPS trackers on individual specks of dust.

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<v Speaker 3>Precisely, they tracked every single time a specific grain moved

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<v Speaker 3>up or down in the disk, every time it drifted

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<v Speaker 3>inward toward the sun, every single photon of UV radiation

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<v Speaker 3>it absorbed, and every fractional degree of temperature change it experienced.

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<v Speaker 2>That is incredible fidelity. So they can say grain number

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<v Speaker 2>four do seventy two started in the deep outer Solar system,

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<v Speaker 2>drifted inward for a million years, lasted by UV light,

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<v Speaker 2>and then got sucked into Jupiter's orbit.

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<v Speaker 3>They can track exactly that life cycle, and by summing

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<v Speaker 3>up that incredibly detailed history for millions of particles, they

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<v Speaker 3>could calculate precisely how much organic material was being cooked

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<v Speaker 3>up and exactly where it was ending up within the

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<v Speaker 3>Jovian system.

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<v Speaker 2>They integrated the physics of the disc evolution with the

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<v Speaker 2>transport data to quantify the environmental history of the entire

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<v Speaker 2>grain population exactly.

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<v Speaker 3>It removes a lot of the guesswork.

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<v Speaker 2>And did they validate this against actual physical data or

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<v Speaker 2>is it purely a math exercise?

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<v Speaker 3>No validation is crucial here. Doctor Olivier Moses from seissuer

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<v Speaker 3>Ari made a very specific point of this. They compared

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<v Speaker 3>their model outputs with physical laboratory experiments. As you, they

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<v Speaker 3>essentially asked, if our computer model says a grain gets

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<v Speaker 3>exactly this much UV radiation and this much heat over time,

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<v Speaker 3>does the physical laboratory show that those specific conditions actually

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<v Speaker 3>produce complex organics?

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<v Speaker 2>And the answer was yes.

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<v Speaker 3>The answer was a definitive yes. The simulation confirms that

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<v Speaker 3>the dynamic physical environment of the early Solar System was

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<v Speaker 3>highly conducive to the synthesis of these specific molecules.

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<v Speaker 2>Okay, so this methodological framework, the time machine, leads us

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<v Speaker 2>to the study central finding regarding the origins of Jovian organics.

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<v Speaker 2>And this is what they call the dual source model.

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<v Speaker 3>Yes, the dual source model. This is the absolute headline

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<v Speaker 3>of the paper. They found that the organic material on

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<v Speaker 3>moons like Europa and Ganymede did not originate from a

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<v Speaker 3>single solitary location.

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<v Speaker 2>It came from two distinct reservoirs.

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<v Speaker 3>Right, Source A and Source B.

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<v Speaker 2>Let's break those down sequentially. Source A is the protosolar neibula,

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<v Speaker 2>the big main solar disc correct.

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<v Speaker 3>The simulation demonstrated that a massive amount of organic synthesis

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<v Speaker 3>happened way out in the general Solar System, long before

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<v Speaker 3>the material ever got anywhere near Jupiter.

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<v Speaker 2>Out in the deep freeze.

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<v Speaker 3>Right, the icy grains were drifting slowly through the outer regions,

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<v Speaker 3>getting hammered by background interstellar UV radiation. They were literally

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<v Speaker 3>accumulating calms just by floating there over millions of years.

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<v Speaker 2>Well, wait, I thought Jupiter creates a gap when a

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<v Speaker 2>giant planet forms, doesn't its massive gravity clear its orbit

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<v Speaker 2>like a snowplow clearing a street.

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<v Speaker 3>It absolutely does, and for a long time planetary scientists

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<v Speaker 3>assumed that gap was a hard barrier, that it would

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<v Speaker 3>effectively cut off the supply line of material from the

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<v Speaker 3>outer Solar.

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<v Speaker 2>System, like a moat around a castle. If Jupiter clears

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<v Speaker 2>the gap, how does fresh organic, rich dust from the

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<v Speaker 2>outside get in.

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<v Speaker 3>It is a moat, But the advanced hydrodynamic simulations in

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<v Speaker 3>this study show that the moat is surprisingly leaky leaky. Yes,

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<v Speaker 3>the gas and dust don't just stop. The pressure builds

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<v Speaker 3>up and the material actually spills over the edges of

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<v Speaker 3>the gap. It flows across the gap at higher altitudes

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<v Speaker 3>and spirals rapidly down into Jupiter's personal circumplanetary disk.

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<v Speaker 2>So the cosmic delivery trucks can actually cross the bridge.

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<v Speaker 3>They can cross the bridge, But the real variable was survival.

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<v Speaker 3>You are taking a very cold ice cre from deep

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<v Speaker 3>space and dropping it into the highly chaotic, dynamic, and

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<v Speaker 3>shockingly hot environment of a forming gas giant.

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<v Speaker 2>That sounds like a violent transition.

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<v Speaker 3>It is extremely violent. You have massive shock waves, intense

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<v Speaker 3>frictional heating. You would intuitively think the sudden heat would

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<v Speaker 3>just destroy the delicate organic.

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<v Speaker 2>Molecules, vaporize them, entirely, sterilize the package before it even

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<v Speaker 2>arrives at the Moon exactly.

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<v Speaker 3>But the model showed something counterintuitive. It showed that nearly

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<v Speaker 3>half fifty percent of the particles actually survived the trip.

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<v Speaker 2>Half of them.

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<v Speaker 3>Yes, they managed to stay just cold enough during the transition.

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<v Speaker 3>They successfully transferred their entire cargo of colms from the

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<v Speaker 3>larger solar nebula down into Jupiter's disk without undergoing major

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<v Speaker 3>chemical alteration or thermal destruction.

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<v Speaker 2>That is a surprisingly high survival rate. So half the

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<v Speaker 2>organic material on the Galilean moons is basically imported from

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<v Speaker 2>the rest of the Solar System.

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<v Speaker 3>Correct that ancient interstellar heritage is source A. But then

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<v Speaker 3>there is source B, the Jovian's circumplanetary.

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<v Speaker 2>Disc itself the local neighborhood, right.

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<v Speaker 3>The research found that Jupiter wasn't just passively collecting material

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<v Speaker 3>from the outside. It was functioning as its own chemical factory.

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<v Speaker 2>It was making its own organics locally.

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<v Speaker 3>Yes, the circumplanetary disc that swirling nursery directly around Jupiter

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<v Speaker 3>had its own localized Goldilock zones. If you think about

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00:16:24.240 --> 00:16:28.200
<v Speaker 3>the physics happening there. You have massive amounts of gas

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<v Speaker 3>swirling incredibly fast into Jupiter's.

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<v Speaker 2>Gravity well, and that creates friction.

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<v Speaker 3>Massive friction like rubbing your hands together vigorously on a

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<v Speaker 3>cold day, but on a planetary scale. This creates what

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<v Speaker 3>physicists call viscous heating.

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00:16:41.360 --> 00:16:42.159
<v Speaker 2>Viscous heating.

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<v Speaker 3>Yes, this viscous heating raised the ambient temperature in certain

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00:16:46.600 --> 00:16:49.759
<v Speaker 3>specific regions of Jupiter's disk just enough to trigger that

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00:16:49.840 --> 00:16:53.000
<v Speaker 3>exact thermal processing we talked about earlier, the slushy ice

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00:16:53.279 --> 00:16:56.279
<v Speaker 3>exactly so, even if the material crossing the gap from

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<v Speaker 3>the outside was completely dead and sterile Jupiter's local disc environment,

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<v Speaker 3>but have cooked that raw material into complex organics anyway.

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<v Speaker 2>This is a redundancy mentioned in the research. It's a

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<v Speaker 2>built in fail safe.

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<v Speaker 3>It is a brilliant natural fail safe. It means you

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<v Speaker 3>don't need to be exceptionally lucky to get organics. If

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<v Speaker 3>the solar nebula source fails, say the interstellar radiation wasn't

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<v Speaker 3>strong enough, the local viscous heating source kicks in and

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<v Speaker 3>does the job.

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00:17:20.400 --> 00:17:23.200
<v Speaker 2>And if the local source is too weak, the solar

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<v Speaker 2>nebula source covers the shortfall.

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<v Speaker 3>Exactly. The convergence of these two distinct mechanisms implies that

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<v Speaker 3>having organic rich moons isn't some rare anomaloust fluke. It

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<v Speaker 3>is a highly robust feature of the system.

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<v Speaker 2>It's an inevitable outcome of the physics. If you build

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<v Speaker 2>a gas giant, you are almost guaranteed to build organic

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<v Speaker 2>rich moons around it.

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<v Speaker 3>The presence of comms is essentially a structural guarantee.

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<v Speaker 2>That is huge. I want to pause on that for

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<v Speaker 2>a second because we always talk about the habitable zone

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<v Speaker 2>in astrobiology strictly in terms of distance from a host star.

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<v Speaker 2>We say Earth is in the zone, Mars is on

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<v Speaker 2>the edge, Venus is too close.

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<v Speaker 3>The traditional liquid water zone.

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00:18:03.680 --> 00:18:06.920
<v Speaker 2>Right. But this research suggests that gas giants carry their

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<v Speaker 2>own portable habitable chemistry sets with them regardless of where

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<v Speaker 2>they are.

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00:18:11.079 --> 00:18:13.279
<v Speaker 3>That is a phenomenal way to put it. A portable

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<v Speaker 3>chemistry set. The disc itself provides the necessary gradients of

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<v Speaker 3>heat and radiation.

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00:18:19.039 --> 00:18:21.359
<v Speaker 2>So let's talk about the final customers in this process.

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00:18:21.440 --> 00:18:26.000
<v Speaker 2>The Galilean moves themselves Europa, Ganymede, Callisto, and Io. They

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<v Speaker 2>are sitting there in this disk growing, sweeping up all

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<v Speaker 2>this material.

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00:18:30.079 --> 00:18:33.079
<v Speaker 3>They grow through a process called pebble accretion. That is

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<v Speaker 3>the current most accepted model in planetary science, pebble accretion. Yes,

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<v Speaker 3>they aren't just getting randomly hit by massive asteroids to grow.

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00:18:42.119 --> 00:18:45.920
<v Speaker 3>They are constantly sweeping up these centimeter sized pebbles of

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<v Speaker 3>ice and dust as they orbit through the.

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00:18:48.160 --> 00:18:50.400
<v Speaker 2>Disc like a vacuum cleaner, very much like that.

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00:18:51.000 --> 00:18:53.440
<v Speaker 3>And thanks to this dual source modeling, we now know

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<v Speaker 3>with high confidence that those pebbles were heavily loaded with colms.

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<v Speaker 2>So when Europa initially formed, it wasn't a pristine white

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<v Speaker 2>ball of ice that slowly got dirty over billions of

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00:19:03.960 --> 00:19:08.200
<v Speaker 2>years of comet impacts. It was what a dirty snowball

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00:19:08.319 --> 00:19:09.160
<v Speaker 2>right from the start.

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00:19:09.279 --> 00:19:13.079
<v Speaker 3>It would have been a profoundly muddy, organic rich slurry,

387
00:19:13.519 --> 00:19:16.400
<v Speaker 3>a dark mix of silicate rock, water, ice, and this

388
00:19:16.519 --> 00:19:19.839
<v Speaker 3>complex organic tar, all mixed together from day one.

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00:19:19.960 --> 00:19:23.119
<v Speaker 2>And this directly challenges the older pristine hypothesis.

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00:19:23.200 --> 00:19:27.240
<v Speaker 3>It completely dismantles it. The pristine hypothesis assumed the foundational

391
00:19:27.279 --> 00:19:30.079
<v Speaker 3>water was pure H two O, but this new model

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00:19:30.119 --> 00:19:33.839
<v Speaker 3>is accurate. These moons were chemically complex from their very inception, and.

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00:19:33.799 --> 00:19:36.079
<v Speaker 2>That matters tremendously because of what happens next in a

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00:19:36.079 --> 00:19:38.759
<v Speaker 2>moon's life cycle differentiation.

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00:19:38.440 --> 00:19:41.359
<v Speaker 3>Yes, the crucial stage of internal differentiation.

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00:19:41.519 --> 00:19:44.400
<v Speaker 2>That's when the moon gets hot and separates into layers.

397
00:19:45.000 --> 00:19:47.279
<v Speaker 2>The heavy stuff sinks to the metal, the light stuff

398
00:19:47.279 --> 00:19:48.440
<v Speaker 2>floats to the top. Right.

399
00:19:48.759 --> 00:19:51.759
<v Speaker 3>As these large moons grew, the immense pressure of their

400
00:19:51.839 --> 00:19:56.000
<v Speaker 3>own gravity, combined with heat from radioactive decay inside the rocks,

401
00:19:56.440 --> 00:20:00.160
<v Speaker 3>caused them to warm up internally. The vast quantities of

402
00:20:00.200 --> 00:20:01.599
<v Speaker 3>ice melted.

403
00:20:01.440 --> 00:20:04.200
<v Speaker 2>Creating the subsurface oceans exactly.

404
00:20:04.759 --> 00:20:07.880
<v Speaker 3>The heavy rocks sank to form a dense core, and

405
00:20:07.960 --> 00:20:11.519
<v Speaker 3>the liquid water formed the massive global mantle and the

406
00:20:11.799 --> 00:20:15.119
<v Speaker 3>icy crust on top. Now, think about the organics. If

407
00:20:15.119 --> 00:20:17.559
<v Speaker 3>the organics were just painted onto the surface much later

408
00:20:17.680 --> 00:20:20.400
<v Speaker 3>by random comets, they would just sit on top of

409
00:20:20.440 --> 00:20:21.279
<v Speaker 3>the frozen crust.

410
00:20:21.319 --> 00:20:24.160
<v Speaker 2>They might never actually reach the liquid ocean deep below.

411
00:20:24.319 --> 00:20:26.759
<v Speaker 3>They might remain isolated forever. But if they were built

412
00:20:26.759 --> 00:20:29.880
<v Speaker 3>directly into the structure of the Moon during pebble.

413
00:20:29.559 --> 00:20:34.000
<v Speaker 2>Accretion, then as the moon melted and differentiated, those organics

414
00:20:34.000 --> 00:20:37.000
<v Speaker 2>were turned right into the liquid mix exactly.

415
00:20:37.240 --> 00:20:39.480
<v Speaker 3>They would be in direct contact with the liquid water.

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00:20:39.559 --> 00:20:44.039
<v Speaker 3>Immediately they would be subjected to intense hydrothermal processing deep

417
00:20:44.119 --> 00:20:46.960
<v Speaker 3>inside the Moon at the boundary between the rocky core

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00:20:46.960 --> 00:20:47.599
<v Speaker 3>and the ocean.

419
00:20:47.680 --> 00:20:49.200
<v Speaker 2>This brings us to the s word.

420
00:20:49.519 --> 00:20:51.160
<v Speaker 3>Soup, primordial soup.

421
00:20:51.240 --> 00:20:53.880
<v Speaker 2>Yes, because that is really the fundamental question we are asking,

422
00:20:53.920 --> 00:20:57.680
<v Speaker 2>isn't it Are the subsurface oceans of Europa andganymy just

423
00:20:58.039 --> 00:21:02.000
<v Speaker 2>sterile salt water or are are they a complex chemical broth?

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00:21:02.359 --> 00:21:06.480
<v Speaker 3>This specific study strongly suggests it is a broth, and

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00:21:06.519 --> 00:21:10.599
<v Speaker 3>not just any broth, a highly potent prebiotic broth.

426
00:21:10.960 --> 00:21:13.559
<v Speaker 2>Break that down for me what actually happens chemically When

427
00:21:13.599 --> 00:21:16.519
<v Speaker 2>you take these space made comms, which remember are just

428
00:21:16.559 --> 00:21:19.960
<v Speaker 2>the precursors, and you soak them in warm pressurize liquid

429
00:21:20.039 --> 00:21:22.319
<v Speaker 2>water for four billion years, you.

430
00:21:22.359 --> 00:21:25.720
<v Speaker 3>Get a process called hydrolysis. You get extensive aqueous alteration

431
00:21:26.079 --> 00:21:29.000
<v Speaker 3>the specific molecular structures we see forming in the space environment,

432
00:21:29.039 --> 00:21:33.720
<v Speaker 3>things like hexamethylnetromine or HMT or various complex organic polymers.

433
00:21:34.000 --> 00:21:36.119
<v Speaker 3>When you subject them to liquid water, they break down

434
00:21:36.160 --> 00:21:40.240
<v Speaker 3>into very very interesting secondary structures, like what they transform

435
00:21:40.240 --> 00:21:45.559
<v Speaker 3>into amino acids. They transform into the nucleobases required for nucleotides.

436
00:21:45.240 --> 00:21:48.440
<v Speaker 2>The actual literal stuff of DNA and RNA.

437
00:21:48.319 --> 00:21:51.960
<v Speaker 3>The foundational components of life, as we understand it. In astrobiology,

438
00:21:52.000 --> 00:21:55.759
<v Speaker 3>we constantly discuss the bottlenecks for life, the immense hurdles

439
00:21:55.759 --> 00:21:57.440
<v Speaker 3>that stop life from initiating.

440
00:21:58.000 --> 00:22:00.799
<v Speaker 2>Usually we think the biggest bottle is just getting the

441
00:22:00.839 --> 00:22:03.480
<v Speaker 2>raw materials in the same place. Do we have enough

442
00:22:03.559 --> 00:22:06.079
<v Speaker 2>reactive nitrogen? Do we have enough reduced carbon?

443
00:22:06.240 --> 00:22:11.039
<v Speaker 3>Exactly? And this paper effectively states yes, the delivery truck arrived,

444
00:22:11.359 --> 00:22:14.640
<v Speaker 3>it emptied an immense cargo of the right materials, and

445
00:22:14.720 --> 00:22:16.279
<v Speaker 3>the planetary environment cooked it.

446
00:22:16.680 --> 00:22:19.720
<v Speaker 2>The study implies that the chemical barrier to habitability is

447
00:22:19.720 --> 00:22:21.480
<v Speaker 2>effectively removed for these worlds.

448
00:22:22.039 --> 00:22:24.400
<v Speaker 3>If you have a moon forming around a gas giant,

449
00:22:24.519 --> 00:22:29.200
<v Speaker 3>you inherently have the foundational ingredients. Consequently, the variables required

450
00:22:29.240 --> 00:22:32.559
<v Speaker 3>for habitability narrowed down significantly. It is no longer a

451
00:22:32.640 --> 00:22:35.240
<v Speaker 3>question of do we have the chemical bricks. It becomes

452
00:22:35.599 --> 00:22:38.720
<v Speaker 3>do we have the sustained energy and the solvent stability

453
00:22:38.759 --> 00:22:39.920
<v Speaker 3>to build something with them?

454
00:22:40.240 --> 00:22:43.039
<v Speaker 2>And we know there's energy. We know Europa has tidal

455
00:22:43.039 --> 00:22:44.440
<v Speaker 2>heating flexing its core.

456
00:22:44.720 --> 00:22:47.680
<v Speaker 3>We know the energy is there. So suddenly the mathematical

457
00:22:47.680 --> 00:22:51.319
<v Speaker 3>equation for life on a world like Europa looks much

458
00:22:51.480 --> 00:22:54.880
<v Speaker 3>much more favorable than it did under the pristine ice models.

459
00:22:55.359 --> 00:22:57.200
<v Speaker 2>Want to shift gears and talk about the odd one

460
00:22:57.200 --> 00:23:02.000
<v Speaker 2>out in this Galilean family. Ah Io is an absolute hellscape.

461
00:23:02.000 --> 00:23:06.759
<v Speaker 2>It's covered in active volcanoes, sulfur flows, lakes of lava.

462
00:23:07.079 --> 00:23:09.160
<v Speaker 2>There is no water ice to be found. But it

463
00:23:09.240 --> 00:23:12.160
<v Speaker 2>formed in the exact same disc right alongside Europa.

464
00:23:12.279 --> 00:23:15.960
<v Speaker 3>It did, and the transport model shows conclusively that ioaccreted

465
00:23:15.960 --> 00:23:19.279
<v Speaker 3>the exact same organic witch pebbles as Europa and Ganymede.

466
00:23:19.680 --> 00:23:22.799
<v Speaker 3>It started with the exact same astrobiological starter kit.

467
00:23:22.880 --> 00:23:24.200
<v Speaker 2>So what on Earth happened to it?

468
00:23:24.200 --> 00:23:27.039
<v Speaker 3>It simply got too close to the boss Io orbits

469
00:23:27.039 --> 00:23:29.839
<v Speaker 3>so close to Jupiter that the gravitational tidal forces are

470
00:23:29.920 --> 00:23:35.119
<v Speaker 3>absolutely immense. The physical friction generated deep inside Io literally

471
00:23:35.279 --> 00:23:36.599
<v Speaker 3>melts solid rock.

472
00:23:36.720 --> 00:23:38.200
<v Speaker 2>It drove off all the water.

473
00:23:38.119 --> 00:23:40.519
<v Speaker 3>It boiled away all the water into space, It drove

474
00:23:40.559 --> 00:23:43.720
<v Speaker 3>off all the volatile elements, and it undoubtedly pyalized, meaning

475
00:23:43.759 --> 00:23:46.480
<v Speaker 3>it essentially burned to a crisp all of those complex

476
00:23:46.599 --> 00:23:48.319
<v Speaker 3>organics billions of years ago.

477
00:23:48.680 --> 00:23:51.400
<v Speaker 2>So Io is what happens when you leave the prebiotic

478
00:23:51.480 --> 00:23:53.319
<v Speaker 2>cake in the oven at five thousand degrees.

479
00:23:53.480 --> 00:23:56.640
<v Speaker 3>That is exactly what it is, a charred remain. The

480
00:23:56.759 --> 00:23:59.839
<v Speaker 3>rich organic material that Io initially accreted would have been

481
00:23:59.839 --> 00:24:03.920
<v Speaker 3>a aggressively broken down into much simpler carbon and sulfur compounds.

482
00:24:04.480 --> 00:24:09.240
<v Speaker 3>This contributes heavily to Io's current bizarre exotic surface chemistry,

483
00:24:09.799 --> 00:24:12.920
<v Speaker 3>but it completely destroyed any potential for biology.

484
00:24:13.359 --> 00:24:16.160
<v Speaker 2>It really demonstrates that accretion is only the first chapter

485
00:24:16.200 --> 00:24:20.359
<v Speaker 2>of the story. The subsequent geological evolution determines the ultimate

486
00:24:20.400 --> 00:24:22.920
<v Speaker 2>fate of those delivered organics exactly.

487
00:24:23.000 --> 00:24:25.319
<v Speaker 3>Delivery is necessary but not sufficient.

488
00:24:25.680 --> 00:24:28.839
<v Speaker 2>And then on the other extreme there is Callisto, the

489
00:24:28.920 --> 00:24:29.720
<v Speaker 2>quiet sibling.

490
00:24:30.160 --> 00:24:34.240
<v Speaker 3>Callisto is scientifically fascinating precisely because it is the control

491
00:24:34.279 --> 00:24:37.799
<v Speaker 3>group in this grand experiment. It orbits much further out

492
00:24:37.839 --> 00:24:41.000
<v Speaker 3>from Jupiter. Because of that distance, it experiences very little

493
00:24:41.039 --> 00:24:42.039
<v Speaker 3>tidal heating.

494
00:24:42.319 --> 00:24:44.519
<v Speaker 2>So it didn't fully differentiate like Europa did.

495
00:24:44.680 --> 00:24:47.920
<v Speaker 3>Right. It is often described by planetary geologists as a

496
00:24:48.000 --> 00:24:51.440
<v Speaker 3>dirty ice ball that never truly separated completely into a

497
00:24:51.480 --> 00:24:55.160
<v Speaker 3>distinct rocky core and a pure water ocean. It's more mixed, So.

498
00:24:55.119 --> 00:24:58.240
<v Speaker 2>If we eventually send a lander to Callisto, we might.

499
00:24:58.160 --> 00:25:02.720
<v Speaker 3>Actually find the pristine foss of this entire accretion process.

500
00:25:03.359 --> 00:25:06.400
<v Speaker 3>The original palms might still be locked within the ice matrix.

501
00:25:06.599 --> 00:25:10.519
<v Speaker 3>Completely untouched, exactly as they were delivered four point five

502
00:25:10.640 --> 00:25:11.640
<v Speaker 3>billion years ago.

503
00:25:12.039 --> 00:25:15.880
<v Speaker 2>Well, Europa has been actively processing and recycling its organics

504
00:25:15.920 --> 00:25:19.079
<v Speaker 2>in a warm ocean, Callisto might just be storing them

505
00:25:19.119 --> 00:25:20.720
<v Speaker 2>in a deep dark freeze.

506
00:25:20.759 --> 00:25:24.319
<v Speaker 3>It is a profound cryogenic time capsule. That is a

507
00:25:24.440 --> 00:25:26.440
<v Speaker 3>highly compelling reason to visit Callisto.

508
00:25:26.599 --> 00:25:29.799
<v Speaker 2>And speaking of visits, we aren't just theorizing about these

509
00:25:29.839 --> 00:25:33.759
<v Speaker 2>moons on whiteboards anymore. We have major hardware currently on

510
00:25:33.759 --> 00:25:34.119
<v Speaker 2>the way.

511
00:25:34.200 --> 00:25:36.680
<v Speaker 3>We absolutely do. We are entering the golden age of

512
00:25:36.799 --> 00:25:37.880
<v Speaker 3>Jovian exploration.

513
00:25:38.240 --> 00:25:41.359
<v Speaker 2>NASA's Europa Clipper mission is en route and the European

514
00:25:41.440 --> 00:25:43.039
<v Speaker 2>Space Agency's Juice mission.

515
00:25:43.200 --> 00:25:45.559
<v Speaker 3>Juice stands for Jupiter icy Moons.

516
00:25:45.279 --> 00:25:48.480
<v Speaker 2>Explorer, Right, Both of these billion dollar spacecraft are flying

517
00:25:48.480 --> 00:25:51.279
<v Speaker 2>there now based strictly on the findings of this study.

518
00:25:51.359 --> 00:25:54.039
<v Speaker 2>What are their instruments actually looking for? If you were

519
00:25:54.039 --> 00:25:56.079
<v Speaker 2>the lead scientist sitting at the console, when the telemetry

520
00:25:56.119 --> 00:25:59.440
<v Speaker 2>starts flowing in, what specific data point tells you, Aha,

521
00:25:59.519 --> 00:26:01.279
<v Speaker 2>the dual source model was correct.

522
00:26:01.480 --> 00:26:03.759
<v Speaker 3>It ultimately comes down to isotopic ratios.

523
00:26:04.279 --> 00:26:05.359
<v Speaker 2>Explain the isotopes.

524
00:26:05.480 --> 00:26:08.400
<v Speaker 3>Isotopes are essentially chemical fingerprints. They tell you where a

525
00:26:08.440 --> 00:26:11.920
<v Speaker 3>molecule was born. Specifically, the instruments will look at the

526
00:26:12.000 --> 00:26:14.359
<v Speaker 3>ratio of deuterium to hydrogen.

527
00:26:14.559 --> 00:26:16.400
<v Speaker 2>Deuterium being heavy hydrogen.

528
00:26:16.599 --> 00:26:20.039
<v Speaker 3>Yes, deuterium is an isotope of hydrogen that possesses an

529
00:26:20.079 --> 00:26:23.640
<v Speaker 3>extra neutron, making it twice as heavy. Now, the physics

530
00:26:23.640 --> 00:26:27.240
<v Speaker 3>of chemical reactions dictate that in the incredibly cold dark

531
00:26:27.319 --> 00:26:30.799
<v Speaker 3>reaches of the interstellar medium and the far outer solar nebula,

532
00:26:31.160 --> 00:26:36.160
<v Speaker 3>reactions tend to strongly favor incorporating duterium over normal hydrogen.

533
00:26:35.799 --> 00:26:38.000
<v Speaker 2>Because the cold temperatures affect the reaction rates.

534
00:26:38.079 --> 00:26:40.559
<v Speaker 3>Yes, it relates to the zero point energy differences in

535
00:26:40.599 --> 00:26:43.559
<v Speaker 3>the chemical bonds. The result is that water and organics

536
00:26:43.599 --> 00:26:46.519
<v Speaker 3>formed in the deep cold are highly deuterium rich. They

537
00:26:46.519 --> 00:26:49.480
<v Speaker 3>have a very specific elevated signature.

538
00:26:49.279 --> 00:26:52.680
<v Speaker 2>Okay, and the material formed in the warmer local Jovian

539
00:26:52.759 --> 00:26:54.480
<v Speaker 2>disc via viscous heating.

540
00:26:54.920 --> 00:26:58.359
<v Speaker 3>That material formed at higher temperatures. Therefore, it would incorporate

541
00:26:58.440 --> 00:27:01.440
<v Speaker 3>much less deuterium. Its ice atopic ratio would look much

542
00:27:01.440 --> 00:27:03.759
<v Speaker 3>more like the standard baseline solar value.

543
00:27:03.839 --> 00:27:08.160
<v Speaker 2>So the Europa Clipper has sophisticated instruments like MASSPECS, the

544
00:27:08.200 --> 00:27:11.799
<v Speaker 2>massive mass spectrometer that can literally taste the dust flying

545
00:27:11.839 --> 00:27:12.839
<v Speaker 2>off the Moon's surface.

546
00:27:12.960 --> 00:27:16.119
<v Speaker 3>Masspex is an incredibly sensitive piece of hardware. It can

547
00:27:16.160 --> 00:27:20.319
<v Speaker 3>sniff the extremely tenuous gas plumes or analyze the microscopic

548
00:27:20.400 --> 00:27:23.799
<v Speaker 3>dust kicked up by micrometeorite impacts on the ice, and.

549
00:27:23.759 --> 00:27:26.599
<v Speaker 2>If it detects these complex organics in that dust, the

550
00:27:26.799 --> 00:27:29.599
<v Speaker 2>very first thing the science team will do is check

551
00:27:29.640 --> 00:27:32.680
<v Speaker 2>that deuterium to hydrogen ratio exactly and if the ratio

552
00:27:32.799 --> 00:27:33.480
<v Speaker 2>is very high.

553
00:27:33.599 --> 00:27:37.519
<v Speaker 3>A high ratio directly points to Source A. It confirms

554
00:27:37.519 --> 00:27:41.039
<v Speaker 3>the material originated in the distant solar nebula and possesses

555
00:27:41.119 --> 00:27:43.400
<v Speaker 3>that ancient interstellar heritage.

556
00:27:43.480 --> 00:27:45.359
<v Speaker 2>But if the ratio is mixed.

557
00:27:45.079 --> 00:27:48.160
<v Speaker 3>If they find a mixed isotopic signature, it serves as

558
00:27:48.240 --> 00:27:52.039
<v Speaker 3>direct observational conformation of the dual source model. It physically

559
00:27:52.079 --> 00:27:54.799
<v Speaker 3>confirms that Europa is a hybrid world built from both

560
00:27:54.839 --> 00:27:56.200
<v Speaker 3>distant and local material.

561
00:27:56.359 --> 00:28:00.279
<v Speaker 2>That is essentially molecular archaeology. Reconstructing the history of the

562
00:28:00.279 --> 00:28:03.240
<v Speaker 2>Solar System by sniffing gas puffs from a moon four

563
00:28:03.319 --> 00:28:04.599
<v Speaker 2>hundred million miles away.

564
00:28:04.839 --> 00:28:09.000
<v Speaker 3>It really is, and doctor Mouse's strongly emphasizes that connecting

565
00:28:09.039 --> 00:28:13.519
<v Speaker 3>this laboratory chemistry and the disk physics is absolutely essential

566
00:28:13.799 --> 00:28:16.880
<v Speaker 3>for interpreting the measurements these spacecraft will send back. The

567
00:28:16.880 --> 00:28:19.759
<v Speaker 3>theory provides the critical framework for the data.

568
00:28:19.400 --> 00:28:22.720
<v Speaker 2>And the SA Juice mission is focusing heavily on Ganymede. Right.

569
00:28:22.839 --> 00:28:26.279
<v Speaker 3>Yes, Ganimate is its primary target, and Ganymede is the

570
00:28:26.440 --> 00:28:29.759
<v Speaker 3>absolute giant of the system. It is the largest moon

571
00:28:29.880 --> 00:28:33.200
<v Speaker 3>in the entire Solar System. It is physically larger than

572
00:28:33.240 --> 00:28:34.119
<v Speaker 3>the planet Mercury.

573
00:28:34.200 --> 00:28:35.880
<v Speaker 2>It even has its own magnetic field.

574
00:28:36.000 --> 00:28:39.720
<v Speaker 3>It does and structurally it possesses a very deep, massive,

575
00:28:39.960 --> 00:28:43.680
<v Speaker 3>multi layered subsurface ocean. Because of its sheer size and

576
00:28:43.720 --> 00:28:48.039
<v Speaker 3>gravitational pull during formation, the raw volume of pebble material

577
00:28:48.079 --> 00:28:50.359
<v Speaker 3>Ganymede swept up is staggering.

578
00:28:50.440 --> 00:28:52.880
<v Speaker 2>So if this dual source model holds true, the sheer

579
00:28:52.920 --> 00:28:56.720
<v Speaker 2>tonnage of complex carbon stored inside ganymate is mind boggling.

580
00:28:56.839 --> 00:28:59.920
<v Speaker 3>It would act as a planetary scale organic storage tank with.

581
00:28:59.839 --> 00:29:02.440
<v Speaker 2>A global ocean sitting right underneath it waiting to mix.

582
00:29:02.559 --> 00:29:05.440
<v Speaker 3>Exactly. The astrobiological potential is immense.

583
00:29:05.599 --> 00:29:07.119
<v Speaker 2>I want to step back a bit and look at

584
00:29:07.119 --> 00:29:11.000
<v Speaker 2>the larger why should I care? Aspect of this research,

585
00:29:12.279 --> 00:29:15.000
<v Speaker 2>we have established that Jupiter's moons are highly likely to

586
00:29:15.039 --> 00:29:17.880
<v Speaker 2>be rich in the complex building blocks of life. We

587
00:29:17.960 --> 00:29:21.200
<v Speaker 2>have established a robust physical mechanism that explains exactly how

588
00:29:21.240 --> 00:29:23.440
<v Speaker 2>it happened. But this paper goes a step further in

589
00:29:23.480 --> 00:29:26.559
<v Speaker 2>its implications. It talks about the universality of these processes.

590
00:29:26.680 --> 00:29:30.119
<v Speaker 3>Yes, this is perhaps the most important takeaway. This isn't

591
00:29:30.119 --> 00:29:33.160
<v Speaker 3>strictly a story about Jupiter. It is a fundamental story

592
00:29:33.200 --> 00:29:36.359
<v Speaker 3>about how gas giants operate everywhere.

593
00:29:35.839 --> 00:29:39.279
<v Speaker 2>Because physics is physics, right. Fluid dynamics and gravity work

594
00:29:39.359 --> 00:29:42.079
<v Speaker 2>the exact same way in the Andromeda Galaxy as they

595
00:29:42.160 --> 00:29:43.480
<v Speaker 2>do right here in our Solar system.

596
00:29:43.559 --> 00:29:48.279
<v Speaker 3>Precisely the specific processes the researchers modeled the viscous heating

597
00:29:48.359 --> 00:29:51.680
<v Speaker 3>of the gas, the ultraviolet rradiation of the grains, the

598
00:29:51.720 --> 00:29:55.000
<v Speaker 3>mechanics of pebble accretion, the hydrodynamic flow across the gap.

599
00:29:55.240 --> 00:29:57.039
<v Speaker 3>These are universal physical laws.

600
00:29:57.119 --> 00:29:59.839
<v Speaker 2>So every time a gas giant forms around any star,

601
00:30:00.079 --> 00:30:01.759
<v Speaker 2>it should behave Similarly.

602
00:30:01.440 --> 00:30:03.799
<v Speaker 3>Every single time a gas giant forms, it generates a

603
00:30:03.839 --> 00:30:07.440
<v Speaker 3>circumplanetary disc, it clears a gap in its local nebula.

604
00:30:07.519 --> 00:30:11.319
<v Speaker 3>It naturally creates these precise thermal and radiation zones, And

605
00:30:11.480 --> 00:30:12.119
<v Speaker 3>if we look.

606
00:30:12.000 --> 00:30:17.119
<v Speaker 2>At the current exoplanet data, our telescopes have found thousands

607
00:30:17.160 --> 00:30:18.319
<v Speaker 2>of gas giants.

608
00:30:18.039 --> 00:30:21.079
<v Speaker 3>Out there, thousands of them. We call them Jovians or

609
00:30:21.119 --> 00:30:25.119
<v Speaker 3>super Jovians, and a significant percentage of them are located

610
00:30:25.200 --> 00:30:28.519
<v Speaker 3>in the habitable zones of their respective host stars, or

611
00:30:28.559 --> 00:30:30.359
<v Speaker 3>even further out in the colder regions.

612
00:30:30.640 --> 00:30:34.799
<v Speaker 2>If this accretion mechanism is truly universal, then every single

613
00:30:34.839 --> 00:30:38.039
<v Speaker 2>one of those thousands of gas giants likely possesses a

614
00:30:38.079 --> 00:30:39.400
<v Speaker 2>system of moons.

615
00:30:39.240 --> 00:30:43.079
<v Speaker 3>And those moons, dictated by this exact physics, should be

616
00:30:43.119 --> 00:30:46.519
<v Speaker 3>heavily loaded with complex organics from the moment they coalesce.

617
00:30:46.680 --> 00:30:49.240
<v Speaker 2>It implies that the universe is essentially functioning as a

618
00:30:49.359 --> 00:30:53.240
<v Speaker 2>massive automated factory for manufacturing habitable moons.

619
00:30:53.319 --> 00:30:56.480
<v Speaker 3>It suggests a paradigm shift. It suggests that the chemical

620
00:30:56.519 --> 00:30:59.359
<v Speaker 3>habitable zone isn't restricted to a narrow band around a star.

621
00:31:00.000 --> 00:31:03.079
<v Speaker 3>Our habitable zone is effectively the entire galaxy. We used

622
00:31:03.079 --> 00:31:04.759
<v Speaker 3>to rigidly think you had to be in a very

623
00:31:04.799 --> 00:31:07.400
<v Speaker 3>specific lucky spot to get the chemistry.

624
00:31:07.039 --> 00:31:09.960
<v Speaker 2>Right, just the right distance, just the right planet size.

625
00:31:09.960 --> 00:31:13.680
<v Speaker 3>But this study says no, The formation disc itself manufactures

626
00:31:13.720 --> 00:31:16.640
<v Speaker 3>the necessary chemistry and actively transports it to the growing

627
00:31:16.680 --> 00:31:17.680
<v Speaker 3>planetary bodies.

628
00:31:17.839 --> 00:31:22.279
<v Speaker 2>That is, a profound philosophical shift. It moves the concept

629
00:31:22.319 --> 00:31:27.319
<v Speaker 2>of life from being a lucky, highly contingent accident of

630
00:31:27.400 --> 00:31:33.119
<v Speaker 2>location to being an almost inevitable consequence of standard planetary formation.

631
00:31:33.400 --> 00:31:37.000
<v Speaker 3>It strongly indicates that the fundamental ingredients for life are

632
00:31:37.160 --> 00:31:41.000
<v Speaker 3>standard equipment for planetary systems rather than premium upgrades.

633
00:31:41.079 --> 00:31:43.559
<v Speaker 2>But of course having the ingredients in the bowl isn't

634
00:31:43.599 --> 00:31:45.039
<v Speaker 2>the same as having a baked cake.

635
00:31:45.279 --> 00:31:48.440
<v Speaker 3>Absolutely not. You still require the spark, you still require

636
00:31:48.599 --> 00:31:52.000
<v Speaker 3>long term environmental stability. We have not found life yet.

637
00:31:52.319 --> 00:31:54.599
<v Speaker 3>But what this research does is force us to stop

638
00:31:54.640 --> 00:31:56.440
<v Speaker 3>making excuses about the chemistry.

639
00:31:56.640 --> 00:31:58.880
<v Speaker 2>You can't say, oh, maybe there's just no carbon out

640
00:31:58.920 --> 00:31:59.519
<v Speaker 2>there in the dark.

641
00:32:00.039 --> 00:32:03.039
<v Speaker 3>Carbon is there, The nitrogen is there, the liquid water

642
00:32:03.200 --> 00:32:04.680
<v Speaker 3>is there, the energy is there.

643
00:32:04.799 --> 00:32:05.960
<v Speaker 2>The table is fully set.

644
00:32:06.039 --> 00:32:07.920
<v Speaker 3>The table is set, and now the scientific community just

645
00:32:07.920 --> 00:32:09.920
<v Speaker 3>has to send the probes to see if anything actually

646
00:32:09.920 --> 00:32:10.799
<v Speaker 3>showed up for dinner.

647
00:32:10.920 --> 00:32:13.119
<v Speaker 2>And that is exactly what Clipper and Juice are going

648
00:32:13.200 --> 00:32:14.680
<v Speaker 2>to tell us in the coming decade.

649
00:32:14.799 --> 00:32:17.680
<v Speaker 3>Fingers crossed, the data return will be historic.

650
00:32:17.920 --> 00:32:20.599
<v Speaker 2>One specific detail in the paper I found really mechanically

651
00:32:20.599 --> 00:32:24.039
<v Speaker 2>interesting was the nitrogen issue. You mentioned nitrogen earlier as

652
00:32:24.039 --> 00:32:27.720
<v Speaker 2>a key component why is that specific element so notoriously

653
00:32:27.759 --> 00:32:28.599
<v Speaker 2>trimplet to model?

654
00:32:28.880 --> 00:32:32.319
<v Speaker 3>Nitrogen is highly volatile in the raw environment of the

655
00:32:32.359 --> 00:32:35.640
<v Speaker 3>solar nebula, it strongly prefers to exist as end two

656
00:32:35.720 --> 00:32:37.599
<v Speaker 3>gas molecular.

657
00:32:37.279 --> 00:32:39.640
<v Speaker 2>Nitrogen, like our atmosphere on Earth exactly.

658
00:32:40.160 --> 00:32:42.720
<v Speaker 3>And the physical problem is that it is exceptionally hard

659
00:32:42.720 --> 00:32:44.920
<v Speaker 3>to build a solid planet or moon out of a gas.

660
00:32:45.279 --> 00:32:47.680
<v Speaker 3>It doesn't stick to the grains, it doesn't freeze onto

661
00:32:47.680 --> 00:32:51.799
<v Speaker 3>the ice until the ambient temperature drops incredibly low, significantly

662
00:32:51.799 --> 00:32:53.359
<v Speaker 3>colder than the orbit of Pluto.

663
00:32:53.720 --> 00:32:56.920
<v Speaker 2>So how do you possibly get enough solid nitrogen into

664
00:32:57.039 --> 00:32:59.400
<v Speaker 2>a forming rock and ice moon like Europa?

665
00:32:59.519 --> 00:33:02.839
<v Speaker 3>That has It's been a major theoretical puzzle. If Europa

666
00:33:02.920 --> 00:33:05.599
<v Speaker 3>just accreted pure water ouse and silicate dust, it would

667
00:33:05.599 --> 00:33:10.440
<v Speaker 3>be severely nitrogen pore and biology absolutely requires nitrogen. Amino

668
00:33:10.480 --> 00:33:14.160
<v Speaker 3>Acids are literally amines. They're built around nitrogen groups. DNA

669
00:33:14.359 --> 00:33:17.920
<v Speaker 3>utilizes neitrogenous spaces. No nitrogen simply no life.

670
00:33:18.079 --> 00:33:20.519
<v Speaker 2>So how did the dual source calm model solve this

671
00:33:20.640 --> 00:33:21.920
<v Speaker 2>missing nitrogen problem?

672
00:33:22.000 --> 00:33:24.960
<v Speaker 3>The study details how the synthesis of comms actively traps

673
00:33:24.960 --> 00:33:29.400
<v Speaker 3>the volatile nitrogen. The chemical reactions form things like complex ammonia,

674
00:33:29.480 --> 00:33:33.240
<v Speaker 3>salts or organic amines that remain in a solid state

675
00:33:33.279 --> 00:33:35.559
<v Speaker 3>and much higher temperatures than end two gas.

676
00:33:35.799 --> 00:33:39.559
<v Speaker 2>So the complex organic chemistry acts like a molecular trap.

677
00:33:40.039 --> 00:33:43.119
<v Speaker 2>It grabs the slippery nitrogen gas out of the nebula

678
00:33:43.440 --> 00:33:46.640
<v Speaker 2>and locks it securely into a solid heavy molecule.

679
00:33:46.839 --> 00:33:50.480
<v Speaker 3>That is the exact mechanism. It chemically sequested the volatile

680
00:33:50.559 --> 00:33:53.559
<v Speaker 3>nitrogen directly into the physical structure of the dust grains.

681
00:33:54.079 --> 00:33:57.079
<v Speaker 3>So when the Galilean moons swept up and accreted that dust,

682
00:33:57.359 --> 00:33:59.839
<v Speaker 3>they got the critical nitrogen delivered for free.

683
00:34:00.119 --> 00:34:02.799
<v Speaker 2>This solid phase delivery mechanism is critical.

684
00:34:03.000 --> 00:34:06.039
<v Speaker 3>Without the specific mechanism, the moons might be incredibly rich

685
00:34:06.079 --> 00:34:10.320
<v Speaker 3>in liquid water and carbon, but lethally nitrogen pore, which

686
00:34:10.360 --> 00:34:15.079
<v Speaker 3>would represent a severe, perhaps insurmountable constraint on their biological potential.

687
00:34:15.239 --> 00:34:19.679
<v Speaker 2>The commaccretion model comprehensively explains how the n in hnops

688
00:34:19.960 --> 00:34:24.559
<v Speaker 2>carbon hydrogen, nitrogen, oxygen, phosphorus sulfur physically arrives at the moons.

689
00:34:24.719 --> 00:34:27.199
<v Speaker 3>Yes, it solves a major mass balance issue in the

690
00:34:27.199 --> 00:34:28.199
<v Speaker 3>planetary chemistry.

691
00:34:28.480 --> 00:34:31.599
<v Speaker 2>It's incredible how many little physical and chemical things have

692
00:34:31.679 --> 00:34:34.960
<v Speaker 2>to go exactly right. But the mathematical model seems to

693
00:34:34.960 --> 00:34:37.639
<v Speaker 2>show that they do go right, naturally and reliably.

694
00:34:38.000 --> 00:34:40.880
<v Speaker 3>That is the structural beauty of it. It isn't a

695
00:34:40.920 --> 00:34:44.800
<v Speaker 3>fragile Rube Goldberg machine where one tiny slip up ruins

696
00:34:44.840 --> 00:34:50.199
<v Speaker 3>the entire sequence. It is a physically robust Redungdent system.

697
00:34:50.519 --> 00:34:55.159
<v Speaker 3>The fundamental physics of the universe actively favors the generation

698
00:34:55.360 --> 00:34:56.639
<v Speaker 3>of chemical complexity.

699
00:34:56.800 --> 00:34:58.800
<v Speaker 2>I want to circle back to the methodology one last

700
00:34:58.840 --> 00:35:03.880
<v Speaker 2>time because Olivia Amousis from Cessyri made a compelling point

701
00:35:03.880 --> 00:35:05.400
<v Speaker 2>about connecting the lab to the sky.

702
00:35:05.639 --> 00:35:09.880
<v Speaker 3>Yes, this represents the new gold standard in planetary science methodology.

703
00:35:09.920 --> 00:35:12.719
<v Speaker 3>You can't just be a traditional astronomer solely looking through

704
00:35:12.719 --> 00:35:15.320
<v Speaker 3>a telescope anymore. And you can't just be a theoretical

705
00:35:15.360 --> 00:35:17.679
<v Speaker 3>coder writing pure simulations.

706
00:35:17.079 --> 00:35:18.960
<v Speaker 2>In a vacuum. You actually have to get your hands dirty.

707
00:35:18.960 --> 00:35:22.039
<v Speaker 3>In a physical lab, you have to execute the empirical chemistry.

708
00:35:22.199 --> 00:35:26.400
<v Speaker 3>They literally utilize advanced vacuum chambers in these laboratories, specifically

709
00:35:26.480 --> 00:35:31.519
<v Speaker 3>at x Marseille and Cessarri, where they meticulously create fake space.

710
00:35:31.639 --> 00:35:32.320
<v Speaker 2>How do they do that.

711
00:35:32.480 --> 00:35:35.960
<v Speaker 3>They physically cool a metallic surface down to ten kelvin

712
00:35:36.039 --> 00:35:40.360
<v Speaker 3>near absolute zero. They then spray precise ratios of water

713
00:35:40.440 --> 00:35:44.760
<v Speaker 3>and methanol vapor onto it to manufacture microscopic layers of ice,

714
00:35:45.480 --> 00:35:48.920
<v Speaker 3>and then they blast that synthetic ice with high powered.

715
00:35:48.760 --> 00:35:51.920
<v Speaker 2>UV lasers just to see exactly what happens to the molecule.

716
00:35:52.000 --> 00:35:56.079
<v Speaker 3>To empirically measure the reaction rates, they ask how fast

717
00:35:56.159 --> 00:35:59.519
<v Speaker 3>does methanol break down under this exact photon flex, how

718
00:35:59.599 --> 00:36:03.679
<v Speaker 3>much secific thermal energy does it actually take to synthesize glyclaldehyde?

719
00:36:03.760 --> 00:36:06.000
<v Speaker 2>And then they take those hard empirical numbers from the

720
00:36:06.039 --> 00:36:09.199
<v Speaker 2>physical lab and plug them directly into the computer code exactly.

721
00:36:09.639 --> 00:36:14.039
<v Speaker 3>This grounds the simulation and reduces the theoretical uncertainty significantly.

722
00:36:14.199 --> 00:36:16.239
<v Speaker 3>We are no longer guessing if the chemistry happens. We

723
00:36:16.320 --> 00:36:20.119
<v Speaker 3>mathematically know it happens under those specific physical conditions, and

724
00:36:20.159 --> 00:36:24.239
<v Speaker 3>the hydrodynamic model verifies those exact conditions existed in the

725
00:36:24.320 --> 00:36:25.000
<v Speaker 3>Jovian disc.

726
00:36:25.320 --> 00:36:29.079
<v Speaker 2>It makes the findings feel much much more solid. It

727
00:36:29.119 --> 00:36:32.000
<v Speaker 2>isn't just we theorized this might happen, it's we observe

728
00:36:32.039 --> 00:36:34.960
<v Speaker 2>this happening in the lab, and the computational physics confirm

729
00:36:35.079 --> 00:36:38.840
<v Speaker 2>the early solar system matched the lab conditions perfectly precisely.

730
00:36:39.400 --> 00:36:43.360
<v Speaker 3>It rigorously bridges the massive gap between the microscopic realm

731
00:36:43.519 --> 00:36:47.320
<v Speaker 3>individual atoms reacting on an ice surface and the macroscopic

732
00:36:47.400 --> 00:36:49.920
<v Speaker 3>realm giant planets forming in a stellar disc.

733
00:36:50.199 --> 00:36:54.000
<v Speaker 2>The particle transport module in the paper also specifically highlighted

734
00:36:54.239 --> 00:36:58.559
<v Speaker 2>radial migration and vertical migration. Can we unpack that fluid

735
00:36:58.639 --> 00:37:01.519
<v Speaker 2>dynamics aspect a bit more because it sounds like these

736
00:37:01.519 --> 00:37:04.440
<v Speaker 2>microscopic grains are undergoing epic journeys.

737
00:37:04.639 --> 00:37:08.599
<v Speaker 3>They absolutely are. The protoplanetary disk is not a static

738
00:37:08.719 --> 00:37:12.599
<v Speaker 3>flat ring. It is a highly turbulent, three dimensional swirling

739
00:37:12.639 --> 00:37:15.719
<v Speaker 3>cloud of gas. Vertical migration means the dust grains are

740
00:37:15.719 --> 00:37:18.559
<v Speaker 3>constantly being lofted high up above the dense midplane of

741
00:37:18.599 --> 00:37:21.599
<v Speaker 3>the disk and then slowly settling back down due to gravity,

742
00:37:21.679 --> 00:37:22.440
<v Speaker 3>like dust.

743
00:37:22.199 --> 00:37:23.840
<v Speaker 2>Modes circulating in a drafty room.

744
00:37:24.119 --> 00:37:27.039
<v Speaker 3>Very much though, But this vertical circulation is crucial for

745
00:37:27.039 --> 00:37:29.960
<v Speaker 3>the chemistry because the ultraviolet radiation from the young Sun

746
00:37:30.159 --> 00:37:33.400
<v Speaker 3>cannot physically penetrate deep into the dense, thick midplane of

747
00:37:33.440 --> 00:37:36.039
<v Speaker 3>the disc. The midplane is completely dark.

748
00:37:36.000 --> 00:37:38.440
<v Speaker 2>So only the upper surface layers get irradiated by the

749
00:37:38.559 --> 00:37:39.480
<v Speaker 2>UV wrecking.

750
00:37:39.199 --> 00:37:42.760
<v Speaker 3>Balls right, So this vertical cycling effectively acts like a

751
00:37:42.800 --> 00:37:47.199
<v Speaker 3>massive conveyor belt. It actively brings fresh simple grains up

752
00:37:47.280 --> 00:37:51.159
<v Speaker 3>to the irradiated surface, zaps them with UV photons to

753
00:37:51.239 --> 00:37:54.800
<v Speaker 3>generate those reactive radicals, and then cycles and back down

754
00:37:54.880 --> 00:37:57.880
<v Speaker 3>deep into the darker, warmer midplane where they can thermally

755
00:37:57.960 --> 00:37:59.000
<v Speaker 3>process safely.

756
00:37:59.320 --> 00:38:02.119
<v Speaker 2>So the inherent turbulence of the gas is actually driving

757
00:38:02.199 --> 00:38:03.639
<v Speaker 2>the complex chemistry.

758
00:38:03.719 --> 00:38:07.440
<v Speaker 3>It is the essential engine. Without that vertical turbulence, the

759
00:38:07.519 --> 00:38:10.639
<v Speaker 3>grains would simply sit in the dark midplane forever and

760
00:38:10.760 --> 00:38:15.159
<v Speaker 3>nothing complex would ever synthesize. The dynamic mixing is mandatory.

761
00:38:15.239 --> 00:38:16.559
<v Speaker 2>And what about radial migration.

762
00:38:16.880 --> 00:38:20.639
<v Speaker 3>Radial migration describes the movement inward toward or outward away

763
00:38:20.719 --> 00:38:24.719
<v Speaker 3>from the central star. The study relies heavily on the concept.

764
00:38:24.320 --> 00:38:26.599
<v Speaker 2>Of gas drag friction with the nebula.

765
00:38:26.639 --> 00:38:30.159
<v Speaker 3>Exactly as the solid grains orbit, they constantly feel the

766
00:38:30.199 --> 00:38:34.559
<v Speaker 3>aerodynamic friction of the surrounding gas. This drag slowly robs

767
00:38:34.599 --> 00:38:37.760
<v Speaker 3>them of orbital momentum, causing them to gradually spiral inward

768
00:38:37.880 --> 00:38:41.000
<v Speaker 3>toward the center toward Jupiter's feeding zone toward the Sun

769
00:38:41.079 --> 00:38:44.639
<v Speaker 3>initially and eventually directly into the gravitational feeding zone of

770
00:38:44.639 --> 00:38:48.079
<v Speaker 3>the forming Jupiter. Now, the speed of this inward migration

771
00:38:48.199 --> 00:38:50.199
<v Speaker 3>depends heavily on the physical size of.

772
00:38:50.199 --> 00:38:53.119
<v Speaker 2>The grain, which is why they focus on specific sizes right.

773
00:38:53.000 --> 00:38:56.239
<v Speaker 3>The study specifically focuses on grains in the micrometer to

774
00:38:56.320 --> 00:39:02.199
<v Speaker 3>millimeter size range, the pebbles pebbles. These precise sizes possess

775
00:39:02.280 --> 00:39:06.159
<v Speaker 3>the exact aerodynamic properties to be most susceptible to gas drag.

776
00:39:06.519 --> 00:39:09.159
<v Speaker 3>If the dust grains are too small, they remain perfectly

777
00:39:09.239 --> 00:39:12.079
<v Speaker 3>coupled to the gas and just float along with it indefinitely.

778
00:39:12.480 --> 00:39:15.159
<v Speaker 3>If they are too massive, like a boulder, they simply

779
00:39:15.199 --> 00:39:16.760
<v Speaker 3>plow through the gas unaffected.

780
00:39:16.880 --> 00:39:20.559
<v Speaker 2>But these specific millimeter pebbles hit the aerodynamic sweet spot

781
00:39:20.920 --> 00:39:23.840
<v Speaker 2>they drift perfectly into the planetary accretion zones.

782
00:39:24.039 --> 00:39:27.159
<v Speaker 3>The hydrodynamic simulations clearly show that these pebbles are the

783
00:39:27.199 --> 00:39:30.440
<v Speaker 3>primary hyper efficient vectors for delivering the bulk colms to

784
00:39:30.480 --> 00:39:31.320
<v Speaker 3>the growing moons.

785
00:39:31.440 --> 00:39:34.159
<v Speaker 2>It is truly amazing to think that the profound building

786
00:39:34.199 --> 00:39:38.039
<v Speaker 2>blocks of biology are basically delivered by cosmic gravel.

787
00:39:38.239 --> 00:39:41.199
<v Speaker 3>It is humbling, and the sheer physical volume of that

788
00:39:41.320 --> 00:39:45.400
<v Speaker 3>gravel is astounding. We aren't talking about a light sprinkling

789
00:39:45.440 --> 00:39:48.920
<v Speaker 3>of organics. We are talking about multiple Earth masses worth

790
00:39:48.960 --> 00:39:52.679
<v Speaker 3>of complex carbon being chemically processed and physically moved around

791
00:39:52.719 --> 00:39:53.559
<v Speaker 3>the Jovian system.

792
00:39:53.679 --> 00:39:55.760
<v Speaker 2>So, looking forward to the future of this field, we

793
00:39:55.800 --> 00:39:58.760
<v Speaker 2>have the upcoming spacecraft missions, we have a highly robust

794
00:39:59.039 --> 00:40:03.840
<v Speaker 2>theoretical frame work. What is the next major theoretical hurdle?

795
00:40:04.119 --> 00:40:07.400
<v Speaker 2>If this paper fundamentally solves the delivery problem, what is

796
00:40:07.440 --> 00:40:09.639
<v Speaker 2>the next major problem we need a deep dive on.

797
00:40:10.159 --> 00:40:13.400
<v Speaker 3>I would say the absolute next big frontier in astrobiology

798
00:40:13.519 --> 00:40:17.719
<v Speaker 3>is the concentration Problementrue. Yes, you have a massive global ocean,

799
00:40:18.239 --> 00:40:22.559
<v Speaker 3>you have trillions of tons of complex organics successfully delivered

800
00:40:22.599 --> 00:40:25.800
<v Speaker 3>and dissolved in it. But biology usually requires a high

801
00:40:25.800 --> 00:40:27.800
<v Speaker 3>local concentration to actually initiate.

802
00:40:27.880 --> 00:40:30.519
<v Speaker 2>It can't just be infinitely diluted exactly.

803
00:40:30.719 --> 00:40:35.000
<v Speaker 3>It needs a tide pool or a porous hydrothermal vent structure,

804
00:40:35.480 --> 00:40:38.079
<v Speaker 3>or perhaps an active ice water interface at the crust.

805
00:40:38.559 --> 00:40:41.719
<v Speaker 3>The chemistry needs to be confined. We need to rigorously

806
00:40:41.840 --> 00:40:46.639
<v Speaker 3>understand how these dilute dissolved organics get concentrated densely enough

807
00:40:46.679 --> 00:40:49.800
<v Speaker 3>to begin the processes of self replication and metabolism.

808
00:40:50.119 --> 00:40:53.039
<v Speaker 2>So we have successfully moved from asking is there any

809
00:40:53.039 --> 00:40:57.239
<v Speaker 2>flour in the kitchen to asking how do we properly

810
00:40:57.280 --> 00:40:57.960
<v Speaker 2>mix the dough.

811
00:40:58.239 --> 00:41:00.320
<v Speaker 3>That is a perfect summary. We are moving up the

812
00:41:00.400 --> 00:41:04.679
<v Speaker 3>hierarchy of biological complexity. But crucially, we couldn't even legitimately

813
00:41:04.719 --> 00:41:08.280
<v Speaker 3>ask the concentration question until we comprehensively solved the delivery question.

814
00:41:08.440 --> 00:41:11.199
<v Speaker 2>In this research solves the delivery. Now we know for

815
00:41:11.239 --> 00:41:14.039
<v Speaker 2>a fact that global ocean is a viable chemical feedstock.

816
00:41:14.519 --> 00:41:17.199
<v Speaker 2>Now we can start accurately modeling the hydrothermal vents.

817
00:41:17.400 --> 00:41:20.760
<v Speaker 3>It is an incredibly exciting time to be following planetary science.

818
00:41:21.119 --> 00:41:23.800
<v Speaker 3>We are literally rewriting the fundamental history of our own

819
00:41:23.880 --> 00:41:25.360
<v Speaker 3>solar system in real.

820
00:41:25.159 --> 00:41:27.880
<v Speaker 2>Time, and potentially rewriting the history of every solar system

821
00:41:27.880 --> 00:41:28.519
<v Speaker 2>in the galaxy.

822
00:41:28.599 --> 00:41:30.440
<v Speaker 3>Absolutely, the implications are universal.

823
00:41:30.719 --> 00:41:33.800
<v Speaker 2>So to comprehensively wrap this up for you listening, we

824
00:41:33.840 --> 00:41:36.760
<v Speaker 2>started this deep dive with a traditional view of the

825
00:41:36.800 --> 00:41:41.480
<v Speaker 2>Galleyan moons as purely icy, potentially habitable in terms of water,

826
00:41:42.199 --> 00:41:45.239
<v Speaker 2>but chemically completely mysterious worlds.

827
00:41:45.400 --> 00:41:47.800
<v Speaker 3>And through the lens of this research we have ended

828
00:41:47.800 --> 00:41:51.320
<v Speaker 3>with a view of them as massive dynamic chemical factories

829
00:41:51.599 --> 00:41:55.519
<v Speaker 3>born from a robust dual lineage of ancient interstellar dust

830
00:41:55.599 --> 00:41:58.320
<v Speaker 3>and vigorous local thermal processing.

831
00:41:58.440 --> 00:42:02.280
<v Speaker 2>They are worlds that were essentially preprogrammed for advanced prebiotic

832
00:42:02.320 --> 00:42:05.280
<v Speaker 2>chemistry from the moment of their physical accretion.

833
00:42:05.119 --> 00:42:08.880
<v Speaker 3>And that profound chemical complexity isn't a random accident. It

834
00:42:08.960 --> 00:42:13.159
<v Speaker 3>is a direct, mathematically predictable consequence of exactly how gas

835
00:42:13.199 --> 00:42:15.599
<v Speaker 3>giants form within a protal planetary disk.

836
00:42:15.480 --> 00:42:18.679
<v Speaker 2>Which strongly means the entire galaxy is highly likely teeming

837
00:42:18.679 --> 00:42:20.480
<v Speaker 2>with organic, rich habital moons.

838
00:42:20.679 --> 00:42:22.599
<v Speaker 3>The statistics certainly point in that direction.

839
00:42:22.719 --> 00:42:25.519
<v Speaker 2>I will leave you with this final thought. In astrobiology,

840
00:42:25.559 --> 00:42:28.320
<v Speaker 2>we spend an enormous amount of time in telescope resources

841
00:42:28.519 --> 00:42:31.159
<v Speaker 2>looking for Earth two point zero. We look for rocky

842
00:42:31.199 --> 00:42:33.920
<v Speaker 2>planets sitting in the warm, comfortable zone around a yellow star.

843
00:42:34.599 --> 00:42:37.719
<v Speaker 2>But perhaps we have been fundamentally biased by our own origins.

844
00:42:38.159 --> 00:42:41.639
<v Speaker 2>We look for what we know exactly. But maybe the

845
00:42:41.760 --> 00:42:45.760
<v Speaker 2>actual default mode for life in the universe isn't sitting

846
00:42:45.760 --> 00:42:47.840
<v Speaker 2>on the dry surface of a rock near a star.

847
00:42:48.800 --> 00:42:52.840
<v Speaker 2>Maybe the default, statistically speaking, is deep under miles of

848
00:42:52.880 --> 00:42:56.360
<v Speaker 2>ice orbiting a massive gas giant swimming in a rich

849
00:42:56.480 --> 00:42:59.519
<v Speaker 2>organic soup that was meticulously cooked up before the planet

850
00:42:59.559 --> 00:43:00.960
<v Speaker 2>was even fit is building itself.

851
00:43:01.119 --> 00:43:06.119
<v Speaker 3>It is a very real, mathematically supported possibility the universe

852
00:43:06.199 --> 00:43:08.559
<v Speaker 3>is vastly more creative than we give it credit for.

853
00:43:08.719 --> 00:43:10.639
<v Speaker 2>It certainly changes how you look at Jupiter when you

854
00:43:10.679 --> 00:43:12.800
<v Speaker 2>see it shining in the night sky. Is not just

855
00:43:12.840 --> 00:43:15.920
<v Speaker 2>a big inert ball of gas. It is the hydrodynamic

856
00:43:16.000 --> 00:43:18.599
<v Speaker 2>engine that might have sparked biology across a dozen moons.

857
00:43:18.760 --> 00:43:22.159
<v Speaker 3>A very large, highly efficient cosmic mixer.

858
00:43:22.480 --> 00:43:24.320
<v Speaker 2>Thanks for taking this deep dive with us today.

859
00:43:24.360 --> 00:44:42.199
<v Speaker 4>What's my pleasures stations said the school

860
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<v Speaker 3>La
