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>So imagine you are standing on a shoreline. But this

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<v Speaker 2>isn't anywhere on Earth. The atmospheric pressure pressing against your

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<v Speaker 2>suit is noticeably heavier, right, It's about fifty percent thicker

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<v Speaker 2>than what you're used to.

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<v Speaker 3>Yeah, it would feel a bit like being at the

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<v Speaker 3>bottom of a shallow pool, just from the air pressure alone.

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<v Speaker 2>Right, But at the exact same time, you feel almost weightless,

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<v Speaker 2>And then a breeze brushes past you. It's barely a zephyr.

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<v Speaker 2>I mean, maybe two or three miles per.

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<v Speaker 3>Hour, which is nothing on a beach here on Earth.

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<v Speaker 3>A wind bit light wouldn't even disrupt the surface tension

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<v Speaker 3>of a tiny tide pool. You wouldn't even see.

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<v Speaker 2>A ripple exactly. But as you look out at the

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<v Speaker 2>liquid expanse in front of you, the physics just totally

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<v Speaker 2>break down. You are watching these massive ten foot tall

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<v Speaker 2>swells rolling toward the shore, and because of the gravitational

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<v Speaker 2>mechanics at play, they're crashing in this like haunting, drawn

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<v Speaker 2>out slow motions. Such an incredible visual, it really is,

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<v Speaker 2>And you are standing on the shores of kraken Mare.

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<v Speaker 2>It's the largest liquid body on Titan, which is Saturn's

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<v Speaker 2>largest moon. And we're not just making up a sci

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<v Speaker 2>fi scenario here. This specific visual is actually the mathematical

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<v Speaker 2>key to solving one of the most perplexing planetary mysteries

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<v Speaker 2>in our entire Solar system.

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<v Speaker 3>It really is. It forces a complete recalibration of our

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<v Speaker 3>intuitive understanding of fluid dynamics. I mean, we've had radar

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<v Speaker 3>imagery of Titan from the Cassini mission for years now.

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<v Speaker 2>Right, Yeah, mapping out all those crazy liquid networks exactly.

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<v Speaker 3>We've mapped these vast, branching river networks that physically carved

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<v Speaker 3>through the icy bedrock and they just empty out into

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<v Speaker 3>these mats of lakes of liquid methane and ethane. But

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<v Speaker 3>here's the thing. Geologically speaking, when you have mature river

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<v Speaker 3>networks feeding into a standing body of liquid, you expect

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<v Speaker 3>to see deltas right like.

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<v Speaker 2>The Mississippi Delta of the Nile. You expect a bunch

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<v Speaker 2>of mud and sand to just pile up exactly.

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<v Speaker 3>You expect to find massive alluvial fans of sediment deposited

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<v Speaker 3>right at the mouths of those rivers. Yeah, but on Titan,

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<v Speaker 3>the deltas are virtually non existent. The rivers just hit

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<v Speaker 3>the coastline and stop. It's a glaring anomaly, and that.

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<v Speaker 2>Anomaly brings us to what we're going to deep dig

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<v Speaker 2>into today. We're looking at a brand new framework developed

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<v Speaker 2>by researchers at the Massachusetts Institute of Technology, specifically in

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<v Speaker 2>their Department of Earth, Atmospheric and Planetary Sciences.

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<v Speaker 1>Yeah.

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<v Speaker 3>Lead author Unashneck and Taylor Puran, they really cracked this open.

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<v Speaker 2>They did. They published this model called Planet Waves in

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<v Speaker 2>the Journal of Geophysical Research Planets. And what's wild is

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<v Speaker 2>they didn't set out to build some like sci fi

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<v Speaker 2>Wina simulator for fun. They built a rigorous mathematical tool

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<v Speaker 2>to solve this exact geological discrepancy on Titan and honestly,

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<v Speaker 2>by extension, any planetary body with liquid.

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<v Speaker 3>Because waves are the engines of coastal erosion. The MIT

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<v Speaker 3>team basically hypothesized that if Titan's coastal environments were volatile enough,

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<v Speaker 3>the wave action would essentially act as a giant planetary sander.

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<v Speaker 3>It would relentlessly obliterate any sediment deposits before delta could

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<v Speaker 3>ever even form.

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<v Speaker 2>Wow, so just wiping the slate clean constantly, exactly.

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<v Speaker 3>But to prove that, they had to understand exactly how

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<v Speaker 3>waves are generated in an environment that shares almost none

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<v Speaker 3>of Earth's baseline.

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<v Speaker 2>Variables, right, because previous attempts to model alien oceans usually

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<v Speaker 2>just stopped at the most obvious variable, which is gravity.

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<v Speaker 3>Yeah, gravity is the simplest calculation, and.

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<v Speaker 2>Titan has roughly one seventh the gravitational pull of Earth.

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<v Speaker 2>So less gravity means less downward force on the liquid,

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<v Speaker 2>which means the liquid is easy to lift. But when

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<v Speaker 2>I was looking at this, that single variable analysis completely

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<v Speaker 2>falls apart when you actually look at momentum transfer. Right.

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<v Speaker 3>Oh, absolutely yeah. If gravity was the only variable that mattered,

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<v Speaker 3>a high pressure atmosphere moving across a low gravity liquid

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<v Speaker 3>should theoretically just shear the surface right off.

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<v Speaker 2>It would atomize it, like, just turn the whole lake

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<v Speaker 2>into a miss.

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<v Speaker 3>Right, So the model had to account for the liquid's

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<v Speaker 3>actual composition, and that is.

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<v Speaker 2>The huge critical advancement of the Planet Waves model. It

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<v Speaker 2>isolates and calculates this intricate dance between gravitational acceleration, atmospheric pressure,

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<v Speaker 2>and the specific the reology of the liquid.

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<v Speaker 3>Its density, its kinematic viscosity, and its surface tension.

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<v Speaker 2>Right and Andrew Ashton, a researcher at the Woodshole Oceanographic

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<v Speaker 2>Institution who collaborated on this. He framed the core math

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<v Speaker 2>challenge around predicting what he calls the first puff.

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<v Speaker 3>I love that phrase, the first puff.

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<v Speaker 2>It's so descriptive. You have a completely quiescent, glassy liquid surface.

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<v Speaker 2>The model has to calculate the exact threshold of atmospheric

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<v Speaker 2>kinetic energy required to overcome the liquid's internal cohesive forces

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<v Speaker 2>and generate a capillary wave, just a tiny ripple, because.

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<v Speaker 3>Once that boundary layer is broken, the physics change entirely.

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<v Speaker 2>Tell me about that, because this transition is fascinating.

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<v Speaker 3>Well, once you get that first ripple, you introduce aerodynamic drag.

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<v Speaker 3>The wind starts catching the windward side of that ripple

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<v Speaker 3>and then compounds the energy transfer, so it turns a

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<v Speaker 3>tiny capillary wave into a full scale gravity wave.

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<v Speaker 2>So the surface roughness increases, which basically allows the wind

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<v Speaker 2>to get a grip on the liquid.

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<v Speaker 3>Exactly the wind grips the water. But modeling that transition

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<v Speaker 3>from a perfectly flat plane to a chaotic turbulent swell

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<v Speaker 3>that requires a flawless understanding of energy transfer coefficients. You

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<v Speaker 3>can't just plug in the density of liquid methane and

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<v Speaker 3>hope for the best.

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<v Speaker 2>No, you have to calibrate the math against a known,

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<v Speaker 2>highly erratic system first.

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<v Speaker 3>Right, which is why the MIT team didn't start with Titan.

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<v Speaker 2>Started in our own backyard. They validated the planet waves

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<v Speaker 2>model using twenty years of continuous meteorological and oceanographic data

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<v Speaker 2>from Lake Superior, which.

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<v Speaker 3>Is perfect because geologically speaking, Lake Superior operates as an

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<v Speaker 3>inland ocean.

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<v Speaker 2>Yeah, it's massive. It has these huge fetch lengths, violent squalls,

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<v Speaker 2>and then prolonged periods of absolute dead calm.

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<v Speaker 3>And the National Data Boyse Center maintains a rays all

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<v Speaker 3>across Lake Superior. They provide high frequency sampling of wave period, amplitude,

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<v Speaker 3>wind sheer, stress, all of.

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<v Speaker 2>It, and having twenty years of that data allows researchers

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<v Speaker 2>to filter out all the statistical noise, right like roague

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<v Speaker 2>currents or localized thermal inversions.

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<v Speaker 3>Exactly atmosphere canomalies, all the weird outliers. They fed the

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<v Speaker 3>Planet Waves model the historical wind velocity and atmosphere of

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<v Speaker 3>pressure for specific days. They locked in Earth's gravity and

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<v Speaker 3>the density of fresh water, and then basically said, okay,

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<v Speaker 3>model predict the wave height and frequency for this civic

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<v Speaker 3>Tuesday in two thousand and eight.

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<v Speaker 2>And it worked flawlessly. The model matched the buoy data perfectly.

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<v Speaker 2>It accurately predicted the exact wind shear required to initiate

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<v Speaker 2>those capillary waves and the subsequent growth into full scale

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<v Speaker 2>gravity waves.

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<v Speaker 3>It's an incredible proof of concept, it really is.

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<v Speaker 2>But this is where the concept of viscosity becomes the

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<v Speaker 2>absolute lynchpin. To kind of visualize this for you listening,

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<v Speaker 2>think about it like this. If I have a wind

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<v Speaker 2>tunnel and I blow a ten knot wind over a

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<v Speaker 2>basin of tap water, I get immediate ripples right instantly.

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<v Speaker 3>Yeah.

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<v Speaker 2>But if I swap that water for something really thick,

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<v Speaker 2>like a bowl of thick honey or heavy syrup, that

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<v Speaker 2>exact same tennot wind does practically nothing right.

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<v Speaker 3>The sheer stress isn't sufficient to overcome the syrup's resistance

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<v Speaker 3>to being deformed exactly.

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<v Speaker 2>The physical effort required is vastly different. The momentum from

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<v Speaker 2>the air mass just kind of slips over the top layer.

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<v Speaker 3>Yeah, the kinetic energy dissipates as microscopic heat rather than

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<v Speaker 3>translating into actual wave motion. So by proving that planet

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<v Speaker 3>waves could account for this specific viscosity and density of

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<v Speaker 3>water on Earth using the lake superior to the MIT

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<v Speaker 3>team confirmed their math was rock.

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<v Speaker 2>Solid, solid enough to handle the weird alien chemistry of

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<v Speaker 2>liquid hydrocarbons precisely.

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<v Speaker 3>So we take this perfectly validated model and we point

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<v Speaker 3>it back at kracken Mare on Titan.

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<v Speaker 2>Let's really look at those parameters, because it is wild.

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<v Speaker 2>The liquid is a cryogenic mixture of methane and ethane.

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<v Speaker 2>It is sitting at roughly minus two hundred and ninety

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<v Speaker 2>degrees fahrenheit, so cold, unbelievably cold, and the density of

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<v Speaker 2>liquid methane is about four hundred and twenty two kilograms

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<v Speaker 2>per cubic meter. Compare that to Earth water, which is

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<v Speaker 2>basically a thousand So this Titan liquid is less than

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<v Speaker 2>half as dense as the water we drink.

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<v Speaker 3>And then you have surface tension which is incredibly low

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<v Speaker 3>on Titan. Methane molecules don't have the strong hydrogen bonds

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<v Speaker 3>that water molecules do.

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<v Speaker 2>Right, Water exist together exactly.

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<v Speaker 3>Water is cohesive, but the force holding the surface of

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<v Speaker 3>a methane lake together is incredibly weak.

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<v Speaker 2>Okay, So then you factor in the gravity, he said earlier.

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<v Speaker 2>It's zero point one four gramsificantly lower than Earth. So

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<v Speaker 2>the restoring force, meaning the gravity that's trying to pull

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<v Speaker 2>a wave crust back down to make the surface flat again,

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<v Speaker 2>is minimal.

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<v Speaker 3>But and this is the kicker, you still have the atmosphere.

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<v Speaker 3>Titan's atmosphere is mostly nitrogen, just like Earth's, but it's

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<v Speaker 3>much colder and denser. It exerts about one point five

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<v Speaker 3>bar of surface pressure.

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<v Speaker 2>Okay, So this is where I struggle with the visualization,

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<v Speaker 2>and maybe you can help break this down. If the

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<v Speaker 2>liquid is that light, right, and the surface tension is

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<v Speaker 2>weak and the gravity is super low, but you have

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<v Speaker 2>a dense, heavy atmosphere pushing across it, why does it

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<v Speaker 2>form a cohesive ten foot wave? That is the big question, right,

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<v Speaker 2>Like why doesn't the atmospheric drag just rip the top

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<v Speaker 2>layer of the methane off into a fine aerosol mist.

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<v Speaker 2>I mean if I take a high pressure air hose

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<v Speaker 2>and blast a puddle of gasoline, I don't get waves.

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<v Speaker 2>I get a spray of vapor.

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<v Speaker 3>Yeah, it's a totally fair question. It comes down to

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<v Speaker 3>a question of kinetic scale and atmospheric density. You aren't

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<v Speaker 3>hitting the lake with a highly localized, high la velocity

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<v Speaker 3>jet of air like from a hose.

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<v Speaker 1>Ah.

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<v Speaker 3>Okay, the low wind speeds on Titan. Remember that two

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<v Speaker 3>to three mile prour breeze we talk about. That means

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<v Speaker 3>the dynamic pressure exerted by the wind is actually quite low,

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<v Speaker 3>even though the atmosphere itself is death.

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<v Speaker 2>So what's spreading the force out exactly?

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<v Speaker 3>The planet? Waves calculation show that the wind transfers its

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<v Speaker 3>momentum across a vast surface area, and it does this

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<v Speaker 3>without ever exceeding the threshold where aerodynamic sheer would rip

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<v Speaker 3>the fluid apart.

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<v Speaker 2>Oh wow, so it's almost gentle.

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<v Speaker 3>It is. In fact, the thick atmosphere actually acts as

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<v Speaker 3>a stabilizing blanket. It presses down uniformly, maintaining the fluid

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<v Speaker 3>phase of the methane, while the wind slowly steadily piles

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<v Speaker 3>that light liquid up into a crest.

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<v Speaker 2>And because there's almost no gravity fighting that upward lift,

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<v Speaker 2>the crest just keeps building and building.

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<v Speaker 3>Exactly, and that lack of gravitational restoring force is what

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<v Speaker 3>dictates the whole kinematics of the wave. Think about Earth.

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<v Speaker 3>On Earth, a ten foot wave crest is incredibly heavy.

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<v Speaker 3>Gravity pulls it down violently. That's what creates the rapid

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<v Speaker 3>crashing turbulence we see when we go surfing.

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<v Speaker 2>Right, that classic crashing sound and foam.

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<v Speaker 3>But on Titan, the mass of that methane crest is

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<v Speaker 3>very low and the gravity pulling it down is very weak,

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<v Speaker 3>so the acceleration of the falling fluid is drastically reduced.

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<v Speaker 3>It literally takes longer for the methane to succumb.

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<v Speaker 2>To gravity, which creates that cinematic suspended slow motion effect

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<v Speaker 2>as it breaks against the shoreline. It's just so mine bending.

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<v Speaker 3>It really is. And returning to the MIT team's original objective,

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<v Speaker 3>this completely solves the mystery of the missing deltas right.

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<v Speaker 2>Because a two mile per hour breeze on Earth does

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<v Speaker 2>absolutely nothing to a shoreline, but a two mile per

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<v Speaker 2>hour breeze on Titan generates a ten foot slow motion

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<v Speaker 2>wall of liquid methane that is carrying a massive amount

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<v Speaker 2>of kinetic energy.

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<v Speaker 3>Exactly. The river networks on Titan are undoubtedly carrying sediment

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<v Speaker 3>down to the coasts. It's likely crushed water, ice and

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<v Speaker 3>hydrocarbon particulates. But the moment those rivers meet the lags,

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<v Speaker 3>they just get they get pulverized. The relentless, easily generated

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<v Speaker 3>wave action just destroys the deposits. The coastal erosion vastly

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<v Speaker 3>outpaces the sediment deposition, so the deltas are being destroyed

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<v Speaker 3>way faster than they can ever form.

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<v Speaker 2>It's just a perfect synthesis of fluid dynamics answering a

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<v Speaker 2>planetary anomaly. It's so satisfying, it really is.

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<v Speaker 3>But Titan represents the system that's in relative equilibrium today.

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<v Speaker 3>The planet waves model becomes even more revealing when we

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<v Speaker 3>apply it chronologically to planetary bodies that have undergone massive

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<v Speaker 3>changes over time.

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<v Speaker 2>Which brings us to a really fascinating part of this

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<v Speaker 2>deep dive Ancient Mars.

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<v Speaker 3>Yes, the Noatian period of Mars.

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<v Speaker 2>Right, because Mars is effectively the ultimate control group for

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<v Speaker 2>atmospheric degradation. If you look at orbital telemetry of Mars today,

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<v Speaker 2>you see this dry, irradiated dead desert, but the topography

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<v Speaker 2>tells a completely different story.

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<v Speaker 3>We have undeniable geomorphological evidence of a hydrological cycle on

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<v Speaker 3>ancient Mars.

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<v Speaker 2>Yeah, and the most famous example right now, the one

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<v Speaker 2>everyone's is jezuro Crater. NASA's Perseverance rover is literally driving

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<v Speaker 2>around in there right now, precisely because it is an

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<v Speaker 2>ancient paleo lake basin, and unlike Titan, jesuro Crater has

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<v Speaker 2>a magnificent, beautifully preserved delta.

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<v Speaker 3>Which mathematically confirms something huge. It confirms that the wave

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<v Speaker 3>action in jezro Crater billions of years ago was not

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<v Speaker 3>powerful enough to erode the sediment being deposited by the

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<v Speaker 3>inflowing river.

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<v Speaker 2>Right so the water was relatively calm, or at least

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<v Speaker 2>the waves weren't titaned sized monsters.

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<v Speaker 3>Exactly, But the conditions of that wave action were not static.

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<v Speaker 3>They changed dramatically during the no action period, which was

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<v Speaker 3>roughly four billion years ago. Mars possessed a global magnetic field.

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<v Speaker 3>It was generated by an active core, just like.

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<v Speaker 2>Earth's, and that magnetic dynamo protected the atmosphere from the

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<v Speaker 2>solar wind, which meant it could hold on to a

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<v Speaker 2>thick atmosphere, which in turn allowed for liquid water to

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<v Speaker 2>just sit on the surface.

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<v Speaker 3>Right. But then the Martian core cooled, the magnetic dynamo failed,

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<v Speaker 3>and the planet was suddenly exposed to continuous atmosphere expedtering.

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<v Speaker 2>The solar wind just started sand blasting the planet exactly.

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<v Speaker 3>It began stripping the upper atmosphere away molecule by.

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<v Speaker 2>Molecule, and as that atmospheric envelope bled away into space,

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<v Speaker 2>the pressure at the surface dropped. So the MIT team

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<v Speaker 2>took the planet Waves model, locked in the gravity of

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<v Speaker 2>Mars and the composition of liquid water, and they effectively

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<v Speaker 2>ran the model backwards through time.

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<v Speaker 3>Tracking the wave dynamics is the atmosphere.

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<v Speaker 2>Thinned out, Yes, and the dynamic pressure of wind is

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<v Speaker 2>governed by a specific equation right where pressure equals one

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<v Speaker 2>half the fluid density times the velocity squared. So if

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<v Speaker 2>the atmosphere density drops, the wind velocity has to increase

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<v Speaker 2>exponentially just to transfer the exact same amount of kinetic

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<v Speaker 2>energy to the water.

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<v Speaker 3>Think about it like, this wind is just moving air.

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<v Speaker 3>It's molecules in motion. The mass of the air on

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<v Speaker 3>Mars physically decreased over time a forty mile per hour

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<v Speaker 3>wind in a thick atmosphere carries billions of tons of

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<v Speaker 3>kinetic energy because of the sheer density of molecules impacting

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<v Speaker 3>the water.

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<v Speaker 2>Right, there's just more physical stuff hitting the water.

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00:15:05.320 --> 00:15:08.240
<v Speaker 3>Exactly, But a forty mile per hour wind in a

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<v Speaker 3>really thin atmosphere, it's mostly empty space. It exerts barely

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<v Speaker 3>any physical sheer stress.

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<v Speaker 2>So if you imagine setting up a time lapse camera

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<v Speaker 2>on the shores of Jezero Crater millions of years ago,

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<v Speaker 2>the model basically illustrates a dying ocean. In the early days,

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<v Speaker 2>regular seasonal weather patterns could weep up totally normal surface waves.

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<v Speaker 2>But as the air literally thinned out over tens of

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<v Speaker 2>millions of years, the exact same storms rolling in century after.

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<v Speaker 3>Century, the same wind velocity.

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<v Speaker 2>Yeah, the exact same speeds became increasingly impotent. The water

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<v Speaker 2>was still there, the wind was still moving at forty

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<v Speaker 2>miles per hour, but the waves just started getting smaller

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<v Speaker 2>and smaller.

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<v Speaker 3>It would require increasingly extreme massive gales just to make

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<v Speaker 3>a splash, let alone generate the baseline wave heights of

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<v Speaker 3>previous eras.

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<v Speaker 2>Wow, you are literally watching the mechanical transfer of play

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<v Speaker 2>planetary energy just grind to a halt. The geological engine

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<v Speaker 2>that powered coastal erosion on Mars slowly suffocated as the

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<v Speaker 2>atmosphere vanished. By the time the lakes ultimately froze or

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<v Speaker 2>evaporated away, their surfaces were likely completely stagnant, no matter

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<v Speaker 2>how fast the wind was blowing.

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<v Speaker 3>It's a pretty chilling visualization of planetary mortality on it.

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<v Speaker 2>It really is. So we've looked at Earth as the baseline,

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<v Speaker 2>We've looked at Titan as the low gravity alien chemistry extreme,

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00:16:28.559 --> 00:16:31.759
<v Speaker 2>and we've looked at Mars as the decaying atmosphere variable.

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00:16:32.159 --> 00:16:33.840
<v Speaker 2>But what I love about this research is that they

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<v Speaker 2>didn't stop there.

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<v Speaker 3>Oh No, they pushed it way further.

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<v Speaker 2>To stress test the math to make sure it wasn't

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<v Speaker 2>just biased toward our local Solar system physics. They pushed

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<v Speaker 2>the parameters to the absolute, terrifying extremes by applying planet

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<v Speaker 2>waves to exoplanets.

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<v Speaker 3>Yeah, testing against extreme parameter spaces is vital if you

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<v Speaker 3>want to confirm the integrity of physico model, Yeah, you

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00:16:52.919 --> 00:16:54.039
<v Speaker 3>have to try and break it right.

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<v Speaker 2>So they modeled three entirely distinct classes of exoplanets. Let's

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<v Speaker 2>start with LHS one forty B.

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00:17:00.159 --> 00:17:02.519
<v Speaker 3>This one has been heavily studied by the James Webb

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00:17:02.600 --> 00:17:06.480
<v Speaker 3>Space Telescope. It classifies as a super Earth, and it

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00:17:06.640 --> 00:17:09.279
<v Speaker 3>orbits in the habitable zone of a red dwarf star.

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00:17:09.839 --> 00:17:13.039
<v Speaker 2>It's a rocky world roughly one point seven times the

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<v Speaker 2>radius of Earth, and its mass suggests it could easily

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<v Speaker 2>host vast oceans of liquid water. But the gravity on

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<v Speaker 2>LHS eleven forty b is.

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00:17:22.160 --> 00:17:25.880
<v Speaker 3>Immense, which creates an incredibly extreme environment for that restoring

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<v Speaker 3>force we talked about earlier. When wind sheer attempts to

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<v Speaker 3>deform the surface of the water on this super Earth,

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00:17:31.319 --> 00:17:33.559
<v Speaker 3>it is fighting a massive gravitational anchor.

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<v Speaker 2>The gravity is just pulling it down so hard exactly.

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<v Speaker 3>The kinetic energy required to lift a volume of water

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00:17:39.480 --> 00:17:42.279
<v Speaker 3>is drastically higher than on Earth. So the planet waves

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00:17:42.279 --> 00:17:45.240
<v Speaker 3>calculations indicate that a windstorm that would generate say a

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<v Speaker 3>six foot swell on.

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<v Speaker 2>Earth like a really decent surfing one right.

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<v Speaker 3>That exact same windstorm might only manage a turbulent chop

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<v Speaker 3>of a few inches on this super Earth. The water

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<v Speaker 3>is effectively pinned to the ocean floor by gravity.

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00:17:57.039 --> 00:18:01.400
<v Speaker 2>That is wild, and that introduces some really fascinating implications

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<v Speaker 2>for oceanic circulation, doesn't it like thermal distribution on a

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00:18:04.880 --> 00:18:08.480
<v Speaker 2>planet like that. If you lack deep water wave propagation,

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<v Speaker 2>the mixing of nutrients and heat might be severely stunted.

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<v Speaker 2>The oceans might just be these heavily stratified, stagnant layers.

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00:18:15.519 --> 00:18:18.960
<v Speaker 3>It completely changes how we think about habitability. But then

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00:18:19.240 --> 00:18:23.440
<v Speaker 3>they shifted from manipulating gravity to manipulating the fluid itself.

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<v Speaker 3>The team analyzed Kepler sixteen forty nine b.

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00:18:27.119 --> 00:18:29.960
<v Speaker 2>Okay, so this one is terrestrial, roughly Earth sized, so

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00:18:30.000 --> 00:18:33.799
<v Speaker 2>the gravity is familiar, but astrobiologists theorize it operates as

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00:18:33.799 --> 00:18:37.960
<v Speaker 2>an exovenus, which means it likely possesses surface liquids composed

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00:18:38.000 --> 00:18:40.599
<v Speaker 2>not of water but of sulfuric acid, and.

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00:18:40.559 --> 00:18:43.640
<v Speaker 3>The reality of sulfuric acid is a completely different beast entirely.

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00:18:43.839 --> 00:18:47.240
<v Speaker 3>We know it's highly corrosive, obviously, but mechanically speaking, it

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00:18:47.279 --> 00:18:49.960
<v Speaker 3>is incredibly dense. It has a density of roughly eighteen

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00:18:50.079 --> 00:18:51.559
<v Speaker 3>hundred and thirty kilograms per.

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<v Speaker 2>Cubic meter, which is nearly double that of liquid water.

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00:18:54.319 --> 00:18:57.440
<v Speaker 3>Exactly so, even with Earth normal gravity, the sheer mass

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<v Speaker 3>of the fluid requires intense aerodynamic drag just to initiate

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<v Speaker 3>that very first capillary wave.

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00:19:02.920 --> 00:19:07.039
<v Speaker 2>You're dealing with extreme fluid inertia. A standard earth breeze

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00:19:07.079 --> 00:19:10.279
<v Speaker 2>simply lacks the physical momentum to overcome the density of

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<v Speaker 2>the acid lakes. The wind would just flow right over

377
00:19:13.279 --> 00:19:15.839
<v Speaker 2>the boundary layer with almost zero energy transfer.

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00:19:15.920 --> 00:19:21.160
<v Speaker 3>It requires extreme violent atmospheric velocities to generate any meaningful

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00:19:21.200 --> 00:19:22.559
<v Speaker 3>wave action on that planet.

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00:19:22.680 --> 00:19:25.720
<v Speaker 2>Okay, but even that pales in comparison to the ultimate

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00:19:25.799 --> 00:19:29.680
<v Speaker 2>stress test. They applied the model to fifty five Cankori.

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00:19:30.039 --> 00:19:30.960
<v Speaker 3>This is the lava world.

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00:19:31.200 --> 00:19:34.680
<v Speaker 2>Yes, the lava world. It's a tidally locked super Earth

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00:19:34.799 --> 00:19:37.039
<v Speaker 2>orbiting so close to its host star that the day

385
00:19:37.079 --> 00:19:40.920
<v Speaker 2>side temperature exceeds four thousand degrees fahrenheit. The planet is

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00:19:41.039 --> 00:19:45.680
<v Speaker 2>literally covered in a global ocean of silicate magma liquid rock.

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00:19:46.200 --> 00:19:49.119
<v Speaker 3>This pushes the planet waves model to the absolute boundary

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00:19:49.119 --> 00:19:52.680
<v Speaker 3>of fluid mechanics because magma doesn't behave like a simple

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00:19:52.720 --> 00:19:56.640
<v Speaker 3>Newtonian fluid like water or even methane. How So, depending

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00:19:56.640 --> 00:20:00.079
<v Speaker 3>on the silica content and the temperature, magma often acts

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00:20:00.160 --> 00:20:01.359
<v Speaker 3>as a Bingham plastic.

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00:20:01.519 --> 00:20:03.799
<v Speaker 2>A Bingham plastic what does that mean? In this context?

393
00:20:04.039 --> 00:20:07.359
<v Speaker 3>It means it has a yield stress, so it actually

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00:20:07.359 --> 00:20:11.359
<v Speaker 3>behaves like a solid until a specific threshold of sheer

395
00:20:11.400 --> 00:20:14.160
<v Speaker 3>stress is applied to it. Only when that threshold is

396
00:20:14.240 --> 00:20:16.599
<v Speaker 3>met does it actually begin to flow like a liquid.

397
00:20:16.680 --> 00:20:19.160
<v Speaker 2>Oh wow, So it's fighting the wind not just with weight,

398
00:20:19.200 --> 00:20:20.839
<v Speaker 2>but with its fundamental state.

399
00:20:20.640 --> 00:20:24.079
<v Speaker 3>Of matter exactly. And the viscosity is just staggering. The

400
00:20:24.119 --> 00:20:28.839
<v Speaker 3>internal friction resisting deformation is astronomically high. We are talking

401
00:20:28.839 --> 00:20:32.359
<v Speaker 3>about a fluid that is incredibly dense under higher than

402
00:20:32.400 --> 00:20:36.000
<v Speaker 3>Earth gravity, with a viscosity millions of times thicker than water.

403
00:20:36.440 --> 00:20:39.039
<v Speaker 2>So the output of the MIT model for fifty five

404
00:20:39.119 --> 00:20:42.359
<v Speaker 2>kankrete is just profound in its darkness. To use an

405
00:20:42.359 --> 00:20:45.400
<v Speaker 2>analogy here, it's like taking an industrial leaf blower right

406
00:20:45.559 --> 00:20:48.039
<v Speaker 2>hurricane force wind and pointing it directly at a swimming

407
00:20:48.079 --> 00:20:52.000
<v Speaker 2>pool filled with wet, heavy, fast drawing cement. You're gonna

408
00:20:52.039 --> 00:20:53.960
<v Speaker 2>make a lot of noise, but you're barely gonna move

409
00:20:54.000 --> 00:20:54.480
<v Speaker 2>the surface.

410
00:20:54.599 --> 00:20:57.119
<v Speaker 3>As the perfect way to visualize it, if you took

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00:20:57.160 --> 00:21:00.000
<v Speaker 3>a category five hurricane sustained winds of over one hundred

412
00:21:00.079 --> 00:21:02.480
<v Speaker 3>fifty miles per hour, which on Earth is capable of

413
00:21:02.519 --> 00:21:06.319
<v Speaker 3>generating forty foot rogue waves, and you unleash that exact

414
00:21:06.319 --> 00:21:10.319
<v Speaker 3>same aerodynamic force across the Magna ocean of fifty five kankerteth.

415
00:21:10.359 --> 00:21:11.519
<v Speaker 2>The result is almost nothing.

416
00:21:11.720 --> 00:21:14.920
<v Speaker 3>Almost nothing. The model predicts waves of maybe a few

417
00:21:14.960 --> 00:21:18.759
<v Speaker 3>centimeters in height. The immense kinetic energy of a hurricane

418
00:21:18.839 --> 00:21:22.799
<v Speaker 3>is utterly neutralized by the rheological resistance of the liquid rock.

419
00:21:23.440 --> 00:21:27.640
<v Speaker 3>The atmospheric drag is entirely insufficient to overcome the yield

420
00:21:27.680 --> 00:21:30.039
<v Speaker 3>stress and the viscosity of the magma.

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00:21:30.160 --> 00:21:33.680
<v Speaker 2>It's just incredible. It's a mathematical proof that aerodynamic force

422
00:21:33.759 --> 00:21:38.200
<v Speaker 2>is highly conditional. It's the ultimate demonstration of boundary layer friction.

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00:21:38.720 --> 00:21:41.599
<v Speaker 2>The atmospheric molecules are colliding with the Magna surface at

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00:21:41.640 --> 00:21:44.319
<v Speaker 2>one hundred and fifty miles per hour, but the energy

425
00:21:44.440 --> 00:21:48.880
<v Speaker 2>just dissipates his heat. The surface remains practically undisturbed.

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00:21:48.359 --> 00:21:51.240
<v Speaker 3>Which is exactly why they ran this test. It validates

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00:21:51.240 --> 00:21:54.440
<v Speaker 3>that the MIT model isn't just calculating wind speed, it's

428
00:21:54.480 --> 00:21:58.599
<v Speaker 3>calculating the total mechanical profile of the entire planetary environment.

429
00:21:58.680 --> 00:22:01.279
<v Speaker 2>Okay, so we've talked about the mind bending physics, We've

430
00:22:01.359 --> 00:22:05.319
<v Speaker 2>visited lava oceans and acid lakes, but practically speaking, why

431
00:22:05.359 --> 00:22:08.480
<v Speaker 2>does this level of precision matter right now? Beyond solving

432
00:22:08.480 --> 00:22:12.799
<v Speaker 2>geological curiosities like Titans missing Delta's, how are scientists actually

433
00:22:12.920 --> 00:22:14.160
<v Speaker 2>using this knowledge today?

434
00:22:14.480 --> 00:22:17.880
<v Speaker 3>Well, it is fundamental to the engineering of future exploratory missions,

435
00:22:18.119 --> 00:22:18.960
<v Speaker 3>right because.

436
00:22:18.720 --> 00:22:22.640
<v Speaker 2>We are actively planning to send actual hardware to these environments.

437
00:22:23.200 --> 00:22:26.359
<v Speaker 2>The proposed missions to Titan, for example, they don't just

438
00:22:26.400 --> 00:22:29.680
<v Speaker 2>involve orbiters taking pictures from space. The goal is to

439
00:22:29.799 --> 00:22:36.880
<v Speaker 2>deploy landers, specifically autonomous robotic vessels space boats, essentially directly

440
00:22:36.920 --> 00:22:39.240
<v Speaker 2>into kraken Mare or Legea Maire.

441
00:22:39.839 --> 00:22:43.839
<v Speaker 3>We are literally conceptualizing extraterrestrial naval engineering.

442
00:22:43.400 --> 00:22:45.519
<v Speaker 2>Which is just the coolest phrase ever.

443
00:22:45.720 --> 00:22:48.519
<v Speaker 3>It really is. But if you are designing an aquatic

444
00:22:48.640 --> 00:22:52.119
<v Speaker 3>probe for an alien ocean, the wave dynamics are the

445
00:22:52.200 --> 00:22:56.799
<v Speaker 3>absolute most critical parameter for structural integrity. As Engishnek pointed

446
00:22:56.799 --> 00:22:59.319
<v Speaker 3>out in the research, the probe has to actually survive

447
00:22:59.400 --> 00:23:00.359
<v Speaker 3>the physical and environment.

448
00:23:00.480 --> 00:23:02.519
<v Speaker 2>They can't just sink or get batter to pieces, right.

449
00:23:02.720 --> 00:23:06.000
<v Speaker 3>And if the engineers assumed Titan's lakes behaved exactly like

450
00:23:06.079 --> 00:23:08.640
<v Speaker 3>Earth's lakes simply because the wind speeds are low, they

451
00:23:08.680 --> 00:23:11.799
<v Speaker 3>would severely underdesign the kinematic shock absorption of.

452
00:23:11.720 --> 00:23:14.519
<v Speaker 2>The hull ah because even though the liquid methane is

453
00:23:14.640 --> 00:23:17.359
<v Speaker 2>less dense than water. A ten foot wave is still

454
00:23:17.400 --> 00:23:19.559
<v Speaker 2>a ten foot wave, and having that crash into an

455
00:23:19.599 --> 00:23:22.759
<v Speaker 2>aluminum or titanium hull at minus two hundred ninety degrees

456
00:23:22.839 --> 00:23:25.759
<v Speaker 2>fahrenheit introduces terrifying mechanical stress.

457
00:23:26.079 --> 00:23:32.000
<v Speaker 3>Exactly, materials become incredibly brittle at cryogenic temperatures. The cyclical

458
00:23:32.079 --> 00:23:36.000
<v Speaker 3>loading of those massive slow motion waves repeatedly slamming against

459
00:23:36.000 --> 00:23:40.079
<v Speaker 3>the probe over and over, that could induce fatigue failure

460
00:23:40.319 --> 00:23:41.160
<v Speaker 3>very very quickly.

461
00:23:41.279 --> 00:23:43.079
<v Speaker 2>The boat would literally just crack apart.

462
00:23:43.119 --> 00:23:45.880
<v Speaker 3>It would. But now because of the Planet Waves model,

463
00:23:46.119 --> 00:23:49.680
<v Speaker 3>it provides the exact wave height, the frequency, and the

464
00:23:49.759 --> 00:23:53.119
<v Speaker 3>kinetic energy distribution that the probe will encounter based on

465
00:23:53.119 --> 00:23:54.240
<v Speaker 3>the local meteorology.

466
00:23:54.400 --> 00:23:57.400
<v Speaker 2>So the engineers can use those specific parameters to design

467
00:23:57.400 --> 00:24:00.279
<v Speaker 2>the buoyancy control, figure out the center of mass, and

468
00:24:00.359 --> 00:24:03.279
<v Speaker 2>reinforce the structural resilience of the vessel. They can actually

469
00:24:03.279 --> 00:24:06.079
<v Speaker 2>simulate the pitch and roll frequencies to ensure the communication

470
00:24:06.160 --> 00:24:08.680
<v Speaker 2>antennas can maintain a lock on Earth or on the

471
00:24:08.759 --> 00:24:11.240
<v Speaker 2>orbital relay despite the high amplitude swells.

472
00:24:11.279 --> 00:24:14.799
<v Speaker 3>It's incredible foresight. We're using a mathematical equation validated by

473
00:24:14.880 --> 00:24:17.799
<v Speaker 3>booys bobbing up and down in Lake Superior to dictate

474
00:24:17.839 --> 00:24:20.720
<v Speaker 3>the exact thickness of a titanium hull that will float

475
00:24:20.720 --> 00:24:23.480
<v Speaker 3>in a sea of liquid methane a billion miles away.

476
00:24:23.599 --> 00:24:27.359
<v Speaker 2>It's the sheer audacity of human engineering. It requires a

477
00:24:27.400 --> 00:24:31.480
<v Speaker 2>flawless grasp of universal physics. It proves that the mechanics

478
00:24:31.480 --> 00:24:35.000
<v Speaker 2>governing the universe aren't localized just to our planet. The

479
00:24:35.079 --> 00:24:38.440
<v Speaker 2>Navier Stokes equations that dictate fluid motion apply just as

480
00:24:38.519 --> 00:24:41.359
<v Speaker 2>rigidly to a lake of sulfuric acid on an exovenus

481
00:24:41.599 --> 00:24:43.680
<v Speaker 2>as they do to a glass of tap water sitting

482
00:24:43.680 --> 00:24:46.680
<v Speaker 2>on your kitchen counter. The only thing that changes are

483
00:24:46.720 --> 00:24:48.400
<v Speaker 2>the inputs, which is really.

484
00:24:48.240 --> 00:24:51.319
<v Speaker 3>The core takeaway here. It strips away are anthropic bias?

485
00:24:51.640 --> 00:24:52.519
<v Speaker 2>Say more about that?

486
00:24:52.559 --> 00:24:55.319
<v Speaker 3>Well, we inherently view planetary mechanics through the lens of

487
00:24:55.319 --> 00:24:59.519
<v Speaker 3>our own environment. We assume water, we assume one atmosphere

488
00:24:59.559 --> 00:25:02.599
<v Speaker 3>of pressure. We assume nine point eight meters per second

489
00:25:02.599 --> 00:25:04.920
<v Speaker 3>squared of gravitational acceleration. That's all we know.

490
00:25:05.119 --> 00:25:07.079
<v Speaker 2>Firsthand, right, It's our default setting.

491
00:25:07.359 --> 00:25:10.279
<v Speaker 3>But this research forces us to view Earth not as

492
00:25:10.319 --> 00:25:14.759
<v Speaker 3>the baseline for reality, but simply as one specific coordinate

493
00:25:15.160 --> 00:25:17.559
<v Speaker 3>on an infinite spectrum of physical.

494
00:25:17.200 --> 00:25:20.640
<v Speaker 2>Variables, and when you adjust those coordinates, when you tweak

495
00:25:20.680 --> 00:25:23.559
<v Speaker 2>the density, or dial down the gravity, or strip away

496
00:25:23.559 --> 00:25:28.000
<v Speaker 2>the atmosphere, the reality of the environment transforms radically. The

497
00:25:28.039 --> 00:25:30.359
<v Speaker 2>next time you look at a puddle trembling in the wind,

498
00:25:30.759 --> 00:25:33.640
<v Speaker 2>or watch waves crash on a beach, realize you are

499
00:25:33.680 --> 00:25:39.279
<v Speaker 2>watching a miraculous invisible equation balancing Earth's exact gravity, air pressure,

500
00:25:39.359 --> 00:25:43.119
<v Speaker 2>and water density. Just tweaking one of those numbers turns

501
00:25:43.160 --> 00:25:46.440
<v Speaker 2>our familiar world into a completely alien landscape.

502
00:25:46.519 --> 00:25:49.079
<v Speaker 3>It completely changes how you look at the natural world.

503
00:25:49.160 --> 00:25:52.160
<v Speaker 2>It really does. The interaction between moving gas and standing

504
00:25:52.240 --> 00:25:56.480
<v Speaker 2>liquid is the primary geological sculptor of coastlines across the cosmos,

505
00:25:56.880 --> 00:25:59.400
<v Speaker 2>and knowing that the mechanics of erosion operate at completely

506
00:25:59.440 --> 00:26:02.240
<v Speaker 2>different extreme depending on the rehology of the local fluids

507
00:26:02.559 --> 00:26:06.079
<v Speaker 2>leaves us with a pretty profound final thought. If the

508
00:26:06.119 --> 00:26:09.720
<v Speaker 2>slow motion methane waves of Titan can erase vast river

509
00:26:09.799 --> 00:26:13.119
<v Speaker 2>deltas and the dense, viscous oceans of other worlds remain

510
00:26:13.200 --> 00:26:16.880
<v Speaker 2>completely undisturbed by hurricane force winds, we really have to

511
00:26:16.920 --> 00:26:20.839
<v Speaker 2>consider the unimaginable geomorphologies waiting out there in the deep universe.

512
00:26:21.519 --> 00:26:25.799
<v Speaker 2>What intricate bizarre coastal architectures, cliffs carved from exotic ices,

513
00:26:25.920 --> 00:26:28.359
<v Speaker 2>or abyssal trenches hollowed out by heavy acidic tides have

514
00:26:28.359 --> 00:26:30.880
<v Speaker 2>been sculpted over billions of years. They are out there

515
00:26:30.920 --> 00:26:33.200
<v Speaker 2>right now, operating under a set of physical rules we

516
00:26:33.240 --> 00:26:36.759
<v Speaker 2>are only just beginning to mathematically comprehend, just waiting to

517
00:26:36.759 --> 00:26:37.440
<v Speaker 2>be discovered,
