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>Welcome curious minds. Today, we're looking at something pretty radical,

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<v Speaker 2>overturning a decade's old idea about Mars. Forget the notion

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<v Speaker 2>of just a you know, a fully liquid, maybe dying

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<v Speaker 2>heart beneath that dusty red surface. New seismic data this

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<v Speaker 2>is from NASA's Insight mission. It reveals Mars holds a

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<v Speaker 2>secret a solid core, and it's shockingly similar to Earth's,

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<v Speaker 2>which is well, it's a discovery that completely rewrites the history,

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<v Speaker 2>the really violent history of the red planet and its

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<v Speaker 2>lost oceans.

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<v Speaker 3>Yeah. What's truly remarkable here is how our understanding of

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<v Speaker 3>Mars just keep evolving. It's constantly pushing the boundaries of

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<v Speaker 3>what we thought was possible. You know, it forces us

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<v Speaker 3>to reevaluate these long held assumptions we've had. We know,

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<v Speaker 3>Mars today is well a cold, dry, seemingly desolate world,

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<v Speaker 3>like a frozen desert basically, Yet the evidence that's been

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<v Speaker 3>building up it strongly suggests a very different past, one

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<v Speaker 3>that held this compelling promise of well abundant liquid water

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<v Speaker 3>and perhaps you know, maybe even the potential for life right,

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<v Speaker 3>and the key to unlocking this huge mystery, it turns out,

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<v Speaker 3>lies hundreds of kilometers down way beneath its now dusty,

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<v Speaker 3>arid surface.

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<v Speaker 2>Yeah, for years, Mars has felt like this colossal planet

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<v Speaker 2>sized cold case, hasn't it? How did it go from

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<v Speaker 2>being potentially watery, maybe even vibrant, to the parched desert

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<v Speaker 2>it is today. It's a question that's really driven decades

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<v Speaker 2>of exploration absolutely and today are let's call them our

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<v Speaker 2>forensic team, the scientists working with the Insight Mission. They

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<v Speaker 2>finally cracked a really crucial piece of that puzzle. It's

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<v Speaker 2>dramatically reshaping our understanding of Mars interior. We're talking incredible

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<v Speaker 2>new insights from seismic studies. They literally offer us a

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<v Speaker 2>peak into its innermost secrets, like a planetary autopsy report.

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<v Speaker 3>Almost, And this raises a really important question for all

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<v Speaker 3>of us. I think, what can the very core of

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<v Speaker 3>a planet actually tell us about its entire history, it's trajectory,

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<v Speaker 3>it's ultimate fate. We'll be looking at how these recent

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<v Speaker 3>observations have not just refined, but really significantly deepened our models,

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<v Speaker 3>suggesting that Mars might be far more like Earth deep

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<v Speaker 3>down than we previously believed. And this is more than

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<v Speaker 3>just geology, you know, it's a profound story planetary evolution,

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<v Speaker 3>the delicate balance of magnetic fields, and the incredibly specific

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<v Speaker 3>conditions that are required for a world to remain hospitable,

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<v Speaker 3>to hold on to its life giving potential over well

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<v Speaker 3>cosmic time scales.

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<v Speaker 2>So our mission today as we dive into this is

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<v Speaker 2>really to uncover the secrets of Mars's core, understand why

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<v Speaker 2>it's structure and its history matters so much to the

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<v Speaker 2>planet's past and maybe its future, and so to see

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<v Speaker 2>how science, like a you know, a persistent detective, painstakingly

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<v Speaker 2>builds knowledge step by careful steps. So, yeah, prepare to

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<v Speaker 2>have your assumptions about the Red planet challenged.

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<v Speaker 3>Well. Trace this fascinating journey of scientific discovery right from

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<v Speaker 3>the initial hypotheses, which were often based on remote observations,

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<v Speaker 3>you know, looking from orbit to the latest and most

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<v Speaker 3>precise seismic measurements from insight. And we'll try to connect

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<v Speaker 3>these seemingly abstract, kind of complex details to the grand

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<v Speaker 3>sweeping narrative of Mars's really dramatic transformation. It really is

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<v Speaker 3>a planetary detective story.

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<v Speaker 2>Okay, So let's start with the Mars. We think we know,

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<v Speaker 2>the one we see today when we look up at

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<v Speaker 2>the night sky see that unmistakable red dot, or when

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<v Speaker 2>we see those amazing images beamed back by the rovers,

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<v Speaker 2>what comes to mind? I mean, it's a vast chili desert, right,

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<v Speaker 2>that's the image most of us have precisely.

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<v Speaker 3>Yeah, you've captured it perfectly. The Mars we observe today

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<v Speaker 3>is characterized by an extremely thin atmosphere, really thin. It's

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<v Speaker 3>mostly carbon dioxide, something like ninety five percent. And this

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<v Speaker 3>thin on belowe it offers very little protection from solar radiation.

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<v Speaker 3>The surface pressure is less than one percent of Earth's

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<v Speaker 3>at sea level, just.

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<v Speaker 2>Incredibly wow, less than one percent.

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<v Speaker 3>Yeah, And temperatures well, they rarely if ever get above freezing,

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<v Speaker 3>often plunging way down to minus sixty degrees celsius or

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<v Speaker 3>even colder at the poles. And the almost complete lack

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<v Speaker 3>of significant stable liquid water on the surface. That's one

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<v Speaker 3>of its most defining features right now. It is, by

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<v Speaker 3>all accounts, a very harsh place inhospitable, a true frozen desert.

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<v Speaker 2>And you think about those pictures, those iconic images from

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<v Speaker 2>the rovers, spirit, opportunity, curiosity, perseverance. You see those dusty,

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<v Speaker 2>rust colored planes stretching out forever, barren, rocky landscapes, those clear,

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<v Speaker 2>often kind of salmon pink skies, sometimes with those swirling

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<v Speaker 2>dust devils. It's got this men's geological beauty for sure.

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<v Speaker 2>That absolutely not a place you'd picture taking a swim

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<v Speaker 2>right or finding a river, seeing oceans. It feels like

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<v Speaker 2>a world strip bear of the very things that make

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<v Speaker 2>Earth so well alive. But that's not the complete picture,

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<v Speaker 2>is it not? By a long shot. That stark reality

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<v Speaker 2>of Mars today actually makes the evidence for past water

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<v Speaker 2>even more compelling, doesn't it. It really underlines the sheer scale

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<v Speaker 2>of the change the planet went through. There's a huge

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<v Speaker 2>amount of compelling, really undeniable evidence telling a very different

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<v Speaker 2>story about Mars's past, a time when it was a

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<v Speaker 2>very different kind of world.

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<v Speaker 3>Indeed, Yeah, what's truly remarkable is the overwhelming geological evidence

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<v Speaker 3>meticulously gathered over decades by orbiters and rovers like Curiosity

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<v Speaker 3>and Perseverance. This evidence suggests that liquid water once flowed freely, abundantly,

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<v Speaker 3>even and perhaps for long periods across the Martian surface.

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<v Speaker 3>We're talking about conditions that were well, incredibly far more

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<v Speaker 3>hospitable than anything we see today, a Mars that would

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<v Speaker 3>be honestly unrecognizable to us, maybe resembling a young.

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<v Speaker 2>Earth, a young or wow. So what kind of evidence

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<v Speaker 2>are we talking about specifically?

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<v Speaker 3>Well, comes in many forms, and each one is like

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<v Speaker 3>a powerful clue, really undeniable. For instance, we found numerous

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<v Speaker 3>dry lake beds. These are expansive basins that clearly once

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<v Speaker 3>held standing water, and you see ancient shorelines, delta structures,

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<v Speaker 3>sedimentary fans like river deltas exactly. I consider Jeseral Crater

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<v Speaker 3>where perseverances right now. The images show these intricate river

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<v Speaker 3>deltas very much like say the Mississippi delta here on Earth.

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<v Speaker 3>This is where river once flowed into a vast lake,

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<v Speaker 3>depositing sediments over potentially millions of years. And within those

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<v Speaker 3>ancient sediments, scientists have found specific minerals, things like clays

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<v Speaker 3>and sulfates, phyllosilicates like smectite chlorite, or evaporates like gypsum jerriscite.

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<v Speaker 3>These are minerals that could only have formed if liquid

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<v Speaker 3>water was present for a long time. They're not subtle hints,

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<v Speaker 3>they're definitive chemical signatures, like a chemical fingerprint of past

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<v Speaker 3>water locked away for billions of years.

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<v Speaker 2>Okay, so dry lakes, specific minerals.

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<v Speaker 3>What else, Well, beyond that, we see these dramatic valley

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<v Speaker 3>networks etched into the landscape. They're not just random cracks,

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<v Speaker 3>intricate branching systems, really similar in their shape their morphology

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<v Speaker 3>to river systems on Earth. Think of those dendritic patterns

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<v Speaker 3>you see in aerial photos of the Amazon Basin, for example,

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<v Speaker 3>right like tree branches spreading out precisely. And these aren't

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<v Speaker 3>just small channels. They're often kilometers wide, hundreds of meters deep.

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<v Speaker 3>They're unmistakable evidence carved by the relentless flow of ancient rivers,

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<v Speaker 3>long lived rivers, not just you know, flash floods. And

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<v Speaker 3>then there are the sedimentary layers. You can see them

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<v Speaker 3>in canyon walls like in valasmarneras or exposed in crater rims.

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<v Speaker 3>These finely stratified deposits laid down layer upon layer over

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<v Speaker 3>vast time scales. There are textbook examples of deposition and

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<v Speaker 3>standing bodies of water to light sediments settle in lakes

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<v Speaker 3>or seas here on Earth, it indicates a long sustained

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<v Speaker 3>period of water activity. All of this taken together piints

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<v Speaker 3>this vivid, irrefutable picture of a world that was once

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<v Speaker 3>rich in water.

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<v Speaker 2>So yeah, this overwhelming evidence that really begs the question,

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<v Speaker 2>doesn't it. How could a planet now so incredibly arid,

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<v Speaker 2>so seemingly lifeless, have once supported such an abundance of

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<v Speaker 2>liquid water. What allowed for that much thicker atmosphere and

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<v Speaker 2>a milder climate, the conditions that were clearly needed for

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<v Speaker 2>surface water to exist. It's just such a radical transformation,

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<v Speaker 2>a monumental shift. What drove such a huge change?

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<v Speaker 4>Okay, To really get a handle on Mars's incredible transformation

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<v Speaker 4>from potentially watery to the col dry world we see,

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<v Speaker 4>we need to understand something absolutely vital about our own planet. First, Earth,

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<v Speaker 4>It's internal engine, it's heart, you could say. So, if

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<v Speaker 4>we're trying to figure out Mars's big shift, we really

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<v Speaker 4>need to start with Earth, don't we. I mean, why

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<v Speaker 4>is our internal engine, so incredibly good at protecting our

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<v Speaker 4>atmosphere and keeping life going.

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<v Speaker 3>Yeah, well it connect this to the bigger picture, the

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<v Speaker 3>whole idea of planetary habitability. A key property of Earth's

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<v Speaker 3>remarkable ability to sustain life comes directly from its core.

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<v Speaker 3>Our planet has what we call a differentiated core. There's

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<v Speaker 3>a solid inner core mostly iron and nickel, and that's

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<v Speaker 3>surrounded by a churning, swirling liquid outer core, also mainly

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<v Speaker 3>iron and nickel, but mixed with some lighter elements like

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<v Speaker 3>soul for an oxygen. It's this dynamic internal structure that's

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<v Speaker 3>absolutely critical for generating or its global magnetic field.

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<v Speaker 2>Okay, solid inner, liquid outer.

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<v Speaker 3>And this specific arrangement is what drives the geodynamo effect. Essentially,

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<v Speaker 3>you have convexing currents within that liquid outer layer. Think

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<v Speaker 3>of like boiling water, but with molten metal. These currents

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<v Speaker 3>are driven by heat escaping from the salt inner core

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<v Speaker 3>as it cools and crystallizes, and also by the planet's rotation.

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<v Speaker 3>The Coriolis effects stirs things up, and this whole process

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<v Speaker 3>generates a powerful expanse of magnetic field. This field stretches

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<v Speaker 3>way out into space, forming this invisible protective bubble around

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<v Speaker 3>our entire planet. We call it the magnetosphere. It's a

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<v Speaker 3>truly amazing self sustaining system.

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<v Speaker 2>So it's like an invisible shield. That's a good way

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<v Speaker 2>to think about it constantly deflecting all this harmful stuff

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<v Speaker 2>from the sun, charged particles exactly.

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<v Speaker 3>It deflects harmful charged particles that are constantly blasted out

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<v Speaker 3>by the Sun, especially during solar flares and chronal mass ejections.

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<v Speaker 3>These solar winds, as they're called, are incredibly energetic streams

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<v Speaker 3>of protons and electrons, and without that magnetospheric shield, they

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<v Speaker 3>would just relentlessly strip away our atmosphere over geological time.

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<v Speaker 2>Like a sand blaster.

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<v Speaker 3>Yeah, that's a good analogy. Much like a powerful sand

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<v Speaker 3>blaster eroding rock. It's this continuous, silent battle happening way

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<v Speaker 3>above our heads. The magnetosphere acts like a bouncer, basically

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<v Speaker 3>redirecting these high energy particles around Earth. Without this magnetic protection,

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<v Speaker 3>our atmosphere, and along with it, the conditions for life

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<v Speaker 3>would slowly but surely vanish. It's also why we get

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<v Speaker 3>the auroras, the northern and Southern lights, that some of

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<v Speaker 3>those deflected particles interacting with our atmosphere near the poles,

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<v Speaker 3>a beautiful side effect of our planet's shield.

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<v Speaker 2>Okay, that makes sense. So with that essential understanding of

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<v Speaker 2>Earth's shield in mind, what about Mars. Does it have

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<v Speaker 2>a similar life preserving magnetic field today? Because I mean,

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<v Speaker 2>if it doesn't, that immediately points to a very different situation,

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<v Speaker 2>doesn't it maybe one vulnerability of loss currently, No.

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<v Speaker 3>It doesn't. Mars utterly lacks a global magnetic field today,

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<v Speaker 3>certainly nothing like Earth's. This is a critical difference and

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<v Speaker 3>a major reason why Mars is the cold, dry world

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<v Speaker 3>we see now. However, and this is a really crucial

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<v Speaker 3>piece of the puzzle. The evidence points to a very

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<v Speaker 3>different pass from Mars too, from residual magnetization found embedded

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<v Speaker 3>in the Martian crust. Essentially, you have rocks on the

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<v Speaker 3>surface that still hold a Foffel magnetic signature. This signature

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<v Speaker 3>dates back to when they first formed and cooled down

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<v Speaker 3>billions of years ago in the presence of an active

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<v Speaker 3>magnetic field. Scientists are quite confident that Mars did once

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<v Speaker 3>possess such a global field.

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<v Speaker 2>So it had a shield too early on, it.

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<v Speaker 3>Seems so orbiting spacecraft like Mars Global surveyor actually mapped

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<v Speaker 3>these magnetic anomalies in the crust. They confirmed that an

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<v Speaker 3>ancient dynamo was active, likely for maybe the first billion

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<v Speaker 3>years or so of Mars's history. And this ancient field

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<v Speaker 3>was probably generated by a core structure similar to Earth's,

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<v Speaker 3>meaning it likely had a soltid inner core and a

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<v Speaker 3>liquid outer core capable of driving that dynamo.

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<v Speaker 2>Okay, so it had one, but lost it. What are

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<v Speaker 2>the implications of that loss?

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<v Speaker 3>They're profound, truly profound. It marks a pivotal moment in

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<v Speaker 3>Mars's story. Scientists generally hypothesize that the eventual loss of

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<v Speaker 3>this magnetic field was a critical turning point, perhaps the

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<v Speaker 3>critical turning point. Without that protective shield, the relentless solar

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<v Speaker 3>wind would have had direct, unimpeded access to Mars's ancient, much.

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<v Speaker 2>Thicker atmosphere, right, no more bouncer.

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<v Speaker 3>Exactly, over millions, hundreds of millions of years, this energetic

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<v Speaker 3>bombardment would have stripped that atmosphere away, particle by particle

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<v Speaker 3>through processes like sputtering where particles get knocked off and

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<v Speaker 3>ion pickup, where atmospheric gases get carried away by the

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<v Speaker 3>solar wind. Think of it like a constant slow leak

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<v Speaker 3>into space. This atmospheric loss, in turn, would have led

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<v Speaker 3>directly to the rapid and irreversible loss of surface liquid water.

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<v Speaker 3>As the atmospheric pressure dropped, water just couldn't stay liquid

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<v Speaker 3>on the surface anymore. It would either freeze or subtlee

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<v Speaker 3>may turn directly into gas and escape into space, or

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<v Speaker 3>maybe retreat underground. It's this cascading chain of events starting

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<v Speaker 3>deep inside the planet with the dying dynamo that ultimately

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<v Speaker 3>led to the barren landscape we see today.

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<v Speaker 2>Wow, so it all comes back to the core. This

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<v Speaker 2>really raises that central question. Then, what exactly happened to

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<v Speaker 2>Mars's internal engine? What switched off that planetary dynamo? What

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<v Speaker 2>turned Mars from potentially vibrant and watery into the desert?

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<v Speaker 2>It is now that's the core mystery, isn't it. And

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<v Speaker 2>to answer that, we couldn't just look at the surface anymore.

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<v Speaker 2>We had to go deeper, which is precisely why missions

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<v Speaker 2>like Insight were conceived right precisely.

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<v Speaker 3>Yeah, while missions like NASA's amazing Rover, Spirit, Opportunity, Curiosity,

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<v Speaker 3>Perseverance have been fantastic surface geologists, you know, analyzing rocks

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<v Speaker 3>and soil and orbiters like esay's exomrs trace gas orbit

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<v Speaker 3>or study the water cycle, and NASA has made an

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<v Speaker 3>end look specifically at an atmospheric loss. A fundamentally different

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<v Speaker 3>kind of mission was needed to probe that core question,

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<v Speaker 3>the question about the planets deep into We needed to listen, not.

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<v Speaker 2>Just look, and that mission was NASA's Insight Lander. It

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<v Speaker 2>touched down quite incredibly back in November twenty eighteen, landed

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<v Speaker 2>in a region called Elysium Planitia, chosen because it's relatively

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<v Speaker 2>flat geologically quiet, which is ideal for its sensitive instruments.

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<v Speaker 2>Its primary goal, really groundbreaking, was to study seismic activity

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<v Speaker 2>marsquakes as we call them. The aim was to reveal

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<v Speaker 2>for the very first time the planet's internal structure, its crust,

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<v Speaker 2>its mantle, and crucially its core. Insight listened patiently to

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<v Speaker 2>Mars for four years, making its last contact in December

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<v Speaker 2>twenty twenty two. Sadly its solar panels got too dusty

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<v Speaker 2>to keep it powered. But it's data that continues to

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<v Speaker 2>revolutionize our understanding. It's this treasure trope scientists are still

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

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<v Speaker 2>In twenty twenty one, there was this seminal paper, a

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<v Speaker 2>truly landmark study that came out of the Insight mission

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<v Speaker 2>led by Simon Staylor and his colleagues. This paper gave

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<v Speaker 2>us the very first direct look, the first robust measurement

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<v Speaker 2>of Mars core. So, after all that anticipation, all that listening,

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<v Speaker 2>what did they actually find? What was the initial verdict

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<v Speaker 2>on Mars depth secret.

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<v Speaker 3>Well, using that invaluable data from the marsquakes, those faint

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<v Speaker 3>rumbles and tremors deep inside the planet, Stealer's team analyzed

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<v Speaker 3>how the seismic waves traveled through Mars. Think of it

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<v Speaker 3>like shouting into a canyon and timing the echoes. Different

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<v Speaker 3>materials inside the planet reflect and transmit seismic waves differently. Okay,

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<v Speaker 3>So by precisely timing how these marsquake echoes, specifically the

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<v Speaker 3>Pea waves which are compressional waves and s ways the

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<v Speaker 3>Shearer waves traveled from the quake's origin through the crust,

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<v Speaker 3>the mantle, down into the core, maybe reflecting off internal boundaries,

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<v Speaker 3>and then finally traveling back up to inside supersensitive seismometer

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<v Speaker 3>called SACE, they could literally map the internal layers like

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<v Speaker 3>a planetary sonogram. It was the first time we ever

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<v Speaker 3>directly heard Mars's internal structure. Incredible, So what did that

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<v Speaker 3>first map show? What did the core look like in

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<v Speaker 3>that twenty twenty one study, Right, So, their in depth analysis,

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<v Speaker 3>based on about a dozen of the larger marsquakes they

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<v Speaker 3>had recorded by then, revealed a few key things. Some

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<v Speaker 3>were a bit surprising at the time. They modeled a

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<v Speaker 3>core with just a single liquid layer, basically a big

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<v Speaker 3>molten ball of metal, and this core was surprisingly large.

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<v Speaker 3>They estimated its radius at about eighteen hundred kilometers, which

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<v Speaker 3>is roughly half of Mars's total radius, quite big for

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<v Speaker 3>a planet Mars.

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<v Speaker 2>Off the radius wow Yeah.

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<v Speaker 3>And furthermore, it turned out to be less dense than

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<v Speaker 3>you'd expect for a purely iron nickel core like Earth's.

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<v Speaker 3>Is mostly this density deficit, which they inferred from how

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<v Speaker 3>fast the seismic waves traveled through it, strongly suggested it

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<v Speaker 3>was rich in lighter elements, things like sulfur or oxygen

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<v Speaker 3>carbon maybe hydrogen mixed in with the iron and nickel.

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<v Speaker 2>And why is that important for lighter elements.

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<v Speaker 3>Well, those lighter elements significantly affect the core's melting temperature

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<v Speaker 3>if they lower it. That makes it much more likely

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<v Speaker 3>for the core to stay liquid for longer, rather than

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<v Speaker 3>solidifying quickly as the planet cools down over billions of years.

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<v Speaker 3>So this was a crucial insight. It potentially explained how

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<v Speaker 3>Mars might have kept a liquid core and maybe a

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<v Speaker 3>dynamo going for some time. And though it's smaller than.

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<v Speaker 2>Earth, okay, so large liquid less dens full of lighter elements,

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<v Speaker 2>did they say anything about a solid inner core like Earth's.

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<v Speaker 3>That's a really crucial detail from Staleler's paper, and it

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<v Speaker 3>shows how careful science is. They did not explicitly rule

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<v Speaker 3>out the possibility of a solid inner core. The authors

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<v Speaker 3>themselves meticulously stated in the paper that the signal strength

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<v Speaker 3>from the data they had at that time, and the

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<v Speaker 3>specific types of seismic waves they could confidently analyze were

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<v Speaker 3>simply not robust enough, not clear enough. They couldn't definitively

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<v Speaker 3>identify the faint signals you'd expect from seismic waves crossing

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<v Speaker 3>an intercore boundary. So it's an excellent first measurement, truly

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<v Speaker 3>a monumental achievement, but they explicitly acknowledged its limitations and

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<v Speaker 3>left room for further discoveries. It's at the stage, you know,

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<v Speaker 3>waiting for more data or better techniques to perhaps see deeper.

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<v Speaker 2>Right, And science is truly a journey, isn't it? Not

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<v Speaker 2>just one destination. So while Staler's work was absolutely monumental,

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<v Speaker 2>a groundbreaking first look, the story of Mars core or

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<v Speaker 2>as you said, didn't stop there. Just recently, new even

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<v Speaker 2>more refined results came out. This was from Hwixingbe and

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<v Speaker 2>colleagues published in the journal Nature. And this took our

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<v Speaker 2>understanding to a whole new level, didn't it. What did

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<v Speaker 2>they uncover that was so significant building on that initial

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<v Speaker 2>foundation laid by Staler's team.

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<v Speaker 3>Yeah, this is a fantastic example of scientific progress in action.

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<v Speaker 3>You see one study building directly on the previous one

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<v Speaker 3>and also the power of persistent, clever data analysis. This

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<v Speaker 3>latest study by Biling colleagues, they leveraged additional insight data

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<v Speaker 3>data collected over a longer period after Staler's first analysis,

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<v Speaker 3>So that meant a larger catalog of Mars quakes to

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<v Speaker 3>work with, including some that were perhaps deeper or more energetic,

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<v Speaker 3>sending clearer signals through the core. Okay, more data, more data, yes,

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<v Speaker 3>But crucially they also employed some novel and highly sophisticated

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<v Speaker 3>data analysis techniques, new ways of processing the signals. By

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<v Speaker 3>carefully selecting specific types of seismic events, ones that happened

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<v Speaker 3>at just the right distances from d site to maximize

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<v Speaker 3>the chance of detecting faint reflections from deep within, and

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<v Speaker 3>then expertly extracting an incredibly weak signal from what was

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<v Speaker 3>often quite a lot of instrument noise, they managed something remarkable.

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<v Speaker 3>It was like seismological detective work, filtering out all the

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<v Speaker 3>background chatter to finally hear the planet's deepest whispers clearly.

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<v Speaker 2>And what did those whispers tell them? What was the

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<v Speaker 2>key finding?

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<v Speaker 3>Their key finding was unambiguous. They identified the clear presence

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<v Speaker 3>of a solid layer within the liquid Martian core. This

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<v Speaker 3>wasn't just a subtle hint. It was the distinct solid

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<v Speaker 3>inner core, and they even estimated its radius at approximately

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<v Speaker 3>six hundred and ten kilometers.

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<v Speaker 2>Six hundred and ten kilometers. How does that compare to

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<v Speaker 2>the overall core size.

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<v Speaker 3>Well, if the total core radius is around eighteen hundred kilometers,

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<v Speaker 3>then six hundred and ten kilometers is a substantial fraction,

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<v Speaker 3>about a third of the radius, or roughly fifteen percent

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<v Speaker 3>of Mars's total radius is this solid inner core. This

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<v Speaker 3>is a profound revision to our understanding. It shifts our

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<v Speaker 3>model of Mars's interior from that simple, fully liquid core

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<v Speaker 3>picture to a more complex, differentiated one, much more like

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<v Speaker 3>Earth's structure.

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<v Speaker 2>Okay, wow, so we thought it was just liquid and

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<v Speaker 2>now we find this distinct solid part inside. That feels

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<v Speaker 2>like a really big shift. What does this solid inner

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<v Speaker 2>core actually mean for understanding Mars's history and crucially for

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<v Speaker 2>that long loss magnetic field we talked about, Why is

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<v Speaker 2>this particular detail solid inside liquid such a big deal?

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<v Speaker 2>How does it connect to a planet's life support system? Well,

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<v Speaker 2>what's truly profound here is the implication this discovery carries.

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<v Speaker 3>It's huge. The very presence of a solid inner core

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<v Speaker 3>tells us definitively that crystallization is happening. Solidification is taking

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<v Speaker 3>place as the planet cools over geological time. This process

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<v Speaker 3>where liquid metal slowly solidifies at the center and in

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<v Speaker 3>doing so releases latent heat and lighter elements. This process

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<v Speaker 3>is absolutely critical for a planet like Earth to generate

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<v Speaker 3>and sustain its magnetic field for billions of years. It's

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<v Speaker 3>essentially the engine that drives the planetary dynamo.

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<v Speaker 2>Ah. Okay, so the solidifying process itself is the key.

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<v Speaker 3>Yeah, exactly. To elaborate a bit on its magnificance, a

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<v Speaker 3>core structure with both a solid inner part and a

390
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<v Speaker 3>liquid outer layer is fundamentally much more like Earth's setup

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<v Speaker 3>On Earth, It's precisely the temperature differences and the chemical

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<v Speaker 3>change is happening at that boundary between the solid inner

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<v Speaker 3>core and the swirling liquid outer core, plus the heat

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<v Speaker 3>flowing out into the surrounding mantle that drive the vigorous

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<v Speaker 3>convection currents in that liquid outer layer. As the core

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<v Speaker 3>cools iron crystallizes onto the inner core, this process releases lighter,

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<v Speaker 3>more buoyant elements into the liquid outer core, and these

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<v Speaker 3>lighter fluids than rise, creating convection like a lava lamp effect,

399
00:21:35.799 --> 00:21:39.279
<v Speaker 3>but with molten metal. These convection currents, this organized movement

400
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<v Speaker 3>of molten electrically conducting metal, coupled with the planet's spin,

401
00:21:43.440 --> 00:21:45.759
<v Speaker 3>are the engine from the dynamo that generates a planetary

402
00:21:45.839 --> 00:21:49.000
<v Speaker 3>magnetic field. Therefore, this new discovery of a solid inner

403
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<v Speaker 3>core on Mars makes it significantly more likely, much more plausible,

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<v Speaker 3>that a robust dynamo capable of producing a protective magnetic field,

405
00:21:58.039 --> 00:22:00.960
<v Speaker 3>was indeed active on Mars early in its own and

406
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<v Speaker 3>perhaps it was sustained for significant period. It provides that

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<v Speaker 3>missing ingredient, that earth like structure needed for a strong,

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<v Speaker 3>long lasting dynamo.

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<v Speaker 2>And for you listening right now, this gives us a

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<v Speaker 2>much clearer, much more scientifically solid pathway for Mars to

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<v Speaker 2>have once had the conditions needed for a thicker atmosphere

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<v Speaker 2>and as a result that abundant flowing liquid water on

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<v Speaker 2>its surface that the geology points to. It connects the

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<v Speaker 2>deep hidden internal processes of the planet directly to the

415
00:22:30.079 --> 00:22:33.039
<v Speaker 2>surface conditions we were talking about earlier. It closes a

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<v Speaker 2>major loop in our understanding of how Mars could have

417
00:22:35.519 --> 00:22:36.799
<v Speaker 2>been so different back then.

418
00:22:37.039 --> 00:22:39.799
<v Speaker 4>Okay, so when we hear about one study like Stalers

419
00:22:39.799 --> 00:22:43.079
<v Speaker 4>in twenty twenty one initially suggesting a fully liquid core,

420
00:22:43.119 --> 00:22:45.960
<v Speaker 4>and then another one like Bins just recently reporting a

421
00:22:46.000 --> 00:22:48.400
<v Speaker 4>solid inner core, it might, you know, at first glance,

422
00:22:48.440 --> 00:22:51.799
<v Speaker 4>sound like a scientific argument, maybe even a controversy or contradiction.

423
00:22:52.559 --> 00:22:53.440
<v Speaker 3>That's absolutely not.

424
00:22:53.480 --> 00:22:55.400
<v Speaker 4>What's happening here is that this is actually a really

425
00:22:55.440 --> 00:22:58.839
<v Speaker 4>wonderful illustration of how science actually works. It's self correcting

426
00:22:58.920 --> 00:22:59.839
<v Speaker 4>progressive nature.

427
00:23:00.000 --> 00:23:02.720
<v Speaker 3>Absolutely not a controversy, noe, not in the sense of

428
00:23:02.720 --> 00:23:06.640
<v Speaker 3>a fight. It's actually an excellent and incredibly common example

429
00:23:06.680 --> 00:23:10.799
<v Speaker 3>of the iterative nature of science how data collection and

430
00:23:10.839 --> 00:23:14.920
<v Speaker 3>analysis evolve. Staler's initial findings in twenty twenty one were,

431
00:23:15.000 --> 00:23:19.519
<v Speaker 3>without question groundbreaking. A huge first step. They provided the

432
00:23:19.559 --> 00:23:22.799
<v Speaker 3>first solid constraints on Mars's core size and state, a

433
00:23:22.880 --> 00:23:26.799
<v Speaker 3>monumental achievement, giving us that first internal glimpse. But as

434
00:23:26.839 --> 00:23:30.119
<v Speaker 3>they themselves very carefully noted in their paper, the data

435
00:23:30.160 --> 00:23:32.559
<v Speaker 3>they had available at that specific time and the methods

436
00:23:32.599 --> 00:23:36.480
<v Speaker 3>they used just didn't have the necessary signal strength or clarity.

437
00:23:36.759 --> 00:23:39.880
<v Speaker 3>They couldn't definitively confirm or deny the existence of a

438
00:23:39.960 --> 00:23:43.440
<v Speaker 3>solid inner core. They were very clear about that limitation,

439
00:23:43.480 --> 00:23:45.519
<v Speaker 3>which is just part of good scientific.

440
00:23:45.039 --> 00:23:47.960
<v Speaker 2>Practice, right. They pointed out what they couldn't see yet exactly.

441
00:23:48.160 --> 00:23:50.319
<v Speaker 3>So it's not about one being right and the other wrong.

442
00:23:50.799 --> 00:23:53.680
<v Speaker 3>Staler's twenty twenty one work was the best possible model

443
00:23:53.720 --> 00:23:56.559
<v Speaker 3>based on the data and techniques available. Then the new

444
00:23:56.599 --> 00:23:59.720
<v Speaker 3>study by billion colleagues, well, they benefited from more data,

445
00:24:00.119 --> 00:24:04.119
<v Speaker 3>newer data accumulated as Insight kept listening recording more marsquakes,

446
00:24:04.119 --> 00:24:07.880
<v Speaker 3>maybe some deeper or stronger ones. And crucially they applied

447
00:24:07.960 --> 00:24:12.559
<v Speaker 3>more refined novel data analysis techniques. They basically found clever

448
00:24:12.640 --> 00:24:15.759
<v Speaker 3>ways to pull out those weaker, more subtle seismic signals

449
00:24:16.359 --> 00:24:19.200
<v Speaker 3>stignals that were previously either buried in the noise or

450
00:24:19.319 --> 00:24:22.319
<v Speaker 3>just beyond the detection capability of the earlier methods. It's

451
00:24:22.319 --> 00:24:25.720
<v Speaker 3>his continuous process. Initial models based on the best evidence

452
00:24:25.759 --> 00:24:28.839
<v Speaker 3>of the time, get tested, refined, expanded upon as new

453
00:24:28.839 --> 00:24:32.240
<v Speaker 3>information comes in and as the analytical tools themselves get better.

454
00:24:32.400 --> 00:24:35.720
<v Speaker 3>This is precisely how scientific understanding deepens. It becomes more

455
00:24:35.720 --> 00:24:38.440
<v Speaker 3>precise over time, with each new study building carefully on

456
00:24:38.480 --> 00:24:39.119
<v Speaker 3>the last one.

457
00:24:39.160 --> 00:24:41.920
<v Speaker 2>It's a fantastic example of the scientific method in action,

458
00:24:42.000 --> 00:24:45.200
<v Speaker 2>isn't it Not like a Suiden Eureka moment, but this persistent,

459
00:24:45.440 --> 00:24:49.240
<v Speaker 2>incremental build up of knowledge, and you see this iterative

460
00:24:49.279 --> 00:24:54.359
<v Speaker 2>process even within related research groups you mentioned. Even Staler's

461
00:24:54.359 --> 00:24:57.000
<v Speaker 2>initial model was revised slightly in twenty twenty three.

462
00:24:57.039 --> 00:24:59.559
<v Speaker 3>That's right by Ari Hamuel from University of Pariseta and

463
00:24:59.640 --> 00:25:03.680
<v Speaker 3>his column. Their updates help to further reconcile insight seismic

464
00:25:03.720 --> 00:25:07.640
<v Speaker 3>findings with other existing evidence about Mars's core size and density.

465
00:25:08.119 --> 00:25:11.359
<v Speaker 3>Often these refinements incorporate other types of geophysical data too,

466
00:25:11.759 --> 00:25:15.480
<v Speaker 3>constraints from Mars's gravity field measurements or its rotation, things

467
00:25:15.519 --> 00:25:19.319
<v Speaker 3>learned from orbiters. This ongoing dialogue, this constant refinement of

468
00:25:19.400 --> 00:25:22.400
<v Speaker 3>models and theories as new data comes in. It's absolutely

469
00:25:22.400 --> 00:25:25.920
<v Speaker 3>central to how science progresses. It's really collaborative, not confrontational,

470
00:25:26.119 --> 00:25:28.160
<v Speaker 3>a shared journey towards getting a clearer picture.

471
00:25:28.359 --> 00:25:31.559
<v Speaker 2>Okay, so this isn't the final word, the absolute end

472
00:25:31.559 --> 00:25:34.559
<v Speaker 2>of the story about Mars's core, but it's a major

473
00:25:34.680 --> 00:25:38.759
<v Speaker 2>new chapter, a really significant one. What does this new discovery,

474
00:25:38.839 --> 00:25:41.880
<v Speaker 2>this confirmation of a solid inner core mean for the

475
00:25:41.920 --> 00:25:45.880
<v Speaker 2>scientific community moving forward? What can we expect next in

476
00:25:45.920 --> 00:25:49.000
<v Speaker 2>Martian science? Now this piece is in place.

477
00:25:49.480 --> 00:25:52.519
<v Speaker 3>Oh, this result is absolutely going to have a significant

478
00:25:52.519 --> 00:25:56.240
<v Speaker 3>and I think very exciting impact within the planetary science community.

479
00:25:56.559 --> 00:26:00.400
<v Speaker 3>We could definitely expect more reanalyzies of the entire insight

480
00:26:00.519 --> 00:26:04.039
<v Speaker 3>data set. That's almost guaranteed. Scientists will be scrutinizing these

481
00:26:04.079 --> 00:26:07.759
<v Speaker 3>new methods used by Bees and colleagues looking for independent confirmation.

482
00:26:08.000 --> 00:26:10.880
<v Speaker 3>They'll likely apply these techniques to other seismic events, maybe

483
00:26:10.880 --> 00:26:12.759
<v Speaker 3>look at different types of seismic waves to see if

484
00:26:12.759 --> 00:26:16.079
<v Speaker 3>they can consistently detect that solid inncore signal and maybe

485
00:26:16.160 --> 00:26:18.839
<v Speaker 3>refine its properties even further. The goal is always to

486
00:26:18.880 --> 00:26:21.519
<v Speaker 3>solidify a finding like this through multiple lines of evidence,

487
00:26:21.599 --> 00:26:23.079
<v Speaker 3>multiple analyzes.

488
00:26:22.640 --> 00:26:24.680
<v Speaker 2>Makes sense, check the work basically.

489
00:26:24.519 --> 00:26:28.079
<v Speaker 3>Exactly, check the work, try different approaches, and beyond just

490
00:26:28.119 --> 00:26:30.680
<v Speaker 3>the seismology, there will be thorough discussion about the broader

491
00:26:30.720 --> 00:26:34.960
<v Speaker 3>geological and geophysical context. Researchers will be looking in detail

492
00:26:35.000 --> 00:26:38.000
<v Speaker 3>at how this new model of Mars's interior solid inner

493
00:26:38.039 --> 00:26:41.400
<v Speaker 3>core liquid outer core fits with everything else we know.

494
00:26:41.920 --> 00:26:45.960
<v Speaker 3>That includes geochemical models of Mars's bulk composition, the precise

495
00:26:46.079 --> 00:26:49.119
<v Speaker 3>gravity field data from orbiters that tells us about mass

496
00:26:49.119 --> 00:26:52.240
<v Speaker 3>distribution inside the planet, and those previous studies of the

497
00:26:52.279 --> 00:26:57.519
<v Speaker 3>crustal magnetic anomalies. This collaborative, cross disciplinary process is how

498
00:26:57.559 --> 00:27:01.519
<v Speaker 3>we strengthen our collective understanding of planetary evil. It ensures

499
00:27:01.519 --> 00:27:05.160
<v Speaker 3>the model makes sense in the big picture. It's honestly

500
00:27:05.200 --> 00:27:08.359
<v Speaker 3>a very exciting time for Martian seismology and planetary science.

501
00:27:08.640 --> 00:27:12.119
<v Speaker 3>It's prompting new theoretical models and definitely fueling further investigations

502
00:27:12.119 --> 00:27:14.720
<v Speaker 3>into the red planet's deep past and maybe even its

503
00:27:14.759 --> 00:27:15.480
<v Speaker 3>future evolution.

504
00:27:15.759 --> 00:27:18.319
<v Speaker 2>So let's pull back for the big picture, then, the

505
00:27:18.440 --> 00:27:23.480
<v Speaker 2>grand narrative of planetary science. Why is understanding the insight

506
00:27:23.559 --> 00:27:27.440
<v Speaker 2>of Mars this newly revealed internal structure. Why is it

507
00:27:27.480 --> 00:27:30.000
<v Speaker 2>so critical not just for Mars itself, but for our

508
00:27:30.079 --> 00:27:33.119
<v Speaker 2>fundamental understanding of planets in general, you know broth here

509
00:27:33.119 --> 00:27:35.319
<v Speaker 2>in our Solar System and maybe even worlds beyond.

510
00:27:35.799 --> 00:27:38.160
<v Speaker 3>Yeah, this really raises an important question that goes way

511
00:27:38.160 --> 00:27:42.119
<v Speaker 3>beyond just Mars. Understanding the interior structure of any planet

512
00:27:42.119 --> 00:27:46.160
<v Speaker 3>in our Solar System is absolutely critical. It's fundamental if

513
00:27:46.200 --> 00:27:49.599
<v Speaker 3>we want to develop robust, accurate theories about how these

514
00:27:49.599 --> 00:27:52.119
<v Speaker 3>celestial bodies form in the first place, how they grow,

515
00:27:52.400 --> 00:27:55.799
<v Speaker 3>and crucially, how they evolve over billions of years. The

516
00:27:55.839 --> 00:27:59.359
<v Speaker 3>core really is the engine of planetary change. It influences

517
00:27:59.400 --> 00:28:01.680
<v Speaker 3>everything from the geology on the surface to whether a

518
00:28:01.720 --> 00:28:05.880
<v Speaker 3>planet can hold onto its atmosphere. Consider this before insights work,

519
00:28:06.000 --> 00:28:10.200
<v Speaker 3>and especially before this latest discovery confirming the solid inner core.

520
00:28:11.519 --> 00:28:14.640
<v Speaker 3>Models for Mars that suggested an internal structure very similar

521
00:28:14.640 --> 00:28:18.079
<v Speaker 3>to or specifically the differentiated core, with both liquid and

522
00:28:18.240 --> 00:28:21.960
<v Speaker 3>solid parts capable of powering a long lived dynamo. Well,

523
00:28:22.359 --> 00:28:26.039
<v Speaker 3>they weren't generally favored. Many models lean towards Mars having

524
00:28:26.079 --> 00:28:29.480
<v Speaker 3>cooled faster, maybe having a fully liquid core, or perhaps

525
00:28:29.559 --> 00:28:31.759
<v Speaker 3>one with a different composition that just couldn't support a

526
00:28:31.839 --> 00:28:33.720
<v Speaker 3>dynamo for as long as Earth's is run.

527
00:28:34.039 --> 00:28:37.720
<v Speaker 2>So this discovery really changes that baseline assumption. It shifts

528
00:28:37.720 --> 00:28:41.759
<v Speaker 2>the perspective dramatically. Yes, this confirmation of a solid inner

529
00:28:41.799 --> 00:28:44.559
<v Speaker 2>core means Mars's early history might have been much more

530
00:28:44.599 --> 00:28:47.759
<v Speaker 2>earth like deep down than we generally thought possible. And

531
00:28:47.839 --> 00:28:51.440
<v Speaker 2>this knowledge helps us cackle these really fundamental, profound questions

532
00:28:51.799 --> 00:28:54.880
<v Speaker 2>like how big does a rocky planet need to be

533
00:28:55.200 --> 00:28:58.200
<v Speaker 2>to generate and sustain a protective magnetic field over billions

534
00:28:58.240 --> 00:29:02.160
<v Speaker 2>of years? What are the keing re radients, the compositional factors,

535
00:29:02.200 --> 00:29:04.519
<v Speaker 2>the thermal conditions required for a planet to maintain the

536
00:29:04.559 --> 00:29:07.720
<v Speaker 2>habitable climate, an environment where liquid water can persist over

537
00:29:07.759 --> 00:29:11.400
<v Speaker 2>those vast stretches of geological time. It pushes us to

538
00:29:11.400 --> 00:29:14.519
<v Speaker 2>rethink the minimum requirements maybe for forming an earth like

539
00:29:14.559 --> 00:29:18.519
<v Speaker 2>planetary system, and for you listening right now, this knowledge

540
00:29:18.519 --> 00:29:21.640
<v Speaker 2>it stretches far beyond just our red neighbor, doesn't it.

541
00:29:21.640 --> 00:29:25.440
<v Speaker 2>It directly feeds into our ongoing very ambitious search for

542
00:29:25.519 --> 00:29:30.079
<v Speaker 2>habitable exoplanets, those world's orbiting distance stars. As we find

543
00:29:30.119 --> 00:29:32.720
<v Speaker 2>more and more exoplanets, this detailed case study of Mars

544
00:29:32.799 --> 00:29:36.000
<v Speaker 2>gives us crucial reference points what to look for. Perhaps

545
00:29:36.200 --> 00:29:39.440
<v Speaker 2>it helps us better understand the precious rarity of Earth conditions,

546
00:29:39.559 --> 00:29:43.599
<v Speaker 2>especially that long lived active geodynamo providing our essential shield.

547
00:29:44.079 --> 00:29:46.400
<v Speaker 2>It really highlights what a truly unique, and you could

548
00:29:46.400 --> 00:29:49.680
<v Speaker 2>say fortunate world, our home planet is still protected by

549
00:29:49.680 --> 00:29:52.279
<v Speaker 2>its powerful internal engine humming along after four and a

550
00:29:52.319 --> 00:29:55.559
<v Speaker 2>half billion years. So we're left with a much richer picture, now,

551
00:29:55.640 --> 00:29:58.519
<v Speaker 2>a far more dramatic and ultimately a more nuanced story

552
00:29:58.519 --> 00:30:00.759
<v Speaker 2>of Mars. It wasn't always it is just the cold,

553
00:30:00.839 --> 00:30:04.680
<v Speaker 2>barren desert we see today, completely lacking that global magnetic protection.

554
00:30:04.759 --> 00:30:07.079
<v Speaker 2>It seems it had a fighting chance, didn't it, an

555
00:30:07.079 --> 00:30:09.599
<v Speaker 2>internal engine that was once very much alive.

556
00:30:09.359 --> 00:30:12.480
<v Speaker 3>In kicking Precisely, we now have much stronger, more direct

557
00:30:12.480 --> 00:30:15.319
<v Speaker 3>seismic evidence supporting it. Past Mars, that was a truly

558
00:30:15.400 --> 00:30:18.720
<v Speaker 3>dynamic world, a world with an earth like core generating

559
00:30:18.720 --> 00:30:21.720
<v Speaker 3>a powerful magnetic field, which in turn likely sustained a

560
00:30:21.720 --> 00:30:26.240
<v Speaker 3>thicker atmosphere and allowed for very probably abundant flowing liquid

561
00:30:26.240 --> 00:30:29.880
<v Speaker 3>water on its surface. Its transformation into the cold, dry

562
00:30:29.920 --> 00:30:32.920
<v Speaker 3>desert planet we know today wasn't instantaneous, but it was

563
00:30:32.960 --> 00:30:37.160
<v Speaker 3>this gradual yet profound planetary drama, a saga driven directly

564
00:30:37.160 --> 00:30:40.279
<v Speaker 3>from its very core outwards as that internal engine eventually

565
00:30:40.279 --> 00:30:43.640
<v Speaker 3>cool slowed down, and the dynamo dyet. It serves as

566
00:30:43.720 --> 00:30:47.519
<v Speaker 3>this really powerful illustration how the internal processes of a planet,

567
00:30:47.680 --> 00:30:50.720
<v Speaker 3>those hidden mechanics deep beneath the surface, ultimately dictate the

568
00:30:50.759 --> 00:30:55.279
<v Speaker 3>surface environment and by extension, is potential for supporting life. Mars,

569
00:30:55.319 --> 00:30:57.640
<v Speaker 3>in many ways, is a cautionary dale. It's a natural

570
00:30:57.680 --> 00:30:59.880
<v Speaker 3>laboratory showing us what can happen when a planet loses

571
00:30:59.880 --> 00:31:03.119
<v Speaker 3>the vital internal protections hashtash tag tag outrop.

572
00:31:03.200 --> 00:31:07.480
<v Speaker 2>Wow, what an incredible journey we've taken today, Venturing from

573
00:31:07.519 --> 00:31:10.480
<v Speaker 2>the dusty, familiar surface of Mars right down to its

574
00:31:10.480 --> 00:31:15.119
<v Speaker 2>newly revealed core, a solid inner core, surprisingly earthlake. We've

575
00:31:15.160 --> 00:31:18.200
<v Speaker 2>seen how this patiently gathered seismic data collected over years

576
00:31:18.240 --> 00:31:22.400
<v Speaker 2>by insight, combined with ingenious refined analysis, can unravel mysteries

577
00:31:22.480 --> 00:31:25.599
<v Speaker 2>millions and millions of miles away. It's just a testament,

578
00:31:25.640 --> 00:31:27.880
<v Speaker 2>isn't it, to the power of scientific exploration and that

579
00:31:27.920 --> 00:31:31.680
<v Speaker 2>relentless human drive to understand our universe, one planet, one

580
00:31:31.680 --> 00:31:34.880
<v Speaker 2>core at a time. It's almost poetic really that after

581
00:31:34.920 --> 00:31:37.440
<v Speaker 2>all these years of just gazing at Mars, sending rovers

582
00:31:37.480 --> 00:31:40.720
<v Speaker 2>to taste soil, or finally getting to listen to its heartbeat.

583
00:31:40.960 --> 00:31:44.640
<v Speaker 3>Yeah, this ongoing exploration of Mars interior, it really reminds

584
00:31:44.680 --> 00:31:47.079
<v Speaker 3>us that the planets in our Solar System aren't just

585
00:31:47.119 --> 00:31:50.839
<v Speaker 3>static objects hanging in space. They are dynamic worlds. They

586
00:31:50.839 --> 00:31:55.319
<v Speaker 3>have complex, often dramatic histories. They're constantly evolving, constantly transforming

587
00:31:55.359 --> 00:31:59.079
<v Speaker 3>over cosmic time scales. The Insight mission, even though it's

588
00:31:59.079 --> 00:32:01.599
<v Speaker 3>now silent on the marsh and planes, it continues to

589
00:32:01.599 --> 00:32:04.799
<v Speaker 3>speak volumes through its invaluable data. It's pushing us ever

590
00:32:04.880 --> 00:32:07.599
<v Speaker 3>closer to understanding the dramatic saga of the red planet

591
00:32:07.640 --> 00:32:10.799
<v Speaker 3>and really, by extension, our own place within the cosmos.

592
00:32:10.880 --> 00:32:14.440
<v Speaker 3>It truly reshapes our understanding of how planets like ours evolve.

593
00:32:14.920 --> 00:32:18.039
<v Speaker 2>So as we wrap up this exploration, maybe consider this

594
00:32:18.400 --> 00:32:21.920
<v Speaker 2>Mars story. It's journey from a potentially vibrant, watery world

595
00:32:22.200 --> 00:32:25.400
<v Speaker 2>shielded by a magnetic field, much like Earliers, perhaps to

596
00:32:25.559 --> 00:32:29.119
<v Speaker 2>the dry, barren desert it is today. It's a stark reminder,

597
00:32:29.160 --> 00:32:32.079
<v Speaker 2>isn't it, of how fragile planetary habitability it can actually be.

598
00:32:32.480 --> 00:32:36.359
<v Speaker 2>It's this delicate balance of internal processes external forces, a

599
00:32:36.440 --> 00:32:38.559
<v Speaker 2>kind of cosmic dance that can turn a world from

600
00:32:38.559 --> 00:32:40.960
<v Speaker 2>blue and wet to red and dry over billions of years.

601
00:32:41.160 --> 00:32:44.200
<v Speaker 3>And maybe ask yourself, what if lurking deep within other

602
00:32:44.359 --> 00:32:48.039
<v Speaker 3>seemingly barren worlds we observe out there there are similar clues,

603
00:32:48.640 --> 00:32:52.279
<v Speaker 3>clues to pass lives, past habitability, or maybe even the

604
00:32:52.279 --> 00:32:55.960
<v Speaker 3>subtle potential for future transformations we haven't considered. Mars really

605
00:32:56.000 --> 00:32:59.119
<v Speaker 3>asks us how truly unique is Earth state? And what

606
00:32:59.160 --> 00:33:02.240
<v Speaker 3>other profound place planetary secrets are just waiting to be revealed,

607
00:33:02.559 --> 00:33:04.920
<v Speaker 3>hidden beneath the surfaces of other worlds, just waiting for

608
00:33:05.000 --> 00:33:07.440
<v Speaker 3>us to listen patiently to their whispers across the silence

609
00:33:07.440 --> 00:33:07.880
<v Speaker 3>of space.

610
00:36:00.039 --> 00:36:10.039
<v Speaker 2>Yousssssss
