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>When you think about Mars, you know, the image that

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<v Speaker 2>instantly pops into your head is the red planet. It's dusty,

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<v Speaker 2>it's cold, desolate and just utterly profoundly dry.

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<v Speaker 3>Right, It's the planet of rust, of a thin, wispy atmosphere,

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<v Speaker 3>and we think of its surface as being carved by wind.

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<v Speaker 2>Not water, and it's looked that way for well, for eons,

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<v Speaker 2>billions of years. But here's the thing, the shift and

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<v Speaker 2>perspective that we really need. Ancient Mars. It was dramatically,

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<v Speaker 2>fantastically wet.

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<v Speaker 3>Oh absolutely, it had water flowing, collecting and eroding in

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<v Speaker 3>volumes that we are i mean only now really beginning

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<v Speaker 3>to quantify.

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<v Speaker 2>And that quantification that's the essential leap forward here, isn't

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<v Speaker 2>it is?

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<v Speaker 3>For decades the debate was really just centered on the

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<v Speaker 3>existence of water, you know, was it there?

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<v Speaker 2>We spent so long just looking for the smoking.

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<v Speaker 3>Gun exactly, and now the question has shifted entirely. It's

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<v Speaker 3>about scale, it's about structure. It wasn't just wet, it

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<v Speaker 3>was and this is the keyword organized organized.

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<v Speaker 2>What do you mean by that? Was it just random

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<v Speaker 2>pooling or yeah.

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<v Speaker 3>Well that's the question. Was it just isolated flash floods

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<v Speaker 3>from say a meteor impact melting some ice, or was

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<v Speaker 3>it sustained, integrated, almost earth like hydrology.

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<v Speaker 2>And that is precisely what we are deep diving into today.

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<v Speaker 2>We have this foundational news study from scientists at the

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<v Speaker 2>University of Texas at Austin, UT Austin, and it's just

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<v Speaker 2>been published in the Proceedings of the National Academy of Sciences.

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<v Speaker 3>And this isn't just another paper confirming water. We're so

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<v Speaker 3>far beyond that now.

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<v Speaker 2>This is the first systematic, truly comprehensive mapping of Mars's

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<v Speaker 2>ancient major river basins, it's watersheds. It's giving us a

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<v Speaker 2>colossal measure of their past power.

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<v Speaker 3>So our mission here is to take this new high

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<v Speaker 3>tech planetary cartography and really use it to gain insight

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<v Speaker 3>into three crucial areas. First, just the sheer, almost unimaginable

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<v Speaker 3>volume of water ancient Mars held, and like we said,

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<v Speaker 3>how it was organized. Second, we need to understand the tools,

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<v Speaker 3>the really ingenious techniques combining old data with new imagery

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<v Speaker 3>that scientists used to map rivers that vanished billions of

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<v Speaker 3>years ago. Fine, Finally we have to tackle the most

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<v Speaker 3>compelling mystery that all this new evidence raises. We're going

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<v Speaker 3>to review the current scientific consensus on where all that

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<v Speaker 3>water went.

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<v Speaker 2>Okay, let's unpack this. Then we're talking about an immense

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<v Speaker 2>planetary plumbing system, one that's been completely silent, dormant for

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<v Speaker 2>geological ages. So to set the scale for you right

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<v Speaker 2>at the top, here's the initial shock factor nugget from

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<v Speaker 2>this study. This first of is kind mapping identified major

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<v Speaker 2>drainage systems that reduced and estimated get this, twenty eight

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<v Speaker 2>thousand cubic kilometers of sediment.

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<v Speaker 3>Twenty eight thousand cubic kilometers. I mean, that is a

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<v Speaker 3>number that forces us to completely recalibrate our models of

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<v Speaker 3>early Mars.

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<v Speaker 2>It's not just little adjustment.

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<v Speaker 3>No, not at all. We are not talking about mere

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<v Speaker 3>streams or temporary ponds. We are talking about Earth scale,

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<v Speaker 3>continental river systems, systems capable of eroding and transporting that

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<v Speaker 3>mind boggling volume of material across vast distances on another world.

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<v Speaker 2>Just to give you an idea of that size, twenty

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<v Speaker 2>eight thousand cubic kilometers is roughly enough sediment to completely

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<v Speaker 2>bury the state of Texas. Wow, to bury it under

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<v Speaker 2>a layer of dirt one hundred.

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<v Speaker 3>Feet deep one hundred feet.

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<v Speaker 2>That's the sheer scale of the erosional power we are

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<v Speaker 2>dealing with. So, okay, we're moving from this general abstract

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<v Speaker 2>idea of water to the specific organization and structure of

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<v Speaker 2>these water systems. We know the water was there, but

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<v Speaker 2>what is the organization to that water tell us about

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<v Speaker 2>the climate on ancient mars. I think this is where

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<v Speaker 2>the new study really provides the critical insight.

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<v Speaker 3>It's the difference between finding, say a small isolated stream

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<v Speaker 3>bed in the desert right that might have been caused

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<v Speaker 3>by one single heavy rain. It's the difference between that

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<v Speaker 3>and mapping the entire Amazon River basin, which requires which

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<v Speaker 3>requires thousands, maybe millions of years of continuous predictable climate patterns.

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<v Speaker 3>And doctor Timothy A. Gouge, who led the research, he

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<v Speaker 3>encapsulated this finding perfectly. He said that while we've known

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<v Speaker 3>for a long time there were rivers on Mars, he said,

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<v Speaker 3>and I'm quoting here, we really didn't know the extent

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<v Speaker 3>to which the rivers were organized in large drainage systems

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<v Speaker 3>at the global scale.

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<v Speaker 2>Okay, let's dig into that. Why does that organization that structure,

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<v Speaker 2>Why does it change the entire debate? Why is it

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<v Speaker 2>such a monumental leap forward compared to just finding more

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<v Speaker 2>evidence of flow.

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<v Speaker 3>Because organization implies, well, it implies sustained, consistent hydrological cycles.

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<v Speaker 2>Okay, an actual cycle like on Earth, exactly like on Earth.

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<v Speaker 2>Think about our planet. When you see a massive dendritic.

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<v Speaker 3>Water dendritic meaning tree like right.

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<v Speaker 2>Like brandecisely, where smaller streams feed into tributaries, which then

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<v Speaker 2>feed into major rivers which eventually empty into an ocean.

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<v Speaker 2>That whole geological structure, it's the accumulated result of millennia

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<v Speaker 2>of stable weather. It means precipitation was consistent enough to

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<v Speaker 2>feed the entire system, runoff was predictable, and the system

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<v Speaker 2>itself was stable enough to carve deep, integrated channels over

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<v Speaker 2>a very very long time.

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<v Speaker 3>So if the water was only caused by these random

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<v Speaker 3>episodic events like a massive asteroid impact melting a bunch

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<v Speaker 3>of ice, or a huge volcano going off. You just

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<v Speaker 3>wouldn't get that integrated structure, would you. You wouldn't not

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<v Speaker 3>at this scale. Those chaotic episodic events they create isolated

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<v Speaker 3>channels or massive outflow features. Sure we see those on Mars,

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<v Speaker 3>but they don't produce a sprawling, globally scaled network of

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<v Speaker 3>interconnected systems that drain thousands of square kilometers in a

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<v Speaker 3>coordinated way. This kind of integrated system, it confirms the

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<v Speaker 3>presence of a climate that'd sustain large scale, stable river

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<v Speaker 3>flow over long periods, and that makes the ancient planet

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<v Speaker 3>much more earth like than some of the colder, dryer

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<v Speaker 3>models previously suggested.

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<v Speaker 2>And it's important to note these researchers weren't just looking

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<v Speaker 2>for small, localized streams. They intentionally set a very high

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<v Speaker 2>bar for what even qualified as a system worth mapping.

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<v Speaker 3>That's a crucial point. They were specifically hunting for the

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<v Speaker 3>planetary heavyweights.

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<v Speaker 2>So what was the threshold to define a scale?

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<v Speaker 3>They established a specific methodological threshold for inclusion. They only

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<v Speaker 3>mapped drainage systems that exceeded one hundred and five square

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<v Speaker 3>kilometers in surface area.

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<v Speaker 2>That sounds incredibly precise one hundred and five. Why that

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<v Speaker 2>specific area is it arbitrary, Not at all.

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<v Speaker 3>It's a crucial methodological anchor. One hundred and five square

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<v Speaker 3>kilometers is a common baseline area used in geology for

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<v Speaker 3>defining what qualifies as a large drainage system right here

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<v Speaker 3>on Earth.

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<v Speaker 2>Ah, so the using our own planet is the yardstick.

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<v Speaker 3>Exactly. By using this comparable terrestrial threshold, they weren't trying

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<v Speaker 3>to capture every small that might have been created by

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<v Speaker 3>some seasonal melt. They were systematically looking for features that

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<v Speaker 3>qualify as major rivers, as large scale drainage basins, the

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<v Speaker 3>kind of systems that define the regional climate and geology

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<v Speaker 3>of a planet.

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<v Speaker 2>So it ensures that what they're studying on Mars is

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<v Speaker 2>comparable in scale and in its implications to a significant

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<v Speaker 2>river system we'd recognize today.

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<v Speaker 3>Right by using that one hundred and five scare kilometer standard,

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<v Speaker 3>they are essentially saying, if the system were on Earth,

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<v Speaker 3>it would be a major hydrological feature we would study

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<v Speaker 3>in depth. It forces the conversation away from any marginal,

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<v Speaker 3>maybe temporary water activity.

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<v Speaker 2>It puts the focus squarely on the systems that did

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<v Speaker 2>the heavy lifting, the ones that really shape the surface.

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<v Speaker 3>It absolutely does, and it supports a central tenet in

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<v Speaker 3>geology we call uniformitarianism.

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<v Speaker 2>The present is the key to the past.

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<v Speaker 3>The very same idea, The same natural laws and processes

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<v Speaker 3>that operate today operated in the past. So if a

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<v Speaker 3>system of a certain size requires a sustained climate here

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<v Speaker 3>on Earth, it almost certainly required a sustained climate there

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<v Speaker 3>on Mars.

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<v Speaker 2>And the systematic approach also meant they had to define

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<v Speaker 2>exactly what components constituted an organized system. They weren't just

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<v Speaker 2>looking for wiggly lines on a map.

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<v Speaker 3>That's right. A watershed is a holistic unit. It's not

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<v Speaker 3>just a single channel. So they listed four key components

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<v Speaker 3>they needed to successfully map and link across these vast

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<v Speaker 3>areas to declare a system organized.

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<v Speaker 2>And you know, major, what were those four defining components?

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<v Speaker 3>Okay, so first the river systems themselves, that's the main channels,

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<v Speaker 3>the smaller tributaries flowing into them, that whole dendritic network

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<v Speaker 3>structure we talked.

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<v Speaker 2>About the branches of the tree right.

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<v Speaker 3>Second, the water deposit systems. These are the region often

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<v Speaker 3>big sedimentary planes where the water lost its speed and

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<v Speaker 3>started to deposit its carried load of sediment.

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<v Speaker 2>So the source in the sink the beginning and the

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<v Speaker 2>end of the line exactly.

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<v Speaker 3>Third, the outlet canyons. These were often dramatic, high energy

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<v Speaker 3>exit points where massive volumes of water estaped a basin,

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<v Speaker 3>potentially flowing out to the vast north than lowlands of Mars.

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<v Speaker 3>And the fourth piece and fourth the lakes and valley networks.

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<v Speaker 3>These represent the temporary or in some cases long term

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<v Speaker 3>reservoirs where water accumulated before either evaporating or flowing out

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<v Speaker 3>through one of those outlet canyons.

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<v Speaker 2>It's just fascinating that they needed to find all four

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<v Speaker 2>of those elements connected together. That really demonstrates an integrated structure.

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<v Speaker 2>It does by linking all those arteries and veins together

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<v Speaker 2>across these huge areas, they essentially move the needle from okay,

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<v Speaker 2>Mars had water to Mars had a functioning planetary scale hydrological.

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<v Speaker 3>Cycle, and it confirms a period of Martian history where

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<v Speaker 3>precipitation and surface conditions were just fundamentally different. To sustain

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<v Speaker 3>sixteen of these massive systems requires more than just occasional melt.

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<v Speaker 3>It requires a warm enough surface and a dense enough

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<v Speaker 3>atmosphere for water to flow, collect and erode across enormous distances.

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<v Speaker 3>It confirms a vast, ancient and very active history for

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<v Speaker 3>the planet.

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<v Speaker 2>Now we get to a part of this that I

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<v Speaker 2>find truly intriguing. Here's where it gets really technical and

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<v Speaker 2>I think really inspiring. How exactly do scientists map the

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<v Speaker 2>beds and channels of rivers that vanished literally billions of

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<v Speaker 2>years ago, right, rivers that are now potentially buried under

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<v Speaker 2>shifting Martian dust or thick lava fields. Are these massive

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<v Speaker 2>wind blown deposits. We are relying entirely on remote sensing,

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<v Speaker 2>on orbiting instruments for this historical reconstruction, and.

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<v Speaker 3>This specific mapping effort is just a masterclass in combining

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<v Speaker 3>different types of orbital data. It's really clever. To reconstruct

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<v Speaker 3>ancient waterflow. You need two crucial, high precision pieces of information.

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<v Speaker 3>You need to know where the ground is so extreme

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<v Speaker 3>precision on altitude topography, the topography exactly, and you need

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<v Speaker 3>a high resolution visual proof of what is actually on

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<v Speaker 3>the surface.

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<v Speaker 2>Okay, let's start with that foundational data set. The altitude component.

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<v Speaker 2>The study relies heavily on an instrument called MOLA.

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<v Speaker 3>Yes, the Mars Orbiter Laser e Limiter MLLA was a

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<v Speaker 3>primary instrument on board NASA is Mars Global Surveyor, which

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<v Speaker 3>operated successfully from nineteen ninety seven all the way to

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<v Speaker 3>two thousand and six.

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<v Speaker 2>So this is legacy technology we're talking about.

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<v Speaker 3>It is, and it's a revolutionary piece of legacy technology.

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<v Speaker 3>MLA works by firing a laser pulse down at the

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<v Speaker 3>Martians surface and then timing exactly how long it takes

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<v Speaker 3>for that pulse to bounce back to the spacecraft.

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<v Speaker 2>So it's basically like a super precise tape measure from space.

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<v Speaker 3>That's a great way to put it. By tracking millions

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<v Speaker 3>and millions of these pulses globally, you can calculate the

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<v Speaker 3>distance and map the topography of Mars with extraordinary precision.

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<v Speaker 2>So EMILA provides the bedrock map. It defines the continental divides,

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<v Speaker 2>the lowest points, the high points. Crucially, it tells us

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<v Speaker 2>which way water would have flowed just based on.

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<v Speaker 3>Gravity exactly right. You simply cannot define a watershed without

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<v Speaker 3>incredibly detailed altitude data. The sheer precision of MLA, which

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<v Speaker 3>is often capable of measuring altitude differences down to the

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<v Speaker 3>meter or even submeter scale.

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<v Speaker 2>That's incredible, it is.

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<v Speaker 3>And that's what allowed the scientists to mathematically model the subtle,

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<v Speaker 3>faint gradients of a four billion year old riverbed that

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<v Speaker 3>might have been partially eroded or buried. It defines the

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<v Speaker 3>pass of least resistance for every theoretical drop of water

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<v Speaker 3>across the entire Martian surface.

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<v Speaker 2>So MLA provides the mathematical framework for the flow paths.

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<v Speaker 2>But altitude data alone doesn't prove that a river was

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<v Speaker 2>actually there right, or that the feature wasn't carved by

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<v Speaker 2>something else like lava, an excellent point. You need the

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<v Speaker 2>visual confirmation, the proof that the flow was indeed fluvial

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<v Speaker 2>water based, and that's where the CTX, the context camera

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<v Speaker 2>comes in.

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<v Speaker 3>Yes, the Context Camera is currently orbiting Mars on board

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<v Speaker 3>the Mars Reconnaissance.

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<v Speaker 2>Orbiter or MRO, which is still active.

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<v Speaker 3>Still very active, and CTX is critical because of its scale. Now,

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<v Speaker 3>there are other cameras on MRO that take higher resolution snapshots,

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<v Speaker 3>like the famous high Rise camera, but ctx's distinction is

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<v Speaker 3>its sheer volume of data and its medium resolution coverage.

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<v Speaker 3>It has achieved nearly complete coverage of the entire red planet.

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<v Speaker 2>So MLA tells you where to look for a drop

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<v Speaker 2>in elevation, and CTX provides the high resolution imagery you

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<v Speaker 2>need to actually identify the erosional features along.

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<v Speaker 3>That path precisely. CTX confirms the geological reality. It allows

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<v Speaker 3>researchers to identify the detailed structures. You can see the

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<v Speaker 3>actual river bends, the meanders, You can see layered sedimentary

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<v Speaker 3>deposits on the valley floors. You can see those subtle

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<v Speaker 3>dendritic or treelike branching patterns of the valley networks that

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<v Speaker 3>are so characteristic of organized water erosion.

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<v Speaker 2>The combination is just so powerful.

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<v Speaker 3>It really is. You use EMLA to trace the flow direction,

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<v Speaker 3>and then you zoom in with CTX to confirm that

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<v Speaker 3>the features along that path are indeed ancient river channels.

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<v Speaker 2>And the beauty of it, as you said, is that

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<v Speaker 2>this study synthesizes data separated by decades. It really proves

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<v Speaker 2>the continuing value of NASA's long term investments in these missions.

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<v Speaker 3>Absolutely, the data from MARS Global Surveyor is still generating

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<v Speaker 3>groundbreaking science today.

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<v Speaker 2>But how do you actually reconcile and overlay these massive,

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<v Speaker 2>complex data sets. This is where the specifics software comes in.

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<v Speaker 2>The source mentions. They used RGIS pro, and.

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<v Speaker 3>This is an important detail for you the listener to note.

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<v Speaker 3>RGIS pro is a commercial industry standard geographic information system

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<v Speaker 3>a GIS. It's used by cartographers, city planners, geologists all

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<v Speaker 3>over the world for Earth.

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<v Speaker 2>So it's off the show software it is.

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<v Speaker 3>And the fact that planetary scientists use this same software

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<v Speaker 3>underscores the universality of their methods. They're using the same

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<v Speaker 3>tools to map mars that someone might use to map

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<v Speaker 3>a new highway system in Ohio.

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<v Speaker 2>So how does that software bridge the gap BETWEENMAS data

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<v Speaker 2>and ctx's images.

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<v Speaker 3>It allows for seamless data layer integration in a GIS.

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<v Speaker 3>You can treat MLA's topography data as one massive layer

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<v Speaker 3>that's your elevation map. Then you can overlay ctx's visual

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<v Speaker 3>imagery as a second layer right on.

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<v Speaker 2>Top of it, and you can add more layers. Isome?

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<v Speaker 3>Oh yeah, you could add a third layer for mineral mapping,

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00:14:51.799 --> 00:14:54.080
<v Speaker 3>which we'll get to later, a fourth layer defining those

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<v Speaker 3>hundred and five square kilometer catchment boundaries. And rgis pro

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<v Speaker 3>allows researchers to define perarameters. You can tell it show

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<v Speaker 3>me all the features from the CTX images that exhibit

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<v Speaker 3>dendritic patterns A and D whose lowest point connects to

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<v Speaker 3>the mathematically predicted flow path we derived from the MLLA data.

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<v Speaker 2>So it automates the search in a way.

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<v Speaker 3>It makes the search systematic, objective and reproducible. It moves

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<v Speaker 3>planetary geology into this new era of verifiable cartography using

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<v Speaker 3>the exact same tools we use to manage resources right

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<v Speaker 3>here on Earth.

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<v Speaker 2>And this systematic, rigorous mapping methodology is what gives these

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00:15:30.480 --> 00:15:33.919
<v Speaker 2>hard numbers their weight, their authority. So let's shift our

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00:15:33.919 --> 00:15:37.600
<v Speaker 2>focus now entirely to the tangible results, the specific measurements,

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00:15:37.639 --> 00:15:40.000
<v Speaker 2>and the sheer impact of these ancient river systems on

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<v Speaker 2>the Martian surface.

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<v Speaker 3>Okay, the findings derived from this MLACTX fusion are remarkably clear.

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<v Speaker 3>The researchers successfully mapped sixteen highly organized drainage systems that

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00:15:52.039 --> 00:15:55.679
<v Speaker 3>exceeded that one hundred and five square kilometer baseline, fifteen

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<v Speaker 3>of them sixteen. And these are not just suggestions of waterways.

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<v Speaker 3>They are now the ignore the knowledge major integrated continental

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<v Speaker 3>scale hydrological features of ancient Mars.

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<v Speaker 2>And once again that sediment volume twenty eight thousand cubic

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<v Speaker 2>kilometers in material I've spent some more time on this number,

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<v Speaker 2>because it really is the core measure of the water's power.

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<v Speaker 2>Can we try and quantify that volume with some more

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00:16:18.559 --> 00:16:20.039
<v Speaker 2>vivid earth based analogies.

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00:16:20.080 --> 00:16:21.840
<v Speaker 3>We have to, it's the only way to grasp it.

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00:16:21.919 --> 00:16:25.080
<v Speaker 3>The sheer volume moved by just these sixteen systems, it's

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00:16:25.480 --> 00:16:28.120
<v Speaker 3>comparable to the mass of a small terrestrial mountain range.

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<v Speaker 3>Instead of being lifted up, it was transported across the surface. Wow,

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00:16:32.200 --> 00:16:33.799
<v Speaker 3>here's another way to think about it. If you took

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<v Speaker 3>all the water in Lake Superior, which is the largest

323
00:16:36.080 --> 00:16:38.879
<v Speaker 3>of the Great Lakes by volume, the sediment moved by

324
00:16:38.919 --> 00:16:42.399
<v Speaker 3>these Martian systems is equivalent to filling Lake Superior approximately

325
00:16:42.440 --> 00:16:44.360
<v Speaker 3>three times over with pack dirt and rock.

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<v Speaker 2>Three Lake Superiors worth of dirt just moved by water.

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<v Speaker 3>That is a stunning measure of the erosional work done

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<v Speaker 3>by Martian water during its wet periods.

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<v Speaker 2>That is a staggering amount of material to move. It's

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<v Speaker 2>so hard to imagine that level of fluvial erosion on

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<v Speaker 2>a planet we think of is static and frozen. It is,

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00:17:02.559 --> 00:17:05.400
<v Speaker 2>but the context becomes even sharper when we look at

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<v Speaker 2>the relative contribution of these sixteen systems to the total planetary.

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<v Speaker 3>History, which brings us to the forty two percent figure.

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<v Speaker 2>Right.

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00:17:13.119 --> 00:17:16.640
<v Speaker 3>The study concluded that these sixteen map systems comprise approximately

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00:17:16.680 --> 00:17:19.680
<v Speaker 3>forty two percent of the total flowing sediment volume across

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00:17:19.720 --> 00:17:22.279
<v Speaker 3>all of ancient Mars, and this is arguably the most

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00:17:22.279 --> 00:17:24.960
<v Speaker 3>crucial takeaway regarding the nature of Martian hydrology.

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<v Speaker 2>Okay, let's stop there and really analyze that forty two percent.

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<v Speaker 2>If Mars had potentially thousands of smaller, unorganized streams, creeks,

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<v Speaker 2>and flash flood events, which we know it did, how

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<v Speaker 2>can just sixteen large systems account for nearly half of

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<v Speaker 2>the planet's total fluvial work.

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<v Speaker 3>It speaks directly to the efficiency and the duration of

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<v Speaker 3>the flow.

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<v Speaker 2>In those systems.

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<v Speaker 3>The power was concentrated, highly concentrated. Think about it, sixteen

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<v Speaker 3>systems doing almost half the work. That means these specific

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<v Speaker 3>systems were disproportionately powerful. They had to have operated consistently,

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<v Speaker 3>efficiently and for a very very long time. It's strongly

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<v Speaker 3>suggests that while episodic water events might have initiated some

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<v Speaker 3>erosion here and there, the bulk of the planet's surface

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<v Speaker 3>sculpting was done by these massive integrated drainage systems.

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00:18:09.920 --> 00:18:12.440
<v Speaker 2>And those systems would require a stable climate.

356
00:18:12.119 --> 00:18:15.920
<v Speaker 3>Regime, a sustained water cycle, perhaps involving rain or snow,

357
00:18:16.119 --> 00:18:19.359
<v Speaker 3>something to keep them flowing for potentially millions of years.

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<v Speaker 2>So instead of a picture where water was just kind

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<v Speaker 2>of everywhere, carding millions of small gullies, the picture shifts.

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00:18:24.400 --> 00:18:27.279
<v Speaker 2>He becomes one where water was highly concentrated in a

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<v Speaker 2>few dominant continental basins that really dictated the planet's geological evolution.

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<v Speaker 3>Precisely, if on Earth forty two percent of all the

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<v Speaker 3>fluvial work were done by only sixteen rivers you know,

364
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<v Speaker 3>the Amazon, the Nile, the Mississippi, and a few others,

365
00:18:42.680 --> 00:18:46.839
<v Speaker 3>that would imply a global uniformity in topography and precipitation

366
00:18:47.039 --> 00:18:49.759
<v Speaker 3>that we just don't see. The fact that the Martian

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00:18:49.759 --> 00:18:53.200
<v Speaker 3>system is so concentrated suggests one of two things. Either

368
00:18:53.279 --> 00:18:56.680
<v Speaker 3>Martian topography was incredibly efficient at funneling precipitation into a

369
00:18:56.680 --> 00:19:00.319
<v Speaker 3>small number of giant basins, or the global climate was

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00:19:00.359 --> 00:19:04.519
<v Speaker 3>remarkably stable, allowing only the largest systems to operate long

371
00:19:04.640 --> 00:19:07.160
<v Speaker 3>enough to accumulate that massive sediment volume.

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00:19:07.480 --> 00:19:10.519
<v Speaker 2>That concentration of power is immense, and it must offer

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<v Speaker 2>important constraints for climate modelers, For the people trying to

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<v Speaker 2>recreate what the ancient Martian atmosphere must have been like

375
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<v Speaker 2>to sustain these giants.

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00:19:17.519 --> 00:19:19.480
<v Speaker 3>Absolutely, it narrows the possibilities.

377
00:19:19.599 --> 00:19:21.839
<v Speaker 2>The study also had a specific finding about the role

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00:19:21.880 --> 00:19:24.960
<v Speaker 2>of the outlet canyons, those dramatic exit points of these systems.

379
00:19:25.079 --> 00:19:28.000
<v Speaker 3>Yes, they quantified the impact of these high energy features,

380
00:19:28.079 --> 00:19:30.400
<v Speaker 3>and they discovered that the outlet canyons, the points where

381
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<v Speaker 3>large bodies of water like lakes breached or overflowed, contributed

382
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<v Speaker 3>approximately twenty four percent of the global river sediment amount

383
00:19:37.720 --> 00:19:38.440
<v Speaker 3>on ancient Mars.

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00:19:38.519 --> 00:19:41.200
<v Speaker 2>Okay, let's put this two numbers together. We have forty

385
00:19:41.240 --> 00:19:44.680
<v Speaker 2>two percent from the sustained large scale river flow within

386
00:19:44.720 --> 00:19:48.400
<v Speaker 2>the basins and twenty four percent from just the outlet canyons. Right,

387
00:19:48.599 --> 00:19:53.240
<v Speaker 2>that twenty four percent implies massive focus potentially catastrophic flows

388
00:19:53.480 --> 00:19:56.599
<v Speaker 2>where the water exited the basin. How do we reconcile

389
00:19:56.640 --> 00:19:59.400
<v Speaker 2>those two things? Does this mean Mars was both sustained

390
00:19:59.440 --> 00:20:00.519
<v Speaker 2>and catastrop I.

391
00:20:00.559 --> 00:20:03.160
<v Speaker 3>Think it paints a very dynamic picture. The forty two

392
00:20:03.160 --> 00:20:07.359
<v Speaker 3>percent confirms the consistency the long, slow work of erosion

393
00:20:07.400 --> 00:20:10.480
<v Speaker 3>and transport inside the basin, But the twenty four percent

394
00:20:10.519 --> 00:20:13.400
<v Speaker 3>from the canyon suggests that these basins, which likely held

395
00:20:13.519 --> 00:20:19.160
<v Speaker 3>massive lakes, occasionally breached or overflowed in huge, violent volumes.

396
00:20:18.720 --> 00:20:20.720
<v Speaker 2>So the system would fill up slowly over time.

397
00:20:20.960 --> 00:20:24.480
<v Speaker 3>Exactly, it implies that the water flowed consistently filling up giant,

398
00:20:24.599 --> 00:20:27.839
<v Speaker 3>long lived lakes, which then sometimes reached a catastrophic tipping

399
00:20:27.839 --> 00:20:31.680
<v Speaker 3>point of discharge. These canyon exits acted as high speed funnels,

400
00:20:31.799 --> 00:20:34.920
<v Speaker 3>transporting massive amounts of material from the interior basins down

401
00:20:34.920 --> 00:20:38.119
<v Speaker 3>to the northern lowlands, and that likely contributed to the

402
00:20:38.119 --> 00:20:41.000
<v Speaker 3>formation of whatever ancient oceans or major bodies of water

403
00:20:41.079 --> 00:20:42.079
<v Speaker 3>may have existed there.

404
00:20:42.240 --> 00:20:46.799
<v Speaker 2>So slow accumulation punctuated by high speed discharge it suggests

405
00:20:46.839 --> 00:20:49.559
<v Speaker 2>the Martian water cycle wasn't just stable, it was also

406
00:20:49.720 --> 00:20:53.920
<v Speaker 2>capable of producing these immense, focused floods at the termination

407
00:20:54.079 --> 00:20:55.720
<v Speaker 2>points of these megasystems.

408
00:20:55.839 --> 00:20:58.279
<v Speaker 3>It makes a lot of sense. Imagine a massive reservoir

409
00:20:58.359 --> 00:21:01.880
<v Speaker 3>filling slowly over a thousand and years, then suddenly breaching

410
00:21:01.880 --> 00:21:05.119
<v Speaker 3>a natural dam. The consistent work of filling it is

411
00:21:05.160 --> 00:21:08.400
<v Speaker 3>the forty two percent. The dramatic breach is the twenty

412
00:21:08.440 --> 00:21:09.039
<v Speaker 3>four percent.

413
00:21:09.240 --> 00:21:12.759
<v Speaker 2>It confirms a truly powerful and very active hydrological cycle

414
00:21:12.839 --> 00:21:16.200
<v Speaker 2>operating in an immense scale. Before we move on to

415
00:21:16.240 --> 00:21:18.640
<v Speaker 2>the great mystery of where it all went, Let's ground

416
00:21:18.680 --> 00:21:21.720
<v Speaker 2>this new cartography in the context of the overwhelming evidence

417
00:21:21.920 --> 00:21:25.519
<v Speaker 2>that already confirmed ancient liquid water dominated the Martian surface.

418
00:21:25.640 --> 00:21:27.799
<v Speaker 2>That's right. This mapping is new in its scope, but

419
00:21:27.880 --> 00:21:31.480
<v Speaker 2>it really builds on decades of geological and mineralogical proof.

420
00:21:31.559 --> 00:21:35.079
<v Speaker 3>That's the key point. This study confirms the system was integrated,

421
00:21:35.240 --> 00:21:37.519
<v Speaker 3>but the physical proof of water has been piling up

422
00:21:37.559 --> 00:21:39.720
<v Speaker 3>since the Viking missions in the seventies, and it just

423
00:21:39.960 --> 00:21:42.000
<v Speaker 3>escalated exponentially with the rovers.

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00:21:42.119 --> 00:21:44.359
<v Speaker 2>And that proof comes in two main forms, right, the

425
00:21:44.359 --> 00:21:47.880
<v Speaker 2>shapes on the surface and the chemical residue less behind.

426
00:21:47.759 --> 00:21:50.880
<v Speaker 3>The geomorphology and the mineralogy exactly.

427
00:21:51.079 --> 00:21:55.599
<v Speaker 2>Let's start with the geomorphological landforms, the geological evidence of

428
00:21:55.640 --> 00:22:00.000
<v Speaker 2>liquid movement. Besides these drainage systems, what are the class

429
00:22:00.480 --> 00:22:03.400
<v Speaker 2>undeniable signs of past water that we see from orbit?

430
00:22:04.039 --> 00:22:07.759
<v Speaker 3>Well, we see clear evidence of deltas. The most famous

431
00:22:07.839 --> 00:22:11.240
<v Speaker 3>right now is the incredibly well preserved delta structure in

432
00:22:11.319 --> 00:22:14.440
<v Speaker 3>Jesero Crater, which is exactly why the Perseverance rover is

433
00:22:14.480 --> 00:22:18.200
<v Speaker 3>operating there. Delta's only form when a flowing river slows

434
00:22:18.240 --> 00:22:21.319
<v Speaker 3>down rapidly and dumps its sediment load as it enters

435
00:22:21.359 --> 00:22:24.400
<v Speaker 3>a large standing body of water. That means there had

436
00:22:24.440 --> 00:22:26.599
<v Speaker 3>to have been a long lived lake or even a

437
00:22:26.680 --> 00:22:27.720
<v Speaker 3>sea in that crater.

438
00:22:27.880 --> 00:22:28.279
<v Speaker 2>What else?

439
00:22:28.440 --> 00:22:31.839
<v Speaker 3>We also see massive outflow channels. These are immense scars

440
00:22:31.839 --> 00:22:34.880
<v Speaker 3>on the surface, sometimes hundreds of kilometers wide. They're often

441
00:22:34.920 --> 00:22:38.640
<v Speaker 3>associated with catastrophic flood events, likely from the rapid release

442
00:22:38.680 --> 00:22:40.480
<v Speaker 3>of pressurized underground reservoirs.

443
00:22:40.519 --> 00:22:43.359
<v Speaker 2>And on a smaller scale, we see smaller features too,

444
00:22:43.400 --> 00:22:44.480
<v Speaker 2>don't we Oh.

445
00:22:44.400 --> 00:22:48.440
<v Speaker 3>Yes, thousands of small scale features like gullies. You often

446
00:22:48.480 --> 00:22:51.119
<v Speaker 3>find these on crater walls, and they may represent more

447
00:22:51.160 --> 00:22:54.799
<v Speaker 3>recent seasonal flows or maybe just near surface ice melting.

448
00:22:55.279 --> 00:22:59.319
<v Speaker 3>And maybe most evocative for suggesting large standing bodies of water,

449
00:22:59.599 --> 00:23:04.119
<v Speaker 3>we see evidence of coastal light terraces. These are horizontal markings,

450
00:23:04.200 --> 00:23:08.279
<v Speaker 3>almost like steps in the landscape, suggesting ancient shorelines where

451
00:23:08.319 --> 00:23:11.440
<v Speaker 3>water stood still at a consistent level for extended periods,

452
00:23:11.880 --> 00:23:14.880
<v Speaker 3>perhaps defining the boundaries of an ancient northern ocean.

453
00:23:15.160 --> 00:23:18.279
<v Speaker 2>So those landforms tell a story of movement, stillness, and

454
00:23:18.359 --> 00:23:21.960
<v Speaker 2>massive flooding. But the most undeniable proof I find comes

455
00:23:21.960 --> 00:23:25.640
<v Speaker 2>from the chemical signatures. The mineralogical evidence that only forms

456
00:23:25.680 --> 00:23:27.000
<v Speaker 2>in the presence of liquid water.

457
00:23:27.359 --> 00:23:30.319
<v Speaker 3>The minerals are the chemical fingerprints of the water's composition

458
00:23:30.400 --> 00:23:33.680
<v Speaker 3>in its history. They are the archives of that wet phase.

459
00:23:33.599 --> 00:23:36.480
<v Speaker 2>And we found several key types identified by orbiters and

460
00:23:36.480 --> 00:23:38.119
<v Speaker 2>then confirmed on the ground by rovers.

461
00:23:38.519 --> 00:23:43.559
<v Speaker 3>We have first clays, or what geologists call phyllosilicates. These

462
00:23:43.640 --> 00:23:48.200
<v Speaker 3>form when water interacts chemically with volcanic rock over prolonged periods.

463
00:23:48.680 --> 00:23:52.200
<v Speaker 3>The very fact that they exist suggests relatively neutral or

464
00:23:52.319 --> 00:23:56.359
<v Speaker 3>alkaline water conditions, which is potentially favorable for life.

465
00:23:56.440 --> 00:23:59.200
<v Speaker 2>But Mars clearly changed because we also found minerals that

466
00:23:59.240 --> 00:24:01.480
<v Speaker 2>suggest a highly acidic environment later on.

467
00:24:01.680 --> 00:24:05.920
<v Speaker 3>That's right. We find vast deposits of sulfate minerals and carbonates.

468
00:24:06.240 --> 00:24:09.519
<v Speaker 3>Sulfates in particular often precipitate out when water is acidic

469
00:24:09.559 --> 00:24:10.799
<v Speaker 3>and evaporates rapidly.

470
00:24:10.880 --> 00:24:13.599
<v Speaker 2>So the minerals themselves tell a story of climate change.

471
00:24:13.720 --> 00:24:17.240
<v Speaker 3>They provide a geological timeline. They confirm that the Martian

472
00:24:17.279 --> 00:24:20.319
<v Speaker 3>water cycle not only existed, but it also changed chemically

473
00:24:20.400 --> 00:24:23.279
<v Speaker 3>as the planet cooled in its atmosphere thinned. You had

474
00:24:23.319 --> 00:24:27.279
<v Speaker 3>clays forming early in a more benign environment than sulfates

475
00:24:27.279 --> 00:24:28.720
<v Speaker 3>forming later in a harsher one.

476
00:24:28.799 --> 00:24:31.119
<v Speaker 2>And of course, you can't talk about water evidence without

477
00:24:31.160 --> 00:24:34.599
<v Speaker 2>mentioning the tiny infamous hematite.

478
00:24:34.039 --> 00:24:37.079
<v Speaker 3>Blueberries, the favorite piece of evidence for so many people,

479
00:24:37.519 --> 00:24:42.079
<v Speaker 3>these small spherical concretions of iron oxide. They were famously

480
00:24:42.119 --> 00:24:44.960
<v Speaker 3>discovered by the NASA Opportunity Rover way back in two

481
00:24:45.000 --> 00:24:49.039
<v Speaker 3>thousand and four, just scattered all over MERIDIANI planum.

482
00:24:48.559 --> 00:24:50.079
<v Speaker 2>And they could only have formed in water.

483
00:24:50.440 --> 00:24:54.759
<v Speaker 3>Hematite strongly indicates formation in the presence of water, likely

484
00:24:54.759 --> 00:24:58.440
<v Speaker 3>as minerals precipitated out of a flowing, slightly acidic solution.

485
00:24:59.000 --> 00:25:03.200
<v Speaker 3>They are the perfect small scale, undeniable proof of prolonged

486
00:25:03.200 --> 00:25:04.920
<v Speaker 3>agueous activity on the surface.

487
00:25:05.160 --> 00:25:08.000
<v Speaker 2>So okay, we have the geomorphological structures, we have the

488
00:25:08.039 --> 00:25:10.599
<v Speaker 2>chemical signatures, and now we have the global map of

489
00:25:10.640 --> 00:25:14.359
<v Speaker 2>sixteen giant river systems. This whole body of evidence leads

490
00:25:14.440 --> 00:25:17.160
<v Speaker 2>us to the crucial timeline debate. When did all this

491
00:25:17.240 --> 00:25:19.359
<v Speaker 2>incredible activity happen and for how.

492
00:25:19.240 --> 00:25:22.079
<v Speaker 3>Long Mars formed with the rest of the Solar system

493
00:25:22.240 --> 00:25:25.559
<v Speaker 3>roughly four point five billion years ago. The generally accepted

494
00:25:25.599 --> 00:25:28.920
<v Speaker 3>wet period, what we call the noation period, occurred relatively

495
00:25:28.960 --> 00:25:32.000
<v Speaker 3>early within the first billion years or so, but the specifics,

496
00:25:32.359 --> 00:25:35.079
<v Speaker 3>especially as the stain that wet period was. That's still

497
00:25:35.119 --> 00:25:36.160
<v Speaker 3>intensely debated.

498
00:25:36.319 --> 00:25:38.400
<v Speaker 2>Let's elaborate on those two main schools of thought.

499
00:25:38.680 --> 00:25:40.880
<v Speaker 3>So on one side you have scientists who argue for

500
00:25:40.920 --> 00:25:45.279
<v Speaker 3>episodic periods of water. This model suggests that while water existed,

501
00:25:45.519 --> 00:25:48.519
<v Speaker 3>warm and wet conditions were transient, they were a flash

502
00:25:48.559 --> 00:25:48.960
<v Speaker 3>in the pan.

503
00:25:49.200 --> 00:25:52.640
<v Speaker 2>So a frozen Mars with brief thows exactly.

504
00:25:53.039 --> 00:25:58.119
<v Speaker 3>Perhaps massive impact events or intense volcanic eruptions released enormous

505
00:25:58.160 --> 00:26:02.400
<v Speaker 3>amounts of greenhouse gases which temporarily warmed and thawed the surface.

506
00:26:02.759 --> 00:26:06.039
<v Speaker 3>That would allow water to flow violently for maybe hundreds

507
00:26:06.119 --> 00:26:09.240
<v Speaker 3>or thousands of years before the planet froze again into

508
00:26:09.319 --> 00:26:10.799
<v Speaker 3>its default cold state.

509
00:26:11.200 --> 00:26:13.839
<v Speaker 2>And the other site argues for a more sustained period.

510
00:26:14.119 --> 00:26:17.480
<v Speaker 3>Yes, the argument for a lone longer period. This suggests

511
00:26:17.519 --> 00:26:20.880
<v Speaker 3>that early Mars maintained a thick enough atmosphere and sufficient heat,

512
00:26:21.079 --> 00:26:24.720
<v Speaker 3>probably via a CO two greenhouse effect, to sustain liquid

513
00:26:24.759 --> 00:26:27.640
<v Speaker 3>water continuously for hundreds of millions of years.

514
00:26:27.799 --> 00:26:31.519
<v Speaker 2>And this new study, with its sixteen large integrated systems

515
00:26:32.119 --> 00:26:35.319
<v Speaker 2>that must lend some serious weight to that longer period model.

516
00:26:35.440 --> 00:26:37.920
<v Speaker 3>It really does. It's hard to imagine carving those massive

517
00:26:37.920 --> 00:26:40.279
<v Speaker 3>systems with just a few thousand years of flow here

518
00:26:40.279 --> 00:26:43.000
<v Speaker 3>and there. It requires immense cumulative flow time.

519
00:26:43.319 --> 00:26:46.680
<v Speaker 2>And the most recent data on this really pushes that timeline.

520
00:26:46.720 --> 00:26:48.519
<v Speaker 2>I mean, it pushes it far into the planet's history,

521
00:26:48.519 --> 00:26:48.920
<v Speaker 2>doesn't it.

522
00:26:48.799 --> 00:26:51.519
<v Speaker 3>It does. The source mentions a twenty twenty two study

523
00:26:51.720 --> 00:26:55.079
<v Speaker 3>that estimated Mars had liquid water as recently as two

524
00:26:55.319 --> 00:26:56.319
<v Speaker 3>billion years ago.

525
00:26:56.440 --> 00:26:59.440
<v Speaker 2>Two billion. That's more than halfway through the planet's history.

526
00:26:59.519 --> 00:27:02.680
<v Speaker 3>It is a dunning longevity. If that timeline holds true,

527
00:27:02.759 --> 00:27:06.920
<v Speaker 3>it suggests water persisted in significant quantities, perhaps protected in

528
00:27:07.000 --> 00:27:10.839
<v Speaker 3>deep subsurface reservoirs or under thick ice sheets at the poles,

529
00:27:10.960 --> 00:27:14.160
<v Speaker 3>far far longer than the original models predicted, and that

530
00:27:14.240 --> 00:27:17.359
<v Speaker 3>dramatically changes the window in which life could potentially have

531
00:27:17.440 --> 00:27:18.400
<v Speaker 3>existed on Mars.

532
00:27:18.480 --> 00:27:21.720
<v Speaker 2>The narrative of ancient Mars has just completely shifted from

533
00:27:21.799 --> 00:27:25.640
<v Speaker 2>a dry, dead desert to a dynamic world of roaring

534
00:27:25.720 --> 00:27:28.799
<v Speaker 2>rivers and massive lakes. We know the environment was capable

535
00:27:28.799 --> 00:27:32.279
<v Speaker 2>of supporting these sixteen megasystems that move twenty eight thousand

536
00:27:32.319 --> 00:27:35.119
<v Speaker 2>cubic kilometers of sediment. It's a different planet. It's a

537
00:27:35.119 --> 00:27:39.039
<v Speaker 2>completely different planet. So given this immense proof, the question

538
00:27:39.160 --> 00:27:42.680
<v Speaker 2>remains the ultimate planetary murder mystery. Why did the water

539
00:27:42.720 --> 00:27:44.680
<v Speaker 2>all go away? And why so completely?

540
00:27:44.880 --> 00:27:47.680
<v Speaker 3>It's not one single event. It was almost certainly a

541
00:27:47.720 --> 00:27:52.519
<v Speaker 3>cascade of failures. There are likely three interacting mechanisms that

542
00:27:52.599 --> 00:27:55.519
<v Speaker 3>led to the collapse of the Martian hydrosphere, and we

543
00:27:55.680 --> 00:27:59.960
<v Speaker 3>really need to examine each leading scientific hypothesis. Recognizing them,

544
00:28:00.079 --> 00:28:01.599
<v Speaker 3>they probably reinforced each other.

545
00:28:01.680 --> 00:28:04.160
<v Speaker 2>Okay, let's start with the big one, the one that

546
00:28:04.200 --> 00:28:08.400
<v Speaker 2>dictates the fate of the entire planet. Hypothesis one the

547
00:28:08.400 --> 00:28:11.240
<v Speaker 2>loss of the magnetic field and atmospheric stripping.

548
00:28:11.599 --> 00:28:14.720
<v Speaker 3>This is the fundamental difference between Mores and Earth. For

549
00:28:14.759 --> 00:28:17.400
<v Speaker 3>a planet to retain a thick atmosphere and liquid water,

550
00:28:17.720 --> 00:28:19.799
<v Speaker 3>it has to protect itself from the solar wind.

551
00:28:20.119 --> 00:28:21.000
<v Speaker 2>It needs a shield.

552
00:28:21.200 --> 00:28:23.960
<v Speaker 3>It needs a shield. Earth does this with its global

553
00:28:24.000 --> 00:28:27.200
<v Speaker 3>magnetic field its magnetosphere, which is generated by our churning

554
00:28:27.640 --> 00:28:30.559
<v Speaker 3>molten core, are planetary dynamo.

555
00:28:30.279 --> 00:28:32.319
<v Speaker 2>And Mars had this protection early in its life.

556
00:28:32.359 --> 00:28:35.279
<v Speaker 3>Correct, it did, but Mars is a much smaller planet,

557
00:28:35.440 --> 00:28:38.240
<v Speaker 3>and because of its size, its molten core cooled far

558
00:28:38.359 --> 00:28:41.319
<v Speaker 3>sooner and much more rapidly than Earth's did. As that

559
00:28:41.400 --> 00:28:45.319
<v Speaker 3>core solidified, the planetary dynamo shut down, and that led

560
00:28:45.359 --> 00:28:48.799
<v Speaker 3>to the slow dissipation of the protective magnetic field, probably

561
00:28:48.880 --> 00:28:50.599
<v Speaker 3>starting around four billion years ago.

562
00:28:50.839 --> 00:28:53.960
<v Speaker 2>So what happens when that planetary shield is removed? When

563
00:28:53.960 --> 00:28:54.640
<v Speaker 2>you turn off the.

564
00:28:54.680 --> 00:28:58.519
<v Speaker 3>Umbrella, the planet's upper atmosphere becomes exposed to the relentless

565
00:28:58.559 --> 00:29:03.480
<v Speaker 3>bombardment of intense solar and cosmic radiation, primarily the solar wind,

566
00:29:03.559 --> 00:29:06.359
<v Speaker 3>which is it's a constant stream of charged particles flowing

567
00:29:06.359 --> 00:29:08.720
<v Speaker 3>from the Sun, and it acts like a sand blaster

568
00:29:08.960 --> 00:29:13.119
<v Speaker 3>on a molecular level. It physically strips away atmosphere gases,

569
00:29:13.200 --> 00:29:18.279
<v Speaker 3>carbon dioxide, nitrogen, and critically water molecules, blasting them off

570
00:29:18.319 --> 00:29:20.440
<v Speaker 3>into space over millions of years.

571
00:29:20.240 --> 00:29:21.880
<v Speaker 2>And we can see this happening even today.

572
00:29:22.039 --> 00:29:26.119
<v Speaker 3>We can current Mars orbiters like NASA's Maven mission, are

573
00:29:26.160 --> 00:29:29.839
<v Speaker 3>designed specifically to study this. They still detect this stripping

574
00:29:29.880 --> 00:29:33.039
<v Speaker 3>process happening today, confirming that a huge amount of Mars's

575
00:29:33.119 --> 00:29:37.119
<v Speaker 3>early water simply escaped to the cosmos molecule by molecule.

576
00:29:37.359 --> 00:29:39.400
<v Speaker 2>So we confirm that a significant amount of water was

577
00:29:39.440 --> 00:29:43.119
<v Speaker 2>lost to space, which thinned the atmosphere dramatically, and that

578
00:29:43.200 --> 00:29:47.160
<v Speaker 2>leads directly to the next consequence hypothesis to climate collapse.

579
00:29:47.440 --> 00:29:50.640
<v Speaker 3>The thinning atmosphere acted as a trigger for a catastrophic

580
00:29:50.680 --> 00:29:55.359
<v Speaker 3>climate shift. Early Mars relied on gases, likely carbon dioxide

581
00:29:55.359 --> 00:29:58.640
<v Speaker 3>and maybe some methane to create a green house effect

582
00:29:58.720 --> 00:30:00.559
<v Speaker 3>that kept the surface warm enough for.

583
00:30:00.559 --> 00:30:02.599
<v Speaker 2>Liquid water the insulation blanket.

584
00:30:02.640 --> 00:30:06.039
<v Speaker 3>That's it exactly. As the magnetic field loss accelerated the

585
00:30:06.079 --> 00:30:09.279
<v Speaker 3>stripping of that atmospheric blanket, the pressure dropped and the

586
00:30:09.279 --> 00:30:10.799
<v Speaker 3>greenhouse effect failed.

587
00:30:10.440 --> 00:30:12.200
<v Speaker 2>So the planet just got colder and colder.

588
00:30:12.279 --> 00:30:15.839
<v Speaker 3>It led to a runaway cooling effect. The atmospheric pressure

589
00:30:15.920 --> 00:30:18.839
<v Speaker 3>dropped below what's called the triple point of water. That's

590
00:30:18.880 --> 00:30:22.440
<v Speaker 3>the specific temperature and pressure where liquid water can remain stable.

591
00:30:23.119 --> 00:30:25.519
<v Speaker 3>Any liquid water that remained on the surface would have

592
00:30:25.559 --> 00:30:28.960
<v Speaker 3>either furzen solid or it would have quickly sublimated.

593
00:30:28.519 --> 00:30:31.759
<v Speaker 2>Meaning it went straight from a solid or liquid into.

594
00:30:31.640 --> 00:30:34.839
<v Speaker 3>A gas, straight to gas unable to pool or flow.

595
00:30:35.400 --> 00:30:37.960
<v Speaker 3>The atmosphere thinned and the planet was locked into a

596
00:30:38.000 --> 00:30:41.680
<v Speaker 3>permanent deep freeze, making it physically impossible for those sixteen

597
00:30:41.720 --> 00:30:43.640
<v Speaker 3>megasystems to flow or persist.

598
00:30:43.839 --> 00:30:46.559
<v Speaker 2>Okay, so these two hypotheses account for the loss of

599
00:30:46.599 --> 00:30:49.839
<v Speaker 2>surface water, but the sources also leave room for a

600
00:30:50.000 --> 00:30:52.680
<v Speaker 2>huge portion of that water to still be around, just

601
00:30:52.759 --> 00:30:57.960
<v Speaker 2>hidden away. Let's discuss hypothesis three, geological burial or the

602
00:30:58.000 --> 00:30:58.839
<v Speaker 2>great hiding place.

603
00:30:59.119 --> 00:31:03.599
<v Speaker 3>This is the domestic counterbalance, and it's a critical consideration

604
00:31:03.720 --> 00:31:07.920
<v Speaker 3>for future exploration. Scientists hypothesize that while a portion of

605
00:31:07.960 --> 00:31:10.319
<v Speaker 3>water was stripped away to space and a portion was

606
00:31:10.359 --> 00:31:14.240
<v Speaker 3>frozen on the surface, a significant reserve potentially billions of

607
00:31:14.279 --> 00:31:18.039
<v Speaker 3>cubic kilometers, migrated underground and it remains there today.

608
00:31:18.400 --> 00:31:21.279
<v Speaker 2>So the water didn't disappear entirely, It just changed its

609
00:31:21.279 --> 00:31:24.759
<v Speaker 2>state and location. It moved from the riverbeds down into

610
00:31:24.759 --> 00:31:25.319
<v Speaker 2>the bedrock.

611
00:31:25.480 --> 00:31:29.000
<v Speaker 3>Yes, modeling suggests that as the surface cooled and the

612
00:31:29.039 --> 00:31:33.440
<v Speaker 3>atmosphere thinned, vast volumes of surface water sank into the subsurface,

613
00:31:33.519 --> 00:31:37.359
<v Speaker 3>becoming groundwater. And because the Martian surface is now permanently frozen,

614
00:31:37.400 --> 00:31:41.200
<v Speaker 3>there's a massive permafrost layer that extends far underground. This

615
00:31:41.319 --> 00:31:45.759
<v Speaker 3>ancient groundwater became trapped and preserved as subsurface ice. It's

616
00:31:45.799 --> 00:31:48.200
<v Speaker 3>protected from the solar shipping that's happening above.

617
00:31:48.599 --> 00:31:50.839
<v Speaker 2>And this is more than just a theory. It's a

618
00:31:50.880 --> 00:31:54.720
<v Speaker 2>critical target for finding resources. Where are scientists looking for

619
00:31:54.759 --> 00:31:56.000
<v Speaker 2>these buried reservoirs.

620
00:31:56.599 --> 00:32:00.000
<v Speaker 3>The evidence points primarily to two areas. Firstly, the plant

621
00:32:00.000 --> 00:32:02.359
<v Speaker 3>and its poles hold massive ice caps, and we know

622
00:32:02.440 --> 00:32:05.839
<v Speaker 3>from weight measurements that there are huge layers of subsurface

623
00:32:05.880 --> 00:32:07.480
<v Speaker 3>ice extending out from those caps.

624
00:32:07.559 --> 00:32:08.960
<v Speaker 2>Yeah. And the secondary.

625
00:32:08.559 --> 00:32:11.319
<v Speaker 3>Secondly, significant water ice is thought to be locked into

626
00:32:11.319 --> 00:32:14.599
<v Speaker 3>subsurface sheets across the mid latitudes, often just a few

627
00:32:14.640 --> 00:32:18.319
<v Speaker 3>meters below the surface dust, and this provides a direct

628
00:32:18.440 --> 00:32:21.640
<v Speaker 3>tangible link to potential future resource exploration.

629
00:32:21.759 --> 00:32:24.599
<v Speaker 2>It's the whole field of in situ resource utilization.

630
00:32:24.880 --> 00:32:28.000
<v Speaker 3>Exactly. If we ever want to establish a permanent human

631
00:32:28.079 --> 00:32:31.960
<v Speaker 3>presence on Mars, we need water for life support, for

632
00:32:32.039 --> 00:32:36.079
<v Speaker 3>growing food, for producing rocket fuel, and these buried reservoirs,

633
00:32:36.160 --> 00:32:40.119
<v Speaker 3>which were originally fed by those sixteen megasystems, they're our

634
00:32:40.160 --> 00:32:43.440
<v Speaker 3>best hope for finding those resources. The river's vanished, but

635
00:32:43.480 --> 00:32:45.480
<v Speaker 3>the water they carried might just be waiting for us

636
00:32:45.599 --> 00:32:46.559
<v Speaker 3>right below the surface.

637
00:32:46.920 --> 00:32:49.200
<v Speaker 2>It's incredible to think that the same water that curved

638
00:32:49.200 --> 00:32:52.240
<v Speaker 2>those canyons billions of years ago might be the water

639
00:32:52.319 --> 00:32:54.839
<v Speaker 2>we use to sustain human life there in the future.

640
00:32:55.119 --> 00:32:59.079
<v Speaker 3>That is the beautiful continuity of planetary geology, the history

641
00:32:59.119 --> 00:33:01.839
<v Speaker 3>of the planet, because the key to its future the

642
00:33:01.920 --> 00:33:06.680
<v Speaker 3>distribution of that ancient water, now stored underground, directly dictates

643
00:33:06.680 --> 00:33:09.640
<v Speaker 3>where we might land and operate future human missions.

644
00:33:09.839 --> 00:33:12.759
<v Speaker 2>This has been a truly monumental deep dive into ancient

645
00:33:12.759 --> 00:33:16.160
<v Speaker 2>Martian history. We have moved so far past the abstract

646
00:33:16.240 --> 00:33:20.519
<v Speaker 2>question of whether water existed to systematically mapping the organization

647
00:33:20.759 --> 00:33:23.200
<v Speaker 2>and the colossal power of its hydrological past.

648
00:33:23.319 --> 00:33:24.680
<v Speaker 3>It's a huge step.

649
00:33:24.400 --> 00:33:27.519
<v Speaker 2>To recap the incredible scale of the new findings Mars

650
00:33:27.559 --> 00:33:32.160
<v Speaker 2>at organized systematic river systems. We've mapped sixteen major systems

651
00:33:32.160 --> 00:33:36.400
<v Speaker 2>that produced an estimated twenty eight thousand cubic kilometers of sediment.

652
00:33:36.119 --> 00:33:39.240
<v Speaker 3>And that volume at single volume accounts for a staggering

653
00:33:39.279 --> 00:33:41.839
<v Speaker 3>forty two percent of the total fluvial work done on.

654
00:33:41.799 --> 00:33:42.799
<v Speaker 2>The entire planet.

655
00:33:42.880 --> 00:33:45.680
<v Speaker 3>The value of this work is just immense, and this

656
00:33:45.759 --> 00:33:50.079
<v Speaker 3>new methodology the successful combination of legacy topographical data like

657
00:33:50.240 --> 00:33:54.319
<v Speaker 3>MLLA and contemporal high resolution imagery like CTS. Using these

658
00:33:54.319 --> 00:33:57.480
<v Speaker 3>integrated GIS systems, it's a crucial new tool in the

659
00:33:57.519 --> 00:33:59.000
<v Speaker 3>toolbox for planetary science.

660
00:33:59.440 --> 00:34:02.920
<v Speaker 2>Not only four forces us to reconstruct Mars's past as

661
00:34:02.960 --> 00:34:07.160
<v Speaker 2>a radically wetter, more dynamic world, but it also develops new,

662
00:34:07.839 --> 00:34:12.079
<v Speaker 2>universally applicable methods for mapping ancient river basins on other

663
00:34:12.119 --> 00:34:13.559
<v Speaker 2>potentially habitable worlds.

664
00:34:13.840 --> 00:34:16.440
<v Speaker 3>I mean, you could apply this to icy moons in

665
00:34:16.480 --> 00:34:19.480
<v Speaker 3>our Solar system, or even to distant exoplanets one day.

666
00:34:19.559 --> 00:34:22.360
<v Speaker 2>It truly is a powerful picture of a completely different planet,

667
00:34:22.639 --> 00:34:24.280
<v Speaker 2>a world of geological giants.

668
00:34:24.320 --> 00:34:29.000
<v Speaker 3>But as always in science, especially planetary science, every answer

669
00:34:29.199 --> 00:34:30.679
<v Speaker 3>only opens up more questions.

670
00:34:30.760 --> 00:34:33.199
<v Speaker 2>Okay, so think back to the sheer efficiency we discussed.

671
00:34:33.679 --> 00:34:37.400
<v Speaker 2>The researcher successfully mapped sixteen drainage systems that account for

672
00:34:37.400 --> 00:34:40.559
<v Speaker 2>forty two percent of the global flowing sediment volume.

673
00:34:40.679 --> 00:34:42.920
<v Speaker 3>So here's the provocative thought for you to carry forward

674
00:34:42.960 --> 00:34:45.280
<v Speaker 3>from this. What stands out to you about the remaining

675
00:34:45.280 --> 00:34:46.679
<v Speaker 3>fifty eight percent that's.

676
00:34:46.559 --> 00:34:49.960
<v Speaker 2>Right, over half the work is still unaccounted for in

677
00:34:50.000 --> 00:34:53.320
<v Speaker 2>a way, that fifty eight percent of global fluvial work

678
00:34:53.679 --> 00:34:56.440
<v Speaker 2>was done by systems that were either too small and

679
00:34:56.519 --> 00:34:59.280
<v Speaker 2>below that one hundred and five square kilometer baseline, which

680
00:34:59.280 --> 00:35:01.880
<v Speaker 2>would mean they were vastly more numerous but less dominant,

681
00:35:02.119 --> 00:35:05.000
<v Speaker 2>or and this is the really fascinating part, that fifty

682
00:35:05.039 --> 00:35:09.480
<v Speaker 2>eight percent represents systems that are currently buried completely invisible

683
00:35:09.480 --> 00:35:13.079
<v Speaker 2>to our current orbiters, perhaps waiting under centuries of dust

684
00:35:13.199 --> 00:35:14.880
<v Speaker 2>or kilometers of volcanic rock.

685
00:35:15.559 --> 00:35:18.000
<v Speaker 3>This research doesn't close the book on Mars's wet history

686
00:35:18.039 --> 00:35:20.599
<v Speaker 3>at all. It confirms that we have mapped the main highways,

687
00:35:20.760 --> 00:35:25.079
<v Speaker 3>but a much larger, as yet unmapped hydrological history still exists,

688
00:35:25.480 --> 00:35:28.599
<v Speaker 3>potentially including even more ancient or protected futures.

689
00:35:28.639 --> 00:35:31.320
<v Speaker 2>At missing fifty eight percent. That's the true frontier of

690
00:35:31.360 --> 00:35:32.840
<v Speaker 2>Martian discovery.

691
00:35:32.360 --> 00:35:36.320
<v Speaker 3>An organized planetary scale system that produced nearly half the erosion,

692
00:35:36.519 --> 00:35:39.360
<v Speaker 3>and a vast unknown majority that still waits to be mapped.

693
00:35:39.519 --> 00:36:52.639
<v Speaker 3>The deep Dive continues last characters
