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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>We've all seen the pictures from Mars, right, It's incredible rovers, curiosity, perseverance.

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<v Speaker 2>They're just engineering marvels.

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<v Speaker 3>Absolutely peak technology, nuclear powered, incredibly complex systems, some of

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<v Speaker 3>the size of a small car.

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<v Speaker 2>And the science they send back is I mean, it's priceless.

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<v Speaker 2>But there's always that butt, isn't there. The cost is

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<v Speaker 2>enormous billions of dollars.

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<v Speaker 3>That's one side, yeah, billions permission.

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<v Speaker 2>And the other thing is they're slow. They cover ground

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<v Speaker 2>really slowly. We measure their progress in what kilometers per year?

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<v Speaker 3>That's pretty much it. And that's the fundamental trade off

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<v Speaker 3>you make with that kind of traditional exploration. You get

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<v Speaker 3>incredible precision, amazing longevity at one specific spot, but you

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<v Speaker 3>totally sacrifice scale. Our picture of Mars, you know, the geography,

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<v Speaker 3>the climate, It's been shaped for decades by what these

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<v Speaker 3>very expensive wheeled robots can see right where they happen to.

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<v Speaker 2>Be, which leaves a pretty big gap, doesn't it. What

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<v Speaker 2>if you want to understand something huge like planet wide

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<v Speaker 2>climate patterns, or I don't know, track geological futures over

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<v Speaker 2>hundreds thousands of kilometers.

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<v Speaker 3>Exactly, a single rover, however advanced, just crawling along it

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<v Speaker 3>can't give you that big picture, that systemic, distributed view.

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<v Speaker 3>And that's precisely why this other idea, the one we're

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<v Speaker 3>looking at today is well, it's so radical, the tumbleweed

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<v Speaker 3>rover concepts.

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<v Speaker 2>Tumbleweed, Okay, Yeah.

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<v Speaker 3>The idea is basically to ditch all that complex propulsion

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<v Speaker 3>that motors the heavy wheels, the nuclear core, and instead

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<v Speaker 3>use the most abundant resource on Mars.

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<v Speaker 2>Which is the wind. You're talking about these sort of spherical,

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<v Speaker 2>lightweight things just getting blown across the surface like giant

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<v Speaker 2>planetary dandelions.

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<v Speaker 3>That's a pretty good analogy, actually. Yeah, And look, we've

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<v Speaker 3>just gotten some really critical results back from wind tunnel tests,

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<v Speaker 3>field tests. This isn't just some sci fi fantasy anymore.

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<v Speaker 3>It's quickly moving towards being a real possibility for future missions.

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<v Speaker 2>Wow.

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<v Speaker 3>Okay, so the really big question here is, you know,

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<v Speaker 3>how can a massive ball we're talking five meters across

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<v Speaker 3>just push by guts of when become this transformative technology?

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<v Speaker 3>How does that let us explore Mars on a continental scale?

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<v Speaker 2>It sounds more like a giant, very sophisticated beach ball

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<v Speaker 2>than a rover.

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<v Speaker 3>Huh. Well, it might look simple, but the science behind

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<v Speaker 3>making it work is anything. But it seems simple, but

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<v Speaker 3>it's actually more pragmatic and scientifically robust then you might

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<v Speaker 3>think at first glance.

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<v Speaker 2>Okay, let's unpack this then, because yeah, it sounds like

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<v Speaker 2>it relies on radical simplification, but simplicity has to be

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<v Speaker 2>grounded in some pretty solid physics.

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<v Speaker 3>Right, absolutely, Let's start with the machine itself.

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<v Speaker 2>Okay, define this tumble weed rover physically. What are we

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<v Speaker 2>talking about? Size construction?

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<v Speaker 3>Physically? Yeah, they're designed as ultra light weight spheres and

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<v Speaker 3>the scale is well, it's kind of astonishing. Fully deployed, the

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<v Speaker 3>target size is five meters in diameters five.

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<v Speaker 2>Meter Wait a minute, perseverance is about three meters long.

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<v Speaker 2>That's huge, like giraffe height rolling on Mars.

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<v Speaker 3>Pretty much. Think about that visual. The structure itself is

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<v Speaker 3>basically an advanced, very durable shell, maybe like a tough

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<v Speaker 3>balloon made from extremely light but really resilient materials. The

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<v Speaker 3>whole design is about maximizing that surface area while keeping

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<v Speaker 3>the mass incredibly low.

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<v Speaker 2>But why so big? Why five meters wouldn't something smaller

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<v Speaker 2>be I don't know, easier to handle, easier to launch.

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<v Speaker 3>Ah, But the size is actually the secret sauce. It's

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<v Speaker 3>directly linked to the challenge of moving anything in Mars's

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<v Speaker 3>atmosphere because it's so thin exactly compared to Earth, Mars

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<v Speaker 3>has almost no atmosphere, less than one percent of ours

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<v Speaker 3>at the surface. So to actually catch enough wind to move.

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<v Speaker 2>You need a big sale.

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<v Speaker 3>You need a huge surface area for that thin wind

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<v Speaker 3>to push against. Combined with the absolute minimum possible weight,

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<v Speaker 3>A five meters sphere seems to hit that sweet spot

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<v Speaker 3>that optimal ratio of sail area to mass. It gives

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<v Speaker 3>you enough oomph, enough rolling torque from the Martian wind.

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<v Speaker 3>It's all engineered around fluid dynamics in that specific environment.

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<v Speaker 2>Okay, so the entire mobility system is just harnessing Martian wind,

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<v Speaker 2>Like you said, like the tumblewheez we see rolling across

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<v Speaker 2>deserts on Earth as a model, which means you're basically

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<v Speaker 2>swapping out the need for well for power sources, no

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<v Speaker 2>complex motors, no RTGs.

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<v Speaker 3>Precisely, and that leads straight to the core goal, the

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<v Speaker 3>really revolutionary part, large scale and low cost exploration. When

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<v Speaker 3>you use the wind that's already there, you sidestep massive

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<v Speaker 3>engineering headaches. Think about traditional rovers, they often rely on

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<v Speaker 3>those RTGs, radioisotope, thermoelectric generators.

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<v Speaker 2>Some nuclear batteries.

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<v Speaker 3>Yeah, basically nuclear batteries, super high cost, very heavy, politically

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<v Speaker 3>tricky to get approved for launch. By taking RTGs out

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<v Speaker 3>of the equation, along with motors, complex gears, heavy wheels,

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<v Speaker 3>the cost just plummets. The whole platform becomes almost disposable,

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<v Speaker 3>relatively speaking, and that opens the door to mass production.

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<v Speaker 2>And if you cut the cost and complexity that much,

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<v Speaker 2>suddenly you can think about not just sending one precious

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<v Speaker 2>billion dollar machine exactly.

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<v Speaker 3>You can employ the swarm strategy. The goal isn't one rover,

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<v Speaker 3>it's deploying entire swarms of these relatively inexpensive rovers all

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<v Speaker 3>at once.

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<v Speaker 2>Swarm. Okay, now that changes things. What's the scientific advantage

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<v Speaker 2>of having a whole bunch of these rolling around.

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<v Speaker 3>That's where this mission concept really truly shines. The scientific

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<v Speaker 3>payoff of a distributed swarm. You shift from measuring things

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<v Speaker 3>at just one point.

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<v Speaker 2>Like Curiosity does now.

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<v Speaker 3>To systemic distributed sensing. The strategy allows for an unprecedented

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<v Speaker 3>simultaneous view. As the team puts it of atmospheric and

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<v Speaker 3>surface processes from different locations on Mars. We could track

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<v Speaker 3>dynamic things happening across the planet that are basically invisible

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<v Speaker 3>to us right now.

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<v Speaker 2>That distributed sensing, Yeah, I can see how that's a

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<v Speaker 2>game changer, especially for climate science, maybe large scale geology too.

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<v Speaker 2>What kind of questions could you actually answer with, say,

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<v Speaker 2>dozens of these spread across the continent and things we

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<v Speaker 2>just can't tackle.

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<v Speaker 3>Now, Okay, think about planetary climate modeling. Yeah, we know

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<v Speaker 3>Mars has these huge, sometimes planet encircling dust storms, right, Yah,

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<v Speaker 3>the massive ones and powerful atmosphere pressure waves sort of

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<v Speaker 3>like big weather fronts moving cross Earth. With one rover

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<v Speaker 3>like perseverance, you can see a wave pass over you.

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<v Speaker 3>You get a snapshot in time at one place, right,

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<v Speaker 3>But imagine you have fifty tumbleweeds spread out over a

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<v Speaker 3>thousand kilometers. Suddenly you can map the pressure gradients, the

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<v Speaker 3>temperature changes within the wave. Simultaneously, you can track its speed,

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<v Speaker 3>how it evolves in real time across a huge area. Wow,

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<v Speaker 3>that's just impossible. With single point sampling or thing geologically

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<v Speaker 3>could give you statistical data on soil composition or magnetic

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<v Speaker 3>fields over a vast region. You move beyond just finding

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<v Speaker 3>one interesting rock. You start understanding planetary scale trends.

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<v Speaker 2>Okay, so the rolling phase is obviously crucial for spreading

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<v Speaker 2>them out and gathering that kind of data, But you

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<v Speaker 2>mentioned there's more to it. The mission isn't just about rolling, that's.

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<v Speaker 3>Right, and this is where it gets, as you said,

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<v Speaker 3>really interesting. The rolling is the deployment method, getting the

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<v Speaker 3>instruments distributed across strategic target areas. But once they reach

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<v Speaker 3>those spots, maybe preplan zones or areas of interest identified

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<v Speaker 3>during the traverse, they stop rolling. The plan is for

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<v Speaker 3>them to actually collapse into fixed positions. Collapse, Yeah, they

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<v Speaker 3>transform into permanent measurement stations dotted strategically across the Martian surface.

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<v Speaker 2>Hold on, how does a five meter lightweight ball just

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<v Speaker 2>stop and anchor itself? Does the source material give any

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<v Speaker 2>clues about that mechanism, how do you deflate it or

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<v Speaker 2>stick it to.

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<v Speaker 3>The ground that specific mechanism. The how is likely still

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<v Speaker 3>part of the team's ongoing development, probably proprietary at this stage,

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<v Speaker 3>but the core concept involves a controlled deflation or maybe

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<v Speaker 3>retraction of that outer shell. Okay, The key is that

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<v Speaker 3>the interior payload bay, the part with the actual science instruments,

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<v Speaker 3>needs to be secured to the ground somehow. This transition

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<v Speaker 3>from mobile to static is absolutely essential for the long

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<v Speaker 3>term science value.

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<v Speaker 2>So they become little weather stations.

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<v Speaker 3>Or something exactly, or size mix stations, radiation monitors. They

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<v Speaker 3>can provide sustained measurements from fixed points over potentially years,

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<v Speaker 3>tracking atmospheric pressure changes, temperature cycles, maybe detecting marsquakes, monitoring

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<v Speaker 3>radiation levels. Long term, they can form a kind of

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<v Speaker 3>data backbone across the planet.

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<v Speaker 2>Or even communication relays for other future missions.

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<v Speaker 3>That's definitely a potential application. So yeah, the movement phase

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<v Speaker 3>is the deployment strategy getting them spread out. But the

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<v Speaker 3>static phases where you get that really long term scientific

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<v Speaker 3>return on investment.

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<v Speaker 2>Okay, the concept is well, it's brilliant, but the practical

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<v Speaker 2>side still feels daunting. We established Mars's atmosphere is incredibly thin.

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<v Speaker 2>Trying to roll a giant, super lightweight ball in that

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<v Speaker 2>low pressure, even with strong winds. It feels like it

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<v Speaker 2>needed some serious proof.

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<v Speaker 3>Hard evidence, absolutely essential. You can't just assume Earth physics

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<v Speaker 3>scales directly to Mars, especially with atmospheres. The staling factors

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<v Speaker 3>are notoriously tricky. So yes, The source material details two

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<v Speaker 3>main experimental phases that have now provided that crucial proof

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<v Speaker 3>of concept, right the tests.

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<v Speaker 2>Let's start with phase one. That was the wind tunnel

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<v Speaker 2>physics right July twenty twenty five at RHUs University's Planetary

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<v Speaker 2>Environment Facility. They basically had to build a little piece

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<v Speaker 2>of Mars on.

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<v Speaker 3>Earth pretty much. They used scaled down prototypes for this,

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<v Speaker 3>specifically models with diameters of thirty, forty and fifty centimeters.

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<v Speaker 3>They put these inside a special wind tunnel.

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<v Speaker 2>Chamber, and the key was the atmosphere, the absolute key.

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<v Speaker 3>The tests were run under a very low atmosphere and

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<v Speaker 3>pressure seventeen.

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<v Speaker 2>Millibars seventeen okay, remind us Earth's atmosphere at sea level is.

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<v Speaker 3>About one thy thirteen millibars, so seventeen is less than

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<v Speaker 3>two percent of earth pressure. It's practically a near vacuum environment.

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<v Speaker 2>Why is simulating that low pressure so vital and I

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<v Speaker 2>imagine technically quite hard to do.

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<v Speaker 3>It's vital because the way air interacts with the surface,

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<v Speaker 3>the whole fluid dynamics picture changes dramatically at such low pressures.

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<v Speaker 3>Air becomes highly rarefied, how wind actually pushes the sphere,

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<v Speaker 3>how the sphere interacts with the ground through that thin air.

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<v Speaker 3>It's just fundamentally different physics in here. Okay, if the

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<v Speaker 3>rover design can roll efficiently at seventeen millibars, it tells

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<v Speaker 3>you the basic aerodynamic and structural design works for Mars.

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<v Speaker 3>And yeah, maintaining that low pressure while also generating controlled

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<v Speaker 3>wind inside a chamber is definitely a technical challenge.

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<v Speaker 2>Did they just test it on a flat surface?

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<v Speaker 3>No, that was another critical part. They ran tests over

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<v Speaker 3>five different simulated Mars terrains, things like smooth planes, rough

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<v Speaker 3>rocky areas, fine sand surfaces with pebbles, even simulated boulder fields.

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<v Speaker 3>They want to make sure it wasn't just a con

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<v Speaker 3>set that worked on a perfectly smooth lab.

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<v Speaker 2>Floor, right, because Mars isn't smooth, and the goal is

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<v Speaker 2>to find that magic number right, the minimum wind speed

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<v Speaker 2>needed to actually get these things rolling consistently across different terrains.

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<v Speaker 2>What did they find?

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<v Speaker 3>The results were really positive and remarkably consistent across the

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<v Speaker 3>different setups. They found that sustained wind speeds of nine

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<v Speaker 3>to ten meters per second were enough to set the

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<v Speaker 3>models into continuous motion.

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<v Speaker 2>Nine to ten meters per second. Okay, is that fast

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<v Speaker 2>like hurricane speeds.

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<v Speaker 3>Not hurricane No. On Earth, ten meters is about twenty

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<v Speaker 3>two miles per hour, a strong breeze, maybe a moderate gale.

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<v Speaker 3>But remember on Mars the ear is so thin you

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<v Speaker 3>need dead speed to get enough force.

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<v Speaker 2>And that threshold nine ten meters it worked even on

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<v Speaker 2>the rough terrain, the pebbles, the boulders.

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<v Speaker 3>That's what they found. It held true across all those

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<v Speaker 3>Mars like terrains they simulated, which is a huge finding.

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<v Speaker 3>It proves the basic mechanism is robust. It can handle

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<v Speaker 3>different geological settings you'd expect to find on Mars.

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<v Speaker 2>Okay, so it rolls, but that's only part of the puzzle.

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<v Speaker 2>If this thing is tumbling end over end, how does

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<v Speaker 2>the science package inside stay working? Can it even collect

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<v Speaker 2>accurate data while it's bouncing?

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<v Speaker 3>Around, great question, And that was the other major validation

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<v Speaker 3>for the wind tunnel tests. Yeah, they had sensors on

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<v Speaker 3>board the prototypes, and yes, the successfully recorded data even

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<v Speaker 3>during that vigorous tumbling motion. Okay, and maybe even more critically,

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<v Speaker 3>the actual physical behavior of the rover, how it accelerated

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<v Speaker 3>its rolling speed, how it reacted to wind gusts. That

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<v Speaker 3>behavior closely matched the complex computer models, the fluid dynamics

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<v Speaker 3>simulations the team had previously developed.

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<v Speaker 2>Why is matching the models so important? Is it just

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<v Speaker 2>about proving their math was right.

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<v Speaker 3>It's much more profound than just checking the math. It

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<v Speaker 3>validates their ability to reliably predict where these things will go. Ah, Okay,

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<v Speaker 3>think about it. If you're a mission control trying to

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<v Speaker 3>manage a whole swarm of these things being blown around

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<v Speaker 3>by the wind, you can't just rely on luck. You

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<v Speaker 3>need high fidelity predictive.

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<v Speaker 2>Model, right, You need to know roughly where they'll end

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<v Speaker 2>up exactly.

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<v Speaker 3>The our host results basically prove that the physics engine

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<v Speaker 3>they're using to calculate, Okay, if the wind blows this

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<v Speaker 3>way tomorrow, where will tumbleweed number seven likely be? That

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<v Speaker 3>engine is accurate. That's absolutely fundamental for planning emission, for

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<v Speaker 3>coordinating the swarm, for actually achieving the science goals.

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<v Speaker 2>Okay, prediction is key. Now another practical thought. Mars isn't flat.

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<v Speaker 2>It has hills, slopes, crater rims. A strong wind might

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<v Speaker 2>push you up a gentle slope maybe, but what happens

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<v Speaker 2>if the train gets steep? Can a wind blown ball

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<v Speaker 2>actually climb up hill?

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<v Speaker 3>That was a specific thing they tested in our house,

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<v Speaker 3>and the results were pretty impressive. The scaled models showed

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<v Speaker 3>they could climb a slope of eleven point five degrees

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<v Speaker 3>inside that low pressure.

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<v Speaker 2>Chamber eleven and a half degrees.

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<v Speaker 3>Now, because of the differences in gravity between Earth and

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<v Speaker 3>Mars and that low atmospheric density they calculator, they climbing

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<v Speaker 3>eleven point five degrees in the chamber is equivalent to

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<v Speaker 3>climbing roughly a thirty degree slope on the actual surface

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<v Speaker 3>of Mars.

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<v Speaker 2>Thirty degrees. Seriously, that's incredibly steep for any vehicle, let

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<v Speaker 2>alone one that doesn't have powered wheels or direct steering.

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<v Speaker 3>It is. It really pushes the boundaries of what we

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<v Speaker 3>thought possible for passive mobility, and it dramatically increases the

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<v Speaker 3>amount of Martian terrain that would theoretically be accessible to

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<v Speaker 3>these rovers, fewer places they could get permanently stuck.

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<v Speaker 2>That's a big deal for mission planning.

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<v Speaker 3>Huge And get this, the lead scientist, Mario Yuaso Carvolio

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<v Speaker 3>dipinto Balsamasso. He noted that these results are probably conservative,

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<v Speaker 3>how so, because the small prototypes they used in the

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<v Speaker 3>wind tunnel they were actually deliberately made heavier relative to

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<v Speaker 3>their size than the final full scale five meter rover

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<v Speaker 3>is designed to be.

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<v Speaker 2>Ah So they were testing a harder to move version.

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<v Speaker 3>Exactly, if they had perfectly scaled down the weight to

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<v Speaker 3>surface area ratio, the actual threshold wind speed needed to

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<v Speaker 3>get the real thing rolling on Mars might be even

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<v Speaker 3>lower than that nine ten meters per second they measure, So.

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<v Speaker 2>The reel rover might be even more responsive to the

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<v Speaker 2>wind than these tests showed.

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<v Speaker 3>That's the suggestion, which is very encouraging.

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<v Speaker 2>Okay, so Phase one in the wind tunnel nailed down

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<v Speaker 2>the physics, the mobility threshold, the slope climbing, and validated

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<v Speaker 2>their predictive models. What was phase two about? That moved

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<v Speaker 2>things out of the lab right right?

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<v Speaker 3>Phase two is about real world operational data gathering. This

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<v Speaker 3>was the field campaign. Back in April twenty twenty five,

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<v Speaker 3>they took it to an inactive quarry in Mastricht in

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<v Speaker 3>the Netherlands.

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<v Speaker 2>Corey why there.

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<v Speaker 3>Good analog for rough, rocky, irregular terrain, more realistic than

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<v Speaker 3>a controlled lab surface, and for this test they used

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<v Speaker 3>a larger prototypes a two point seven meters diameter version

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<v Speaker 3>called the Tumbleweed Science Test.

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<v Speaker 2>Bit so bigger, closer to the real scale. And the

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<v Speaker 2>focus here wasn't if it rolls, but could the electronics

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<v Speaker 2>survive and work exactly?

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<v Speaker 3>The primary goal was proving that the internal science package

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<v Speaker 3>the electronics could not only survive the chaotic tumbling motion

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<v Speaker 3>over natural ground, but also rather clean usable scientific data

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<v Speaker 3>while tumbling.

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<v Speaker 2>What kind of instruments did this testbed carry? Was it

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<v Speaker 2>just dummy weight or actual sensors?

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<v Speaker 3>Actual sensors. It had a modular payload bay designed to

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<v Speaker 3>fit standard off the shelf components, which helps keep costs

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<v Speaker 3>down too. For this test. It carried a camera, a

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<v Speaker 3>magnetometer for measuring magnetic fields, a GPS obviously for tracking

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<v Speaker 3>his path on Earth during the test, and critically, an

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<v Speaker 3>inertial measurement unit or IMU.

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<v Speaker 2>Okay an IMU on a normal rover that helps with navigation,

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<v Speaker 2>knowing its orientation precisely. But what does an IMU do

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<v Speaker 2>inside something that's constantly spinning and tumbling. Seems like it

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<v Speaker 2>would just be chaos.

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<v Speaker 3>Well, the IMU is maybe the most critical piece for

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<v Speaker 3>getting good data in this unique situation. It measures the

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<v Speaker 3>rover's acceleration and its angular velocity. Basically, attracks exactly how

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<v Speaker 3>fast and in which direction the sphere is rotating at

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<v Speaker 3>every single moment.

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<v Speaker 2>Okay.

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<v Speaker 3>With that raw motion data, the onboard computer can then

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<v Speaker 3>mathematically comp and state for the spin. It can essentially

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<v Speaker 3>despin the readings from the other instruments.

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<v Speaker 2>Ah, so it lets the camera take a stable picture

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<v Speaker 2>or the magnetometer get a consistent reading even while the

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<v Speaker 2>whole thing is rolling.

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<v Speaker 3>Precisely, it allows you to extract stable, scientifically meaningful data

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00:17:15.400 --> 00:17:18.599
<v Speaker 3>streams from the chaos of the tumbling motion. And the

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00:17:18.640 --> 00:17:22.559
<v Speaker 3>mostric tests confirmed it worked. The platform successfully gathered and

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<v Speaker 3>processed environmental data in real time while tumbling over that

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<v Speaker 3>rough natural quarry terrain.

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<v Speaker 2>Okay, so we have proof they can roll if the

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<v Speaker 2>wind hits nine ten meters per second, they can climb

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<v Speaker 2>surprisingly steep slopes, and they can actually collect scientific data

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<v Speaker 2>while they're rolling. That brings us back to the big

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<v Speaker 2>question about the fuel source you mentioned earlier. Near surface

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<v Speaker 2>winds on Mars. We don't actually know that much about them.

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<v Speaker 3>That's been the historical challenge. Yes, our understanding is patchy.

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<v Speaker 3>Near surface winds are officially described as not well understood.

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<v Speaker 3>Why because most of our data comes from landers or rovers.

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<v Speaker 2>Which tend to land in relatively safe calm air.

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<v Speaker 3>Exactly. We pick landing sites for safety primarily not necessarily,

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<v Speaker 3>because they're the windiest places on Mars. So our data

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<v Speaker 3>has been sparse and localized.

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<v Speaker 2>That sounds like a potential achilles heel for the whole concept,

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<v Speaker 2>doesn't it relying entirely on a power source that we

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<v Speaker 2>admit we don't fully understand.

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<v Speaker 3>It definitely would be except for some more recent data

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<v Speaker 3>that's come in from let's say, non traditional wind sensors.

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<v Speaker 3>And this new data really seems to bolster the tumbleweed

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<v Speaker 3>idea quite significantly.

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<v Speaker 1>Oh like what well.

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<v Speaker 3>NASA's Insight Lander, for instance, its main job with seismology

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<v Speaker 3>listening for marsquakes, but its seismometer.

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<v Speaker 2>Was so sensitive it kicked up vibrations from the wind exactly.

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00:18:42.559 --> 00:18:45.720
<v Speaker 3>It recorded ground vibrations generated by the wind blowing across

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<v Speaker 3>the lander in the surface, and it did this for

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<v Speaker 3>over two Martian years, giving us a much longer baseline

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<v Speaker 3>of wind activity at one location.

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<v Speaker 2>Interesting any other sources, Yes.

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<v Speaker 3>And perhaps even more directly relevant measurements taken during the

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<v Speaker 3>flights of the Ingenuity Hell helicopter ah the little drone. Yeah.

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<v Speaker 3>As it flew, it sensors gathered data on air density, temperature,

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<v Speaker 3>and wind speeds much closer to the surface than orbiting

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<v Speaker 3>satellites can measure. And what both Insight and Ingenuity showed

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<v Speaker 3>was that higher wind speeds the kind cumble wheat needs

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<v Speaker 3>seem to occur to hear the surface surprisingly frequently, more

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<v Speaker 3>often than the older, lower average speeds typically reported.

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<v Speaker 2>Okay, so we're getting better evidence that strong winds near

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<v Speaker 2>the ground aren't just rare flukes. They might be a

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<v Speaker 2>regular part of the Martian weather cycle. How does this

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<v Speaker 2>new data line up with that ten meter per second

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<v Speaker 2>threshold they need?

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<v Speaker 3>The analysis, particularly of the Insight data by Mario's team,

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<v Speaker 3>is really encouraging. They suggest that, especially in Mars's northern

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<v Speaker 3>hemisphere during its summer season, the daytime wind speeds show

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<v Speaker 3>a wide distribution, but it skewed towards those higher speeds.

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<v Speaker 3>Needed Around ten meters per second isn't uncommon during the day.

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<v Speaker 2>So it's like a reliable daily power source during summer days.

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00:19:59.480 --> 00:20:02.440
<v Speaker 3>That seems to be the pattern. And interestingly, even the nights,

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00:20:02.559 --> 00:20:06.000
<v Speaker 3>which are generally calmer, aren't always dead calm. They found

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<v Speaker 3>that sometimes even at night, speeds can spike above ten

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<v Speaker 3>meters per second, maybe due to atmospheric shifts or cold

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<v Speaker 3>air drainage, winds flowing down slopes or canyon walls.

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<v Speaker 2>Okay, so the fuel seems to be there, and maybe

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<v Speaker 2>more reliably than we used to think. That's great news

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00:20:20.079 --> 00:20:23.000
<v Speaker 2>for planning emission. Now let's get to the numbers that

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<v Speaker 2>really show why this is such a different approach the range.

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00:20:26.960 --> 00:20:29.319
<v Speaker 2>If you take that r who's wind tunnel data feed

399
00:20:29.359 --> 00:20:32.720
<v Speaker 2>it into their validated prediction models, what kind of distances

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00:20:32.799 --> 00:20:34.640
<v Speaker 2>could these things actually cover on Mars.

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00:20:34.960 --> 00:20:38.160
<v Speaker 3>This is where the sheer advantage of just letting the

402
00:20:38.200 --> 00:20:42.880
<v Speaker 3>wind do the work becomes incredibly clear. Their models predict

403
00:20:42.920 --> 00:20:46.440
<v Speaker 3>that an average tumbleweed rover, just following the typical daily

404
00:20:46.480 --> 00:20:49.200
<v Speaker 3>shifts and day night cycles of the Martian wind, it

405
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<v Speaker 3>could travel about four hundred and twenty two kilometers over

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00:20:52.039 --> 00:20:53.359
<v Speaker 3>one hundred Martian souls.

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00:20:53.519 --> 00:20:56.440
<v Speaker 2>Four hundred and twenty two kilometers in one hundred souls, okay,

408
00:20:56.519 --> 00:20:59.119
<v Speaker 2>sol is a Martian day just a bit longer than ours.

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00:20:59.000 --> 00:21:01.079
<v Speaker 3>Right, about twenty four hours in thirty nine minutes. So

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<v Speaker 3>one hundred souls is roughly three earth months.

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00:21:03.480 --> 00:21:06.000
<v Speaker 2>Okay, let's put four hundred and twenty two kilometers in

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00:21:06.079 --> 00:21:08.960
<v Speaker 2>three months into perspective. How does that compare to say,

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<v Speaker 2>Curiosity or perseverance.

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00:21:10.880 --> 00:21:13.279
<v Speaker 3>It absolutely dwarfs them. I mean, think about Curiosity. The

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00:21:13.319 --> 00:21:16.519
<v Speaker 3>gold Standard landed in twenty twelve. It took over a decade,

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00:21:16.559 --> 00:21:18.839
<v Speaker 3>ten years to drive a total distance of just over

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<v Speaker 3>thirty kilometer.

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00:21:19.720 --> 00:21:22.200
<v Speaker 2>Thirty kilometers in ten years. Wow.

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00:21:22.440 --> 00:21:25.519
<v Speaker 3>Perseverance is on a similar track, measured in tens of

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00:21:25.599 --> 00:21:30.359
<v Speaker 3>kilometers total traverse. So far, this tumbleweed concept is projected

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00:21:30.359 --> 00:21:33.519
<v Speaker 3>to cover more than ten times the distance Curiosity managed

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00:21:33.759 --> 00:21:37.119
<v Speaker 3>in its entire mission in just the first three months.

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00:21:36.519 --> 00:21:39.680
<v Speaker 2>That's a completely different scale of exploration.

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00:21:39.839 --> 00:21:43.279
<v Speaker 3>It's moving from a slow, methodical crawl in one small

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00:21:43.319 --> 00:21:47.799
<v Speaker 3>area to potentially widespread, almost regional or continental coverage. That's

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00:21:47.839 --> 00:21:49.119
<v Speaker 3>the technological leap here.

427
00:21:49.160 --> 00:21:50.880
<v Speaker 2>If you break down that four hundred and twenty two

428
00:21:50.960 --> 00:21:53.839
<v Speaker 2>kilometers in one hundred souls, what's the average speed? Must

429
00:21:53.880 --> 00:21:55.160
<v Speaker 2>still be pretty slow overall.

430
00:21:55.200 --> 00:21:57.599
<v Speaker 3>The average overall speed works out to abouto point three

431
00:21:57.640 --> 00:21:59.839
<v Speaker 3>to six kilometers per hour. Yeah, it sounds slow if

432
00:21:59.880 --> 00:22:01.839
<v Speaker 3>you think about a car, but the key thing to

433
00:22:01.839 --> 00:22:05.880
<v Speaker 3>remember is that speed is sustained whenever the wind blows adequately.

434
00:22:06.359 --> 00:22:09.319
<v Speaker 3>It requires no fuel from the rover itself. It only

435
00:22:09.359 --> 00:22:12.319
<v Speaker 3>stops when the wind drops below the threshold. It's persistent.

436
00:22:12.400 --> 00:22:14.680
<v Speaker 2>Okay, So four hundred and twenty two kilometers is the

437
00:22:14.759 --> 00:22:17.920
<v Speaker 2>average predition based on typical wind cycles. What about the

438
00:22:17.920 --> 00:22:21.519
<v Speaker 2>best case scenario if you get lucky with strong, consistent

439
00:22:21.640 --> 00:22:24.440
<v Speaker 2>winds blowing in the same general direction for a long time.

440
00:22:24.640 --> 00:22:26.559
<v Speaker 2>What's the maximum potential range?

441
00:22:26.680 --> 00:22:30.319
<v Speaker 3>According to their modeling under those ideal conditions favorable terrain,

442
00:22:31.039 --> 00:22:35.839
<v Speaker 3>sustained strong winds, the maximum potential range is just staggering.

443
00:22:36.559 --> 00:22:39.720
<v Speaker 3>A single tumbleweed rover could potentially traverse as much as

444
00:22:39.839 --> 00:22:41.160
<v Speaker 3>twenty eight hundred kilometers.

445
00:22:41.240 --> 00:22:45.599
<v Speaker 2>Twenty eight hundred kilometers, that's like driving from Chicago to Denver,

446
00:22:46.039 --> 00:22:47.359
<v Speaker 2>or maybe halfway across the US.

447
00:22:47.440 --> 00:22:51.039
<v Speaker 3>It's enormous. We're talking about the potential to map geological

448
00:22:51.160 --> 00:22:56.359
<v Speaker 3>changes atmospheric phenomena across entire, vast regions of Mars that

449
00:22:56.400 --> 00:23:00.000
<v Speaker 3>are currently completely inaccessible to us, all powered by nothing

450
00:23:00.119 --> 00:23:02.920
<v Speaker 3>more than the thin Martian air. It really opens the

451
00:23:02.960 --> 00:23:05.559
<v Speaker 3>door to true continent scale exploration.

452
00:23:05.799 --> 00:23:08.680
<v Speaker 2>That twenty eight hundred kilometer figure, Wow, that really sells

453
00:23:08.680 --> 00:23:12.240
<v Speaker 2>the vision. So who's behind this, who's the engine driving this? Well?

454
00:23:12.519 --> 00:23:15.680
<v Speaker 2>Pretty bowl high risk but potentially a very high reward idea.

455
00:23:15.839 --> 00:23:18.960
<v Speaker 3>The group is called Team Tumbleweed, and they're specifically described

456
00:23:18.960 --> 00:23:23.119
<v Speaker 3>as an interdisciplinary group of young, entrepreneurial scientists. Their structure

457
00:23:23.200 --> 00:23:26.039
<v Speaker 3>kind of reflects the whole low cost, high impact vibe

458
00:23:26.039 --> 00:23:27.000
<v Speaker 3>of the project itself.

459
00:23:27.119 --> 00:23:30.680
<v Speaker 2>Young and entrepreneurial often means agile, quick to adapt, and

460
00:23:30.720 --> 00:23:32.799
<v Speaker 2>you mentioned they're international very much.

461
00:23:32.640 --> 00:23:36.839
<v Speaker 3>So, which definitely helps when you're tackling a complex, multifaceted

462
00:23:36.880 --> 00:23:39.480
<v Speaker 3>problem like this. While the main hubs seem to be

463
00:23:39.519 --> 00:23:42.759
<v Speaker 3>in Vienna, Austria, and Delft in the Netherlands, the team

464
00:23:42.839 --> 00:23:45.640
<v Speaker 3>actually brings together people from over twenty different countries.

465
00:23:45.839 --> 00:23:49.799
<v Speaker 2>That's impressive. That global collaboration must be key for pulling

466
00:23:49.880 --> 00:23:56.000
<v Speaker 2>together expertise in what atmospheric physics, material science, robotics, software, all.

467
00:23:55.880 --> 00:23:58.759
<v Speaker 3>Of the above. You need all those disciplines working together

468
00:23:58.799 --> 00:24:01.599
<v Speaker 3>simultaneously to make concept fly literally.

469
00:24:01.799 --> 00:24:04.640
<v Speaker 2>Okay, so they've proven the basic physics works, they prove

470
00:24:04.720 --> 00:24:08.039
<v Speaker 2>mobility and simulated Mars conditions. They prove they can collect

471
00:24:08.079 --> 00:24:10.680
<v Speaker 2>data while tumbling. What are the next big steps? What

472
00:24:10.720 --> 00:24:12.799
<v Speaker 2>do they need to do to get this platform from

473
00:24:12.920 --> 00:24:16.519
<v Speaker 2>say a working prototype, to something genuinely flight ready.

474
00:24:16.759 --> 00:24:19.160
<v Speaker 3>The main goal now is moving up the ladder of

475
00:24:19.200 --> 00:24:21.200
<v Speaker 3>technology readiness levels or.

476
00:24:21.119 --> 00:24:26.079
<v Speaker 2>Trls TRLS, right, that's the standard scale NASA and eesus

477
00:24:26.160 --> 00:24:28.799
<v Speaker 2>to gauge how mature a space technology is. Isn't it

478
00:24:28.839 --> 00:24:30.799
<v Speaker 2>goes from one to nine exactly?

479
00:24:30.960 --> 00:24:34.599
<v Speaker 3>TRL one is just basic principles observed. Tier nine is

480
00:24:34.680 --> 00:24:38.519
<v Speaker 3>flight proven on a successful mission. These recent tests, the

481
00:24:38.519 --> 00:24:41.319
<v Speaker 3>wind tunnel and the Qrey field test have likely pushed

482
00:24:41.359 --> 00:24:45.240
<v Speaker 3>Tumbleweed into the mid level TRLS, maybe TROL four or five.

483
00:24:45.319 --> 00:24:48.000
<v Speaker 3>Validation in a lab or relevant environment.

484
00:24:48.160 --> 00:24:48.480
<v Speaker 2>Okay.

485
00:24:48.759 --> 00:24:51.599
<v Speaker 3>To get to flight readiness, say TRL seven, eight, or nine,

486
00:24:51.720 --> 00:24:53.880
<v Speaker 3>they need to push forward on primarily two tracks.

487
00:24:53.920 --> 00:24:57.039
<v Speaker 2>Now, Track one, I'm guessing is making those prediction models

488
00:24:57.039 --> 00:24:59.400
<v Speaker 2>even better. Since you can't steer it, you absolutely have

489
00:24:59.400 --> 00:25:00.839
<v Speaker 2>to know where it's going precisely.

490
00:25:01.039 --> 00:25:03.920
<v Speaker 3>They need to keep refining those rover dynamics models. The

491
00:25:03.960 --> 00:25:08.079
<v Speaker 3>real challenge is modeling the chaotic nature of Martian wind accurately.

492
00:25:08.680 --> 00:25:12.559
<v Speaker 3>You've got turbulence, unpredictable gusts, maybe small dust devils that

493
00:25:12.599 --> 00:25:15.559
<v Speaker 3>could knock it off course. Terrain features like canyons or

494
00:25:15.640 --> 00:25:17.839
<v Speaker 3>large dune fields. It could block it or channel the

495
00:25:17.880 --> 00:25:22.119
<v Speaker 3>wind in unexpected ways. Mission control needs models sophisticated enough

496
00:25:22.240 --> 00:25:24.319
<v Speaker 3>that they can feed in the latest wind data, maybe

497
00:25:24.359 --> 00:25:29.200
<v Speaker 3>from orbiters or other assets, and get reliable trajectory predictions hours,

498
00:25:29.440 --> 00:25:33.160
<v Speaker 3>maybe even souls in advance. That's essential for coordinating the

499
00:25:33.200 --> 00:25:35.559
<v Speaker 3>swarm and making sure they actually hit their scientific targets.

500
00:25:35.640 --> 00:25:38.359
<v Speaker 2>What happens if one does get stuck, you know, rolls

501
00:25:38.359 --> 00:25:40.559
<v Speaker 2>into a deep crack or gets wedged in a really

502
00:25:40.640 --> 00:25:43.400
<v Speaker 2>dense field of boulders, there's no way to drive it out.

503
00:25:43.839 --> 00:25:45.680
<v Speaker 2>How do they handle that inevitability?

504
00:25:46.000 --> 00:25:49.160
<v Speaker 3>That's the inherent risk, and the operational philosophy has to

505
00:25:49.240 --> 00:25:53.359
<v Speaker 3>accept it. There's no rescue capability like with a wheeled rover,

506
00:25:54.160 --> 00:25:58.240
<v Speaker 3>so the mission relies on two things. First, that's surprising

507
00:25:58.319 --> 00:26:01.759
<v Speaker 3>thirty degree slope climbing ability. We talked about that significantly

508
00:26:01.799 --> 00:26:04.640
<v Speaker 3>reduces the chances of getting permanently stuck in many types

509
00:26:04.680 --> 00:26:05.960
<v Speaker 3>of unfavorable.

510
00:26:05.480 --> 00:26:07.519
<v Speaker 2>Terrain, okay, makes it more robust.

511
00:26:07.680 --> 00:26:12.240
<v Speaker 3>Second, and maybe more importantly, the swarm strategy itself provides

512
00:26:12.400 --> 00:26:16.440
<v Speaker 3>redundancy because each rover is relatively low cost. If one

513
00:26:16.519 --> 00:26:19.720
<v Speaker 3>or two out of a swarm of say twenty, get incapacitated,

514
00:26:20.079 --> 00:26:21.119
<v Speaker 3>it's not mission failure.

515
00:26:21.160 --> 00:26:22.880
<v Speaker 2>It's an acceptable loss exactly.

516
00:26:23.039 --> 00:26:25.920
<v Speaker 3>The overall mission continues with the remaining units. The low

517
00:26:25.960 --> 00:26:29.079
<v Speaker 3>cost allows for a higher tolerance for individual unit failure

518
00:26:29.279 --> 00:26:31.279
<v Speaker 3>compared to a single billion dollar asset.

519
00:26:31.400 --> 00:26:34.480
<v Speaker 2>Okay. So refining prediction models is track one. What's track

520
00:26:34.519 --> 00:26:38.079
<v Speaker 2>two for reaching higher trls? Integrating better instruments?

521
00:26:38.319 --> 00:26:43.039
<v Speaker 3>Yes, moving beyond the foundational sensors like the camera and

522
00:26:43.160 --> 00:26:45.720
<v Speaker 3>IMU that they used in the test bed. The next

523
00:26:45.759 --> 00:26:50.440
<v Speaker 3>phase is about integrating more specialized science focused instruments into

524
00:26:50.480 --> 00:26:53.960
<v Speaker 3>that payload bay. Instruments that really leverage the fact that

525
00:26:54.000 --> 00:26:55.359
<v Speaker 3>you'll have many of these spread out.

526
00:26:55.640 --> 00:26:57.319
<v Speaker 2>Like what specifically are they looking at.

527
00:26:57.559 --> 00:27:00.960
<v Speaker 3>They're focusing on things like advanced radiation set to map

528
00:27:01.039 --> 00:27:05.599
<v Speaker 3>radiation levels across different latitudes and terrains, specialized soil probes.

529
00:27:05.960 --> 00:27:08.279
<v Speaker 3>Maybe something that can be quickly deployed or inserted into

530
00:27:08.279 --> 00:27:10.319
<v Speaker 3>the ground when the rover naturally pauses for.

531
00:27:10.319 --> 00:27:13.240
<v Speaker 2>A bit ah interesting like a little quick sample.

532
00:27:13.119 --> 00:27:16.759
<v Speaker 3>Maybe, And also highly sensitive dust sensors. Given that the

533
00:27:16.799 --> 00:27:20.920
<v Speaker 3>whole vehicle relies on atmospheric dynamics in Mars is famously dusty,

534
00:27:21.400 --> 00:27:25.160
<v Speaker 3>understanding dust transport and properties across wide areas is crucial.

535
00:27:25.759 --> 00:27:28.880
<v Speaker 3>These instruments make the platform much more scientifically potent.

536
00:27:28.799 --> 00:27:32.440
<v Speaker 2>More sophisticated instruments, better models. That brings us to the

537
00:27:32.480 --> 00:27:35.960
<v Speaker 2>next big test, doesn't it, the final really critical field

538
00:27:36.000 --> 00:27:38.559
<v Speaker 2>test before they can claim high TRL status. They're going

539
00:27:38.559 --> 00:27:41.039
<v Speaker 2>somewhere very specific, very Mars like.

540
00:27:41.480 --> 00:27:44.680
<v Speaker 3>That's right. The next major field campaign is scheduled for November,

541
00:27:45.039 --> 00:27:47.440
<v Speaker 3>and it's taking place in the Atacama Desert in Chile.

542
00:27:47.599 --> 00:27:50.000
<v Speaker 2>The Atacamma, Yeah, that's famous for being one of the

543
00:27:50.000 --> 00:27:53.400
<v Speaker 2>best Mars analog environments on Earth, Isn't it? Super dry,

544
00:27:53.640 --> 00:27:55.319
<v Speaker 2>high altitude, intense UV.

545
00:27:55.799 --> 00:27:57.920
<v Speaker 3>Exactly. It's about as close as you can get to

546
00:27:57.960 --> 00:28:02.160
<v Speaker 3>Martian surface conditions without lee the planet ideal for pushing

547
00:28:02.200 --> 00:28:03.400
<v Speaker 3>the system to its limits?

548
00:28:03.480 --> 00:28:05.480
<v Speaker 2>And what's the main goal in the Atacamma. It's not

549
00:28:05.519 --> 00:28:07.960
<v Speaker 2>just about proving one rover can roll again.

550
00:28:07.799 --> 00:28:10.759
<v Speaker 3>Right, No, this is a system's level test. The plan

551
00:28:10.920 --> 00:28:13.200
<v Speaker 3>is to deploy at least two of the Tumbleweed Science

552
00:28:13.240 --> 00:28:18.440
<v Speaker 3>Test bed rovers simultaneously and significantly, they'll be carrying instruments

553
00:28:18.480 --> 00:28:21.759
<v Speaker 3>provided by researchers from external partner organizations.

554
00:28:21.799 --> 00:28:24.759
<v Speaker 2>Oh interesting, So other science teams are starting to buy in,

555
00:28:24.839 --> 00:28:27.759
<v Speaker 2>wanting to get their instruments on this platform, it seems so.

556
00:28:28.200 --> 00:28:30.839
<v Speaker 3>That's a really good sign for the project's credibility within

557
00:28:30.880 --> 00:28:34.759
<v Speaker 3>the wider planetary science community. But the absolute key objective

558
00:28:34.759 --> 00:28:36.720
<v Speaker 3>in the ATA comma, the thing they really need to

559
00:28:36.799 --> 00:28:41.200
<v Speaker 3>nail down the swarm. Yes, operationalizing the core concept the

560
00:28:41.240 --> 00:28:42.079
<v Speaker 3>swarm itself.

561
00:28:42.440 --> 00:28:45.960
<v Speaker 2>Testing how multiple windblown balls coordinate with each other? How

562
00:28:46.000 --> 00:28:47.000
<v Speaker 2>does that even work?

563
00:28:47.240 --> 00:28:49.759
<v Speaker 3>That's what they need to figure out and demonstrate. The

564
00:28:49.839 --> 00:28:54.720
<v Speaker 3>priory goal is testing and validating the swarm coordination strategies

565
00:28:55.400 --> 00:29:00.720
<v Speaker 3>in that realistic, harsh Mars like environment. This involves some

566
00:29:00.759 --> 00:29:04.720
<v Speaker 3>pretty complex software and algorithms. How do two or more

567
00:29:04.839 --> 00:29:08.720
<v Speaker 3>rovers constantly moving semi randomly based on the wind maintain

568
00:29:08.799 --> 00:29:09.839
<v Speaker 3>communication links?

569
00:29:09.920 --> 00:29:11.279
<v Speaker 2>Yeah? How do they talk to each other?

570
00:29:11.359 --> 00:29:14.759
<v Speaker 3>How do they coordinate their science? For example, can mission

571
00:29:14.799 --> 00:29:17.400
<v Speaker 3>control instruct one rover that happens to be an interesting

572
00:29:17.440 --> 00:29:19.599
<v Speaker 3>spot to try and stop or slow down to take

573
00:29:19.640 --> 00:29:23.079
<v Speaker 3>a soil measurement while another nearby rover keeps rolling to

574
00:29:23.160 --> 00:29:26.599
<v Speaker 3>track an incoming weatherfront. Can they re elect data between

575
00:29:26.599 --> 00:29:28.160
<v Speaker 3>themselves to get back to an orbiter.

576
00:29:28.319 --> 00:29:30.960
<v Speaker 2>So it's moving way beyond just a single tech demo.

577
00:29:31.000 --> 00:29:34.279
<v Speaker 2>It's about proving they can operate as an intelligent distributed.

578
00:29:33.839 --> 00:29:37.759
<v Speaker 3>Network, precisely autonomous coordination. That's the final piece needed to

579
00:29:37.799 --> 00:29:41.880
<v Speaker 3>show this is a viable, functional scientific exploration strategy ready

580
00:29:41.880 --> 00:29:42.359
<v Speaker 3>for space.

581
00:29:42.680 --> 00:29:46.960
<v Speaker 2>So they're really ticking the boxes mobility, proven data integrity,

582
00:29:47.039 --> 00:29:51.720
<v Speaker 2>while tumbling, proven wind availability, looking more promising, slow climbing

583
00:29:51.799 --> 00:29:57.799
<v Speaker 2>capability demonstrated, and now the final hurdle. Autonomous swarm coordination

584
00:29:58.119 --> 00:29:59.960
<v Speaker 2>in a Mars like place.

585
00:30:00.119 --> 00:30:03.480
<v Speaker 3>Really is the comprehensive arc of the validation process they've undertaken.

586
00:30:03.519 --> 00:30:06.200
<v Speaker 3>It's fascinating, isn't it. The core idea is so simple,

587
00:30:06.319 --> 00:30:08.880
<v Speaker 3>let the wind push it. But making it actually work

588
00:30:09.119 --> 00:30:14.240
<v Speaker 3>reliably as a coordinated scientific tool requires this incredibly complex,

589
00:30:14.319 --> 00:30:18.039
<v Speaker 3>highly specialized software and system design to manage the inherent

590
00:30:18.119 --> 00:30:19.279
<v Speaker 3>chaos of the environment.

591
00:30:19.400 --> 00:30:21.599
<v Speaker 2>It really is a remarkable achievement just to get to

592
00:30:21.640 --> 00:30:24.319
<v Speaker 2>the stage all this experimental validation. It feels like it

593
00:30:24.400 --> 00:30:27.240
<v Speaker 2>successfully dragged the tumbleweed concept out of the realm of

594
00:30:27.880 --> 00:30:31.759
<v Speaker 2>cool idea and into something measured, practical, application focused. They've

595
00:30:31.759 --> 00:30:34.400
<v Speaker 2>shown the mobility works. They can survive steep slopes, they

596
00:30:34.400 --> 00:30:37.279
<v Speaker 2>can get real time data, all using Martian wind.

597
00:30:37.440 --> 00:30:41.440
<v Speaker 3>Yeah. I think this project really signifies a potential shift,

598
00:30:41.480 --> 00:30:45.440
<v Speaker 3>maybe a fundamental one, in how we think about exploring planets.

599
00:30:46.440 --> 00:30:49.880
<v Speaker 3>We could be moving away, or at least augmenting the

600
00:30:49.960 --> 00:30:54.119
<v Speaker 3>traditional model centralized very high cost, low moving platforms towards

601
00:30:54.160 --> 00:30:57.720
<v Speaker 3>methods that are inherently cheaper, much more extensive in coverage,

602
00:30:57.839 --> 00:31:00.799
<v Speaker 3>and actually use the planetary environment itself for mobility.

603
00:31:00.960 --> 00:31:01.079
<v Speaker 2>Right.

604
00:31:01.319 --> 00:31:05.119
<v Speaker 3>It just completely redefines what parts of Mars we consider accessible.

605
00:31:05.359 --> 00:31:07.279
<v Speaker 3>The Tumbleweed is kind of a testament to the idea

606
00:31:07.319 --> 00:31:10.559
<v Speaker 3>that sometimes the biggest breakthroughs come from embracing well radical

607
00:31:10.559 --> 00:31:13.519
<v Speaker 3>simplification in the core engineering, even if the supporting systems

608
00:31:13.519 --> 00:31:14.119
<v Speaker 3>get complex.

609
00:31:14.400 --> 00:31:17.759
<v Speaker 2>So what does this huge leap in potential coverage actually

610
00:31:17.799 --> 00:31:20.759
<v Speaker 2>mean for the science we can do on Mars? If

611
00:31:20.799 --> 00:31:23.440
<v Speaker 2>you really could have dozens of these low cost sensors

612
00:31:23.519 --> 00:31:26.799
<v Speaker 2>rolling potentially thousands of kilometers like that twenty eight hundred

613
00:31:26.839 --> 00:31:31.799
<v Speaker 2>kilometer max range. What revolutionary questions could we finally answer

614
00:31:31.880 --> 00:31:35.200
<v Speaker 2>things that are impossible now, Questions that only as swarm

615
00:31:35.279 --> 00:31:39.920
<v Speaker 2>traversing continents simultaneously could tackle. Think about tracking atmospheric waves

616
00:31:40.279 --> 00:31:44.480
<v Speaker 2>or mapping huge geological boundaries over time. What discoveries might

617
00:31:44.480 --> 00:31:46.680
<v Speaker 2>be out there just waiting for a rover that doesn't

618
00:31:46.759 --> 00:31:49.319
<v Speaker 2>need to stop for fuel, doesn't need complex repairs, It

619
00:31:49.440 --> 00:31:50.519
<v Speaker 2>just needs the wind to blow.

620
00:31:50.599 --> 00:31:52.720
<v Speaker 3>That's the million dollar question, isn't it, or maybe the

621
00:31:52.799 --> 00:31:55.920
<v Speaker 3>multimillion dollar question. Even if the rovers themselves are cheaper,

622
00:31:56.440 --> 00:31:59.000
<v Speaker 3>it genuinely changes the scale of what we even think

623
00:31:59.039 --> 00:33:38.720
<v Speaker 3>of as planetary exploration.
