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>Okay, let's unpack this. When you think about space travel,

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<v Speaker 2>what's the first image that comes to mind.

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<v Speaker 3>For most people? I bet it's that classic rocket line.

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<v Speaker 2>Exactly, fire, smoke, this enormous vehicle just fighting its way

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<v Speaker 2>off the planet. Maybe you know a Soyuz lifting off

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<v Speaker 2>from Bacon Ore.

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<v Speaker 3>It's an incredible sight, no doubt powerful.

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<v Speaker 2>Definitely powerful. But that image, that very picture of a

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<v Speaker 2>rocket launch, it actually highlights this this huge fundamental problem,

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<v Speaker 2>a challenge that's really held back our bigger dreams for

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<v Speaker 2>exploring deep space or well over a century now.

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<v Speaker 3>It really has because despite all our advanced engineering, rockets

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<v Speaker 3>still work on a pretty simple.

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<v Speaker 2>Principle Judent's third law.

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<v Speaker 3>That's the one for every action, there's an equal and

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<v Speaker 3>opposite reaction. You burn fuel, throw that mass backwards. Really fast, and.

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<v Speaker 2>The reaction pushes the rocket forwards. Simple physics, simple.

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<v Speaker 3>But brutal and inescapable really.

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<v Speaker 2>And needing to throw a mass away like that. That

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<v Speaker 2>leads straight to the big mathematical hurdle, the one constantin

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<v Speaker 2>Siolkowski figured out way back in nineteen oh three.

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<v Speaker 3>Ah, Yes, the famous rocket equation.

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<v Speaker 2>It basically spells out this limit the mass ratio problem.

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<v Speaker 2>And people call it a tyranny for a reason.

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<v Speaker 3>It absolutely is a tyranny. It traps us in this well,

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<v Speaker 3>this vicious cycle. See the fuel you need to speed

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<v Speaker 3>up your spacecraft. It's heavy, really heavy.

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<v Speaker 2>And you have to carry that fuel on the rocket.

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<v Speaker 3>Which means you need more fuel just to lift the

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<v Speaker 3>first batch of fuel.

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<v Speaker 2>It gets exponential, right, Skiolkowski's equation just lays it bare

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<v Speaker 2>that desired speed change engineers call it to v It

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<v Speaker 2>depends exponentially on how much of your rocket is fuel

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<v Speaker 2>versus payload.

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<v Speaker 3>And exponential here is well, that's punishing.

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<v Speaker 2>Maybe give us a sense of that. Like, if you

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<v Speaker 2>want to double your speed leaving Earth orbit.

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<v Speaker 3>Yeah, good point. Doubling your speed might mean you need

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<v Speaker 3>say five times the fuel, not just twice as much,

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<v Speaker 3>maybe even more Wow. And for really ambitious stuff deep

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<v Speaker 3>space or you know, a big dream interstellar travel, you

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<v Speaker 3>need huge delta V.

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<v Speaker 2>So the amount of fuel you need just skyrockets.

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<v Speaker 3>Exactly the mass fraction, the percentage of your rocket that's

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<v Speaker 3>just propelling it gets closer and closer to one hundred percent.

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<v Speaker 2>Like ninety nine percent fuel, one percent.

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<v Speaker 3>Space ship, or even ninety nine point nine to nine

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<v Speaker 3>percent fuel. You're basically launching fuel to launch fuel to

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<v Speaker 3>launch fuel. It makes high speed interstellar travels seem well,

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<v Speaker 3>not just hard, but almost physically impossible. With chemical rockets,

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<v Speaker 3>we just can't carry enough energy that way.

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<v Speaker 2>Okay, So that sets up our mission for this deep dive.

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<v Speaker 2>Then the sources you've looked at, they're all about breaking

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<v Speaker 2>that cycle, aren't they.

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<v Speaker 3>Precisely the big much in driving this is what if

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<v Speaker 3>spacecraft didn't have to carry their propellant, What if they

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<v Speaker 3>could just leave the fuel behind, find another way, find

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<v Speaker 3>another way. And that's exactly what's explored in this really

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<v Speaker 3>comprehensive new review. It popped up on the arcs of

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<v Speaker 3>Preprint Server by Roma Nya, kezerashphili.

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<v Speaker 2>Arxif right, the Physics preprint place.

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<v Speaker 3>Yeah, and this review looks carefully at different ways to

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<v Speaker 3>get propellent less propulsion, so systems that don't burn on

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<v Speaker 3>board masks, but instead tap into forces and energy that

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<v Speaker 3>are already out there in space.

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<v Speaker 2>We're not just talking about making rockets a bit more

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<v Speaker 2>efficient here.

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<v Speaker 3>No, no, not at all. This is a whole different

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<v Speaker 3>way of thinking, a paradigm shift, really.

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<v Speaker 2>So the big takeaway right up front, the.

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<v Speaker 3>Crucial point from the review is that these propellantless methods,

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<v Speaker 3>they aren't just improvements. They could actually enable missions that

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<v Speaker 3>are completely impossible right now with conventional rockets.

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<v Speaker 2>Especially if you want to go far, like really far

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<v Speaker 2>beyond Pluto, kind.

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<v Speaker 3>Of far exactly. Getting rid of that need for propellant

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<v Speaker 3>escaping the mass trap, it changes everything, mission design, what's feasible,

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<v Speaker 3>the whole game.

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<v Speaker 2>Right, So where do we start. There's one method that's

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<v Speaker 2>actually been used for quite a while, hasn't it? Less

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<v Speaker 2>future tech, more clever maneuvering.

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<v Speaker 3>That's right, the gravity assist. It's probably the simplest propellantless

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<v Speaker 3>technique and it's got a proven track record going back decades.

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<v Speaker 3>We could call it maybe the easiest theft.

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<v Speaker 2>Huh, I like that a theft of momentum.

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<v Speaker 3>Conceptually, yeah, that's pretty much it. It's elegant. Really. You

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<v Speaker 3>time a spacecraft's flight path very very carefully, so it

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<v Speaker 3>swings close by a big planet like Jupiter or Venus.

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<v Speaker 2>You fly past it on a specific path, a hyperbolic trajectory,

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<v Speaker 2>I think is called correct.

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<v Speaker 3>And as it swings by, the spacecraft and the planet

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<v Speaker 3>exchange a bit of momentum. The planet has so much

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<v Speaker 3>momentum it barely.

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<v Speaker 2>Notices but for the tiny spacecraft.

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<v Speaker 3>For the spacecraft, it's huge. It effectively steals a tiny

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<v Speaker 3>fraction of the planet's orbital momentum, and that translates into

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<v Speaker 3>a significant speed boost for the probe, completely free in

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<v Speaker 3>terms of fuel.

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<v Speaker 2>It's like a cosmic sling shot conservation of energy, doing.

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<v Speaker 3>The work exactly. And the textbook example, the one everyone

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<v Speaker 3>points to, has to be the Voyager Probes.

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<v Speaker 2>AH Voyager one and two. The Grand Tour.

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<v Speaker 3>The Grand Tour, Yeah, launched back in the late seventies.

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<v Speaker 3>They took advantage of this really rare alignment of the outer.

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<v Speaker 2>Planets Jupiter, Saturn, Uranus, Neptune, the visit at all four didn't.

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<v Speaker 3>They did, using one gravity assist after another to hop

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<v Speaker 3>from planet to planet, getting boosts along the way, and

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<v Speaker 3>doing that.

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<v Speaker 2>With chemical rockets alone, carrying enough fuel impossible.

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<v Speaker 3>Just completely impossible. The amount of fuel needed would have

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<v Speaker 3>been astronomical. Voyager is just the stunning example of how

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<v Speaker 3>powerful orbital mechanics can be.

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<v Speaker 2>It really is brilliant, a testament to clever engineering and physics.

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<v Speaker 2>But there's always a butt, isn't there. The review mentions

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<v Speaker 2>the trade offs.

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<v Speaker 3>There are always trade offs. Gravity assists work, We've mastered

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<v Speaker 3>the technique, but they have some pretty big practical limitations.

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<v Speaker 2>You can't just decide to do one whenever you feel

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<v Speaker 2>like it.

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<v Speaker 3>No apps not, That's the main constraint. You are completely

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<v Speaker 3>dependent on the planets being in the right place at

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<v Speaker 3>the right time.

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<v Speaker 2>Relative to each other and relative to where you want.

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<v Speaker 3>To go exactly. These alignments are where the Voyager opportunity,

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<v Speaker 3>for instance, only comes around once every one hundred and

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<v Speaker 3>seventy six years.

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<v Speaker 2>Wow. So mission planners aren't just looking at next Tuesday.

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<v Speaker 2>They're looking decades ahead mapping planetary positions.

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<v Speaker 3>They use these things called pork chop plots.

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<v Speaker 2>Pork chop plots.

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<v Speaker 3>Serious, seriously, they're graphs that show the possible launch windows

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<v Speaker 3>flight times and energy needed. They basically highlight how you

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<v Speaker 3>only get these narrow windows maybe a few weeks every

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<v Speaker 3>few years or even decades to launch if you want

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<v Speaker 3>to use a specific gravity assist.

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<v Speaker 2>Path, so very limited opportunities, and the path.

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<v Speaker 3>Itself it's totally inflexible. Once you launch, you're locked into

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<v Speaker 3>that trajectory. It's dictated by celestial mechanics, by the cosmic clock,

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<v Speaker 3>not by where you might want to go explore next week.

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<v Speaker 2>So great for preplan tours, but not for flexible on

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<v Speaker 2>demand exploration. If you need continuous thrust or the ability

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<v Speaker 2>to change course easily.

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<v Speaker 3>You need something else. You need to look beyond planets

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<v Speaker 3>and start tapping into the energy sources that are always

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<v Speaker 3>there in space.

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<v Speaker 2>Okay, which takes us to the next step, moving away

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<v Speaker 2>from these occasional gravitational boosts towards something more constant. And

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<v Speaker 2>this is where I think you said it gets really interesting,

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<v Speaker 2>harnessing sunlight itself.

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<v Speaker 3>Exactly solar sales. This shifts the concept from borrowing momentum

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<v Speaker 3>from a planet to catching momentum from the most abundant

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<v Speaker 3>energy source in the Solar system.

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<v Speaker 2>Sunlight solar pressure. Now I know some listeners might hear

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<v Speaker 2>solar sale and think of old sci fi. Is the

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<v Speaker 2>physics really solid here? How can light push something if

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<v Speaker 2>photons don't have mass?

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<v Speaker 3>It's fundamental physics. Actually, photons, the particles of light, might

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<v Speaker 3>have zero rest mass, but they definitely carry momentum. So

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<v Speaker 3>when photons hit something, they transfer that momentum. If they

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<v Speaker 3>get absorbed, they transfer some, But if they get reflected,

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<v Speaker 3>which is what a shiny sale is designed to do,

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<v Speaker 3>they transfer about twice the momentum, like bouncing a ball

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<v Speaker 3>off a wall.

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<v Speaker 2>Ah. Okay, so the sails like a giant mirror.

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<v Speaker 3>Essentially, yes, a huge, incredibly thin reflective membrane. It catches

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<v Speaker 3>the momentum from countless photons hitting it, But the.

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<v Speaker 2>Push from a single photon must be minuscule.

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<v Speaker 3>Oh, absolutely tiny, infantesimal. But the sun is always shining,

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<v Speaker 3>so that tiny push is constant. It's there two entred

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<v Speaker 3>and forty seven week after week.

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<v Speaker 2>Year after year, and over time, that constant, gentle push

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<v Speaker 2>adds up.

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<v Speaker 3>It adds up, It builds velocity, gradually, slowly at first,

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<v Speaker 3>but persistently, And the most beautiful part, it uses zero

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<v Speaker 3>fuel once it's deployed. Zero.

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<v Speaker 2>That dream became reality thanks to Japan Space Agency JAXA.

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<v Speaker 3>Right yes, with the Ikros probe. That was a fantastic

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<v Speaker 3>mission back in twenty ten, a real game changer.

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<v Speaker 2>What did it do?

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<v Speaker 3>JAXA successfully deployed the square sale in space, controlled it

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<v Speaker 3>and used it to fly the probe all the way

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<v Speaker 3>to Venus, powered only by sunlight.

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<v Speaker 2>Wow, just push by light, just push by light.

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<v Speaker 3>It proved the works in the real world, not just

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<v Speaker 3>on paper or in in computer models.

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<v Speaker 2>Okay, so proof of concept check. But the review it

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<v Speaker 2>really digs into the challenges the downsides. The engineering side sounds.

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<v Speaker 3>Delicate, extremely delicate. Material science is the huge bottleneck here.

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<v Speaker 3>For a solar sale to be effective, it needs to

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<v Speaker 3>be incredibly light, but also incredibly large. We talk about

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<v Speaker 3>aerial density, the mass per square meter.

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<v Speaker 2>You want that number to be tiny, as low as possible.

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<v Speaker 3>We're talking materials that are almost like smoke gossamer thin,

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<v Speaker 3>maybe just a few milligrams per square meter, but the

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<v Speaker 3>sale itself needs to be vast. Think multiple football fields

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<v Speaker 3>in area.

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<v Speaker 2>So imagine trying to unfold something thinner than kitchen plastic

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<v Speaker 2>wrap but kilometers across in space without ripping it exactly.

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<v Speaker 3>And then you have to keep it tensioned, stable, pointed correctly.

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<v Speaker 3>It's an engineer's nightmak.

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<v Speaker 2>What are these materials? Usually made of.

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<v Speaker 3>Specialized plastics, often polymers like CP one or types of

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<v Speaker 3>polymide film coated with a thin layer of aluminum for reflectivity.

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<v Speaker 3>But they also have to be incredibly tough.

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<v Speaker 2>Tough against what space is empty, right.

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<v Speaker 3>Not quite empty enough. They have to survive years, maybe decades,

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<v Speaker 3>bathed in intense ultraviolet radiation from the Sun, which degrades

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<v Speaker 3>materials over time. Plus there's constant bombardment by tiny dust particles, micrometeoroids.

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<v Speaker 2>H space dust. Even a tiny speck hitting that thin

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<v Speaker 2>film at high speed.

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<v Speaker 3>Could potentially cause a tear, and enough small tiers could

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<v Speaker 3>affect the sale's structure, its tension, its ability to generate

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<v Speaker 3>thrust efficiently.

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<v Speaker 2>Okay, so materials and deployment are hard, Yeah, but there's

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<v Speaker 2>a more fundamental physics limitation too, right, tied to distance.

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<v Speaker 3>Yes, And this is a big one sunlight and therefore

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<v Speaker 3>the radiation pressure it creates follows the inverse square law, meaning.

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<v Speaker 2>The further you get from the Sun, the weaker the push.

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<v Speaker 3>Dramatically weaker. The forest drops off with the square of

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<v Speaker 3>the distance. So if you go from Earth's distance one

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<v Speaker 3>astronomical unit or AU out to Jupiter, which is about

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<v Speaker 3>five away.

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<v Speaker 2>The force isn't five times weaker.

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<v Speaker 3>It's twenty five times weaker five square oach.

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<v Speaker 2>That's a massive drop in acceleration.

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<v Speaker 3>It really is. It makes solar sales potentially great permissions

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<v Speaker 3>inside the orbit of Mars, maybe out to the asteroid belt,

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<v Speaker 3>but for deep space, going out past Jupiter to Saturn, Uranus,

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<v Speaker 3>Neptune or beyond.

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<v Speaker 2>The push becomes almost nothing, pretty much negligible.

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<v Speaker 3>Your acceleration just fades away. So for exploring the outer

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<v Speaker 3>Solar System or heading towards the stars, solar cells alone

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<v Speaker 3>probably aren't the answer.

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<v Speaker 2>Okay, So if sunlight pressure gets too weak out there,

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<v Speaker 2>what else is constantly flowing outwards from the Sun that

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<v Speaker 2>we could potentially push.

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<v Speaker 3>Against that leads us to the solar wind?

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<v Speaker 2>Uh, not light pressure, but actual particles exactly.

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<v Speaker 3>The solar wind is this continuous supersonic stream of charged

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<v Speaker 3>particles plasma mostly protons and electrons, that flows out from

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<v Speaker 3>the Sun all the time, and crucially, it carries significant

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<v Speaker 3>momentum and keeps a decent density much further out than

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<v Speaker 3>where sunlight pressure.

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<v Speaker 2>Because okay, so if we can push against that, maybe

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<v Speaker 2>we can get thrust further out. Yeah, this brings us

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<v Speaker 2>to magnetic sales.

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<v Speaker 3>Mag sales, correct magnetic sales. It's a totally different concept

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<v Speaker 3>from reflecting.

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<v Speaker 2>Light because there's no physical sail, right, you can't reflect

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<v Speaker 2>charged particles with a sheet of plastic right.

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<v Speaker 3>Instead of a physical membrane, a mag sail uses loops

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<v Speaker 3>of superconducting wire to generate a really powerful, large magnetic field,

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<v Speaker 3>an artificial magnetosphere, essentially like.

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<v Speaker 2>Earth's magnetic field, but generated by the spacecraft sort of.

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<v Speaker 3>Yes, And when the charged particles of the solar wind

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<v Speaker 3>hit this magnetic field.

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<v Speaker 2>They get deflected like how Earth's field deflects the solar

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<v Speaker 2>wind exactly.

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<v Speaker 3>That magnetic field pushes the plasma particles aside, and by

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<v Speaker 3>Newton's third law again, pushing the solar wind plasma away

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<v Speaker 3>pushes the spacecraft forward. You're essentially sailing on the solar

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<v Speaker 3>wind using a magnetic bubble.

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<v Speaker 2>That sounds incredibly cool, and it avoids the whole problem

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<v Speaker 2>of deploying and maintaining huge, fragile sheets of material.

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<v Speaker 3>That's a major theoretical advantage. Yes, No, worries about UV

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<v Speaker 3>degradation or micrometeoroid tears on a physical sale.

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<v Speaker 2>And because the solar wind doesn't drop off as quickly

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<v Speaker 2>as light pressure.

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<v Speaker 3>The potential acceleration profile, especially in the outer solar system,

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<v Speaker 3>could be much better than a solar sale, better performance,

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<v Speaker 3>potentially more durable.

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<v Speaker 2>Okay, sounds great. What's the catch? The review mentioned a

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<v Speaker 2>massive technological chasim ah.

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<v Speaker 3>Yes, the catch is well, it's the scale, the sheer

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<v Speaker 3>mind boggling scale required.

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<v Speaker 2>How big are we talking?

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<v Speaker 3>To generate a magnetic field strong enough and large enough

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<v Speaker 3>to effectively interact with the relatively low density solar wind,

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<v Speaker 3>especially far from the Sun, you need enormous superconducting.

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<v Speaker 2>Coils define enormous.

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<v Speaker 3>The review polling from technical studies suggests these superconducting loops

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<v Speaker 3>might need to be get ready for this up to

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<v Speaker 3>fifty kilometers in radius.

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<v Speaker 2>Wait kilometers fifty radius.

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<v Speaker 3>Fifty kilometer radius, meaning the whole structure the magnetic field

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<v Speaker 3>generator would be one hundred kilometers across once deployed.

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<v Speaker 2>One hundred kilometers. That's bigger than any structure we've ever

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<v Speaker 2>put in space by orders of magnitude. That's not a

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<v Speaker 2>spacecraft that's an orbiting installation.

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<v Speaker 3>We're heating on the core problem. The scale is just immense,

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<v Speaker 3>and that's only part one of the challenge. There's more

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<v Speaker 3>to get that magnetic field strength efficiently. The coils need

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<v Speaker 3>to be super conducting.

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<v Speaker 2>Meaning they have zero electrical resistance, but that only happens

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<v Speaker 2>when they're incredibly cold.

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<v Speaker 3>Exactly cryogenic temperatures. We're talking temperatures close to absolute zero.

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<v Speaker 2>So you have this one hundred kilometer wide structure made

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<v Speaker 2>of superconducting wire that needs to be kept freezing cold

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<v Speaker 2>in space where sunlight is still hitting it.

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<v Speaker 3>Yes, you need a massive, complex and incredibly reliable cryogenic

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<v Speaker 3>cooling system cryocolers running constantly for potentially decades.

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<v Speaker 2>The power requirements alone for that cooling system must be huge,

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<v Speaker 2>not to mention just building, launching, and deploying one hundred colimater.

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<v Speaker 3>Structure precisely, and the superconducting wire itself. It needs to

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<v Speaker 3>be structurally strong enough to handle the immense magnetic forces

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<v Speaker 3>trying to tear the coil apart while staying superconducting while

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<v Speaker 3>being lightweight. We'd need breakthroughs in material science just for

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<v Speaker 3>the wire.

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<v Speaker 2>So the technology to build the structure, deploy it power

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<v Speaker 2>the cooling maintain those temperatures reliably for years.

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<v Speaker 3>It simply doesn't exist yet, not even close. We're researching

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<v Speaker 3>things like high temperature superconductors or HTS, which could operate

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<v Speaker 3>it slightly warmer though still very cool temperatures, reducing the

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<v Speaker 3>cooling load a.

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<v Speaker 2>Bit, but still needing significant cool.

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<v Speaker 3>Well, absolutely compared to the ambient temperature of space. Even

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<v Speaker 3>HTS needs serious refrigeration, the power generation, the thermal management,

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<v Speaker 3>the deployment mechanisms for something that size. It puts mag

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<v Speaker 3>sales firmly in the far future breakthrough category. For now.

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<v Speaker 2>It's an incredible concept, but the engineering hurdles are just astronomical. Yeah, okay,

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<v Speaker 2>So if the magsail is yes, potentially too big, too heavy,

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<v Speaker 2>too complex with the cryogenics, is there a lighter way

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<v Speaker 2>to push against that solar wind?

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<v Speaker 3>Well, that's the thinking behind the next concept, electric sales

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<v Speaker 3>or E sales electric not magnetic.

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<v Speaker 2>How does that work?

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<v Speaker 3>E sales try to achieve a similar goal using the

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<v Speaker 3>solar wind, but with a different physical principle and hopefully

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<v Speaker 3>a much lighter structure. Instead of a magnetic field, they

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<v Speaker 3>use electric fields.

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<v Speaker 2>Okay, how do you make an electric field push things

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<v Speaker 2>in space.

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<v Speaker 3>The idea is to deploy a number of very long,

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<v Speaker 3>very thin conductive wires or tethers radially outwards from the spacecraft,

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00:16:34.000 --> 00:16:36.240
<v Speaker 3>maybe spun out using centrifugal.

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<v Speaker 2>Force kilometers long These.

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<v Speaker 3>Wire potentially tens of kilometers long, yes, but very lightweight.

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<v Speaker 3>Then you use an electron gun on board the spacecraft.

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<v Speaker 2>An electron gun what forour to.

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00:16:47.480 --> 00:16:50.480
<v Speaker 3>Shoot electrons away from the spacecraft and the tethers, leaving

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<v Speaker 3>the tethers with a strong positive electric charge, maybe thousands

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<v Speaker 3>of volts positive.

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<v Speaker 2>Ah. I see where this is going. The solar wind

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<v Speaker 2>is mostly positively charged protons.

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<v Speaker 3>Exactly like charges repel, So the positively charged tethers create

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<v Speaker 3>an electric field around them that repels the incoming positive

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<v Speaker 3>protons of the solar wind.

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<v Speaker 2>So you're pushing the solar wind away using electrostatics, not magnetism.

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<v Speaker 3>Precisely, and again Newton's third law means pushing the wind

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<v Speaker 3>away pushes the cell forward away from the Sun.

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<v Speaker 2>And the big advantage here is replacing those massive crygenic

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<v Speaker 2>superconducting coils with.

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00:17:25.680 --> 00:17:29.599
<v Speaker 3>Just long, thin wires and an electron gun, potentially a

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00:17:29.720 --> 00:17:32.920
<v Speaker 3>much much lighter system than a magsail. That's the main appeal.

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<v Speaker 3>Escaping some of that enormous mass and complexity.

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00:17:35.640 --> 00:17:38.640
<v Speaker 2>Sounds like a definite improvement in terms of mass, but

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00:17:38.720 --> 00:17:41.359
<v Speaker 2>the review probably points out new challenges too.

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00:17:41.720 --> 00:17:45.680
<v Speaker 3>No free lunch, No free lunch in space propulsion. Unfortunately, yeah,

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00:17:45.759 --> 00:17:48.519
<v Speaker 3>E sales swap one set of problems for another. The

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<v Speaker 3>review highlights issues with again materials and also power.

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00:17:52.799 --> 00:17:56.279
<v Speaker 2>Let's start with the materials. Kilometers of thin wires floating

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<v Speaker 2>in space sounds fragile.

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<v Speaker 3>They would be very thin, to say, mass very long

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<v Speaker 3>to create a large enough for pulseivaria. That makes them

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<v Speaker 3>incredibly vulnerable to micrometeoroids. Again space dust YEP, a single

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<v Speaker 3>hit probably wouldn't be catastrophic. The designs often involve multiple

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<v Speaker 3>tethers for redundancy, but cumulative damage over years from tiny

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<v Speaker 3>impacts could degrade the tethers, potentially sever them, or cause

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<v Speaker 3>oscillations that make navigation tricky. Maintaining the integrity of potentially

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00:18:23.319 --> 00:18:26.640
<v Speaker 3>hundreds of kilometers of deployed wire over decades is a

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00:18:26.759 --> 00:18:27.680
<v Speaker 3>huge challenge.

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00:18:27.799 --> 00:18:30.440
<v Speaker 2>Okay, so durability is one issue. What about power? You

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00:18:30.480 --> 00:18:31.759
<v Speaker 2>mentioned electron.

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00:18:31.319 --> 00:18:35.440
<v Speaker 3>Gun right, If mag sales need power for cryogenic cooling,

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00:18:35.799 --> 00:18:39.759
<v Speaker 3>E sales need continuous significant electrical power to run that

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00:18:39.839 --> 00:18:40.599
<v Speaker 3>electron gun.

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00:18:41.000 --> 00:18:44.359
<v Speaker 2>Why continuously don't you just charge the wires once?

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00:18:45.000 --> 00:18:48.240
<v Speaker 3>If only it were that simple. Space isn't a perfect vacuum.

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00:18:48.279 --> 00:18:52.720
<v Speaker 3>There's plasma everywhere. The electrons in the surrounding solar wind

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00:18:52.759 --> 00:18:55.640
<v Speaker 3>plasma are attracted to the positive tethers and will try

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00:18:55.680 --> 00:18:58.720
<v Speaker 3>to neutralize their charge. It's called plasma screening.

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00:18:58.839 --> 00:19:01.599
<v Speaker 2>So you're constantly fighting to keep the wires charged up.

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00:19:01.759 --> 00:19:04.960
<v Speaker 3>Exactly, you need to keep pumping electrons off the wires

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00:19:05.000 --> 00:19:08.000
<v Speaker 3>with the electron gun to maintain that high positive potential

391
00:19:08.039 --> 00:19:11.880
<v Speaker 3>against the surrounding plasma. That requires a pretty beefy power

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00:19:11.920 --> 00:19:15.960
<v Speaker 3>source multikilowatt level, running constantly, efficiently and reliably for the

393
00:19:16.119 --> 00:19:18.519
<v Speaker 3>entire mission duration potentially decades.

394
00:19:18.960 --> 00:19:21.799
<v Speaker 2>So you trade the mag sales challenge of huge scale

395
00:19:21.839 --> 00:19:24.920
<v Speaker 2>and cryo cooling for the E sales challenge of extreme

396
00:19:24.960 --> 00:19:27.279
<v Speaker 2>wire fragility and continuous high power generation.

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00:19:27.440 --> 00:19:30.000
<v Speaker 3>That's a good summary of the trade off. Yes, still

398
00:19:30.039 --> 00:19:35.000
<v Speaker 3>requires advanced materials, reliable long term power systems. Significant hurdles remain.

399
00:19:35.319 --> 00:19:38.319
<v Speaker 2>Okay, Wow, we've covered quite a range here, from the

400
00:19:38.359 --> 00:19:41.920
<v Speaker 2>tried and true gravity assist to light sales to these

401
00:19:41.920 --> 00:19:45.759
<v Speaker 2>more exotic magnetic and electric concepts pushing against the solar wind.

402
00:19:45.799 --> 00:19:48.599
<v Speaker 2>Let's try and break it all together. What's the synthesis here?

403
00:19:48.640 --> 00:19:51.680
<v Speaker 2>What does the review conclude when looking at all these options.

404
00:19:51.759 --> 00:19:54.720
<v Speaker 3>Well, when you lay them all out gravity assist, solar sale,

405
00:19:54.720 --> 00:19:58.400
<v Speaker 3>MAG sale, E sale, you see this clear spectrum. On

406
00:19:58.400 --> 00:20:02.119
<v Speaker 3>one end you have gravity assists proven working now but

407
00:20:02.400 --> 00:20:04.960
<v Speaker 3>totally inflexible. On the other end, you have mag sales

408
00:20:04.960 --> 00:20:08.640
<v Speaker 3>and E sales potentially much higher performance, especially for deep space,

409
00:20:08.880 --> 00:20:13.519
<v Speaker 3>but requiring technology that is frankly way beyond our current capabilities.

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00:20:13.559 --> 00:20:14.880
<v Speaker 3>Solar sales are somewhere in the middle.

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00:20:14.960 --> 00:20:17.839
<v Speaker 2>Let's quickly recap the killer limitation for each based on

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00:20:17.880 --> 00:20:18.240
<v Speaker 2>the review.

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00:20:18.319 --> 00:20:22.039
<v Speaker 3>Okay, gravity assists work great, but you're tied to rare

414
00:20:22.079 --> 00:20:24.799
<v Speaker 3>planetary alignments, no flexibility, no autonomy.

415
00:20:24.839 --> 00:20:29.240
<v Speaker 2>Solar sales proven concept, steady thrust near the Sun, but

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00:20:29.279 --> 00:20:32.480
<v Speaker 2>the materials are incredibly delicate and the thrust just dies

417
00:20:32.480 --> 00:20:34.920
<v Speaker 2>off way too fast with distance because of the inverse

418
00:20:34.960 --> 00:20:37.319
<v Speaker 2>square law useless for the outer solar system.

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00:20:37.359 --> 00:20:42.480
<v Speaker 3>Are beyond right, then mag sales great potential performance, avoids

420
00:20:42.519 --> 00:20:46.400
<v Speaker 3>material degradation, pushes against the solar wind further out, but

421
00:20:46.480 --> 00:20:50.160
<v Speaker 3>the showstopper is the scale those fifty kilometer radius superconducting

422
00:20:50.200 --> 00:20:54.559
<v Speaker 3>coils needing constant cryogenic cooling just not feasible today, and E.

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00:20:54.640 --> 00:20:57.240
<v Speaker 2>Sales lighter than mag sales, also uses the solar wind,

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00:20:57.680 --> 00:21:01.200
<v Speaker 2>but you trade the massive coils for potentially fragile kilometers

425
00:21:01.240 --> 00:21:04.680
<v Speaker 2>long tethers and the need for continuous high power electron

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00:21:04.720 --> 00:21:08.720
<v Speaker 2>guns to keep them charged. Still big tech hurdles exactly.

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00:21:08.880 --> 00:21:11.680
<v Speaker 3>So the big conclusion from the review, looking across all

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00:21:11.720 --> 00:21:11.960
<v Speaker 3>of this.

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00:21:12.200 --> 00:21:14.279
<v Speaker 2>What does it all mean for actually getting out there?

430
00:21:14.480 --> 00:21:18.680
<v Speaker 3>It means there's no silver bullet, No single propellantless method

431
00:21:18.799 --> 00:21:21.359
<v Speaker 3>solves all the problems right now. Each one has a

432
00:21:21.400 --> 00:21:25.200
<v Speaker 3>critical flaw, whether it's flexibility, fragility, distance limits, or just

433
00:21:25.240 --> 00:21:27.680
<v Speaker 3>requiring currently non existent technology.

434
00:21:27.920 --> 00:21:30.359
<v Speaker 2>So the path forward probably isn't picking just one winner.

435
00:21:30.799 --> 00:21:34.119
<v Speaker 3>Very unlikely. The review strongly suggests the future probably lies

436
00:21:34.160 --> 00:21:37.519
<v Speaker 3>in combining these approaches. Maybe use a powerful launch stage,

437
00:21:37.559 --> 00:21:40.279
<v Speaker 3>then a solar sale to get good initial acceleration out

438
00:21:40.319 --> 00:21:41.960
<v Speaker 3>of the inner solar system, and.

439
00:21:41.920 --> 00:21:45.359
<v Speaker 2>Then maybe deploy an E sale or mag sale once

440
00:21:45.400 --> 00:21:49.160
<v Speaker 2>a solar cell becomes ineffective to continue accelerating using the

441
00:21:49.200 --> 00:21:49.759
<v Speaker 2>solar wind.

442
00:21:50.000 --> 00:21:54.359
<v Speaker 3>Something like that, or using gravity assists strategically in combination

443
00:21:54.480 --> 00:21:59.279
<v Speaker 3>with continuous low thrust propulsion, hybrid approaches seem much more

444
00:21:59.319 --> 00:22:02.519
<v Speaker 3>plausible than relying on a single magic solution, and.

445
00:22:02.440 --> 00:22:08.480
<v Speaker 2>That idea needing these advanced propellantless methods, perhaps in combination,

446
00:22:08.640 --> 00:22:11.839
<v Speaker 2>becomes absolutely critical when we talk about the really big goals,

447
00:22:11.880 --> 00:22:13.720
<v Speaker 2>doesn't it, Yeah, interstellar travel.

448
00:22:13.880 --> 00:22:17.680
<v Speaker 3>It's non negotiable for interstellar really. The review hammers this home.

449
00:22:17.799 --> 00:22:20.519
<v Speaker 3>If you're serious about reaching another star system within a

450
00:22:20.599 --> 00:22:24.319
<v Speaker 3>human lifetime or even a couple of centuries, chemical rockets

451
00:22:24.400 --> 00:22:28.000
<v Speaker 3>just won't cut it. Because of that Silkovski mass ratio limit.

452
00:22:28.279 --> 00:22:29.720
<v Speaker 2>You simply can't carry enough fuel.

453
00:22:29.799 --> 00:22:32.319
<v Speaker 3>You can't, So leaving the propellant behind isn't just a

454
00:22:32.400 --> 00:22:34.960
<v Speaker 3>nice to have for interstellar missions, it's probably the only

455
00:22:35.000 --> 00:22:38.720
<v Speaker 3>way it could ever be feasible. It fundamentally changes the challenge.

456
00:22:38.319 --> 00:22:41.359
<v Speaker 2>From a challenge of energy storage fuel to a challenge

457
00:22:41.400 --> 00:22:43.720
<v Speaker 2>of energy harvesting light, wind, gravity.

458
00:22:43.880 --> 00:22:47.759
<v Speaker 3>Perfectly put, it becomes about building incredibly efficient, large scale

459
00:22:47.960 --> 00:22:52.240
<v Speaker 3>energy harvesting structures that can operate reliably for centuries.

460
00:22:51.799 --> 00:22:56.200
<v Speaker 2>Which suddenly makes those huge engineering hurdles. The fifty kilometer coils,

461
00:22:56.599 --> 00:23:00.799
<v Speaker 2>the super durable tethers. The decades long power sources seem

462
00:23:00.880 --> 00:23:03.039
<v Speaker 2>less like science fiction pipe dreams.

463
00:23:02.839 --> 00:23:05.359
<v Speaker 3>And more like the necessary entry ticket. They define the

464
00:23:05.359 --> 00:23:07.839
<v Speaker 3>scale of engineering required if we actually want to become

465
00:23:07.920 --> 00:23:12.039
<v Speaker 3>an interstellar species. It's less about building slightly better rockets

466
00:23:12.079 --> 00:23:15.279
<v Speaker 3>and more about inventing fundamentally new ways to build and

467
00:23:15.400 --> 00:23:16.559
<v Speaker 3>power things in space.

468
00:23:17.079 --> 00:23:20.880
<v Speaker 2>This has been a really fascinating journey breaking free conceptually,

469
00:23:20.920 --> 00:23:23.519
<v Speaker 2>at least from the tyranny of the rocket equation. We've

470
00:23:23.519 --> 00:23:27.400
<v Speaker 2>looked at gravity assists, solar sales, magnetic sales, electric sales,

471
00:23:28.119 --> 00:23:33.400
<v Speaker 2>each with its promise and its major roadblocks, flexibility, materials, scale, power.

472
00:23:33.039 --> 00:23:35.559
<v Speaker 3>And maybe as we wrap up, it's worth focusing on

473
00:23:35.599 --> 00:23:40.000
<v Speaker 3>that biggest technological gap, the mag sale scale. For instance,

474
00:23:40.559 --> 00:23:44.200
<v Speaker 3>if we accept that something like a fifty kilometer superconducting

475
00:23:44.240 --> 00:23:48.440
<v Speaker 3>structure kept near absolute zero for decades might be what

476
00:23:48.519 --> 00:23:52.519
<v Speaker 3>it takes for truly fast deep space or interstellar travel,

477
00:23:53.759 --> 00:23:56.440
<v Speaker 3>pose is a really interesting question for you, the listener,

478
00:23:56.480 --> 00:23:59.200
<v Speaker 3>to think about. Go on, what kind of fundamental science

479
00:23:59.279 --> 00:24:01.880
<v Speaker 3>needs to be discovered first before we can even think

480
00:24:01.880 --> 00:24:06.839
<v Speaker 3>about designing the propulsion system. What breakthrough in say, material science,

481
00:24:06.880 --> 00:24:11.079
<v Speaker 3>may be practical room temperature superconductors or in compact ultralong

482
00:24:11.119 --> 00:24:14.720
<v Speaker 3>life power generation, maybe fusion power plants small enough for spacecraft.

483
00:24:15.279 --> 00:24:17.480
<v Speaker 3>What needs to happen in the lab before the engineers

484
00:24:17.480 --> 00:24:20.359
<v Speaker 3>can even start drawing up the blueprints for these proportion systems.

485
00:24:20.400 --> 00:24:22.200
<v Speaker 2>It's a great point. We might not just be waiting

486
00:24:22.240 --> 00:24:24.920
<v Speaker 2>for better engineering. We might be waiting for a whole

487
00:24:25.000 --> 00:24:28.359
<v Speaker 2>new piece of physics or material science to unlock the

488
00:24:28.440 --> 00:24:31.480
<v Speaker 2>path forward, the invention that enables.

489
00:24:31.160 --> 00:24:35.559
<v Speaker 3>The invention exactly. The next leap in propulsion might start

490
00:24:35.680 --> 00:24:38.960
<v Speaker 3>not in a rocket factory, but maybe with a discovery

491
00:24:39.039 --> 00:24:42.720
<v Speaker 3>in condensed matter physics or advanced energy research. It really

492
00:24:42.720 --> 00:24:45.000
<v Speaker 3>shifts your perspective on where the bottleneck lies.

493
00:24:45.200 --> 00:24:48.240
<v Speaker 2>A powerful thought. Indeed, we need the science before we

494
00:24:48.279 --> 00:24:51.279
<v Speaker 2>can build the sales to truly navigate the void. Thank

495
00:24:51.279 --> 00:24:53.200
<v Speaker 2>you for joining us on this deep dive into leaving

496
00:24:53.200 --> 00:25:03.720
<v Speaker 2>the fuel behind U

497
00:25:09.680 --> 00:25:25.000
<v Speaker 3>S S
