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>I really want you to just take a moment right

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<v Speaker 2>now and picture the moon. And I don't mean a

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<v Speaker 2>high resolution photograph from some astronomy textbook, but the actual

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<v Speaker 2>moon you see when you step outside on a clear

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<v Speaker 2>night and just look up.

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<v Speaker 3>Right, just that familiar glowing sphere we all.

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<v Speaker 2>Know exactly to the naked eye. It's just this well,

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<v Speaker 2>this glowing cratered ball. It's undeniably beautiful, but it also

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<v Speaker 2>looks like a completely dead, dusty rock, just sort of

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<v Speaker 2>floating in the cold void.

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<v Speaker 3>Yeah, and I mean humanity has grown up with that

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<v Speaker 3>exact same image. Yeah, for tens of thousands of years,

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<v Speaker 3>we look up and we basically just see a monochrome desert.

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<v Speaker 2>We do. But okay, what if you could put on

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<v Speaker 2>a pair of magic glasses. What if the second you

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<v Speaker 2>slip those glasses on that pale gray rock completely transformed.

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<v Speaker 3>Oh I love this analogy. It's like flipping a switch

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<v Speaker 3>on the universe.

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<v Speaker 2>Right Suddenly you know you aren't looking at a lifeless

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<v Speaker 2>desert anymore. You're looking at this vibrant neon glowing map

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<v Speaker 2>of hidden chemical elements spreading all across the lunar surface.

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<v Speaker 3>You'd see pockets of brilliant blues, sweeping streaks of radiant reds,

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<v Speaker 3>deep pools of vivid greens.

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<v Speaker 2>Yeah, exactly, you would be seeing the actual chemical makeup

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<v Speaker 2>of the Moon glowing in real time. It would completely

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<v Speaker 2>rewrite our understanding of our closest celestial neighbor.

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<v Speaker 3>It's an absolutely stunning visual to imagine it really is.

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<v Speaker 3>What is truly incredible about where we stand right now

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<v Speaker 3>in astrophysics is that we are no longer confined to

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<v Speaker 3>just imagining it.

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<v Speaker 2>We're building them.

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<v Speaker 3>Yes, we are actively building those magic glasses.

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<v Speaker 2>And that is the massive breakthrough we are getting into

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<v Speaker 2>today because a team of researchers at Tokyo Metropolitan University,

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<v Speaker 2>specifically led by Ori Tida and Professor Yuchiro Izoe, have

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<v Speaker 2>developed something that frankly feels like it belongs in a

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<v Speaker 2>sci fi.

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<v Speaker 3>Novel, it really does. It sounds like pure science.

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<v Speaker 2>Fiction, but it's real. They have created this highly compact

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<v Speaker 2>X ray telescope that is capable of giving humanity its

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<v Speaker 2>very first complete, comprehensive chemical map of the lunar surface.

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<v Speaker 3>And we really need to establish the stakes here right away.

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<v Speaker 3>This effort. It's not about capturing prettier, more colorful pictures

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<v Speaker 3>of the Moon to just hang in a gallery or

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<v Speaker 3>put on a magazine.

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<v Speaker 2>Cover, right, It's not just for the aesthetics.

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<v Speaker 3>Not at all. We are looking at a fundamental paradigm

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<v Speaker 3>shift in space exploration. This specific technology is going to

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<v Speaker 3>completely change how we understand the Moon's deep, violent geological history.

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<v Speaker 2>Which is fascinating on its own. But there's a practical

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<v Speaker 2>side too, right.

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<v Speaker 3>Oh, massively practical, perhaps even more importantly for our lifetime.

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<v Speaker 3>The data this telescope gathers is going to literally dictate

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<v Speaker 3>the Moon's potential to support human life in the very

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<v Speaker 3>near future.

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<v Speaker 2>Okay, So let's unpack this a bit because whenever someone

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<v Speaker 2>says X ray telescope, my mind immediately goes to these massive,

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<v Speaker 2>multi billion dollar orbital observatories.

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<v Speaker 3>Oh sure, like Chandra or XMM Newton. Yeah, the giants.

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<v Speaker 2>I'm picturing these instruments that are the size of a

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<v Speaker 2>school bus, requiring the largest rockets we have just to

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<v Speaker 2>get them off the ground. How can a single university

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<v Speaker 2>team be building something that maps the entire Moon? Are

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<v Speaker 2>we talking about sending a massive new space station into

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<v Speaker 2>lunar orbit?

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<v Speaker 3>That is the crucial engineering hurdle that makes this breakthrough

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<v Speaker 3>so significant. If you know anything about the history of

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<v Speaker 3>X ray astronomy, you know that traditional X ray telescopes

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<v Speaker 3>are notoriously massive.

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<v Speaker 2>They're huge.

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<v Speaker 3>They are some of the heaviest, most cumbersome instruments humanity

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<v Speaker 3>is ever put into space. And there is a very specific,

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<v Speaker 3>unforgiving physical reason for that bulk. You can't just shrink

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<v Speaker 3>them normally.

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<v Speaker 2>Right. It has to do with how X rays behave

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<v Speaker 2>compared to normal visible light, Because I know that if

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<v Speaker 2>I take a standard telescope mirror like the kind you

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<v Speaker 2>might have in your backyard to look at Jupiter, and

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<v Speaker 2>I try to point it at an X ray source,

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<v Speaker 2>it just doesn't work.

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<v Speaker 3>It doesn't work at all. It's useless.

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<v Speaker 2>Why is that? Why doesn't it reflect?

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<v Speaker 3>Because X rays are incredibly high energy photons They carry

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<v Speaker 3>so much energy, and their wavelengths are so incredibly short

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<v Speaker 3>that if you fire an X ray at a standard

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<v Speaker 3>curved optical mirror, it will not bounce off the surface

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<v Speaker 3>and focus into an eyepiece like normal light does.

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<v Speaker 2>So what does it do? Does it just break the mirror?

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<v Speaker 3>Well, it will either be completely absorbed by the mirror's

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<v Speaker 3>material or it will just blast right through it, almost

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<v Speaker 3>like the mirror wasn't even there.

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<v Speaker 2>Oh wow, So I'm imagining like trying to bounce a

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<v Speaker 2>tennis ball off a wall. A tennis ball bounces easily.

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<v Speaker 2>That's our visible light. But an X ray is like

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<v Speaker 2>firing a high caliber bullet at a piece of tissue paper.

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<v Speaker 3>That is a fantastic analogy. Yes, the tissue or doesn't

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<v Speaker 3>stand a chance of deflecting that bullet. It just punches

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<v Speaker 3>a hole straight through.

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<v Speaker 2>So how do you fix that? How do you catch

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<v Speaker 2>a bullet with a mirror.

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<v Speaker 3>Well, because of that penetrating power, astronomers in the mid

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<v Speaker 3>twentieth century had to completely reinvent how a telescope even works.

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<v Speaker 3>In order to capture X rays. They had to vent

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<v Speaker 3>something called grazing incidents.

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<v Speaker 2>Mirror the raising incidents. Okay, I think I know where

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<v Speaker 2>this is going. But break down the physics for me.

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<v Speaker 2>How do you force a high energy bullet to actually bounce?

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<v Speaker 3>You have to change the angle. Think about the angle

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<v Speaker 3>of attack. Imagine you're standing on the shore of a

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<v Speaker 3>completely calm lake. If you take a heavy stone and

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<v Speaker 3>throw it straight down into the water, what happens?

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<v Speaker 2>It just violently breaks the surface and sinks immediately exactly.

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<v Speaker 3>That is our X ray hitting a standard mirror head on.

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<v Speaker 3>But if you take that exact same stone, crouch down

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<v Speaker 3>low and throw it at a very shallow, almost parallel

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<v Speaker 3>angle to the.

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<v Speaker 2>Water, Oh, it skips. It skips across the surfer right.

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<v Speaker 3>It skips Even though water is soft and the stone

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<v Speaker 3>is heavy. The extreme shallow angle forces the stone to

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<v Speaker 3>deflect grazing incidence. Mirrors work on that exact same principle.

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<v Speaker 2>So instead of a dish that faces the target directly,

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<v Speaker 2>like a satellite dish on a house, what does it

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<v Speaker 2>look like?

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<v Speaker 3>X ray mirrors are shaped like long, hollow cylinders, and

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<v Speaker 3>they're often nested one inside the other, kind of like

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<v Speaker 3>Russian nesting dolls.

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<v Speaker 2>Wait, hollow cylinders, how does the light get in?

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<v Speaker 3>The incoming X rays enter the open top of the cylinder,

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<v Speaker 3>and because the walls are angled, it's just a fraction

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<v Speaker 3>of a degree. The X rays skip off the ultra

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<v Speaker 3>smooth inside surface like the stone on the pond precisely.

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<v Speaker 3>They skip and skip, and they are slowly funneled down

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<v Speaker 3>a long tube until they hit a detector at the

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<v Speaker 3>far end.

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<v Speaker 2>I see the problem immediately, though. To skip an X

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<v Speaker 2>ray down a tube and actually bring it to a

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<v Speaker 2>focused point, that too has to be incredibly long.

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<v Speaker 3>It has to be immensely long. The focal lengths required

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<v Speaker 3>to gently guide these high energy photons requires so much

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<v Speaker 3>physical space, so the telescope ends up being ten, ten, fifteen,

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<v Speaker 3>or even twenty meters long.

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<v Speaker 2>That's the size of a building it is.

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<v Speaker 3>And they are incredibly heavy due to the layers of

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<v Speaker 3>dense metal required to make those nested cylindrical mirrors, which

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<v Speaker 3>means they are astronomically expensive to launch.

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<v Speaker 2>So if you want to put a massive X ray

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<v Speaker 2>observatory into orbit around the Earth, you put it on

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<v Speaker 2>top of a heavy lip rocket, blast it into low

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<v Speaker 2>Earth orbit, and you just leave it there. And we've

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<v Speaker 2>done that.

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<v Speaker 3>We have. It takes massive resources, but we do it.

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<v Speaker 2>But sending something that huge all the way to the Moon.

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<v Speaker 2>I mean, that's a completely different mathematical universe, isn't it.

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<v Speaker 3>It is an absolute logistical nightmare. Launching a massive payload

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<v Speaker 3>from Earth's surface is hard enough. But pushing a school

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<v Speaker 3>bus sized instrument across the quarter million miles to.

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<v Speaker 2>The Moon, Yeah, that takes so much fuel.

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<v Speaker 3>And not just to get it there. You have to

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<v Speaker 3>carry enough heavy rocket fuel to physically slow that massive

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<v Speaker 3>object down once it arrives, so it doesn't just fly

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<v Speaker 3>right past the Moon into deep space. Oh right, You

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<v Speaker 3>have to hit the brakes exactly. The fuel requirements alone

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<v Speaker 3>for lunar orbit insertion of traditional X ray observatory would

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<v Speaker 3>bankrupt most space agencies. It's just not feasible, which.

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<v Speaker 2>Brings us directly to the core of the Tokyo Metropolitan

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<v Speaker 2>University breakthrough. If traditional telescopes are heavy, long, and basically

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<v Speaker 2>impossible to maneuver into a tight lunar orbit, what did

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<v Speaker 2>Touda and Eazoe actually build.

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<v Speaker 3>They built a telescope that completely upends those traditional engineering constraints.

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<v Speaker 3>The instrument they've designed is not weigh thousands of kilograms.

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<v Speaker 3>The entire sensor payload weighs less than ten kilogram.

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<v Speaker 2>Wall, I need to stop you their ten kilograms.

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<v Speaker 3>Less than ten kilograms? Yes, this is.

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<v Speaker 2>Roughly the weight of a medium sized dog, or like

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<v Speaker 2>a couple of bags of groceries. How is it physically

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<v Speaker 2>possible to replace a twenty meter long, multi ton orbital

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<v Speaker 2>observatory with something I could carry on too an airplane

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<v Speaker 2>as hand luggage.

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<v Speaker 3>It sounds impossible.

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<v Speaker 2>I know what is the catch here? Because you know

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<v Speaker 2>in physics you can't shoot the rules. There is always

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<v Speaker 2>a catch.

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<v Speaker 3>It's the exact right question to ask. You cannot cheat physics.

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<v Speaker 3>The high energy nature of X rays hasn't magically changed.

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<v Speaker 3>What is fascinating here is that the catch isn't a

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<v Speaker 3>loss of precision or some magical new element.

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<v Speaker 2>So what is it?

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<v Speaker 3>It is a brilliant, radical change in engineering strategy. And

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<v Speaker 3>to understand that strategy we actually have to look at

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<v Speaker 3>where this technology was born, because this ultra lightweight telescope

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<v Speaker 3>was not originally invented to look at the Moon at all.

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<v Speaker 2>Really, what was it for?

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<v Speaker 3>It was initially developed to study Earth's magnetosphere.

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<v Speaker 2>So this entire lunar mapping project is actually a pivot

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<v Speaker 2>from a totally different mission.

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<v Speaker 3>A magnificent opportunistic pivot.

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<v Speaker 2>Yes.

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<v Speaker 3>For years, researchers have been trying to figure out how

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<v Speaker 3>to put highly sensitive, extremely lightweight X ray detectors into

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<v Speaker 3>orbit around.

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<v Speaker 2>Earth to monitor what exactly.

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<v Speaker 3>A monitor how the violent solar wind interacts with our

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<v Speaker 3>planet's magnetic shield. They needed an instrument that was nimble,

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<v Speaker 3>something that could be launched cheaply in large clusters.

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<v Speaker 2>Uh okay, So they needed something small, right.

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<v Speaker 3>So material scientists and astrophysicists collaborated and they developed something

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<v Speaker 3>called micropoor optics.

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<v Speaker 2>Micropoor optics, Okay, I'm guessing micromeans. We are shrinking those

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<v Speaker 2>giant skipping stones cylinders down, but how do you shrink

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<v Speaker 2>a twenty meter telescope mirror?

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<v Speaker 3>You basically replace those massive, heavy nested metal cylinders with

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<v Speaker 3>incredibly thin, lightweight plates. Imagine a plate made of advanced

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<v Speaker 3>silicon or glass that is absolutely riddled with microscopic.

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<v Speaker 2>Holes like a sponge kind of.

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<v Speaker 3>But much more structured. These aren't just random round holes

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<v Speaker 3>drilled into a plate. They are perfectly structured microscopic square pores.

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<v Speaker 2>I am struggling to visualize this a bit. Why square

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<v Speaker 2>pores and how small are we actually talking.

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<v Speaker 3>We are talking about pores that are fractions of a

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<v Speaker 3>millimeter wide, tiny, and the reason they are square is

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<v Speaker 3>critical to the physics of focusing the X ray.

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<v Speaker 2>How does the square shape help focus it?

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<v Speaker 3>Well? When an X ray enters a microscopic square poor,

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<v Speaker 3>it skips off the flat internal walls of that tiny tunnel.

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<v Speaker 3>By having a square geometry, the X ray can reflect

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<v Speaker 3>off two adjacent walls in sequence.

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<v Speaker 2>So it hits like the top wall and then immediately

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<v Speaker 2>hits the sidewall exactly.

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<v Speaker 3>This double reflection inside the microscopic pore mimics the exact

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<v Speaker 3>same shallow grazing incidents funneling effect of the giant metal

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<v Speaker 3>cylinders we talked about earlier.

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<v Speaker 2>Oh, but it accomplishes it in a fraction of the distance.

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<v Speaker 3>Yes, you get the exact same skipping stone effect, but

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<v Speaker 3>shrunk down to the microscopic level.

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<v Speaker 2>So instead of one giant tube slowly funneling a photon

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<v Speaker 2>over twenty meters, you have millions of microscopic square tubes

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<v Speaker 2>rapidly funneling millions of photons over a distance of just

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<v Speaker 2>a few centimeters.

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<v Speaker 3>That is the exact mechanism. You're replacing brute force mass

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<v Speaker 3>with hyper engineer geometry. The X rays skip through these

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<v Speaker 3>microscopic pores just like they do through the giant orbital observatories,

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<v Speaker 3>but the whole apparatus is shrunk down.

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<v Speaker 2>And so the weight drops from tons to kilograms.

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<v Speaker 3>Precisely from a school bus to a bag of groceries.

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<v Speaker 2>It sounds so Sima went to the evolution of computing.

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<v Speaker 2>To me, like moving from those giant room size vacuum

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<v Speaker 2>tube computers of the nineteen fifties down to a modern

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<v Speaker 2>silicon microchip.

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<v Speaker 3>That is a very solid parallel. You aren't changing the

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<v Speaker 3>fundamental math of computing, or in this case, the physics

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<v Speaker 3>of X rays. You are just miniaturizing the physical architecture

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<v Speaker 3>that performs the task.

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<v Speaker 2>That's brilliant.

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<v Speaker 3>And when the team at TMU, led by Toyta and Ezoi,

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<v Speaker 3>look at the performance specifications of this micro poor technology,

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<v Speaker 3>they realize something profound.

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<v Speaker 2>They realized it was perfect for.

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<v Speaker 3>The Moon exactly. They realized they were holding the perfect

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<v Speaker 3>tool for a lunar orbital mission. But the brilliance of

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<v Speaker 3>their proposal doesn't stop it just sending one of these

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<v Speaker 3>small telescopes to the Moon.

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<v Speaker 2>What do you mean They're sending more than one.

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<v Speaker 3>Because the individual units are so incredibly lightweight and small,

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<v Speaker 3>A single lunar orbiting satellite doesn't have to carry just

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<v Speaker 3>one sensor. It can carry a grid of them.

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<v Speaker 2>Oh, they're packing multiples onto one satellite.

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<v Speaker 3>Specifically, they have designed the system that utilizes a five

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<v Speaker 3>y five array. That's twenty five individual micropoor X ray

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<v Speaker 3>telescopes all mounted together on a single lightweight orbital platform.

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<v Speaker 2>I love the elegance of this concept. If you have

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<v Speaker 2>a ten kilogram sensor, you don't just celebrate that it's

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<v Speaker 2>light and launch one. You take advantage of that weight

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<v Speaker 2>savings to multiply your observational Pathwer.

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<v Speaker 3>Absolutely, it's incredibly efficient.

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<v Speaker 2>It immediately reminds me of the compound eye of a fly.

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<v Speaker 2>Oh how so well, a human eye is essentially one

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<v Speaker 2>massive lens trying to take in a wide field of view.

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<v Speaker 2>But a fly doesn't have the space or mass for

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<v Speaker 2>a giant, heavy eye, so nature gave it thousands of tiny,

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<v Speaker 2>highly efficient individual lenses. Right omatidia, right, the little facets. Yeah,

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<v Speaker 2>each one captures a tiny sliver of light, but when

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<v Speaker 2>the fly's brain stitches all those slivers together, it gets

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<v Speaker 2>this massive, wide angle, highly sensitive view of its entire environment.

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<v Speaker 2>The five x five array is basically a mechanical compound.

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<v Speaker 3>Eye that analogy hits the nail right on the head.

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<v Speaker 3>By utilizing a five y five array of micropoor telescopes,

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<v Speaker 3>the TMU team is exponentially compounding the power of the.

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<v Speaker 2>Instrument, because if you only had one, you'd just be

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<v Speaker 2>looking through a straw.

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<v Speaker 3>Exactly, if you only had one small telescope in lunar orbit,

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<v Speaker 3>you w'ud be looking at a tiny pinprick of the

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<v Speaker 3>lunar regolith at any given moment. You would take millennia

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<v Speaker 3>to map the whole surface.

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<v Speaker 2>But with the array.

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<v Speaker 3>With the array, you are sweeping a massive, wide net

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<v Speaker 3>across the regolith. As the satellite orbits, you dramatically increase

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<v Speaker 3>the coverage area and the overall speed of data collection.

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<v Speaker 2>So the catch I asked about earlier really isn't a

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<v Speaker 2>compromise in the quality of the science at all. It

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<v Speaker 2>is just a completely different engineering philosophy.

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<v Speaker 3>Precisely, instead of building one giant, heavy ducat to catch

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<v Speaker 3>X ray slowly, we are casting a wide net of tiny,

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<v Speaker 3>hyper efficient buckets to catch them rapidly.

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<v Speaker 2>We are utilizing a smart, distributed geometric design rather than

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<v Speaker 2>brew force physical mass. I love that, but we have

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<v Speaker 2>to remember the design of the telescope array itself is

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<v Speaker 2>only half of the equation, right right.

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<v Speaker 3>The telescope is just a passive receiver.

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<v Speaker 2>It is essentially just a very fancy camera lens sitting

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<v Speaker 2>in the dark. To understand how we can actually map

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<v Speaker 2>the chemical elements of the Moon, we need to understand

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<v Speaker 2>the source of the signal. We need a flash of light.

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<v Speaker 3>Yes, because this telescope isn't shooting X rays down at

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<v Speaker 3>the Moon like a radar dish.

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<v Speaker 2>It's waiting for something to happen.

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<v Speaker 3>It is, and that's something is an incredibly violent interaction

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<v Speaker 3>between the Moon and the Sun.

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<v Speaker 2>Let's dive into the cosmic physics here. Specifically, this mechanism

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<v Speaker 2>called X ray fluorescence because this is the cool part oh.

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<v Speaker 3>X ray fluorescence or XRF, is one of the most

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<v Speaker 3>elegant and reliable mechanisms in all of astrophysics. It is

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<v Speaker 3>the core physical process that makes this entire mission possible.

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<v Speaker 2>Okay, so how does it work? How does XRF let

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<v Speaker 2>us map a giant rock?

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<v Speaker 3>Well, to truly grasp how it allows us to map

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<v Speaker 3>a celestial body, we actually need to zoom all the

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<v Speaker 3>way down to the microscopic atomic level. Think about the

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<v Speaker 3>lunar surface.

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<v Speaker 2>Okay, the dirt, the rocks.

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<v Speaker 3>Every rock, every boulder, every single grain of that fine

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<v Speaker 3>abrasive dust we call regolith is made of atoms. You

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<v Speaker 3>have oxygen, magnesium, aluminum, silicon, iron.

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<v Speaker 2>The fundamental building blocks of planetary geology.

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<v Speaker 3>Correct and in a normal, calm state, these atoms are

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<v Speaker 3>just sitting there on the lunar surface doing nothing to

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<v Speaker 3>an X ray telescope. They are completely dark. They're not

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<v Speaker 3>emitting any high energy radiation on their own.

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<v Speaker 2>So the telescope would just see pitch black exactly.

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<v Speaker 3>But our Sun is not a calm, quiet neighbor. The

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<v Speaker 3>Sun is a raging, churning, violently magnetic ball of superheated plasma.

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<v Speaker 2>It's basically a continuous explosion, and due.

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<v Speaker 3>To the complex twisting of its magnetic fields, it frequently

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<v Speaker 3>unleashes intense solar flares.

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<v Speaker 2>These flares are massive eruptions, right like billions of megatons

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<v Speaker 2>of energy just snapping and exploding outward into the solar system.

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<v Speaker 3>Yes, magnetic reconnection of and during these events, the Sun

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<v Speaker 3>throws massive amounts of extremely high energy X rays out

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<v Speaker 3>into the void of space, traveling outward at the speed

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<v Speaker 3>of light.

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<v Speaker 2>I am really trying to picture the sheer scale of this.

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<v Speaker 2>The Sun erupts and this wave of invisible high energy

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<v Speaker 2>X rays washes over the entire inner Solar system.

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<v Speaker 3>It's a cosmic tsunami of radiation.

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<v Speaker 2>But here on Earth we don't really notice when a

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<v Speaker 2>solar flares X rays hit us, unless we are looking

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<v Speaker 2>at specific atmospheric phenomena like the auroras or monitoring satellite interference.

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00:17:32.400 --> 00:17:33.960
<v Speaker 2>Why is that? Why don't we get cooked?

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<v Speaker 3>Because Earth has armor, We have a remarkably thick, dense atmosphere,

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<v Speaker 3>and we have a powerful global magnetic field generated by

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<v Speaker 3>our planet's spinning molten core, our shield. Right when those

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<v Speaker 3>high energy solar X rays hit Earth, our atmosphere absorbs

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<v Speaker 3>and scatters them long before they ever reach the surface.

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<v Speaker 3>That atmospheric shield is the only reason complex life can

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<v Speaker 3>exist down here.

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<v Speaker 2>The Moon doesn't have that. The Moon has no atmosphere

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<v Speaker 2>at all, just the hard vacuum of space right down

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<v Speaker 2>to the dirt.

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<v Speaker 3>None, and it has no active global magnetic field. It

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<v Speaker 3>is completely naked and exposed.

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<v Speaker 2>So when that wave hits and.

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<v Speaker 3>The solar flare erupts those high energy X rays from

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<v Speaker 3>the Sun slam unimpeded, directly into the raw, exposed lunar regolith.

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<v Speaker 2>Okay, here's where I really need you to explain the

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<v Speaker 2>quantum mechanics of this, because it sounds like magic if

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<v Speaker 2>we don't break it down. What actually happens when a

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<v Speaker 2>high energy solar X ray traveling at the speed of

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<v Speaker 2>light slams into a single atom of say aluminum, sitting

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<v Speaker 2>quietly on the lunar surface.

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00:18:35.240 --> 00:18:37.000
<v Speaker 3>It's a violent microscopic collision.

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00:18:37.079 --> 00:18:39.839
<v Speaker 2>Does the atom just absorb the heat? Does it shatter?

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00:18:39.960 --> 00:18:40.599
<v Speaker 2>What happens?

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00:18:40.680 --> 00:18:43.960
<v Speaker 3>It triggers a very specific atomic reaction. Think of the

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00:18:44.000 --> 00:18:47.000
<v Speaker 3>aluminum atom as a miniature solar system. You have it

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00:18:47.240 --> 00:18:50.319
<v Speaker 3>dense nucleus in the center, and you have electrons orbiting

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00:18:50.400 --> 00:18:51.960
<v Speaker 3>around it in different shells.

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<v Speaker 2>Or energy level like planets around the Sun.

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<v Speaker 3>Exactly now, the incoming solar X ray essentially acts like

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<v Speaker 3>an unimaginably fat microscopic cubeall on a billiard table. It

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<v Speaker 3>smashes into the aluminum atom with so much energy that

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<v Speaker 3>it completely bypasses the outer electrons and strikes one of

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00:19:09.160 --> 00:19:10.680
<v Speaker 3>the atom's innermost electrons.

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00:19:10.839 --> 00:19:12.119
<v Speaker 2>It goes straight for the inner shell.

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00:19:12.240 --> 00:19:14.920
<v Speaker 3>It does, it transfers its energy and knocks that inter

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00:19:14.960 --> 00:19:17.720
<v Speaker 3>electron completely out of its orbit and ejects it from

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00:19:17.720 --> 00:19:18.640
<v Speaker 3>the atom entirely.

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00:19:19.000 --> 00:19:22.000
<v Speaker 2>Wow. So the atom has just been violently assaulted by

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00:19:22.000 --> 00:19:23.960
<v Speaker 2>this X ray. It has a gaping hole in its

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00:19:23.960 --> 00:19:27.000
<v Speaker 2>innermost shell. Now I imagine the atom doesn't like being

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00:19:27.000 --> 00:19:27.559
<v Speaker 2>in that state.

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00:19:27.799 --> 00:19:31.720
<v Speaker 3>It absolutely does not. In quantum mechanics, systems always seek

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00:19:31.759 --> 00:19:35.519
<v Speaker 3>their lowest, most stable energy state. An atom with a

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00:19:35.559 --> 00:19:39.240
<v Speaker 3>missing inter electron is highly unstable. It is in what

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00:19:39.279 --> 00:19:42.119
<v Speaker 3>we call an excited state. It wants to fix itself

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00:19:42.279 --> 00:19:46.799
<v Speaker 3>exactly so, almost instantaneously, an electron from a higher outer

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00:19:47.000 --> 00:19:50.039
<v Speaker 3>orbit falls down to fill that newly created hole in

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00:19:50.079 --> 00:19:50.680
<v Speaker 3>the inner shell.

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00:19:50.839 --> 00:19:52.480
<v Speaker 2>It drops down to restore the balance.

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00:19:52.519 --> 00:19:55.200
<v Speaker 3>That makes sense, But here is the critical rule of physics.

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00:19:55.720 --> 00:19:59.480
<v Speaker 3>An outer electron possesses more potential energy than an inter electron.

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00:20:00.119 --> 00:20:02.480
<v Speaker 3>In order to drop down to that lower inner orbit,

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00:20:02.720 --> 00:20:05.319
<v Speaker 3>the outer electron has to shed its excess energy.

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00:20:05.400 --> 00:20:07.559
<v Speaker 2>It can't just take that extra energy down with it

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00:20:07.640 --> 00:20:08.359
<v Speaker 2>to the inner ring.

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00:20:08.480 --> 00:20:10.960
<v Speaker 3>No, it cannot. It has to release it, and it

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00:20:11.039 --> 00:20:14.480
<v Speaker 3>releases that exact specific amount of energy in the form

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00:20:14.519 --> 00:20:17.680
<v Speaker 3>of a brand new photon specifically an X ray photon.

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00:20:17.960 --> 00:20:19.519
<v Speaker 3>The atom fluoresces.

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00:20:19.160 --> 00:20:25.000
<v Speaker 2>Ah, hence X ray fluorescence. The atom absorbs the Sun's chaotic, violent,

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00:20:25.160 --> 00:20:29.000
<v Speaker 2>high energy X ray, uses it to eject an electron,

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00:20:29.200 --> 00:20:31.880
<v Speaker 2>and then as it heals itself, it spits out its

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00:20:31.960 --> 00:20:34.559
<v Speaker 2>own brand new X ray in response.

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00:20:34.759 --> 00:20:37.039
<v Speaker 3>And this right here is the magic key that makes

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00:20:37.079 --> 00:20:40.240
<v Speaker 3>the entire TMU mission possible. Because the energy of the

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00:20:40.319 --> 00:20:42.240
<v Speaker 3>X ray that gets spit out by the atom is

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00:20:42.319 --> 00:20:45.319
<v Speaker 3>not random, it is mathematically precise.

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00:20:45.119 --> 00:20:48.319
<v Speaker 2>Because the distance between the electron shells is fixed.

433
00:20:48.440 --> 00:20:51.559
<v Speaker 3>Yes, it is completely unique to the specific element that

434
00:20:51.680 --> 00:20:54.480
<v Speaker 3>created it. The energy difference between the outer shell and

435
00:20:54.519 --> 00:20:57.119
<v Speaker 3>the inner shell of an aluminum atom is a very

436
00:20:57.119 --> 00:20:58.880
<v Speaker 3>specific constant number.

437
00:20:58.680 --> 00:21:01.440
<v Speaker 2>So it only ever releases that exact amount of energy.

438
00:21:01.559 --> 00:21:04.400
<v Speaker 3>Correct. Therefore, the X ray emitted by an aliminum atom

439
00:21:04.640 --> 00:21:06.720
<v Speaker 3>has a totally different energy level than an X ray

440
00:21:06.720 --> 00:21:08.960
<v Speaker 3>emitted by a silicon atom, yeah, which is different from

441
00:21:08.960 --> 00:21:11.680
<v Speaker 3>the energy emitted by oxygen, which is different from magnesium.

442
00:21:11.720 --> 00:21:14.920
<v Speaker 2>So they act like absolute, unmistakable atomic fingerprints.

443
00:21:15.039 --> 00:21:19.200
<v Speaker 3>They are definitive elemental signatures. An X ray detector measures

444
00:21:19.200 --> 00:21:23.440
<v Speaker 3>the energy of these incoming photons in units called electron volts.

445
00:21:24.480 --> 00:21:27.279
<v Speaker 3>When the detector sees a spike at a specific number

446
00:21:27.279 --> 00:21:31.720
<v Speaker 3>of electron volts, it knows with absolute certainty that is aluminum.

447
00:21:31.759 --> 00:21:33.400
<v Speaker 2>There is no gaswork none.

448
00:21:33.720 --> 00:21:36.480
<v Speaker 3>When it sees a spike at a different, specific energy level,

449
00:21:36.599 --> 00:21:38.279
<v Speaker 3>it knows that is silicon.

450
00:21:38.680 --> 00:21:41.880
<v Speaker 2>This completely reframes the visual for me, going back to

451
00:21:41.960 --> 00:21:44.880
<v Speaker 2>our magic glasses idea. From the beginning, it's like the

452
00:21:44.920 --> 00:21:48.960
<v Speaker 2>Sun is acting as a giant, unpredictable cosmic black light.

453
00:21:49.160 --> 00:21:50.880
<v Speaker 3>I love the black light comparesson all right.

454
00:21:50.920 --> 00:21:53.200
<v Speaker 2>The moon is just sitting there in the dark, gray

455
00:21:53.319 --> 00:21:56.839
<v Speaker 2>and monochrome. But the moment a solar flare hits, the

456
00:21:57.000 --> 00:21:59.519
<v Speaker 2>entire surface suddenly glows in X ray wavelength.

457
00:21:59.559 --> 00:22:00.599
<v Speaker 3>It lights up completely.

458
00:22:00.640 --> 00:22:03.160
<v Speaker 2>And if you are orbiting overhead looking down through this

459
00:22:03.319 --> 00:22:07.240
<v Speaker 2>ten kilogram micropore array, you aren't just seeing a flash

460
00:22:07.279 --> 00:22:09.519
<v Speaker 2>of white light. You are seeing different colors of this

461
00:22:09.599 --> 00:22:10.559
<v Speaker 2>invisible spectrum.

462
00:22:10.640 --> 00:22:12.400
<v Speaker 3>You see the specific energy signatures.

463
00:22:12.519 --> 00:22:14.920
<v Speaker 2>Yeah, you see patches of the surface glowing with the

464
00:22:15.000 --> 00:22:18.640
<v Speaker 2>exact energetic fingerprint of aluminum, right next to pools glowing

465
00:22:18.680 --> 00:22:20.119
<v Speaker 2>with the fingerprint of silicon.

466
00:22:20.359 --> 00:22:22.960
<v Speaker 3>That is precisely what the instrument is designed to see.

467
00:22:23.400 --> 00:22:26.079
<v Speaker 3>The telescope sits up there and it's stable lunar orbit,

468
00:22:26.440 --> 00:22:30.440
<v Speaker 3>passively waiting when a flare hits. It catches these characteristic

469
00:22:30.559 --> 00:22:32.559
<v Speaker 3>X rays as they bounce back up from the surface,

470
00:22:33.079 --> 00:22:36.359
<v Speaker 3>sorts them by their specific energy levels, and plots them

471
00:22:36.359 --> 00:22:39.240
<v Speaker 3>onto a geographical map of the ground directly below.

472
00:22:39.519 --> 00:22:41.920
<v Speaker 2>Here's where it gets really interesting to me. We are

473
00:22:42.039 --> 00:22:48.279
<v Speaker 2>literally using solar flares, these massive, violent, sometimes terrifying eruptions

474
00:22:48.839 --> 00:22:52.039
<v Speaker 2>on our star, as a giant flashlight to read the

475
00:22:52.119 --> 00:22:55.279
<v Speaker 2>chemical dirt on the moon. We are we are hijacking

476
00:22:55.319 --> 00:22:57.920
<v Speaker 2>the Sun's fury to do our scientific surveying for us,

477
00:22:58.119 --> 00:23:01.119
<v Speaker 2>basically for free. But wait, this brings up a very

478
00:23:01.119 --> 00:23:03.920
<v Speaker 2>obvious logistical hurdle that we definitely need to address.

479
00:23:04.000 --> 00:23:06.000
<v Speaker 3>I suspect, I know exactly what you're going to ask.

480
00:23:06.240 --> 00:23:10.119
<v Speaker 2>Solar flares are notoriously unpredictable. I mean we cannot schedule that.

481
00:23:10.319 --> 00:23:11.359
<v Speaker 3>No, we certainly can't.

482
00:23:11.440 --> 00:23:14.240
<v Speaker 2>We have a general understanding of the eleven year solar cycle,

483
00:23:14.279 --> 00:23:17.480
<v Speaker 2>you know, solar maximum and solar minimum, but we cannot

484
00:23:17.480 --> 00:23:20.200
<v Speaker 2>predict a specific flare with pinpoint accuracy.

485
00:23:20.279 --> 00:23:22.119
<v Speaker 3>It's space weather. It's chaotic.

486
00:23:22.559 --> 00:23:26.279
<v Speaker 2>Sometimes the Sun is incredibly active, throwing out flares every day,

487
00:23:26.640 --> 00:23:29.480
<v Speaker 2>and sometimes it is stubbornly quiet for weeks or even

488
00:23:29.559 --> 00:23:32.359
<v Speaker 2>months at a time. If our telescope only works when

489
00:23:32.359 --> 00:23:35.400
<v Speaker 2>the sun flares, doesn't that make mapping the entire Moon

490
00:23:35.440 --> 00:23:37.720
<v Speaker 2>a massive, frustrating waiting game.

491
00:23:37.839 --> 00:23:40.279
<v Speaker 3>It absolutely makes it a waiting game. There's no getting

492
00:23:40.279 --> 00:23:42.480
<v Speaker 3>around that. You cannot just send this satellite up for

493
00:23:42.480 --> 00:23:45.960
<v Speaker 3>a long weekend, snap a global picture, and come.

494
00:23:45.799 --> 00:23:47.799
<v Speaker 2>Home because it might not flash while you're there.

495
00:23:47.960 --> 00:23:51.079
<v Speaker 3>Exactly, you are entirely at the mercy of the space

496
00:23:51.119 --> 00:23:55.039
<v Speaker 3>weather environment. If the sun is quiet, your highly advanced

497
00:23:55.160 --> 00:23:58.960
<v Speaker 3>X ray telescope is essentially blind. It is seeing almost

498
00:23:58.960 --> 00:24:00.920
<v Speaker 3>nothing but cosmic background noise.

499
00:24:01.279 --> 00:24:03.440
<v Speaker 2>So how long does it actually take to build a

500
00:24:03.519 --> 00:24:07.640
<v Speaker 2>complete high resolution map of an entire planetary body if

501
00:24:07.640 --> 00:24:10.640
<v Speaker 2>you are just waiting for random, unpredictable flashes of light

502
00:24:10.960 --> 00:24:13.480
<v Speaker 2>from a star ninety three million miles away.

503
00:24:13.519 --> 00:24:16.920
<v Speaker 3>Well, this is exactly why the TMU team's specific approach

504
00:24:16.960 --> 00:24:19.480
<v Speaker 3>with the five x five array is so critical. Remember

505
00:24:19.480 --> 00:24:20.960
<v Speaker 3>when we talked about the wide net.

506
00:24:20.839 --> 00:24:21.839
<v Speaker 2>Oh right, the flies.

507
00:24:21.920 --> 00:24:26.200
<v Speaker 3>I Yes, If you only had one small micropore sensor

508
00:24:26.680 --> 00:24:29.039
<v Speaker 3>and you only caught a tiny narrow sliver of the

509
00:24:29.039 --> 00:24:32.640
<v Speaker 3>Moon's surface during a brief flare, it would take centuries

510
00:24:32.640 --> 00:24:35.000
<v Speaker 3>of orbiting to piece together a full map.

511
00:24:35.079 --> 00:24:37.200
<v Speaker 2>Because the odds of you looking at the right spot

512
00:24:37.240 --> 00:24:40.359
<v Speaker 2>at the exact right millisecond are so low.

513
00:24:40.640 --> 00:24:43.880
<v Speaker 3>The probability would be incredibly low. But because you have

514
00:24:43.920 --> 00:24:46.759
<v Speaker 3>a wide field of view provided by the distributed array,

515
00:24:47.279 --> 00:24:50.680
<v Speaker 3>every single time the sun flares, you cast a massive net,

516
00:24:51.000 --> 00:24:53.519
<v Speaker 3>you illuminate and capture a huge swad of the surface.

517
00:24:53.519 --> 00:24:56.160
<v Speaker 2>Simultaneously, you are capturing a much bigger chunk of the

518
00:24:56.240 --> 00:24:58.279
<v Speaker 2>jigsaw puzzle with every single flash.

519
00:24:58.319 --> 00:25:02.319
<v Speaker 3>Exactly the complex orbit simulations run by Toyta and Professor

520
00:25:02.359 --> 00:25:06.160
<v Speaker 3>Ezoe suggests that by maintaining this orbital vigilance, just passively

521
00:25:06.200 --> 00:25:08.640
<v Speaker 3>flying over the surface and catching these flashes whenever the

522
00:25:08.680 --> 00:25:12.319
<v Speaker 3>Sun decides to cooperate, you could achieve a full, comprehensive

523
00:25:12.359 --> 00:25:15.240
<v Speaker 3>map of the Moon's surface chemistry in just a few

524
00:25:15.279 --> 00:25:16.920
<v Speaker 3>years of continuous observation.

525
00:25:17.359 --> 00:25:19.880
<v Speaker 2>Just a few years. That's actually amazing. It is like

526
00:25:20.000 --> 00:25:23.599
<v Speaker 2>building a massive long exposure photograph. You piece it together

527
00:25:23.680 --> 00:25:27.039
<v Speaker 2>flare by flair, photon by photon, pixel by pixel until

528
00:25:27.039 --> 00:25:30.039
<v Speaker 2>the entire global map comes into sharp focus.

529
00:25:30.319 --> 00:25:32.400
<v Speaker 3>That's a great way to put it. A long exposure

530
00:25:32.640 --> 00:25:33.720
<v Speaker 3>cosmic photograph.

531
00:25:33.799 --> 00:25:36.839
<v Speaker 2>Okay, so we have established the brilliant engineering. We have

532
00:25:36.920 --> 00:25:42.720
<v Speaker 2>this lightweight micropore telescope array. We understand the cosmic physics

533
00:25:42.799 --> 00:25:45.279
<v Speaker 2>of how we use the sun as a black light

534
00:25:45.559 --> 00:25:48.839
<v Speaker 2>to trigger these atomic fingerprints via X ray fluorescence.

535
00:25:48.920 --> 00:25:50.680
<v Speaker 3>The mechanism is perfectly sound.

536
00:25:50.759 --> 00:25:54.039
<v Speaker 2>The engineering is revolutionary. Yeah, but now we really have.

537
00:25:54.000 --> 00:25:57.079
<v Speaker 3>To talk about the why, like the scientific application of

538
00:25:57.119 --> 00:25:57.839
<v Speaker 3>all this data.

539
00:25:57.920 --> 00:26:00.519
<v Speaker 2>Because once we spend those few years in orbit and

540
00:26:00.519 --> 00:26:03.200
<v Speaker 2>we finally catch all these fluorescent fingerprints and we build

541
00:26:03.240 --> 00:26:07.319
<v Speaker 2>this beautiful, colorful map of oxygen, magnesium, aluminum in silicon,

542
00:26:08.079 --> 00:26:10.680
<v Speaker 2>what story do those colors actually tell us?

543
00:26:10.759 --> 00:26:12.640
<v Speaker 3>He tell us the story of the Moon's birth.

544
00:26:12.720 --> 00:26:14.480
<v Speaker 2>We need to move from the how it works to

545
00:26:14.519 --> 00:26:17.519
<v Speaker 2>the what it means, because reading these elements across the

546
00:26:17.559 --> 00:26:21.200
<v Speaker 2>global surface is basically like reading the deep geological bones

547
00:26:21.200 --> 00:26:21.599
<v Speaker 2>of the Moon.

548
00:26:22.200 --> 00:26:25.680
<v Speaker 3>It is the ultimate exercise in planetary forensics. And to

549
00:26:25.759 --> 00:26:29.039
<v Speaker 3>truly understand why this new global map is so vital

550
00:26:29.119 --> 00:26:32.119
<v Speaker 3>to planetary scientists, we have to look honestly at the

551
00:26:32.200 --> 00:26:33.640
<v Speaker 3>data we are currently working with.

552
00:26:33.799 --> 00:26:35.960
<v Speaker 2>What do you mean don't we already know a lot

553
00:26:36.000 --> 00:26:36.559
<v Speaker 2>about the Moon?

554
00:26:36.839 --> 00:26:39.960
<v Speaker 3>We do. Humanity has actually known a fair bit about

555
00:26:39.960 --> 00:26:44.119
<v Speaker 3>the Moon's fundamental chemistry for decades, but our knowledge is

556
00:26:44.160 --> 00:26:48.279
<v Speaker 3>incredibly localized. It is severely limited by geography.

557
00:26:48.359 --> 00:26:50.559
<v Speaker 2>Oh, we were talking about the physical samples we brought

558
00:26:50.599 --> 00:26:52.359
<v Speaker 2>back the Apollo missions.

559
00:26:52.480 --> 00:26:56.759
<v Speaker 3>Yes, the Apollo missions were a monumental, unparalleled achievement in

560
00:26:56.839 --> 00:27:00.799
<v Speaker 3>human history. The hundreds of pounds of physic rock and

561
00:27:00.880 --> 00:27:05.359
<v Speaker 3>regolith that those astronauts brought back to Earth completely revolutionized

562
00:27:05.359 --> 00:27:07.880
<v Speaker 3>our understanding of the Solar System. But they only went

563
00:27:07.920 --> 00:27:10.400
<v Speaker 3>to a few places, right, we have to remember the

564
00:27:10.440 --> 00:27:15.720
<v Speaker 3>strict operational constraints of Apollo. The astronauts landed in very specific,

565
00:27:16.160 --> 00:27:20.680
<v Speaker 3>carefully chosen, relatively flat and safe equatorial regions on the

566
00:27:20.680 --> 00:27:23.519
<v Speaker 3>near side of the Moon. Think of the Sea of Tranquility.

567
00:27:23.640 --> 00:27:25.920
<v Speaker 2>They couldn't exactly land in the middle of a jagged

568
00:27:26.000 --> 00:27:26.720
<v Speaker 2>crater field.

569
00:27:26.799 --> 00:27:29.039
<v Speaker 3>No, it was too dangerous, and they only had a

570
00:27:29.079 --> 00:27:31.640
<v Speaker 3>few hours or days to scoop up material from their

571
00:27:31.680 --> 00:27:34.200
<v Speaker 3>immediate local surroundings before they had to leave.

572
00:27:34.519 --> 00:27:38.000
<v Speaker 2>So our current hands on understanding of the Moon's global

573
00:27:38.079 --> 00:27:42.359
<v Speaker 2>chemical makeup is essentially based on a few tiny pinpricks

574
00:27:42.400 --> 00:27:45.079
<v Speaker 2>of data clustered near the equator on one side of

575
00:27:45.119 --> 00:27:45.599
<v Speaker 2>the sphere.

576
00:27:45.759 --> 00:27:48.519
<v Speaker 3>That is the reality we have extravagated a lot from

577
00:27:48.519 --> 00:27:52.759
<v Speaker 3>those samples, but extrapolating is not the same as observing globally.

578
00:27:53.039 --> 00:27:54.359
<v Speaker 2>I am trying to think of a good way to

579
00:27:54.400 --> 00:27:58.400
<v Speaker 2>conceptualize how limited that is. It feels like trying to

580
00:27:58.480 --> 00:28:03.079
<v Speaker 2>understand the entire, complex, diverse geography of the Earth, trying

581
00:28:03.119 --> 00:28:06.960
<v Speaker 2>to comprehend the existence of the Himalayas, the Sahara Desert,

582
00:28:07.000 --> 00:28:11.759
<v Speaker 2>the Amazon Rainforest, the deep Marianna's Trench, the polar ice caps.

583
00:28:11.920 --> 00:28:12.720
<v Speaker 3>Where you going with us?

584
00:28:12.920 --> 00:28:15.319
<v Speaker 2>By only looking at a handful of dirt you scooped

585
00:28:15.400 --> 00:28:18.160
<v Speaker 2>up from a single backyard in a suburb of Ohio.

586
00:28:17.839 --> 00:28:20.759
<v Speaker 3>Oh that is a wonderfully apt comparison. Yes, if you

587
00:28:20.799 --> 00:28:23.640
<v Speaker 3>only looked at the dirt from that Ohio backyard, you

588
00:28:23.720 --> 00:28:26.799
<v Speaker 3>might reasonably conclude that the entire Earth is covered in temperate,

589
00:28:26.839 --> 00:28:28.480
<v Speaker 3>loamy soil and green grass.

590
00:28:28.640 --> 00:28:31.680
<v Speaker 2>You would completely miss the frozen tundra of Antarica. You'd

591
00:28:31.680 --> 00:28:34.319
<v Speaker 2>miss the volcanic islands of Hawaii.

592
00:28:34.079 --> 00:28:37.119
<v Speaker 3>You would miss the deep ocean trenches. And with the moon,

593
00:28:37.559 --> 00:28:40.759
<v Speaker 3>we know from orbital imaging that there are massive physical

594
00:28:40.839 --> 00:28:43.359
<v Speaker 3>and geographical differences between different regions.

595
00:28:43.559 --> 00:28:46.640
<v Speaker 2>Just visually, it looks totally different depending on where you look.

596
00:28:46.599 --> 00:28:50.200
<v Speaker 3>Exactly We know the near sight is covered in those huge, dark,

597
00:28:50.319 --> 00:28:53.480
<v Speaker 3>flat basaltic plains we call Maria, but we know the

598
00:28:53.480 --> 00:28:57.599
<v Speaker 3>far side looks completely different. It is heavily cratered, ancient,

599
00:28:57.799 --> 00:29:00.680
<v Speaker 3>rugged highlands with almost no dark Maria.

600
00:29:00.839 --> 00:29:03.119
<v Speaker 2>The two sides of the Moon barely even look like

601
00:29:03.160 --> 00:29:04.519
<v Speaker 2>they belong to the same planet.

602
00:29:04.640 --> 00:29:07.920
<v Speaker 3>It's true. Furthermore, we know that the South Pole Acin

603
00:29:08.000 --> 00:29:10.519
<v Speaker 3>Basin on the far side is one of the largest

604
00:29:10.680 --> 00:29:13.359
<v Speaker 3>deepest impact craters in the entire Solar System.

605
00:29:13.440 --> 00:29:14.440
<v Speaker 2>How deep is it?

606
00:29:14.440 --> 00:29:17.960
<v Speaker 3>It is so incredibly deep that it potentially excavated material

607
00:29:17.960 --> 00:29:21.039
<v Speaker 3>from the deep lunar mantle itself. But because we only

608
00:29:21.079 --> 00:29:23.480
<v Speaker 3>have rocks from a few backyards on the near side,

609
00:29:23.680 --> 00:29:27.079
<v Speaker 3>we do not have a high resolution global chemical map

610
00:29:27.279 --> 00:29:31.799
<v Speaker 3>to connect all these massive geographical pieces together. We have theories,

611
00:29:32.000 --> 00:29:34.200
<v Speaker 3>but we lack global chemical conformation.

612
00:29:34.720 --> 00:29:36.759
<v Speaker 2>So we have the corner pieces of a thousand piece

613
00:29:36.839 --> 00:29:39.960
<v Speaker 2>jigsaw puzzle, but we are missing the vast majority of

614
00:29:39.960 --> 00:29:40.880
<v Speaker 2>the picture in the middle.

615
00:29:41.160 --> 00:29:44.680
<v Speaker 3>And a comprehensive geochemical map finally gives us the complete picture.

616
00:29:45.400 --> 00:29:48.680
<v Speaker 3>If we can see the precise global distribution of elements

617
00:29:48.759 --> 00:29:53.119
<v Speaker 3>like magnesium, iron, and aluminum, we can actually reverse engineer

618
00:29:53.599 --> 00:29:56.039
<v Speaker 3>billions of years of planetary evolution.

619
00:29:55.920 --> 00:29:58.240
<v Speaker 2>We can test if our theories are actually right.

620
00:29:58.559 --> 00:30:02.680
<v Speaker 3>Yes, allows us to empirically test our fundamental models of

621
00:30:02.720 --> 00:30:05.279
<v Speaker 3>how the Moon formed and how it evolved in its

622
00:30:05.279 --> 00:30:06.079
<v Speaker 3>earliest days.

623
00:30:06.720 --> 00:30:09.680
<v Speaker 2>Let's dig deep into that early history. When we talk

624
00:30:09.720 --> 00:30:11.839
<v Speaker 2>about the formation of the Moon, we are talking about

625
00:30:11.880 --> 00:30:16.240
<v Speaker 2>a cataclysmic event, right, the giant impact hypothesis followed by

626
00:30:16.240 --> 00:30:17.400
<v Speaker 2>the magma ocean.

627
00:30:17.400 --> 00:30:21.160
<v Speaker 3>That is the leading scientific consensus. Yes, the theory dictates

628
00:30:21.160 --> 00:30:24.039
<v Speaker 3>that over four billion years ago, the very early proto

629
00:30:24.079 --> 00:30:27.079
<v Speaker 3>Earth was struck by another developing planet roughly the size

630
00:30:27.079 --> 00:30:28.960
<v Speaker 3>of Mars, which scientists call thee.

631
00:30:28.960 --> 00:30:30.759
<v Speaker 2>Just a full on planetary collision, a.

632
00:30:30.720 --> 00:30:33.559
<v Speaker 3>Glancing blow, but yes, yeah, the sheer kinetic energy of

633
00:30:33.599 --> 00:30:36.920
<v Speaker 3>that collision vaporized a massive aunt of material from both bodies,

634
00:30:37.279 --> 00:30:40.400
<v Speaker 3>blowing a ring of superheated debris into orbit around the Earth.

635
00:30:40.960 --> 00:30:43.599
<v Speaker 3>Over time, gravity pulled that ring and debris together to

636
00:30:43.599 --> 00:30:44.160
<v Speaker 3>form the Moon.

637
00:30:44.440 --> 00:30:47.680
<v Speaker 2>It is a terrifying and awesome thing to visualize, just

638
00:30:47.799 --> 00:30:51.880
<v Speaker 2>a massive glowing sphere of liquid fire coalescing in space.

639
00:30:52.519 --> 00:30:56.240
<v Speaker 2>The entire Moon in its infancy was just a global

640
00:30:56.279 --> 00:30:57.839
<v Speaker 2>ocean of molten rock.

641
00:30:58.079 --> 00:31:02.599
<v Speaker 3>A global magma ocean, potentially hundreds of kilometers deep. Now,

642
00:31:02.680 --> 00:31:06.000
<v Speaker 3>as of that magma ocean slowly radiate its heat away

643
00:31:06.039 --> 00:31:08.920
<v Speaker 3>into the cold of space over millions of years, a

644
00:31:08.960 --> 00:31:12.559
<v Speaker 3>profound geological process called differentiation occurred.

645
00:31:12.839 --> 00:31:15.519
<v Speaker 2>Let's break down the mechanics of differentiation, because I am

646
00:31:15.559 --> 00:31:19.160
<v Speaker 2>trying to picture this without wind or weather or tectonic

647
00:31:19.200 --> 00:31:22.039
<v Speaker 2>plates like we have on modern Earth. Wouldn't a ball

648
00:31:22.079 --> 00:31:25.799
<v Speaker 2>of liquid rock just cool down into one solid, uniform,

649
00:31:25.920 --> 00:31:29.240
<v Speaker 2>evenly mixed sphere of gray rock. Why does it change?

650
00:31:29.519 --> 00:31:32.440
<v Speaker 3>Because of gravity and the varying densities of different minerals.

651
00:31:32.759 --> 00:31:34.119
<v Speaker 3>Even though it was a liquid ocean, it was a

652
00:31:34.119 --> 00:31:37.240
<v Speaker 3>liquid suspended in a gravitational field. As the magma slowly

653
00:31:37.279 --> 00:31:40.920
<v Speaker 3>cool different minerals began to crystallize at different temperatures.

654
00:31:40.279 --> 00:31:42.640
<v Speaker 2>Meaning they turned from liquid to solid at different times.

655
00:31:42.720 --> 00:31:45.079
<v Speaker 3>Right. This is a process called fractional crystallization.

656
00:31:45.319 --> 00:31:48.279
<v Speaker 2>Okay, so the liquid rock starts turning into solid crystals,

657
00:31:48.319 --> 00:31:50.240
<v Speaker 2>but not all at once exactly.

658
00:31:50.759 --> 00:31:55.319
<v Speaker 3>And as these crystals form they respond to gravity. The heavier,

659
00:31:55.599 --> 00:31:59.880
<v Speaker 3>denser minerals, specifically those rich in iron and magnesium like

660
00:32:00.079 --> 00:32:04.319
<v Speaker 3>olivine and pyroxene, crystallized and physically sank down toward the

661
00:32:04.319 --> 00:32:04.839
<v Speaker 3>center of the.

662
00:32:04.799 --> 00:32:07.640
<v Speaker 2>Moon, like heavy sand sinking in a pool of water.

663
00:32:07.839 --> 00:32:12.279
<v Speaker 3>Yes, over millions of years, this sinking material formed the deep,

664
00:32:12.599 --> 00:32:14.000
<v Speaker 3>dense lunar mantle.

665
00:32:14.160 --> 00:32:16.319
<v Speaker 2>The heavy stuff sinks to the bottom of the ocean.

666
00:32:16.400 --> 00:32:17.319
<v Speaker 2>What about the rest.

667
00:32:17.640 --> 00:32:22.279
<v Speaker 3>Well, Meanwhile, lighter minerals were also crystallizing, sophifically, a mineral

668
00:32:22.319 --> 00:32:26.400
<v Speaker 3>called plagioclase feldspar, which is heavily rich in aluminum and calcium.

669
00:32:26.440 --> 00:32:29.359
<v Speaker 3>And because it's lighter, because this mineral was significantly lighter

670
00:32:29.400 --> 00:32:31.960
<v Speaker 3>and less dense than the surrounding magma, it did not sink.

671
00:32:32.319 --> 00:32:34.119
<v Speaker 3>It floated to the top of the magma ocean.

672
00:32:34.200 --> 00:32:37.839
<v Speaker 2>Oh, like foam on top of a cappuccino, That's exactly it.

673
00:32:37.319 --> 00:32:41.079
<v Speaker 3>It essentially formed a massive global scum of lightweight rock

674
00:32:41.119 --> 00:32:44.759
<v Speaker 3>floating on the surface. As the ocean finally cooled completely,

675
00:32:45.240 --> 00:32:48.519
<v Speaker 3>that sloating layer of aluminum rich rock solidified to become

676
00:32:48.559 --> 00:32:49.640
<v Speaker 3>the primary crust of the.

677
00:32:49.559 --> 00:32:53.480
<v Speaker 2>Moon, the ancient lunar highlands. So, according to this model,

678
00:32:53.759 --> 00:32:56.480
<v Speaker 2>the original outer shell of the Moon should be absolutely

679
00:32:56.480 --> 00:32:59.799
<v Speaker 2>packed with that lightweight aluminum, while all the heavy magnesium

680
00:32:59.799 --> 00:33:01.920
<v Speaker 2>and o iron should be locked away deep underground.

681
00:33:02.119 --> 00:33:05.039
<v Speaker 3>Yes, and this is exactly why the X ray fluorescence

682
00:33:05.079 --> 00:33:08.720
<v Speaker 3>map from our tiny telescope is so crucial. If we

683
00:33:08.759 --> 00:33:12.519
<v Speaker 3>can map the exact concentrations of aluminum versus magnesium globally,

684
00:33:13.000 --> 00:33:17.720
<v Speaker 3>we can mathematically prove, refine, or even challenge the parameters

685
00:33:17.759 --> 00:33:19.200
<v Speaker 3>of this Magna ocean model.

686
00:33:19.279 --> 00:33:21.359
<v Speaker 2>We can see if it actually happened that way everywhere.

687
00:33:21.400 --> 00:33:23.640
<v Speaker 3>We can see exactly how thick the aluminum crust is

688
00:33:23.680 --> 00:33:26.400
<v Speaker 3>in different regions. We could see if the differentiation process

689
00:33:26.480 --> 00:33:28.960
<v Speaker 3>was uniform, or if it was interrupted or altered in

690
00:33:29.000 --> 00:33:29.680
<v Speaker 3>certain areas.

691
00:33:29.799 --> 00:33:33.799
<v Speaker 2>But the Moon isn't just a perfectly pristine, layered jawbreaker today.

692
00:33:34.119 --> 00:33:36.839
<v Speaker 2>That crust didn't just sit there untouched for four billion years.

693
00:33:36.839 --> 00:33:37.799
<v Speaker 2>It has been abused.

694
00:33:37.960 --> 00:33:40.640
<v Speaker 3>It has suffered relentless abuse, and that brings us to

695
00:33:40.720 --> 00:33:43.799
<v Speaker 3>the second major geological gap. This X ray map will

696
00:33:43.799 --> 00:33:47.720
<v Speaker 3>fill the violent volcanic and impact history of the Moon.

697
00:33:47.599 --> 00:33:49.839
<v Speaker 2>Because over the last four billion years, the Moon has

698
00:33:49.880 --> 00:33:52.720
<v Speaker 2>been relentlessly bombarded by asteroids and commets.

699
00:33:53.039 --> 00:33:56.000
<v Speaker 3>The Late Heavy bombardment in just billions of years of

700
00:33:56.160 --> 00:33:58.240
<v Speaker 3>random space rock smashing into it.

701
00:33:58.160 --> 00:34:01.279
<v Speaker 2>And some of those impacts were huge.

702
00:34:00.640 --> 00:34:04.720
<v Speaker 3>Beyond huge. Some of these astray impacts were so unimaginably

703
00:34:04.799 --> 00:34:08.119
<v Speaker 3>colossal that They didn't just dent the surface, They punched

704
00:34:08.159 --> 00:34:12.119
<v Speaker 3>completely through the outer light aluminum crust, and they physically

705
00:34:12.159 --> 00:34:15.840
<v Speaker 3>excavated the heavy, dense magnesium and iron rich mantle from

706
00:34:15.840 --> 00:34:16.400
<v Speaker 3>deep below.

707
00:34:16.559 --> 00:34:20.320
<v Speaker 2>They essentially acted as cosmic drills, digging up the buried

708
00:34:20.440 --> 00:34:22.480
<v Speaker 2>layers and splashing them all over the surface.

709
00:34:22.599 --> 00:34:26.239
<v Speaker 3>Right and furthermore, later in the Moon's history, massive internal

710
00:34:26.320 --> 00:34:29.639
<v Speaker 3>volcanic eruptions brought molten basalt from deep inside the Moon

711
00:34:30.079 --> 00:34:30.880
<v Speaker 3>up to the surface.

712
00:34:31.000 --> 00:34:32.440
<v Speaker 2>Is that where the dark spots come from.

713
00:34:32.559 --> 00:34:36.400
<v Speaker 3>Yes, this heavy lava float out, filling in the giant

714
00:34:36.440 --> 00:34:39.960
<v Speaker 3>impact basins and creating those dark patches the maria that

715
00:34:40.039 --> 00:34:41.239
<v Speaker 3>we see from Earth today.

716
00:34:41.559 --> 00:34:44.639
<v Speaker 2>So when our tiny TMU X ray telescope is orbiting

717
00:34:44.639 --> 00:34:47.800
<v Speaker 2>the Moon, sweeping over a region of ancient highlands and

718
00:34:47.840 --> 00:34:51.400
<v Speaker 2>it suddenly sees a massive, unexpected spike in the elemental

719
00:34:51.440 --> 00:34:54.199
<v Speaker 2>signature of magnesium right in the middle of an area

720
00:34:54.239 --> 00:34:57.400
<v Speaker 2>that should be pure aluminum crust, scientists know exactly what

721
00:34:57.400 --> 00:34:58.000
<v Speaker 2>they're looking at.

722
00:34:58.280 --> 00:35:02.000
<v Speaker 3>They absolutely do looking at a location where a giant

723
00:35:02.079 --> 00:35:05.880
<v Speaker 3>asteroid penetrated the crust and brought the deep interior up

724
00:35:05.920 --> 00:35:07.840
<v Speaker 3>to the surface for us to analyze.

725
00:35:07.880 --> 00:35:10.239
<v Speaker 2>If we connect this to the bigger picture. The entire

726
00:35:10.320 --> 00:35:13.119
<v Speaker 2>surface of the Moon is just a written chemical record

727
00:35:13.119 --> 00:35:15.360
<v Speaker 2>of the violent history of the early Solar System.

728
00:35:15.559 --> 00:35:17.360
<v Speaker 3>It is a diary of catastrophe.

729
00:35:17.440 --> 00:35:22.000
<v Speaker 2>Every single asteroid impact, every single ancient lava flow, left

730
00:35:22.039 --> 00:35:26.400
<v Speaker 2>a permanent chemical signature. By mapping the exact distribution of

731
00:35:26.400 --> 00:35:30.679
<v Speaker 2>these elements globally, we aren't just looking at interesting, colorful rocks.

732
00:35:31.159 --> 00:35:34.440
<v Speaker 2>We are reading the history book of our cosmic neighborhood.

733
00:35:34.519 --> 00:35:37.320
<v Speaker 3>We are learning the fundamental mechanics of how planets coalesce

734
00:35:37.360 --> 00:35:41.199
<v Speaker 3>from dust, how they differentiate into layers, how they evolve

735
00:35:41.280 --> 00:35:44.360
<v Speaker 3>over eons, and how they endure cosmic bombardment.

736
00:35:44.480 --> 00:35:47.199
<v Speaker 2>It is incredibly profound to think about. We are using

737
00:35:47.280 --> 00:35:51.400
<v Speaker 2>microscopic atomic fingerprints triggered by violent solar flares to read

738
00:35:51.440 --> 00:35:54.400
<v Speaker 2>a geological history book that was written billions of years

739
00:35:54.400 --> 00:35:57.440
<v Speaker 2>before the first single celled life even existed on Earth.

740
00:35:57.519 --> 00:35:59.599
<v Speaker 3>It is pure awe inspiring science.

741
00:36:00.079 --> 00:36:03.280
<v Speaker 2>But as thrilling as all that deep ancient history is,

742
00:36:03.719 --> 00:36:07.599
<v Speaker 2>there is an entirely different side to this coin. Understanding

743
00:36:07.639 --> 00:36:11.639
<v Speaker 2>the Moon's past is intellectually fascinating, but this chemical map

744
00:36:11.679 --> 00:36:16.519
<v Speaker 2>has a highly practical, incredibly urgent application for humanity's immediate future.

745
00:36:16.599 --> 00:36:18.559
<v Speaker 3>Oh absolutely, This isn't just academic.

746
00:36:18.639 --> 00:36:20.840
<v Speaker 2>We aren't just matching the past. We are drawing the

747
00:36:20.960 --> 00:36:22.599
<v Speaker 2>literal roadmap to the future.

748
00:36:22.639 --> 00:36:28.039
<v Speaker 3>And this is where the theoretical astrophysics means hard logistical reality, because,

749
00:36:28.079 --> 00:36:31.760
<v Speaker 3>as everyone paying attention to space exploration knows, humanity is

750
00:36:31.800 --> 00:36:34.760
<v Speaker 3>not content to just look at the Moon through telescopes anymore.

751
00:36:35.360 --> 00:36:37.239
<v Speaker 3>We are actively preparing to go back.

752
00:36:37.440 --> 00:36:39.519
<v Speaker 2>We are going back, and this time we are planning

753
00:36:39.559 --> 00:36:42.239
<v Speaker 2>to stay. We are talking about the Artemis program and

754
00:36:42.320 --> 00:36:46.800
<v Speaker 2>the massive international effort to establish a sustained, permanent human

755
00:36:46.880 --> 00:36:48.280
<v Speaker 2>presence on the lunar surface.

756
00:36:48.360 --> 00:36:50.880
<v Speaker 3>It is a completely different mission profile than Apollo.

757
00:36:51.159 --> 00:36:53.960
<v Speaker 2>Right. We are not talking about planting a flag, leaving

758
00:36:54.039 --> 00:36:56.159
<v Speaker 2>some footprints and coming home a few days later like

759
00:36:56.199 --> 00:36:59.280
<v Speaker 2>the Apollo era. We are talking about building base camps.

760
00:36:59.320 --> 00:37:04.159
<v Speaker 2>We are talking about about pressurized habitats, lunar rovers power stations,

761
00:37:04.440 --> 00:37:06.480
<v Speaker 2>a permanent foothold on another world.

762
00:37:06.760 --> 00:37:11.519
<v Speaker 3>And establishing a permanent foothold requires a completely different operational

763
00:37:11.559 --> 00:37:16.760
<v Speaker 3>mindset than a brief exploratory visit. Consider the logistics of

764
00:37:16.800 --> 00:37:18.000
<v Speaker 3>exploration on Earth.

765
00:37:18.159 --> 00:37:19.519
<v Speaker 2>Okay, like going camping.

766
00:37:19.760 --> 00:37:22.599
<v Speaker 3>Exactly, if you go camping for the weekend, you can

767
00:37:22.639 --> 00:37:25.920
<v Speaker 3>easily pack all your drinking water, all your food, and

768
00:37:25.920 --> 00:37:28.199
<v Speaker 3>your nylon tent in the trunk of your car. You

769
00:37:28.280 --> 00:37:30.519
<v Speaker 3>bring everything with you and you bring your trash home.

770
00:37:30.719 --> 00:37:31.400
<v Speaker 2>Easy enough.

771
00:37:31.440 --> 00:37:34.360
<v Speaker 3>But if you are moving into the deep wilderness permanently

772
00:37:34.760 --> 00:37:37.199
<v Speaker 3>to build a cabin and live there year round, you

773
00:37:37.239 --> 00:37:40.599
<v Speaker 3>cannot possibly bring a lifetime supply of water and lumber

774
00:37:40.679 --> 00:37:42.559
<v Speaker 3>in your car. It's impossible.

775
00:37:42.679 --> 00:37:44.440
<v Speaker 2>You have to learn how to live off the land.

776
00:37:44.559 --> 00:37:46.920
<v Speaker 2>You have to chop local wood, find a local stream,

777
00:37:47.119 --> 00:37:48.280
<v Speaker 2>hunt local food.

778
00:37:48.360 --> 00:37:50.639
<v Speaker 3>And living off the land in the unforgiving vacuum of

779
00:37:50.679 --> 00:37:54.079
<v Speaker 3>space is governed by a critical engineering concept. This is

780
00:37:54.079 --> 00:37:56.280
<v Speaker 3>a very clunky acronym, but it might be the most

781
00:37:56.320 --> 00:37:58.679
<v Speaker 3>important term in all of space exploration.

782
00:37:59.239 --> 00:38:02.840
<v Speaker 2>Isru iru incitu resource utilization.

783
00:38:03.039 --> 00:38:06.159
<v Speaker 3>Yes, it simply means utilizing the physical resources you find

784
00:38:06.199 --> 00:38:09.239
<v Speaker 3>naturally occurring at your destination, rather than bringing them all

785
00:38:09.239 --> 00:38:09.960
<v Speaker 3>the way from Earth.

786
00:38:10.280 --> 00:38:13.719
<v Speaker 2>And ru is not just a neat idea. It is

787
00:38:13.760 --> 00:38:17.840
<v Speaker 2>a mandatory requirement for human survival in space. Right.

788
00:38:18.159 --> 00:38:19.800
<v Speaker 3>It is absolutely non negotiable.

789
00:38:19.880 --> 00:38:22.480
<v Speaker 2>Let's explore why it's mandatory, because it all comes down

790
00:38:22.559 --> 00:38:25.760
<v Speaker 2>to the brutal physics of gravity wells and the rocket equation.

791
00:38:26.679 --> 00:38:29.039
<v Speaker 2>Bringing things from the surface of the Earth to the

792
00:38:29.039 --> 00:38:32.079
<v Speaker 2>surface of the Moon is mine bogglingly expensive.

793
00:38:32.239 --> 00:38:34.519
<v Speaker 3>It takes massive amounts of fuel just to lift a

794
00:38:34.599 --> 00:38:37.679
<v Speaker 3>tiny amount of mass out of Earth's gravity. It currently

795
00:38:37.719 --> 00:38:40.719
<v Speaker 3>costs thousands and thousands of dollars to launch a single

796
00:38:40.840 --> 00:38:42.760
<v Speaker 3>kilogram of mass into orbit.

797
00:38:42.719 --> 00:38:45.280
<v Speaker 2>A single kilogram. So if we want to build a

798
00:38:45.320 --> 00:38:49.159
<v Speaker 2>sprawling lunar habitat, we simply cannot afford to launch every

799
00:38:49.199 --> 00:38:52.559
<v Speaker 2>single steel beam, every single heavy solar panel, and every

800
00:38:52.599 --> 00:38:55.880
<v Speaker 2>single drop of drinking water on top of a giant rocket.

801
00:38:55.960 --> 00:38:58.800
<v Speaker 3>We would bankrupt the global economy before we even poured

802
00:38:58.840 --> 00:39:00.239
<v Speaker 3>the concrete for the foundation.

803
00:39:00.480 --> 00:39:03.800
<v Speaker 2>The gravity well of Earth is basically a tyrannical accountant.

804
00:39:03.960 --> 00:39:06.519
<v Speaker 2>It punishes every ounce of mass you try to take

805
00:39:06.559 --> 00:39:06.800
<v Speaker 2>with you.

806
00:39:06.960 --> 00:39:09.599
<v Speaker 3>That's a brutal way to put it, but it's completely accurate.

807
00:39:10.199 --> 00:39:13.000
<v Speaker 3>To survive long term on the Moon and to eventually

808
00:39:13.000 --> 00:39:15.719
<v Speaker 3>push onward to build colonies on Mars, we have to

809
00:39:15.760 --> 00:39:16.960
<v Speaker 3>find what we need on the Moon.

810
00:39:17.159 --> 00:39:19.920
<v Speaker 2>We have to become cosmic scavengers and miners.

811
00:39:19.960 --> 00:39:22.960
<v Speaker 3>We do, and this is exactly where our ten kilogram

812
00:39:23.320 --> 00:39:27.960
<v Speaker 3>micropore x ray telescope suddenly transitions from a purely scientific

813
00:39:28.000 --> 00:39:32.280
<v Speaker 3>instrument into the most valuable prospecting tool in the Solar system.

814
00:39:32.039 --> 00:39:34.920
<v Speaker 2>Because it isn't just looking for common rocks to validate

815
00:39:34.960 --> 00:39:39.519
<v Speaker 2>ancient geological theories. It is actively globally hunting for the

816
00:39:39.639 --> 00:39:42.199
<v Speaker 2>vital resources hidden in the dusty regolith.

817
00:39:42.280 --> 00:39:43.519
<v Speaker 3>It's looking for the gold mines.

818
00:39:44.039 --> 00:39:46.480
<v Speaker 2>So what specific resources are we talking about here? When

819
00:39:46.519 --> 00:39:48.960
<v Speaker 2>a mission planner at NASA looks at this glowing X

820
00:39:49.039 --> 00:39:52.239
<v Speaker 2>ray map, what are the gold mines they are desperately

821
00:39:52.280 --> 00:39:52.920
<v Speaker 2>searching for.

822
00:39:53.119 --> 00:39:55.880
<v Speaker 3>There are two main categories of resources that are absolutely

823
00:39:55.880 --> 00:39:59.480
<v Speaker 3>critical for ISRU. First, we are looking for the widespread

824
00:39:59.519 --> 00:40:03.400
<v Speaker 3>distribution of specific industrial metals and rare earth elements. We're

825
00:40:03.400 --> 00:40:07.559
<v Speaker 3>looking for high concentrations of titanium, iron, and aluminum.

826
00:40:06.960 --> 00:40:08.880
<v Speaker 2>Structural metals, things we can build with.

827
00:40:09.159 --> 00:40:12.840
<v Speaker 3>Exactly, if we're going to build robust structures on the Moon, habitats,

828
00:40:12.960 --> 00:40:16.079
<v Speaker 3>landing pads, blast shields, we need to know where the

829
00:40:16.119 --> 00:40:18.559
<v Speaker 3>highest concentrations of structural metals are located.

830
00:40:18.599 --> 00:40:19.400
<v Speaker 2>And what about power?

831
00:40:19.639 --> 00:40:22.280
<v Speaker 3>If we want to build sprawling fields of solar panels

832
00:40:22.280 --> 00:40:25.320
<v Speaker 3>to generate power during leaner day, we need to locate

833
00:40:25.440 --> 00:40:30.159
<v Speaker 3>massive deposits of silicon. The technology exists to literally scoop

834
00:40:30.239 --> 00:40:34.000
<v Speaker 3>up the lunar regolith, refine it using solar furnaces, extract

835
00:40:34.000 --> 00:40:36.440
<v Speaker 3>the metals, and three D print our habitats directly from

836
00:40:36.440 --> 00:40:37.239
<v Speaker 3>the lunar dirt.

837
00:40:37.320 --> 00:40:40.280
<v Speaker 2>That is wild three D printing a house from moon dirt.

838
00:40:40.639 --> 00:40:43.239
<v Speaker 3>But that entire industrial process only works if we know

839
00:40:43.320 --> 00:40:46.960
<v Speaker 3>exactly where the richest, most accessible veins of ore are located.

840
00:40:47.519 --> 00:40:49.920
<v Speaker 3>You don't build a massive mining facility in an area

841
00:40:49.960 --> 00:40:50.840
<v Speaker 3>with low grade dirt.

842
00:40:51.000 --> 00:40:54.960
<v Speaker 2>Okay, so building materials and power generation. That makes perfect

843
00:40:55.000 --> 00:40:58.360
<v Speaker 2>logistical sense. But there is something even more fundamental than

844
00:40:58.400 --> 00:41:01.559
<v Speaker 2>building materials and survive without a steel beam for a

845
00:41:01.599 --> 00:41:04.599
<v Speaker 2>few days, But there is one resource you cannot survive without.

846
00:41:04.960 --> 00:41:07.960
<v Speaker 3>The most universally valuable substance in the cosmos for human

847
00:41:08.000 --> 00:41:09.880
<v Speaker 3>beings water Water.

848
00:41:10.159 --> 00:41:13.880
<v Speaker 2>Every deep space mission, every search for life, every colonization plan,

849
00:41:14.000 --> 00:41:16.559
<v Speaker 2>it always always comes back to water.

850
00:41:16.400 --> 00:41:19.280
<v Speaker 3>Because it is the foundation of human biology and surprisingly

851
00:41:19.320 --> 00:41:21.480
<v Speaker 3>the foundation of our spacefaring infrastructure.

852
00:41:21.559 --> 00:41:24.840
<v Speaker 2>Now, the X ray telescope itself is primarily looking for

853
00:41:25.000 --> 00:41:29.239
<v Speaker 2>elemental fingerprints like oxygen right, not water molecules directly.

854
00:41:28.920 --> 00:41:31.960
<v Speaker 3>Correct, and while oxygen is locked up in silicate rocks

855
00:41:32.079 --> 00:41:36.280
<v Speaker 3>everywhere on the Moon, scientists are specifically hoping to correlate

856
00:41:36.599 --> 00:41:40.280
<v Speaker 3>these highly detailed elemental maps of oxygen and other trace

857
00:41:40.320 --> 00:41:44.000
<v Speaker 3>elements with existing data from other orbiters to find the

858
00:41:44.039 --> 00:41:47.800
<v Speaker 3>water Yes, to locate high concentrations of water related compounds.

859
00:41:48.360 --> 00:41:51.440
<v Speaker 3>Finding the precise location and volume of water is the

860
00:41:51.559 --> 00:41:53.840
<v Speaker 3>key to unlocking the entire solar system.

861
00:41:54.159 --> 00:41:56.719
<v Speaker 2>Let's really break down why water is so critical, because

862
00:41:56.719 --> 00:41:58.440
<v Speaker 2>I think a lot of people just assume it's only

863
00:41:58.480 --> 00:42:02.280
<v Speaker 2>for astronauts to drink. Obviously, biological hydration is paramount. But

864
00:42:02.440 --> 00:42:06.320
<v Speaker 2>water in a space colony is basically a miraculous Swiss

865
00:42:06.400 --> 00:42:07.039
<v Speaker 2>Army knife.

866
00:42:07.280 --> 00:42:10.719
<v Speaker 3>It truly is. Yes, you need it for direct life support, drinking, sanitation,

867
00:42:10.840 --> 00:42:15.039
<v Speaker 3>and growing food in hydroponic or aeroponic agricultural base. But

868
00:42:15.199 --> 00:42:19.400
<v Speaker 3>water has incredible physical properties that make it essential for survival.

869
00:42:19.679 --> 00:42:21.159
<v Speaker 2>Physical properties like what.

870
00:42:21.119 --> 00:42:24.000
<v Speaker 3>It is incredibly dense, and its molecular structure makes it

871
00:42:24.039 --> 00:42:28.079
<v Speaker 3>one of the absolute best available shields against dangerous cosmic radiation.

872
00:42:28.320 --> 00:42:30.360
<v Speaker 2>Wait, let me stop you there. Water acts as armor.

873
00:42:31.039 --> 00:42:35.000
<v Speaker 2>How does water stop radiation better than say, a thick

874
00:42:35.039 --> 00:42:35.679
<v Speaker 2>sheet of lead.

875
00:42:35.840 --> 00:42:38.079
<v Speaker 3>It has to do with the specific type of radiation

876
00:42:38.199 --> 00:42:42.800
<v Speaker 3>astronauts face in deep space. They're bombarded by galactic cosmic

877
00:42:42.880 --> 00:42:46.559
<v Speaker 3>rays and solar particle events, which are essentially high energy

878
00:42:46.559 --> 00:42:49.400
<v Speaker 3>protons screaming through space at near the speed of light.

879
00:42:49.480 --> 00:42:51.519
<v Speaker 2>Okay, so these protons are just flying everywhere.

880
00:42:51.599 --> 00:42:54.679
<v Speaker 3>Yes, if a high energy proton hits a heavy element

881
00:42:54.760 --> 00:42:58.119
<v Speaker 3>like lead, it can actually shatter the lead nucleus, creating

882
00:42:58.119 --> 00:43:02.039
<v Speaker 3>a shower of secondary radiation that is incredibly dangerous to

883
00:43:02.079 --> 00:43:04.559
<v Speaker 3>human tissue. It makes it worse in a way. Yes,

884
00:43:05.039 --> 00:43:07.599
<v Speaker 3>but water is H two O two parts hydrogen. A

885
00:43:07.679 --> 00:43:10.840
<v Speaker 3>hydrogen nucleus is basically just a single proton, So when

886
00:43:10.840 --> 00:43:13.960
<v Speaker 3>a high energy cosmic proton hits the hydrogen in water,

887
00:43:14.159 --> 00:43:17.239
<v Speaker 3>it's like two billiard balls of the exact same mass colliding.

888
00:43:17.280 --> 00:43:18.760
<v Speaker 2>The incoming proton just stops.

889
00:43:18.880 --> 00:43:22.639
<v Speaker 3>The incoming proton transfers its energy efficiently, slowing down rapidly

890
00:43:22.679 --> 00:43:25.360
<v Speaker 3>without creating a dangerous shower of secondary radiation.

891
00:43:25.719 --> 00:43:28.239
<v Speaker 2>That is fascinating. So if you want to build a

892
00:43:28.280 --> 00:43:32.079
<v Speaker 2>safe liner habitat, you don't necessarily need to drag massive

893
00:43:32.239 --> 00:43:35.840
<v Speaker 2>lead plates from Earth. You just build double walled habitats

894
00:43:35.840 --> 00:43:37.760
<v Speaker 2>and pump your water supply into the walls.

895
00:43:37.880 --> 00:43:41.400
<v Speaker 3>You literally live inside a giant protective water balloon.

896
00:43:41.119 --> 00:43:44.320
<v Speaker 2>That is brilliant, So it is hydration, it is agriculture,

897
00:43:44.320 --> 00:43:48.400
<v Speaker 2>and it is vital armor. But there is one more massive,

898
00:43:48.519 --> 00:43:51.480
<v Speaker 2>game changing application for water on the Moon, and it

899
00:43:51.519 --> 00:43:55.599
<v Speaker 2>relies on the basic chemistry of the molecule itself. H

900
00:43:55.679 --> 00:43:58.800
<v Speaker 2>two two parts hydrogen, one cart oxygen.

901
00:43:58.840 --> 00:44:00.239
<v Speaker 3>I know exactly where this is going.

902
00:44:00.360 --> 00:44:03.280
<v Speaker 2>If you have a sprawling field of solar panels providing

903
00:44:03.320 --> 00:44:06.599
<v Speaker 2>abundant electricity during the two week lunar day, you can

904
00:44:06.639 --> 00:44:09.920
<v Speaker 2>pass a strong electric current directly through that water, a.

905
00:44:09.840 --> 00:44:14.119
<v Speaker 3>Simple, well understood process called electrolysis. When you pass electricity

906
00:44:14.119 --> 00:44:17.000
<v Speaker 3>through water, you break the chemical bonds. You split the

907
00:44:17.000 --> 00:44:21.079
<v Speaker 3>water molecule apart into its constituent gases hydrogen gas and

908
00:44:21.159 --> 00:44:22.039
<v Speaker 3>oxygen gas.

909
00:44:22.079 --> 00:44:23.880
<v Speaker 2>And what do you get when you capture a liquid

910
00:44:23.920 --> 00:44:27.199
<v Speaker 2>hydrogen and liquid oxygen, pipe them into a combustion chamber

911
00:44:27.199 --> 00:44:27.960
<v Speaker 2>and ignite them.

912
00:44:28.239 --> 00:44:33.440
<v Speaker 3>You get rocket fuel, specifically hydrolocks. It is the most powerful,

913
00:44:33.639 --> 00:44:37.920
<v Speaker 3>most efficient chemical propellant humanity currently possesses. It is the

914
00:44:37.960 --> 00:44:40.480
<v Speaker 3>exact same fuel that powered the Space Shuttle main engines

915
00:44:40.519 --> 00:44:44.239
<v Speaker 3>in the core stage of the massive Artemis SLS rocket.

916
00:44:44.599 --> 00:44:47.599
<v Speaker 2>This is the absolute game changer for human expansion. If

917
00:44:47.639 --> 00:44:51.639
<v Speaker 2>we find abundant accessible water on the Moon, and we

918
00:44:51.719 --> 00:44:54.639
<v Speaker 2>use solar power to refine it into fuel. The Moon

919
00:44:54.719 --> 00:44:57.400
<v Speaker 2>stops being just a remote scientific outpost.

920
00:44:57.559 --> 00:44:59.440
<v Speaker 3>It becomes a cosmic gas station exactly.

921
00:44:59.480 --> 00:45:02.159
<v Speaker 2>It becomes the critical port from which we launch massive

922
00:45:02.159 --> 00:45:06.039
<v Speaker 2>missions to Mars, the Asteroid Belt, and the outer Solar System.

923
00:45:05.800 --> 00:45:09.079
<v Speaker 3>Because the economics of space travel completely change at that point.

924
00:45:09.320 --> 00:45:12.320
<v Speaker 3>Launching a fully fueled massive rocket from the deep gravity

925
00:45:12.320 --> 00:45:15.119
<v Speaker 3>well of Earth requires an agonizing amount of energy.

926
00:45:15.199 --> 00:45:17.079
<v Speaker 2>It's so hard to get off this planet.

927
00:45:16.800 --> 00:45:19.360
<v Speaker 3>It really is. But launching that same rocket from the Moon,

928
00:45:19.440 --> 00:45:21.800
<v Speaker 3>which has only one sixth of Earth's gravity and no

929
00:45:21.880 --> 00:45:25.519
<v Speaker 3>atmospheric drag to fight against it, takes a tiny fraction

930
00:45:25.599 --> 00:45:28.119
<v Speaker 3>of the fuel. You can launch massive payloads across the

931
00:45:28.159 --> 00:45:30.559
<v Speaker 3>Solar System if you just fuel up at the Moon first.

932
00:45:30.880 --> 00:45:33.679
<v Speaker 2>But we can only turn the Moon into a gas station,

933
00:45:33.840 --> 00:45:36.800
<v Speaker 2>a shipyard, and a permanent thriving colony if we know

934
00:45:36.880 --> 00:45:39.920
<v Speaker 2>exactly where the resources are physically located exactly.

935
00:45:40.159 --> 00:45:42.039
<v Speaker 3>And that brings us to the ultimate impact of the

936
00:45:42.039 --> 00:45:42.880
<v Speaker 3>TM emission.

937
00:45:43.280 --> 00:45:46.000
<v Speaker 2>So what does this all mean for the immediate future

938
00:45:46.039 --> 00:45:49.000
<v Speaker 2>of the Artemis program? If we send this ten kilogram

939
00:45:49.199 --> 00:45:52.559
<v Speaker 2>micropoor array up into orbit and it spends a few

940
00:45:52.639 --> 00:45:56.920
<v Speaker 2>years meticulously mapping the surface, reading the atomic fingerprints triggered

941
00:45:56.920 --> 00:45:58.199
<v Speaker 2>by solar flares.

942
00:45:57.880 --> 00:45:59.679
<v Speaker 3>And it builds that complete map.

943
00:45:59.639 --> 00:46:02.719
<v Speaker 2>Right and what if it finds incredibly high concentrations of

944
00:46:02.800 --> 00:46:07.159
<v Speaker 2>water related compounds or easily accessible shallow veins of structural

945
00:46:07.199 --> 00:46:11.719
<v Speaker 2>titanium in a specific, unexpected region. Does this fundamentally change

946
00:46:11.760 --> 00:46:14.599
<v Speaker 2>where humanity decides to build its first permanent base.

947
00:46:14.840 --> 00:46:17.719
<v Speaker 3>I would argue it changes everything. Right now, almost all

948
00:46:17.760 --> 00:46:20.639
<v Speaker 3>the focus for Artemis is targeted at the lunar South Pole.

949
00:46:20.719 --> 00:46:21.719
<v Speaker 2>Why the South Pole.

950
00:46:21.599 --> 00:46:24.880
<v Speaker 3>Because radar and neutron spectrometers have hinted at the presence

951
00:46:24.920 --> 00:46:28.880
<v Speaker 3>of water ice hidden deep inside permanently shadowed craters there.

952
00:46:29.079 --> 00:46:32.800
<v Speaker 2>But I've read about those craters. They are nightmarish environments

953
00:46:32.840 --> 00:46:36.559
<v Speaker 2>to operate in. They are freezing, plunged in eternal darkness,

954
00:46:37.000 --> 00:46:41.039
<v Speaker 2>and the terrain is incredibly rugged and dangerous for landers

955
00:46:41.079 --> 00:46:41.679
<v Speaker 2>and rovers.

956
00:46:41.800 --> 00:46:45.639
<v Speaker 3>They are arguably the most hostile environment we could possibly

957
00:46:45.719 --> 00:46:48.880
<v Speaker 3>choose to build our first colony. We are targeting them

958
00:46:48.920 --> 00:46:51.280
<v Speaker 3>out of desperation, basically because we think that's where the

959
00:46:51.320 --> 00:46:51.960
<v Speaker 3>only water is.

960
00:46:52.000 --> 00:46:53.320
<v Speaker 2>Oh, what if the map changes that?

961
00:46:53.599 --> 00:46:57.079
<v Speaker 3>What if the high resolution global chemical map generated by

962
00:46:57.199 --> 00:47:01.199
<v Speaker 3>TOYDA and the Ezoe's telescope reveals a completeletely different reality.

963
00:47:01.679 --> 00:47:05.440
<v Speaker 3>What if it finds a massive, easily extractable concentration of

964
00:47:05.559 --> 00:47:09.320
<v Speaker 3>vital elements right near the equator in a flat, safe

965
00:47:09.360 --> 00:47:13.360
<v Speaker 3>area bathed in constant, predictable sunlight for endless solar power.

966
00:47:14.000 --> 00:47:15.599
<v Speaker 2>The map dictates the real estate.

967
00:47:15.760 --> 00:47:19.639
<v Speaker 3>The map is everything. This data is essentially the ultimate

968
00:47:19.679 --> 00:47:22.760
<v Speaker 3>real estate guide for future lunar colonies. You do not

969
00:47:22.840 --> 00:47:25.800
<v Speaker 3>build a massive, complex mining town in a perilous ravine

970
00:47:25.800 --> 00:47:27.679
<v Speaker 3>if there's no gold there. You build it where the

971
00:47:27.719 --> 00:47:30.320
<v Speaker 3>resources are richest, safest, and most accessible.

972
00:47:30.440 --> 00:47:31.360
<v Speaker 2>It makes perfect sense.

973
00:47:31.599 --> 00:47:36.440
<v Speaker 3>The data provided by this specific revolutionary technological breakthrough from

974
00:47:36.480 --> 00:47:40.920
<v Speaker 3>Tokyo Metropolitan University will be the foundational text that mission

975
00:47:40.960 --> 00:47:46.480
<v Speaker 3>planners at NASA, EASA, JXAS, and commercial spaceflight companies use

976
00:47:46.760 --> 00:47:50.159
<v Speaker 3>to literally draw the physical borders of humanity's first off

977
00:47:50.199 --> 00:47:51.039
<v Speaker 3>world settlements.

978
00:47:51.119 --> 00:47:53.039
<v Speaker 2>It is stunning to take a step back and think

979
00:47:53.079 --> 00:47:54.119
<v Speaker 2>about the chain of events.

980
00:47:54.119 --> 00:47:54.400
<v Speaker 3>Here.

981
00:47:54.639 --> 00:47:56.960
<v Speaker 2>We are talking about a piece of technology that weighs

982
00:47:57.039 --> 00:48:00.000
<v Speaker 2>less than a bag of groceries, a piece of technology

983
00:48:00.079 --> 00:48:02.920
<v Speaker 2>that was originally designed for a completely different purpose to

984
00:48:02.960 --> 00:48:05.760
<v Speaker 2>look at Earth's magnetic field and solar wind interactions.

985
00:48:05.840 --> 00:48:07.280
<v Speaker 3>This incredible pivot.

986
00:48:07.039 --> 00:48:10.760
<v Speaker 2>But through brilliant observation and adaptation, it pivots to lunar orbit,

987
00:48:11.360 --> 00:48:13.719
<v Speaker 2>uses the violent eruptions of the Sun as a tool,

988
00:48:14.159 --> 00:48:17.199
<v Speaker 2>maps the atomic history of a dead world, and ultimately

989
00:48:17.239 --> 00:48:20.320
<v Speaker 2>becomes the compass that guides humanity's permanent settlement of the

990
00:48:20.360 --> 00:48:21.119
<v Speaker 2>Solar System.

991
00:48:21.239 --> 00:48:24.360
<v Speaker 3>It is the perfect beautiful example of how the scientific

992
00:48:24.400 --> 00:48:28.239
<v Speaker 3>pursuit operates. Discovery is rarely a straight line, It really

993
00:48:28.280 --> 00:48:32.039
<v Speaker 3>Isn't You solve a complex engineering problem in one specific field,

994
00:48:32.519 --> 00:48:34.760
<v Speaker 3>like how to make a lightweight X ray sensor for

995
00:48:34.800 --> 00:48:38.840
<v Speaker 3>the magnetosphere, and it unexpectedly unlocks the door to a

996
00:48:38.880 --> 00:48:44.239
<v Speaker 3>completely different monumental achievement in planetary geology and human survival.

997
00:48:44.320 --> 00:48:47.840
<v Speaker 2>Tools like this compact X ray telescope are the absolutely

998
00:48:47.880 --> 00:48:52.280
<v Speaker 2>necessary precursors to humanity transitioning from a single planet species

999
00:48:52.320 --> 00:48:55.199
<v Speaker 2>into a true multiplanetary civilization.

1000
00:48:55.480 --> 00:48:56.440
<v Speaker 3>They absolutely are.

1001
00:48:56.599 --> 00:48:59.559
<v Speaker 2>Okay, let's take a breath and recap the incredible multi

1002
00:48:59.599 --> 00:49:02.559
<v Speaker 2>billion year journey we've just been on today. We started

1003
00:49:02.599 --> 00:49:06.920
<v Speaker 2>with a ten kilogram bundle of microscopic square pores, a

1004
00:49:07.079 --> 00:49:10.400
<v Speaker 2>brilliant pivot by the team at Tokyo Metropolitan University that

1005
00:49:10.519 --> 00:49:13.480
<v Speaker 2>solved the crushing weight problem of traditional X ray astronomy.

1006
00:49:13.519 --> 00:49:16.039
<v Speaker 3>We explore the deep quantum mechanics of how this tiny

1007
00:49:16.159 --> 00:49:20.440
<v Speaker 3>array utilizes the violent, unpredictable solar flares of our Sun

1008
00:49:20.800 --> 00:49:22.599
<v Speaker 3>as a cosmic flashlight.

1009
00:49:22.239 --> 00:49:26.000
<v Speaker 2>Triggering microscopic atomic reactions to reveal the invisible fingerprints of

1010
00:49:26.039 --> 00:49:26.719
<v Speaker 2>the lunar dust.

1011
00:49:26.920 --> 00:49:30.639
<v Speaker 3>We saw how those specific fingerprints oxygen, magnesium, aluminum, silicon

1012
00:49:30.679 --> 00:49:33.519
<v Speaker 3>allow us to peel back billions of years of silent.

1013
00:49:33.239 --> 00:49:36.880
<v Speaker 2>History, revealing the chaotic story of a molten magma ocean,

1014
00:49:37.119 --> 00:49:42.119
<v Speaker 2>planetary differentiation driven by gravity and cataclysmic asteroid impacts that

1015
00:49:42.199 --> 00:49:44.400
<v Speaker 2>relentlessly churned the lunar crust.

1016
00:49:44.559 --> 00:49:48.360
<v Speaker 3>And finally, we connected that ancient, violent history to our

1017
00:49:48.639 --> 00:49:50.840
<v Speaker 3>immediate ambitious future.

1018
00:49:50.760 --> 00:49:54.039
<v Speaker 2>Seeing how mapping those exact same elements will guide the

1019
00:49:54.119 --> 00:49:58.000
<v Speaker 2>artemis missions, locate the vital resources needed for NC two

1020
00:49:58.039 --> 00:50:02.519
<v Speaker 2>resource utilization, and really draw the map for where humanity

1021
00:50:02.519 --> 00:50:05.840
<v Speaker 2>will build its permanent homes on the Moon. It is

1022
00:50:05.840 --> 00:50:11.599
<v Speaker 2>a profound convergence of cutting edge engineering, deep astrophysics, ancient geology,

1023
00:50:11.920 --> 00:50:13.360
<v Speaker 2>and bold human ambition.

1024
00:50:13.639 --> 00:50:16.559
<v Speaker 3>It represents a turning point in our relationship with the cosmos.

1025
00:50:16.599 --> 00:50:18.480
<v Speaker 2>It really does, and before we wrap up today, I

1026
00:50:18.480 --> 00:50:21.360
<v Speaker 2>want to leave you with one final mind expanding idea

1027
00:50:21.400 --> 00:50:24.039
<v Speaker 2>to ponder. We spend this entire time talking about the Moon,

1028
00:50:24.079 --> 00:50:26.440
<v Speaker 2>our closest neighbor, but think about the scale and the

1029
00:50:26.480 --> 00:50:27.920
<v Speaker 2>modularity of this new text.

1030
00:50:28.000 --> 00:50:29.400
<v Speaker 3>Oh, this is the really exciting part.

1031
00:50:29.519 --> 00:50:32.880
<v Speaker 2>If a single ten kilogram telescope array can map the

1032
00:50:33.039 --> 00:50:36.400
<v Speaker 2>entire chemical composition of an entire Moon using just the

1033
00:50:36.440 --> 00:50:39.960
<v Speaker 2>ambient background radiation of our Sun, what happens next?

1034
00:50:40.239 --> 00:50:42.719
<v Speaker 3>The implications for the rest of the Solar System are staggering.

1035
00:50:42.840 --> 00:50:45.880
<v Speaker 2>Imagine what happens when we start mass producing these tiny,

1036
00:50:46.280 --> 00:50:49.559
<v Speaker 2>highly efficient micropore sensors. We do not have to stop

1037
00:50:49.559 --> 00:50:52.400
<v Speaker 2>at the Moon. What happens when we send swarms of

1038
00:50:52.440 --> 00:50:56.440
<v Speaker 2>these arrays out to map the thousands of unprobed asteroids

1039
00:50:56.480 --> 00:51:00.719
<v Speaker 2>in the main asteroid belt looking for incredibly valuable deposits

1040
00:51:00.760 --> 00:51:03.519
<v Speaker 2>of platinum, palladium, and rare earth metals.

1041
00:51:03.599 --> 00:51:04.920
<v Speaker 3>We're sending them further out.

1042
00:51:05.079 --> 00:51:08.000
<v Speaker 2>Exactly what happens when we send them into orbit around

1043
00:51:08.039 --> 00:51:11.920
<v Speaker 2>Phobos and Deimos, the tiny mysterious moons of Mars, to

1044
00:51:11.960 --> 00:51:14.760
<v Speaker 2>see if they hold the specific resources we need to

1045
00:51:14.880 --> 00:51:17.559
<v Speaker 2>fuel and build a sprawling Martian colony.

1046
00:51:17.639 --> 00:51:20.719
<v Speaker 3>Because they are so incredibly lightweight and draw so little power.

1047
00:51:20.960 --> 00:51:25.519
<v Speaker 3>They do not require massive, multi billion dollar flagship missions

1048
00:51:25.519 --> 00:51:27.679
<v Speaker 3>of their own. They can simply hitch a ride as

1049
00:51:27.719 --> 00:51:31.239
<v Speaker 3>secondary payloads on almost any interplanetary probe we launch in

1050
00:51:31.280 --> 00:51:31.679
<v Speaker 3>the future.

1051
00:51:31.719 --> 00:51:33.159
<v Speaker 2>They just become standard equipment.

1052
00:51:33.280 --> 00:51:33.719
<v Speaker 3>Exactly.

1053
00:51:33.719 --> 00:51:35.800
<v Speaker 2>We aren't just looking at a new way to understand

1054
00:51:35.840 --> 00:51:39.360
<v Speaker 2>our moon. We are looking at the exact blueprint for

1055
00:51:39.400 --> 00:51:43.679
<v Speaker 2>how humanity will eventually prospect, map, and utilize the entire

1056
00:51:43.719 --> 00:51:47.559
<v Speaker 2>solar system. The technology developed by Toyda and Ezo is

1057
00:51:47.599 --> 00:51:50.079
<v Speaker 2>the key that unlocks the door to an age of

1058
00:51:50.239 --> 00:51:53.079
<v Speaker 2>true sustainable cosmic exploration.

1059
00:51:53.360 --> 00:51:56.599
<v Speaker 3>It changes our relationship with space from one of brief,

1060
00:51:56.920 --> 00:52:01.519
<v Speaker 3>tentative observation to one of deep, sustainable interaction. We move

1061
00:52:01.559 --> 00:52:04.760
<v Speaker 3>from being temporary visitors to becoming permanent residents.

1062
00:52:04.800 --> 00:52:06.679
<v Speaker 2>And it all starts with looking at things just a

1063
00:52:06.760 --> 00:52:09.239
<v Speaker 2>little differently, taking the tools we have and applying them

1064
00:52:09.280 --> 00:52:12.079
<v Speaker 2>in bold new ways. Thank you so much for joining

1065
00:52:12.159 --> 00:52:14.800
<v Speaker 2>us on this exploration today. The next time you step

1066
00:52:14.840 --> 00:52:17.079
<v Speaker 2>outside on a clear night and look up at that

1067
00:52:17.239 --> 00:52:20.840
<v Speaker 2>seemingly dead, dusty, gray sphere in the sky, I want

1068
00:52:20.840 --> 00:52:23.719
<v Speaker 2>you to remember what is really up there. Think about

1069
00:52:23.760 --> 00:52:26.840
<v Speaker 2>the hidden elements, think about the atomic fingerprints waiting to

1070
00:52:26.840 --> 00:52:29.199
<v Speaker 2>be illuminated by the fire of the sun, and keep

1071
00:52:29.239 --> 00:52:32.440
<v Speaker 2>wondering what vibrant hidden colors are glowing right beneath the dust,

1072
00:52:32.719 --> 00:52:34.920
<v Speaker 2>waiting for us to finally put on the magic glasses

1073
00:52:34.960 --> 00:52:35.480
<v Speaker 2>and see them
