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>So I want you to imagine stepping outside tomorrow morning.

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<v Speaker 2>You know you've got your coffee in hand.

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<v Speaker 3>That's time of the day.

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<v Speaker 2>Oh absolutely, So you walk out onto your porch, you

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<v Speaker 2>look up at the morning sky, and instead of our

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<v Speaker 2>single familiar yellow sugn just kind of rising in the east, right,

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<v Speaker 2>you see five massive burning spheres of plasma just right

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<v Speaker 2>there in the sky.

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<v Speaker 3>That would definitely wake you up faster than the coffee.

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<v Speaker 2>Right. I mean, they'd be casting these multiple overlapping shadows

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<v Speaker 2>on your lawn. You'd have different hues of orange and

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<v Speaker 2>red and this stark, blinding white.

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<v Speaker 3>It sounds like a backdrop for a massive space opera.

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<v Speaker 2>Or something exactly like something cooked up into sci fi

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<v Speaker 2>writer's room. But the crazy thing is in our immediate

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<v Speaker 2>cosmic neighborhood. This is actually an absolute, ongoing reality.

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<v Speaker 3>Yeah, it really is. And I think you know our

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<v Speaker 3>daily experience waking up to just one sun that makes

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<v Speaker 3>its journey across the sky completely alone. It creates this massive,

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<v Speaker 3>ingrained psychological bias for us. We just naturally assume the

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<v Speaker 3>rest of the universe operates on this exact same single

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<v Speaker 3>sun blueprint, because.

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<v Speaker 2>That's all we know. But being a single star like

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<v Speaker 2>our sun actually makes us the absolute weirdos of the galaxy,

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<v Speaker 2>doesn't it.

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<v Speaker 3>We really are the odd ones out. I mean that

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<v Speaker 3>human experience is just incredibly localized. We project our solar

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<v Speaker 3>system's orderly, single anchor structure onto the rest of the.

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<v Speaker 2>Cosmos, which makes sense logically, sure it does.

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<v Speaker 3>But the sheer volume of stars out there that are

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<v Speaker 3>actively bound up in these complex gravitational relationships with other stars,

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<v Speaker 3>it's staggering.

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<v Speaker 2>It's a crowded universe out there.

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<v Speaker 3>Oh, Incredibly, the universe is a far more dynamic and

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<v Speaker 3>chaotic and just crowded environment than a casual glance at

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<v Speaker 3>our night sky would ever lead you to believe.

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<v Speaker 2>So today our mission is to basically dismantle that bias completely.

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<v Speaker 2>We're going to map out the precise relationship statuses of

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<v Speaker 2>the star's closest.

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<v Speaker 3>To us, which is such a fascinating project, it really is.

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<v Speaker 2>Astronomers the University Madrid have just completed this incredible, definitive

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<v Speaker 2>census of our local cosmic neighborhood and they're combining you know,

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<v Speaker 2>modern space telescope data with century old catalogs.

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<v Speaker 3>And we are going to explore exactly who is paired up,

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<v Speaker 3>who is flying solo and why. Untangling these incredibly complex

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<v Speaker 3>stellar relationships is so important.

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<v Speaker 2>Right because it's essentially the ultimate prerequisite for one of

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<v Speaker 2>the greatest quests in human history, which is finding a.

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<v Speaker 3>Second Earth exactly. I mean, if the ultimate goal is

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<v Speaker 3>to find habitable planets, you know, worlds where liquid water

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<v Speaker 3>could exist and life might thrive, we first have to

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<v Speaker 3>thoroughly understand the stars those planets might be orbiting.

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<v Speaker 2>You can't just blindly point a telescope and hope for

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<v Speaker 2>the best.

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<v Speaker 3>No, you really can't. The only way to build that

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<v Speaker 3>understanding is to know exactly what is happening in our

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<v Speaker 3>own backyard. We cannot filter the noise of the deep

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<v Speaker 3>universe if we do not even know who is living

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<v Speaker 3>next door.

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<v Speaker 2>Okay, so let's start by defining that backyard. Yeah, because

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<v Speaker 2>we need a boundary, right, We can't just say nearby.

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<v Speaker 3>In astronomy, nearby could mean a million light years.

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<v Speaker 2>Yeah, exactly. So the astronomers compiling this definitive map, they

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<v Speaker 2>do this highly specific mathematical bubble around our solar system.

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<v Speaker 2>The boundary is set at exactly ten parsecs away.

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<v Speaker 3>From the Sun, extending in every single direction to form

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<v Speaker 3>a perfect sphere.

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<v Speaker 2>Right, and for anyone doing the cosmic math at home,

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<v Speaker 2>ten parsecs translates to thirty two point six light years.

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<v Speaker 3>Which is a very specific number.

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<v Speaker 2>It is, and inside this specific ten carsec bubble there

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<v Speaker 2>are exactly four hundred twenty four known stellar and substellar objects.

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<v Speaker 2>But I mean thirty two point six light years feels

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<v Speaker 2>strangely arbitrary.

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<v Speaker 3>It does sound random at first.

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<v Speaker 2>Yeah, because the Milky Way Galaxy is over one hundred

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<v Speaker 2>thousand light years across. So why draw the lines so

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<v Speaker 2>close to home? Why ten parsecs?

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<v Speaker 3>Well, it all comes down to this foundational concept in

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<v Speaker 3>observational astronomy, which is completeness.

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<v Speaker 2>Completeness meaning we know everything that's.

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<v Speaker 3>In there exactly. The primary enemy of any astronomical survey

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<v Speaker 3>is distance. The further out into the galaxy you look,

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<v Speaker 3>the harder it becomes to visually resolve the fine details

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<v Speaker 3>of a star system.

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<v Speaker 2>Like trying to see the details of a car from

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<v Speaker 2>ten miles away.

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<v Speaker 3>Precisely, it becomes intensely mathematically difficult to see whether a

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<v Speaker 3>star has a companion hidden right next to it, because

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<v Speaker 3>it just gets lost in the blinding glare of the

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<v Speaker 3>primary star.

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<v Speaker 2>You know, I was thinking about this like a neighborhood

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<v Speaker 2>watch program.

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<v Speaker 3>Oh I like that?

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<v Speaker 2>How so well, it's incredibly easy to know exactly who

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<v Speaker 2>lives on your own street. Right, you see your neighbors

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<v Speaker 2>taking out the trash, You recognize their You know exactly

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<v Speaker 2>who lives in which house. Sure, you might even have

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<v Speaker 2>a pretty good read on the street behind yours, But

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<v Speaker 2>if you try to figure out who is permanently crashing

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<v Speaker 2>on the couch of a house like three towns away.

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<v Speaker 3>You wouldn't have a clue exactly.

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<v Speaker 2>From where you're standing. It is completely impossible. You just

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<v Speaker 2>cannot see through the structural noise of the intervening houses

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<v Speaker 2>and the distance to know for sure.

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<v Speaker 3>That captures the structural problem perfectly, expanding the bubble to

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<v Speaker 3>say fifty or one hundred parsecs would introduce a massive

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<v Speaker 3>amount of uncertainty into the data.

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<v Speaker 2>We just start missing the cosmic couch surfers.

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<v Speaker 3>Exactly, We would start missing things. By strictly limiting the

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<v Speaker 3>boundary to exactly ten parsecs, astronomers can mathematically lower the

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<v Speaker 3>probability of missing those starry companions that are hiding in

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<v Speaker 3>the wings.

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<v Speaker 2>So it's about confidence in the data, oh, one hundred percent.

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<v Speaker 3>This constraint allows for a very high degree of statistical

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<v Speaker 3>confidence the map is considered complete. We know we haven't

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<v Speaker 3>missed any hidden roommate.

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<v Speaker 2>Okay, but wait, that still doesn't quite add up for me.

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<v Speaker 3>Oh why not?

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<v Speaker 2>Because we currently have telescopes operating in space that are

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<v Speaker 2>sending back crystal clear, high definition images of galaxies that

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<v Speaker 2>are billions of late years away.

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<v Speaker 3>Oh right, like James Webb and Hubble.

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<v Speaker 2>Yeah, we are literally looking back in time to the

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<v Speaker 2>dawn of the universe. So if the optics exist to

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<v Speaker 2>capture a galaxy on the edge of the observable universe,

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<v Speaker 2>why is it mechanically so difficult to spot a single

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<v Speaker 2>companion star that is just say, fifteen parsex down the

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<v Speaker 2>cosmic street. That's a really great point right, Why does

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<v Speaker 2>the physics fall apart at such a relatively short distance.

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<v Speaker 3>Well, the distinction lies in what those telescopes are actually resolving.

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<v Speaker 3>When you look at a galaxy billions of late years away,

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<v Speaker 3>you are not resolving individual stars.

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<v Speaker 2>You're just seeing the whole thing at once.

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<v Speaker 3>Exactly, you are observing the combined massive glow of hundreds

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<v Speaker 3>of billions of stars spread out over an unfathomably huge area.

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<v Speaker 3>It's a massive smear of light.

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<v Speaker 2>Ok.

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<v Speaker 3>When you look at a star system just fifteen parsecs away,

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<v Speaker 3>you are trying to resolve a tiny, specific point source

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<v Speaker 3>of light.

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<v Speaker 2>You are looking for a single microscopic.

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<v Speaker 3>Dot, and that dot is unimaginably bright. I mean, stars

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<v Speaker 3>are colossal nuclear fusion engines. They create a blinding amount

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<v Speaker 3>of glare.

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<v Speaker 2>Right, They are just reflecting light, They're making.

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<v Speaker 3>It exactly so. If a companion star is orbiting relatively

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<v Speaker 3>close to a primary star, the light from the primary

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<v Speaker 3>completely washes out the dimmer companion.

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<v Speaker 2>Ah. I see.

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<v Speaker 3>Think of it like trying to spot a firefly hovering

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<v Speaker 3>three inches away from a stadium floodlight while you are

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<v Speaker 3>standing two miles down the road.

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<v Speaker 2>Oh wow, Yeah, the sheer volume of photons from the

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<v Speaker 2>floodlight would just utterly destroy your ability to perceive the

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<v Speaker 2>firefly exactly.

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<v Speaker 3>The firefly is completely swallowed by the visual noise.

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<v Speaker 2>So it's not a distance problem, it's a glare problem.

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<v Speaker 3>Precisely. This limitation is governed by something called angular resolution.

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<v Speaker 3>No matter how perfectly polished your telescope mirror is or

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<v Speaker 3>how advanced your sensors are, light ultimately behaves as a wave.

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<v Speaker 2>Right, So when light.

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<v Speaker 3>Waves past the edges of a telescope's aperture, they bend

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<v Speaker 3>and spread out. This is a phenomenon called diffraction diffraction, okay,

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<v Speaker 3>And this creates a tiny blur around every point of

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<v Speaker 3>light on the sensor. If two stars are too close

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<v Speaker 3>together in the sky, their diffraction blurs.

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<v Speaker 2>Overlap and they just merge into a single blob of

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<v Speaker 2>light exactly.

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<v Speaker 3>Keeping the sensus tightly constrained to ten parsecs means the

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<v Speaker 3>physical distance between the stars translates to a wide enough

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<v Speaker 3>angle in our sky. It ensures the floodlight and the

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<v Speaker 3>firefly appear far enough apart that our instruments can reliably

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<v Speaker 3>separate them.

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<v Speaker 2>Okay, that makes that urbitrainer would make total sense. It's

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<v Speaker 2>literally the physical limit of knowing our data is pure

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<v Speaker 2>exactly now, compiling a flawless map of four hundred and

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<v Speaker 2>twenty four objects isn't something you do by just pointing

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<v Speaker 2>a backyard telescope at the sky and taking notes, right,

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<v Speaker 2>Definitely not the data required to prove these objects exist,

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<v Speaker 2>and more importantly, to prove they are at interacting with

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<v Speaker 2>each other. That must be monumental.

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<v Speaker 3>Oh, it's staggering. The Census is the culmination of combining

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<v Speaker 3>two of the most sophisticated massive data sets ever compiled

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<v Speaker 3>by humanity.

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<v Speaker 2>Wow, what are they?

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<v Speaker 3>The structural backbone of this map comes from the d

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<v Speaker 3>R three data release from the European Space Agency's Gaya telescope.

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<v Speaker 2>Gaya, I've heard of that one.

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<v Speaker 3>It's an incredible piece of technology. Gaya is a space

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<v Speaker 3>observatory specifically designed for astrometry.

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<v Speaker 2>That's the precise measurement of where things.

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<v Speaker 3>Are, vacation distance, and motion exactly. Gaya is essentially building

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<v Speaker 3>a highly dynamic, three dimensional map of the entire Milky

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<v Speaker 3>Way Galaxy.

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<v Speaker 2>That's ambitious, very.

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<v Speaker 3>It measures the positions of over a billion stars with

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<v Speaker 3>a level of precision that is honestly difficult to overstate.

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<v Speaker 3>It can measure the width of a human hair from

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<v Speaker 3>hundreds of miles away.

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<v Speaker 2>Seriously, that is insane.

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<v Speaker 3>It's phenomenal engineering. But positional data is really only half

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<v Speaker 3>the puzzle.

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<v Speaker 2>Right, because just knowing where two stars are it doesn't

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<v Speaker 2>mean they are interacting exactly.

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<v Speaker 3>To know if stars are actually in a relationship, you

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<v Speaker 3>need movement over time. That is where the researcher is

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<v Speaker 3>brought in the Washington Double Star Catalog.

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<v Speaker 2>Now, I was looking at the history of the Washington

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<v Speaker 2>Double Star Catalog. It is fascinating because it isn't just

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<v Speaker 2>a modern digital list. It represents decades, even centuries of

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<v Speaker 2>human observation.

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<v Speaker 3>It really is a historical treasure. It's the world's principal

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<v Speaker 3>database of visual double stars. It actually contains historical observations

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<v Speaker 3>dating all the way back to the nineteenth century.

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<v Speaker 2>Wow, so people with early telescopes sketching things out basically.

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<v Speaker 3>Yeah, And that historical data is combined with decades of

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<v Speaker 3>modern radial velocity measurements.

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<v Speaker 2>Radio velocity being how fast a star is moving along

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<v Speaker 2>our line of sight, like either toward us or away

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<v Speaker 2>from us.

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<v Speaker 3>You've got it perfectly by fusing Guya's ultra precise three

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<v Speaker 3>D positioning. With the deep historical motion data from the

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<v Speaker 3>Washington Catalog, astronomers could trace the exact trey objectories of

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<v Speaker 3>these objects over time, so.

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<v Speaker 2>They can see the actual dance.

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<v Speaker 3>Yes, they could definitively prove which stars were locked in

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<v Speaker 3>a gravitational embrace and which were just optical illusions.

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<v Speaker 2>Optical illusions like stars that look close together from Earth

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<v Speaker 2>but are actually separated by vast distances in deep space.

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<v Speaker 3>Exactly we call those optical binaries. They just happen to

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<v Speaker 3>line up perfectly from our vantage point, but they have

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<v Speaker 3>nothing to do with each other.

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<v Speaker 2>Okay, so the ten Parsak bubble is set, the pristine

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<v Speaker 2>data is gathered, and all the false positives those optical

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<v Speaker 2>illusions are filtered out. Let's dig into the actual census results.

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<v Speaker 2>Let's do it. Who is actually paired up in our neighborhood.

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<v Speaker 2>Out of the four hundred and twenty four objects inside

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<v Speaker 2>this bubble, two hundred and fifteen of them are bound

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<v Speaker 2>up in multiple star systems, which means over half the

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<v Speaker 2>population is coupled up. Literally, more than half the neighborhood

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<v Speaker 2>is in a relationship, and they aren't just in simple pairs. Either.

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<v Speaker 3>No, it gets much more complicated.

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<v Speaker 2>These two hundred and fifteen objects are distributed across ninety

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<v Speaker 2>two distinct multiple star systems, and the structural breakdown of

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<v Speaker 2>these systems is shockingly diverse.

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<v Speaker 3>It really runs the gamut.

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<v Speaker 2>Right, So there are sixty eight classic double star systems,

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<v Speaker 2>you know, binaries. But then there are nineteen triple star systems.

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<v Speaker 3>Three stars all dancing together.

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<v Speaker 2>Yeah. And then there are three quadruple systems, and perhaps

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<v Speaker 2>the most mind bending of all, there are two incredibly

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<v Speaker 2>rare kintuple star systems. Five star, five separate stars, all

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<v Speaker 2>gravitationally bound to each other, existing is a single cohesive unit.

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<v Speaker 3>You know. Visualizing a system with five massive bodies of

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<v Speaker 3>burning plasma is challenging because our brains just naturally default

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<v Speaker 3>to our own solar system model.

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<v Speaker 2>Right. I was reading about the structural dynamics of these

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<v Speaker 2>quintuple systems and my mind went straight to how they

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<v Speaker 2>even organize themselves without crashing.

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<v Speaker 3>It's a delicate balance.

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<v Speaker 2>Because you can't just have five stars orbiting a single

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<v Speaker 2>point like a cosmic merry ground.

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<v Speaker 3>Right.

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<v Speaker 2>The n body problem in physics dictates that throwing five

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<v Speaker 2>massive objects into a random clump just results in pure.

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<v Speaker 3>Chaos, absolute chaos. They would violently fling each other.

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<v Speaker 2>Yeah, they completely destabilize the orbits until the system either

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<v Speaker 2>collapsed inward on itself or forcefully ejected stars out into

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<v Speaker 2>deep space.

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<v Speaker 3>Exactly. So, to survive for billions of years, gravity forces

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<v Speaker 3>them into highly organized, compartmentalized layers.

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<v Speaker 2>What's the term for that.

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<v Speaker 3>It's called a hierarchical structure. They do not orbit a

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<v Speaker 3>central star. They orbit a shared center of mass, a

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<v Speaker 3>shared center, yes, and there's a barry center. And they

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<v Speaker 3>do this through nested levels of organization.

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<v Speaker 2>Nested levels. You know. It reminds me of the intricate

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<v Speaker 2>gears inside of mechanical Swiss watch.

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<v Speaker 3>Oh that's a brilliant comparison.

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<v Speaker 2>Because you don't have five gears all grinding against the

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<v Speaker 2>exact same central axle. You have a massive, slow moving

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<v Speaker 2>outer gear, and then nested inside that you have small

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<v Speaker 2>assemblies spinning independently, and within those even tighter, faster moving parts.

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<v Speaker 3>The watch analogy perfectly captures the mechanics. So in a

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<v Speaker 3>quintuple system, you might have two stars in a very

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<v Speaker 3>tight binary orbits circling each other.

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<v Speaker 2>Rapidly, like the ticking secondhand.

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<v Speaker 3>Exactly, then a massive distance away, but still within the

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<v Speaker 3>exact same system. You have another tight binary pair.

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<v Speaker 2>Okay, two separate pairs, Yes, And those.

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00:14:11.919 --> 00:14:14.639
<v Speaker 3>Two separate binary pairs will then orbit each other.

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<v Speaker 2>Wait, the pairs orbit each other.

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00:14:16.759 --> 00:14:20.559
<v Speaker 3>Yes, The gravitational center of pair A orbits the gravitational

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<v Speaker 3>center of pair B. They treat the other pair almost

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<v Speaker 3>as if it were a single extra heavy star.

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00:14:26.039 --> 00:14:29.919
<v Speaker 2>Orbiting pairs of orbiting pairs. That is dizzying. And the

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<v Speaker 2>fifth star.

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00:14:30.799 --> 00:14:34.320
<v Speaker 3>The fifth star is often situated in an incredibly wide orbit,

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00:14:34.799 --> 00:14:38.360
<v Speaker 3>just slowly circling the entire inner quadruple structure from a

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00:14:38.399 --> 00:14:39.639
<v Speaker 3>massive distance.

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00:14:39.320 --> 00:14:41.000
<v Speaker 2>Like the outer casing of the watch.

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00:14:40.879 --> 00:14:44.320
<v Speaker 3>Exactly, moving at a glacial pace compared to the rapid

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<v Speaker 3>ticking of the inner binaries. And the sheer vastness of

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<v Speaker 3>space between these hierarchical levels is actually what preserves.

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<v Speaker 2>The system, because they're kept far enough apart to not interfere.

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<v Speaker 3>Right, the gravitational forces at play locally within a tight

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00:14:57.799 --> 00:15:01.000
<v Speaker 3>binary are intense, but because the what X structural level

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<v Speaker 3>is located so far away that competing gravitational poll is diluted.

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<v Speaker 2>Ah I see, they establish a long term stable resonance Chris.

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<v Speaker 2>But Okay, if I am a planet in one of

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<v Speaker 2>these quadruple or quintuple systems, what does my existence even

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<v Speaker 2>look like with all these competing gravitational wells. Do planets

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00:15:19.559 --> 00:15:22.519
<v Speaker 2>even survive in these environments? Or are they just shredded

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<v Speaker 2>into asteroid belts.

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00:15:24.200 --> 00:15:27.440
<v Speaker 3>It's a rough neighborhood for a planet. The gravitational environment

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00:15:27.559 --> 00:15:32.639
<v Speaker 3>is incredibly hostile unless they settle into very specific mathematically

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<v Speaker 3>safe zones. Safe zones like where well a planet can

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<v Speaker 3>survive if it is in an extremely tight close orbit

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00:15:40.320 --> 00:15:43.480
<v Speaker 3>around just one of the individual stars. In that scenario,

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<v Speaker 3>it effectively ignores the distant pole of the other stars

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<v Speaker 3>in the system.

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00:15:47.639 --> 00:15:50.279
<v Speaker 2>It just hugs its parent star really tightly exactly.

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<v Speaker 3>Or on the flip side, a planet can exist in

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<v Speaker 3>a circumbinary orbit.

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<v Speaker 2>Circumbinary meaning orbiting the whole.

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00:15:56.399 --> 00:15:59.919
<v Speaker 3>Thing right, orbiting incredibly far away from the entire complex,

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<v Speaker 3>treating the inner mess of stars as a single gravitational point.

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00:16:03.440 --> 00:16:05.559
<v Speaker 2>Okay, so way inside or way outside.

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00:16:05.159 --> 00:16:07.840
<v Speaker 3>Exactly anything in the middle ground, the spaces between the

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00:16:07.879 --> 00:16:11.080
<v Speaker 3>interacting stars. That is a dynamically unstable death.

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00:16:10.919 --> 00:16:12.360
<v Speaker 2>Zone, a death zone.

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00:16:12.399 --> 00:16:15.240
<v Speaker 3>A planet caught there would eventually be ejected from the

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00:16:15.240 --> 00:16:19.759
<v Speaker 3>system entirely or pulled into a catastrophic collision course with

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00:16:19.840 --> 00:16:20.440
<v Speaker 3>a star.

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00:16:20.519 --> 00:16:23.799
<v Speaker 2>So no middle ground. The mechanics are just awe inspiring.

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00:16:24.440 --> 00:16:27.759
<v Speaker 2>But you know, beyond just mapping the structures, the Census

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<v Speaker 2>revealed this really striking mathematical rule about who actually ends

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<v Speaker 2>up in these complex relationships.

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00:16:34.000 --> 00:16:37.320
<v Speaker 3>Oh, yes, the relationship between mass and multiplicity.

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00:16:37.600 --> 00:16:41.240
<v Speaker 2>Right, there is a definitive, unyielding link between a star's

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00:16:41.320 --> 00:16:43.279
<v Speaker 2>mass and its relationship status.

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00:16:43.320 --> 00:16:44.279
<v Speaker 3>It's fascinating.

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<v Speaker 2>If a star is categorized as a heavyweight, meaning it

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00:16:47.279 --> 00:16:50.120
<v Speaker 2>possesses more than half the mass of our Sun, it

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<v Speaker 2>has a massive forty one percent chance of being paired

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<v Speaker 2>up with at least one companion.

354
00:16:53.919 --> 00:16:58.080
<v Speaker 3>Almost a coin flip. Mass dictates cosmic sociability. The heavier

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00:16:58.120 --> 00:16:59.840
<v Speaker 3>the star, the more likely it is to exist in

356
00:16:59.879 --> 00:17:00.840
<v Speaker 3>a complex system.

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00:17:00.960 --> 00:17:03.360
<v Speaker 2>But then the complete opposite is true for the lightweights.

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<v Speaker 2>We're talking about objects under point one solar masses.

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00:17:06.480 --> 00:17:08.319
<v Speaker 3>Right, the red dwarfs and the brown dwarfs.

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00:17:08.400 --> 00:17:11.240
<v Speaker 2>Yeah, for these lightweights, the fraction of being found in

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<v Speaker 2>a multi star system absolutely plummets. It drops all the

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00:17:14.240 --> 00:17:16.640
<v Speaker 2>way down to just nine percent. They actively seem to

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<v Speaker 2>avoid entanglements, and that.

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00:17:18.880 --> 00:17:22.319
<v Speaker 3>Massive statistical drop off from forty one percent down to

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00:17:22.440 --> 00:17:26.839
<v Speaker 3>nine percent is not just a quirk of our local neighborhood. No, No,

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<v Speaker 3>it provides crucial forensic evidence for one of the most

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<v Speaker 3>intense ongoing debates in stellar astrophysics, the mystery of how

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<v Speaker 3>substellar objects actually form.

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00:17:39.119 --> 00:17:42.759
<v Speaker 2>The first place interesting because I look at gravity like

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<v Speaker 2>a form of cosmic social currency.

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<v Speaker 3>Social currency.

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00:17:45.759 --> 00:17:49.599
<v Speaker 2>Yeah, Like, the heavier you are, the more gravitational charisma

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<v Speaker 2>you possess, you can attract other bodies, lock them into orbit,

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<v Speaker 2>and basically hold on to them through the chaotic early

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<v Speaker 2>days of star formation.

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00:17:56.799 --> 00:17:59.640
<v Speaker 3>That's a great way to visualize it. The heavyweights clearly

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00:17:59.680 --> 00:18:00.480
<v Speaker 3>have that currency.

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00:18:00.519 --> 00:18:03.359
<v Speaker 2>They travel in packs, right, But it begs the question

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<v Speaker 2>regarding these tiny red and brown dwarfs. Are they born

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00:18:06.799 --> 00:18:09.720
<v Speaker 2>alone because they simply lack the gravitational mass to attract

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00:18:09.759 --> 00:18:12.359
<v Speaker 2>a partner, or is something more violent happening?

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00:18:12.480 --> 00:18:13.000
<v Speaker 3>More violent?

383
00:18:13.039 --> 00:18:15.160
<v Speaker 2>Could they have been born into a larger group dynamic

384
00:18:15.160 --> 00:18:16.319
<v Speaker 2>and then violently kicked out.

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00:18:16.400 --> 00:18:18.880
<v Speaker 3>Well, you are outlining the two leading models for brown

386
00:18:18.960 --> 00:18:23.000
<v Speaker 3>dwarf formation right there. Oh yep. But to understand the debate,

387
00:18:23.160 --> 00:18:25.400
<v Speaker 3>you first have to look at what a brown dwarf

388
00:18:25.480 --> 00:18:29.440
<v Speaker 3>actually is. It is the ultimate cosmic tweener, a.

389
00:18:29.480 --> 00:18:32.279
<v Speaker 2>Tweener, not a planet, not a star exactly.

390
00:18:32.640 --> 00:18:35.839
<v Speaker 3>It is significantly more massive than a gas giant planet

391
00:18:35.880 --> 00:18:38.720
<v Speaker 3>like Jupiter, but it does not have quite enough mass

392
00:18:38.799 --> 00:18:44.240
<v Speaker 3>to generate the core pressure needed to ignite sustained nuclear fusion.

393
00:18:43.880 --> 00:18:45.720
<v Speaker 2>Of hydrogen, so it never caught fire.

394
00:18:45.920 --> 00:18:49.519
<v Speaker 3>Right. It glows faintly from the residual heat of its formation,

395
00:18:50.039 --> 00:18:53.759
<v Speaker 3>but it is not a true hydrogen burning stars kind

396
00:18:53.759 --> 00:18:57.920
<v Speaker 3>of smoldering exactly. Now, consider the birthplace of stars. They

397
00:18:57.960 --> 00:19:01.640
<v Speaker 3>form in these massive freezing cloud clouds of interstellar gas

398
00:19:01.680 --> 00:19:03.640
<v Speaker 3>and dust called molecular.

399
00:19:03.079 --> 00:19:05.279
<v Speaker 2>Clouds, okay, giant freezing clouds, right.

400
00:19:05.559 --> 00:19:08.039
<v Speaker 3>And as these clouds collapse under their own gravity, they

401
00:19:08.079 --> 00:19:12.519
<v Speaker 3>do not form a single smooth sphere. They fragment into dozens, hundreds,

402
00:19:12.559 --> 00:19:14.319
<v Speaker 3>or even thousands of dense clumps.

403
00:19:14.400 --> 00:19:16.039
<v Speaker 2>So it's a messy, very messy.

404
00:19:16.319 --> 00:19:19.440
<v Speaker 3>This fragmentation is why stars naturally form in clusters. And

405
00:19:19.440 --> 00:19:22.240
<v Speaker 3>this perfectly explains the forty one percent pairing rate of

406
00:19:22.279 --> 00:19:23.440
<v Speaker 3>the heavyweights, because.

407
00:19:23.240 --> 00:19:26.039
<v Speaker 2>They form together out of the same dense, chaotic clump of.

408
00:19:26.079 --> 00:19:30.319
<v Speaker 3>Material exactly, and they simply never left each other's gravitational grip.

409
00:19:30.440 --> 00:19:32.000
<v Speaker 3>They were born as a bound pack.

410
00:19:32.400 --> 00:19:35.720
<v Speaker 2>So where do the lightweights, the brown dwarfs, fit into

411
00:19:35.759 --> 00:19:36.720
<v Speaker 2>that chaotic cloud.

412
00:19:37.559 --> 00:19:39.880
<v Speaker 3>Well, the first theory is the ejection.

413
00:19:39.599 --> 00:19:42.599
<v Speaker 2>Hypothesis, ejection getting kicked out right.

414
00:19:42.759 --> 00:19:46.680
<v Speaker 3>It proposes that brown dwarfs start forming just like their

415
00:19:46.720 --> 00:19:50.559
<v Speaker 3>massive siblings within these dense, crowded fragments of the molecular cloud.

416
00:19:50.680 --> 00:19:51.920
<v Speaker 2>Okay, but because they.

417
00:19:51.880 --> 00:19:55.599
<v Speaker 3>Are forming in an environment alongside much heavier, much faster

418
00:19:55.720 --> 00:20:00.119
<v Speaker 3>growing stars, the gravitational tug of war is incredibly viol.

419
00:20:00.359 --> 00:20:02.759
<v Speaker 2>So there are the runts of the litter getting pushed around.

420
00:20:02.799 --> 00:20:05.759
<v Speaker 3>Basically, before the brown dwarf can gather enough gas to

421
00:20:05.799 --> 00:20:09.599
<v Speaker 3>reach the critical mass for fusion, the heavier stars gravitationally

422
00:20:09.640 --> 00:20:14.079
<v Speaker 3>bully it debiliate through complex orbital interactions, the massive stars

423
00:20:14.119 --> 00:20:17.640
<v Speaker 3>slingshot the tiny brown dwarf, violently ejecting it from the

424
00:20:17.720 --> 00:20:19.200
<v Speaker 3>multi star system entirely.

425
00:20:19.680 --> 00:20:22.119
<v Speaker 2>So they were part of the complex watch gears for

426
00:20:22.279 --> 00:20:24.960
<v Speaker 2>just this brief chaotic moment, but got stripped out and

427
00:20:25.000 --> 00:20:25.519
<v Speaker 2>flung into the.

428
00:20:25.559 --> 00:20:29.079
<v Speaker 3>Void exactly under the ejection hypothesis, their isolation is the

429
00:20:29.119 --> 00:20:30.359
<v Speaker 3>result of a violent eviction.

430
00:20:30.519 --> 00:20:31.759
<v Speaker 2>Brutal What's the other theory?

431
00:20:31.839 --> 00:20:34.920
<v Speaker 3>The competing theory argues for isolated formation, which.

432
00:20:34.720 --> 00:20:36.359
<v Speaker 2>Means they were alone from the start.

433
00:20:36.480 --> 00:20:40.240
<v Speaker 3>Right, this model suggests that the immense molecular cloud also

434
00:20:40.319 --> 00:20:45.000
<v Speaker 3>contains very tiny, isolated, extremely low mass pockets of gas

435
00:20:45.000 --> 00:20:46.160
<v Speaker 3>on the fringes.

436
00:20:46.000 --> 00:20:48.079
<v Speaker 2>So away from the dense chaotic center.

437
00:20:48.359 --> 00:20:52.160
<v Speaker 3>Yes, a brown dwarf forms from one of these tiny

438
00:20:52.160 --> 00:20:55.200
<v Speaker 3>pockets entirely on its own. It was borne alone in

439
00:20:55.240 --> 00:20:59.519
<v Speaker 3>a quiet, isolated environment with barely enough material to scrape.

440
00:20:59.200 --> 00:21:03.200
<v Speaker 2>By scraping together whatever gas it could find. The census

441
00:21:03.279 --> 00:21:06.240
<v Speaker 2>data showing a nine percent pairing rate feels like a

442
00:21:06.279 --> 00:21:07.279
<v Speaker 2>massive clue here.

443
00:21:07.519 --> 00:21:10.480
<v Speaker 3>It strongly limits the theoretical models. I mean, the fact

444
00:21:10.480 --> 00:21:12.960
<v Speaker 3>that ninety one percent of these lightweights are flying solo

445
00:21:13.039 --> 00:21:16.240
<v Speaker 3>in our ten parsec bubble heavily suggests that whatever mechanism

446
00:21:16.319 --> 00:21:19.359
<v Speaker 3>creates them, whether it is violent injection or isolated formation,

447
00:21:19.519 --> 00:21:21.640
<v Speaker 3>is incredibly efficient at leaving them alone.

448
00:21:21.680 --> 00:21:24.759
<v Speaker 2>It's so cool how this works. The local census essentially

449
00:21:24.839 --> 00:21:28.920
<v Speaker 2>acts as a forensic time machine. It allows astrophysicists to

450
00:21:29.000 --> 00:21:32.839
<v Speaker 2>test the mathematical models of star formation from billions of

451
00:21:32.920 --> 00:21:35.680
<v Speaker 2>years ago against the reality of our current neighborhood.

452
00:21:35.759 --> 00:21:38.680
<v Speaker 3>It really grounds the abstract theories and hard data.

453
00:21:38.720 --> 00:21:42.119
<v Speaker 2>And that perfectly transitions into the actual mechanics of how

454
00:21:42.119 --> 00:21:45.759
<v Speaker 2>these surviving relationships operate. Because we know the mass rules,

455
00:21:45.799 --> 00:21:49.160
<v Speaker 2>we know the structures, but the orbital physics within these

456
00:21:49.200 --> 00:21:53.319
<v Speaker 2>systems are pushed to absolute logic, defying extreme.

457
00:21:53.440 --> 00:21:55.400
<v Speaker 3>Oh, the extremes are mind boggling.

458
00:21:55.599 --> 00:21:58.359
<v Speaker 2>Right the time it takes for these stars to complete

459
00:21:58.400 --> 00:22:02.759
<v Speaker 2>one full lap around each other, their orbital period varies

460
00:22:02.799 --> 00:22:06.960
<v Speaker 2>wildly depending in the system, immensely. On one extreme, you

461
00:22:07.039 --> 00:22:10.920
<v Speaker 2>have tightly bound pairs that whip completely around each other

462
00:22:10.960 --> 00:22:13.720
<v Speaker 2>in a matter of days. I mean, imagine a planetary

463
00:22:13.799 --> 00:22:15.160
<v Speaker 2>year lasting seventy two hours.

464
00:22:15.200 --> 00:22:16.599
<v Speaker 3>You'd have a birthday twice a week.

465
00:22:16.759 --> 00:22:19.519
<v Speaker 2>Right. But then on the far opposite extreme, you have

466
00:22:19.599 --> 00:22:23.240
<v Speaker 2>stars so widely separated that a single orbit takes tens

467
00:22:23.279 --> 00:22:24.480
<v Speaker 2>of millions of years.

468
00:22:24.440 --> 00:22:27.680
<v Speaker 3>And dealing with those extremely wide binaries presents one of

469
00:22:27.720 --> 00:22:31.559
<v Speaker 3>the most massive observational challenges in all of astronomy.

470
00:22:31.599 --> 00:22:33.960
<v Speaker 2>I bet, I mean the tight orbits are easy to comprehend.

471
00:22:34.240 --> 00:22:36.359
<v Speaker 2>It is like a couple holding hands twenty four to seven.

472
00:22:36.480 --> 00:22:38.160
<v Speaker 3>You can clearly see they're together.

473
00:22:38.279 --> 00:22:41.880
<v Speaker 2>Exactly, they are inseparable. A single glance tells you they

474
00:22:41.880 --> 00:22:46.000
<v Speaker 2>are bound together. But a wide binary with an orbit

475
00:22:46.119 --> 00:22:50.079
<v Speaker 2>taking twenty million years. That is like a long distance

476
00:22:50.119 --> 00:22:54.720
<v Speaker 2>relationship maintained by a single text message sent once every millennium.

477
00:22:54.759 --> 00:22:57.400
<v Speaker 3>That's hilarious, but scientifically accurate.

478
00:22:57.799 --> 00:23:00.960
<v Speaker 2>If I point a telescope at a wide binary, the

479
00:23:01.000 --> 00:23:05.359
<v Speaker 2>physical distance between them is staggering. They don't look gravitationally bound.

480
00:23:05.400 --> 00:23:08.400
<v Speaker 2>They just look like two passing strangers who happen to

481
00:23:08.440 --> 00:23:12.119
<v Speaker 2>be drifting through the exact same cosmic zip code.

482
00:23:12.160 --> 00:23:14.799
<v Speaker 3>Well, when an orbital period is measured in the tens

483
00:23:14.839 --> 00:23:17.960
<v Speaker 3>of millions of years, the curvature of that orbit is

484
00:23:18.079 --> 00:23:21.759
<v Speaker 3>virtually flat from the perspective of human observation, because.

485
00:23:21.519 --> 00:23:24.279
<v Speaker 2>We're only seeing a tiny slice of time exactly.

486
00:23:24.480 --> 00:23:26.680
<v Speaker 3>You are not watching a circle being drawn. You are

487
00:23:26.720 --> 00:23:27.960
<v Speaker 3>looking at a straight line.

488
00:23:28.039 --> 00:23:30.799
<v Speaker 2>Wait, if the orbit takes tens of millions of years,

489
00:23:31.240 --> 00:23:33.720
<v Speaker 2>human history has been around long enough to watch even

490
00:23:33.759 --> 00:23:36.000
<v Speaker 2>a microscopic fraction of a percent of it happen, not

491
00:23:36.039 --> 00:23:39.880
<v Speaker 2>even close. I mean Galileo first pointed a telescope at

492
00:23:39.880 --> 00:23:43.279
<v Speaker 2>the sky a mere four hundred years ago. If we

493
00:23:43.759 --> 00:23:47.319
<v Speaker 2>cannot wait millions of years to watch the orbit actually curve,

494
00:23:48.079 --> 00:23:51.119
<v Speaker 2>how can we possibly calculate the binding energy.

495
00:23:51.319 --> 00:23:52.400
<v Speaker 3>It's a great question.

496
00:23:52.599 --> 00:23:56.000
<v Speaker 2>How do astronomers definitively prove they are actually tethered together

497
00:23:56.079 --> 00:23:59.400
<v Speaker 2>by gravity and not just two random stars drifting past

498
00:23:59.440 --> 00:24:01.799
<v Speaker 2>each other in the.

499
00:24:00.799 --> 00:24:04.799
<v Speaker 3>The detective work required to prove wide binarias bound relies

500
00:24:04.839 --> 00:24:08.519
<v Speaker 3>on a concept called common proper motion, and that's combined

501
00:24:08.559 --> 00:24:11.000
<v Speaker 3>with highly precise kinetic energy calculation.

502
00:24:11.160 --> 00:24:13.440
<v Speaker 2>Okay, break that down for me, common proper motion.

503
00:24:13.799 --> 00:24:17.480
<v Speaker 3>Since we cannot observe the orbital curve, we measure velocity

504
00:24:17.559 --> 00:24:21.640
<v Speaker 3>and direction. Imagine two airplanes flying across the ocean.

505
00:24:21.720 --> 00:24:22.559
<v Speaker 2>Okay, two planes.

506
00:24:22.839 --> 00:24:25.160
<v Speaker 3>They are separated by miles, but they are flying in

507
00:24:25.200 --> 00:24:29.200
<v Speaker 3>the exact same direction at the exact same speed. Even

508
00:24:29.240 --> 00:24:31.960
<v Speaker 3>if you cannot see a physical tether between them, it

509
00:24:32.039 --> 00:24:36.119
<v Speaker 3>is mathematically highly improbable that two unrelated planes just happen

510
00:24:36.200 --> 00:24:38.680
<v Speaker 3>to perfectly match speed and heading over the middle of

511
00:24:38.720 --> 00:24:39.279
<v Speaker 3>the Atlantic.

512
00:24:39.319 --> 00:24:41.359
<v Speaker 2>They have to be flying in formation exactly.

513
00:24:41.440 --> 00:24:43.960
<v Speaker 3>They're part of the same group. The same principle applies

514
00:24:43.960 --> 00:24:44.839
<v Speaker 3>to stars.

515
00:24:44.839 --> 00:24:46.519
<v Speaker 2>So they're moving together across the sky.

516
00:24:46.720 --> 00:24:50.960
<v Speaker 3>Yes, GAIA measures the proper motion of these stars, which

517
00:24:51.000 --> 00:24:53.839
<v Speaker 3>is how fast and in what direction they are physically

518
00:24:53.880 --> 00:24:55.599
<v Speaker 3>moving across the backdrop of the galaxy.

519
00:24:55.680 --> 00:24:57.200
<v Speaker 2>Oh I see if.

520
00:24:57.079 --> 00:25:01.200
<v Speaker 3>Two widely separated stars share a common proper it is

521
00:25:01.240 --> 00:25:04.079
<v Speaker 3>a massive red flag that they are associated.

522
00:25:03.559 --> 00:25:05.519
<v Speaker 2>A red flag in a good way, right.

523
00:25:05.880 --> 00:25:09.119
<v Speaker 3>But association is not the same as being gravitationally bound.

524
00:25:09.240 --> 00:25:12.799
<v Speaker 3>They could still be slowly drifting apart. To prove the

525
00:25:12.839 --> 00:25:16.880
<v Speaker 3>tether actually exists, astronomers have to calculate the system's total

526
00:25:17.000 --> 00:25:17.759
<v Speaker 3>energy balance.

527
00:25:17.920 --> 00:25:19.839
<v Speaker 2>Wait, how do you weigh a star you can't touch.

528
00:25:20.240 --> 00:25:22.319
<v Speaker 2>You need to know their mass to know their gravity right.

529
00:25:22.279 --> 00:25:25.559
<v Speaker 3>Now, exactly, and we do that through spectroscopy. By analyzing

530
00:25:25.559 --> 00:25:28.440
<v Speaker 3>the spectrum of light the star emits, we can determine

531
00:25:28.480 --> 00:25:32.119
<v Speaker 3>its temperature, its composition, and ultimately its mass.

532
00:25:32.400 --> 00:25:35.240
<v Speaker 2>Light reveals mass. That's so elegant.

533
00:25:35.400 --> 00:25:38.279
<v Speaker 3>It is so. Once we know the mass of both stars,

534
00:25:38.400 --> 00:25:41.319
<v Speaker 3>we know exactly how much gravitational pull they exert on

535
00:25:41.359 --> 00:25:44.839
<v Speaker 3>each other. Then we look at the historical radial velocity

536
00:25:44.880 --> 00:25:46.839
<v Speaker 3>measurements from the Washington Double.

537
00:25:46.559 --> 00:25:48.680
<v Speaker 2>Star Catalog to see the push and pull.

538
00:25:48.640 --> 00:25:52.400
<v Speaker 3>To determine their exact three dimensional velocity relative to each other.

539
00:25:52.759 --> 00:25:55.359
<v Speaker 2>So we figure out exactly how heavy they are and

540
00:25:55.440 --> 00:25:57.960
<v Speaker 2>exactly how fast they are moving apart from one another.

541
00:25:58.160 --> 00:26:02.359
<v Speaker 3>Yes, because every mass generates an escape velocity.

542
00:26:02.480 --> 00:26:06.160
<v Speaker 2>Escape velocity like a rocket trying to leave Earth the

543
00:26:06.240 --> 00:26:08.480
<v Speaker 2>speed required for an object to break free of its

544
00:26:08.480 --> 00:26:09.920
<v Speaker 2>gravitational pull forever.

545
00:26:10.160 --> 00:26:14.880
<v Speaker 3>Precisely, the researchers painstakingly calculate the kinetic energy of their

546
00:26:14.920 --> 00:26:19.000
<v Speaker 3>relative motion against the potential energy of their combined gravity.

547
00:26:18.720 --> 00:26:20.240
<v Speaker 2>So speed versus gravity.

548
00:26:20.400 --> 00:26:23.960
<v Speaker 3>Exactly if their relative speed is even a fraction lower

549
00:26:24.000 --> 00:26:27.240
<v Speaker 3>than the escape velocity at that specific distance, the math

550
00:26:27.359 --> 00:26:29.559
<v Speaker 3>is unequivocal. They cannot escape.

551
00:26:29.720 --> 00:26:30.240
<v Speaker 2>Wow.

552
00:26:30.319 --> 00:26:32.680
<v Speaker 3>Even if it takes ten million years for the gravitational

553
00:26:32.720 --> 00:26:35.480
<v Speaker 3>tether to haul them back around, they are prominently bound.

554
00:26:35.920 --> 00:26:39.079
<v Speaker 3>The math proves a physical reality that time itself moves

555
00:26:39.119 --> 00:26:40.599
<v Speaker 3>too slowly for us to witness.

556
00:26:40.920 --> 00:26:44.440
<v Speaker 2>I love that. I absolutely love how the math reveals

557
00:26:44.480 --> 00:26:47.279
<v Speaker 2>the invisible mechanics of the universe. It's almost poetic.

558
00:26:47.359 --> 00:26:49.359
<v Speaker 3>It's what makes astrophysics so rewarding.

559
00:26:49.559 --> 00:26:53.599
<v Speaker 2>But as incredibly fascinating as a million year orbit or

560
00:26:53.640 --> 00:26:58.039
<v Speaker 2>a quintuple star system is. These stellar companions are not

561
00:26:58.279 --> 00:27:01.720
<v Speaker 2>universally celebrated by all this ronomers are They Oh definitely not.

562
00:27:01.839 --> 00:27:04.680
<v Speaker 2>In fact, if you talk to a planetary scientist, companion

563
00:27:04.720 --> 00:27:08.319
<v Speaker 2>stars are often described as a massive, absolute.

564
00:27:07.880 --> 00:27:09.880
<v Speaker 3>Nuisance, a total headache right.

565
00:27:10.240 --> 00:27:11.839
<v Speaker 2>When we are trying to do one of the most

566
00:27:11.839 --> 00:27:16.640
<v Speaker 2>important things in modern science hunt for habitable exoplanets, these

567
00:27:16.799 --> 00:27:19.279
<v Speaker 2>multistar systems become an observational nightmare.

568
00:27:19.400 --> 00:27:22.480
<v Speaker 3>A hitting companion star is literally the last thing you

569
00:27:22.519 --> 00:27:24.920
<v Speaker 3>want to uncover in a target system when you are

570
00:27:24.920 --> 00:27:26.279
<v Speaker 3>searching for a second Earth.

571
00:27:26.640 --> 00:27:29.880
<v Speaker 2>Why is that? I mean, the sheer physics of multiple

572
00:27:29.920 --> 00:27:33.799
<v Speaker 2>massive bodies interacting does it just completely ruin the delicate

573
00:27:33.880 --> 00:27:35.640
<v Speaker 2>data required for exoplanet detection.

574
00:27:35.799 --> 00:27:38.319
<v Speaker 3>It completely ruins it. To understand why the data is

575
00:27:38.359 --> 00:27:41.200
<v Speaker 3>so fragile, we have to look at the primary methods

576
00:27:41.279 --> 00:27:42.559
<v Speaker 3>used to find exoplanets.

577
00:27:42.720 --> 00:27:45.160
<v Speaker 2>Okay, because we aren't just looking through a telescope and

578
00:27:45.200 --> 00:27:45.880
<v Speaker 2>seeing a planet.

579
00:27:46.000 --> 00:27:48.759
<v Speaker 3>No, planets do not generate their own visible light. They

580
00:27:48.799 --> 00:27:52.079
<v Speaker 3>only reflect the light of their host star. And next

581
00:27:52.119 --> 00:27:54.640
<v Speaker 3>to the blind and glare of a star, a rocky

582
00:27:54.680 --> 00:27:57.640
<v Speaker 3>planet like Earth is virtually invisible.

583
00:27:57.240 --> 00:27:59.000
<v Speaker 2>The firefly and the floodlight again.

584
00:27:58.920 --> 00:28:02.160
<v Speaker 3>Exactly, so, instead of looking for the planet itself, we

585
00:28:02.200 --> 00:28:05.720
<v Speaker 3>look for the gravitational influence the planet exerts on its.

586
00:28:05.640 --> 00:28:08.799
<v Speaker 2>Host star, looking for the footprint instead of the person.

587
00:28:09.039 --> 00:28:11.519
<v Speaker 3>Right, and the most established method for doing this is

588
00:28:11.599 --> 00:28:12.480
<v Speaker 3>radial velocity.

589
00:28:12.960 --> 00:28:16.000
<v Speaker 2>We touched on radio velocity with the catalog data. It

590
00:28:16.079 --> 00:28:18.680
<v Speaker 2>measures the star moving toward or away from us.

591
00:28:18.960 --> 00:28:25.599
<v Speaker 3>When applied to planet hunting, radial velocity requires staggering almost incomprehensible.

592
00:28:24.759 --> 00:28:26.880
<v Speaker 2>Precision because the planet is so small.

593
00:28:27.000 --> 00:28:30.960
<v Speaker 3>Yes, here is the physical mechanism. Gravity is a two

594
00:28:30.960 --> 00:28:34.480
<v Speaker 3>way street. When a planet orbits a star, it doesn't

595
00:28:34.519 --> 00:28:37.880
<v Speaker 3>just circle a stationary object pinned to the fabric of space.

596
00:28:38.480 --> 00:28:41.559
<v Speaker 3>The planet has mass, so it's gravity tugs back on the.

597
00:28:41.519 --> 00:28:43.119
<v Speaker 2>Star, so the star is moving too.

598
00:28:43.359 --> 00:28:46.440
<v Speaker 3>Yes, both the star and the planet orbit that shared

599
00:28:46.519 --> 00:28:49.480
<v Speaker 3>center of mass, the Berry center, But because the star

600
00:28:49.559 --> 00:28:52.400
<v Speaker 3>is exponentially heavier than the planet, the Bury center is

601
00:28:52.480 --> 00:28:54.559
<v Speaker 3>usually located deep inside the star itself.

602
00:28:54.640 --> 00:28:57.200
<v Speaker 2>It's like a seesaw where a massive adult is sitting

603
00:28:57.279 --> 00:28:59.559
<v Speaker 2>right next to the fulcrum and a toddler is all

604
00:28:59.599 --> 00:29:00.720
<v Speaker 2>the way out on the other end.

605
00:29:00.759 --> 00:29:01.880
<v Speaker 3>That's a perfect visual.

606
00:29:02.160 --> 00:29:05.279
<v Speaker 2>The adult barely moves, but they do shift just a

607
00:29:05.359 --> 00:29:06.960
<v Speaker 2>little bit to balance it out.

608
00:29:06.920 --> 00:29:10.920
<v Speaker 3>Exactly, so the star doesn't trace a wide orbital circle.

609
00:29:11.079 --> 00:29:14.440
<v Speaker 3>It just wobbles back and forth around that internal Berry center.

610
00:29:15.160 --> 00:29:15.960
<v Speaker 2>It wobbles.

611
00:29:16.039 --> 00:29:18.640
<v Speaker 3>As the star wobbles toward Earth, the light waves it

612
00:29:18.680 --> 00:29:22.799
<v Speaker 3>emits gets slightly compressed, shifting toward the blue end of.

613
00:29:22.720 --> 00:29:24.799
<v Speaker 2>The spectrum blue shift yes.

614
00:29:25.079 --> 00:29:28.200
<v Speaker 3>And as it wobbles away, the light waves stretch out,

615
00:29:28.480 --> 00:29:29.960
<v Speaker 3>shifting toward the red end.

616
00:29:30.079 --> 00:29:33.240
<v Speaker 2>Red shift like a police siren changing pitch as it

617
00:29:33.319 --> 00:29:34.039
<v Speaker 2>drives past you.

618
00:29:34.279 --> 00:29:37.119
<v Speaker 3>The exact same principle, but with light instead of sound.

619
00:29:37.519 --> 00:29:41.119
<v Speaker 3>Astronomers measure these microscopic color shifts to prove an unseen

620
00:29:41.160 --> 00:29:42.440
<v Speaker 3>planet is pulling.

621
00:29:42.119 --> 00:29:44.720
<v Speaker 2>On the star. The scale of this measurement is what

622
00:29:44.880 --> 00:29:47.799
<v Speaker 2>just completely blows my mind. I mean, looking for a massive,

623
00:29:48.079 --> 00:29:51.200
<v Speaker 2>Jupiter sized planet is one thing. That's a big toddler.

624
00:29:50.839 --> 00:29:52.680
<v Speaker 3>On the seaside, right, it creates a big wobble.

625
00:29:52.799 --> 00:29:56.440
<v Speaker 2>But looking for a small, rocky, potentially habitable Earth like

626
00:29:56.519 --> 00:30:00.640
<v Speaker 2>planet using radial velocity, that's like try to listen to

627
00:30:00.680 --> 00:30:02.559
<v Speaker 2>a mouse's heartbeat through a stethoscope.

628
00:30:02.680 --> 00:30:03.920
<v Speaker 3>It's incredibly faint.

629
00:30:04.119 --> 00:30:07.599
<v Speaker 2>The signal is so delicate. A planet the mass of

630
00:30:07.680 --> 00:30:11.720
<v Speaker 2>Earth barely moves our Sun at all. It induces a

631
00:30:11.759 --> 00:30:14.400
<v Speaker 2>wabble of maybe nine centimeters per.

632
00:30:14.279 --> 00:30:16.440
<v Speaker 3>Second, which is what the speed of a slow crawl.

633
00:30:16.519 --> 00:30:19.440
<v Speaker 2>Yeah, a slow crawl. Trying to measure a star moving

634
00:30:19.480 --> 00:30:22.079
<v Speaker 2>at nine centimeters per second from thirty light years away

635
00:30:22.119 --> 00:30:24.279
<v Speaker 2>is an absolute triumph of human engineering.

636
00:30:24.400 --> 00:30:25.759
<v Speaker 3>It's a miracle. We can do it at.

637
00:30:25.680 --> 00:30:28.880
<v Speaker 2>All, but if that star has a companion star. A

638
00:30:28.920 --> 00:30:31.400
<v Speaker 2>companion star is like someone standing right next to you

639
00:30:31.440 --> 00:30:33.759
<v Speaker 2>while you have that stethoscope pressed to the mouse and

640
00:30:33.799 --> 00:30:36.079
<v Speaker 2>they just start blasting a heavy metal concert out of

641
00:30:36.079 --> 00:30:36.960
<v Speaker 2>a stadium speaker.

642
00:30:37.279 --> 00:30:40.799
<v Speaker 3>The heavy metal concert completely drowns out the mouse. Every time,

643
00:30:40.960 --> 00:30:44.920
<v Speaker 3>the gravitational tug of war inflicted by an entire other star,

644
00:30:45.440 --> 00:30:49.640
<v Speaker 3>even a small red dwarf, completely warps the radial velocity

645
00:30:49.640 --> 00:30:50.920
<v Speaker 3>readings because.

646
00:30:50.599 --> 00:30:53.119
<v Speaker 2>The star is being yanked around so violently by the

647
00:30:53.160 --> 00:30:57.079
<v Speaker 2>stellar companion that you could never ever detect the gentle

648
00:30:57.200 --> 00:31:00.559
<v Speaker 2>centimeter per second PUG of an Earth sized planet hiding

649
00:31:00.559 --> 00:31:01.359
<v Speaker 2>in the same system.

650
00:31:01.559 --> 00:31:04.759
<v Speaker 3>The data is entirely polluted by gravitational noise.

651
00:31:04.720 --> 00:31:07.000
<v Speaker 2>So radio velocity is completely off the table. For these

652
00:31:07.079 --> 00:31:09.400
<v Speaker 2>multi star systems. We just can't use it.

653
00:31:09.400 --> 00:31:10.400
<v Speaker 3>It's useless there.

654
00:31:10.519 --> 00:31:13.720
<v Speaker 2>But the future of exoplanet hunting is moving beyond just

655
00:31:13.799 --> 00:31:16.680
<v Speaker 2>detecting shadows and wabbles, isn't it? Oh very much so,

656
00:31:16.960 --> 00:31:19.440
<v Speaker 2>we are entering an era where astronomers want to actually

657
00:31:19.480 --> 00:31:24.000
<v Speaker 2>see the planets. The next generation of space observatories is

658
00:31:24.039 --> 00:31:26.200
<v Speaker 2>currently being designed and funded as we speak.

659
00:31:26.319 --> 00:31:27.640
<v Speaker 3>It's a very exciting time.

660
00:31:27.839 --> 00:31:30.799
<v Speaker 2>The heavy hitters coming down the pipeline are NASA's Habitable

661
00:31:30.839 --> 00:31:35.599
<v Speaker 2>World's Observatory known as HWO, and the European Space Agency's

662
00:31:35.880 --> 00:31:39.839
<v Speaker 2>larger Interferometer for exoplanets or life.

663
00:31:40.200 --> 00:31:44.319
<v Speaker 3>These observatories represent the absolute pinnacle of astronomical ambition.

664
00:31:44.599 --> 00:31:48.839
<v Speaker 2>They really do. Their primary mission is monumental. They're specifically

665
00:31:48.839 --> 00:31:52.400
<v Speaker 2>designed to directly image and earth analog, which.

666
00:31:52.240 --> 00:31:55.200
<v Speaker 3>Means they want to physically capture the photons bouncing off

667
00:31:55.240 --> 00:31:57.240
<v Speaker 3>a rocky habitable zone planet.

668
00:31:57.400 --> 00:32:01.319
<v Speaker 2>Direct imaging, no more inferring a planet exists through gravity,

669
00:32:01.359 --> 00:32:05.000
<v Speaker 2>your shadows. Just pointing a massive camera into space, blocking

670
00:32:05.039 --> 00:32:06.920
<v Speaker 2>out the star and taking a picture of a.

671
00:32:06.839 --> 00:32:09.680
<v Speaker 3>Blue dot exactly. And the mechanism they use to block

672
00:32:09.720 --> 00:32:11.559
<v Speaker 3>the star is called a coronagraph.

673
00:32:11.720 --> 00:32:13.759
<v Speaker 2>A coronagraph how does that work?

674
00:32:14.079 --> 00:32:18.279
<v Speaker 3>It is essentially a highly engineered physical mask inside the

675
00:32:18.359 --> 00:32:23.839
<v Speaker 3>telescope that perfectly eclipses the primary stars light. By blocking

676
00:32:23.880 --> 00:32:27.519
<v Speaker 3>the blinding floodlight, it allows the incredibly faint light from

677
00:32:27.599 --> 00:32:29.799
<v Speaker 3>any orbiting planets to become visible.

678
00:32:29.960 --> 00:32:31.759
<v Speaker 2>It's like putting your thumb over the Sun so you

679
00:32:31.799 --> 00:32:33.119
<v Speaker 2>can see a bird flying past.

680
00:32:33.480 --> 00:32:36.880
<v Speaker 3>That's a great everyday example. However, the stakes for this

681
00:32:37.000 --> 00:32:40.640
<v Speaker 3>kind of observation are almost unquantifiable because of the cost.

682
00:32:40.920 --> 00:32:44.519
<v Speaker 3>Telescope time for observatories of this magnitude is one of

683
00:32:44.519 --> 00:32:49.039
<v Speaker 3>the most expensive and fiercely contested resources in human history.

684
00:32:49.400 --> 00:32:53.079
<v Speaker 3>We're talking about billions of dollars of engineering and decades

685
00:32:53.119 --> 00:32:53.640
<v Speaker 3>of planning.

686
00:32:54.000 --> 00:32:56.839
<v Speaker 2>Think about the tax dollars and the sheer human effort

687
00:32:56.920 --> 00:33:00.000
<v Speaker 2>poured into a project like HWO. I mean, as a listener,

688
00:33:00.039 --> 00:33:02.920
<v Speaker 2>your tax dollars are likely helping fund this pursuit right now.

689
00:33:03.279 --> 00:33:06.119
<v Speaker 2>The pressure to point that multi billion dollar lens at

690
00:33:06.160 --> 00:33:07.720
<v Speaker 2>the correct target is immense.

691
00:33:07.960 --> 00:33:10.359
<v Speaker 3>It is because to get a direct image of an

692
00:33:10.400 --> 00:33:13.519
<v Speaker 3>Earth analog, these observatories cannot just snap a quick photo

693
00:33:13.599 --> 00:33:14.279
<v Speaker 3>like a smartphone.

694
00:33:14.359 --> 00:33:15.400
<v Speaker 2>It's not a point and shoot.

695
00:33:15.640 --> 00:33:19.279
<v Speaker 3>No, the target planet is so dim billions of times

696
00:33:19.319 --> 00:33:21.640
<v Speaker 3>dimmer than the star, that the telescope will need to

697
00:33:21.680 --> 00:33:24.960
<v Speaker 3>lock on and stare at a promising candidate system four

698
00:33:25.000 --> 00:33:25.839
<v Speaker 3>weeks at a time.

699
00:33:26.039 --> 00:33:26.440
<v Speaker 2>Weeks.

700
00:33:26.920 --> 00:33:30.640
<v Speaker 3>It takes weeks of constant observation to gather enough individual

701
00:33:30.680 --> 00:33:35.640
<v Speaker 3>photons to slowly build a single workable image of the planet.

702
00:33:35.319 --> 00:33:38.480
<v Speaker 2>Weeks of staring at one single spot in the sky.

703
00:33:39.279 --> 00:33:42.559
<v Speaker 2>So if you dedicate three weeks of multi billion dollar

704
00:33:42.640 --> 00:33:46.880
<v Speaker 2>telescope time to a star system, and you unknowingly target

705
00:33:46.880 --> 00:33:50.279
<v Speaker 2>a star that has a hidden, widely separated companion in

706
00:33:50.319 --> 00:33:51.079
<v Speaker 2>the background, it.

707
00:33:51.079 --> 00:33:53.440
<v Speaker 3>Would be an unmitigated disaster for the observation.

708
00:33:53.519 --> 00:33:54.640
<v Speaker 2>The whole thing is ruined.

709
00:33:54.720 --> 00:33:57.960
<v Speaker 3>Oh absolutely. If there is a hidden companion star sitting

710
00:33:58.000 --> 00:34:00.960
<v Speaker 3>just outside the edge of the coronagraph's mask, the background

711
00:34:01.039 --> 00:34:04.359
<v Speaker 3>light noise the glare from that companion would completely wash

712
00:34:04.400 --> 00:34:06.680
<v Speaker 3>out the delicate, sparse photons arriving from.

713
00:34:06.599 --> 00:34:08.719
<v Speaker 2>The exoplanet just to wash a white noise.

714
00:34:08.880 --> 00:34:11.840
<v Speaker 3>The resulting data would be utterly ruined. The researchers would

715
00:34:11.840 --> 00:34:14.280
<v Speaker 3>have wasted the most valuable scientific time off the planet

716
00:34:14.360 --> 00:34:15.480
<v Speaker 3>staring at light pollution.

717
00:34:15.840 --> 00:34:19.119
<v Speaker 2>Oh man, that hurts to even think about. But this

718
00:34:19.199 --> 00:34:22.360
<v Speaker 2>begs the entire purpose of the Cosmic Sensus into brilliant

719
00:34:22.719 --> 00:34:25.719
<v Speaker 2>sharp focus, doesn't it. It does. This massive effort to

720
00:34:25.719 --> 00:34:27.920
<v Speaker 2>map four hundred and twenty four objects in our ten

721
00:34:28.000 --> 00:34:31.280
<v Speaker 2>Parsik bubble is not just about cataloging stars for the

722
00:34:31.320 --> 00:34:32.280
<v Speaker 2>sake of having a list.

723
00:34:32.360 --> 00:34:33.519
<v Speaker 3>No, it's highly practical.

724
00:34:33.639 --> 00:34:36.880
<v Speaker 2>It is essentially a highly vetted do not call list

725
00:34:37.320 --> 00:34:39.039
<v Speaker 2>for these future mega telescopes.

726
00:34:39.119 --> 00:34:40.480
<v Speaker 3>That's the perfect term for it.

727
00:34:40.480 --> 00:34:43.599
<v Speaker 2>It is a precise target map that tells HWO and

728
00:34:43.800 --> 00:34:46.840
<v Speaker 2>life exactly where it is mathematically safe to look.

729
00:34:46.960 --> 00:34:51.079
<v Speaker 3>It is the ultimate filtering mechanism. By painstakingly identifying the

730
00:34:51.079 --> 00:34:54.000
<v Speaker 3>two hundred and fifteen bound objects and cataloging the ninety

731
00:34:54.000 --> 00:34:58.000
<v Speaker 3>two multiple star systems, the researchers have instantly identified which

732
00:34:58.039 --> 00:35:01.880
<v Speaker 3>stars have a high probability of polluting direct imaging data.

733
00:35:01.519 --> 00:35:04.719
<v Speaker 2>With either light, noise or chaotic gravity exactly.

734
00:35:04.559 --> 00:35:08.039
<v Speaker 3>The telescope operators can confidently cross those systems off the

735
00:35:08.079 --> 00:35:09.159
<v Speaker 3>primary target list.

736
00:35:09.440 --> 00:35:11.679
<v Speaker 2>The paradox of this research is just brilliant to me.

737
00:35:11.840 --> 00:35:14.920
<v Speaker 2>I mean, we spend all this incredible effort combining decades

738
00:35:14.920 --> 00:35:18.559
<v Speaker 2>of the Washington Double Star catalog with the cutting edge

739
00:35:18.599 --> 00:35:23.000
<v Speaker 2>astrometry of Gaya, calculating complex binding energies for a million

740
00:35:23.039 --> 00:35:26.760
<v Speaker 2>year orbits, and mapping four hundred and twenty four objects

741
00:35:26.760 --> 00:35:30.119
<v Speaker 2>down to their precise coordinates, largely so we know exactly

742
00:35:30.119 --> 00:35:31.159
<v Speaker 2>which ones to ignore.

743
00:35:31.280 --> 00:35:33.840
<v Speaker 3>I know it sounds counterintuitive, but in the realm of

744
00:35:33.920 --> 00:35:37.920
<v Speaker 3>high stakes astronomy, eliminating false positives is just as vital

745
00:35:37.960 --> 00:35:39.559
<v Speaker 3>as identifying a prime target.

746
00:35:39.639 --> 00:35:40.920
<v Speaker 2>You have to clear the brush right.

747
00:35:41.320 --> 00:35:43.760
<v Speaker 3>If you are searching for a needle in a massive

748
00:35:43.800 --> 00:35:47.199
<v Speaker 3>cosmic haystack. The most efficient strategy you can employ is

749
00:35:47.239 --> 00:35:50.440
<v Speaker 3>to aggressively and systematically burn away all the hay that

750
00:35:50.480 --> 00:35:53.360
<v Speaker 3>you know definitively does not contain a needle.

751
00:35:53.440 --> 00:35:54.000
<v Speaker 2>Burn the hay.

752
00:35:54.320 --> 00:35:57.119
<v Speaker 3>By clearing the board of these multi star systems, we

753
00:35:57.159 --> 00:36:03.280
<v Speaker 3>can focus all our precious limited observational ress on the quiet, stable, isolated.

754
00:36:02.719 --> 00:36:06.400
<v Speaker 2>Stars, the loaners, the stars drifting through the galaxy, completely.

755
00:36:06.079 --> 00:36:08.360
<v Speaker 3>Unattached stars exactly like our sun.

756
00:36:08.679 --> 00:36:11.000
<v Speaker 2>Let's pull all these threads together to see the complete

757
00:36:11.000 --> 00:36:15.039
<v Speaker 2>picture of our cosmic neighborhood. Because we started by drawing

758
00:36:15.079 --> 00:36:18.760
<v Speaker 2>a mathematical boundary, a perfect thirty two point six light

759
00:36:18.880 --> 00:36:23.119
<v Speaker 2>year sphere around our solar system, just to ensure absolute.

760
00:36:22.599 --> 00:36:26.800
<v Speaker 3>Completeness, and inside that ten parsk neighborhood, we analyzed four

761
00:36:26.880 --> 00:36:27.880
<v Speaker 3>hundred and twenty four.

762
00:36:27.719 --> 00:36:30.960
<v Speaker 2>Objects, and we discovered that our human bias is completely wrong.

763
00:36:31.440 --> 00:36:33.360
<v Speaker 2>Roughly half the neighborhood is actually paired up.

764
00:36:33.400 --> 00:36:34.760
<v Speaker 3>It's a busy street, it is.

765
00:36:35.400 --> 00:36:39.559
<v Speaker 2>We learned that mass dictates relationship status. Right with massive

766
00:36:39.599 --> 00:36:44.280
<v Speaker 2>stars thriving in complex, double, triple and even intricately layered

767
00:36:44.400 --> 00:36:45.920
<v Speaker 2>quintuple systems.

768
00:36:45.519 --> 00:36:47.760
<v Speaker 3>The Swiss watches of the galaxy.

769
00:36:47.400 --> 00:36:51.400
<v Speaker 2>Exactly while the tiny brown dwarfs remain isolated, likely due

770
00:36:51.440 --> 00:36:53.440
<v Speaker 2>to violent injections early in their formation.

771
00:36:53.559 --> 00:36:54.559
<v Speaker 3>The outcasts.

772
00:36:54.840 --> 00:36:58.400
<v Speaker 2>We explored the dizzying extremes of orbital physics, from pairs

773
00:36:58.400 --> 00:37:01.880
<v Speaker 2>whipping around each other in days to wide binaries tethered

774
00:37:01.920 --> 00:37:06.119
<v Speaker 2>together across tens of millions of years by invisible, calculatingly

775
00:37:06.159 --> 00:37:07.880
<v Speaker 2>precise gravitational bond.

776
00:37:07.719 --> 00:37:10.800
<v Speaker 3>And ultimately we uncovered why this definitive map is so

777
00:37:10.880 --> 00:37:11.920
<v Speaker 3>critical right.

778
00:37:12.599 --> 00:37:15.719
<v Speaker 2>It clears the literal and figurative noise. It provides our

779
00:37:15.760 --> 00:37:19.800
<v Speaker 2>next generation telescopes like HWO and Life with a clean,

780
00:37:19.920 --> 00:37:23.199
<v Speaker 2>pristine roadmap to hunt for a second Earth by actively

781
00:37:23.239 --> 00:37:27.039
<v Speaker 2>avoiding the chaotic heavy metal concerts of multiple Star systems.

782
00:37:27.400 --> 00:37:31.079
<v Speaker 3>It is a remarkable achievement that fundamentally changes our perception

783
00:37:31.159 --> 00:37:35.360
<v Speaker 3>of our local environment. It transforms a mysterious chaotic void

784
00:37:35.559 --> 00:37:38.239
<v Speaker 3>into a meticulously mapped, understood terrain.

785
00:37:38.559 --> 00:37:40.599
<v Speaker 2>We now know the layout of the neighborhood we do.

786
00:37:40.800 --> 00:37:43.519
<v Speaker 2>It is the foundation for everything that comes next. And

787
00:37:43.559 --> 00:37:45.480
<v Speaker 2>as we wrap up this exploration, I want to leave

788
00:37:45.519 --> 00:37:47.840
<v Speaker 2>you with a final lingering thought. Tom all over, Okay,

789
00:37:47.920 --> 00:37:50.639
<v Speaker 2>when we look up at our lone, companionless sun, it

790
00:37:50.760 --> 00:37:53.440
<v Speaker 2>is really easy to feel a sense of profound isolation.

791
00:37:54.239 --> 00:37:56.440
<v Speaker 2>We feel like we're just drifting through the dark, empty

792
00:37:56.480 --> 00:38:00.159
<v Speaker 2>space of the Milky Way, entirely by ourselves, disconnected from

793
00:38:00.159 --> 00:38:02.000
<v Speaker 2>the cosmic dance happening all around us.

794
00:38:02.039 --> 00:38:03.039
<v Speaker 3>It can feel very lonely.

795
00:38:03.320 --> 00:38:07.360
<v Speaker 2>But given everything we've just unpacked, given how violently companion

796
00:38:07.440 --> 00:38:10.679
<v Speaker 2>stars warp the gravitational environment, given how they flood a

797
00:38:10.679 --> 00:38:14.320
<v Speaker 2>solar system with blinding light noise, and given how inherently

798
00:38:14.440 --> 00:38:17.599
<v Speaker 2>hostile a multi star system is to the delicate formation

799
00:38:17.719 --> 00:38:21.639
<v Speaker 2>of a planet, think about what that implies for our

800
00:38:21.800 --> 00:38:22.599
<v Speaker 2>very existence.

801
00:38:22.880 --> 00:38:24.159
<v Speaker 3>The silence is the point.

802
00:38:24.360 --> 00:38:29.480
<v Speaker 2>If human ingenuity ever does pinpoint a perfect, tranquil, alternative

803
00:38:29.480 --> 00:38:33.159
<v Speaker 2>Earth nearby, a world where life has had the billions

804
00:38:33.159 --> 00:38:36.119
<v Speaker 2>of years of uninterrupted quiet necessary to evolve, it will

805
00:38:36.119 --> 00:38:38.880
<v Speaker 2>almost certainly be orbiting a star just as lonely as ours.

806
00:38:39.280 --> 00:38:42.159
<v Speaker 3>The visual spectacle of a multi star system with five

807
00:38:42.239 --> 00:38:44.559
<v Speaker 3>suns in the sky might be breathtaking.

808
00:38:44.119 --> 00:38:46.000
<v Speaker 2>From a distance, it'll be stunning that.

809
00:38:45.840 --> 00:38:49.760
<v Speaker 3>That sheer chaos is fundamentally incompatible with the fragile, steady

810
00:38:49.760 --> 00:38:51.480
<v Speaker 3>development of a habitable world.

811
00:38:51.719 --> 00:38:55.320
<v Speaker 2>So perhaps our sun's isolation isn't some tragic cosmic anomaly.

812
00:38:55.360 --> 00:38:58.280
<v Speaker 2>It isn't something to feel lonely or adrift about. Maybe

813
00:38:58.320 --> 00:39:02.159
<v Speaker 2>being a lone star is the precise, absolutely necessary prerequisite

814
00:39:02.159 --> 00:39:02.599
<v Speaker 2>for life.

815
00:39:02.519 --> 00:39:04.000
<v Speaker 3>Our requirement, not a bug.

816
00:39:04.320 --> 00:39:07.119
<v Speaker 2>The quiet solitude of our single sun's sky isn't a

817
00:39:07.119 --> 00:39:10.760
<v Speaker 2>flaw in our solar system's design. It is the exact

818
00:39:10.960 --> 00:39:14.280
<v Speaker 2>tranquil reason we are here, sitting on this porch, able

819
00:39:14.280 --> 00:39:16.159
<v Speaker 2>to look up at the sky and wonder about the

820
00:39:16.239 --> 00:39:17.280
<v Speaker 2>universe in the first place.
