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.

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<v Speaker 2>The night sky.

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<v Speaker 3>So I want you to just imagine for a second,

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<v Speaker 3>stepping outside on a really crisp, clear.

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<v Speaker 2>Night mm hm, the kind of where the stars just

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<v Speaker 2>kind of.

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<v Speaker 3>Pop exactly, and you look up and you find the

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<v Speaker 3>constellation Orion.

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<v Speaker 2>Right, highly recognizable.

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<v Speaker 3>Yeah, and you look at Orion's right shoulder, that glowing

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<v Speaker 3>kind of reddish orange dot, beetle goose, beetlejuice. Right. Humanity

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<v Speaker 3>has been staring at the specific star for millennia, But

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<v Speaker 3>it turns out it's been keeping this absolutely massive secret,

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<v Speaker 3>a really massive one.

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<v Speaker 2>Yeah.

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<v Speaker 3>I mean, think about it this way. If you took

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<v Speaker 3>our sun, the blindingly bright center of our entire solar system,

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<v Speaker 3>and you just dropped it right next to Beetlejuice, our

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<v Speaker 3>Sun would be completely invisible.

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<v Speaker 2>Entirely erased by the glare, right.

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<v Speaker 3>You wouldn't be able to see it with the naked eye,

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<v Speaker 3>and honestly, you would struggle to see it with our

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<v Speaker 3>most advanced telescopes, which kind of explains this really uncomfortable

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<v Speaker 3>reality in modern astronomy.

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<v Speaker 2>It's very humbling, honestly, totally.

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<v Speaker 3>For the last hundred years, a massive star up to

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<v Speaker 3>three times the size of our Sun has just been

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<v Speaker 3>hiding in plain sight right there, orbiting Orion's shoulder, and.

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<v Speaker 2>We didn't definitively find it until right now.

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<v Speaker 3>It's wild. So today we're unpacking the stunning conclusion to

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<v Speaker 3>this century long astronomical quest. We are breaking down the

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<v Speaker 3>definitive discovery of batel gouse b, the hidden companion star, Yeah,

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<v Speaker 3>the hidden companion. We're going to track the historical suspicions,

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<v Speaker 3>like why we even thought there was a hidden star

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<v Speaker 3>in the first place.

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<v Speaker 2>Right, because the clues were always there exactly.

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<v Speaker 3>I will analyze the mechanics of that crazy false alarm

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<v Speaker 3>from a few years ago.

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<v Speaker 2>Oh, the great dimming when everyone thought it was going to.

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<v Speaker 3>Explode, Yes, when everyone was panicking about a supernova. And

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<v Speaker 3>then we're going deep into the specific optical physics and

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<v Speaker 3>the planet hunting technology that finally allowed astronomers in the

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<v Speaker 3>Atacoma Desert to capture a direct image of this thing.

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<v Speaker 2>Because the implications here they go far beyond just solving

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<v Speaker 2>an old mystery. Oh, for sure, finding a companion star

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<v Speaker 2>of this magnitude hiding in the glare of a highly

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<v Speaker 2>evolved supergen in it introduces a whole new set of

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<v Speaker 2>incredibly high stakes physics. The eventual death of Beetlegoose, which

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<v Speaker 2>we know is coming, is going to be fundamentally altered

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<v Speaker 2>by the presence of this neighbor.

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<v Speaker 3>So to understand why finding beetlejuice Bee is such a

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<v Speaker 3>massive paradigm shift, we really have to establish the baseline

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<v Speaker 3>of Beatleges itself.

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<v Speaker 2>Yeah, we have to talk about the scale.

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<v Speaker 3>The scale is just it's hard to wrap your head around.

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<v Speaker 3>The reason astronomers have spent nearly a century frustrat by

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<v Speaker 3>the star comes down to sheer physical dominance. It's a

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<v Speaker 3>red supergin, right. If you dropped Batylviews into the center

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<v Speaker 3>of our Solar system, its surface would extend out past

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<v Speaker 3>the orbit of Jupiter.

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<v Speaker 2>Just swallows everything.

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<v Speaker 3>Yeah, Mercury, Venus, Earth, Mars, the asteroid belt all completely

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<v Speaker 3>gone inside the star, and that.

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<v Speaker 2>Scale dictates everything about how we observe it. We are

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<v Speaker 2>dealing with a bloated, highly evolved star that's in the

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<v Speaker 2>final stages of its life cycle.

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<v Speaker 3>Right, it's running out of gas exactly.

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<v Speaker 2>And because it's so massive and relatively close to us,

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<v Speaker 2>I mean roughly six hundred and fifty light years away,

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<v Speaker 2>it is one of the brightest objects in our.

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<v Speaker 3>Sky, with that really unmistakable reddish orange color.

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<v Speaker 2>Right. But the defining characteristic of Beetlejuice, the quirk that

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<v Speaker 2>caught the attention of everyone from ancient aboriginal astronomers to

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<v Speaker 2>like Sir John Herschel in the eighteen thirties, is its variability.

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<v Speaker 3>It doesn't just sit there.

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<v Speaker 2>No, It's brightness is not constant.

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<v Speaker 3>It dims and brightens. And the crucial detail here, the

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<v Speaker 3>thing that really kicked off this whole century long hunt,

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<v Speaker 3>is that it doesn't just flicker randomly. There's a rhythm

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<v Speaker 3>to it.

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<v Speaker 2>Yeah. In atrophysics, when you plot a star's light curve,

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<v Speaker 2>you know the graph of its brightness over time, and

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<v Speaker 2>you see a repeating, predictable variation, it's a massive red flag.

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<v Speaker 3>It signals a mechanical cycle exactly.

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<v Speaker 2>The star of that magnitude doesn't just change its luminous

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<v Speaker 2>output on a strict schedule without a physical driver.

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<v Speaker 3>Think of it like this. Say you look out your

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<v Speaker 3>window right, and the street light at the end of

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<v Speaker 3>your block.

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<v Speaker 2>Is flickering completely randomly.

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<v Speaker 3>Yeah, if it's random, you just assume the internal mechanism

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<v Speaker 3>is breaking down. It's a dying bulb. But if you

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<v Speaker 3>sit there with a stockwatch and you time it, and

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<v Speaker 3>you realize that street light is dimming on a precise,

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<v Speaker 3>predictable schedule, like say, every four hundred days, like clockwork,

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<v Speaker 3>you stop blaming the bolt.

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<v Speaker 2>Right. You assume someone is messing.

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<v Speaker 3>With the power exactly. You assume a neighbor is routinely

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<v Speaker 3>tapping the power line. And for roughly a century, astronomers

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<v Speaker 3>looking at the periodicity of Biddle Juice's brightness suspected a

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<v Speaker 3>stellar neighbor was tapping the line.

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<v Speaker 2>Right. The hypothesis was that as a smaller companion star

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<v Speaker 2>orbited the supergent, its gravity would tug on the larger star.

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<v Speaker 3>Or maybe it was periodically passing through the outer layers

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<v Speaker 3>of the supergen's extended atmosphere.

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<v Speaker 2>Yeah, exactly, creating those rhythmic dips in the light. We

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<v Speaker 2>receive on Earth.

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<v Speaker 3>But the frustration here, like the maddening part for astronomers,

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<v Speaker 3>is the gap between mathematical suspicion and visual confirmation.

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<v Speaker 2>Oh it's the worst.

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<v Speaker 3>You can have the light curves, you can track the

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<v Speaker 3>scheduled flicker, but no matter how much you upgrade your lenses,

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<v Speaker 3>the culprit remains completely invisible because.

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<v Speaker 2>Of the sheer luminosity of beetlejuice. I mean, the supurgeon

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<v Speaker 2>is pumping out something like one hundred thousand times more

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<v Speaker 2>photons than our sun. That's it's blinding. Yeah, that contrast

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<v Speaker 2>ratio is the primary enemy of observational astronomy. When you're

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<v Speaker 2>trying to image a faint object next to an incredibly

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<v Speaker 2>bright one, the photons from the bright object literally spill

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<v Speaker 2>over the pixels on your detector.

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<v Speaker 3>It just washes out the faint signal entirely completely.

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<v Speaker 2>So the companion was basically trapped in the mathematical realm.

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<v Speaker 2>We could see the gravitational footprints it was leaving on beetlejuice,

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<v Speaker 2>but we couldn't actually see the star making them.

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<v Speaker 3>Okay, let's actually get into the mechanics of those footprints,

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<v Speaker 3>because before they get to the direct image. They knew

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<v Speaker 3>something was there through something called radial velocity. So how

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<v Speaker 3>exactly does a hidden star leave a measurable footprint in

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<v Speaker 3>the light of the main star.

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<v Speaker 2>It really all comes down to the Doppler effect, but

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<v Speaker 2>applied to starlight.

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<v Speaker 3>Okay, like a police siren changing pitch when it drives

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<v Speaker 3>past you.

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<v Speaker 2>Precisely. So, when two stars orbit each other, they don't

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<v Speaker 2>actually just have one sitting still while the other goes

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<v Speaker 2>around it. They orbit their common center of mass, which

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<v Speaker 2>we call the Berry center. Right now, even though battle

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<v Speaker 2>Juice is immensely massive, the companion still exerts a gravitational

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<v Speaker 2>pull on it, and this causes Bettle Juwe to wobble

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<v Speaker 2>slightly as it moves through space.

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<v Speaker 3>So they're both doing this kind of slightly off center

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<v Speaker 3>waltz together exactly, Yeah.

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<v Speaker 2>And we can measure that wobble using spectroscopy. We take

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<v Speaker 2>the light from Batel Duice and we spread it out

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<v Speaker 2>into a spectrum like.

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<v Speaker 3>A rainbow, like shining it through a prism.

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<v Speaker 2>Right and in that spectrum there are dark lines absorption

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<v Speaker 2>lines that are created by specific elements in the star's

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<v Speaker 2>atmosphere absorbing specific wavelengths of light, like a barcode perfect analogy. Yeah,

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<v Speaker 2>a barcode as bettle juice wobbles toward Earth, those barcode

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<v Speaker 2>lines shift slightly toward the blue end of the spectrum

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<v Speaker 2>because the light waves are getting.

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<v Speaker 3>Compressed, and then as it wobbles away from us.

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<v Speaker 2>The lines shift toward the red end because the waves

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<v Speaker 2>are getting stretched out.

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<v Speaker 3>So by meticulously tracking how those dark barcode lines slide

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<v Speaker 3>back and forth over decades of observation, astronomers could calculate

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<v Speaker 3>the exact gravitational pull required to cause that specific wobble exactly.

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<v Speaker 2>They basically mapped the invisible orbit, could determined the orbital period,

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<v Speaker 2>the eccentricity of the orbit, and theoretically, the mass of

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<v Speaker 2>the hidden companion that had to be causing the wobble.

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<v Speaker 3>Okay, but wait, I'm going to push back on this

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<v Speaker 3>right here. Sure you just said they use this radial

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<v Speaker 3>velocity data to calculate the mass of the companion, and

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<v Speaker 3>based on that math, for years, the astronomical community predicted

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<v Speaker 3>the companion would be roughly one solar mass, so about

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<v Speaker 3>the size of our Sun. Right, but the brand new

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<v Speaker 3>discovery that we're talking about today confirmed the star is

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<v Speaker 3>actually two to three times that.

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<v Speaker 2>Mass, yeah, much bigger.

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<v Speaker 3>So how can the spectroscopic math be so perfectly accurate

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<v Speaker 3>about the orbit and the location but miss the actual

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<v Speaker 3>mass of the object by a factor of three?

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<v Speaker 2>Ah. That points to one of the most notorious ambiguities

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<v Speaker 2>in all of astrophysics. It's called the inclination angle, or

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<v Speaker 2>often the sign do degeneracy.

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<v Speaker 3>Okay, break that down for us. Why does the angle

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<v Speaker 3>matter so much?

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<v Speaker 2>Well, radio velocity only measures movement along our specific line

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<v Speaker 2>of sight, so directly toward us or directly away from us, right,

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<v Speaker 2>It tells us absolutely nothing about the star's movement up, down, left, right,

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<v Speaker 2>across the sky.

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<v Speaker 3>Okay, So imagine you're looking at a Merry Go Round.

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<v Speaker 2>Yes, perfect, If you're.

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<v Speaker 3>Looking at it perfectly edge on, you can clearly see

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<v Speaker 3>the horses moving directly toward you and directly away from

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<v Speaker 3>you exactly.

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<v Speaker 2>That is a ninety degree inclination. You're getting the full

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<v Speaker 2>velocity measurement.

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<v Speaker 3>But if I'm hovering in a helicopter looking at that

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<v Speaker 3>same Merry Go Round from directly above, so a zero

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<v Speaker 3>degree inclination, the horses are just moving in a circle

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<v Speaker 3>across my field of view.

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<v Speaker 2>They are never moving towards you or away from you right,

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<v Speaker 2>and therefore your radio velocity measurement would be zero, even

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<v Speaker 2>though the Merry Go Round is spinning rapidly.

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<v Speaker 3>Oh wow.

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<v Speaker 2>Yeah, So when we look at a binary star system

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<v Speaker 2>out in deep space, we almost never know the exact

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<v Speaker 2>tilt of the orbit relative to Earth. The spectroscopic wobble

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<v Speaker 2>only gives us the minimum possible mass of the companion.

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<v Speaker 3>Because if the orbit is tilted relative to our line

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<v Speaker 3>of sight, the true mass has to be higher to

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<v Speaker 3>produce the wobble we're measuring.

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<v Speaker 2>Ailed it. The astronomers who predicted a one solar mass

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<v Speaker 2>companion assumed a fairly edge on orbit. But because Beetlejew's

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<v Speaker 2>b turned out to be nearly three solar masses, we

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<v Speaker 2>now know the orbit must be significantly tilted.

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<v Speaker 3>So the math wasn't wrong. It was just incomplete due

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<v Speaker 3>to our fixed vantage point in.

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<v Speaker 2>The cosmo exactly we're stuck here on Earth.

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<v Speaker 3>It's fascinating how a physical limitation of our perspective entirely

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<v Speaker 3>masked the true nature of the star for one hundred years.

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<v Speaker 3>It really is, and it's wild because just as researchers

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<v Speaker 3>were aggressively dialing in on these orbital predictions, Beetle Jews

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<v Speaker 3>decided to throw this massive curveball that derailed the hunt

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<v Speaker 3>and triggered a global panic. Oh yes, we have to

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<v Speaker 3>talk about the great dimming.

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<v Speaker 2>This is such a critical chapter in the story because

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<v Speaker 2>it highlights just how volatile red supergins are and it

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<v Speaker 2>perfectly sets the stage for the specific team that ultimately

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<v Speaker 2>found the companion.

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<v Speaker 3>Right, So, a few years ago Beetle Jews underwent this

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<v Speaker 3>completely unprecedented drop in luminosity.

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<v Speaker 2>Is visible to the naked eye. Anyone could go outside

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<v Speaker 2>and see it.

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<v Speaker 3>The star lost a massive fraction of its brightness in

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<v Speaker 3>a matter of weeks, and I remember the absolute frenzy

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<v Speaker 3>in the astronomical community.

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<v Speaker 2>Oh, Twitter was going crazy.

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<v Speaker 3>Because Beetlejewice is a known ticking time bomb. It has

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<v Speaker 3>exhausted the hydrogen fuel in its core, it's burning heavier elements,

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<v Speaker 3>and it is on a one way trip to a

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<v Speaker 3>core collapse supernova.

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<v Speaker 2>Right, And when a star with that specific doomed profile

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<v Speaker 2>suddenly drops in brightness, the immediate assumption is that the

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<v Speaker 2>engine is.

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<v Speaker 3>Failing, core is destabilizing.

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<v Speaker 2>Exactly, the explosion is imminent.

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<v Speaker 3>So the scientific tension centered on whether we were witnessing

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<v Speaker 3>an intrinsic change or an extrinsic change.

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<v Speaker 2>Right, Yes, an intrinsic change would mean the internal thermodynamics

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<v Speaker 2>of the star were actually failing, like perhaps the outward

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<v Speaker 2>radiation pressure that holds the star against its own gravity

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<v Speaker 2>had suddenly dropped.

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<v Speaker 3>Which is the precursor to collapse exactly.

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<v Speaker 2>But an extrinsic change would mean the star's internal engine

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<v Speaker 2>was totally fine, but something physical moved between the star

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<v Speaker 2>and our telescopes, basically blocking the photons.

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<v Speaker 3>So to solve this, French researcher Miguel Montage and his

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<v Speaker 3>team secured observation time on the very large telescope the VLT,

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<v Speaker 3>down in Chile, and they didn't just measure the light.

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<v Speaker 3>They actually managed to resolve the surface of Beetlejuice to

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<v Speaker 3>see what was happening.

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<v Speaker 2>Which is incredible. Resolving the surface of any star other

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<v Speaker 2>than our own sun is an extreme technical achievement.

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<v Speaker 3>Because they're usually just points of light.

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<v Speaker 2>Right, Yes, even the biggest telescopes usually you see a dot.

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<v Speaker 2>But because Beetle Juice is so physically massive and relatively close,

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<v Speaker 2>the VLT could capture its actual disc Wow, and what

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<v Speaker 2>Montage's team discovered debunked the supernova panic completely. The dimming

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<v Speaker 2>was not an internal collapse, it was a massive, localized

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<v Speaker 2>extrinsic block.

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<v Speaker 3>They found out the star had essentially burped out a

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<v Speaker 3>massive cloud of gas.

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<v Speaker 2>Yeah, a huge burp. We need to look at the

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<v Speaker 2>flow dynamics of a red supergent to understand how violent

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<v Speaker 2>that burp actually was.

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<v Speaker 3>Okay, set the scene.

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<v Speaker 2>So, Unlike our Sun, which has millions of relatively small

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<v Speaker 2>convection cells boiling on its surface kind of like a

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<v Speaker 2>pot of boiling water, a bloated supergent, like beetlejuice, has

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<v Speaker 2>convection cells that are just staggeringly huge. A single one

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<v Speaker 2>can cover a huge fraction of the star's entire surface.

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<v Speaker 2>We are talking about bubbles of boiling plasma the size

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<v Speaker 2>of our inner solar systm.

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<v Speaker 3>Wait, really just one bubble, Just.

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<v Speaker 2>One bubble rising from the interior, releasing heat and sinking

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<v Speaker 2>back down.

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<v Speaker 3>Okay, So one of these colossal convection cells breaches the

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<v Speaker 3>surface and violently ejects a massive plume of stellar material

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<v Speaker 3>deep into space.

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00:13:38.080 --> 00:13:41.000
<v Speaker 2>Yes, a massive bubble of hot gas is blown off

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<v Speaker 2>the star, and as this plume travels rapidly away from

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<v Speaker 2>the intense heat the photosphere, the thermodynamics drop sharply. It

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<v Speaker 2>cools down. It cools down very fast. And when stellar gas,

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<v Speaker 2>which contains elements like silicon, oxygen, and carbon, cools past

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<v Speaker 2>a specific temperature threshold, it undergoes a phase change. The

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<v Speaker 2>gas condenses into solid particulates.

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00:14:00.200 --> 00:14:02.799
<v Speaker 3>So it quite literally turns into rock and soot in

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<v Speaker 3>the vacuum of space.

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00:14:04.159 --> 00:14:08.000
<v Speaker 2>Exactly, it forms silicon dust. Yeah, and this immense cloud

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<v Speaker 2>of newly formed dust happened to condense directly in our

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<v Speaker 2>line of sight, physically eclipsing the southern hemisphere of the star.

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<v Speaker 3>Unbelievable.

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00:14:17.240 --> 00:14:20.399
<v Speaker 2>It absorbed the visible light from Beetle jews and re

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00:14:20.480 --> 00:14:24.159
<v Speaker 2>emitted it in the infrared, which caused the dramatic dimming

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00:14:24.240 --> 00:14:24.960
<v Speaker 2>we saw on Earth.

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00:14:25.080 --> 00:14:26.799
<v Speaker 3>It basically created its own eclipse.

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00:14:26.879 --> 00:14:31.759
<v Speaker 2>Yeah, no, supernova, just localized atmospheric chaos, resulting in a

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00:14:31.799 --> 00:14:32.360
<v Speaker 2>dust cloud.

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00:14:32.840 --> 00:14:35.399
<v Speaker 3>Now, while that might have disappointed the people hoping to

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00:14:35.440 --> 00:14:38.519
<v Speaker 3>see a star explode in our lifetime, the scientific yield

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00:14:38.600 --> 00:14:39.519
<v Speaker 3>from that event.

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<v Speaker 2>Was vital, oh absolutely crucial.

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00:14:40.840 --> 00:14:44.080
<v Speaker 3>Because it forced Montage and his team to become intimately

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<v Speaker 3>familiar with the optical quirks of Beetle Juice.

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00:14:46.559 --> 00:14:49.480
<v Speaker 2>Right. They learned how to handle the overwhelming glare of

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00:14:49.519 --> 00:14:52.399
<v Speaker 2>its surface, how to process the noise in the data,

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00:14:52.799 --> 00:14:55.360
<v Speaker 2>and how to push the VLT to its absolute limits.

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00:14:55.399 --> 00:14:58.559
<v Speaker 3>They basically forged the exact specific skill set required to

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00:14:58.639 --> 00:15:00.120
<v Speaker 3>hunt down the companion star.

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00:15:00.120 --> 00:15:03.759
<v Speaker 2>Exactly, and once the dust cleared, literally, the focus shifted

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00:15:03.879 --> 00:15:05.080
<v Speaker 2>back to that century old.

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00:15:04.879 --> 00:15:07.559
<v Speaker 3>Mystery because the periodicity was still there, still there, the

321
00:15:07.679 --> 00:15:10.519
<v Speaker 3>radial velocity wobble was still there, but they needed a

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00:15:10.600 --> 00:15:14.559
<v Speaker 3>highly specific window to actually attempt a direct observation. You

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00:15:14.600 --> 00:15:17.679
<v Speaker 3>can't just point the VLT at Beetlejuice on a random

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00:15:17.720 --> 00:15:20.080
<v Speaker 3>Tuesday and hope to spot the companion.

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00:15:20.200 --> 00:15:21.759
<v Speaker 2>No, you need a treasure map.

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00:15:21.720 --> 00:15:25.720
<v Speaker 3>Right, And in twenty twenty four, two robust astronomical studies

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00:15:25.799 --> 00:15:27.320
<v Speaker 3>essentially provided that map.

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00:15:27.480 --> 00:15:32.200
<v Speaker 2>They synthesized decades of astrometric and radial velocity data by

329
00:15:32.679 --> 00:15:36.840
<v Speaker 2>meticulously mapping the gravitational wobble we talked about. They reconstructed

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00:15:36.840 --> 00:15:37.879
<v Speaker 2>the invisible orbit.

331
00:15:38.000 --> 00:15:41.519
<v Speaker 3>They didn't just confirm the companion's existence, they calculated its

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00:15:41.559 --> 00:15:43.120
<v Speaker 3>exact orbital trajectory.

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00:15:43.240 --> 00:15:46.240
<v Speaker 2>Yes, and they predicted that in December of twenty twenty four,

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00:15:46.720 --> 00:15:50.039
<v Speaker 2>the companion would reach a very specific geometric point known

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00:15:50.080 --> 00:15:51.960
<v Speaker 2>as maximum elongation.

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00:15:52.159 --> 00:15:54.679
<v Speaker 3>Okay, this is the critical physical concept that made the

337
00:15:54.720 --> 00:15:58.559
<v Speaker 3>discovery possible. Let's map out maximum elongation for everyone. Why

338
00:15:58.600 --> 00:16:01.639
<v Speaker 3>does the physical distance the visual separation from the main

339
00:16:01.720 --> 00:16:04.360
<v Speaker 3>star dictate whether or not we can see it.

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00:16:04.360 --> 00:16:06.399
<v Speaker 2>It comes right back to the contrast ratio and the

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00:16:06.440 --> 00:16:09.799
<v Speaker 2>physical limits of our optics. The anglier separation between the

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00:16:09.799 --> 00:16:12.559
<v Speaker 2>primary star and the companion, as viewed from Earth is

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00:16:12.600 --> 00:16:13.799
<v Speaker 2>incredibly small.

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00:16:13.679 --> 00:16:15.840
<v Speaker 3>Because they're six hundred and fifty light years away.

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00:16:16.159 --> 00:16:19.039
<v Speaker 2>Exactly so, when the companion is moving through the part

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00:16:19.039 --> 00:16:21.120
<v Speaker 2>of its orbit that brings it in front of or

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00:16:21.120 --> 00:16:25.799
<v Speaker 2>behind Beetle Juice, the angular separation is virtually zero. The

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00:16:25.879 --> 00:16:29.159
<v Speaker 2>light of the companion is entirely swallowed by the diffraction

349
00:16:29.320 --> 00:16:30.519
<v Speaker 2>halo of the supergent.

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00:16:30.679 --> 00:16:34.960
<v Speaker 3>It's like trying to spot a single faint firefly buzzing

351
00:16:35.000 --> 00:16:39.039
<v Speaker 3>around a massive stadium floodlight. Perfect If the firefly is

352
00:16:39.120 --> 00:16:41.919
<v Speaker 3>hovering just an inch from the glass of the floodlight,

353
00:16:42.240 --> 00:16:45.840
<v Speaker 3>it is completely consumed by the glare. You have absolutely

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00:16:45.960 --> 00:16:48.759
<v Speaker 3>zero chance of resolving the light of the insect against

355
00:16:48.799 --> 00:16:51.120
<v Speaker 3>the millions of lumens pouring out of the bulb. Right

356
00:16:51.480 --> 00:16:53.840
<v Speaker 3>your only hope is to wait for the exact moment

357
00:16:53.919 --> 00:16:56.200
<v Speaker 3>the firefly flies a few feet away from the bulb

358
00:16:56.399 --> 00:16:59.000
<v Speaker 3>out toward the very edge of the floodlight's beam.

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00:16:59.000 --> 00:17:02.120
<v Speaker 2>And maximum elong is that exact moment. It is the

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00:17:02.159 --> 00:17:04.920
<v Speaker 2>point in the orbit where the physical geometry places the

361
00:17:04.960 --> 00:17:08.720
<v Speaker 2>companion at its widest possible apparent distance from the primary star.

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00:17:09.119 --> 00:17:10.880
<v Speaker 2>From our perspective here on Earth.

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00:17:10.720 --> 00:17:13.880
<v Speaker 3>It maximizes the angular separation. So the twenty twenty four

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00:17:13.920 --> 00:17:17.559
<v Speaker 3>mathematical models basically provided Montage and his team with a

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00:17:17.640 --> 00:17:21.799
<v Speaker 3>definitive deadline. They mapped the orbit and said the firefly

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00:17:21.920 --> 00:17:24.160
<v Speaker 3>will be at the edge of the floodlight's beam in

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00:17:24.240 --> 00:17:27.400
<v Speaker 3>December twenty twenty four. If you want to take a picture,

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00:17:27.599 --> 00:17:30.119
<v Speaker 3>this is your only window before the orbit carries it

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00:17:30.160 --> 00:17:31.000
<v Speaker 3>back into the glare.

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00:17:31.279 --> 00:17:34.160
<v Speaker 2>Yeah, we gave them the win, but knowing when to

371
00:17:34.279 --> 00:17:37.880
<v Speaker 2>look is useless if you lack the optical hardware to

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00:17:37.920 --> 00:17:40.680
<v Speaker 2>overcome the fundamental physics of light diffraction.

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00:17:40.440 --> 00:17:44.079
<v Speaker 3>Which is where the story shifts to the engineering marvel

374
00:17:44.160 --> 00:17:48.039
<v Speaker 3>of the VLT and a specific instrument called sphere. Yes,

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00:17:48.200 --> 00:17:51.920
<v Speaker 3>let's break down the VLT, the very Large telescope located

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00:17:51.920 --> 00:17:55.640
<v Speaker 3>in the Atacama Desert in Chile, the location itself is

377
00:17:55.680 --> 00:17:57.440
<v Speaker 3>basically half the technology, right.

378
00:17:57.519 --> 00:17:59.920
<v Speaker 2>Oh, absolutely, yeah. You need an environment that removes it

379
00:18:00.000 --> 00:18:03.000
<v Speaker 2>as much of Earth's atmosphere from the equation as possible.

380
00:18:02.680 --> 00:18:04.960
<v Speaker 3>Because atmosphere is the enemy of astronomy.

381
00:18:05.039 --> 00:18:07.720
<v Speaker 2>The ATA comma is one of the highest driest environments

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00:18:07.759 --> 00:18:11.680
<v Speaker 2>on the planet. Atmospheric water vapor absorbs light and atmosphere

383
00:18:11.680 --> 00:18:15.359
<v Speaker 2>turbulence you know, hot and cold pockets of air mixing

384
00:18:15.400 --> 00:18:17.240
<v Speaker 2>together that bends and distorted starlight.

385
00:18:17.359 --> 00:18:20.599
<v Speaker 3>It's what causes stars to twinkle, right, And for.

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00:18:20.559 --> 00:18:24.119
<v Speaker 2>An astronomer, trying to resolve a faint companion star next

387
00:18:24.160 --> 00:18:27.759
<v Speaker 2>to a supergent twinkling is catastrophic. It smears the light

388
00:18:27.799 --> 00:18:28.799
<v Speaker 2>all across the detector.

389
00:18:28.960 --> 00:18:31.039
<v Speaker 3>But even in the auta comma, you still have some

390
00:18:31.200 --> 00:18:34.759
<v Speaker 3>atmosphere to punch through. You're not in space, and more importantly,

391
00:18:34.880 --> 00:18:38.240
<v Speaker 3>you still have the overwhelming blinding glare of beetle juice

392
00:18:38.279 --> 00:18:40.039
<v Speaker 3>itself to deal with, which.

393
00:18:39.799 --> 00:18:42.920
<v Speaker 2>Is where the sphere instrument comes in. Anthony Baccaletti, a

394
00:18:42.920 --> 00:18:45.880
<v Speaker 2>co author on the new study, pointed out something really fascinating.

395
00:18:46.359 --> 00:18:49.759
<v Speaker 2>Sphere was not designed to look at aging superdians. No, No,

396
00:18:49.880 --> 00:18:51.680
<v Speaker 2>it is an exoplanet hunting tool.

397
00:18:51.799 --> 00:18:53.359
<v Speaker 3>Oh Wow, so they repurposed it.

398
00:18:53.559 --> 00:18:56.880
<v Speaker 2>Yeah, but the crossover an application is brilliant. Finding a

399
00:18:56.920 --> 00:19:00.799
<v Speaker 2>Jupiter sized planet orbiting a distant stars the exact same

400
00:19:00.839 --> 00:19:04.799
<v Speaker 2>optical challenge as finding a massive companion star orbiting an

401
00:19:04.880 --> 00:19:06.920
<v Speaker 2>impossibly bright supergion.

402
00:19:06.599 --> 00:19:09.880
<v Speaker 3>Because in both cases, the primary star is billions of

403
00:19:09.920 --> 00:19:11.200
<v Speaker 3>times brighter than the target.

404
00:19:11.400 --> 00:19:14.839
<v Speaker 2>Exactly to reveal the target, you must artificially suppress the

405
00:19:14.920 --> 00:19:16.440
<v Speaker 2>light of the primary star.

406
00:19:16.799 --> 00:19:20.160
<v Speaker 3>But how exactly does sphere suppress the light of a

407
00:19:20.200 --> 00:19:23.559
<v Speaker 3>star that bright without blinding the rest of the image.

408
00:19:23.759 --> 00:19:25.799
<v Speaker 3>I mean, I know we can block light physically, like

409
00:19:25.880 --> 00:19:27.799
<v Speaker 3>holding your hand up to the sun to see an airplane,

410
00:19:28.519 --> 00:19:32.000
<v Speaker 3>but at an astronomical scale, diffraction must cause the light

411
00:19:32.079 --> 00:19:34.960
<v Speaker 3>waves to bleed around the edges of whatever block you use, Right,

412
00:19:35.279 --> 00:19:37.400
<v Speaker 3>how do they solve the physics of the light bending

413
00:19:37.440 --> 00:19:38.160
<v Speaker 3>around the mass?

414
00:19:38.240 --> 00:19:40.920
<v Speaker 2>That is the defining genius of a coronagraph, which is

415
00:19:40.960 --> 00:19:44.440
<v Speaker 2>the absolute heart of the sphere instrument. It doesn't just

416
00:19:44.640 --> 00:19:47.799
<v Speaker 2>use a simple physical block. It uses a series of

417
00:19:47.920 --> 00:19:52.599
<v Speaker 2>highly engineered optical masks and stops to actively manage the

418
00:19:52.640 --> 00:19:53.759
<v Speaker 2>diffraction of light waves.

419
00:19:54.000 --> 00:19:56.119
<v Speaker 3>Okay, walk me through this. Walk through the path of

420
00:19:56.119 --> 00:19:57.960
<v Speaker 3>the light as it enters the telescope.

421
00:19:58.119 --> 00:20:01.279
<v Speaker 2>Right First, the light from beetlejuice enters the primary mirror

422
00:20:01.359 --> 00:20:04.640
<v Speaker 2>of the VLT, but before it reaches the chronograph, it

423
00:20:04.720 --> 00:20:06.799
<v Speaker 2>passes through an adaptive optic system.

424
00:20:06.880 --> 00:20:08.920
<v Speaker 3>Okay, to fix the twinkling exactly.

425
00:20:09.240 --> 00:20:12.519
<v Speaker 2>This is crucial for correcting that atmospheric smearing we just discussed.

426
00:20:13.119 --> 00:20:17.160
<v Speaker 2>The VLT actually fires a powerful laser into the upper atmosphere.

427
00:20:17.200 --> 00:20:17.680
<v Speaker 3>A laser.

428
00:20:17.759 --> 00:20:20.240
<v Speaker 2>Yeah. It excites sodium atoms in the mesosphere to create

429
00:20:20.279 --> 00:20:21.799
<v Speaker 2>an artificial guide star.

430
00:20:21.839 --> 00:20:24.160
<v Speaker 3>A fake star that uses a reference point.

431
00:20:24.079 --> 00:20:27.720
<v Speaker 2>Exactly, and a sensor measures exactly how the atmosphere is

432
00:20:27.759 --> 00:20:30.920
<v Speaker 2>distorting the light of that artificial guide star thousands of

433
00:20:30.960 --> 00:20:31.640
<v Speaker 2>times a second.

434
00:20:31.880 --> 00:20:34.319
<v Speaker 3>That's crazy fast, it has to be ya.

435
00:20:34.480 --> 00:20:38.160
<v Speaker 2>It feeds that distortion data to a deformable mirror inside

436
00:20:38.160 --> 00:20:42.000
<v Speaker 2>the telescope. This mirror has hundreds of tiny actuators behind

437
00:20:42.039 --> 00:20:44.599
<v Speaker 2>it that physically change the shape of the mirror surface

438
00:20:44.640 --> 00:20:45.359
<v Speaker 2>in real time.

439
00:20:45.920 --> 00:20:47.440
<v Speaker 3>Wait, they bend the mirror.

440
00:20:47.599 --> 00:20:51.200
<v Speaker 2>They constantly ripple and bend the glass, perfectly countering the

441
00:20:51.200 --> 00:20:55.160
<v Speaker 2>atmospheric turbulence. It essentially flattens the light waves back out,

442
00:20:55.240 --> 00:20:56.599
<v Speaker 2>removing the twinkle entirely.

443
00:20:56.880 --> 00:20:59.960
<v Speaker 3>So now you have a perfectly sharp, pristine beam of

444
00:21:00.160 --> 00:21:02.480
<v Speaker 3>light from Beetlejuice entering the coronagraph.

445
00:21:02.559 --> 00:21:06.319
<v Speaker 2>Yes, and the beam hits a focal plane mask. This

446
00:21:06.440 --> 00:21:09.400
<v Speaker 2>is a tiny opaque dot precisely aligned to block the

447
00:21:09.440 --> 00:21:11.440
<v Speaker 2>central core of Beetlejuice's.

448
00:21:10.839 --> 00:21:12.960
<v Speaker 3>Light, the hand locking the sun right.

449
00:21:13.720 --> 00:21:15.759
<v Speaker 2>But as you pointed out, light acts as a wave.

450
00:21:16.279 --> 00:21:18.799
<v Speaker 2>When it hits the edge of that opaque dot, it diffracts.

451
00:21:19.000 --> 00:21:21.480
<v Speaker 2>It bends around the mask, creating a series of bright

452
00:21:21.559 --> 00:21:23.839
<v Speaker 2>concentric rings called an airy pattern.

453
00:21:23.920 --> 00:21:24.559
<v Speaker 3>So it leaks.

454
00:21:24.920 --> 00:21:28.799
<v Speaker 2>It leaks badly. If you stop there, those diffraction rings

455
00:21:28.839 --> 00:21:31.000
<v Speaker 2>will completely wash out the companion star.

456
00:21:31.279 --> 00:21:33.160
<v Speaker 3>The light bleeds over, So how do you clean up

457
00:21:33.160 --> 00:21:33.559
<v Speaker 3>the bleed?

458
00:21:34.079 --> 00:21:37.119
<v Speaker 2>The light passes through a second lens which refocuses the beam,

459
00:21:37.200 --> 00:21:40.319
<v Speaker 2>and then it hits a lio stop. A lio stop, Yeah,

460
00:21:40.319 --> 00:21:44.039
<v Speaker 2>it's a highly specific aperture placed further down the optical

461
00:21:44.079 --> 00:21:48.400
<v Speaker 2>path that is mathematically designed to block those diffracted light

462
00:21:48.480 --> 00:21:51.200
<v Speaker 2>rings while letting the rest of the light pass through.

463
00:21:51.880 --> 00:21:54.720
<v Speaker 2>It essentially clips the noisy edges off the light beam.

464
00:21:54.799 --> 00:21:57.480
<v Speaker 3>You are physically stripping away the glare a layer by

465
00:21:57.599 --> 00:21:59.240
<v Speaker 3>layer using wave optics.

466
00:21:59.319 --> 00:22:02.920
<v Speaker 2>It's pievable engineering. But even with adaptive optics in a

467
00:22:02.920 --> 00:22:06.599
<v Speaker 2>perfect coronagraph. The suppression is never one hundred percent perfect.

468
00:22:06.680 --> 00:22:08.200
<v Speaker 3>There's always some noise leftover.

469
00:22:08.359 --> 00:22:13.079
<v Speaker 2>Always there are microscopic imperfections in the mirrors, slight thermal

470
00:22:13.079 --> 00:22:16.200
<v Speaker 2>shifts in the instrument itself, resulting in a residual halo

471
00:22:16.240 --> 00:22:18.759
<v Speaker 2>of scattered light. We call it speckel noise.

472
00:22:18.920 --> 00:22:21.400
<v Speaker 3>And let me guess, these speckles can look exactly like

473
00:22:21.440 --> 00:22:22.960
<v Speaker 3>a faint companion star.

474
00:22:23.119 --> 00:22:26.039
<v Speaker 2>Exactly like it. So when Montages and his team look

475
00:22:26.119 --> 00:22:29.720
<v Speaker 2>through Sphere in December twenty twenty four during that maximum

476
00:22:29.720 --> 00:22:33.480
<v Speaker 2>elongation window, they don't just see a clean image of

477
00:22:33.559 --> 00:22:35.519
<v Speaker 2>beetle juiced bee sitting there in the dark.

478
00:22:35.599 --> 00:22:36.720
<v Speaker 3>They just see static.

479
00:22:37.079 --> 00:22:40.079
<v Speaker 2>They capture the raw data, which looks like a chaotic,

480
00:22:40.640 --> 00:22:44.640
<v Speaker 2>noisy halo of residual light. The actual discovery happens during

481
00:22:44.680 --> 00:22:50.720
<v Speaker 2>the post processing phase, which takes months of intense computational labor. Months.

482
00:22:51.200 --> 00:22:54.519
<v Speaker 2>The use a technique called angular differential imaging or EIGHTYI.

483
00:22:55.079 --> 00:22:58.839
<v Speaker 3>How does ADI separate the fake speckles of noise from

484
00:22:58.880 --> 00:23:00.559
<v Speaker 3>the actual light of the hidden star.

485
00:23:00.839 --> 00:23:03.720
<v Speaker 2>It's actually brilliant. It exploits the rotation of the Earth. Okay,

486
00:23:03.759 --> 00:23:06.559
<v Speaker 2>how as the telescope tracks beetle jews cross the sky

487
00:23:06.640 --> 00:23:10.480
<v Speaker 2>over several hours, the optical field of view naturally rotates

488
00:23:10.519 --> 00:23:14.359
<v Speaker 2>relative to the instrument itself. This means the actual astrophysical

489
00:23:14.359 --> 00:23:17.559
<v Speaker 2>objects like the companion star will slowly rotate through the

490
00:23:17.559 --> 00:23:19.000
<v Speaker 2>field of view over time.

491
00:23:18.839 --> 00:23:22.519
<v Speaker 3>But the optical imperfections the speckles caused by the telescope's

492
00:23:22.519 --> 00:23:23.599
<v Speaker 3>own mirrors.

493
00:23:23.200 --> 00:23:26.000
<v Speaker 2>They stay fixed in place relative to the detector.

494
00:23:26.079 --> 00:23:28.119
<v Speaker 3>Oh that is so smart, isn't it.

495
00:23:28.480 --> 00:23:32.119
<v Speaker 2>By taking hundreds of images over several hours, astronomers can

496
00:23:32.160 --> 00:23:36.279
<v Speaker 2>run complex algorithms that isolate the static noise and literally

497
00:23:36.319 --> 00:23:37.920
<v Speaker 2>subtract it out of the sequence.

498
00:23:38.039 --> 00:23:38.519
<v Speaker 3>Wow.

499
00:23:38.599 --> 00:23:41.559
<v Speaker 2>Once you peel away the static speckel noise, the true

500
00:23:41.640 --> 00:23:44.359
<v Speaker 2>light of the companion star, which rotated with the sky,

501
00:23:45.000 --> 00:23:46.039
<v Speaker 2>is finally revealed.

502
00:23:46.240 --> 00:23:48.680
<v Speaker 3>I really want to focus on the psychological weight of

503
00:23:48.720 --> 00:23:51.519
<v Speaker 3>those months of data processing for a second. It must

504
00:23:51.519 --> 00:23:56.759
<v Speaker 3>have been excruciating, right you are, Miguel Montage. Use the

505
00:23:57.039 --> 00:24:00.519
<v Speaker 3>exact window predicted by the twenty twenty four orbital models.

506
00:24:00.880 --> 00:24:04.319
<v Speaker 3>You used sphere, the most advanced coronograph on the planet.

507
00:24:04.599 --> 00:24:06.839
<v Speaker 3>But you also know that for one hundred years, this

508
00:24:06.920 --> 00:24:09.759
<v Speaker 3>star has defeated every single astronomer who tried to find

509
00:24:09.799 --> 00:24:10.519
<v Speaker 3>its companion.

510
00:24:10.759 --> 00:24:12.039
<v Speaker 2>Every single one, and you.

511
00:24:12.000 --> 00:24:15.160
<v Speaker 3>Were sitting at a computer running eighty I algorithms, ruthlessly

512
00:24:15.240 --> 00:24:18.079
<v Speaker 3>doubting your own findings, wondering if a speck of light

513
00:24:18.079 --> 00:24:20.640
<v Speaker 3>on the screen is a thermal artifact or a century

514
00:24:20.640 --> 00:24:21.200
<v Speaker 3>old ghost.

515
00:24:21.720 --> 00:24:24.519
<v Speaker 2>The rigor required in that phase is immense. You have

516
00:24:24.559 --> 00:24:26.839
<v Speaker 2>to prove to yourself that you haven't just manufactured a

517
00:24:26.880 --> 00:24:29.599
<v Speaker 2>star at a statistical noise. You have to be your

518
00:24:29.640 --> 00:24:31.039
<v Speaker 2>own harshest critic.

519
00:24:31.039 --> 00:24:34.720
<v Speaker 3>Until the final algorithm finishes and the residual light of

520
00:24:34.759 --> 00:24:39.680
<v Speaker 3>beetlejuice is completely digitally subtracted, and there, sitting in the

521
00:24:39.759 --> 00:24:42.480
<v Speaker 3>dark space exactly where the math predicted it would be,

522
00:24:43.079 --> 00:24:45.799
<v Speaker 3>is a distinct, undeniable source of light.

523
00:24:46.240 --> 00:24:49.519
<v Speaker 2>And Montage has actually described his reaction to seeing the

524
00:24:49.559 --> 00:24:53.240
<v Speaker 2>final processed image. He said, he jumped from his chair.

525
00:24:53.400 --> 00:24:54.559
<v Speaker 3>I would have screamed.

526
00:24:54.920 --> 00:24:58.640
<v Speaker 2>It is the ultimate vindication of predictive science. The light

527
00:24:58.720 --> 00:25:02.240
<v Speaker 2>of the Companions star traveling across six hundred and fifty

528
00:25:02.319 --> 00:25:06.240
<v Speaker 2>light years of space, finally extracted from the glare by

529
00:25:06.359 --> 00:25:07.359
<v Speaker 2>human engineering.

530
00:25:07.799 --> 00:25:11.359
<v Speaker 3>But the discovery immediately pivoted from a technological victory into

531
00:25:11.359 --> 00:25:14.720
<v Speaker 3>a massive scientific shock, A huge shock because they found it. Yes,

532
00:25:15.119 --> 00:25:18.240
<v Speaker 3>but the reality of what beetlejewics Be actually has wildly

533
00:25:18.279 --> 00:25:20.119
<v Speaker 3>contradicted the long standing theories.

534
00:25:20.200 --> 00:25:21.880
<v Speaker 2>Oh totally threw the models out the window.

535
00:25:22.000 --> 00:25:24.759
<v Speaker 3>Yeah, Montage admitted he honestly didn't think spear had the

536
00:25:24.799 --> 00:25:28.720
<v Speaker 3>sensitivity to detect the star based on those earlier predictions.

537
00:25:28.160 --> 00:25:31.160
<v Speaker 2>Because the predictive math was flawless regarding the location of

538
00:25:31.200 --> 00:25:34.400
<v Speaker 2>the companion, but it was drastically wrong about the nature

539
00:25:34.440 --> 00:25:35.079
<v Speaker 2>of the companion.

540
00:25:35.240 --> 00:25:35.480
<v Speaker 3>Right.

541
00:25:35.680 --> 00:25:38.359
<v Speaker 2>If beetlejews Bee had been a one solar mass star,

542
00:25:38.960 --> 00:25:43.039
<v Speaker 2>as the radial velocity models initially suggested, its luminosity would

543
00:25:43.039 --> 00:25:45.720
<v Speaker 2>have been too faint to pierce through the residual speckel

544
00:25:45.759 --> 00:25:48.559
<v Speaker 2>noise even at maximum elongation.

545
00:25:48.319 --> 00:25:51.480
<v Speaker 3>Even with all that incredible tech. Exactly so, why could

546
00:25:51.480 --> 00:25:52.640
<v Speaker 3>they see it because it.

547
00:25:52.640 --> 00:25:56.799
<v Speaker 2>Wasn't one solar mass. The VLT data confirmed that beatlejewics

548
00:25:56.839 --> 00:25:59.480
<v Speaker 2>B is actually two to three times the.

549
00:25:59.440 --> 00:26:02.319
<v Speaker 3>Mass of our That is a massive difference.

550
00:26:01.960 --> 00:26:05.160
<v Speaker 2>It really is. The increase in mass corresponds to an

551
00:26:05.200 --> 00:26:10.839
<v Speaker 2>exponential increase in luminosity. It was significantly brighter than anyone anticipated,

552
00:26:11.279 --> 00:26:14.880
<v Speaker 2>pushing it above the detection threshold of these seas vera.

553
00:26:14.640 --> 00:26:16.759
<v Speaker 3>Instrument which goes right back to your point about the

554
00:26:16.880 --> 00:26:20.960
<v Speaker 3>orbital tilt the cyanide degeneracy exactly. Because the orbit was

555
00:26:21.039 --> 00:26:23.799
<v Speaker 3>highly tilted relative to Earth, the actual mass had to

556
00:26:23.799 --> 00:26:27.440
<v Speaker 3>be much higher to produce the wobble We measured precisely.

557
00:26:27.240 --> 00:26:30.160
<v Speaker 2>And finding a three solar mass star hiding next to

558
00:26:30.240 --> 00:26:34.160
<v Speaker 2>Beetlejews forces a total recalibration of our understanding of the

559
00:26:34.319 --> 00:26:38.240
<v Speaker 2>entire system. Now, there were previous hints, like a possible

560
00:26:38.279 --> 00:26:41.799
<v Speaker 2>direct detection using the Gemini North Telescope in Hawaii.

561
00:26:41.519 --> 00:26:42.759
<v Speaker 3>But it wasn't definitive, right.

562
00:26:43.200 --> 00:26:47.000
<v Speaker 2>This ease Fear image is the definitive proof. It completely

563
00:26:47.039 --> 00:26:48.359
<v Speaker 2>removes the ambiguity.

564
00:26:48.559 --> 00:26:51.480
<v Speaker 3>Let's grasp the sheer scale of this. Again, a star

565
00:26:51.720 --> 00:26:54.400
<v Speaker 3>three times the mass of our entire Sun has been

566
00:26:54.680 --> 00:26:57.720
<v Speaker 3>hiding in plain sight for a century. I mean, if

567
00:26:57.720 --> 00:27:01.200
<v Speaker 3>you replaced our Sun with Beetletre's be the Earth would

568
00:27:01.240 --> 00:27:02.599
<v Speaker 3>be instantly vaporized.

569
00:27:02.680 --> 00:27:03.319
<v Speaker 2>One.

570
00:27:03.519 --> 00:27:06.519
<v Speaker 3>It is a massive, intensely bright star in its own right.

571
00:27:07.640 --> 00:27:10.440
<v Speaker 3>How does something that massive remain hidden?

572
00:27:10.680 --> 00:27:14.720
<v Speaker 2>It just highlights the monstrous immensity of the primary star. Yes,

573
00:27:14.759 --> 00:27:18.039
<v Speaker 2>Beetlejuice Bee is highly luminous, but Beetlejuice itself is emitting

574
00:27:18.119 --> 00:27:19.880
<v Speaker 2>roughly one hundred thousand times more light.

575
00:27:20.039 --> 00:27:21.680
<v Speaker 3>It's like trying to hear a whisper next to a

576
00:27:21.759 --> 00:27:23.240
<v Speaker 3>jet engine exactly.

577
00:27:23.680 --> 00:27:26.359
<v Speaker 2>Even a three solar mass star is completely lost in

578
00:27:26.359 --> 00:27:29.359
<v Speaker 2>that deluge of photons. You think you understand a stellar

579
00:27:29.400 --> 00:27:31.960
<v Speaker 2>neighborhood because you've observed it for hundreds of years, and

580
00:27:32.000 --> 00:27:34.559
<v Speaker 2>then you discover a mansion hidden behind a billboard you

581
00:27:34.599 --> 00:27:35.759
<v Speaker 2>never managed to look around.

582
00:27:35.880 --> 00:27:38.799
<v Speaker 3>Okay, so we have definitively found the hidden companion. We

583
00:27:38.880 --> 00:27:43.039
<v Speaker 3>know its mass, its orbit, and its reality. But in astrophysics,

584
00:27:43.200 --> 00:27:46.599
<v Speaker 3>answering a century old question immediately spawns a drastically more

585
00:27:46.640 --> 00:27:48.440
<v Speaker 3>complex set of physical problems.

586
00:27:48.519 --> 00:27:51.799
<v Speaker 2>Oh. Absolutely, the future of this system is fascinating because

587
00:27:51.799 --> 00:27:52.200
<v Speaker 2>we have to.

588
00:27:52.119 --> 00:27:54.720
<v Speaker 3>Look at the future of this binary system. But before

589
00:27:54.759 --> 00:27:57.759
<v Speaker 3>we get into the explosive stuff, we should mention the caveats.

590
00:27:57.279 --> 00:28:01.359
<v Speaker 2>Right, yes, rigorous scientific caveats. First, the team notes that

591
00:28:01.440 --> 00:28:05.599
<v Speaker 2>to achieve absolute certainty regarding the exact orbital mechanics, they

592
00:28:05.640 --> 00:28:08.039
<v Speaker 2>do need to observe it again in a year or so.

593
00:28:08.079 --> 00:28:11.839
<v Speaker 3>When the orbit carries beetlejuice Bee to the opposite side.

594
00:28:11.599 --> 00:28:14.720
<v Speaker 2>Of the supergent right, tracking it across multiple points in

595
00:28:14.759 --> 00:28:19.559
<v Speaker 2>its orbit locks in the kinematics. However, as Montage stated,

596
00:28:19.839 --> 00:28:22.119
<v Speaker 2>there is very little space left for doubt.

597
00:28:22.319 --> 00:28:25.559
<v Speaker 3>Okay, So, assuming Beetlejuice BEE is exactly what this data shows,

598
00:28:25.839 --> 00:28:29.839
<v Speaker 3>we face a monumental physical dilemma. We do Beetlejuice is

599
00:28:29.839 --> 00:28:33.920
<v Speaker 3>an evolved red supergent. It is on an irreversible path

600
00:28:34.000 --> 00:28:37.799
<v Speaker 3>to a core collapse supernova. How does the confirmed presence

601
00:28:37.839 --> 00:28:41.279
<v Speaker 3>of a massive three solar mass companion star alter the

602
00:28:41.319 --> 00:28:43.160
<v Speaker 3>explosive fate of the supergent.

603
00:28:43.480 --> 00:28:46.440
<v Speaker 2>It changes the entire paradigm of stellar death for.

604
00:28:46.440 --> 00:28:48.559
<v Speaker 3>This system because it's not alone anymore.

605
00:28:48.720 --> 00:28:53.160
<v Speaker 2>Exactly when a single isolated massive star goes supernova, the

606
00:28:53.200 --> 00:28:54.960
<v Speaker 2>physics are relatively straightforward.

607
00:28:55.079 --> 00:28:57.720
<v Speaker 3>Straightforward for a supernova anyway, fair point.

608
00:28:57.799 --> 00:29:00.559
<v Speaker 2>Yeah, But basically, the core runs out a new clear fuel,

609
00:29:00.839 --> 00:29:04.319
<v Speaker 2>the outward radiation pressure stops, gravity takes over, and the

610
00:29:04.319 --> 00:29:06.720
<v Speaker 2>core collapses inward at a fraction of the speed.

611
00:29:06.440 --> 00:29:08.160
<v Speaker 3>Of light, just a catastrophic free fall.

612
00:29:08.319 --> 00:29:12.440
<v Speaker 2>Right. The core compresses until it hits quantum degeneracy, basically

613
00:29:12.480 --> 00:29:16.480
<v Speaker 2>bounces off itself, rebounds, and sends a shockwave outward that

614
00:29:16.559 --> 00:29:19.640
<v Speaker 2>blows the outer layers of the star into a spherical,

615
00:29:19.680 --> 00:29:20.680
<v Speaker 2>expanding nebula.

616
00:29:21.039 --> 00:29:24.039
<v Speaker 3>But when you introduce a massive companion star into the

617
00:29:24.240 --> 00:29:26.000
<v Speaker 3>immediate vicinity.

618
00:29:25.720 --> 00:29:28.599
<v Speaker 2>The dynamics of that collapse become infinitely more chaotic.

619
00:29:28.799 --> 00:29:31.519
<v Speaker 3>We enter the realm of binary stellar evolution.

620
00:29:31.880 --> 00:29:35.880
<v Speaker 2>Yes, and the most critical factor here is gravity and

621
00:29:35.920 --> 00:29:37.720
<v Speaker 2>a concept known as the rochlobe.

622
00:29:37.960 --> 00:29:41.680
<v Speaker 3>Okay, let's explore the roach slobe. How does gravity fundamentally

623
00:29:41.720 --> 00:29:44.279
<v Speaker 3>alter the shape and behavior of the supergent before it

624
00:29:44.319 --> 00:29:45.119
<v Speaker 3>even explodes.

625
00:29:45.400 --> 00:29:48.880
<v Speaker 2>Well, In a binary system, each star exerts a gravitational pull.

626
00:29:49.640 --> 00:29:52.480
<v Speaker 2>The roachlobe is basically the tear drop shaped region of

627
00:29:52.519 --> 00:29:55.559
<v Speaker 2>space around a star where its own gravity is dominant

628
00:29:55.599 --> 00:29:56.880
<v Speaker 2>over the companion's gravity.

629
00:29:56.920 --> 00:29:58.759
<v Speaker 3>It's like a gravitational boundary line.

630
00:29:58.960 --> 00:30:03.400
<v Speaker 2>Yes. When Beetlegoose was a younger, smaller star, it sat

631
00:30:03.519 --> 00:30:05.920
<v Speaker 2>comfortably deep within its own roachlobe.

632
00:30:05.960 --> 00:30:08.480
<v Speaker 3>All of its gas and plasma were securely bound to

633
00:30:08.519 --> 00:30:10.519
<v Speaker 3>its own gravitational center exactly.

634
00:30:11.119 --> 00:30:15.559
<v Speaker 2>But as it evolved into a red supergient, it expanded massively.

635
00:30:15.960 --> 00:30:20.359
<v Speaker 2>Its outer atmosphere puffed up to an incredible degree. Now,

636
00:30:20.519 --> 00:30:23.640
<v Speaker 2>if the outer layers of beetle Jews expands so much

637
00:30:23.960 --> 00:30:27.000
<v Speaker 2>that they breached the boundary of its roachlobe, the material

638
00:30:27.079 --> 00:30:30.240
<v Speaker 2>is no longer gravitationally bound to the suburgent. It crosses

639
00:30:30.279 --> 00:30:30.920
<v Speaker 2>the tipping.

640
00:30:30.680 --> 00:30:33.079
<v Speaker 3>Point, which is the l one Lagrangeen point right, Yes,

641
00:30:33.079 --> 00:30:34.359
<v Speaker 3>the l one Lagrangian point yea.

642
00:30:34.599 --> 00:30:37.960
<v Speaker 2>At that point, the gravitational pull of beetlejuice B actually

643
00:30:37.960 --> 00:30:38.480
<v Speaker 2>takes over.

644
00:30:38.720 --> 00:30:39.319
<v Speaker 3>Oh wow.

645
00:30:39.440 --> 00:30:42.559
<v Speaker 2>The three solar mass companion can begin actively stripping the

646
00:30:42.599 --> 00:30:46.200
<v Speaker 2>outer layers of hydrogen away from the dying supergent. We

647
00:30:46.279 --> 00:30:49.119
<v Speaker 2>call this rochlobe overflow or mass transfer.

648
00:30:49.480 --> 00:30:53.000
<v Speaker 3>So the companion is essentially cannibalizing the supergen's atmosphere before

649
00:30:53.000 --> 00:30:54.960
<v Speaker 3>the core even collapses.

650
00:30:54.440 --> 00:30:56.039
<v Speaker 2>Actively pulling material onto itself.

651
00:30:56.119 --> 00:30:59.400
<v Speaker 3>Yes, how to stripping those outer layers change the mechanics

652
00:30:59.400 --> 00:31:00.759
<v Speaker 3>of the eventual supernova?

653
00:31:00.799 --> 00:31:03.400
<v Speaker 2>It can fundamentally alter the classification in the light curve

654
00:31:03.440 --> 00:31:04.160
<v Speaker 2>of the explosion.

655
00:31:04.440 --> 00:31:05.359
<v Speaker 3>Okay, how so.

656
00:31:05.480 --> 00:31:08.839
<v Speaker 2>If red supergen explodes with its massive outer envelope of

657
00:31:08.920 --> 00:31:13.000
<v Speaker 2>hydrogen mostly intact, it typically produces what we call a

658
00:31:13.119 --> 00:31:17.519
<v Speaker 2>TYPEIP supernova. The P stands for plateau.

659
00:31:17.480 --> 00:31:19.640
<v Speaker 3>Meaning the brightness stays stable for a while.

660
00:31:19.799 --> 00:31:23.599
<v Speaker 2>Exactly, the explosion stays incredibly bright for months as the

661
00:31:23.640 --> 00:31:27.640
<v Speaker 2>shockwave slowly pushes through that thick, dense hydrogen envelope.

662
00:31:27.680 --> 00:31:31.079
<v Speaker 3>But if Beetleg's B has stripped a significant portion of

663
00:31:31.119 --> 00:31:33.160
<v Speaker 3>that hydrogen envelope away beforehand.

664
00:31:33.279 --> 00:31:36.640
<v Speaker 2>Then the shockwave encounters much less resistance. You might get

665
00:31:36.640 --> 00:31:39.839
<v Speaker 2>a totally different light curve, potentially closer to a tybil

666
00:31:40.160 --> 00:31:43.240
<v Speaker 2>or even pushing toward a stripped envelope supernova if enough

667
00:31:43.279 --> 00:31:44.759
<v Speaker 2>mass is transferred so.

668
00:31:44.759 --> 00:31:47.200
<v Speaker 3>The neighbor changes the whole explosion profile.

669
00:31:47.400 --> 00:31:49.720
<v Speaker 2>Right, The total mass of the star at the absolute

670
00:31:49.720 --> 00:31:53.000
<v Speaker 2>moment of core collapse dictates how the explosion unfolds, how

671
00:31:53.039 --> 00:31:56.119
<v Speaker 2>bright it gets, and what specific heavy elements are synthesized

672
00:31:56.119 --> 00:31:58.160
<v Speaker 2>and ejected out into the interstellar medium.

673
00:31:58.319 --> 00:32:00.960
<v Speaker 3>Let's use an analogy for this. Imagine you were watching

674
00:32:01.039 --> 00:32:04.319
<v Speaker 3>the scheduled demolition of a massive, derelict skyscraper.

675
00:32:04.359 --> 00:32:05.359
<v Speaker 2>Okay, I'm picturing it.

676
00:32:05.680 --> 00:32:08.359
<v Speaker 3>You have the blueprints, you know exactly where the demolition

677
00:32:08.480 --> 00:32:10.920
<v Speaker 3>charges replaced, and you can calculate exactly how it's going

678
00:32:10.960 --> 00:32:13.640
<v Speaker 3>to fall into its own footprint. It's a known quantity,

679
00:32:13.799 --> 00:32:17.359
<v Speaker 3>very predictable. But right before they push the plunger, you

680
00:32:17.400 --> 00:32:22.160
<v Speaker 3>suddenly realize there is a highly pressurized, fully fueled gas

681
00:32:22.160 --> 00:32:27.000
<v Speaker 3>station sitting directly on the property line, deeply entangled with

682
00:32:27.079 --> 00:32:29.359
<v Speaker 3>the structural supports of the skyscraper.

683
00:32:29.440 --> 00:32:30.720
<v Speaker 2>Oh, that's a brilliant way to put it.

684
00:32:30.720 --> 00:32:32.839
<v Speaker 3>The demolition is still going to happen, right The core

685
00:32:32.920 --> 00:32:36.279
<v Speaker 3>collapse is inevitable, but the dynamics of the fall, the

686
00:32:36.319 --> 00:32:39.599
<v Speaker 3>structural integrity of the outer walls, and the ensuing shockwave

687
00:32:39.920 --> 00:32:43.839
<v Speaker 3>just became infinitely more unpredictable because of that massive gravitational

688
00:32:43.839 --> 00:32:44.799
<v Speaker 3>anchor sitting.

689
00:32:44.559 --> 00:32:48.599
<v Speaker 2>Next door exactly, which brings up the ultimate question regarding

690
00:32:48.599 --> 00:32:50.720
<v Speaker 2>the fate of Beetlejeos B itself.

691
00:32:50.960 --> 00:32:53.599
<v Speaker 3>Yeah, what happens to the neighbor when the core of

692
00:32:53.640 --> 00:32:57.519
<v Speaker 3>the supergent collapses and unleashes literally the most violent event

693
00:32:57.559 --> 00:33:00.759
<v Speaker 3>in the universe. What happens to the companion stars sitting

694
00:33:00.880 --> 00:33:02.359
<v Speaker 3>right in the blast zone.

695
00:33:02.599 --> 00:33:05.240
<v Speaker 2>This is one of the most intense areas of study

696
00:33:05.359 --> 00:33:09.279
<v Speaker 2>in binary astrophysics right now. The survival of the companion

697
00:33:09.640 --> 00:33:14.519
<v Speaker 2>depends on several factors. Its orbital distance at the absolute

698
00:33:14.559 --> 00:33:18.359
<v Speaker 2>moment of explosion, its own density, and the sheer kinetic

699
00:33:18.480 --> 00:33:20.759
<v Speaker 2>energy of the supernova ejecta.

700
00:33:21.000 --> 00:33:24.680
<v Speaker 3>Is it possible the shockwave vaporizes the companion entirely?

701
00:33:25.000 --> 00:33:28.480
<v Speaker 2>Vaporization of a three solar mass star is unlikely given

702
00:33:28.519 --> 00:33:30.960
<v Speaker 2>its own significant gravitational binding energy.

703
00:33:31.519 --> 00:33:32.720
<v Speaker 3>It's so it'll survive.

704
00:33:32.920 --> 00:33:37.160
<v Speaker 2>But the supernova shockwave slamming into the companion will cause

705
00:33:37.240 --> 00:33:41.039
<v Speaker 2>extreme structural damage. It will likely strip away the outer

706
00:33:41.160 --> 00:33:45.440
<v Speaker 2>layers of beetlejuice B, injecting massive amounts of heavy radioactive

707
00:33:45.440 --> 00:33:48.920
<v Speaker 2>elements from the supernova directly into the companion's.

708
00:33:48.480 --> 00:33:51.440
<v Speaker 3>Atmosphere, just blasting it with radioactive shrapnel.

709
00:33:51.559 --> 00:33:54.319
<v Speaker 2>Essentially, Yes, it will heavily pollute the surviving star.

710
00:33:54.240 --> 00:33:58.079
<v Speaker 3>But beyond the physical damage, the orbital mechanics completely shatter instantly.

711
00:33:58.119 --> 00:33:59.599
<v Speaker 2>This is what we call the slingshot effect.

712
00:33:59.839 --> 00:34:02.079
<v Speaker 3>Now, how Beatlege's B is being held in orbit by

713
00:34:02.079 --> 00:34:04.440
<v Speaker 3>the immense gravitational mass of the succursion.

714
00:34:04.799 --> 00:34:09.119
<v Speaker 2>Yes, but when the supernova occurs, the primary star ejects

715
00:34:09.159 --> 00:34:12.800
<v Speaker 2>a massive percentage of its total mass outward at significant

716
00:34:12.800 --> 00:34:14.039
<v Speaker 2>fractions of the speed of light.

717
00:34:14.159 --> 00:34:18.480
<v Speaker 3>The gravitational anchor just disappears almost instantaneously.

718
00:34:17.760 --> 00:34:20.960
<v Speaker 2>And because of the conservation of momentum, Beetlegbe will no

719
00:34:21.039 --> 00:34:23.800
<v Speaker 2>longer have a central mass to orbit. It's just gone.

720
00:34:24.000 --> 00:34:24.800
<v Speaker 3>So what does it do.

721
00:34:25.199 --> 00:34:28.159
<v Speaker 2>It will continue moving along its orbital trajectory at whatever

722
00:34:28.239 --> 00:34:31.239
<v Speaker 2>velocity it had at the exact moment of the explosion.

723
00:34:31.679 --> 00:34:34.000
<v Speaker 2>It will literally be launched out of the binary system

724
00:34:34.079 --> 00:34:34.840
<v Speaker 2>like a cannon ball.

725
00:34:34.920 --> 00:34:36.920
<v Speaker 3>It becomes a runaway star exactly.

726
00:34:37.440 --> 00:34:40.360
<v Speaker 2>Depending on its orbital velocity, it could become a hypervelocity

727
00:34:40.360 --> 00:34:44.760
<v Speaker 2>star shooting across the galaxy entirely unbound from its previous neighborhood.

728
00:34:44.800 --> 00:34:46.519
<v Speaker 3>That is wild to think about.

729
00:34:46.719 --> 00:34:50.119
<v Speaker 2>The discovery of this hidden companion has provided astrophysicists with

730
00:34:50.199 --> 00:34:53.960
<v Speaker 2>the ultimate real time laboratory to study the chaotic interplay

731
00:34:54.000 --> 00:34:57.800
<v Speaker 2>of mass transfer, orbital dynamics, and stellar death at the

732
00:34:57.840 --> 00:34:59.480
<v Speaker 2>extreme edge of physics.

733
00:34:59.599 --> 00:35:02.760
<v Speaker 3>It's just the scope of this entire journey forces a

734
00:35:02.800 --> 00:35:04.280
<v Speaker 3>complete shift in perspective.

735
00:35:04.440 --> 00:35:05.039
<v Speaker 2>It really does.

736
00:35:05.360 --> 00:35:05.639
<v Speaker 1>I mean.

737
00:35:05.880 --> 00:35:08.639
<v Speaker 3>We began with a brilliant, blinking red dot in the

738
00:35:08.679 --> 00:35:13.199
<v Speaker 3>winter sky, observed by generations of ancient astronomers who carefully

739
00:35:13.280 --> 00:35:17.119
<v Speaker 3>tracked its rhythmic variations just using their ice right. And

740
00:35:17.199 --> 00:35:20.719
<v Speaker 3>then we moved through a century of mathematical frustration, watching

741
00:35:20.840 --> 00:35:24.840
<v Speaker 3>light curves and radial velocity wobbles, mathematically proving a ghost

742
00:35:24.960 --> 00:35:27.320
<v Speaker 3>was in the machine, but lacking the optical hardware to

743
00:35:27.400 --> 00:35:28.199
<v Speaker 3>actually see it.

744
00:35:28.840 --> 00:35:32.199
<v Speaker 2>Then we analyzed the fluid dynamics of a subpergion, watching

745
00:35:32.280 --> 00:35:35.519
<v Speaker 2>a massive convective plume condense into a dust cloud that

746
00:35:35.559 --> 00:35:38.000
<v Speaker 2>triggered a global false alarm.

747
00:35:37.840 --> 00:35:41.000
<v Speaker 3>But which ultimately trained a specific team on how to

748
00:35:41.079 --> 00:35:43.519
<v Speaker 3>observe this exact, tricky system.

749
00:35:43.760 --> 00:35:47.000
<v Speaker 2>Yes, and we followed the predictive power of celestial mechanics,

750
00:35:47.320 --> 00:35:52.280
<v Speaker 2>calculating the exact window of maximum elongation in December twenty twenty.

751
00:35:51.960 --> 00:35:57.119
<v Speaker 3>Four, and finally, using advanced coronagraphs, adaptive optics correcting atmospheric

752
00:35:57.159 --> 00:36:00.679
<v Speaker 3>turbulence thousands of times a second, and months of angular

753
00:36:00.719 --> 00:36:05.199
<v Speaker 3>differential imaging algorithms to digitally strip away the diffraction glare,

754
00:36:05.679 --> 00:36:07.239
<v Speaker 3>human engineering pierced the veil.

755
00:36:07.400 --> 00:36:08.320
<v Speaker 2>We finally saw it.

756
00:36:08.440 --> 00:36:10.960
<v Speaker 3>We didn't just find a tiny rock. We confirmed a

757
00:36:11.079 --> 00:36:14.400
<v Speaker 3>massive three solar mass star hiding in plain sight.

758
00:36:14.719 --> 00:36:17.400
<v Speaker 2>It is a profound reminder that our models of the

759
00:36:17.480 --> 00:36:21.559
<v Speaker 2>universe are constantly subject to revision. The cosmos is inherently

760
00:36:21.599 --> 00:36:25.400
<v Speaker 2>more complex and more dramatic than our initial assumptions ever allow.

761
00:36:25.599 --> 00:36:27.840
<v Speaker 3>So the next time you step outside on a clear night,

762
00:36:28.119 --> 00:36:30.360
<v Speaker 3>allow your eyes to adjust to the dark and look

763
00:36:30.440 --> 00:36:33.519
<v Speaker 3>up at Orion's right shoulder. The relationship you have with

764
00:36:33.559 --> 00:36:35.920
<v Speaker 3>that ruby red point of light must change.

765
00:36:36.039 --> 00:36:40.079
<v Speaker 2>You're no longer looking at a solitary, dying giant quietly

766
00:36:40.119 --> 00:36:41.159
<v Speaker 2>waiting to collapse.

767
00:36:41.360 --> 00:36:44.880
<v Speaker 3>You are witnessing a high stakes gravitational dance. You are

768
00:36:44.880 --> 00:36:48.599
<v Speaker 3>looking at a system actively exchanging mass, altering its own

769
00:36:48.599 --> 00:36:49.960
<v Speaker 3>fate across the centuries.

770
00:36:50.199 --> 00:36:52.280
<v Speaker 2>It's beautiful and terrifying at the same time.

771
00:36:52.440 --> 00:36:56.280
<v Speaker 3>Completely consider the reality of that impending explosion when the

772
00:36:56.320 --> 00:36:59.840
<v Speaker 3>core of beetlegists finally fails, when the outward pressure drops

773
00:36:59.840 --> 00:37:02.920
<v Speaker 3>in a shockwave tears through the hydrogen envelope to light

774
00:37:03.000 --> 00:37:05.679
<v Speaker 3>up our night sky. Whether that happens tomorrow or one

775
00:37:05.760 --> 00:37:07.880
<v Speaker 3>hundred thousand years from now, we won't just be watching

776
00:37:07.920 --> 00:37:09.000
<v Speaker 3>the death of a single star.

777
00:37:09.320 --> 00:37:09.960
<v Speaker 2>No we won't.

778
00:37:10.239 --> 00:37:14.400
<v Speaker 3>We will be witnessing the violent, chaotic, and incredibly complicated

779
00:37:14.440 --> 00:37:18.320
<v Speaker 3>climax of a cosmic relationship that managed to stay entirely

780
00:37:18.400 --> 00:37:20.599
<v Speaker 3>hidden from human eyes for one hundred years.
