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 just imagine something for a second. Okay,

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<v Speaker 2>picture a ghost, but you know, not a sheet wearing

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<v Speaker 2>hovering in a hallway.

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<v Speaker 3>Kind of ghost, right, something a bit more substantial exactly.

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<v Speaker 2>I'm talking about a cosmic ghost, an entity that possesses

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<v Speaker 2>the mass of one million of our suns. That is

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<v Speaker 2>a lot of mass, it really is. And it's just

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<v Speaker 2>wandering entirely invisible through the dark, quiet suburbs of a

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<v Speaker 2>distant galaxy.

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<v Speaker 3>Just completely out in the open, but totally hidden.

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<v Speaker 2>Yeah, because it emits absolutely zero light. I mean, it

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<v Speaker 2>makes no sound. It is a perfect voice drifting through

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<v Speaker 2>the blackness of space.

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<v Speaker 3>It is the ultimate cosmic ambush, really.

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<v Speaker 2>Right, And the only reason we even know this staggering

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<v Speaker 2>thing is out there, the only reason we can perceive

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<v Speaker 2>it at all is because it just violently ate a star, a.

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<v Speaker 3>Million solar masses of pure gravity, completely hidden until the

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<v Speaker 3>exact moment a star takes one wrong step.

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<v Speaker 2>And today is July twenty seven, twenty twenty six, and

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<v Speaker 2>the entire world of astronomy just realized they were looking

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<v Speaker 2>at a massive reality bending paradigm shift.

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<v Speaker 3>Because it completely breaks the rules we thought we knew.

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<v Speaker 2>It totally does because we are looking at the discovery

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<v Speaker 2>of one of the universe's absolute rarest events. I'm talking

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<v Speaker 2>about a supermassive black hole, a true monster that is

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<v Speaker 2>not where it is supposed to be.

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<v Speaker 3>It's tens of thousands of light years away from its

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<v Speaker 3>designated home.

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<v Speaker 2>Right. It is a rogue, a wanderer. But you know,

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<v Speaker 2>before we get to the fact that this black hole

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<v Speaker 2>is wandering through the galactic suburbs, we really need to

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<v Speaker 2>set the scene.

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<v Speaker 3>Yeah, we have to talk about the catalyst.

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<v Speaker 2>Exactly, the murder scene itself. What exactly happens physically when

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<v Speaker 2>a star wanders too close to an invisible monster.

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<v Speaker 3>Well, the actual scientific term for this catalyst is a

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<v Speaker 3>tidal disruption event, or we usually just call it a TDE.

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<v Speaker 2>A TDE, got it, And it is.

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<v Speaker 3>Truly one of the most violent physical processes in the

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<v Speaker 3>known universe. To understand what happens, you really have to

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<v Speaker 3>look at the mechanics of gravity. Okay, specifically, you have

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<v Speaker 3>to understand that the gravity of a supermassive black hole

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<v Speaker 3>isn't just strong, it creates this extreme gradient.

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<v Speaker 2>The gradient meaning the poll is significantly stronger the closer

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<v Speaker 2>you get ragsactly, But wait, gravity always gets stronger the

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<v Speaker 2>closer you get to something like That's just how gravity works.

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<v Speaker 2>Why is it so extreme here that it literally shreds

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<v Speaker 2>a star?

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<v Speaker 3>So it has to do with the density and the

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<v Speaker 3>extreme proximity. Imagine a star very similar to our own Sun,

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<v Speaker 3>just tracing a path through a galaxy.

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<v Speaker 2>Okay, tracing its path.

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<v Speaker 3>Over millions of years. Its orbit happens to drift a

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<v Speaker 3>little too close to this hidden million solar mass black.

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<v Speaker 2>Hole, just a little too close.

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<v Speaker 3>Right, And because a black hole is so incredibly dense,

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<v Speaker 3>the star can get extremely close to the center of

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<v Speaker 3>that mass without hitting a physical surface.

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<v Speaker 2>Because it's a singularity, not a giant rock.

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<v Speaker 3>Yes, So as it approaches the gravitational poll on the

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<v Speaker 3>side of the star facing the black hole becomes exponentially

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<v Speaker 3>stronger than the pole on the far side of the star.

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<v Speaker 2>Oh well, okay, so if the star is say a

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<v Speaker 2>million miles wide, the front edge of the star is

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<v Speaker 2>a million miles deeper into the black hole's gravity well than.

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<v Speaker 3>The back edge precisely, And that difference in gravitational pull

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<v Speaker 3>across the diameter of the star that is what we

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<v Speaker 3>call the tidal force.

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<v Speaker 2>Like the tides on Earth, but cranked up to.

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<v Speaker 3>A trillion exactly like that, and eventually that tidal force

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<v Speaker 3>exceeds the star's own internal gravity.

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<v Speaker 2>The force that's holding the star together is a burning

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<v Speaker 2>sphere of plasma.

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<v Speaker 3>Yeah, that force is simply overwhelmed by the difference in

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<v Speaker 3>the black holes.

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<v Speaker 2>So the star doesn't just bump into it like a

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<v Speaker 2>car crash, No, not at all. The front is yank

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<v Speaker 2>so much harder than the back that the star simply

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<v Speaker 2>cannot hold itself together. It fails structurally.

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<v Speaker 3>It is literally torn apart. The term astrophysicists sometimes use

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<v Speaker 3>is spaghettification.

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<v Speaker 2>Spaghettification that sounds a bit whimsical for an absolute categorism.

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<v Speaker 3>Well I know it really does, but it's accurate. The

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<v Speaker 3>stars stretched into a long, thin stream of superheated stellar

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<v Speaker 3>material like a noodle, like a noodle of plasma. Yeah,

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<v Speaker 3>but what happens next is what makes this detectable to

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<v Speaker 3>us here on Earth, because.

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<v Speaker 2>It doesn't just quietly fall straight down into the void.

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<v Speaker 3>No, it definitely doesn't. The crumbs of the splintering star,

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<v Speaker 3>this immense volume of gas and plasma, they get caught

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<v Speaker 3>in the black hole's gravitational grip.

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<v Speaker 2>And they start to orbit.

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<v Speaker 3>They do. They begin to swirl around the black hole,

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<v Speaker 3>forming what we call an accretion disc.

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<v Speaker 2>Okay, so it's like water circling a drain, very similar, Yes,

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<v Speaker 2>but the drain is a bottomless pit in space time,

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<v Speaker 2>and the water is superheated plasma moving at what a

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<v Speaker 2>fraction of the speed of light.

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<v Speaker 3>A significant fraction of the speed of light, and that

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<v Speaker 3>speed is the key to everything.

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<v Speaker 2>Why is the speed so important?

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<v Speaker 3>Because the material is orbiting so incredibly fast. The friction

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<v Speaker 3>within the gas is unimaginable friction in space. Yeah. As

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<v Speaker 3>the layers of plasma rub against each other in that

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<v Speaker 3>swirling disc, they undergo intense compression.

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<v Speaker 2>And friction, which generates heat.

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<v Speaker 3>It heats the material to temperatures that defy human comprehension.

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<v Speaker 3>We're talking millions of degrees.

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<v Speaker 2>Millions of degrees. That is insane, it is.

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<v Speaker 3>And this heat creates an incredibly brilliant glow, radiating intense

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<v Speaker 3>ultraviolet light and X rays across the cosmos.

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<v Speaker 2>It's basically screaming its existence out into the universe exactly.

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<v Speaker 3>And furthermore, the immense magnetic fields and the rotational energy

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<v Speaker 3>involved in this whole process can cause the black hole

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<v Speaker 3>to launch a relativistic jet into space.

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<v Speaker 2>A relativistic jet, what is that?

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<v Speaker 3>It's basic a highly concentrated beam of energy and matter

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<v Speaker 3>shooting outward along the poles of the black hole, moving

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<v Speaker 3>at nearly the speed of light.

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<v Speaker 2>So it's like a cosmic lighthouse beam. It's the universe's

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<v Speaker 2>most dramatic dinner bell.

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<v Speaker 3>That's a great way to put it.

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<v Speaker 2>Because black holes themselves emit zero light. I mean, you

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<v Speaker 2>could be looking right at one and see nothing but

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<v Speaker 2>the darkness of space.

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<v Speaker 3>Right. They are functionally invisible.

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<v Speaker 2>But this tde, this destruction of the star, completely lights

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<v Speaker 2>up the dark.

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<v Speaker 3>Assistant Professor igor Andreoni down at UNC Chapel Hill perfectly

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<v Speaker 3>describe these events. He called them cosmic billboards.

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<v Speaker 2>Cosmic billboards, I like that.

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<v Speaker 3>Yeah, because they are quite literally advertising the presence of

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<v Speaker 3>something that would otherwise remain completely stubbornly invisible.

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<v Speaker 2>Which is huge for astronomy.

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<v Speaker 3>It's a scientific gold mine. Catching these events in the

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<v Speaker 3>act illuminates the actual mechanics of how massive black holes feed.

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<v Speaker 2>Okay, but if we are just sitting around waiting for

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<v Speaker 2>a star to accidentally bump into an invisible black hole,

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<v Speaker 2>how often does that actually happen?

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<v Speaker 3>Well, space is famously.

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<v Speaker 2>Very empty, right, so it can't be that often.

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<v Speaker 3>It is extraordinarily rare. On average, a tidal disruption event

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<v Speaker 3>happens only once every one hundred thousand years anywhere in

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<v Speaker 3>a given galaxy.

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<v Speaker 2>Wait, wait, once every one hundred thousand years for a

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<v Speaker 2>whole galaxy.

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<v Speaker 3>That is the average rate.

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<v Speaker 2>Yes, but a galaxy has billions of stars, you're telling

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<v Speaker 2>me at billions of stars circling around, this crash only

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<v Speaker 2>happens once every hundred millennia.

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<v Speaker 3>It is a true testament to exactly what you just said.

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<v Speaker 3>Space is incredibly empty. The distances between stars are vast,

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<v Speaker 3>unimaginably vast, and the distances between a star and a

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<v Speaker 3>central black hole are even vaster. The orbital alignment required

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<v Speaker 3>for a star to perfectly cross that fatal threshold, what

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<v Speaker 3>we call the title radius, is mathematically highly improbable.

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<v Speaker 2>So it can't just be passing through the neighborhood.

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<v Speaker 3>No, It's specific trajectory has to intersect a very precise,

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<v Speaker 3>very narrow zone right around the block.

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<v Speaker 2>To put that one hundred thousand year timeline and perspective

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<v Speaker 2>for you listening, one hundred thousand years ago, anatomically modern

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<v Speaker 2>humans were just starting to seriously migrate out of Africa.

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<v Speaker 3>It's a massive span of time.

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<v Speaker 2>Neanderthals were still the dominant hominins in Europe back then.

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<v Speaker 2>We've gone from stone tools to quantum computers in the

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<v Speaker 2>time it takes for a single galaxy to produce one

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<v Speaker 2>of these flashes.

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<v Speaker 3>Which is exactly why in the past decade of intensive

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<v Speaker 3>modern astronomy, with all our advanced telescopes constantly scanning the skies,

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<v Speaker 3>astronomers have only identified a little over one hundred of

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<v Speaker 3>these TDEs in total.

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<v Speaker 2>One hundred across millions of galaxies.

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<v Speaker 3>Across the millions of galaxies we can actively observe.

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<v Speaker 2>Yes, it makes me think of an analogy. Let's hear it. Okay,

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<v Speaker 2>imagine you are in a massive pitch black warehouse. You

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<v Speaker 2>have absolutely no idea what's in the room, but you

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<v Speaker 2>suspect there's a giant, invisible spinning fan blades somewhere in there. Okay,

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<v Speaker 2>a dangerous room, very and you can't use a flashlight,

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<v Speaker 2>you can't make a sound. The only way you can

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<v Speaker 2>find that fan blade is by taking a glowing, exploding

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<v Speaker 2>paint bomb and tossing it into the dark.

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<v Speaker 3>I see where this is going, right.

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<v Speaker 2>If you toss it and it hits the floor, nothing happens.

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<v Speaker 2>If you toss it and hits a wall, nothing happens.

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<v Speaker 3>Because it's not hitting the target exactly.

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<v Speaker 2>But if you just happen to toss that paint bomb

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<v Speaker 2>perfectly into the spinning blades, boom, it shred The paint

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<v Speaker 2>is violently shredded. It heats up, it splatters everywhere, and suddenly,

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<v Speaker 2>for just a brief few weeks or months, the destruction

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<v Speaker 2>of the paint reveals the exact shape, location, and violence

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<v Speaker 2>of the monster in the dark.

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<v Speaker 3>That is a highly accurate visualization. Actually, the star is

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<v Speaker 3>your paint bomb, right. The destruction of the star is

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<v Speaker 3>the only mechanism that renders the invisible fan blade. The

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<v Speaker 3>black hole temporarily visible.

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<v Speaker 2>But here's the thing, fighting one of these paint BOMs.

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<v Speaker 2>Finding a TDE is not the real paradigm shift here today,

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<v Speaker 2>is it. No, it's not, because we found one hundred

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<v Speaker 2>of them before. The universe breaking mystery. Here is where

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<v Speaker 2>this specific paint bam went off.

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<v Speaker 3>Which brings us to this specific event designated as TDE

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<v Speaker 3>twenty twenty five ABCR.

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<v Speaker 2>Catch you name?

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<v Speaker 3>They always are in astronomy.

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<v Speaker 2>So researchers track this massive flare to a nearby galaxy.

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<v Speaker 2>It doesn't even catch your very poetic catalog name.

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<v Speaker 3>Oh why is a JJ zero one four sixty five

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<v Speaker 3>six point zero four one five two two fourteen point seven?

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<v Speaker 2>Wow? You memorized that. We'll just call it the wiser

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<v Speaker 2>galaxy for sure?

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<v Speaker 3>That idea.

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<v Speaker 2>Usually when we see a TDE, it's dead center in

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<v Speaker 2>the galaxy, right, almost always. But TDE twenty twenty five

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<v Speaker 2>ABCR happened thirty thousand light years.

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<v Speaker 3>Away from the center, which represents the farthest offset ever

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<v Speaker 3>observed for an optically discovered title disruption event.

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<v Speaker 2>Thirty thousand light years. That's a massive distance.

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<v Speaker 3>It is, and it breaks a fundamental rule that astronomers

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<v Speaker 3>have operated under for a very long time.

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<v Speaker 2>Which rule is that well.

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<v Speaker 3>Jonathan Carney, who's a PhD student in physics and astronomy

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<v Speaker 3>at UNC Chapel Hill, pointed this out very clearly. He

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<v Speaker 3>noted that almost every title disruption event we have ever

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<v Speaker 3>observed has occurred at the absolute sence h of a galaxy.

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<v Speaker 2>Because that is where the giant black holes live.

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<v Speaker 3>Exactly. The galactic nucleus is where the supermassive black holes reside.

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<v Speaker 3>It's where the gravitational well of the galaxy is the deepest.

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<v Speaker 2>It's like the drain at the bottom of a massive sink, right.

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<v Speaker 3>It's where the most matter has accumulated over billions of years.

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<v Speaker 3>That is where we expect the biggest monsters to be.

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<v Speaker 2>So to find a tidal disruption event tens of thousands

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<v Speaker 2>of light years away from the center.

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<v Speaker 3>It implies there is a massive black hole lurking in

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<v Speaker 3>a place we would normally never ever expect to find one.

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<v Speaker 2>I have to stop you here, though, because the scale

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<v Speaker 2>and the physics are kind of messing with my head.

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<v Speaker 2>How So, the black hole responsible for this event is

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<v Speaker 2>estimated to be roughly one million times the mass of

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<v Speaker 2>our sun one million solar.

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<v Speaker 3>Masses that is the current estimate.

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<v Speaker 2>Yes, how on Earth do you hide something with a

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<v Speaker 2>million solar masses in the quiet suburbs of a galaxy?

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<v Speaker 3>I mean, I feel like it's gravity would just be

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<v Speaker 3>completely tearing the neighborhood apart.

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<v Speaker 2>It's a fair assumption to make be like.

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<v Speaker 3>A cosmic vacuum cleaner when we notice all the stars

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<v Speaker 3>around it swirling down a drain before a TD even happens.

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<v Speaker 3>It is a very common misconception about black holes, this

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<v Speaker 3>idea that they are cosmic vacuum cleaners.

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<v Speaker 2>Because pop culture always shows them sucking everything in.

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<v Speaker 3>Right, we assume something that massive must be inherently disruptive,

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<v Speaker 3>just constantly pulling in everything around it. But you really

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<v Speaker 3>have to remember two things here.

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<v Speaker 2>Okay, what are they?

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<v Speaker 3>First the sheer scale of the space we are talking about,

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<v Speaker 3>and second, the inverse square law of gravity.

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<v Speaker 2>Okay, let's break down the inverse square law. Yeah, that

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<v Speaker 2>sounds like the actual key to this whole hiding trick.

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<v Speaker 3>It absolutely is. Gravity is entirely dependent on distance. The

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<v Speaker 3>inverse square law basically states that if you double the

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<v Speaker 3>distance between two objects, the gravitational force doesn't just drop

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<v Speaker 3>by half.

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<v Speaker 2>It doesn't.

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<v Speaker 3>No, it drops by a factor of four. It weakens

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<v Speaker 3>exponentially the further away you get. Oh wow, if you

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<v Speaker 3>triple the distance, the force is nine times weaker.

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<v Speaker 2>So gravity basically falls off a cliff once you take

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<v Speaker 2>a few steps away from the source.

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<v Speaker 3>Precisely, let me give you a local example. If you

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<v Speaker 3>were to replace our own Sun right now with a

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<v Speaker 3>black hole of the exact same mass, one solar mass,

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<v Speaker 3>Earth would not get sucked in.

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<v Speaker 2>Wait, really, we wouldn't just spiral to our doom, not

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<v Speaker 2>at all.

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<v Speaker 3>The Earth would continue orbiting in the exact same path

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<v Speaker 3>in exactly three hundred and sixty five.

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<v Speaker 2>Days because the mass hasn't changed.

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<v Speaker 3>Because the mass hasn't changed, and our distance hasn't changed.

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<v Speaker 2>The only difference is that we'd all freeze and it

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<v Speaker 2>would get very very dark.

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<v Speaker 3>It would be a bad day for life on Earth. Yes,

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<v Speaker 3>but gravitationally, nothing changes.

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<v Speaker 2>So let's apply that to this wandering monster in the

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<v Speaker 2>wiser galaxy. It has the mass of a million suns.

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<v Speaker 3>Right, and a million solar masses is immense compared to

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<v Speaker 3>our Sun, obviously, but on a galactic scale, it's just

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<v Speaker 3>a drop in the ocean.

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<v Speaker 2>Really, a million suns is a drop the.

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<v Speaker 3>Entire galaxy weighs billions or even trillions of solar masses

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<v Speaker 3>thirty thousand light years from the center. Puts this black

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<v Speaker 3>hole out in the outer galactic disc, or maybe even

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<v Speaker 3>the halo.

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<v Speaker 2>Which is the sparsely populated part of town.

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<v Speaker 3>Exactly. These are regions where the density of stars is

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<v Speaker 3>significantly lower than in the packed galactic core.

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<v Speaker 2>So it's not packed like sardines out there. The stars

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<v Speaker 2>have a lot of elbow room, lots of rooms.

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<v Speaker 3>So because of that inverse square law we just talked about,

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<v Speaker 3>unless a star crosses that very specific, very narrow threshold

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<v Speaker 3>right next to the black hole's event horizon, it will

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<v Speaker 3>simply orbit the black hole.

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<v Speaker 2>Safely or just pass right by it.

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<v Speaker 3>Yes, completely unaffected in any catastrophic way.

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<v Speaker 2>So it really isn't a vacuum cleaner at all. It's

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<v Speaker 2>more like, Okay, it's like a really really deep pothole

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<v Speaker 2>on a very wide, empty, dark highway. I like that, Like,

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<v Speaker 2>if you don't drive your tire directly over it, you're

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<v Speaker 2>totally fine. You don't even know it's there.

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<v Speaker 3>That is a perfect way to look at it, and

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<v Speaker 3>scientists have actually theorized for a while that these wandering

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<v Speaker 3>black holes likely exist in massive galaxies.

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<v Speaker 2>They suspected they were out there.

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<v Speaker 3>Oh, definitely the mathematics when the really complex computer simulations

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<v Speaker 3>of galactic evolution strongly suggest they should be out there

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<v Speaker 3>wandering around.

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<v Speaker 2>But knowing they exist in a computer model and actually

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<v Speaker 2>finding one in the dark are two very different.

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<v Speaker 3>Things, extremely different. As Jonathan Carney highlighted, they are notoriously

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<v Speaker 3>difficult to study because unless they are actively feeding, unless

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<v Speaker 3>they briefly disrupt a star like this one, did, they

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<v Speaker 3>produce absolutely no light.

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<v Speaker 2>They're perfectly camouflaged against the darkness of empty.

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<v Speaker 3>Space, literally invisible.

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<v Speaker 2>Okay, So if a one million solar mass black hole

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<v Speaker 2>does not naturally belong in the galactic suburbs, if it's

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<v Speaker 2>supposed to be downtown in the galactic core where it

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<v Speaker 2>was born, how in the universe did he get thirty

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<v Speaker 2>thousand light years away?

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<v Speaker 3>That is the big question.

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<v Speaker 2>I mean, what could possibly have the leverage to move

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<v Speaker 2>an object that weighs a million times more than our sun.

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<v Speaker 3>Well. Astrophysics offers two leading theoretical scenarios for how a

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<v Speaker 3>supermassive black hole becomes a wanderer, A rogue drifting far

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00:15:59.039 --> 00:16:02.200
<v Speaker 3>from home to hear them. Both scenarios are rooted in

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<v Speaker 3>immense violence and cosmic scale upheaval. The first theory proposes

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<v Speaker 3>that this black hole is essentially a remnant left behind

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<v Speaker 3>after a massive galactic merger in the distant past.

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<v Speaker 2>Let's talk about a galactic merger for a second. We're

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<v Speaker 2>talking about two entirely separate galaxies colliding.

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<v Speaker 3>With each other, right, Yes, a cosmic collision. Picture a

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<v Speaker 3>massive galaxy in a smaller satellite galaxy nearby. Over billions

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<v Speaker 3>of years, their mutual gravitational attractions slowly dries them.

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<v Speaker 2>Together billions of years. Yeah, so this is not a

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<v Speaker 2>fast crash.

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00:16:34.360 --> 00:16:39.480
<v Speaker 3>No, it is an incredibly slow, majestic, and entirely destructive process.

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<v Speaker 3>As the two galaxies merge, their outer halos touch first,

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<v Speaker 3>what happens?

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<v Speaker 2>Then?

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<v Speaker 3>Gas clouds collide, which compresses the gas and ignites massive

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<v Speaker 3>bursts of new star formation. It would look like fireworks

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<v Speaker 3>on a cosmic scale.

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00:16:52.960 --> 00:16:55.440
<v Speaker 2>But do the actual stars crash into each other?

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<v Speaker 3>Surprisingly? No, The stars themselves rarely collide because of the

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<v Speaker 3>vast distance between them, but their orbits are thrown into

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<v Speaker 3>complete and utter chaos.

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<v Speaker 2>Okay, but what happens to the black holes because both

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<v Speaker 2>of these galaxies started with their own supermassive black hole

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<v Speaker 2>in their respective centers, right.

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<v Speaker 3>Most galaxies do.

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<v Speaker 2>Yes.

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00:17:12.839 --> 00:17:16.119
<v Speaker 3>Now, in a perfect symmetrical merger, the two central black

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<v Speaker 3>holes would undergo a process called dynamical friction. Dynamical friction,

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<v Speaker 3>they would interact with the gas and stars around them,

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<v Speaker 3>slowly losing orbital energy, and they'd gradually sync to the

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<v Speaker 3>center of the newly combined larger galaxy.

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<v Speaker 2>So they sort of spiral down the new drain together exactly.

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<v Speaker 3>Eventually they would orbit each other in a binary pair,

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<v Speaker 3>and over millions of years, merge into one even larger

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<v Speaker 3>supermassive black hole.

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00:17:40.680 --> 00:17:44.319
<v Speaker 2>That sounds very neat and orderly, but I'm guessing space

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00:17:44.359 --> 00:17:45.400
<v Speaker 2>isn't always that tidy.

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00:17:45.519 --> 00:17:49.839
<v Speaker 3>Far from it. Mergers are very messy asymmetrical events. Sometimes

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<v Speaker 3>the smaller galaxy is essentially stripped apart before it even

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<v Speaker 3>reaches the center.

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00:17:53.680 --> 00:17:54.279
<v Speaker 2>Stripped apart.

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00:17:54.319 --> 00:17:57.839
<v Speaker 3>How its outer layers of stars and gas are literally

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<v Speaker 3>peeled away by the tidal forces of the larger.

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00:18:00.640 --> 00:18:02.960
<v Speaker 2>Galaxy, So it's just dismantled, right.

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<v Speaker 3>And by the time the smaller galaxy is fully swallowed,

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00:18:06.079 --> 00:18:09.440
<v Speaker 3>its central black hole is left completely stranded because.

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00:18:09.240 --> 00:18:11.079
<v Speaker 2>All the stuff around it that was helping it sinc

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00:18:11.240 --> 00:18:11.640
<v Speaker 2>is gone.

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00:18:11.880 --> 00:18:15.359
<v Speaker 3>Yes, it loses its surrounding mass and never manages to

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00:18:15.440 --> 00:18:18.519
<v Speaker 3>sync to the new galactic core through that dynamical friction.

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00:18:19.160 --> 00:18:22.119
<v Speaker 3>It simply gets marooned out in the newly expanded outer

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00:18:22.200 --> 00:18:23.640
<v Speaker 3>halo of the merged.

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00:18:23.359 --> 00:18:27.440
<v Speaker 2>Galaxy, just orbiting aimlessly, just wandering. So it's basically the

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00:18:27.559 --> 00:18:31.759
<v Speaker 2>orphan heart of a dead, consumed galaxy, just floating through

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00:18:31.759 --> 00:18:35.039
<v Speaker 2>the outer ruins of its former home. That is incredibly

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00:18:35.079 --> 00:18:36.240
<v Speaker 2>poetic and kind of sad.

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00:18:36.480 --> 00:18:39.759
<v Speaker 3>It is a profound cosmic artifact of a billion year

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00:18:39.799 --> 00:18:40.759
<v Speaker 3>old collision.

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00:18:40.799 --> 00:18:43.279
<v Speaker 2>Okay, what's the second theory? Because you said there.

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00:18:43.160 --> 00:18:45.799
<v Speaker 3>Were two, there's a second, perhaps even more violent theory,

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00:18:46.160 --> 00:18:50.079
<v Speaker 3>the ejection scenario objection. This theory suggests that the black

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00:18:50.119 --> 00:18:53.200
<v Speaker 3>hole wasn't passively left behind by a merger, but was

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00:18:53.319 --> 00:18:57.440
<v Speaker 3>actively violently thrown outward from the center of its own galaxy.

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00:18:57.519 --> 00:19:02.359
<v Speaker 2>Wait, thrown, yes, you throw a million suns. What could

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00:19:02.400 --> 00:19:06.519
<v Speaker 2>possibly generate enough force to eject a super massive black hole?

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00:19:07.039 --> 00:19:13.119
<v Speaker 3>Gravity itself, specifically, the chaotic gravitational interactions between multiple massive

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00:19:13.160 --> 00:19:15.039
<v Speaker 3>black holes near a galaxy.

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00:19:14.599 --> 00:19:17.200
<v Speaker 2>Center, multiple like more than two exactly.

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00:19:17.240 --> 00:19:20.119
<v Speaker 3>This often happens in the chaotic aftermath of not just one,

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00:19:20.160 --> 00:19:24.839
<v Speaker 3>but multiple successive galactic mergers. Imagine a scenario where three

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00:19:24.880 --> 00:19:27.200
<v Speaker 3>massive black holes end up drawn toward the center of

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00:19:27.240 --> 00:19:30.000
<v Speaker 3>a newly forming galaxy before they have a chance to merge.

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00:19:30.240 --> 00:19:32.319
<v Speaker 2>Okay, I could see where this is going. It's like

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00:19:32.319 --> 00:19:35.599
<v Speaker 2>a cosmic game of billiards, but the billiard balls weigh

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00:19:35.680 --> 00:19:37.160
<v Speaker 2>millions of solar masses.

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00:19:37.319 --> 00:19:39.400
<v Speaker 3>And this brings us to one of the most famously

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00:19:39.640 --> 00:19:43.440
<v Speaker 3>unsolvable concepts in astrophysics, the three body problem.

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00:19:43.559 --> 00:19:45.759
<v Speaker 2>Oh, I've heard of this. It's notorious.

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00:19:45.839 --> 00:19:50.000
<v Speaker 3>It is in classical mechanics. If you have two massive

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00:19:50.039 --> 00:19:52.880
<v Speaker 3>bodies orbiting each other, like the Earth and the Sun,

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00:19:53.000 --> 00:19:57.200
<v Speaker 3>or two black holes, their orbits are stable, predictable, and

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00:19:57.319 --> 00:19:58.599
<v Speaker 3>mathematically elegant.

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00:19:58.720 --> 00:20:01.279
<v Speaker 2>Right, it's a balanced equation. We can calculate where the

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00:20:01.319 --> 00:20:03.720
<v Speaker 2>Earth will be next year with perfect accuracy.

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00:20:03.799 --> 00:20:06.880
<v Speaker 3>We can calculate their positions billions of years into the future.

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00:20:07.039 --> 00:20:09.920
<v Speaker 3>But the moment you introduce a third massive body into

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00:20:09.920 --> 00:20:13.400
<v Speaker 3>that gravitational system, the mathematics completely breaks down.

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00:20:13.559 --> 00:20:14.519
<v Speaker 2>It just stops working.

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00:20:14.640 --> 00:20:17.599
<v Speaker 3>The system becomes inherently chaotic and unstable. There is no

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00:20:17.759 --> 00:20:21.559
<v Speaker 3>simple mathematical solution. The three black holes whip around each

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00:20:21.599 --> 00:20:26.039
<v Speaker 3>other faster and faster, exchanging orbital energy in totally unpredictable ways,

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00:20:26.119 --> 00:20:26.799
<v Speaker 3>because every.

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00:20:26.599 --> 00:20:28.960
<v Speaker 2>Time body A gets close to body B body C

435
00:20:29.160 --> 00:20:31.799
<v Speaker 2>is pulling on them from a different angle, constantly changing

436
00:20:31.839 --> 00:20:32.680
<v Speaker 2>the trajectories.

437
00:20:32.880 --> 00:20:36.359
<v Speaker 3>Precisely, they are constantly stealing kinetic energy from one another.

438
00:20:36.720 --> 00:20:40.359
<v Speaker 3>And in these unstable three body interactions, the inevitable outcome

439
00:20:40.440 --> 00:20:41.920
<v Speaker 3>is almost always an injection.

440
00:20:42.279 --> 00:20:43.559
<v Speaker 2>Something gets kicked out of the club.

441
00:20:43.720 --> 00:20:47.319
<v Speaker 3>Always. The laws of conservation of energy and angular momentum

442
00:20:47.359 --> 00:20:51.160
<v Speaker 3>basically demand a resolution to the chaos. The lightest of

443
00:20:51.200 --> 00:20:53.640
<v Speaker 3>the three objects, or the one that simply hits the

444
00:20:53.640 --> 00:20:56.000
<v Speaker 3>wrong angle at the wrong time in this complex dance,

445
00:20:56.400 --> 00:20:59.920
<v Speaker 3>receives a massive sudden kick of kinetic energy.

446
00:21:00.039 --> 00:21:01.960
<v Speaker 2>It's violently kicked off the billiard tabe.

447
00:21:02.079 --> 00:21:05.640
<v Speaker 3>It is quite literally slang shotted outward. And this kick

448
00:21:05.720 --> 00:21:09.640
<v Speaker 3>is so powerful it overcomes the immense escape velocity of

449
00:21:09.680 --> 00:21:11.359
<v Speaker 3>the entire galactic center.

450
00:21:11.599 --> 00:21:13.960
<v Speaker 2>That is mind boggling, Propelled.

451
00:21:13.480 --> 00:21:16.279
<v Speaker 3>By the very gravitational forces that drew it inward in

452
00:21:16.319 --> 00:21:19.559
<v Speaker 3>the first place, it is flung out into the galactic halo,

453
00:21:19.839 --> 00:21:22.079
<v Speaker 3>destined to wander the suburbs forever.

454
00:21:22.359 --> 00:21:24.680
<v Speaker 2>I really want you listening to this right now to

455
00:21:24.799 --> 00:21:28.640
<v Speaker 2>just pause and sit with the sheer scale of time

456
00:21:28.720 --> 00:21:29.319
<v Speaker 2>involved here.

457
00:21:29.400 --> 00:21:30.720
<v Speaker 3>It's hard to wrap your head around.

458
00:21:31.000 --> 00:21:34.079
<v Speaker 2>It really is, because whether this black hole was stranded

459
00:21:34.079 --> 00:21:36.640
<v Speaker 2>by a slow motion merger or kicked out in a

460
00:21:36.720 --> 00:21:40.839
<v Speaker 2>chaotic gravitational slang shot, these are events that happened millions,

461
00:21:40.880 --> 00:21:44.359
<v Speaker 2>possibly billions of years ago, deep Pine right, Which means

462
00:21:44.400 --> 00:21:47.680
<v Speaker 2>this giant, this entity, with the mass of a million suns,

463
00:21:47.960 --> 00:21:53.039
<v Speaker 2>has just been silently, stealthily drifting through the dark for eons.

464
00:21:52.799 --> 00:21:55.960
<v Speaker 3>For longer than the Earth has had complex life.

465
00:21:55.799 --> 00:22:00.359
<v Speaker 2>Totally undetectable, emitting no light, just waiting for me millions

466
00:22:00.400 --> 00:22:04.359
<v Speaker 2>of years. It waited until one single unlucky star finally

467
00:22:04.440 --> 00:22:06.799
<v Speaker 2>crossed its path and brushed the edge of that pothole.

468
00:22:06.960 --> 00:22:11.119
<v Speaker 3>It highlights the vast quiet patients of the universe, time

469
00:22:11.200 --> 00:22:13.839
<v Speaker 3>scales that basically render human history irrelevant.

470
00:22:14.160 --> 00:22:15.920
<v Speaker 2>But you know, a black hole waiting in the dark

471
00:22:16.000 --> 00:22:17.279
<v Speaker 2>is only half the equation.

472
00:22:17.000 --> 00:22:18.680
<v Speaker 3>Here, right. We still had to find it.

473
00:22:18.640 --> 00:22:21.400
<v Speaker 2>Because for a billion years it was invisible, and frankly,

474
00:22:21.400 --> 00:22:23.039
<v Speaker 2>if we had been looking, we wouldn't have seen it.

475
00:22:23.160 --> 00:22:25.319
<v Speaker 2>Even when the star exploded, we almost missed it.

476
00:22:25.359 --> 00:22:27.119
<v Speaker 3>We came very close to missing it.

477
00:22:27.640 --> 00:22:31.160
<v Speaker 2>Finding this thing required us to actually overcome our own

478
00:22:31.519 --> 00:22:35.759
<v Speaker 2>deeply ingrained blind spots. We had to fundamentally change how

479
00:22:35.799 --> 00:22:38.759
<v Speaker 2>we look at the night sky. And that brings us

480
00:22:38.759 --> 00:22:41.160
<v Speaker 2>to the methodology and kind of the unsung hero of

481
00:22:41.200 --> 00:22:42.079
<v Speaker 2>this entire.

482
00:22:42.200 --> 00:22:46.119
<v Speaker 3>Discovery, the actual mechanism by which we found a single

483
00:22:46.200 --> 00:22:49.440
<v Speaker 3>flash of light thirty thousand light years away from where

484
00:22:49.440 --> 00:22:50.279
<v Speaker 3>it was supposed to be.

485
00:22:50.279 --> 00:22:51.880
<v Speaker 2>Because we didn't just stumble on this by having a

486
00:22:51.880 --> 00:22:54.240
<v Speaker 2>guy look through an eyepiece at the exact right second.

487
00:22:54.480 --> 00:22:55.720
<v Speaker 3>Those days are long gone.

488
00:22:55.920 --> 00:23:00.279
<v Speaker 2>We found this using artificial intelligence, specifically an AI classification

489
00:23:00.440 --> 00:23:04.200
<v Speaker 2>tool called disocters. Yes, and this tool was originally developed

490
00:23:04.200 --> 00:23:07.400
<v Speaker 2>by Robert Stein at the University of Maryland and NASA Goddard, and.

491
00:23:07.359 --> 00:23:11.799
<v Speaker 3>Its application here is a total masterclass in modern astronomical

492
00:23:11.839 --> 00:23:15.240
<v Speaker 3>technique because it addresses a fundamental crisis in the field

493
00:23:15.319 --> 00:23:15.720
<v Speaker 3>right now.

494
00:23:16.079 --> 00:23:17.440
<v Speaker 2>A crisis, yes.

495
00:23:18.039 --> 00:23:21.559
<v Speaker 3>But to understand why the AI is so necessary, we

496
00:23:21.640 --> 00:23:23.759
<v Speaker 3>have to look at how akash anamar Laputti, who is

497
00:23:23.799 --> 00:23:27.440
<v Speaker 3>a postdoctoral researcher in physics and astronomy at UNC Chapel Hill,

498
00:23:27.880 --> 00:23:29.240
<v Speaker 3>how he actually utilized it.

499
00:23:29.279 --> 00:23:30.680
<v Speaker 2>Okay, what did he do differently.

500
00:23:30.759 --> 00:23:35.359
<v Speaker 3>He adapted this desk to score AI to scan enormous

501
00:23:35.400 --> 00:23:39.000
<v Speaker 3>amounts of telescope data. But here is the critical innovation.

502
00:23:39.119 --> 00:23:43.160
<v Speaker 3>He adapted it specifically to search for TDE candidates away

503
00:23:43.200 --> 00:23:44.359
<v Speaker 3>from galaxy centers.

504
00:23:44.400 --> 00:23:46.640
<v Speaker 2>Okay, stop, because this is the part that completely blew

505
00:23:46.720 --> 00:23:48.119
<v Speaker 2>my mind when I first learned about this.

506
00:23:48.200 --> 00:23:49.039
<v Speaker 3>It's a great twist.

507
00:23:49.160 --> 00:23:52.640
<v Speaker 2>Are you telling me that because human scientists assume that

508
00:23:52.839 --> 00:23:55.759
<v Speaker 2>massive black holes only lived in the center of galaxies,

509
00:23:56.279 --> 00:24:01.000
<v Speaker 2>we literally programmed our own blind spots into our telescopes. Yes,

510
00:24:01.799 --> 00:24:04.720
<v Speaker 2>like we were deliberately ignoring the outer edges because we

511
00:24:04.759 --> 00:24:06.200
<v Speaker 2>thought we already knew nothing was there.

512
00:24:06.279 --> 00:24:08.759
<v Speaker 3>That is essentially correct, and it is a fascinating look

513
00:24:08.759 --> 00:24:12.279
<v Speaker 3>at the intersection of human bias and computational limits.

514
00:24:12.400 --> 00:24:13.440
<v Speaker 2>How does that even happen?

515
00:24:13.640 --> 00:24:16.279
<v Speaker 3>Well, in astronomy, you are dealing with an infinite sky

516
00:24:16.599 --> 00:24:20.599
<v Speaker 3>and very limited computational resources. You have to prioritize where

517
00:24:20.640 --> 00:24:22.319
<v Speaker 3>you look and how you filter the data.

518
00:24:22.480 --> 00:24:23.880
<v Speaker 2>You can't look at everything all the time.

519
00:24:24.119 --> 00:24:27.599
<v Speaker 3>Exactly. For nearly a century, the established theory, which was

520
00:24:27.599 --> 00:24:30.799
<v Speaker 3>backed by almost every observation we had ever made. Mind you,

521
00:24:30.880 --> 00:24:35.559
<v Speaker 3>dictated that supermassive black holes exist exclusively in galactic nuclei, so.

522
00:24:35.559 --> 00:24:38.440
<v Speaker 2>It wasn't a crazy assumption. It was based on past

523
00:24:38.519 --> 00:24:39.240
<v Speaker 2>data right.

524
00:24:39.799 --> 00:24:43.519
<v Speaker 3>Therefore, when astronomers wrote the initial algorithms to sift through

525
00:24:43.559 --> 00:24:48.440
<v Speaker 3>telescope data to find TDEs, they heavily weighted the galactic center.

526
00:24:48.920 --> 00:24:51.599
<v Speaker 2>So they literally wrote code that said, if a flash

527
00:24:51.599 --> 00:24:54.519
<v Speaker 2>of light happens far away from the center, ignore it.

528
00:24:54.519 --> 00:24:55.400
<v Speaker 2>It's not a TDE.

529
00:24:55.680 --> 00:24:59.319
<v Speaker 3>Functionally, yes, if a flash occurred in the outer suburbs

530
00:24:59.359 --> 00:25:03.079
<v Speaker 3>of a galaxy, the algorithms were trained to classify it

531
00:25:03.160 --> 00:25:06.599
<v Speaker 3>as a supernova or maybe a variable star, or perhaps

532
00:25:06.640 --> 00:25:08.400
<v Speaker 3>just an observational error.

533
00:25:08.200 --> 00:25:09.759
<v Speaker 2>Because supernova's happened everywhere.

534
00:25:09.799 --> 00:25:12.759
<v Speaker 3>Supernova have it all over galaxies? Yes, but a TDE

535
00:25:12.839 --> 00:25:15.359
<v Speaker 3>in the suburbs. It didn't fit the established model, so

536
00:25:15.400 --> 00:25:18.920
<v Speaker 3>the system filtered it out as noise or mithcategorized it.

537
00:25:19.400 --> 00:25:22.039
<v Speaker 3>We trained the machines to ignore the anomalies.

538
00:25:22.160 --> 00:25:23.960
<v Speaker 2>We let our assumptions dictate our reality.

539
00:25:24.039 --> 00:25:24.400
<v Speaker 3>We did.

540
00:25:24.599 --> 00:25:27.839
<v Speaker 2>We told the computers don't look over there, there's nothing interesting.

541
00:25:28.480 --> 00:25:31.920
<v Speaker 2>So we only found this wandering giant because we finally

542
00:25:31.960 --> 00:25:34.279
<v Speaker 2>told the AI to remove our human assumptions.

543
00:25:34.559 --> 00:25:40.279
<v Speaker 3>Precisely, akash Anumar Laputi stated it perfectly. By explicitly removing

544
00:25:40.279 --> 00:25:43.440
<v Speaker 3>the constraint that these events only happened in the galactic center,

545
00:25:44.119 --> 00:25:46.200
<v Speaker 3>the team was able to find a black hole that

546
00:25:46.200 --> 00:25:49.440
<v Speaker 3>would have otherwise been completely missed by standard search parameter.

547
00:25:49.640 --> 00:25:51.400
<v Speaker 2>Just looked at the raw data exactly.

548
00:25:51.880 --> 00:25:55.480
<v Speaker 3>The AI, once unchained from that geographical bias, just looked

549
00:25:55.480 --> 00:25:58.480
<v Speaker 3>at the physics. It analyzed the characteristics of the flash

550
00:25:58.519 --> 00:26:01.160
<v Speaker 3>and flagged it regardless of the zip code it occurred in.

551
00:26:01.440 --> 00:26:04.079
<v Speaker 2>Wait, how does an AI know the difference between a

552
00:26:04.119 --> 00:26:07.519
<v Speaker 2>star exploding as a supernova in the suburbs and a

553
00:26:07.559 --> 00:26:10.240
<v Speaker 2>star being shredded by a black hole in the suburbs.

554
00:26:10.319 --> 00:26:12.440
<v Speaker 3>That's the real magic of it, because they're both.

555
00:26:12.400 --> 00:26:14.799
<v Speaker 2>Just bright flashes of light in a telescope. Right, Hey,

556
00:26:15.119 --> 00:26:16.599
<v Speaker 2>to me, a flash is a flash.

557
00:26:16.759 --> 00:26:19.640
<v Speaker 3>That is where the power of modern machine learning really

558
00:26:19.680 --> 00:26:22.000
<v Speaker 3>comes in. AI doesn't just see a flash of light.

559
00:26:22.359 --> 00:26:25.200
<v Speaker 3>It analyzes the light curve and the spectral signature.

560
00:26:25.240 --> 00:26:26.200
<v Speaker 2>Okay, a white curve.

561
00:26:26.319 --> 00:26:26.400
<v Speaker 3>Ye.

562
00:26:26.519 --> 00:26:28.759
<v Speaker 2>That means how the brightness changes over time?

563
00:26:28.839 --> 00:26:31.400
<v Speaker 3>Yeah, exactly. When a star explodes as a supernova, it

564
00:26:31.440 --> 00:26:34.759
<v Speaker 3>expands outward, it gets very bright, very quickly, and then

565
00:26:34.759 --> 00:26:38.720
<v Speaker 3>it cools off in a very specific predictable mathematical curve.

566
00:26:38.960 --> 00:26:40.839
<v Speaker 2>Okay, so it has a known fingerprint. Yes.

567
00:26:41.039 --> 00:26:44.240
<v Speaker 3>Furthermore, the light from a supernova contains the chemical signatures

568
00:26:44.319 --> 00:26:50.200
<v Speaker 3>of heavy elements synthesized in the explosion, things like iron, nickel, silicon.

569
00:26:50.519 --> 00:26:52.799
<v Speaker 2>So what does a TD look like to an AI? Then?

570
00:26:53.039 --> 00:26:53.920
<v Speaker 2>How is it different?

571
00:26:54.279 --> 00:26:57.599
<v Speaker 3>A TD looks fundamentally different. Remember the accretion disc we

572
00:26:57.720 --> 00:26:59.119
<v Speaker 3>talked about earlier.

573
00:26:58.799 --> 00:27:00.680
<v Speaker 2>The swirling superheat plasma.

574
00:27:00.839 --> 00:27:04.880
<v Speaker 3>Yes, that disc stays incredibly hot for a much longer

575
00:27:04.880 --> 00:27:08.839
<v Speaker 3>time than a supernova. It emits massive amounts of ultraviolet

576
00:27:08.920 --> 00:27:12.240
<v Speaker 3>light and X rays, far more than a typical exploding star.

577
00:27:12.480 --> 00:27:14.960
<v Speaker 2>So it's hotter and stays hot longer.

578
00:27:14.640 --> 00:27:18.680
<v Speaker 3>And spectrally, it often shows broad smeared emission lines of

579
00:27:18.759 --> 00:27:21.960
<v Speaker 3>hydrogen and helium, which is literally the shredded atmosphere of

580
00:27:21.960 --> 00:27:25.720
<v Speaker 3>the dead star moving at relativistic speeds around the black hole.

581
00:27:25.839 --> 00:27:28.519
<v Speaker 2>Okay, So the AI is looking at millions of flashes,

582
00:27:28.880 --> 00:27:33.079
<v Speaker 2>and it's analyzing the temperature, the cooling rate, the ultraviolet spikes,

583
00:27:33.119 --> 00:27:36.240
<v Speaker 2>and the chemical fingerprints all in fractions of a second.

584
00:27:36.359 --> 00:27:39.440
<v Speaker 3>Yes, it's doing all of that simultaneously. But this also

585
00:27:39.440 --> 00:27:41.119
<v Speaker 3>brings up why we need AI to do this in

586
00:27:41.119 --> 00:27:43.400
<v Speaker 3>the first place, rather than just having astronomers look at

587
00:27:43.440 --> 00:27:44.200
<v Speaker 3>the light curves.

588
00:27:44.000 --> 00:27:47.039
<v Speaker 2>Themselves, why couldn't a team of grad students just look

589
00:27:47.079 --> 00:27:47.759
<v Speaker 2>at the graphs?

590
00:27:48.119 --> 00:27:50.960
<v Speaker 3>Because it touches on the fundamental reality of modern science.

591
00:27:51.440 --> 00:27:55.319
<v Speaker 3>We are deeply entrenched in the big data era of astronomy.

592
00:27:55.559 --> 00:27:58.200
<v Speaker 2>Big data is almost an understatement here, isn't it?

593
00:27:58.200 --> 00:28:02.400
<v Speaker 3>It is a massive understatement. Modern survey telescopes don't operate

594
00:28:02.519 --> 00:28:05.160
<v Speaker 3>like the telescopes of the past, where you pointed at

595
00:28:05.200 --> 00:28:08.640
<v Speaker 3>one specific galaxy, took a long exposure and developed a

596
00:28:08.680 --> 00:28:09.640
<v Speaker 3>glass plate.

597
00:28:09.599 --> 00:28:11.519
<v Speaker 2>Like the old man Palomar photos right.

598
00:28:11.839 --> 00:28:16.160
<v Speaker 3>Today's survey telescopes continuously image vast swaths of the sky

599
00:28:16.720 --> 00:28:21.240
<v Speaker 3>night after night after night. They generate terabytes, sometimes petabytes

600
00:28:21.440 --> 00:28:25.440
<v Speaker 3>of raw data petabytes. They capture millions of transient events,

601
00:28:25.440 --> 00:28:27.880
<v Speaker 3>things that flash, dim or move every single night.

602
00:28:28.079 --> 00:28:30.039
<v Speaker 2>It's like trying to drink from a fire hose that

603
00:28:30.119 --> 00:28:31.960
<v Speaker 2>is spraying the entire universe at you.

604
00:28:32.160 --> 00:28:35.000
<v Speaker 3>The volume of information has far surpassed the capacity of

605
00:28:35.079 --> 00:28:38.720
<v Speaker 3>human eyes. Even if you had teams of thousands of

606
00:28:38.799 --> 00:28:40.880
<v Speaker 3>humans to process it, it wouldn't be enough.

607
00:28:41.119 --> 00:28:42.599
<v Speaker 2>They just fall behind instantly.

608
00:28:42.920 --> 00:28:45.400
<v Speaker 3>If a human tried to look at every single flash

609
00:28:45.480 --> 00:28:48.039
<v Speaker 3>recorded by a modern telescope to determine if it was

610
00:28:48.480 --> 00:28:53.519
<v Speaker 3>a TD, a supernova, a variable star, an asteroid, or

611
00:28:53.599 --> 00:28:56.400
<v Speaker 3>just a reflection off a satellite. They would never finish

612
00:28:56.440 --> 00:28:57.640
<v Speaker 3>a single night's data.

613
00:28:58.039 --> 00:29:01.440
<v Speaker 2>So the AI isn't just a convene need helper anymore.

614
00:29:01.200 --> 00:29:04.559
<v Speaker 3>Not at all. It is the fundamental, necessary lens through

615
00:29:04.599 --> 00:29:06.880
<v Speaker 3>which we must filter the noise of the universe.

616
00:29:07.240 --> 00:29:10.480
<v Speaker 2>The AI is doing the sifting. It's panning for gold

617
00:29:10.720 --> 00:29:13.640
<v Speaker 2>in a river of raw data, looking for a flake

618
00:29:13.680 --> 00:29:15.720
<v Speaker 2>of gold that we used to literally throw away because

619
00:29:15.720 --> 00:29:17.720
<v Speaker 2>we didn't think gold belonged in that part of the river.

620
00:29:17.880 --> 00:29:22.200
<v Speaker 3>It finds the impossible by tirelessly applying complex pattern recognition

621
00:29:22.240 --> 00:29:25.960
<v Speaker 3>to data sets far too large for human comprehension. AI

622
00:29:26.039 --> 00:29:29.279
<v Speaker 3>tools like discore are becoming the primary engines of discovery

623
00:29:29.519 --> 00:29:32.400
<v Speaker 3>in chasing down these incredibly rare astronomical events.

624
00:29:32.400 --> 00:29:33.000
<v Speaker 2>It's amazing.

625
00:29:33.079 --> 00:29:37.119
<v Speaker 3>They remove the human computational bottleneck and critically they remove

626
00:29:37.160 --> 00:29:37.880
<v Speaker 3>the human bias.

627
00:29:37.960 --> 00:29:40.640
<v Speaker 2>So the AI looks at millions of data points, it

628
00:29:40.720 --> 00:29:44.480
<v Speaker 2>sees this specific super hot UV heavy light signature thirty

629
00:29:44.519 --> 00:29:47.640
<v Speaker 2>thousand light years off center in the Wiser galaxy, and

630
00:29:47.720 --> 00:29:50.200
<v Speaker 2>it basically raises a digital hand and says, look at

631
00:29:50.200 --> 00:29:53.319
<v Speaker 2>this es. But finding a candidate in a computer model

632
00:29:53.400 --> 00:29:56.400
<v Speaker 2>is one thing, right, Proving it is real. Proving that

633
00:29:56.480 --> 00:30:00.480
<v Speaker 2>a million mass monster actually just shredded a star in

634
00:30:00.519 --> 00:30:03.759
<v Speaker 2>the outer rim of a galaxy that requires pointing physical

635
00:30:03.759 --> 00:30:04.720
<v Speaker 2>glass at the sky.

636
00:30:05.160 --> 00:30:08.680
<v Speaker 3>Absolutely, a flag in a database is just a hypothesis.

637
00:30:08.880 --> 00:30:12.960
<v Speaker 3>It requires rigorous observational conformation. You need to gather the

638
00:30:13.000 --> 00:30:14.680
<v Speaker 3>actual photons hitting the Earth.

639
00:30:14.759 --> 00:30:15.359
<v Speaker 2>You need proof.

640
00:30:16.000 --> 00:30:18.839
<v Speaker 3>This leads us to the critical ground game involved in

641
00:30:18.880 --> 00:30:23.480
<v Speaker 3>this discovery. Once the AI flagged TDE twenty twenty five ABCR,

642
00:30:23.799 --> 00:30:27.799
<v Speaker 3>the Carolina team needed rapid, high quality optical observation to

643
00:30:27.839 --> 00:30:30.759
<v Speaker 3>confirm its nature before the flare faded back into.

644
00:30:30.640 --> 00:30:32.759
<v Speaker 2>The dark, because it's not going to glow forever.

645
00:30:32.640 --> 00:30:35.279
<v Speaker 3>No, it phades relatively quickly. And to do that follow

646
00:30:35.319 --> 00:30:38.200
<v Speaker 3>up they use the SOR Telescope. The SOR telescope, yes,

647
00:30:38.400 --> 00:30:42.160
<v Speaker 3>the Southern Astrophysical Research Telescope. It is located on Sarah Pachon,

648
00:30:42.200 --> 00:30:44.400
<v Speaker 3>which is a mountain in the Chilean Andes.

649
00:30:44.720 --> 00:30:46.480
<v Speaker 2>Chile is famous for its observatories.

650
00:30:46.559 --> 00:30:50.440
<v Speaker 3>Right it boasts some of the clearest driest skies on Earth,

651
00:30:50.720 --> 00:30:54.319
<v Speaker 3>perfect for astronomy. So R is a four point one

652
00:30:54.400 --> 00:30:57.960
<v Speaker 3>meter optical and near infrared telescope, and it is highly

653
00:30:58.000 --> 00:31:01.240
<v Speaker 3>relevant that UNC helped build s s and continues to

654
00:31:01.279 --> 00:31:03.759
<v Speaker 3>operate it as part of an international consortium.

655
00:31:03.799 --> 00:31:06.440
<v Speaker 2>Having your own four point one meter telescope on speed

656
00:31:06.440 --> 00:31:10.160
<v Speaker 2>dial seems incredibly handy when you're hunting transient flashes in

657
00:31:10.200 --> 00:31:10.599
<v Speaker 2>the dark.

658
00:31:10.799 --> 00:31:13.359
<v Speaker 3>It is the difference between capturing an event and missing

659
00:31:13.359 --> 00:31:18.039
<v Speaker 3>it entirely. Benjamin C. Kaiser, a postdoctoral researcher at UNC

660
00:31:18.200 --> 00:31:21.039
<v Speaker 3>Chapel Hill, pointed out the immense value of.

661
00:31:21.000 --> 00:31:22.920
<v Speaker 2>This facility because of the speed.

662
00:31:22.720 --> 00:31:26.200
<v Speaker 3>When dealing with short lived astronomical phenomena like a TDE,

663
00:31:26.759 --> 00:31:29.839
<v Speaker 3>time is of the essence the accretion disc will eventually

664
00:31:29.839 --> 00:31:32.359
<v Speaker 3>be consumed, or it will cool down, the evidence will

665
00:31:32.359 --> 00:31:33.359
<v Speaker 3>literally disappear.

666
00:31:33.440 --> 00:31:34.359
<v Speaker 2>It's a ticking clock.

667
00:31:34.799 --> 00:31:37.160
<v Speaker 3>Sor allowed the team to rapidly follow up on the

668
00:31:37.160 --> 00:31:40.799
<v Speaker 3>AIS candidate, point a highly sensitive spectrograph at those exact

669
00:31:40.880 --> 00:31:44.680
<v Speaker 3>coordinates and analyze the light to confirm definitively that this

670
00:31:44.839 --> 00:31:47.319
<v Speaker 3>was indeed a massive black hole shredding a star.

671
00:31:47.720 --> 00:31:50.000
<v Speaker 2>But this wasn't just checking a box to confirm what

672
00:31:50.079 --> 00:31:55.079
<v Speaker 2>event was it. This specific optical confirmation is a monumental

673
00:31:55.079 --> 00:31:58.000
<v Speaker 2>proof of concept for the entire field of astronomy.

674
00:31:58.079 --> 00:32:00.759
<v Speaker 3>It truly is a milestone, which as have stated that

675
00:32:00.839 --> 00:32:05.240
<v Speaker 3>TDE twenty twenty five ABCR provides the very first strong

676
00:32:05.279 --> 00:32:09.599
<v Speaker 3>evidence that astronomers can reliably hunt for wandering supermassive black

677
00:32:09.640 --> 00:32:12.960
<v Speaker 3>holes using ground based visible light telescopes.

678
00:32:13.119 --> 00:32:15.359
<v Speaker 2>Let's make sure we underline why that is so important.

679
00:32:15.640 --> 00:32:19.599
<v Speaker 2>Up until now, to find really weird extreme stuff like

680
00:32:19.680 --> 00:32:23.279
<v Speaker 2>black holes, we often had to rely on space telescopes

681
00:32:23.319 --> 00:32:25.000
<v Speaker 2>looking at X rays or gamma rays.

682
00:32:24.839 --> 00:32:27.759
<v Speaker 3>R usually yes like the Chonder X ray observatory, and

683
00:32:27.799 --> 00:32:31.160
<v Speaker 3>those space observatories are incredibly expensive, They have limited lifespans,

684
00:32:31.200 --> 00:32:34.200
<v Speaker 3>and securing observation time on them is highly highly competitive.

685
00:32:34.279 --> 00:32:36.039
<v Speaker 3>You basically have to win a lottery to get time

686
00:32:36.039 --> 00:32:36.359
<v Speaker 3>on them.

687
00:32:36.400 --> 00:32:39.279
<v Speaker 2>But this proves we can find these invisible monsters just

688
00:32:39.359 --> 00:32:41.440
<v Speaker 2>by looking for the visible flash of their meals from

689
00:32:41.480 --> 00:32:44.319
<v Speaker 2>right here on Earth using glass on a mountain in Chili.

690
00:32:44.559 --> 00:32:48.880
<v Speaker 3>It effectively opens an entirely new sub field of astrophysics.

691
00:32:49.160 --> 00:32:52.799
<v Speaker 3>It proves the methodology is sound. You combine unbiased AI

692
00:32:52.920 --> 00:32:56.599
<v Speaker 3>scanning of large optical survey data with rapid follow up

693
00:32:56.640 --> 00:32:58.880
<v Speaker 3>from agile ground based optical.

694
00:32:58.519 --> 00:33:00.759
<v Speaker 2>Telescopes like SR one two punch.

695
00:33:01.039 --> 00:33:03.720
<v Speaker 3>This combination is the blueprint for how we will map

696
00:33:03.759 --> 00:33:05.200
<v Speaker 3>the hidden universe in the future.

697
00:33:05.279 --> 00:33:08.640
<v Speaker 2>And that future is coming fast because that fire hose

698
00:33:08.680 --> 00:33:10.920
<v Speaker 2>of data we were talking about earlier, it's about to

699
00:33:10.960 --> 00:33:12.799
<v Speaker 2>turn into a complete ocean.

700
00:33:12.920 --> 00:33:16.200
<v Speaker 3>We are standing on the precipice of an observational explosion.

701
00:33:16.680 --> 00:33:20.319
<v Speaker 3>We have next generation survey telescopes coming online very soon

702
00:33:20.480 --> 00:33:23.119
<v Speaker 3>that will absolutely dwarf for current capabilities.

703
00:33:23.240 --> 00:33:24.200
<v Speaker 2>Give me some examples.

704
00:33:24.279 --> 00:33:27.680
<v Speaker 3>Well, the NSF does Veric Reuben Observatory, which is currently

705
00:33:27.720 --> 00:33:31.160
<v Speaker 3>being built in Chile, features a thirty two hundred megapixel camera.

706
00:33:31.319 --> 00:33:33.440
<v Speaker 2>Thirty two hundred megapixels, that's absurd.

707
00:33:33.720 --> 00:33:37.319
<v Speaker 3>It will essentially film a continuous high definition time lapse

708
00:33:37.400 --> 00:33:40.559
<v Speaker 3>movie of the entire Southern sky every few nights. It

709
00:33:40.559 --> 00:33:43.039
<v Speaker 3>will generate fifteen terabytes of data a night.

710
00:33:43.160 --> 00:33:46.559
<v Speaker 2>Fifteen terabytes a night. Human eyes literally cannot look at that.

711
00:33:46.880 --> 00:33:50.880
<v Speaker 3>It is physically impossible. We also have the Roman Space Telescope,

712
00:33:51.039 --> 00:33:55.519
<v Speaker 3>which will survey vast areas of space with incredible infrared resolution.

713
00:33:56.240 --> 00:33:59.799
<v Speaker 3>And UNC's own Argus Array, which is a uniquely designed

714
00:33:59.799 --> 00:34:04.119
<v Speaker 3>telescope system meant to monitor the entire visible sky simultaneously

715
00:34:04.480 --> 00:34:06.079
<v Speaker 3>for rapid transient events.

716
00:34:06.160 --> 00:34:08.800
<v Speaker 2>So what does that transition look like for finding these things?

717
00:34:09.039 --> 00:34:11.679
<v Speaker 2>If we've only found a little over one hundred TDEs

718
00:34:11.719 --> 00:34:15.400
<v Speaker 2>in the past decade, what happens when Reuben and Roman

719
00:34:15.400 --> 00:34:16.880
<v Speaker 2>and Argus actually turn.

720
00:34:16.719 --> 00:34:20.039
<v Speaker 3>On The estimates are staggering. Astronomers expect to go from

721
00:34:20.079 --> 00:34:23.280
<v Speaker 3>discovering tens of tidal disruption events per year in the

722
00:34:23.320 --> 00:34:27.719
<v Speaker 3>relatively nearby universe to discovering many hundreds, if not thousands

723
00:34:27.760 --> 00:34:32.000
<v Speaker 3>of them per year. Thousands, and at much greater cosmological distances.

724
00:34:31.679 --> 00:34:35.079
<v Speaker 2>Thousands of stars being shredded by black holes spotted every

725
00:34:35.119 --> 00:34:35.880
<v Speaker 2>single year.

726
00:34:35.800 --> 00:34:38.400
<v Speaker 3>Which means we won't just be finding the standard centrally

727
00:34:38.400 --> 00:34:42.000
<v Speaker 3>located black holes anymore. By applying the unbiased AI tools

728
00:34:42.039 --> 00:34:44.599
<v Speaker 3>we just discussed to this massive new influx of data,

729
00:34:44.960 --> 00:34:48.239
<v Speaker 3>we are bound to find countless more wandering black holes.

730
00:34:47.960 --> 00:34:50.320
<v Speaker 2>Because we finally know how to look for them exactly.

731
00:34:50.360 --> 00:34:53.639
<v Speaker 3>We will finally be able to map their populations, understand

732
00:34:53.679 --> 00:34:57.719
<v Speaker 3>their distribution across galactic halos, and finally piece together the

733
00:34:57.760 --> 00:35:02.320
<v Speaker 3>full chaotic history of galactic evilllution, of ancient mergers, and

734
00:35:02.360 --> 00:35:03.679
<v Speaker 3>of three body slingshots.

735
00:35:03.719 --> 00:35:06.000
<v Speaker 2>I want to connect this back to you listening right now.

736
00:35:06.199 --> 00:35:10.039
<v Speaker 2>We've talked about billion year old galactic mergers, million mass

737
00:35:10.039 --> 00:35:14.199
<v Speaker 2>ghosts hiding in the dark, AI algorithms rewriting their own biases,

738
00:35:14.559 --> 00:35:17.360
<v Speaker 2>and giant pieces of glass on mountaintops in Chile.

739
00:35:17.559 --> 00:35:18.679
<v Speaker 3>There's a lot of ground to cover.

740
00:35:18.800 --> 00:35:21.679
<v Speaker 2>It's an incredible narrative of scale. But why should you

741
00:35:21.760 --> 00:35:24.960
<v Speaker 2>care beyond just the sci fi cool factor of a

742
00:35:25.079 --> 00:35:28.039
<v Speaker 2>rogue black hole eating a star? What is the actual

743
00:35:28.119 --> 00:35:32.320
<v Speaker 2>relevance of this knowledge to humanity? Why does it matter

744
00:35:32.400 --> 00:35:34.159
<v Speaker 2>to the physics of our own reality?

745
00:35:34.280 --> 00:35:36.920
<v Speaker 3>It matters because it is a question of fundamental physics.

746
00:35:37.199 --> 00:35:40.400
<v Speaker 3>These extreme events a supermassive black hole shredding a star

747
00:35:40.480 --> 00:35:44.119
<v Speaker 3>release enormous amounts of energy energy we can't make here exactly.

748
00:35:44.239 --> 00:35:48.000
<v Speaker 3>They create environments with gravitational forces, magnetic fields, and extreme

749
00:35:48.000 --> 00:35:51.639
<v Speaker 3>states of matter that are absolutely fundamentally impossible to recreate

750
00:35:51.679 --> 00:35:53.280
<v Speaker 3>in any laboratory on Earth.

751
00:35:53.760 --> 00:35:56.039
<v Speaker 2>Right like, we can't build a black hole in a

752
00:35:56.039 --> 00:35:59.400
<v Speaker 2>particle accelerator in Switzerland to see how space time bends.

753
00:36:00.119 --> 00:36:02.159
<v Speaker 3>That would be ill advised even if we could.

754
00:36:02.360 --> 00:36:06.280
<v Speaker 2>Very true, we can't compress matter into a singularity to

755
00:36:06.320 --> 00:36:08.679
<v Speaker 2>see what happens to the laws of thermodynamics.

756
00:36:08.719 --> 00:36:13.119
<v Speaker 3>Precisely, we cannot generate those magnetic fields, those temperatures, or

757
00:36:13.119 --> 00:36:18.119
<v Speaker 3>that extreme space time curvature. Therefore, the universe itself must

758
00:36:18.159 --> 00:36:19.000
<v Speaker 3>become our.

759
00:36:18.960 --> 00:36:21.199
<v Speaker 2>Laboratory, the ultimate testing ground.

760
00:36:21.679 --> 00:36:24.760
<v Speaker 3>Every time we observe a tde we are watching a

761
00:36:24.800 --> 00:36:28.960
<v Speaker 3>fundamental physics experiment play out on a cosmic scale. By

762
00:36:29.000 --> 00:36:32.320
<v Speaker 3>studying the light curves, the relativistic jets, the friction of

763
00:36:32.360 --> 00:36:35.800
<v Speaker 3>the accretion disk, we are unraveling the bedrock laws that

764
00:36:35.880 --> 00:36:37.880
<v Speaker 3>govern the entire universe.

765
00:36:37.760 --> 00:36:39.920
<v Speaker 2>The same laws of physics that govern the atoms in

766
00:36:39.960 --> 00:36:41.760
<v Speaker 2>your body right now, sitting in your car.

767
00:36:41.679 --> 00:36:46.639
<v Speaker 3>Or walking your dog exactly, Gravity, electromagnetism, thermodynamics, These are

768
00:36:46.679 --> 00:36:49.239
<v Speaker 3>the rules of the ecosystem we live inside. We are

769
00:36:49.320 --> 00:36:53.320
<v Speaker 3>learning how gravity truly operates at its absolute extremes.

770
00:36:53.039 --> 00:36:54.880
<v Speaker 2>Testing the limits of Einstein's theories.

771
00:36:55.199 --> 00:36:59.079
<v Speaker 3>We are uncovering the full life cycles of stars and galaxies,

772
00:36:59.480 --> 00:37:02.639
<v Speaker 3>the violence mechanisms of how structure forms in the universe.

773
00:37:03.119 --> 00:37:06.519
<v Speaker 3>Every single observation brings us one step closer to understanding

774
00:37:06.519 --> 00:37:09.760
<v Speaker 3>the mechanics of reality itself. We are not separate from

775
00:37:09.800 --> 00:37:13.039
<v Speaker 3>these events. We are a byproduct of a universe dynamic

776
00:37:13.159 --> 00:37:14.519
<v Speaker 3>enough to create them.

777
00:37:14.760 --> 00:37:17.400
<v Speaker 2>It is awe inspiring to think about to recap the

778
00:37:17.400 --> 00:37:20.159
<v Speaker 2>sheer scale of what we've just covered. We started with

779
00:37:20.199 --> 00:37:23.840
<v Speaker 2>a single star drifting through a quiet galactic suburb, completely

780
00:37:23.920 --> 00:37:26.960
<v Speaker 2>unaware that it was approaching a hazard it couldn't possibly.

781
00:37:26.559 --> 00:37:28.199
<v Speaker 3>See, a cosmic ghost.

782
00:37:28.559 --> 00:37:31.440
<v Speaker 2>We witnessed it splintering in the dark, pulled apart by

783
00:37:31.440 --> 00:37:35.760
<v Speaker 2>tidal forces, illuminating a rogue one million solar mass black

784
00:37:35.800 --> 00:37:39.280
<v Speaker 2>hole that had been violently exiled from its home millions

785
00:37:39.400 --> 00:37:40.760
<v Speaker 2>or billions of years ago.

786
00:37:40.679 --> 00:37:43.119
<v Speaker 3>And we saw how our own human assumptions almost hid

787
00:37:43.159 --> 00:37:43.960
<v Speaker 3>it forever right.

788
00:37:44.199 --> 00:37:46.400
<v Speaker 2>Our belief that monsters only hide in the center of

789
00:37:46.440 --> 00:37:49.360
<v Speaker 2>the room almost kept this ghost hidden until we allowed

790
00:37:49.360 --> 00:37:52.440
<v Speaker 2>an artificial intelligence to look at the data without our bias.

791
00:37:52.960 --> 00:37:54.920
<v Speaker 2>We saw a telescope in Chile a pivot just in

792
00:37:54.960 --> 00:37:57.320
<v Speaker 2>time to catch the fading light, proving that we can

793
00:37:57.400 --> 00:37:59.440
<v Speaker 2>hunt these invisible anomalies from the ground.

794
00:38:00.000 --> 00:38:02.760
<v Speaker 3>And we looked ahead to a very near future.

795
00:38:02.800 --> 00:38:07.400
<v Speaker 2>A future where new massive observatories will soon find thousands

796
00:38:07.440 --> 00:38:11.199
<v Speaker 2>of these violent cosmic meals, turning the night sky into

797
00:38:11.280 --> 00:38:13.039
<v Speaker 2>the ultimate physics laboratory.

798
00:38:13.400 --> 00:38:16.159
<v Speaker 3>It is a profound reminder that there is always more

799
00:38:16.199 --> 00:38:18.599
<v Speaker 3>to learn, and that our understanding of the universe is

800
00:38:18.679 --> 00:38:23.559
<v Speaker 3>constantly evolving. The cosmos is far more dynamic, chaotic, and

801
00:38:23.599 --> 00:38:27.239
<v Speaker 3>beautifully violent than we often assume. But you know, there

802
00:38:27.280 --> 00:38:30.159
<v Speaker 3>is one final piece of this puzzle, a final implication

803
00:38:30.320 --> 00:38:32.159
<v Speaker 3>that I think we need to leave hanging in the air.

804
00:38:32.320 --> 00:38:33.360
<v Speaker 2>Oh what's that?

805
00:38:33.840 --> 00:38:35.960
<v Speaker 3>Think about the math for a second. Okay, If a

806
00:38:36.000 --> 00:38:39.480
<v Speaker 3>single massive galaxy can hide a one million solar mass

807
00:38:39.559 --> 00:38:43.679
<v Speaker 3>black hole roaming its outer edges, an entity completely invisible,

808
00:38:43.880 --> 00:38:47.599
<v Speaker 3>entirely undetectable, drifting silently through the suburbs until the exact

809
00:38:47.639 --> 00:38:49.400
<v Speaker 3>moment a random star bumps into it.

810
00:38:49.519 --> 00:38:51.039
<v Speaker 2>Oh man, I see where this is going.

811
00:38:51.119 --> 00:38:53.960
<v Speaker 3>How many other silent gravitational giants are wandering through the

812
00:38:54.039 --> 00:38:57.079
<v Speaker 3>dark right now, perhaps even in our own galactic neighborhood,

813
00:38:57.280 --> 00:38:59.800
<v Speaker 3>reshaping the universe in ways we cannot even see, just

814
00:39:00.039 --> 00:39:01.079
<v Speaker 3>eating in the pitch black
