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>Hello everyone, and welcome back to the show. We have

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<v Speaker 2>a truly massive topic on the table today. And I

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<v Speaker 2>don't mean massive in the you know, the casual sense.

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<v Speaker 2>I mean we are literally talking about the heaviest, densest

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<v Speaker 2>objects in the entire universe.

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<v Speaker 3>We really are.

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<v Speaker 2>We're looking at a paper that just dropped yesterday February twelve,

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<v Speaker 2>twenty twenty six, in Physical Review Letters.

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<v Speaker 3>Yeah, it's about as hot off the press as it

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<v Speaker 3>gets in this field.

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<v Speaker 2>It really is. And I have to say, reading through

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<v Speaker 2>it this morning, it just felt like one of those

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<v Speaker 2>moments where you realize we might have been looking at

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<v Speaker 2>the sky in well in the wrong way for the

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<v Speaker 2>last fifty years.

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<v Speaker 3>That's honestly not much of an exaggeration. This paper. It's

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<v Speaker 3>by Henksy Wang and a team from the Max Planck

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<v Speaker 3>Institute in Oxford. It takes a problem that has frustrated

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<v Speaker 3>astrophysicists for decades and just completely flips it on its head.

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<v Speaker 2>It really does. It turns a limitation into a tool.

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<v Speaker 3>Exactly.

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<v Speaker 2>We are talking about the universe as hidden strobes. More specifically,

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<v Speaker 2>we're talking about supermassive black hole binaries, two absolute monsters

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<v Speaker 2>locked in a death spiral, hiding in the dark.

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<v Speaker 3>And until yesterday, hiding was definitely the right word.

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<v Speaker 2>Right, So let's set the stage here for everyone, because

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<v Speaker 2>I think most people have this image of a black

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<v Speaker 2>hole as this lonely cosmic vacuum cleaner floating out there by.

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<v Speaker 3>Itself, a solitary monster.

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<v Speaker 2>Yeah, but that's not really the whole story.

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<v Speaker 3>Is it not at all? I mean, sure, solitary black

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<v Speaker 3>holes exist, of course, But if you look at the

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<v Speaker 3>grand structure of the cosmos, the whole thing is hierarchical.

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<v Speaker 3>Galaxies grow by eating other galaxies.

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<v Speaker 2>It's galactic cannibalism.

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<v Speaker 3>It is. It's a violent, messy history. Our own Milky

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<v Speaker 3>Way has eaten smaller dwarf galaxies in the past, and

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<v Speaker 3>we're famously on a collision course with Andromeda.

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<v Speaker 2>Which is by the way still terrifying, but that's a

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<v Speaker 2>problem for a few billion years from now, I guess, right.

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<v Speaker 3>But just think about the architecture for a second. We

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<v Speaker 3>know that pretty much every massive galaxy, including our own,

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<v Speaker 3>has a superassive black hole in SMBH at its heart.

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<v Speaker 3>Ours is SAGITTARIUSA, SAGITTARIUSA exactly, Andromeda has one that's much bigger.

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<v Speaker 3>So when Galaxy A smashes into Galaxy B, the.

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<v Speaker 2>Two big black holes have to go somewhere.

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<v Speaker 3>They have to. They don't just vanish. As the two

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<v Speaker 3>galaxies merge and all the stars and gas settle down

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<v Speaker 3>into a new larger structure. Those two central black holes

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<v Speaker 3>they have to interact. They sink.

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<v Speaker 2>They sink towards the middle of the new galaxy.

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<v Speaker 3>Right through a process we call dynamical friction. They sink

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<v Speaker 3>toward the new center of gravity, and so logic dictates

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<v Speaker 3>they must eventually find each.

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<v Speaker 2>Other and form a pair a binary.

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<v Speaker 3>A binary two super massive black holes orbiting each other.

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<v Speaker 2>And this is the invisible dance we're talking about. The

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<v Speaker 2>physics says they have to be there. All our models

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<v Speaker 2>of how galaxies evolve say the universe should be well

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<v Speaker 2>teeming with these.

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<v Speaker 3>Things, it should be a common phenomenon.

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<v Speaker 2>But when we point our best telescopes at those centers

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<v Speaker 2>of these big merged galaxies, we see nothing.

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<v Speaker 3>Well, not quite nothing. We see the galaxy the bright core.

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<v Speaker 3>But trying to resolve two distinct black holes that are

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<v Speaker 3>orbiting closely. It's arguably one of the single hardest observational

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<v Speaker 3>challenges in all of astronomy.

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<v Speaker 2>Okay, but why I mean we have the event horizon telescope.

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<v Speaker 2>We literally took a picture of a black hole shadow

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<v Speaker 2>a few years back. Why can't we just zoom in

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<v Speaker 2>and see two of them?

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<v Speaker 3>It's all about scale and resolution. The event Horizon telescope

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<v Speaker 3>was an incredible feat, but it essentially turned the entire

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<v Speaker 3>planet Earth into one giant radio dish to look at

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<v Speaker 3>two very specific tars targets our own Sagittarius A and

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<v Speaker 3>the one in M eighty seven.

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<v Speaker 2>So it's not something we can just point anywhere.

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<v Speaker 3>No, not at all. And for these binarias, we're talking

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<v Speaker 3>about objects that could be millions or even billions of

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<v Speaker 3>light years away. Now, when they're still very far apart

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<v Speaker 3>from each other, say a few thousand light years, we

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<v Speaker 3>can sometimes see them. We have confirmed cases of dual

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<v Speaker 3>active galactic nuclei.

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<v Speaker 2>So two bright spots and a messy colliding galaxy exactly.

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<v Speaker 3>You can resolve them as two distinct points of light.

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<v Speaker 2>Okay, so we can see the ones that have just

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<v Speaker 2>started dating.

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<v Speaker 3>You could put it that way. They're just waving at

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<v Speaker 3>each other from across the room. But the ones we

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<v Speaker 3>really care about, the ones that are gravitationally bound and

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<v Speaker 3>are spiraling in towards an inevitable cataclysmic merger, those are

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<v Speaker 3>effectively invisible.

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<v Speaker 2>Why because they're too close, way too close.

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<v Speaker 3>At that distance, they're separated by less than a light year,

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<v Speaker 3>maybe much less. To our telescopes, they just blur together

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<v Speaker 3>into a single blob of light.

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<v Speaker 2>So they're either hiding in the glare of the galaxy's core.

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<v Speaker 3>Or hiding in complete darkness if there isn't a lot

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<v Speaker 3>of gas around them for them to eat and light up.

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<v Speaker 3>And this has created this huge frustrating gap in our understanding.

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<v Speaker 2>A cosmic blind spot.

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<v Speaker 3>It is. We see them when they're far apart, and

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<v Speaker 3>thanks to detectors like Lego, we can hear them in

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<v Speaker 3>the final fraction of a second when they actually crash

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<v Speaker 3>together and merge.

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<v Speaker 2>But the whole middle part, the millions of years they

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<v Speaker 2>spend spiraling closer and closer.

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<v Speaker 3>It's a complete black box. We have almost no confirmed

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<v Speaker 3>observations of that inspiral phase for supermassive black hole.

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<v Speaker 2>Which is where this new paper comes in because the

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<v Speaker 2>team from Max Plank in Oxford is basically saying, Okay,

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<v Speaker 2>stop looking for the black holes.

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<v Speaker 3>Exactly. They're saying, stop trying to resolve the dark objects themselves. Instead,

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<v Speaker 3>look at the background, look at the wallpaper, look at

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<v Speaker 3>the stars sitting behind them. They are proposing we use

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<v Speaker 3>these binary black holes not as targets, but as lenses,

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<v Speaker 3>as natural telescopes.

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<v Speaker 2>Okay, this is where we need to go into the details.

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<v Speaker 2>Because gravitational lensing is a term that gets tossed around

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<v Speaker 2>a lot. You always hear the same analogy, you know,

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<v Speaker 2>a bowling ball on a trampoline.

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<v Speaker 3>The trampoline analogy.

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<v Speaker 2>Yeah, that's not going to cut it today. We need

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<v Speaker 2>to go deeper, we really do.

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<v Speaker 3>The trampoline analogy is well, it's fine for getting the

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<v Speaker 3>basic idea across, but it completely fails to explain why

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<v Speaker 3>what this paper's proposing is so groundbreaking.

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<v Speaker 2>So walk us through the actual mechanism. Let's start with

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<v Speaker 2>lensing one oh one, a single black hole, okay.

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<v Speaker 3>Einstein's general relativity mass warps the fabric of space time,

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<v Speaker 3>and light, which we normally think of as traveling in

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<v Speaker 3>a straight line, has to follow the curves in space time.

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<v Speaker 2>So it's not that gravity is pulling on the light,

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<v Speaker 2>it's that the path itself is bent precisely.

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<v Speaker 3>Light is just taking the straightest possible path through a

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<v Speaker 3>curved space. So if you have a massive object, the lens,

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<v Speaker 3>and a light source directly behind it, the light from

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<v Speaker 3>that source has to travel around the lens to get.

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<v Speaker 2>To us, flowing around a rock in a stream.

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<v Speaker 3>That's a decent analogy. Now, if you have a single

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<v Speaker 3>perfectly spherical mass, like a single non spinning black hole,

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<v Speaker 3>that lensing effect is very, very symmetric, okay. And if

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<v Speaker 3>the alignment is perfect, the background, star, the black hole,

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<v Speaker 3>and you, the observer are all in a perfect line.

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<v Speaker 3>That symmetry focuses the light into what we call an

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<v Speaker 3>Einstein ring.

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<v Speaker 2>A perfect circle of light, a perfect circle.

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<v Speaker 3>We've seen these. We use them to weigh distant galaxies

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<v Speaker 3>and find exoplanets. It's a standard tool in the astronomical toolkit.

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<v Speaker 2>But what's the catch.

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<v Speaker 3>The catch is that word perfect. For a single spherical

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<v Speaker 3>lens that has a single focal point, you have to

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<v Speaker 3>be exactly on that line of sight to get that

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<v Speaker 3>extreme magnification to see the ring. It's like a laser beam.

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<v Speaker 2>So if a background star is just a tiny bit

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<v Speaker 2>off to the side of the black hole, we don't

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<v Speaker 2>see the ring.

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<v Speaker 3>You'll see some distortion. The star might appear as two separate,

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<v Speaker 3>slightly brighter images, but you don't get that massive, massive

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<v Speaker 3>spike and brightness unless the alignment is just so. It's rare,

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<v Speaker 3>very rare.

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<v Speaker 2>Okay, that's lensing one oh one. Now enter the second

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<v Speaker 2>black hole lensing two to two.

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<v Speaker 3>This is where everything changes. You aren't just adding a

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<v Speaker 3>second lens next to the first one. You are creating

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<v Speaker 3>a complex interference pattern between two deep gravitational wells.

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<v Speaker 2>The paper uses this term costic curves, and I know

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<v Speaker 2>costic usually means something that burns.

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<v Speaker 3>It does, but in optics and in gravitational lensing, it

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<v Speaker 3>means something else. Left you back to that swimming pool

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<v Speaker 3>analogy I mentioned earlier.

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<v Speaker 2>The squiggly lines on the bottom.

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<v Speaker 3>Exactly Think about why those lines are there. The surface

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<v Speaker 3>of the water isn't flat. It's covered in little waves

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<v Speaker 3>and ripples. Right, each ripple acts like a tiny, imperfect lens.

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<v Speaker 2>Okay, I'm with you.

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<v Speaker 3>So these ripples aren't focusing the sunlight into lots of

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<v Speaker 3>little single points. They're focusing the light into lines, into curves.

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<v Speaker 3>And those bright, dancing webs of light on the bottom

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<v Speaker 3>of the pool, those are the caustics. It's where the

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<v Speaker 3>light rays pile up, where the intensity is highest.

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<v Speaker 2>Got it. So the water ripples are the imperfect lens,

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<v Speaker 2>and the bright lines are the You've got it.

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<v Speaker 3>Now take that concept and scale it up to the cosmos.

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<v Speaker 3>Instead of ripples on water, you have two supermassive black

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<v Speaker 3>holes orbiting each other. Their combined gravity creates a very

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<v Speaker 3>complex surface in space time. It's not a smooth bowl anymore.

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<v Speaker 2>It has ridges and valleys exactly.

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<v Speaker 3>And those gravitational ridges focus the light from background stars,

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<v Speaker 3>not into a point, but into a network of high

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<v Speaker 3>magnification lines. Those are the caustic curves.

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<v Speaker 2>And what do they look like?

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<v Speaker 3>For a binary system? This network creates a very specific shape.

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<v Speaker 3>The paper describes it as a diamond shaped structure. In mathematics,

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<v Speaker 3>it's called an.

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<v Speaker 2>Astroid, an asteroid like video game.

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<v Speaker 3>Spelled differently, but yeah, it looks a bit like that.

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<v Speaker 3>It's a star shape, a diamond with four points, but

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<v Speaker 3>the sides are curved inwards. They're concave.

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<v Speaker 2>So let me picture this floating in empty space behind

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<v Speaker 2>these two invisible black holes. Is this other invisible thing,

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<v Speaker 2>this geometric diamond of pure magnification?

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<v Speaker 3>That is exactly what it is. And here is the

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<v Speaker 3>absolute critical difference between a single black hole and a binary.

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<v Speaker 3>For a single black hole, the region of very high

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<v Speaker 3>magnification is a tiny point. For a binary, the region

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<v Speaker 3>of very high magnification is this entire much larger diamond

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<v Speaker 3>shaped perimeter.

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<v Speaker 2>So the target is just bigger.

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<v Speaker 3>Massively bigger. Ben's Coxus, one of the authors, makes this

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<v Speaker 3>exact point in the press release. The chances of a

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<v Speaker 3>background star's light being hugely amplified increase enormously for a

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<v Speaker 3>binary compared to a single black hole.

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<v Speaker 2>It's the difference between trying to hit the bull's eye

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<v Speaker 2>with a single dart and just trying to hit any

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<v Speaker 2>part of the dark.

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<v Speaker 3>Board, a much much bigger darkboard. You've gone from trying

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<v Speaker 3>to thread a needle to trying to hit a barn door,

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<v Speaker 3>the probability just skyrockets.

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<v Speaker 2>Okay, so the net is bigger. We have a much

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<v Speaker 2>better chance of a background star lining up with this

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<v Speaker 2>diamond shape. But the black holes aren't just sitting there.

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<v Speaker 3>No, they're not. And this is where the strobe concept

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<v Speaker 3>finally clicks into place. If the two black holes were

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<v Speaker 3>just frozen in space, the diamond caustic would be frozen too.

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<v Speaker 3>A star that falls on it would just look like

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<v Speaker 3>a permanently distorted, brightened image.

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<v Speaker 2>But they're not frozen. They're orbiting each other.

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<v Speaker 3>They're orbiting. They're in a constant dance.

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<v Speaker 2>So the diamond spins.

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<v Speaker 3>The diamond spins, it rotates right along with the binary.

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<v Speaker 3>Imagine a lighthouse and the beam is rotating. But in

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<v Speaker 3>this case, the beam isn't a simple ray of light.

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<v Speaker 3>It's this entire complex caustic structure. It's a diamond shaped

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<v Speaker 3>beam of magnification.

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<v Speaker 2>And that beam is sweeping across the background sky.

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<v Speaker 3>Constantly sweeping. And the background sky, even in a seemingly

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<v Speaker 3>empty patch, is just filled with faint, distant stars.

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<v Speaker 2>So it's only a matter of time before that sweeping

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<v Speaker 2>line of magnification runs over one of those stars.

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<v Speaker 3>It's inevitable, purely by chance, the caustic curve will cross

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<v Speaker 3>a background star.

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<v Speaker 2>And when it hits, yeah, what do we see?

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<v Speaker 3>We see a flash. The mathematics of the caustic means

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<v Speaker 3>the magnification just shoots up. Hanksy Wang, the lead author,

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<v Speaker 3>describes it as an extraor ordinarily bright flash for a

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<v Speaker 3>brief period of time. It could be hours, could be days.

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<v Speaker 3>It depends on the geometry and the speed. That background

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<v Speaker 3>star will suddenly become hundreds or even thousands of times

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<v Speaker 3>brighter than it normally.

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<v Speaker 2>Is like someone switched on a cosmic light.

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<v Speaker 3>Bulb, a very powerful one. And then as the caustic

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<v Speaker 3>line passes over the star and moves on.

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<v Speaker 2>The star goes back to normal.

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<v Speaker 3>It fades back to its regular faint baseline brightness, as

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<v Speaker 3>if nothing happened.

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<v Speaker 2>But the binary is still orbiting.

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<v Speaker 3>The binary keeps spinning, so the diamond cost it comes

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<v Speaker 3>around again.

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<v Speaker 2>On the next orbit, and if that star is still

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<v Speaker 2>in the path, it hits.

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<v Speaker 3>The star again.

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<v Speaker 2>Flash flash. So we get a repeating signal a.

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<v Speaker 3>Blank Hey, you get a strobe light, a repeating predictable

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<v Speaker 3>burst of starlight, all caused by two invisible objects dancing

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<v Speaker 3>in front of it.

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<v Speaker 2>Okay, okay, I have to play Devil's advocate here. You know,

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<v Speaker 2>I love this idea. But the universe is a really

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<v Speaker 2>noisy place. It's full of things that blink and flash.

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<v Speaker 2>We have variable stars, sefeed's, flarre stars, cataclysmic variables, super no.

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<v Speaker 2>I mean, the list goes on. How can we possibly

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<v Speaker 2>be sure that a blink we see is from this

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<v Speaker 2>weird lensing effect and not just you know, a star

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<v Speaker 2>having a hiccup.

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<v Speaker 3>That is probably the most important question in this entire

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<v Speaker 3>field of time domain astronomy. Is this transient, this flash unique?

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<v Speaker 3>And the authors of this paper argue that, yes, this

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<v Speaker 3>signal is remarkably distinct. It has a fingerprint distinction. What way,

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<v Speaker 3>the timing, the shape, It all comes down to the

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<v Speaker 3>light curve. That's what astronomers call a plot of an

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<v Speaker 3>object's brightness over time. Okay, so if you look at

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<v Speaker 3>the light curve of a typical variable star like a sephid,

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<v Speaker 3>it often looks like a smooth wave. The brightness swells

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<v Speaker 3>up and then it shrinks back down. It's often quite symmetric.

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<v Speaker 3>That's because the physics is internal to the star. It's

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<v Speaker 3>literally breathing, expanding and contracting.

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<v Speaker 2>And a costic crossing. What does that look like on

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<v Speaker 2>the graph?

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00:13:49.960 --> 00:13:53.919
<v Speaker 3>It looks nothing like that. Acostic crossing is purely geometric.

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<v Speaker 3>It's not about stellar physics. It's about the geometry of

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<v Speaker 3>crossing a fold in space time. The light curve is sharp,

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<v Speaker 3>it's asymmetric. Asymmetric, you get a very very sharp rise

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<v Speaker 3>in brightness and then a slightly slower fall. The peak

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<v Speaker 3>is less of a gentle curve and more of a well,

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00:14:10.159 --> 00:14:14.480
<v Speaker 3>a spike. The math predicts a very specific U shaped

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00:14:14.519 --> 00:14:17.320
<v Speaker 3>profile right at the peak. It's a fingerprint that just

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<v Speaker 3>doesn't look like anything a star does on its own.

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<v Speaker 2>So if we see that specific, jagged spike shape, we

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00:14:23.799 --> 00:14:26.519
<v Speaker 2>know we're looking at gravity, not chemistry or fusion.

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00:14:26.600 --> 00:14:29.159
<v Speaker 3>That's the idea, and there's another layer to it. It's

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<v Speaker 3>not just periodic. The paper calls it quasi period.

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00:14:32.120 --> 00:14:34.039
<v Speaker 2>Quasi periodic, so almost repeating.

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00:14:34.120 --> 00:14:36.879
<v Speaker 3>It repeats, but not perfectly. And the reason it's not

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<v Speaker 3>perfect is the most exciting part. It's the very thing

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00:14:39.720 --> 00:14:41.000
<v Speaker 3>we've been trying to measure for.

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<v Speaker 2>Decades, the inspiral.

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<v Speaker 3>The inspiral. We should probably pause here and really dig

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<v Speaker 3>into why these black holes are merging in the first place.

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<v Speaker 3>We mentioned dynamical fresh earlier how they sink to the center,

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00:14:52.399 --> 00:14:56.440
<v Speaker 3>but that process isn't perfect. It leads to a famous problem.

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00:14:56.279 --> 00:14:59.240
<v Speaker 2>The final parsec problem. I remember this one. It's the

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00:14:59.279 --> 00:15:02.000
<v Speaker 2>idea that they get really close and then they just

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<v Speaker 2>get stuck exactly.

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00:15:03.720 --> 00:15:07.120
<v Speaker 3>Dynamical friction works great when the black holes are far apart,

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00:15:07.399 --> 00:15:10.559
<v Speaker 3>moving through a dense sea of stars. They transfer their

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00:15:10.639 --> 00:15:13.559
<v Speaker 3>orbital energy to the stars and sink. But once they

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00:15:13.600 --> 00:15:16.960
<v Speaker 3>get close enough to form a tight binary, they well,

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<v Speaker 3>they clear out their neighborhood.

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00:15:18.480 --> 00:15:22.000
<v Speaker 2>They kick all the nearby stars away with gravitational slingshots, right.

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00:15:22.120 --> 00:15:24.639
<v Speaker 3>And once they've kicked all the nearby stars away, there's

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00:15:24.720 --> 00:15:27.559
<v Speaker 3>nothing left to create that friction. There's nothing left for

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00:15:27.600 --> 00:15:30.919
<v Speaker 3>them to transfer their energy to. So in theory, they

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00:15:30.919 --> 00:15:33.440
<v Speaker 3>should just stall. They should orbit each other forever at

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<v Speaker 3>a distance of about a parsec or a few light years.

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<v Speaker 3>They should never get close enough to merge.

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00:15:38.360 --> 00:15:41.960
<v Speaker 2>But we know they do merge. We hear the gravitational

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00:15:41.960 --> 00:15:45.600
<v Speaker 2>waves from stellar mass black holes merging with lego all the.

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00:15:45.559 --> 00:15:49.519
<v Speaker 3>Time, exactly, so something has to bridge that final parsec gap.

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00:15:49.840 --> 00:15:51.519
<v Speaker 3>For a long time, we weren't sure what it was.

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00:15:51.759 --> 00:15:55.120
<v Speaker 3>Maybe friction from a big gas disc, maybe interactions with

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00:15:55.159 --> 00:15:58.840
<v Speaker 3>a third black hole. But for these really massive binaries,

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00:15:59.120 --> 00:16:01.759
<v Speaker 3>the dominant four that brings them together in the end

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00:16:02.200 --> 00:16:04.679
<v Speaker 3>is the emission of gravitational waves.

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00:16:04.600 --> 00:16:06.840
<v Speaker 2>And this is the key to decoding the strobes.

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00:16:06.960 --> 00:16:10.559
<v Speaker 3>This is the Rosetta stone. As these two huge masses

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00:16:10.559 --> 00:16:14.039
<v Speaker 3>whip around each other, they are constantly churning space time,

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00:16:14.559 --> 00:16:17.440
<v Speaker 3>radiating enormous amounts of energy away in the form of

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00:16:17.480 --> 00:16:18.679
<v Speaker 3>these gravitational waves.

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00:16:18.759 --> 00:16:20.320
<v Speaker 2>And if they're losing energy.

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00:16:20.080 --> 00:16:23.600
<v Speaker 3>Their orbit has to shrink. As the orbit shrinks, conservation

347
00:16:23.679 --> 00:16:26.120
<v Speaker 3>of angular momentum means they have to speed up.

348
00:16:26.159 --> 00:16:29.600
<v Speaker 2>And if they orbit faster, the strobe light blinks faster.

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00:16:29.799 --> 00:16:32.440
<v Speaker 3>Precisely, this is the decoding part of the whole thing.

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00:16:32.639 --> 00:16:34.759
<v Speaker 3>If we can find one of these systems and watch

351
00:16:34.799 --> 00:16:37.600
<v Speaker 3>the flashes over time, we aren't just seeing a blink.

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00:16:37.879 --> 00:16:40.399
<v Speaker 3>We are seeing a cosmic clock that is ticking faster

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00:16:40.639 --> 00:16:42.200
<v Speaker 3>and faster and faster.

354
00:16:42.440 --> 00:16:44.840
<v Speaker 2>So we can literally measure the rate of orbital decay

355
00:16:45.080 --> 00:16:47.360
<v Speaker 2>just by timing the flashes from a background star.

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00:16:47.840 --> 00:16:51.120
<v Speaker 3>Yes, we can watch general relativity happen in real time.

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00:16:51.679 --> 00:16:54.399
<v Speaker 3>But the paper points out something even more profound, even

358
00:16:54.440 --> 00:16:57.759
<v Speaker 3>more subtle. What's that The emission of gravitational waves doesn't

359
00:16:57.799 --> 00:17:01.360
<v Speaker 3>just change the orbital period, it actually changes the shape

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00:17:01.360 --> 00:17:02.759
<v Speaker 3>of the caustic diamond itself.

361
00:17:02.840 --> 00:17:06.359
<v Speaker 2>Wait, what how the waves themselves are distorting the lens

362
00:17:06.599 --> 00:17:07.119
<v Speaker 2>in a way.

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00:17:07.240 --> 00:17:10.640
<v Speaker 3>Yes, the loss of energy and the shrinking separation between

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00:17:10.640 --> 00:17:14.400
<v Speaker 3>the two black holes alters the overall gravitational potential of

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00:17:14.440 --> 00:17:18.519
<v Speaker 3>the system. This, in turn subtly alters the geometrre of

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00:17:18.559 --> 00:17:21.480
<v Speaker 3>the caustic curve. The paper states that it imprints a

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00:17:21.559 --> 00:17:23.279
<v Speaker 3>characteristic modulation on.

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00:17:23.240 --> 00:17:25.759
<v Speaker 2>The flashes, So the lens itself is warping as the

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00:17:25.839 --> 00:17:27.119
<v Speaker 2>orbit decays.

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00:17:26.759 --> 00:17:30.000
<v Speaker 3>In cosmic real time. Yes, so maybe the peak brightness

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00:17:30.039 --> 00:17:32.599
<v Speaker 3>of the flash gets a tiny bit higher with each pass,

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00:17:33.039 --> 00:17:34.720
<v Speaker 3>or the U shape of the light curve gets a

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00:17:34.759 --> 00:17:37.599
<v Speaker 3>little bit wider. The timing between the flashes will shift

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00:17:37.599 --> 00:17:40.559
<v Speaker 3>in a very specific, predictable way. That is a direct

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00:17:40.599 --> 00:17:42.799
<v Speaker 3>signature of gravitational wave emission.

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00:17:43.200 --> 00:17:45.319
<v Speaker 2>Let me see if we get this straight. We find

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00:17:45.319 --> 00:17:47.960
<v Speaker 2>a star that's flashing, We check the light curve and

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00:17:48.000 --> 00:17:51.319
<v Speaker 2>confirm it has that jagged asymmetric shape of a costa crossing.

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00:17:51.480 --> 00:17:54.240
<v Speaker 2>We watch it repeat from the time between the flashes,

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00:17:54.559 --> 00:17:57.839
<v Speaker 2>we get the orbital period. From the brightness and shape

381
00:17:57.839 --> 00:18:00.440
<v Speaker 2>of the flash, we can work out the total mass

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00:18:00.440 --> 00:18:01.519
<v Speaker 2>of the binary.

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00:18:01.200 --> 00:18:02.119
<v Speaker 3>In their mass ratio.

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00:18:02.240 --> 00:18:05.359
<v Speaker 2>Yes, and then from the tiny change in the timing

385
00:18:05.440 --> 00:18:08.079
<v Speaker 2>and the shape of the flashes over years, we can

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00:18:08.119 --> 00:18:09.799
<v Speaker 2>measure how fast they're spiraling.

387
00:18:09.839 --> 00:18:09.880
<v Speaker 1>It.

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00:18:10.039 --> 00:18:12.599
<v Speaker 3>You've got it. It's a complete telemetry package for an

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00:18:12.640 --> 00:18:16.680
<v Speaker 3>invisible system. We can extract the masses of the black holes,

390
00:18:16.720 --> 00:18:19.000
<v Speaker 3>their distance from each other, their orbital speed, and the

391
00:18:19.079 --> 00:18:21.440
<v Speaker 3>exact rate at which they are falling towards too.

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00:18:22.279 --> 00:18:25.400
<v Speaker 2>That's just that's mind blowing. It's like finding the black

393
00:18:25.440 --> 00:18:28.640
<v Speaker 2>box of a plane crash months before the plane actually crashes.

394
00:18:28.839 --> 00:18:32.839
<v Speaker 3>That's a grim but surprisingly accurate analogy. We are watching

395
00:18:33.000 --> 00:18:34.319
<v Speaker 3>the slow motion collision.

396
00:18:34.480 --> 00:18:36.759
<v Speaker 2>But we have to talk about time scales here because

397
00:18:36.799 --> 00:18:39.599
<v Speaker 2>in astronomy, slow motion usually means check back in a

398
00:18:39.640 --> 00:18:42.680
<v Speaker 2>million years. If a big binary has an orbited period

399
00:18:42.680 --> 00:18:44.960
<v Speaker 2>of say five years, do we have to wait a

400
00:18:45.000 --> 00:18:46.839
<v Speaker 2>whole career to see the orbit change?

401
00:18:46.920 --> 00:18:48.119
<v Speaker 3>That is the practical challenge.

402
00:18:48.200 --> 00:18:48.359
<v Speaker 2>Yes.

403
00:18:48.960 --> 00:18:52.359
<v Speaker 3>For the most massive, super massive black holes, we're talking

404
00:18:52.680 --> 00:18:56.160
<v Speaker 3>billions of solar masses. The orbital period in this phase

405
00:18:56.200 --> 00:18:58.480
<v Speaker 3>could be a few years. So you see a flash

406
00:18:58.880 --> 00:19:01.039
<v Speaker 3>and you set a reminder on your calendar for twenty

407
00:19:01.119 --> 00:19:01.759
<v Speaker 3>thirty one and.

408
00:19:01.759 --> 00:19:05.079
<v Speaker 2>Five years later flash hopefully. Yeah.

409
00:19:05.119 --> 00:19:07.640
<v Speaker 3>So for any single system, yes, it's a very slow

410
00:19:07.640 --> 00:19:10.720
<v Speaker 3>accumulation of data, But the real power of this method

411
00:19:10.880 --> 00:19:14.119
<v Speaker 3>isn't in staring at one system forever, it's in watching

412
00:19:14.160 --> 00:19:14.640
<v Speaker 3>all of them.

413
00:19:14.720 --> 00:19:16.519
<v Speaker 2>A population study exactly.

414
00:19:17.119 --> 00:19:20.000
<v Speaker 3>The paper really emphasizes this point. They say, what is

415
00:19:20.079 --> 00:19:23.920
<v Speaker 3>possible our snapshots. Think of it like walking into a forest.

416
00:19:23.920 --> 00:19:25.880
<v Speaker 3>You can't just sit there and watch a single acorn

417
00:19:25.920 --> 00:19:28.359
<v Speaker 3>grow into a mighty oak tree. That takes a century.

418
00:19:28.920 --> 00:19:30.680
<v Speaker 2>But you can look around and see an acorn on

419
00:19:30.680 --> 00:19:33.559
<v Speaker 2>the ground, a little sapling over there, a young tree,

420
00:19:33.599 --> 00:19:34.680
<v Speaker 2>and a huge old.

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00:19:34.440 --> 00:19:37.720
<v Speaker 3>One, and a rotting log. Exactly. By piecing together all

422
00:19:37.759 --> 00:19:41.039
<v Speaker 3>those different snapshots, you can understand the entire life cycle

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00:19:41.079 --> 00:19:41.599
<v Speaker 3>of the tree.

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00:19:41.680 --> 00:19:43.759
<v Speaker 2>So we apply that to the sky. We look for

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00:19:43.799 --> 00:19:46.480
<v Speaker 2>these flashes everywhere, everywhere.

426
00:19:46.200 --> 00:19:48.680
<v Speaker 3>And if we scan the whole sky, we will find

427
00:19:48.839 --> 00:19:53.559
<v Speaker 3>binary black holes at every single stage of this inspiral process.

428
00:19:54.000 --> 00:19:57.880
<v Speaker 3>We'll find some that are widely separated, flashing every decade

429
00:19:57.960 --> 00:20:00.359
<v Speaker 3>or so. We'll find some that are tighter and faster,

430
00:20:00.559 --> 00:20:03.119
<v Speaker 3>flashing every few months, and we'll find some that are

431
00:20:03.279 --> 00:20:05.400
<v Speaker 3>right on the brink of merging.

432
00:20:05.359 --> 00:20:08.000
<v Speaker 2>And by putting all those data points together, we can

433
00:20:08.039 --> 00:20:10.079
<v Speaker 2>build the movie of how these things evolve.

434
00:20:10.440 --> 00:20:13.240
<v Speaker 3>We can finally fill in that massive gap in our

435
00:20:13.279 --> 00:20:15.119
<v Speaker 3>knowledge of galaxy evolution.

436
00:20:14.920 --> 00:20:17.839
<v Speaker 2>Which brings us to the tools. Because to scan the

437
00:20:17.880 --> 00:20:20.640
<v Speaker 2>whole sky and catch a random flash that might only

438
00:20:20.680 --> 00:20:24.039
<v Speaker 2>be visible for a few days, that just sounds incredibly expensive,

439
00:20:24.039 --> 00:20:26.359
<v Speaker 2>like we'd need a new, dedicated.

440
00:20:25.799 --> 00:20:28.359
<v Speaker 3>Telescope, and it would be if we weren't already building

441
00:20:28.359 --> 00:20:30.559
<v Speaker 3>the perfect machines to do it. For other reasons.

442
00:20:30.640 --> 00:20:32.519
<v Speaker 2>This is the part I love. We don't need a

443
00:20:32.519 --> 00:20:34.200
<v Speaker 2>new line item in the federal budget for this.

444
00:20:34.519 --> 00:20:37.119
<v Speaker 3>No, we can just piggyback on the next generation of

445
00:20:37.160 --> 00:20:39.839
<v Speaker 3>survey telescopes that are about to come online. The paper

446
00:20:39.880 --> 00:20:42.559
<v Speaker 3>specifically calls out two of them, the Vera ce Reuben

447
00:20:42.599 --> 00:20:45.359
<v Speaker 3>Observatory and the Nancy Grace Roman Space Telescope.

448
00:20:45.480 --> 00:20:47.880
<v Speaker 2>Let's talk about Ruben first. That's the one down in Chile, right,

449
00:20:47.920 --> 00:20:49.640
<v Speaker 2>the one that used to be called the LSST.

450
00:20:49.880 --> 00:20:52.640
<v Speaker 3>That's the one the Legacy Survey of Space and Time.

451
00:20:53.519 --> 00:20:56.680
<v Speaker 3>Ruben is an absolute beast of a telescope. It's not

452
00:20:56.759 --> 00:20:59.519
<v Speaker 3>like Hubble or the James web Hubble is like a

453
00:20:59.559 --> 00:21:03.000
<v Speaker 3>sniper rifle. It stares at one tiny, tiny patch of

454
00:21:03.039 --> 00:21:08.000
<v Speaker 3>sky with incredible detail. Reuben is a wide angle lens.

455
00:21:08.039 --> 00:21:08.839
<v Speaker 3>It's a shotgun.

456
00:21:09.039 --> 00:21:10.519
<v Speaker 2>It takes a picture of the whole sky.

457
00:21:10.880 --> 00:21:14.599
<v Speaker 3>It will photograph the entire visible southern sky every three

458
00:21:14.680 --> 00:21:18.599
<v Speaker 3>or four nights, over and over and over again, for

459
00:21:18.759 --> 00:21:19.599
<v Speaker 3>ten years straight.

460
00:21:19.759 --> 00:21:22.000
<v Speaker 2>That's I can't even comprehend that amount of data.

461
00:21:22.079 --> 00:21:26.160
<v Speaker 3>It's something like twenty terabytes of data every single night.

462
00:21:26.559 --> 00:21:29.400
<v Speaker 3>It is literally creating a high definition movie of the

463
00:21:29.480 --> 00:21:29.960
<v Speaker 3>night sky.

464
00:21:30.200 --> 00:21:32.960
<v Speaker 2>So if a background star behind a binary black hole

465
00:21:33.319 --> 00:21:35.839
<v Speaker 2>flashes on a Tuesday night and then goes back to

466
00:21:35.880 --> 00:21:37.240
<v Speaker 2>normal by Friday.

467
00:21:36.920 --> 00:21:39.200
<v Speaker 3>Ruben will see it. It is designed from the ground

468
00:21:39.319 --> 00:21:42.519
<v Speaker 3>up to find transience, things that change, things that flash,

469
00:21:42.559 --> 00:21:45.759
<v Speaker 3>things that move, supernovae, asteroids, variable.

470
00:21:45.400 --> 00:21:49.279
<v Speaker 2>Stars, and now, thanks to this paper, binary black hole strobe.

471
00:21:48.960 --> 00:21:50.720
<v Speaker 3>So on the list of targets. Now the data will

472
00:21:50.720 --> 00:21:52.000
<v Speaker 3>just be sitting there in the archive.

473
00:21:52.240 --> 00:21:54.680
<v Speaker 2>So it's not an observational problem, it's a data science problem.

474
00:21:54.720 --> 00:21:58.119
<v Speaker 3>Exactly. The photons will hit the detector. The challenge is

475
00:21:58.319 --> 00:22:02.519
<v Speaker 3>writing the sophisticated soft where the algorithms that can sift

476
00:22:02.559 --> 00:22:05.960
<v Speaker 3>through those petabytes of data and automatically flag it. To

477
00:22:06.039 --> 00:22:08.519
<v Speaker 3>have a program that says, hey, wait a minute, that

478
00:22:08.599 --> 00:22:12.480
<v Speaker 3>little blink in sector seven G that has the asymmetric

479
00:22:12.559 --> 00:22:15.559
<v Speaker 3>caustic light curve flag it for a human to look at.

480
00:22:15.559 --> 00:22:17.319
<v Speaker 2>And what about the Roman Space Telescope.

481
00:22:17.400 --> 00:22:21.160
<v Speaker 3>That's NASA's next great observatory. It's space based, so no

482
00:22:21.279 --> 00:22:24.640
<v Speaker 3>atmosphere to worry about, and its key feature is its

483
00:22:24.680 --> 00:22:27.039
<v Speaker 3>field of view. It can see a patch of sky

484
00:22:27.119 --> 00:22:29.960
<v Speaker 3>one hundred times larger than Hubble can in a single

485
00:22:30.000 --> 00:22:30.839
<v Speaker 3>pointing so.

486
00:22:30.799 --> 00:22:32.519
<v Speaker 2>It's like a Hubble quality shotgun.

487
00:22:32.640 --> 00:22:34.119
<v Speaker 3>That's a great way to put it. It's doing what

488
00:22:34.200 --> 00:22:37.079
<v Speaker 3>Reuben does, but from space and in the infrared, So

489
00:22:37.160 --> 00:22:39.640
<v Speaker 3>between the two of them, we're going to have eyes

490
00:22:39.720 --> 00:22:42.440
<v Speaker 3>on almost the entire sky almost all the time.

491
00:22:42.519 --> 00:22:44.599
<v Speaker 2>We're really entering a new era of astronomy.

492
00:22:44.680 --> 00:22:47.759
<v Speaker 3>It's the golden age of time domain astronomy. For most

493
00:22:47.759 --> 00:22:51.319
<v Speaker 3>of human history, the sky was static. We took a photograph.

494
00:22:51.559 --> 00:22:52.640
<v Speaker 3>Now we're watching the video.

495
00:22:52.920 --> 00:22:54.440
<v Speaker 2>I want to pivot for a minute to what you

496
00:22:54.519 --> 00:22:58.599
<v Speaker 2>might call the competition, or maybe the partnership. We mentioned

497
00:22:58.640 --> 00:23:03.160
<v Speaker 2>Igo before, but there's a future mission that's specifically designed

498
00:23:03.640 --> 00:23:05.559
<v Speaker 2>for these super massive systems.

499
00:23:05.920 --> 00:23:09.640
<v Speaker 3>Lisa LISA, the Laser Interferometer space antenna.

500
00:23:09.720 --> 00:23:11.680
<v Speaker 2>It's still just the coolest acronym in science.

501
00:23:11.839 --> 00:23:16.119
<v Speaker 3>It really is. LISA IS. It's essentially a gravitational wave

502
00:23:16.119 --> 00:23:20.720
<v Speaker 3>observatory in space. Imagine three separate spacecraft flying in a

503
00:23:20.720 --> 00:23:24.359
<v Speaker 3>perfect triangle formation, millions of kilometers apart from each.

504
00:23:24.240 --> 00:23:26.279
<v Speaker 2>Other, and they just shoot lasers at each other.

505
00:23:26.440 --> 00:23:28.839
<v Speaker 3>They constantly shoot lasers at each other to measure the

506
00:23:28.880 --> 00:23:33.160
<v Speaker 3>distance between them with unbelievable precision. When a gravitational wave

507
00:23:33.160 --> 00:23:36.640
<v Speaker 3>from a supermassive black hole merger passes through the Solar System,

508
00:23:37.039 --> 00:23:40.039
<v Speaker 3>it will stretch and squeeze the distance between those spacecraft

509
00:23:40.119 --> 00:23:41.279
<v Speaker 3>by less than the width.

510
00:23:41.119 --> 00:23:42.880
<v Speaker 2>Of an atom, and LISA can detect that.

511
00:23:42.960 --> 00:23:45.960
<v Speaker 3>LISA will be able to detect that. It's designed specifically

512
00:23:46.000 --> 00:23:49.400
<v Speaker 3>to hear the low frequency hum of these supermassive black

513
00:23:49.400 --> 00:23:51.559
<v Speaker 3>hole binaries as they spiral together.

514
00:23:51.960 --> 00:23:55.440
<v Speaker 2>So Lisa, here's the gravitational waves, and this new method

515
00:23:55.680 --> 00:23:57.960
<v Speaker 2>sees the light from the strobes. Right.

516
00:23:58.440 --> 00:24:01.559
<v Speaker 3>But here's the timeline issue. LISA is not scheduled to

517
00:24:01.599 --> 00:24:05.000
<v Speaker 3>launch until the mid twenty thirties, maybe twenty thirty five,

518
00:24:05.039 --> 00:24:06.400
<v Speaker 3>twenty thirty seven, somewhere in there.

519
00:24:06.440 --> 00:24:07.799
<v Speaker 2>So we have a decade long gap.

520
00:24:07.920 --> 00:24:10.240
<v Speaker 3>We have a gap. And this is where the new

521
00:24:10.319 --> 00:24:13.680
<v Speaker 3>lensing method claims a huge, huge victory in the paper

522
00:24:14.160 --> 00:24:18.920
<v Speaker 3>Cox has caused an extremely exciting prospect. Using Reuben and

523
00:24:18.960 --> 00:24:22.519
<v Speaker 3>other telescopes, we can detect these inspiraling binaries with the

524
00:24:22.559 --> 00:24:25.359
<v Speaker 3>strobe method years before Lisa ever gets off the ground.

525
00:24:25.400 --> 00:24:26.880
<v Speaker 2>We can build the catalog of targets.

526
00:24:26.920 --> 00:24:29.079
<v Speaker 3>Now we can find them, we can map them, We

527
00:24:29.119 --> 00:24:31.599
<v Speaker 3>can say okay, at these coordinates in the sky, we

528
00:24:31.680 --> 00:24:34.079
<v Speaker 3>have a binary with a mass of a billion suns

529
00:24:34.119 --> 00:24:36.480
<v Speaker 3>and a two year orbital period. We can build a

530
00:24:36.480 --> 00:24:37.119
<v Speaker 3>watch list.

531
00:24:37.359 --> 00:24:40.160
<v Speaker 2>And then in the twenty thirties, when LESA launches.

532
00:24:39.880 --> 00:24:42.119
<v Speaker 3>We turn it on and we already know where to listen.

533
00:24:42.279 --> 00:24:44.519
<v Speaker 3>And this opens the door to the holy grail of

534
00:24:44.599 --> 00:24:47.599
<v Speaker 3>modern astrophysics. Multi messenger astronomy.

535
00:24:47.640 --> 00:24:49.640
<v Speaker 2>That's a buzzword I hear constantly. Can you break that

536
00:24:49.680 --> 00:24:50.200
<v Speaker 2>down for us?

537
00:24:50.319 --> 00:24:52.839
<v Speaker 3>It just means observing the same cosmic event with more

538
00:24:52.880 --> 00:24:55.240
<v Speaker 3>than one messenger or more than one sense, seeing it

539
00:24:55.240 --> 00:24:58.079
<v Speaker 3>with light, and hearing it with gravitational waves. Think about

540
00:24:58.119 --> 00:25:01.799
<v Speaker 3>watching a thunderstorm, see the flash of lightning. That's your

541
00:25:01.839 --> 00:25:05.160
<v Speaker 3>light signal, that's the strobe. A few seconds later, you

542
00:25:05.200 --> 00:25:08.400
<v Speaker 3>hear the boom of the thunder, that's your second signal.

543
00:25:08.359 --> 00:25:11.039
<v Speaker 2>And from the delay between the two, you know how

544
00:25:11.079 --> 00:25:12.799
<v Speaker 2>far away the storm is exactly.

545
00:25:13.000 --> 00:25:15.880
<v Speaker 3>If you only have one, you have incomplete information. But

546
00:25:15.960 --> 00:25:18.400
<v Speaker 3>if you have both you can learn so much more.

547
00:25:19.000 --> 00:25:22.079
<v Speaker 3>Now apply that to black holes. If we can see

548
00:25:22.119 --> 00:25:25.839
<v Speaker 3>the flash from the caustic and hear the gravitational hum

549
00:25:25.839 --> 00:25:28.319
<v Speaker 3>from the inspiral coming from the same object at the

550
00:25:28.319 --> 00:25:32.240
<v Speaker 3>same time, we can test fundamental physics in ways that

551
00:25:32.279 --> 00:25:34.000
<v Speaker 3>are currently just science fiction.

552
00:25:34.400 --> 00:25:35.960
<v Speaker 2>Like what, what's the first thing you'd test?

553
00:25:36.359 --> 00:25:40.599
<v Speaker 3>The speed of gravity? Einstein's theory says gravitational waves travel

554
00:25:40.599 --> 00:25:42.960
<v Speaker 3>at the speed of light, but do they do they

555
00:25:43.039 --> 00:25:47.039
<v Speaker 3>really to the fifteenth decimal place. If the flash and

556
00:25:47.039 --> 00:25:49.839
<v Speaker 3>the wave arrive at our detectors at slightly different times

557
00:25:49.880 --> 00:25:53.119
<v Speaker 3>after traveling for a billion years, that could mean Einstein was.

558
00:25:53.079 --> 00:25:54.960
<v Speaker 2>Wrong, which would be a Nobel prize.

559
00:25:55.000 --> 00:25:57.359
<v Speaker 3>Instantly, we break physics as we know it.

560
00:25:57.680 --> 00:26:00.640
<v Speaker 2>Wow. And it would also tell us about the environment

561
00:26:00.640 --> 00:26:03.400
<v Speaker 2>around the black holes, wouldn't it, Because light gets affected

562
00:26:03.400 --> 00:26:05.319
<v Speaker 2>by gas and dust, but gravity.

563
00:26:05.480 --> 00:26:08.839
<v Speaker 3>Gravity just plows right through everything. It doesn't care. So

564
00:26:08.920 --> 00:26:11.039
<v Speaker 3>if the light signal is a little bit delayed or

565
00:26:11.079 --> 00:26:14.519
<v Speaker 3>scattered compared to the pristine gravity signal. It tells us

566
00:26:14.559 --> 00:26:19.599
<v Speaker 3>exactly how much messy stuff gas, dust, accretion disks is

567
00:26:19.640 --> 00:26:22.319
<v Speaker 3>sitting around the binary. It gives us a complete picture.

568
00:26:22.480 --> 00:26:25.400
<v Speaker 2>It really feels like we're moving from just guessing about

569
00:26:25.400 --> 00:26:27.119
<v Speaker 2>these systems to being able to put them on a

570
00:26:27.200 --> 00:26:28.400
<v Speaker 2>lab bench and measure them.

571
00:26:28.519 --> 00:26:30.839
<v Speaker 3>That's the transition the whole field is making. We are

572
00:26:30.839 --> 00:26:36.200
<v Speaker 3>moving from purely theoretical models of binary evolution to direct

573
00:26:36.400 --> 00:26:37.839
<v Speaker 3>observational telemetry.

574
00:26:38.200 --> 00:26:40.240
<v Speaker 2>I want to circle back to something you mentioned earlier

575
00:26:40.279 --> 00:26:43.359
<v Speaker 2>about the background the stars. Okay, for my whole life,

576
00:26:43.400 --> 00:26:46.920
<v Speaker 2>I've thought of the background stars as well as just noise.

577
00:26:47.160 --> 00:26:49.160
<v Speaker 2>They're just the wallpaper. They are the things you have

578
00:26:49.200 --> 00:26:52.000
<v Speaker 2>to subtract from your image to see the galaxy you're

579
00:26:52.039 --> 00:26:52.960
<v Speaker 2>actually interested in.

580
00:26:53.279 --> 00:26:56.200
<v Speaker 3>Astronomers have a term for it, the confusion limit. When

581
00:26:56.200 --> 00:26:58.839
<v Speaker 3>there are so many faint stars you can't distinguish your

582
00:26:58.880 --> 00:27:01.240
<v Speaker 3>target from the background, just stuff in the way.

583
00:27:01.519 --> 00:27:05.000
<v Speaker 2>But this paper just completely inverts that idea. It says

584
00:27:05.039 --> 00:27:07.799
<v Speaker 2>the background stars aren't the noise, they're the tool.

585
00:27:08.079 --> 00:27:10.000
<v Speaker 3>They are the screen. That's the best way to think

586
00:27:10.000 --> 00:27:12.759
<v Speaker 3>about it. The binary black hole is like an invisible

587
00:27:12.799 --> 00:27:17.480
<v Speaker 3>film projector it's projecting its gravitational shape, this spinning diamond

588
00:27:17.640 --> 00:27:21.759
<v Speaker 3>out into the universe. We can't see the projector itself,

589
00:27:21.960 --> 00:27:22.240
<v Speaker 3>but we.

590
00:27:22.200 --> 00:27:24.359
<v Speaker 2>Can see the image it's casting on the screen at

591
00:27:24.359 --> 00:27:26.039
<v Speaker 2>background stars exactly.

592
00:27:26.240 --> 00:27:28.720
<v Speaker 3>We see the flash as the beam sweeps past. The

593
00:27:28.799 --> 00:27:31.920
<v Speaker 3>universe is a cinema and we're finally figuring out where

594
00:27:31.920 --> 00:27:33.000
<v Speaker 3>to look to see the show.

595
00:27:33.480 --> 00:27:35.200
<v Speaker 2>I want to end on a thought that really struck

596
00:27:35.240 --> 00:27:37.599
<v Speaker 2>me when I was reading the discussion section of the paper,

597
00:27:38.319 --> 00:27:41.839
<v Speaker 2>and it's about old data, archival data.

598
00:27:42.039 --> 00:27:45.359
<v Speaker 3>Ah, yes, the potential for data archaeology.

599
00:27:45.480 --> 00:27:47.599
<v Speaker 2>We've been taking digital pictures of the sky for a

600
00:27:47.640 --> 00:27:51.039
<v Speaker 2>long time now, the Sloan Digital Sky Survey, pan Stars

601
00:27:51.079 --> 00:27:55.079
<v Speaker 2>a dozen other projects. We literally have petabytes of images

602
00:27:55.119 --> 00:27:58.599
<v Speaker 2>sored on hard drives and server farms going back decades.

603
00:27:58.720 --> 00:28:00.839
<v Speaker 3>We do a treasure trap of information.

604
00:28:00.960 --> 00:28:03.960
<v Speaker 2>And if these invisible costic curves are constantly sweeping across

605
00:28:03.960 --> 00:28:06.160
<v Speaker 2>the sky all the time, everywhere.

606
00:28:06.079 --> 00:28:09.559
<v Speaker 3>Then they have, without a doubt, triggered flashes that we

607
00:28:09.599 --> 00:28:10.920
<v Speaker 3>have already photographed.

608
00:28:10.960 --> 00:28:12.759
<v Speaker 2>We've already seen them, we just didn't know what we

609
00:28:12.759 --> 00:28:13.279
<v Speaker 2>were looking at.

610
00:28:13.319 --> 00:28:16.680
<v Speaker 3>Statistically, it's almost a certainty we have very likely recorded

611
00:28:16.680 --> 00:28:17.960
<v Speaker 3>these exact events.

612
00:28:18.039 --> 00:28:19.519
<v Speaker 2>So why didn't anyone notice?

613
00:28:19.599 --> 00:28:22.039
<v Speaker 3>Because if you're looking at an image from nineteen ninety

614
00:28:22.079 --> 00:28:24.880
<v Speaker 3>eight and you see a faint star that for one

615
00:28:24.960 --> 00:28:27.319
<v Speaker 3>night was one hundred times brighter, and then in the

616
00:28:27.359 --> 00:28:31.000
<v Speaker 3>next image it's gone again, what do you do.

617
00:28:31.359 --> 00:28:32.480
<v Speaker 2>I assume it was an error.

618
00:28:32.559 --> 00:28:36.200
<v Speaker 3>You'd shrug, You'd call it a cosmic ray hitting the detector,

619
00:28:36.720 --> 00:28:40.200
<v Speaker 3>a glitch in the CCD chip, an anomaly. You discard

620
00:28:40.240 --> 00:28:43.240
<v Speaker 3>it because it doesn't fit any pattern. You know, it's

621
00:28:43.240 --> 00:28:44.240
<v Speaker 3>a one off weirdo.

622
00:28:44.519 --> 00:28:47.079
<v Speaker 2>We didn't have the dictionary to translate what we were seeing.

623
00:28:47.160 --> 00:28:49.640
<v Speaker 3>We didn't know the language. We didn't know that a

624
00:28:49.720 --> 00:28:53.640
<v Speaker 3>jagged asymmetric spike was the signature of a binary supermassive

625
00:28:53.640 --> 00:28:56.720
<v Speaker 3>black hole caustic. We just filed it under noise. Now

626
00:28:57.000 --> 00:29:00.279
<v Speaker 3>now we have the template. Now we can write new

627
00:29:00.279 --> 00:29:03.039
<v Speaker 3>algorithms to go back into all that old data from

628
00:29:03.079 --> 00:29:06.880
<v Speaker 3>Sloan from pan stars and specifically hunt for that unique

629
00:29:07.119 --> 00:29:08.400
<v Speaker 3>light curve shape.

630
00:29:08.480 --> 00:29:11.480
<v Speaker 2>So the very first discovery of one of these binary

631
00:29:11.559 --> 00:29:14.920
<v Speaker 2>black hole stripes might not happen with the Rubin telescope

632
00:29:14.920 --> 00:29:17.559
<v Speaker 2>in twenty twenty seven. It could happen on a supercomputer

633
00:29:17.680 --> 00:29:20.480
<v Speaker 2>next week, sifting through data from twenty fifteen.

634
00:29:20.920 --> 00:29:24.039
<v Speaker 3>That is entirely possible. The evidence could very well be

635
00:29:24.079 --> 00:29:27.279
<v Speaker 3>sitting there gathering digital dust on a server rack somewhere.

636
00:29:27.599 --> 00:29:29.400
<v Speaker 3>We just need to blow off the dust and look

637
00:29:29.400 --> 00:29:30.480
<v Speaker 3>at it with these new eyes.

638
00:29:30.799 --> 00:29:33.359
<v Speaker 2>That to me is the most exciting kind of science,

639
00:29:33.680 --> 00:29:36.640
<v Speaker 2>the treasure hunt, where you realize the map leads back

640
00:29:36.640 --> 00:29:37.519
<v Speaker 2>to your own basement.

641
00:29:37.640 --> 00:29:40.759
<v Speaker 3>It's a fantastic reminder that data is never truly dead.

642
00:29:40.799 --> 00:29:43.160
<v Speaker 3>It just waits for a new theory, a new idea

643
00:29:43.319 --> 00:29:44.519
<v Speaker 3>to bring it back to life.

644
00:29:44.759 --> 00:29:47.440
<v Speaker 2>Well, I think that is a perfect and very hopeful

645
00:29:47.480 --> 00:29:51.119
<v Speaker 2>place to wrap things up. We've gone from invisible monsters,

646
00:29:51.480 --> 00:29:54.920
<v Speaker 2>to diamond shape lenses, to cosmic strobes, and finally to

647
00:29:55.000 --> 00:29:57.480
<v Speaker 2>divving for treasure in old hard drives. It's been quite

648
00:29:57.480 --> 00:30:00.279
<v Speaker 2>a journey, it really has. And for everyone listening. The

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00:30:00.319 --> 00:30:01.759
<v Speaker 2>next time you look up at a star and you

650
00:30:01.759 --> 00:30:05.039
<v Speaker 2>see a twinkle, well, okay, it's probably just the Earth's atmosphere,

651
00:30:05.519 --> 00:30:08.799
<v Speaker 2>but somewhere out there a star is blinking for a much,

652
00:30:08.920 --> 00:30:12.319
<v Speaker 2>much grander reason because two giants are dancing in front

653
00:30:12.319 --> 00:30:12.519
<v Speaker 2>of it.

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00:30:12.720 --> 00:30:13.640
<v Speaker 3>Keep watching the data.

655
00:30:13.960 --> 00:32:03.359
<v Speaker 2>Thanks for listening, everyone, We'll catch you on the next one.

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00:31:02.160 --> 00:31:31.480
<v Speaker 3>Sai
